Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.stsci.edu/ftp/documents/ghrs-handbook/ghrs-handbook.gz Дата изменения: Tue Jun 21 19:35:55 1994 Дата индексирования: Sat Dec 22 17:29:42 2007 Кодировка: Поисковые слова: aldebaran

%!PS-Adobe-3.0
%%BoundingBox: (atend)
%%Pages: (atend)
%%PageOrder: (atend)
%%DocumentFonts: (atend)
%%Creator: Frame 4.0
%%DocumentData: Clean7Bit
%%EndComments
%%BeginProlog
%
% Frame ps_prolog 4.0, for use with Frame 4.0 products
% This ps_prolog file is Copyright (c) 1986-1993 Frame Technology
% Corporation. All rights reserved. This ps_prolog file may be
% freely copied and distributed in conjunction with documents created
% using FrameMaker, FrameBuilder and FrameViewer as long as this
% copyright notice is preserved.
%
% Frame products normally print colors as their true color on a color printer
% or as shades of gray, based on luminance, on a black-and white printer. The
% following flag, if set to True, forces all non-white colors to print as pure
% black. This has no effect on bitmap images.
/FMPrintAllColorsAsBlack false def
%
% Frame products can either set their own line screens or use a printer's
% default settings. Three flags below control this separately for no
% separations, spot separations and process separations. If a flag
% is true, then the default printer settings will not be changed. If it is
% false, Frame products will use their own settings from a table based on
% the printer's resolution.
/FMUseDefaultNoSeparationScreen true def
/FMUseDefaultSpotSeparationScreen true def
/FMUseDefaultProcessSeparationScreen false def
%
% For any given PostScript printer resolution, Frame products have two sets of
% screen angles and frequencies for printing process separations, which are
% recomended by Adobe. The following variable chooses the higher frequencies
% when set to true or the lower frequencies when set to false. This is only
% effective if the appropriate FMUseDefault...SeparationScreen flag is false.
/FMUseHighFrequencyScreens true def
%
% PostScript Level 2 printers contain an "Accurate Screens" feature which can
% improve process separation rendering at the expense of compute time. This
% flag is ignored by PostScript Level 1 printers.
/FMUseAcccurateScreens true def
%
% The following PostScript procedure defines the spot function that Frame
% products will use for process separations. You may un-comment-out one of
% the alternative functions below, or use your own.
%
% Dot function
/FMSpotFunction {abs exch abs 2 copy add 1 gt
{1 sub dup mul exch 1 sub dup mul add 1 sub }
{dup mul exch dup mul add 1 exch sub }ifelse } def
%
% Line function
% /FMSpotFunction { pop } def
%
% Elipse function
% /FMSpotFunction { dup 5 mul 8 div mul exch dup mul exch add
% sqrt 1 exch sub } def
%
%
/FMversion (4.0) def
/FMLevel1 /languagelevel where {pop languagelevel} {1} ifelse 2 lt def
/FMPColor
FMLevel1 {
false
/colorimage where {pop pop true} if
} {
true
} ifelse
def
/FrameDict 400 dict def
systemdict /errordict known not {/errordict 10 dict def
errordict /rangecheck {stop} put} if
% The readline in PS 23.0 doesn't recognize cr's as nl's on AppleTalk
FrameDict /tmprangecheck errordict /rangecheck get put
errordict /rangecheck {FrameDict /bug true put} put
FrameDict /bug false put
mark
% Some PS machines read past the CR, so keep the following 3 lines together!
currentfile 5 string readline
00
0000000000
cleartomark
errordict /rangecheck FrameDict /tmprangecheck get put
FrameDict /bug get {
/readline {
/gstring exch def
/gfile exch def
/gindex 0 def
{
gfile read pop
dup 10 eq {exit} if
dup 13 eq {exit} if
gstring exch gindex exch put
/gindex gindex 1 add def
} loop
pop
gstring 0 gindex getinterval true
} bind def
} if
/FMshowpage /showpage load def
/FMquit /quit load def
/FMFAILURE {
dup = flush
FMshowpage
/Helvetica findfont 12 scalefont setfont
72 200 moveto
show FMshowpage
FMquit
} def
/FMVERSION {
FMversion ne {
(Frame product version does not match ps_prolog!) FMFAILURE
} if
} def
/FMBADEPSF {
(PostScript Lang. Ref. Man., 2nd Ed., H.2.4 says EPS must not call X )
dup dup (X) search pop exch pop exch pop length
4 -1 roll
putinterval
FMFAILURE
} def
/FMLOCAL {
FrameDict begin
0 def
end
} def
/concatprocs
{
/proc2 exch cvlit def/proc1 exch cvlit def/newproc proc1 length proc2 length add array def
newproc 0 proc1 putinterval newproc proc1 length proc2 putinterval newproc cvx
}def
FrameDict begin
/FMnone 0 def
/FMcyan 1 def
/FMmagenta 2 def
/FMyellow 3 def
/FMblack 4 def
/FMcustom 5 def
/FrameNegative false def
/FrameSepIs FMnone def
/FrameSepBlack 0 def
/FrameSepYellow 0 def
/FrameSepMagenta 0 def
/FrameSepCyan 0 def
/FrameSepRed 1 def
/FrameSepGreen 1 def
/FrameSepBlue 1 def
/FrameCurGray 1 def
/FrameCurPat null def
/FrameCurColors [ 0 0 0 1 0 0 0 ] def
/FrameColorEpsilon .001 def
/eqepsilon {
sub dup 0 lt {neg} if
FrameColorEpsilon le
} bind def
/FrameCmpColorsCMYK {
2 copy 0 get exch 0 get eqepsilon {
2 copy 1 get exch 1 get eqepsilon {
2 copy 2 get exch 2 get eqepsilon {
3 get exch 3 get eqepsilon
} {pop pop false} ifelse
}{pop pop false} ifelse
} {pop pop false} ifelse
} bind def
/FrameCmpColorsRGB {
2 copy 4 get exch 0 get eqepsilon {
2 copy 5 get exch 1 get eqepsilon {
6 get exch 2 get eqepsilon
}{pop pop false} ifelse
} {pop pop false} ifelse
} bind def
/RGBtoCMYK {
1 exch sub
3 1 roll
1 exch sub
3 1 roll
1 exch sub
3 1 roll
3 copy
2 copy
le { pop } { exch pop } ifelse
2 copy
le { pop } { exch pop } ifelse
dup dup dup
6 1 roll
4 1 roll
7 1 roll
sub
6 1 roll
sub
5 1 roll
sub
4 1 roll
} bind def
/CMYKtoRGB {
dup dup 4 -1 roll add
5 1 roll 3 -1 roll add
4 1 roll add
1 exch sub dup 0 lt {pop 0} if 3 1 roll
1 exch sub dup 0 lt {pop 0} if exch
1 exch sub dup 0 lt {pop 0} if exch
} bind def
/FrameSepInit {
1.0 RealSetgray
} bind def
/FrameSetSepColor {
/FrameSepBlue exch def
/FrameSepGreen exch def
/FrameSepRed exch def
/FrameSepBlack exch def
/FrameSepYellow exch def
/FrameSepMagenta exch def
/FrameSepCyan exch def
/FrameSepIs FMcustom def
setCurrentScreen
} bind def
/FrameSetCyan {
/FrameSepBlue 1.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 1.0 def
/FrameSepIs FMcyan def
setCurrentScreen
} bind def

/FrameSetMagenta {
/FrameSepBlue 1.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 1.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMmagenta def
setCurrentScreen
} bind def

/FrameSetYellow {
/FrameSepBlue 0.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 1.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMyellow def
setCurrentScreen
} bind def

/FrameSetBlack {
/FrameSepBlue 0.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 1.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMblack def
setCurrentScreen
} bind def

/FrameNoSep {
/FrameSepIs FMnone def
setCurrentScreen
} bind def
/FrameSetSepColors {
FrameDict begin
[ exch 1 add 1 roll ]
/FrameSepColors
exch def end
} bind def
/FrameColorInSepListCMYK {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsCMYK
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/FrameColorInSepListRGB {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsRGB
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/RealSetgray /setgray load def
/RealSetrgbcolor /setrgbcolor load def
/RealSethsbcolor /sethsbcolor load def
end
/setgray {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetgray }
{
FrameSepIs FMblack eq
{ RealSetgray }
{ FrameSepIs FMcustom eq
FrameSepRed 0 eq and
FrameSepGreen 0 eq and
FrameSepBlue 0 eq and {
RealSetgray
} {
1 RealSetgray pop
} ifelse
} ifelse
} ifelse
end
} bind def
/setrgbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetrgbcolor }
{
3 copy [ 4 1 roll ]
FrameColorInSepListRGB
{
FrameSepBlue eq exch
FrameSepGreen eq and exch
FrameSepRed eq and
{ 0 } { 1 } ifelse
}
{
FMPColor {
RealSetrgbcolor
currentcmykcolor
} {
RGBtoCMYK
} ifelse
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
RealSetgray
}
ifelse
end
} bind def
/sethsbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSethsbcolor }
{
RealSethsbcolor
currentrgbcolor
setrgbcolor
}
ifelse
end
} bind def
FrameDict begin
/setcmykcolor where {
pop /RealSetcmykcolor /setcmykcolor load def
} {
/RealSetcmykcolor {
4 1 roll
3 { 3 index add 0 max 1 min 1 exch sub 3 1 roll} repeat
setrgbcolor pop
} bind def
} ifelse
userdict /setcmykcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetcmykcolor }
{
4 copy [ 5 1 roll ]
FrameColorInSepListCMYK
{
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
{ 0 } { 1 } ifelse
}
{
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
RealSetgray
}
ifelse
end
} bind put
FMLevel1 not {

/patProcDict 5 dict dup begin
<0f1e3c78f0e1c387> { 3 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<0f87c3e1f0783c1e> { 3 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
<8142241818244281> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-1 -1 moveto 9 9 lineto stroke } bind def
<03060c183060c081> { 1 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<8040201008040201> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
end def
/patDict 15 dict dup begin
/PatternType 1 def
/PaintType 2 def
/TilingType 3 def
/BBox [ 0 0 8 8 ] def
/XStep 8 def
/YStep 8 def
/PaintProc {
begin
patProcDict bstring known {
patProcDict bstring get exec
} {
8 8 true [1 0 0 -1 0 8] bstring imagemask
} ifelse
end
} bind def
end def
} if
/combineColor {
FrameSepIs FMnone eq
{
graymode FMLevel1 or not {

[/Pattern [/DeviceCMYK]] setcolorspace
FrameCurColors 0 4 getinterval aload pop FrameCurPat setcolor
} {
FrameCurColors 3 get 1.0 ge {
FrameCurGray RealSetgray
} {
FMPColor graymode and {
0 1 3 {
FrameCurColors exch get
1 FrameCurGray sub mul
} for
RealSetcmykcolor
} {
4 1 6 {
FrameCurColors exch get
graymode {
1 exch sub 1 FrameCurGray sub mul 1 exch sub
} {
1.0 lt {FrameCurGray} {1} ifelse
} ifelse
} for
RealSetrgbcolor
} ifelse
} ifelse
} ifelse
} {
FrameCurColors 0 4 getinterval aload
FrameColorInSepListCMYK {
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
FrameSepIs FMcustom eq and
{ FrameCurGray } { 1 } ifelse
} {
FrameSepIs FMblack eq
{FrameCurGray 1.0 exch sub mul 1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop FrameCurGray 1.0 exch sub mul 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
graymode FMLevel1 or not {

[/Pattern [/DeviceGray]] setcolorspace
FrameCurPat setcolor
} {
graymode not FMLevel1 and {

dup 1 lt {pop FrameCurGray} if
} if
RealSetgray
} ifelse
} ifelse
} bind def
/savematrix {
orgmatrix currentmatrix pop
} bind def
/restorematrix {
orgmatrix setmatrix
} bind def
/dmatrix matrix def
/dpi 72 0 dmatrix defaultmatrix dtransform
dup mul exch dup mul add sqrt def

/freq dpi dup 72 div round dup 0 eq {pop 1} if 8 mul div def
/sangle 1 0 dmatrix defaultmatrix dtransform exch atan def
/dpiranges [ 2540 2400 1693 1270 1200 635 600 0 ] def
/CMLowFreqs [ 100.402 94.8683 89.2289 100.402 94.8683 66.9349 63.2456 47.4342 ] def
/YLowFreqs [ 95.25 90.0 84.65 95.25 90.0 70.5556 66.6667 50.0 ] def
/KLowFreqs [ 89.8026 84.8528 79.8088 89.8026 84.8528 74.8355 70.7107 53.033 ] def
/CLowAngles [ 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 ] def
/MLowAngles [ 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 ] def
/YLowTDot [ true true false true true false false false ] def
/CMHighFreqs [ 133.87 126.491 133.843 108.503 102.523 100.402 94.8683 63.2456 ] def
/YHighFreqs [ 127.0 120.0 126.975 115.455 109.091 95.25 90.0 60.0 ] def
/KHighFreqs [ 119.737 113.137 119.713 128.289 121.218 89.8026 84.8528 63.6395 ] def
/CHighAngles [ 71.5651 71.5651 71.5651 70.0169 70.0169 71.5651 71.5651 71.5651 ] def
/MHighAngles [ 18.4349 18.4349 18.4349 19.9831 19.9831 18.4349 18.4349 18.4349 ] def
/YHighTDot [ false false true false false true true false ] def
/PatFreq [ 10.5833 10.0 9.4055 10.5833 10.0 10.5833 10.0 9.375 ] def
/screenIndex {
0 1 dpiranges length 1 sub { dup dpiranges exch get 1 sub dpi le {exit} {pop} ifelse } for
} bind def
/getCyanScreen {
FMUseHighFrequencyScreens { CHighAngles CMHighFreqs} {CLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getMagentaScreen {
FMUseHighFrequencyScreens { MHighAngles CMHighFreqs } {MLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getYellowScreen {
FMUseHighFrequencyScreens { YHighTDot YHighFreqs} { YLowTDot YLowFreqs } ifelse
screenIndex dup 3 1 roll get 3 1 roll get { 3 div
{2 { 1 add 2 div 3 mul dup floor sub 2 mul 1 sub exch} repeat
FMSpotFunction } } {/FMSpotFunction load } ifelse
0.0 exch
} bind def
/getBlackScreen {
FMUseHighFrequencyScreens { KHighFreqs } { KLowFreqs } ifelse
screenIndex get 45.0 /FMSpotFunction load
} bind def
/getSpotScreen {
getBlackScreen
} bind def
/getCompositeScreen {
getBlackScreen
} bind def
/FMSetScreen
FMLevel1 { /setscreen load
}{ {
8 dict begin
/HalftoneType 1 def
/SpotFunction exch def
/Angle exch def
/Frequency exch def
/AccurateScreens FMUseAcccurateScreens def
currentdict end sethalftone
} bind } ifelse
def
/setDefaultScreen {
FMPColor {
orgrxfer cvx orggxfer cvx orgbxfer cvx orgxfer cvx setcolortransfer
}
{
orgxfer cvx settransfer
} ifelse
orgfreq organgle orgproc cvx setscreen
} bind def
/setCurrentScreen {
FrameSepIs FMnone eq {
FMUseDefaultNoSeparationScreen {
setDefaultScreen
} {
getCompositeScreen FMSetScreen
} ifelse
} {
FrameSepIs FMcustom eq {
FMUseDefaultSpotSeparationScreen {
setDefaultScreen
} {
getSpotScreen FMSetScreen
} ifelse
} {
FMUseDefaultProcessSeparationScreen {
setDefaultScreen
} {
FrameSepIs FMcyan eq {
getCyanScreen FMSetScreen
} {
FrameSepIs FMmagenta eq {
getMagentaScreen FMSetScreen
} {
FrameSepIs FMyellow eq {
getYellowScreen FMSetScreen
} {
getBlackScreen FMSetScreen
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} bind def
end
/gstring FMLOCAL
/gfile FMLOCAL
/gindex FMLOCAL
/orgrxfer FMLOCAL
/orggxfer FMLOCAL
/orgbxfer FMLOCAL
/orgxfer FMLOCAL
/orgproc FMLOCAL
/orgrproc FMLOCAL
/orggproc FMLOCAL
/orgbproc FMLOCAL
/organgle FMLOCAL
/orgrangle FMLOCAL
/orggangle FMLOCAL
/orgbangle FMLOCAL
/orgfreq FMLOCAL
/orgrfreq FMLOCAL
/orggfreq FMLOCAL
/orgbfreq FMLOCAL
/yscale FMLOCAL
/xscale FMLOCAL
/edown FMLOCAL
/manualfeed FMLOCAL
/paperheight FMLOCAL
/paperwidth FMLOCAL
/FMDOCUMENT {
array /FMfonts exch def
/#copies exch def
FrameDict begin
0 ne /manualfeed exch def
/paperheight exch def
/paperwidth exch def
0 ne /FrameNegative exch def
0 ne /edown exch def
/yscale exch def
/xscale exch def
FMLevel1 {
manualfeed {setmanualfeed} if
/FMdicttop countdictstack 1 add def
/FMoptop count def
% setpapername
% manualfeed {true} {papersize} ifelse
% {manualpapersize} {false} ifelse
% {desperatepapersize} {false} ifelse
% { (Can't select requested paper size for Frame print job!) FMFAILURE } if
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
}
{{1 dict dup /PageSize [paperwidth paperheight]put setpagedevice}stopped
{ (Can't select requested paper size for Frame print job!) FMFAILURE } if
{1 dict dup /ManualFeed manualfeed put setpagedevice } stopped pop }
ifelse

FMPColor {
currentcolorscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def
cvlit /orgbproc exch def
/orgbangle exch def
/orgbfreq exch def
cvlit /orggproc exch def
/orggangle exch def
/orggfreq exch def
cvlit /orgrproc exch def
/orgrangle exch def
/orgrfreq exch def
currentcolortransfer
FrameNegative {
1 1 4 {
pop { 1 exch sub } concatprocs 4 1 roll
} for
4 copy
setcolortransfer
} if
cvlit /orgxfer exch def
cvlit /orgbxfer exch def
cvlit /orggxfer exch def
cvlit /orgrxfer exch def
} {
currentscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def

currenttransfer
FrameNegative {
{ 1 exch sub } concatprocs
dup settransfer
} if
cvlit /orgxfer exch def
} ifelse
end
} def
/pagesave FMLOCAL
/orgmatrix FMLOCAL
/landscape FMLOCAL
/pwid FMLOCAL
/FMBEGINPAGE {
FrameDict begin
/pagesave save def
3.86 setmiterlimit
/landscape exch 0 ne def
landscape {
90 rotate 0 exch dup /pwid exch def neg translate pop
}{
pop /pwid exch def
} ifelse
edown { [-1 0 0 1 pwid 0] concat } if
0 0 moveto paperwidth 0 lineto paperwidth paperheight lineto
0 paperheight lineto 0 0 lineto 1 setgray fill
xscale yscale scale
/orgmatrix matrix def
gsave
} def
/FMENDPAGE {
grestore
pagesave restore
end
showpage
} def
/FMFONTDEFINE {
FrameDict begin
findfont
ReEncode
1 index exch
definefont
FMfonts 3 1 roll
put
end
} def
/FMFILLS {
FrameDict begin dup
array /fillvals exch def
dict /patCache exch def
end
} def
/FMFILL {
FrameDict begin
fillvals 3 1 roll put
end
} def
/FMNORMALIZEGRAPHICS {
newpath
0.0 0.0 moveto
1 setlinewidth
0 setlinecap
0 0 0 sethsbcolor
0 setgray
} bind def
/fx FMLOCAL
/fy FMLOCAL
/fh FMLOCAL
/fw FMLOCAL
/llx FMLOCAL
/lly FMLOCAL
/urx FMLOCAL
/ury FMLOCAL
/FMBEGINEPSF {
end
/FMEPSF save def
/showpage {} def
% See Adobe's "PostScript Language Reference Manual, 2nd Edition", page 714.
% "...the following operators MUST NOT be used in an EPS file:" (emphasis ours)
/banddevice {(banddevice) FMBADEPSF} def
/clear {(clear) FMBADEPSF} def
/cleardictstack {(cleardictstack) FMBADEPSF} def
/copypage {(copypage) FMBADEPSF} def
/erasepage {(erasepage) FMBADEPSF} def
/exitserver {(exitserver) FMBADEPSF} def
/framedevice {(framedevice) FMBADEPSF} def
/grestoreall {(grestoreall) FMBADEPSF} def
/initclip {(initclip) FMBADEPSF} def
/initgraphics {(initgraphics) FMBADEPSF} def
/initmatrix {(initmatrix) FMBADEPSF} def
/quit {(quit) FMBADEPSF} def
/renderbands {(renderbands) FMBADEPSF} def
/setglobal {(setglobal) FMBADEPSF} def
/setpagedevice {(setpagedevice) FMBADEPSF} def
/setshared {(setshared) FMBADEPSF} def
/startjob {(startjob) FMBADEPSF} def
/lettertray {(lettertray) FMBADEPSF} def
/letter {(letter) FMBADEPSF} def
/lettersmall {(lettersmall) FMBADEPSF} def
/11x17tray {(11x17tray) FMBADEPSF} def
/11x17 {(11x17) FMBADEPSF} def
/ledgertray {(ledgertray) FMBADEPSF} def
/ledger {(ledger) FMBADEPSF} def
/legaltray {(legaltray) FMBADEPSF} def
/legal {(legal) FMBADEPSF} def
/statementtray {(statementtray) FMBADEPSF} def
/statement {(statement) FMBADEPSF} def
/executivetray {(executivetray) FMBADEPSF} def
/executive {(executive) FMBADEPSF} def
/a3tray {(a3tray) FMBADEPSF} def
/a3 {(a3) FMBADEPSF} def
/a4tray {(a4tray) FMBADEPSF} def
/a4 {(a4) FMBADEPSF} def
/a4small {(a4small) FMBADEPSF} def
/b4tray {(b4tray) FMBADEPSF} def
/b4 {(b4) FMBADEPSF} def
/b5tray {(b5tray) FMBADEPSF} def
/b5 {(b5) FMBADEPSF} def
FMNORMALIZEGRAPHICS
[/fy /fx /fh /fw /ury /urx /lly /llx] {exch def} forall
fx fw 2 div add fy fh 2 div add translate
rotate
fw 2 div neg fh 2 div neg translate
fw urx llx sub div fh ury lly sub div scale
llx neg lly neg translate
/FMdicttop countdictstack 1 add def
/FMoptop count def
} bind def
/FMENDEPSF {
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
FMEPSF restore
FrameDict begin
} bind def
FrameDict begin
/setmanualfeed {
%%BeginFeature *ManualFeed True
statusdict /manualfeed true put
%%EndFeature
} bind def
/max {2 copy lt {exch} if pop} bind def
/min {2 copy gt {exch} if pop} bind def
/inch {72 mul} def
/pagedimen {
paperheight sub abs 16 lt exch
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(Editor and principal author is David R. Soderblom.) 72 676.67 T
(Date of issue is May 31, 1994.) 72 652.67 T
(Date of last revision was May 2, 1994) 72 640.67 T
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(410-338-4543) 389.62 371 T
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(soderblom@stsci.edu) 454.13 371 T
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(Stephen J. Hulbert) 173.62 356 T
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(hulbert@stsci.edu) 454.13 356 T
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(410-338-4425) 389.62 341 T
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(leither) 454.13 341 T
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(Lisa Sherbert) 173.62 326 T
(T) 257.6 326 T
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(lisa@stsci.edu) 454.13 326 T
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(GHRS Instrument Handbook Revision History) 207 245 T
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(V) 220.78 221.67 T
(ersion) 225.67 221.67 T
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(1.0) 220.78 207 T
(1985 October) 274.78 207 T
(D. Ebbets) 357.03 207 T
(2.0) 220.78 192 T
(1989 May) 274.78 192 T
(D. Duncan and D. Ebbets) 357.03 192 T
(2.1) 220.78 177 T
(1990 March) 274.78 177 T
(D. Duncan) 357.03 177 T
(3.0) 220.78 162 T
(1992 January) 274.78 162 T
(D. Duncan) 357.03 162 T
(4.0) 220.78 147 T
(1993 January) 274.78 147 T
(D. Soderblom) 357.03 147 T
(4.1) 220.78 132 T
(1993 March) 274.78 132 T
(D. Soderblom) 357.03 132 T
(5.0) 220.78 117 T
(1994 May) 274.78 117 T
(D. Soderblom) 357.03 117 T
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168.87 534.75 443.13 534.75 2 L
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448.13 398.25 448.13 294.75 2 L
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(8) 388.17 605.35 T
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(Instrument Summary \321 Why Use the GHRS?) 171 552.68 T
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(...................) 441 552.68 T
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(1) 508.77 552.68 T
(1) 515 552.68 T
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2 10 Q
(2.1) 184.1 535.35 T
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0 0 0 1 0 0 0 K
(Fundamental properties of the instrument) 207 535.35 T
(12) 415.36 535.35 T
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0 0 0 1 0 0 0 K
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(2.2) 184.1 519.35 T
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(A Brief Description of the Instrument and Its Operation) 207 519.35 T
(13) 477.04 519.35 T
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(2.3) 184.1 503.35 T
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(A Little About How) 207 503.35 T
6 F
(HST) 299.22 503.35 T
2 F
( and GHRS W) 319.22 503.35 T
(ork) 383.49 503.35 T
(15) 409.05 503.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(2.4) 184.1 487.35 T
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0 0 0 1 0 0 0 K
(GHRS Modes of Operation) 207 487.35 T
(17) 342.57 487.35 T
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0 0 0 1 0 0 0 K
2 14 Q
(Part II: W) 72 450.68 T
(riting GHRS Proposals) 132.42 450.68 T
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0 0 0 1 0 0 0 K
5 F
(Chapter 3) 72 412.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Phase I: What the T) 171 412.68 T
(AC Sees) 281.29 412.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(...................................................) 329 412.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(21) 508 412.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
(3.1) 184.1 395.35 T
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0 0 0 1 0 0 0 K
(Essential questions) 207 395.35 T
(22) 310.92 395.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(3.2) 184.1 379.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Creating an Observation Scenario) 207 379.35 T
(23) 378.16 379.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(3.3) 184.1 363.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Specifying T) 207 363.35 T
(arget Acquisition) 265.72 363.35 T
(24) 357.4 363.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(3.4) 184.1 347.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Calculating the Exposure T) 207 347.35 T
(ime) 335.74 347.35 T
(26) 362.97 347.35 T
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0 0 0 1 0 0 0 K
5 14 Q
(Chapter 4) 72 310.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Y) 171 310.68 T
(our Phase II Pr) 178.78 310.68 T
(oposal) 264.46 310.68 T
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0 0 0 1 0 0 0 K
(...........................................................) 301 310.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(33) 508 310.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
(4.1) 184.1 293.35 T
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0 0 0 1 0 0 0 K
(Acquisitions) 207 293.35 T
(35) 277.01 293.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(4.2) 184.1 277.35 T
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(Image Mode) 207 277.35 T
(42) 274.79 277.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(4.3) 184.1 261.35 T
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0 0 0 1 0 0 0 K
(Accumulation Mode) 207 261.35 T
(43) 312.01 261.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(4.4) 184.1 245.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Rapid Readout Mode) 207 245.35 T
(45) 316.45 245.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(4.5) 184.1 229.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(The Precision and Accuracy of Standard Calibrations) 207 229.35 T
(46) 469.85 229.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(4.6) 184.1 213.35 T
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(Other Considerations) 207 213.35 T
(47) 319.24 213.35 T
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5 14 Q
(Chapter 5) 72 176.68 T
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(Phase II Pr) 171 176.68 T
(oposal Examples) 233.73 176.68 T
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(...................................................) 329 176.68 T
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(49) 508 176.68 T
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2 10 Q
(4) 54 60.29 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(GHRS Instrument Handbook 5.0) 189 60.29 T
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0 0 0 1 0 0 0 K
2 14 Q
(Part III: GHRS Reference Information) 54 676.68 T
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5 F
(Chapter 6) 54 638.68 T
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(Design and Construction of the GHRS) 153 638.68 T
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(.................................) 374.5 638.68 T
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(55) 490 638.68 T
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2 10 Q
(6.1) 166.1 621.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(The HST Focal Plane and the GHRS Apertures) 189 621.35 T
(56) 417.94 621.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(6.2) 166.1 605.35 T
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0 0 0 1 0 0 0 K
(Gratings and Optical Elements) 189 605.35 T
(60) 344.6 605.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(6.3) 166.1 589.35 T
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0 0 0 1 0 0 0 K
(The Digicon Detectors) 189 589.35 T
(62) 305.13 589.35 T
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5 14 Q
(Chapter 7) 54 552.68 T
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0 0 0 1 0 0 0 K
(T) 153 552.68 T
(ar) 160 552.68 T
(get Acquisition Refer) 171.41 552.68 T
(ence Information) 290.69 552.68 T
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0 0 0 1 0 0 0 K
(.............................) 388.5 552.68 T
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(67) 490 552.68 T
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2 10 Q
(7.1) 166.1 535.35 T
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0 0 0 1 0 0 0 K
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(arget Acquisition Count Rates for Stars) 246.05 535.35 T
(68) 443.3 535.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(7.2) 166.1 519.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Constraints on the V) 189 519.35 T
(alue of the STEP-TIME Parameter) 286.24 519.35 T
(71) 454.06 519.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
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(7.3) 166.1 503.35 T
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(Acquisition Count Rates for Extended Objects) 189 503.35 T
(76) 418.48 503.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(7.4) 166.1 487.35 T
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0 0 0 1 0 0 0 K
(Other Acquisition Information) 189 487.35 T
(78) 340.68 487.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 14 Q
(Chapter 8) 54 450.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Refer) 153 450.68 T
(ence T) 182.32 450.68 T
(ables for Instrument Performance) 217.19 450.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(.......................) 409.5 450.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(81) 490 450.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
(8.1) 166.1 433.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(The Effect of COST) 189 433.35 T
(AR on the GHRS) 279.38 433.35 T
(82) 368.27 433.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(8.2) 166.1 417.35 T
0 0 0 1 0 0 0 K
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(Properties of the First-Order Gratings) 189 417.35 T
(83) 377.37 417.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
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(8.3) 166.1 401.35 T
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(Properties of the Echelle Gratings) 189 401.35 T
(87) 360.16 401.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(8.4) 166.1 385.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Standard Patterns for Substepping and Background Measurement) 189 385.35 T
(92) 513.5 385.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(8.5) 166.1 369.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(The Effects of Reddening in the Ultraviolet) 189 369.35 T
(93) 400.7 369.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(8.6) 166.1 353.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Instrumental Properties) 189 353.35 T
(94) 311.25 353.35 T
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0 0 0 1 0 0 0 K
5 14 Q
(Chapter 9) 54 316.68 T
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0 0 0 1 0 0 0 K
(GHRS Bibliography) 153 316.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(.............................................................) 269.5 316.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(101) 483 316.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
(9.1) 166.1 299.35 T
0 0 0 1 0 0 0 K
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(Ultraviolet Extinction) 189 299.35 T
(102) 299.02 299.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
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(9.2) 166.1 283.35 T
0 0 0 1 0 0 0 K
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(GHRS-Related T) 189 283.35 T
(echnical Papers) 265.49 283.35 T
(102) 351.64 283.35 T
0 0 0 1 0 0 0 K
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(9.3) 166.1 267.35 T
0 0 0 1 0 0 0 K
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(GHRS Scienti\336c Papers) 189 267.35 T
(104) 311.26 267.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
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(9.4) 166.1 251.35 T
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(Acknowledgments) 189 251.35 T
(109) 287.35 251.35 T
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2 14 Q
(Part IV) 54 214.68 T
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5 F
(Glossary of T) 153 176.68 T
(erms and Abbr) 226.88 176.68 T
(eviations) 310.37 176.68 T
0 0 0 1 0 0 0 K
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(..................................) 364 176.68 T
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(1) 484.54 176.68 T
(1) 490.77 176.68 T
(1) 497 176.68 T
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(Index) 153 138.68 T
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(.....................................................................................) 185.5 138.68 T
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(1) 483.77 138.68 T
(15) 490 138.68 T
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2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (5) 552.44 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
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72 445.03 558 445.03 2 L
2 Z
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72 74.02 558 74.02 2 L
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72 445.03 558 445.03 2 L
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72 74.02 558 74.02 2 L
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7 12 Q
1.2 (Chapter 1) 72 677 S
5 24 Q
-0.48 (Pr) 207 677 S
-0.48 (eliminaries and) 229.61 677 S
-0.48 (Essential Reading) 207 647 S
4 12 Q
(1.1) 144 424 T
( This Handbook) 164.02 424 T
8 F
( 7) 511.99 424 T
4 F
(1.2) 144 406 T
( Changes since the previous version) 164.02 406 T
8 F
( 8) 511.99 406 T
4 10 Q
(1.2.1) 162 389.33 T
( This Handbook) 187.02 389.33 T
8 F
( 8) 513.66 389.33 T
4 F
(1.2.2) 162 373.33 T
( Side 1 A) 187.02 373.33 T
(vailability) 227.42 373.33 T
8 F
( 8) 513.66 373.33 T
4 F
(1.2.3) 162 357.33 T
( Acquiring Extended Objects with the GHRS) 187.02 357.33 T
8 F
( 8) 513.66 357.33 T
4 F
(1.2.4) 162 341.33 T
( Acquiring Faint Objects with the GHRS or FOS) 187.02 341.33 T
8 F
( 8) 513.66 341.33 T
4 F
(1.2.5) 162 325.33 T
( Noise Rejection for V) 187.02 325.33 T
(ery Faint Objects) 283.17 325.33 T
8 F
( 9) 513.66 325.33 T
4 F
(1.2.6) 162 309.33 T
( The Proposal Process for Cycle 5) 187.02 309.33 T
8 F
( 9) 513.66 309.33 T
4 F
(1.2.7) 162 293.33 T
( Updated Instrument Parameters) 187.02 293.33 T
8 F
( 9) 513.66 293.33 T
4 F
(1.2.8) 162 277.33 T
( GHRS Sensitivity) 187.02 277.33 T
8 F
( 9) 513.66 277.33 T
4 F
(1.2.9) 162 261.33 T
( GHRS Aperture Nomenclature) 187.02 261.33 T
8 F
( 9) 513.66 261.33 T
4 12 Q
(1.3) 144 244 T
( Where to \336nd additional information, changes, errata, etc.) 164.02 244 T
8 F
( 10) 505.32 244 T
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(Preliminaries and Essential Reading) 189 736.18 T
54 726.98 540 726.98 2 L
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54 74.02 540 74.02 2 L
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2 10 Q
(6) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
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54 726.98 540 726.98 2 L
0.25 H
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54 74.02 540 74.02 2 L
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54 750.02 540 750.02 2 L
2 H
0 Z
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54 726.98 540 726.98 2 L
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54 74.02 540 74.02 2 L
2 Z
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0 F
-0.13 (There are two reasons you may be referring to this) 189 679.35 P
3 F
-0.13 (Handbook) 392.06 679.35 P
0 F
-0.13 (. First, you may be consid-) 433.72 679.35 P
1.12 (ering using the GHRS to observe some celestial object, and you would like to know) 189 667.35 P
0.13 (what the instrument can do and how long it might take. Better yet, your proposal to use) 189 655.35 P
0.58 (the) 189 643.35 P
3 F
0.58 (Hubble Space T) 204.3 643.35 P
0.58 (elescope) 268.41 643.35 P
0 F
0.58 ( with the GHRS has been successful and you now need to) 302.84 643.35 P
0.57 (supply all the details of your observations that are needed in Phase II of proposal pro-) 189 631.35 P
(cessing.) 189 619.35 T
2.31 (Both tasks may seem daunting at \336rst because any versatile instrument has many) 189 599.35 P
0.85 (options. But for what most people want to do most of the time there are defaults that) 189 587.35 P
0.84 (apply) 189 575.35 P
0.84 (, and the GHRS is, in fact, a very easy-to-use device. Once you know that what) 210.57 575.35 P
-0.23 (you want to do falls within the bounds of conventional uses of the spectrograph, you can) 189 563.35 P
0.88 (proceed with some con\336dence that your observations will be successfully obtained in) 189 551.35 P
-0.23 (the form you originally desired. Or you can at least get a sense that what you are propos-) 189 539.35 P
(ing is truly unusual and may push the limits of the instrument.) 189 527.35 T
1.38 (This) 189 507.35 P
3 F
1.38 (Handbook) 210.66 507.35 P
0 F
1.38 ( exists as a basic reference manual for the Goddard High Resolution) 252.32 507.35 P
1.49 (Spectrograph \050GHRS\051, and describes its properties and operation. This) 189 495.35 P
3 F
1.49 (Handbook) 487.68 495.35 P
0 F
1.49 ( is) 529.34 495.35 P
-0.12 (revised and reissued approximately once each year) 189 483.35 P
-0.12 (. This version is written for observers) 391.01 483.35 P
0.77 (wishing to propose to use the GHRS in) 189 471.35 P
3 F
0.77 (HST\325) 354.06 471.35 P
0 F
0.77 (s Cycle 5, and it supersedes all previous) 374.62 471.35 P
1.76 (versions of the) 189 459.35 P
3 F
1.76 ( Instrument Handbook) 251.4 459.35 P
0 F
1.76 (. No) 344.91 459.35 P
3 F
1.76 (HST) 368.15 459.35 P
0 F
1.76 ( document stands alone in providing) 385.93 459.35 P
0.77 (complete information because each \336lls a particular need. The) 189 447.35 P
3 F
0.77 (Call for Pr) 446.95 447.35 P
0.77 (oposals) 492.01 447.35 P
0 F
0.77 (, for) 522.57 447.35 P
1.56 (example, describes the proposal submission process and provides a summary of the) 189 435.35 P
2.61 (observatory and its instruments. The) 189 423.35 P
3 F
2.61 (Phase II Pr) 350.38 423.35 P
2.61 (oposal Instructions) 401.33 423.35 P
0 F
2.61 ( give detailed) 480.9 423.35 P
0.02 (instructions for providing STScI with the speci\336cations that translate your program into) 189 411.35 P
0.73 (commands that) 189 399.35 P
3 F
0.73 (HST) 253.79 399.35 P
0 F
0.73 ( executes. The instrument handbooks supplement both documents) 271.57 399.35 P
0.95 (by providing the technical details of instrument performance and operation. The) 189 387.35 P
3 F
0.95 (HST) 522.22 387.35 P
-0.19 (Data Handbook) 189 375.35 P
0 F
-0.19 (describes how software takes the raw data from the telescope and trans-) 255.27 375.35 P
0.34 (forms it into a reduced and calibrated form for your further analysis and interpretation,) 189 363.35 P
(and how you can duplicate those steps.) 189 351.35 T
3 F
0.35 (HST) 189 331.35 P
0 F
0.35 ( is now a fairly mature spacecraft and so we can predict what many observers will) 206.78 331.35 P
1.46 (need. This) 189 319.35 P
3 F
1.46 (Handbook) 236.09 319.35 P
0 F
1.46 ( is designed around the needs of the majority of users, so that) 277.75 319.35 P
0.4 (essential information is concentrated in a few sections. Full details must also be given,) 189 307.35 P
0.26 (of course, and they are provided in a reference section. W) 189 295.35 P
0.26 (e demonstrate the ease of use) 421.8 295.35 P
1.44 (of the GHRS by providing examples for some of the dif) 189 283.35 P
1.44 (ferent situations that a user) 426.49 283.35 P
-0.17 (might encounter) 189 271.35 P
-0.17 (. W) 253.55 271.35 P
-0.17 (e have also tried to provide the information you need to decide when) 267.03 271.35 P
(your observations deviate from the \322normal\323 and involve special aspects.) 189 259.35 T
0.8 (No handbook of this kind can be complete and error) 189 239.35 P
0.8 (-free until the instrument itself is) 404.6 239.35 P
0.21 (obsolete. W) 189 227.35 P
0.21 (e have, of course, edited it thoroughly) 236.18 227.35 P
0.21 (, but if signi\336cant revisions are called) 388.46 227.35 P
0.09 (for they will be announced via STEIS) 189 215.35 P
0 8 Q
0.07 (1) 340.65 219.35 P
0 10 Q
0.09 (, as with other) 344.65 215.35 P
3 F
0.09 (HST) 404.18 215.35 P
0 F
0.09 ( news items. Do not be afraid) 421.96 215.35 P
-0.04 (to consult with us if you have questions; the means of contact are provided just after the) 189 203.35 P
(title page.) 189 191.35 T
0.51 (As we said, this particular version of the) 189 171.35 P
3 F
0.51 (GHRS Instrument Handbook) 357.2 171.35 P
0 F
0.51 ( is being written) 473.76 171.35 P
0.22 (for Cycle 5 of the) 189 159.35 P
3 F
0.22 (HST) 263.11 159.35 P
0 F
0.22 ( science program. That means that we are providing information) 280.89 159.35 P
1.82 (on how the instrument works after the Servicing Mission installed COST) 189 147.35 P
1.82 (AR and a) 498.59 147.35 P
0.4 (GHRS Repair Kit. COST) 189 135.35 P
0.4 (AR changed the image scale of) 291.07 135.35 P
3 F
0.4 (HST) 420.66 135.35 P
0 F
0.4 ( at the entrance apertures) 438.44 135.35 P
54 96.98 540 126.98 C
0 0 0 1 0 0 0 K
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189 104.98 333 104.98 2 L
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(1. This and other terms are de\336ned and described in a Glossary at the end of this) 189 90.98 T
3 F
(Handbook.) 482.7 90.98 T
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72 726.98 558 726.98 2 L
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2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (7) 552.44 60.29 P
72 750.02 558 750.02 2 L
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72 726.98 558 726.98 2 L
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2 9 Q
(Preliminaries and Essential Reading) 207 736.18 T
0 10 Q
-0.25 (of the GHRS; it also produces dif) 207 679.35 P
-0.25 (fraction-limited images, but does not alter GHRS oper-) 339.21 679.35 P
-0.01 (ations in any fundamental manner) 207 667.35 P
-0.01 (. In other words, COST) 342.51 667.35 P
-0.01 (AR alters some of the parame-) 435.56 667.35 P
1.22 (ters used in various calculations for pointing and throughput, but the instrument still) 207 655.35 P
(operates in the same way) 207 643.35 T
(.) 306.88 643.35 T
0.26 (The GHRS Repair Kit enabled the reactivation of Side 1 of the GHRS, once again per-) 207 623.35 P
1.64 (mitting short-wavelength echelle spectra to be obtained, as well as spectra with the) 207 611.35 P
1.12 (G140L and G140M gratings. At the time this is written Side 1 reactivation has been) 207 599.35 P
1.09 (completed and a few observations have been made. They indicate that Side 1 is per-) 207 587.35 P
0.79 (forming with essentially the same science capabilities that it had at the time of) 207 575.35 P
3 F
0.79 (HST\325) 533.55 575.35 P
0 F
0.79 (s) 554.11 575.35 P
(launch.) 207 563.35 T
72 520.02 558 523.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 521.52 558 521.52 2 L
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2 Z
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0 0 0 1 0 0 0 K
N
72 521.52 198 521.52 2 L
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N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(1.1) 181.32 527.02 T
(This Handbook) 207 527.02 T
0 10 Q
0.78 (If you have looked through the T) 207 503.35 P
0.78 (able of Contents, you will have seen that this) 343.2 503.35 P
3 F
0.78 (Hand-) 532.45 503.35 P
(book) 207 491.35 T
0 F
( is divided into four parts:) 226.44 491.35 T
0.4 (Part I is a summary in which this) 221.4 473.35 P
3 F
0.4 (Handbook) 359 473.35 P
0 F
0.4 ( is described and suggestions are made) 400.66 473.35 P
0.48 (on how to use this document and how it is related to other) 221.4 461.35 P
3 F
0.48 (HST) 461.79 461.35 P
0 F
0.48 (-related documents.) 478.65 461.35 P
0.42 (Part I also describes how) 221.4 449.35 P
3 F
0.42 (HST) 325.97 449.35 P
0 F
0.42 ( proposals are processed for review by the T) 343.75 449.35 P
0.42 (elescope) 523.57 449.35 P
1.41 (Allocation Committee \050T) 221.4 437.35 P
1.41 (AC\051 and how successful proposals get turned into com-) 324.53 437.35 P
0.06 (mands that the spacecraft can execute; and it describes how the installation of COS-) 221.4 425.35 P
(T) 221.4 413.35 T
(AR af) 226.71 413.35 T
(fects the GHRS and what the basic properties of the instrument are.) 250.69 413.35 T
0.16 (Part II elaborates on the writing of proposals to use the GHRS, both for Phase I and) 221.4 398.35 P
0.63 (Phase II. The Phase I proposal is what the T) 221.4 386.35 P
0.63 (AC sees, and it describes the observa-) 402.33 386.35 P
0.14 (tions to be made in broad terms. The most important technical decisions to be made) 221.4 374.35 P
0.89 (regard the tar) 221.4 362.35 P
0.89 (get acquisition strategy to adopt and the amount of exposure time to) 276.31 362.35 P
1.5 (request. The Phase II proposal encompasses all the details that the planning and) 221.4 350.35 P
(scheduling systems need to turn your program into commands for the spacecraft.) 221.4 338.35 T
1.21 (Part III is a reference section, and it includes the details that a) 221.4 323.35 P
3 F
1.21 (Handbook) 485.96 323.35 P
0 F
1.21 ( should) 527.62 323.35 P
(without cluttering the introductory explanations.) 221.4 311.35 T
(Part IV is a short glossary of GHRS terms and abbreviations and an index.) 221.4 296.35 T
0.49 (Data reduction and analysis are not covered in this) 207 276.35 P
3 F
0.49 (Handbook) 416.09 276.35 P
0 F
0.49 ( because they are treated) 457.75 276.35 P
0.9 (in detail in the) 207 264.35 P
3 F
0.9 (HST Data Handbook,) 270.62 264.35 P
0 F
0.9 (although we anticipate mer) 362.77 264.35 P
0.9 (ging portions of that) 473.9 264.35 P
(document into this in the future.) 207 252.35 T
-0.14 (External references have been included where appropriate in order not to duplicate what) 207 232.35 P
-0.1 (is available elsewhere, but we have tried to include almost everything you need to know) 207 220.35 P
0.37 (about the GHRS when writing a proposal. If you \336nd that you need information that is) 207 208.35 P
(not in here, please consult with us.) 207 196.35 T
0.22 (This document follows the usual STScI convention in which terms, words, and phrases) 207 176.35 P
0.19 (which are to be entered by the user in a literal way on a form are shown in a typewriter) 207 164.35 P
(font \050e.g.,) 207 152.35 T
9 F
(BRIGHT=RETURN,EARLY ACQ) 248.38 152.35 T
0 F
(\051.) 386.38 152.35 T
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2 9 Q
(Preliminaries and Essential Reading) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(8) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 671.02 540 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 672.52 540 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 672.52 180 672.52 2 L
0 Z
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0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(1.2) 163.32 678.02 T
(Changes since the previous version) 189 678.02 T
2 10 Q
(1.2.1) 157.76 644.35 T
(This Handbook) 189 644.35 T
0 F
0.94 (This version of the) 189 624.35 P
3 F
0.94 (GHRS) 270.54 624.35 P
0.94 (Instrument) 299.54 624.35 P
0.94 (Handbook) 346.31 624.35 P
0 F
0.94 ( has been only modestly rewritten. It) 387.97 624.35 P
1.85 (incorporates a few updates since version 4.0 that were issued electronically) 189 612.35 P
1.85 (. Please) 507.6 612.35 P
0.14 (bring errors to the attention of a GHRS Instrument Scientist \050see back of title page\051. As) 189 600.35 P
0.06 (before, wavelength units in this) 189 588.35 P
3 F
0.06 (Handbook) 317.62 588.35 P
0 F
0.06 ( are in \201ngstroms \050\201\051, in keeping with astro-) 359.28 588.35 P
(nomical tradition. A transition to SI units may take place in a future edition.) 189 576.35 T
2 F
(1.2.2) 157.76 546.35 T
(Side 1 A) 189 546.35 T
(vailability) 228.09 546.35 T
0 F
1.64 (At the time this is written, the capabilities of Side 1 of the GHRS have been fully) 189 526.35 P
1.86 (restored, permitting one to obtain high-, medium-, or low-resolution spectra with a) 189 514.35 P
0.34 (cesium iodide photocathode. W) 189 502.35 P
0.34 (e encourage you to consider its use. The low-resolution) 315.89 502.35 P
-0.07 (mode on Side 1 using grating G140L particularly makes the GHRS useful for observing) 189 490.35 P
1.36 (faint objects in the far ultraviolet. The next two paragraphs discuss issues related to) 189 478.35 P
(acquiring such tar) 189 466.35 T
(gets.) 260.47 466.35 T
2 F
(1.2.3) 157.76 436.35 T
(Acquiring Extended Objects with the GHRS) 189 436.35 T
0 F
2.07 (An) 189 416.35 P
9 F
4.97 (EXTENDED) 205.79 416.35 P
0 F
2.07 ( option for) 253.79 416.35 P
9 F
4.97 (ACQ/PEAKUP) 304.72 416.35 P
0 F
2.07 ( was described in earlier versions of this) 364.72 416.35 P
3 F
2.07 (Handbook.) 189 404.35 P
0 F
2.07 (It will be tested in Cycle 4 and should be available for routine use in) 237.73 404.35 P
1.12 (Cycle) 189 392.35 P
1.12 (5. It was written with the Gallilean satellites of Jupiter in mind, but should be) 214.83 392.35 P
(applicable to other extended objects. See Section) 189 380.35 T
(4.1.5.4 on page) 387.3 380.35 T
(39 for more details.) 451.18 380.35 T
1.32 (W) 189 360.35 P
1.32 (e have also provided some guidance for users who may wish to observe extended) 197.64 360.35 P
(objects so that acquisition count rates can be estimated; see Section) 189 348.35 T
(7.3 on page) 460.91 348.35 T
(76.) 509.79 348.35 T
2 F
(1.2.4) 157.76 318.35 T
(Acquiring Faint Objects with the GHRS or FOS) 189 318.35 T
0 F
-0.01 (In some cases the G140L grating on Side 1 may provide an ef) 189 298.35 P
-0.01 (\336cient means of obtaining) 435.87 298.35 P
1.89 (a low-resolution spectrum of a source, but acquiring that object can be dif) 189 286.35 P
1.89 (\336cult or) 506.72 286.35 P
-0.06 (impossible with the GHRS\325 Side 1 because of the limited response of mirror N1 and the) 189 274.35 P
-0.04 (maximum permissible) 189 262.35 P
9 F
-0.1 (STEP-TIME) 280.59 262.35 P
0 F
-0.04 ( of 12.75 seconds. There are two ways to overcome) 334.59 262.35 P
(this problem:) 189 250.35 T
10 11 Q
(\245) 189 232.35 T
0 10 Q
0.28 (Acquire the object with Side 2 of the GHRS \050mirror N2\051, then observe with Side 1.) 203.4 232.35 P
-0.15 (Using this technique will add about 40 minutes of overhead time involved in switch-) 203.4 220.35 P
(ing Sides, but often that can occur when the spacecraft is behind the earth anyway) 203.4 208.35 T
(.) 530.73 208.35 T
10 11 Q
(\245) 189 193.35 T
0 10 Q
0.28 (Acquire the object with the Faint Object Spectrograph and then move it to the LSA) 203.4 193.35 P
1.14 (of the GHRS. The positions of the COST) 203.4 181.35 P
1.14 (AR mirrors for the FOS and GHRS are) 375.61 181.35 P
0.36 (quite close, so that the movement of an object from an FOS aperture to the LSA of) 203.4 169.35 P
0.59 (the GHRS is only about 1 arcmin, a small enough motion to ensure that the object) 203.4 157.35 P
1.26 (will fall within the LSA because one set of guide stars will suf) 203.4 145.35 P
1.26 (\336ce. This method) 467.76 145.35 P
(should) 203.4 133.35 T
3 F
(not) 232.57 133.35 T
0 F
( be used for SSA observations.) 245.35 133.35 T
0.14 (At the time this is being written this method of cross-spectrograph acquisitions is being) 189 113.35 P
-0.1 (evaluated and tested. Please consult with us if you wish to consider using it. Also please) 189 101.35 P
FMENDPAGE
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[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (9) 552.44 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Preliminaries and Essential Reading) 207 736.18 T
0 10 Q
0.17 (note that the opposite sense will also work, namely acquiring a \322bright\323 object with the) 207 679.35 P
(GHRS in order to observe it with the FOS.) 207 667.35 T
2 F
(1.2.5) 175.76 637.35 T
(Noise Rejection for V) 207 637.35 T
(ery Faint Objects) 307.03 637.35 T
0 F
1.48 (A special commanding option called) 207 617.35 P
9 F
3.55 (FLYLIM) 363.54 617.35 P
0 F
1.48 ( can be invoked to reject noise in the) 399.54 617.35 P
-0.11 (GHRS when the object observed is signi\336cantly fainter than the level of the background) 207 605.35 P
-0.03 (noise. Although only applicable in special situations, it can be very ef) 207 593.35 P
-0.03 (fective. Please see) 485.04 593.35 P
(Section) 207 581.35 T
(8.6.3 on page) 239.5 581.35 T
(97.) 295.88 581.35 T
2 F
(1.2.6) 175.76 551.35 T
(The Proposal Process for Cycle 5) 207 551.35 T
0 F
0.16 (The basic methodology of proposal writing for) 207 531.35 P
3 F
0.16 (HST) 397.8 531.35 P
0 F
0.16 ( has been changed. Y) 415.58 531.35 P
0.16 (ou should rely) 500.46 531.35 P
0.62 (on the proposal instructions being issued with this) 207 519.35 P
3 F
0.62 (Handbook) 414.7 519.35 P
0 F
0.62 ( for guidance if there are) 456.36 519.35 P
0.95 (any con\337icts, but the essential information needed \050sequence of operations and expo-) 207 507.35 P
(sure times\051 has not changed.) 207 495.35 T
2 F
(1.2.7) 175.76 465.35 T
(Updated Instrument Parameters) 207 465.35 T
0 F
2.38 (Because of the Servicing Mission, the GHRS is a brand-new instrument in many) 207 445.35 P
0.95 (respects. W) 207 433.35 P
0.95 (e have undertaken to measure many basic instrumental quantities, such as) 253.8 433.35 P
0.37 (sensitivities,) 207 421.35 P
3 F
0.37 (ab) 259.6 421.35 P
0.37 (initio) 272.47 421.35 P
0 F
0.37 ( so that observations obtained in Cycle 4 and beyond can be cali-) 293.59 421.35 P
0.69 (brated to the best possible level. Many of those observations were not been fully ana-) 207 409.35 P
0.72 (lyzed at the time this) 207 397.35 P
3 F
0.72 (Handbook) 296.45 397.35 P
0 F
0.72 ( was last revised before issuance. The numeric values) 338.11 397.35 P
0.1 (herein, particularly sensitivities, are therefore not \322\336nal\323 values that will be in place for) 207 385.35 P
0.34 (data reduction, but they do re\337ect our knowledge of the post-Servicing Mission GHRS) 207 373.35 P
0.16 (and will therefore lead to reliable exposure estimates. Updated information will be pro-) 207 361.35 P
(vided on STEIS as it becomes available.) 207 349.35 T
2 F
(1.2.8) 175.76 319.35 T
(GHRS Sensitivity) 207 319.35 T
0 F
0.14 (The sensitivity of the GHRS has turned out to be more wavelength-dependent than was) 207 303.35 P
0.46 (anticipated prior to the Servicing Mission; see Section) 207 291.35 P
0.46 (8.1 on page) 429.63 291.35 P
0.46 (82. The reasons for) 479.43 291.35 P
-0.11 (this are not known, but users should use the measured sensitivity values in Section) 207 279.35 P
-0.11 (8.2.3) 538 279.35 P
0.85 (on page) 207 267.35 P
0.85 (85 and Section) 241.73 267.35 P
0.85 (8.3.1 on page) 305.38 267.35 P
0.85 (87 when calculating exposure times and should) 363.46 267.35 P
(de\336nitely) 207 255.35 T
3 F
(not) 247.28 255.35 T
0 F
( scale exposures from older proposals.) 260.06 255.35 T
2 F
(1.2.9) 175.76 225.35 T
(GHRS Aperture Nomenclature) 207 225.35 T
0 F
0.37 (The plate scale at the entrance apertures of the GHRS is altered by COST) 207 205.35 P
0.37 (AR such that) 505.05 205.35 P
0.22 (the angular scale per unit of physical length is reduced by a factor of 0.87. \050COST) 207 193.35 P
0.22 (AR\325) 537.44 193.35 P
0.22 (s) 554.11 193.35 P
0.03 (mirrors also introduce anamorphic magni\336cation, but its ef) 207 181.35 P
0.03 (fect is so small \320 about 0.5%) 442.55 181.35 P
1.14 (\320 that it is ignored here.\051 That means that the aperture sizes change in the following) 207 169.35 P
(way:) 207 157.35 T
2 8 Q
(Aperture) 211.3 135.68 T
(Nomenclature) 341.16 135.68 T
-0.2 (Pre-COST) 425.19 135.68 P
-0.2 (AR Size) 462.38 135.68 P
(New Size) 503.96 135.68 T
0 9 Q
(Lar) 211.3 121.02 T
(ge Science Aperture \050LSA\051) 223.63 121.02 T
9 F
(2.0) 369.07 121.02 T
0 F
(2.00 arcsec) 438.34 121.02 T
(1.74 arcsec) 503.96 121.02 T
(Small Science Aperture \050SSA\051) 211.3 106.02 T
9 F
(0.25) 366.37 106.02 T
0 F
(0.25 arcsec) 438.34 106.02 T
(0.22 arcsec) 503.96 106.02 T
205.3 147.77 205.3 101.27 2 L
V
0.5 H
0 Z
N
335.16 148.27 335.16 100.77 2 L
V
N
419.19 148.27 419.19 100.77 2 L
V
N
497.96 148.27 497.96 100.77 2 L
V
N
553.72 147.77 553.72 101.27 2 L
V
N
205.05 148.02 553.97 148.02 2 L
V
N
205.05 131.02 553.97 131.02 2 L
V
2 H
N
205.05 101.02 553.97 101.02 2 L
V
0.5 H
N
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Preliminaries and Essential Reading) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(10) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
-0.17 (Note that the names used to designate the apertures of the GHRS have not changed even) 189 679.35 P
0.58 (though their angular sizes did. T) 189 667.35 P
0.58 (o lessen confusion somewhat, we will use \322LSA\323 and) 320.64 667.35 P
(\322SSA\323 to refer to the lar) 189 655.35 T
(ge and small apertures, respectively) 285.74 655.35 T
(, of the GHRS.) 428.11 655.35 T
54 612.02 540 615.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 613.52 540 613.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 613.52 180 613.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(1.3) 163.32 619.02 T
(Where to \336nd additional information, changes, errata, etc.) 189 619.02 T
0 10 Q
0.19 (As we mentioned, the) 189 595.35 P
3 F
0.19 (Call for Pr) 279.48 595.35 P
0.19 (oposals) 323.4 595.35 P
0 F
0.19 ( provides an overview of) 353.96 595.35 P
3 F
0.19 (HST) 456.84 595.35 P
0 F
0.19 ( capabilities and) 474.62 595.35 P
1.92 (describes how a Phase I proposal is to be prepared. It goes hand-in-hand with the) 189 583.35 P
3 F
-0.06 (Phase) 189 571.35 P
-0.06 (I Pr) 215.94 571.35 P
-0.06 (oposal Instructions) 231.34 571.35 P
0 F
-0.06 ( and documents for the Remote Proposal Submission Sys-) 308.24 571.35 P
0.2 (tem \050RPSS\051. If your proposal is successful, you will need to submit a Phase II proposal) 189 559.35 P
2.28 (that provides all the speci\336c details we need to ensure that your observations are) 189 547.35 P
0.25 (obtained in the form you intend. This) 189 535.35 P
3 F
0.25 (Handbook) 342.41 535.35 P
0 F
0.25 ( provides much of the information you) 384.07 535.35 P
0.64 (will need in Phase II, with the proposal procedures themselves in a) 189 523.35 P
3 F
0.64 (Phase II Pr) 466.33 523.35 P
0.64 (oposal) 513.33 523.35 P
0.29 (Instructions) 189 511.35 P
0 F
0.29 (book. There is also a separate document that describes how to process and) 239.57 511.35 P
2.08 (reduce GHRS data. Contact the User Support Branch of STScI for further details.) 189 499.35 P
0.6 (\050Please note, incidentally) 189 487.35 P
0.6 (, that the) 290.37 487.35 P
3 F
0.6 (T) 329.38 487.35 P
0.6 (ar) 334.02 487.35 P
0.6 (get Acquisition Handbook) 342.54 487.35 P
0 F
0.6 (is no longer produced) 451.27 487.35 P
(because it is redundant.\051) 189 475.35 T
0.62 (There is a separate document titled) 189 455.35 P
3 F
0.62 (HST Data Handbook) 334.88 455.35 P
0 F
0.62 (that describes how) 423.67 455.35 P
3 F
0.62 (HST) 502.44 455.35 P
0 F
0.62 ( data) 520.22 455.35 P
0.75 (are reduced by the \322pipeline\323 system and how you can reproduce those steps to tailor) 189 443.35 P
(the reduction to your needs. A copy may be obtained from the User Support Branch.) 189 431.35 T
1.01 (This) 189 411.35 P
3 F
1.01 ( Instrument Handbook) 206.78 411.35 P
0 F
1.01 (is written to apply to the Goddard High Resolution Spec-) 302.3 411.35 P
0.97 (trograph as it will be con\336gured and will operate in Cycle 5 of the) 189 399.35 P
3 F
0.97 (HST) 469.19 399.35 P
0 F
0.97 ( science pro-) 486.97 399.35 P
1.24 (gram. The installation of COST) 189 387.35 P
1.24 (AR has changed the dimensions of the apertures and) 320.11 387.35 P
0.7 (other elements of GHRS as measured in arcsec projected on the sky) 189 375.35 P
0.7 (. The new dimen-) 467.36 375.35 P
-0.06 (sions have been used throughout this document. This) 189 363.35 P
3 F
-0.06 (Handbook) 403.25 363.35 P
0 F
-0.06 ( supersedes all previous) 444.91 363.35 P
0.19 (versions, but if another document con\337icts with this) 189 351.35 P
3 F
0.19 (Handbook) 400.75 351.35 P
0 F
0.19 (, you should use the one) 442.41 351.35 P
(with the most recent date-of-issue.) 189 339.35 T
0.86 (Y) 189 319.35 P
0.86 (ou should also be aware of STEIS, the) 195.22 319.35 P
3 F
0.86 (Space T) 357.89 319.35 P
0.86 (elescope Electr) 389.77 319.35 P
0.86 (onic Information Ser-) 451.62 319.35 P
-0.04 (vice) 189 307.35 P
0 F
-0.04 (. STEIS provides an easy way to check for updates to existing documents and to get) 205.1 307.35 P
3 F
0.55 (HST) 189 295.35 P
0 F
0.55 (-related information and news. T) 205.86 295.35 P
0.55 (o use STEIS,) 338.7 295.35 P
3 F
0.55 (ftp) 395.34 295.35 P
0 F
0.55 (to) 408.95 295.35 P
3 F
0.55 (stsci.edu) 419.77 295.35 P
0 F
0.55 (, enter) 454.49 295.35 P
3 F
0.55 (anonymous) 483.07 295.35 P
0 F
0.55 (as) 531.67 295.35 P
0.17 (the user and your last name as the password. T) 189 283.35 P
0.17 (ransfer the README \336le in the highest-) 376.79 283.35 P
-0.17 (level directory with a) 189 271.35 P
3 F
-0.17 ( get) 273.76 271.35 P
0 F
-0.17 (command to get basic information. V) 290.65 271.35 P
-0.17 (arious subdirectories pro-) 438.13 271.35 P
0.01 (vide details on speci\336c subjects. For more information on STEIS, contact the User Sup-) 189 259.35 P
0.55 (port Branch. The xterm interface to) 189 247.35 P
3 F
0.55 (ftp) 336.41 247.35 P
0 F
0.55 ( called) 346.97 247.35 P
3 F
0.55 (Mosaic) 376.94 247.35 P
0 F
0.55 ( is an especially ef) 406.38 247.35 P
0.55 (fective way to) 482.26 247.35 P
(access STEIS.) 189 235.35 T
-0.14 (Y) 189 215.35 P
-0.14 (ou are always welcome to call us, the STScI GHRS team, to get information when you) 195.22 215.35 P
0.01 (\336nd yourself confused or at a loss. W) 189 203.35 P
0.01 (e prefer e-mail \050to the addresses on the back of the) 337.71 203.35 P
(title page\051, but you may contact us by telephone if you wish.) 189 191.35 T
(Finally) 189 171.35 T
(, you will \336nd some additional sources of information in Chapter 9.) 216.69 171.35 T
54 265.71 180.29 403.3 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 265.71 180.29 403.3 R
6 X
0 0 0 1 0 0 0 K
V
63 274.59 171.29 395.02 R
7 X
V
11 11 Q
0 X
0.3 (Do not use out-of-) 68.76 383.68 P
7.07 (date documents) 68.76 370.68 P
7.34 (as a sour) 68.76 357.68 P
7.34 (ce of) 130.22 357.68 P
1.86 (infor) 68.76 344.68 P
1.86 (mation! If this) 91.95 344.68 P
12 F
10.86 (Handbook) 68.76 331.68 P
11 F
10.86 ( does) 125.46 331.68 P
7.13 (not contain the) 68.76 318.68 P
13.07 (infor) 68.76 305.68 P
13.07 (mation you) 91.95 305.68 P
26.34 (need, please) 68.76 292.68 P
(consult us.) 68.76 279.68 T
63 274.59 171.29 395.02 R
1 H
2 Z
N
54.5 266.21 179.79 402.8 R
0 Z
N
0 0 612 792 C
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[ 1 0 1 0 0 1 0]
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[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (1) 547.43 60.29 P
-2.78 (1) 552.44 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
7 12 Q
1.2 (Chapter 2) 72 677 S
5 24 Q
-0.48 (Instrument Summary \321) 207 677 S
-0.48 (Why Use the GHRS?) 207 647 S
4 12 Q
(2.1) 144 424 T
( Fundamental properties of the instrument) 164.02 424 T
8 F
( 12) 505.32 424 T
4 10 Q
(2.1.1) 162 407.33 T
( Entrance Apertures) 187.02 407.33 T
8 F
( 12) 508.1 407.33 T
4 F
(2.1.2) 162 391.33 T
( Useful W) 187.02 391.33 T
(avelength Range) 229.99 391.33 T
8 F
( 12) 508.1 391.33 T
4 F
(2.1.3) 162 375.33 T
( A) 187.02 375.33 T
(vailable Resolving Powers) 196.29 375.33 T
8 F
( 12) 508.1 375.33 T
4 F
(2.1.4) 162 359.33 T
( Photometric Precision and Accuracy) 187.02 359.33 T
8 F
( 13) 508.1 359.33 T
4 F
(2.1.5) 162 343.33 T
( T) 187.02 343.33 T
(ime Resolution) 195.54 343.33 T
8 F
( 13) 508.1 343.33 T
4 F
(2.1.6) 162 327.33 T
( Operational Complexity) 187.02 327.33 T
8 F
( 13) 508.1 327.33 T
4 12 Q
(2.2) 144 310 T
( A Brief Description of the Instrument and Its Operation) 164.02 310 T
8 F
( 13) 505.32 310 T
4 F
(2.3) 144 292 T
( A Little About How HST and GHRS W) 164.02 292 T
(ork) 369.2 292 T
8 F
( 15) 505.32 292 T
4 F
(2.4) 144 274 T
( GHRS Modes of Operation) 164.02 274 T
8 F
( 17) 505.32 274 T
4 10 Q
(2.4.1) 162 257.33 T
( T) 187.02 257.33 T
(arget Acquisition Mode) 194.8 257.33 T
8 F
( 17) 508.1 257.33 T
4 F
(2.4.2) 162 241.33 T
( Science Data Acquisition Modes) 187.02 241.33 T
8 F
( 19) 508.1 241.33 T
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0 0 0 1 0 0 0 K
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2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Instrument Summary \321 Why Use the GHRS?) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(12) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
0.37 (The Goddard High Resolution Spectrograph was built to obtain high-quality spectra of) 189 679.35 P
1.38 (astronomical sources ef) 189 667.35 P
1.38 (\336ciently) 286.01 667.35 P
1.38 (. The GHRS can also record images of the objects it) 318.14 667.35 P
1.66 (observes, but that is mostly as an adjunct to its spectroscopic properties to con\336rm) 189 655.35 P
(pointing.) 189 643.35 T
54 600.02 540 603.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 601.52 540 601.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 601.52 180 601.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(2.1) 163.32 607.02 T
(Fundamental properties of the instrument) 189 607.02 T
0 10 Q
0.78 (Here we provide a brief overview of the basic properties of the GHRS. Each of these) 189 583.35 P
-0.12 (aspects is described in more detail in the next two chapters. Chapters 6, 7, and 8 provide) 189 571.35 P
(illustrations of the GHRS and tables of instrument parameters.) 189 559.35 T
2 F
(2.1.1) 157.76 529.35 T
(Entrance Apertures) 189 529.35 T
0 F
1.18 (The source to be observed may be centered in a) 189 509.35 P
1.18 (Lar) 393.51 509.35 P
1.18 (ge Science Aperture \050LSA\051 or a) 407.21 509.35 P
1.16 (Small Science Aperture \050SSA\051) 189 497.35 P
0 8 Q
0.93 (1) 314.96 501.35 P
0 10 Q
1.16 (. Because of the installation of COST) 318.96 497.35 P
1.16 (AR, the LSA is) 474.85 497.35 P
1.09 (1.74 arcsec square and the SSA is 0.22 arcsec square, although they retain their pre-) 189 485.35 P
-0.1 (COST) 189 473.35 P
-0.1 (AR names \050) 213.76 473.35 P
9 F
-0.25 (2.0) 261.32 473.35 P
0 F
-0.1 ( and) 279.32 473.35 P
9 F
-0.25 (0.25) 298.55 473.35 P
0 F
-0.1 (, respectively\051. The high-quality images that COST) 322.55 473.35 P
-0.1 (AR) 526.11 473.35 P
0.5 (produces mean that spectra with good spectroscopic resolution result when the LSA is) 189 461.35 P
0.42 (used. The SSA has about 50 to 70% of the throughput of the LSA; using the LSA will) 189 449.35 P
1.46 (degrade resolution by 10 to 20% compared to the SSA because of the wings to the) 189 437.35 P
(instrumental pro\336le.) 189 425.35 T
0.03 (The LSA has a shutter which automatically closes when an observation with the SSA is) 189 405.35 P
(being performed, in order to reduce stray light.) 189 393.35 T
2 F
(2.1.2) 157.76 363.35 T
(Useful W) 189 363.35 T
(avelength Range) 231.41 363.35 T
0 F
0.66 (The GHRS can obtain spectra from about 1) 189 343.35 P
0.66 (150 to 3200 \201. These limits are set by the) 366.84 343.35 P
1.02 (magnesium \337uoride coatings on) 189 331.35 P
3 F
1.02 (HST) 323.63 331.35 P
0 F
1.02 (\325) 341.41 331.35 P
1.02 (s optics and by the nature of the detectors. The) 344.19 331.35 P
3.84 (additional two re\337ections introduced by COST) 189 319.35 P
3.84 (AR\325) 394.88 319.35 P
3.84 (s mirrors signi\336cantly reduce) 411.55 319.35 P
1.25 (throughput at the very shortest wavelengths \050i.e., below L) 189 307.35 P
1.25 (yman-) 429.26 307.35 P
13 F
1.25 (a) 454.81 307.35 P
0 F
1.25 (\051 so that even very) 461.12 307.35 P
-0.22 (bright stars \050e.g.,) 189 295.35 P
13 F
-0.22 (m) 258.34 295.35 P
0 F
-0.22 (Col\051 have failed to produce detectable \337ux below 1) 266.6 295.35 P
-0.22 (150 \201. It is possi-) 469.47 295.35 P
(ble to observe bright stars out to 3400 \201.) 189 283.35 T
2 F
(2.1.3) 157.76 253.35 T
(A) 189 253.35 T
(vailable Resolving Powers) 195.85 253.35 T
0 F
0.14 (W) 189 233.35 P
0.14 (ith Side 1, observations may be made) 198.04 233.35 P
0.14 (from 1) 351.23 233.35 P
0.14 (150 to 1800 \201 at) 377.94 233.35 P
14 F
0.12 (R) 448.36 233.35 P
0 F
0.14 ( = 2,000, 25,000, and) 454.36 233.35 P
-0.2 (80,000 \050gratings G140L, G140M, and Ech-A, respectively\051. W) 189 221.35 P
-0.2 (ith Side 2, the options are) 438.8 221.35 P
14 F
0.29 (R) 189 209.35 P
0 F
0.33 ( = 25,000 from 1) 195 209.35 P
0.33 (150 to 3200 \201 \050G160M, G200M, and G270M\051 and) 263.55 209.35 P
14 F
0.29 (R) 472.92 209.35 P
0 F
0.33 ( = 80,000 from) 478.92 209.35 P
0.29 (1680 to 3400 \201 \050Ech-B\051. For certain applications it can be advantageous to use grating) 189 197.35 P
(G270M to wavelengths as low as 2100 \201 because of its high ef) 189 185.35 T
(\336ciency) 441.56 185.35 T
(.) 472.57 185.35 T
54 130.98 540 160.98 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 138.98 333 138.98 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(1. W) 189 124.98 T
(e will use \322LSA\323 and \322SSA\323 to denote the two science apertures of the GHRS in this docu-) 208.03 124.98 T
-0.13 (ment in order to lessen ambiguity about their apparent size. Note that the of) 189 114.98 P
-0.13 (\336cial nomenclature of) 459.15 114.98 P
(\322) 189 104.98 T
9 F
(2.0) 193 104.98 T
0 F
(\323 and \322) 209.2 104.98 T
9 F
(0.25) 234.68 104.98 T
0 F
(\323 does not change despite the fact that these two apertures are now 1.74 and) 256.28 104.98 T
(0.22 arcsec square respectively) 189 94.98 T
(.) 300.38 94.98 T
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2 H
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0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (13) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Instrument Summary \321 Why Use the GHRS?) 207 736.18 T
2 10 Q
(2.1.4) 175.76 679.35 T
(Photometric Precision and Accuracy) 207 679.35 T
0 F
-0.23 (Routine calibrations on standard stars provide \337ux-calibrated spectra that are accurate to) 207 659.35 P
0.76 (10%) 207 647.35 P
0 8 Q
0.61 (1) 225.33 651.35 P
0 10 Q
0.76 (. Relative \337uxes obtained at dif) 229.33 647.35 P
0.76 (ferent wavelengths should be good to better than) 357.96 647.35 P
0.07 (5%. The repeatability of \337uxes is even better) 207 635.35 P
0.07 (, being better than 1%; i.e., it is possible to) 386.52 635.35 P
0.41 (compare measures of the same wavelength in the same star at dif) 207 623.35 P
0.41 (ferent times to within) 470.95 623.35 P
(1% for observations with the LSA.) 207 611.35 T
1.47 (W) 207 591.35 P
1.47 (ithin a single bandpass \050i.e., one grating setting\051, relative photometric precision is) 216.04 591.35 P
0.75 (limited by photon statistics for S/N < 30 and by detector non-uniformities above that,) 207 579.35 P
1.02 (provided that the detectors are being used within the linear portion of their response.) 207 567.35 P
0.52 (W) 207 555.35 P
0.52 (ith suitable observing strategies, it is possible to achieve relative S/N as high as 900) 216.04 555.35 P
(\050Lambert et al. 1994\051) 207 543.35 T
0 8 Q
(2) 291.98 547.35 T
0 10 Q
(.) 295.98 543.35 T
0.13 (W) 207 523.35 P
0.13 (e have found that the photometric sensitivity of the GHRS has not changed with time) 215.64 523.35 P
(to within 1% or less.) 207 511.35 T
2 F
(2.1.5) 175.76 481.35 T
(T) 207 481.35 T
(ime Resolution) 212.93 481.35 T
0 F
0.59 (Most observers use the GHRS to accumulate photons for the time needed to reach the) 207 461.35 P
0.59 (signal-to-noise they desire. In) 207 449.35 P
9 F
1.42 (ACCUM) 330.74 449.35 P
0 F
0.59 ( mode the exposures may be as short as 0.2 sec-) 360.74 449.35 P
0.65 (onds, although use of standard procedures for improving S/N usually limits exposures) 207 437.35 P
-0 (to no shorter than about 15 seconds. The GHRS has a rapid readout mode \050) 207 425.35 P
9 F
-0.01 (RAPID) 507.17 425.35 P
0 F
-0 (\051 that) 537.17 425.35 P
0.05 (can obtain spectra as often as every 50 milliseconds, but that can only be done by sacri-) 207 413.35 P
(\336cing many features that are important for producing high-quality spectra.) 207 401.35 T
2 F
(2.1.6) 175.76 371.35 T
(Operational Complexity) 207 371.35 T
0 F
-0.24 (The limited availability of memory on the) 207 351.35 P
3 F
-0.24 (HST) 375.58 351.35 P
0 F
-0.24 ( spacecraft means that there exists a max-) 393.36 351.35 P
0.61 (imum number of operating commands that can be in place for a single set of observa-) 207 339.35 P
2.64 (tions. That can be a limit for use of the GHRS in certain cases, described later) 207 327.35 P
(\050Section) 207 315.35 T
(4.6 on page) 242.83 315.35 T
(47\051.) 291.71 315.35 T
72 272.02 558 275.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 273.52 558 273.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 273.52 198 273.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(2.2) 181.32 279.02 T
(A Brief Description of the Instrument and Its Operation) 207 279.02 T
0 10 Q
0.73 (The GHRS has the usual components of an astronomical spectrograph: entrance aper-) 207 255.35 P
1.21 (tures, a collimator) 207 243.35 P
1.21 (, dispersers, camera mirrors, and detectors. There are also a wave-) 281.52 243.35 P
0.04 (length calibration lamp, \337at \336eld lamps, and mirrors to acquire and center objects in the) 207 231.35 P
0.69 (observing apertures. The apertures were described above in basic terms, and are illus-) 207 219.35 P
0.58 (trated in Section) 207 207.35 P
0.58 (6.1 on page) 276.2 207.35 P
0.58 (56. The collimator and camera mirrors are unexceptional) 326.24 207.35 P
-0.19 (and need no further description here \050see Section) 207 195.35 P
-0.19 (6.2 on page) 403.92 195.35 P
-0.19 (60 for details\051. The impor-) 452.41 195.35 P
(tant elements are the dispersers and the detectors.) 207 183.35 T
72 133.98 558 163.98 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 141.98 351 141.98 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(1. Starting in Cycle 4, the routine \337uxes delivered by the pipeline data reduction system are no) 207 127.98 T
-0.19 (longer on the) 207 117.98 P
3 F
-0.19 (IUE) 256.17 117.98 P
0 F
-0.19 ( system but instead have been adjusted to conform to models of the white dwarf) 271.16 117.98 P
(G191B2B. This can produce systematic dif) 207 107.98 T
(ferences when comparing observations.) 362.32 107.98 T
(2. References are listed in Chapter 9.) 207 94.98 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Instrument Summary \321 Why Use the GHRS?) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(14) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
0.3 (The dispersers are mounted on a rotating carrousel, together with several plane mirrors) 189 679.35 P
-0.18 (used for acquisition. The \336rst-order gratings are designated as G140L, G140M, G160M,) 189 667.35 P
1.36 (G200M, and G270M, where \322G\323 indicates a grating, the number indicates the blaze) 189 655.35 P
0.07 (wavelength \050in nm\051, and the \322L\323 or \322M\323 suf) 189 643.35 P
0.07 (\336x denotes a \322low\323 or \322medium\323 resolution) 365.16 643.35 P
0.03 (grating, respectively) 189 631.35 P
0.03 (. The GHRS medium resolution \336rst-order gratings are holographic) 270.03 631.35 P
0.15 (in order to achieve very high ef) 189 619.35 P
0.15 (\336ciency within a limited wavelength region. G140L is a) 315.23 619.35 P
0.57 (ruled grating. The \336rst two \336rst-order gratings, G140L and G140M, have their spectra) 189 607.35 P
0.68 (imaged by mirror Cam-A onto detector D1, which is optimized for the shortest wave-) 189 595.35 P
0.02 (lengths. The other three gratings have their spectra imaged by Cam-B onto detector D2,) 189 583.35 P
0.51 (which works best at wavelengths from about 1700 to 3200 \201, but which is also useful) 189 571.35 P
(down to 1200 \201.) 189 559.35 T
1.28 (The carrousel also has an echelle grating. The higher orders are designated as mode) 189 539.35 P
0.36 (Ech-A, and they are imaged onto D1 by the cross-disperser CD1. The lower orders are) 189 527.35 P
-0.11 (designated as mode Ech-B, and they are directed to D2 by CD2. Finally) 189 515.35 P
-0.11 (, mirrors N1 and) 474.23 515.35 P
0.53 (A1 image the apertures onto detector D1, and mirrors N2 and A2 image onto D2. The) 189 503.35 P
2.36 (\322N\323 mirrors are \322normal,\323 i.e., unattenuated, while the \322A\323 mirrors \050\322attenuated\323\051) 189 491.35 P
0.5 (re\337ect a smaller fraction of the light to the detectors, so as to enable the acquisition of) 189 479.35 P
1.48 (bright stars. \050T) 189 467.35 P
1.48 (o be precise, the mode designated as N1 actually uses the zero-order) 250.43 467.35 P
(image produced by grating G140L.\051) 189 455.35 T
0.31 (Use of the various gratings or mirrors in concert with the camera mirrors produces one) 189 435.35 P
-0.05 (of three kinds of image at the camera focus: 1\051 an image of the entrance aperture, which) 189 423.35 P
-0.25 (may be mapped to \336nd and center the object of interest; 2\051 a single-order spectrum; or 3\051) 189 411.35 P
(a cross-dispersed, two-dimensional echelle spectrum.) 189 399.35 T
-0.04 (The \337ux in these images is measured by Digicon detectors, and the portion of the image) 189 379.35 P
0.51 (plane that is mapped onto the Digicon is determined by magnetic de\337ection coils. The) 189 367.35 P
0.04 (detectors are the heart of the GHRS and they involve subtleties that must be understood) 189 355.35 P
(if the instrument is to be used competently) 189 343.35 T
(.) 358.62 343.35 T
0.9 (First, there are two Digicons: D1 and D2. D1 has a cesium iodide photocathode on a) 189 323.35 P
1.48 (lithium \337uoride window; that makes D1 ef) 189 311.35 P
1.48 (fectively) 368.22 311.35 P
1.48 (\322solar) 407.18 311.35 P
1.48 (-blind,\323 i.e., the enormous) 430.86 311.35 P
0.74 (\337ux of visible-light photons that dominate the spectrum of most stars will produce no) 189 299.35 P
1.49 (signal with this detector) 189 287.35 P
1.49 (, and only far) 288.89 287.35 P
1.49 (-ultraviolet photons \0501) 346.47 287.35 P
1.49 (100 to 1800 \201\051 produce) 438.51 287.35 P
0.15 (electrons that are accelerated by the 23 kV \336eld onto the diodes. D2 has a cesium tellu-) 189 275.35 P
0.35 (ride photocathode on a magnesium \337uoride window) 189 263.35 P
0.35 (. Each Digicon has 512 diodes that) 398.76 263.35 P
0.78 (accumulate counts from accelerated electrons. 500 of those are \322science diodes,\323 plus) 189 251.35 P
(there are \322corner diodes\323 and \322focus diodes\323 \050see Chapter 6\051.) 189 239.35 T
1.71 (Second, both photocathodes have granularity \320 irregularities in response \320 of about) 189 219.35 P
0.39 (0.5% \050rms\051 that can limit the S/N achieved, and there are localized blemishes that pro-) 189 207.35 P
0.02 (duce irregularities of several percent. The Side 1 photocathode also exhibits \322sleeking,\323) 189 195.35 P
-0 (which is slanted, scratch-like features that have an amplitude of 1 to 2% over regions as) 189 183.35 P
2.08 (lar) 189 171.35 P
2.08 (ge as half the faceplate. The ef) 199.37 171.35 P
2.08 (fects of these irregularities could in principle be) 334.11 171.35 P
0.8 (removed by obtaining a \337at \336eld measurement at every position on the photocathode,) 189 159.35 P
0.44 (but that is impractical. Instead, the observing strategy is to rotate the carrousel slightly) 189 147.35 P
-0.01 (between separate exposures and so use dif) 189 135.35 P
-0.01 (ferent portions of the photocathode. This pro-) 357.6 135.35 P
0.85 (cedure is called an) 189 123.35 P
9 F
2.03 (FP-SPLIT) 269.02 123.35 P
0 F
0.85 (, and with it each exposure is divided into two or four) 316.28 123.35 P
-0.18 (separate-but-equal parts, with the carrousel moving the spectrum about 5.2 diode widths) 189 111.35 P
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (15) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Instrument Summary \321 Why Use the GHRS?) 207 736.18 T
0 10 Q
1.82 (each time in the direction of dispersion. These individual spectra can be combined) 207 679.35 P
(together during the reduction phase.) 207 667.35 T
0.96 (Third, the diodes in the Digicons also have response irregularities, but these are very) 207 647.35 P
-0.05 (slight. The biggest ef) 207 635.35 P
-0.05 (fect is a systematic of) 291.1 635.35 P
-0.05 (fset of about 1% in response of the odd-num-) 377.35 635.35 P
1.56 (bered diodes relative to the even-numbered ones. This ef) 207 623.35 P
1.56 (fect can be almost entirely) 446.22 623.35 P
1.39 (defeated by use of the default) 207 611.35 P
9 F
3.33 (COMB) 335.86 611.35 P
0 F
1.39 ( addition procedure.) 359.86 611.35 P
9 F
3.33 (COMB) 446.78 611.35 P
0 F
1.39 ( addition de\337ects the) 470.78 611.35 P
0.18 (spectrum by an integral number of diodes between subexposures and has the additional) 207 599.35 P
1.38 (bene\336t of working around dead diodes in the instrument that would otherwise leave) 207 587.35 P
(image defects.) 207 575.35 T
0.73 (Fourth, the Digicons\325 diodes are only slightly smaller than the image of the SSA pro-) 207 555.35 P
0.48 (duced by the optics, and are lar) 207 543.35 P
0.48 (ger than the point spread function \050PSF\051 for) 334.41 543.35 P
3 F
0.48 (HST) 515.48 543.35 P
0 F
0.48 (. Thus) 532.52 543.35 P
0.72 (the true resolution of the spectrum cannot be realized unless it is adequately sampled.) 207 531.35 P
0.2 (That is done by making the magnetic \336eld move the spectrum by fractions of the width) 207 519.35 P
1 (of a diode, by either half- or quarter) 207 507.35 P
1 (-diode widths, and then storing those as separate) 357.11 507.35 P
1.19 (spectra in the onboard memory) 207 495.35 P
1.19 (. These are mer) 335.52 495.35 P
1.19 (ged into a single spectrum in the data) 400.54 495.35 P
1.44 (reduction phase. The manner in which this is done is speci\336ed by the) 207 483.35 P
9 F
3.45 (STEP-PATT) 504 483.35 P
0 F
0.81 (parameter) 207 471.35 P
0.81 (, described in more detail later) 246.58 471.35 P
0.81 (. The choice of) 371.7 471.35 P
9 F
1.93 (STEP-PATT) 437.4 471.35 P
0 F
0.81 ( also determines) 491.4 471.35 P
(how the background around the spectrum is measured.) 207 459.35 T
0.79 (Defaults exist for these parameters and they have been set to yield the best quality of) 207 439.35 P
1.68 (spectrum for the con\336guration to which they apply \050except for) 207 427.35 P
9 F
4.02 (FP-SPLIT,) 475.38 427.35 P
0 F
1.68 ( which) 529.38 427.35 P
0.85 (must be invoked explicitly\051. Details on the defaults are provided later \050Section) 207 415.35 P
0.85 (4.3 on) 532.15 415.35 P
0.06 (page) 207 403.35 P
0.06 (43\051, but we strongly encourage you to use the defaults unless there are compelling) 228.38 403.35 P
(reasons not to.) 207 391.35 T
72 348.02 558 351.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 349.52 558 349.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 349.52 198 349.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(2.3) 181.32 355.02 T
(A Little About How) 207 355.02 T
6 F
(HST) 317.66 355.02 T
2 F
( and GHRS W) 341.66 355.02 T
(ork) 418.79 355.02 T
0 10 Q
0.5 (Because of the dif) 207 331.35 P
0.5 (\336culties of working with and communicating with a satellite in low-) 280.8 331.35 P
0.66 (earth orbit, and in order to make) 207 319.35 P
3 F
0.66 (HST) 343.23 319.35 P
0 F
0.66 ( more ef) 361.01 319.35 P
0.66 (\336cient, virtually all actions taken by the) 395.46 319.35 P
0.89 (spacecraft are planned weeks in advance. Only a small fraction of) 207 307.35 P
3 F
0.89 (HST) 482.28 307.35 P
0 F
0.89 (\325) 500.06 307.35 P
0.89 (s time can be) 502.84 307.35 P
0.88 (used for real-time actions that are at the discretion of the observer) 207 295.35 P
0.88 (, and even then the) 479.23 295.35 P
-0.14 (realm of possible actions is very limited, being restricted to deciding which object in the) 207 283.35 P
(\336eld should be centered in the aperture before a subsequent observation is begun.) 207 271.35 T
1.15 (This need for detailed planning of) 207 251.35 P
3 F
1.15 (HST) 352.19 251.35 P
0 F
1.15 ( observations lies at the heart of the apparent) 369.97 251.35 P
0.5 (complexity of the use of the spacecraft and its instruments. At the same time, by care-) 207 239.35 P
0.1 (fully laying out every aspect of what you want done you will \336nd yourself with a better) 207 227.35 P
1.28 (understanding of what actually happens and more con\336dence that the desired results) 207 215.35 P
(will be achieved.) 207 203.35 T
1.45 (All) 207 183.35 P
3 F
1.45 (HST) 223.73 183.35 P
0 F
1.45 ( observations begin with an acquisition. An acquisition can be as simple as) 241.51 183.35 P
3.24 (blindly pointing to particular celestial coordinates, although such a procedure is) 207 171.35 P
1.19 (unlikely to succeed with the GHRS because its entrance apertures are small. For the) 207 159.35 P
-0.08 (GHRS, an acquisition usually means a pointing to precisely speci\336ed coordinates, small) 207 147.35 P
0.08 (motions of the telescope in a spiral pattern to sample the region of sky in the vicinity of) 207 135.35 P
0.07 (the coordinates, and then a peakup motion to center a star in the aperture after on-board) 207 123.35 P
-0.19 (software has determined its location. V) 207 111.35 P
-0.19 (ariations include of) 361.58 111.35 P
-0.19 (fsetting from the acquired star) 438.23 111.35 P
-0.04 (to another nearby object or moving the star to the small aperture. In rare cases it may be) 207 99.35 P
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
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0 0 0 1 0 0 0 K
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54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Instrument Summary \321 Why Use the GHRS?) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(16) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
1.91 (necessary to perform an interactive acquisition, in which the observer speci\336es the) 189 679.35 P
0.81 (object in real time. An intermediate possibility is to take an image with one of) 189 667.35 P
3 F
0.81 (HST) 515.55 667.35 P
0 F
0.81 (\325) 533.33 667.35 P
0.81 (s) 536.11 667.35 P
0.32 (cameras \050or with the GHRS itself\051 in advance of the spectroscopic observation \050by one) 189 655.35 P
-0.12 (to two months\051 and to then derive precise coordinates from that image \050an early acquisi-) 189 643.35 P
-0.09 (tion\051. For very faint objects, especially those to be observed with Side 1 of the GHRS, it) 189 631.35 P
0.19 (is possible to acquire the object with the Faint Object Spectrograph before moving it to) 189 619.35 P
(the LSA.) 189 607.35 T
-0.14 (Once the star has been properly positioned in the appropriate aperture of the GHRS, sci-) 189 587.35 P
0.23 (ence observations may begin. In some cases you may wish to use) 189 575.35 P
9 F
0.56 (IMAGE) 455.37 575.35 P
0 F
0.23 ( mode, which) 485.37 575.35 P
0.68 (can map the LSA at ultraviolet wavelengths, but in general this part means dispersing) 189 563.35 P
1.71 (the light with one of the gratings and adding up the counts to form a spectrum. A) 189 551.35 P
9 F
2.13 (RAPID) 189 539.35 P
0 F
0.89 ( mode also exists to record spectra that change on very short time scales. The) 219 539.35 P
-0.03 (GHRS has no independent microprocessor and so depends on the spacecraft\325) 189 527.35 P
-0.03 (s computer) 495.87 527.35 P
1.11 (and memory for control of its operations. One implication of that dependence is that) 189 515.35 P
1.22 (there is a maximum number of commands that can be stored at any one time. Since) 189 503.35 P
0.3 (those commands are generally loaded into the spacecraft only a few times per day) 189 491.35 P
0.3 (, that) 519.7 491.35 P
0.23 (limitation restricts the total number of GHRS exposures that may be made in a 24 hour) 189 479.35 P
1.14 (period. At the same time, image motion within the instrument that is induced by the) 189 467.35 P
0.4 (earth\325) 189 455.35 P
0.4 (s magnetic \336eld \050see Section) 211.77 455.35 P
0.4 (8.6.5 on page) 330.3 455.35 P
0.4 (98\051 is best dealt with by making indi-) 387.48 455.35 P
-0.05 (vidual exposures no longer than about 5 minutes, thereby increasing the total number of) 189 443.35 P
0.49 (exposures you need to make to get a science observation. In some cases these require-) 189 431.35 P
1.94 (ments come into con\337ict and compromises must be made to accommodate science) 189 419.35 P
(goals.) 189 407.35 T
(Some other relevant aspects of scheduling) 189 387.35 T
3 F
(HST) 360.08 387.35 T
0 F
( observations are:) 377.86 387.35 T
10 11 Q
(\245) 189 369.35 T
0 10 Q
0.2 (Objects in most regions of the sky \322rise\323 and \322set\323 and will be available for science) 203.4 369.35 P
0.6 (observations for about half of an orbit \050about 45 to 50 minutes\051. Longer exposures) 203.4 357.35 P
-0.16 (get spread over several orbits, with a reacquisition at the beginning of each orbit, but) 203.4 345.35 P
0.32 (this occurs at no practical cost in science terms since the GHRS\325 detectors are pho-) 203.4 333.35 P
0.08 (ton counters. Some objects sometimes fall within) 203.4 321.35 P
3 F
0.08 (HST\325) 403.41 321.35 P
0 F
0.08 (s Continuous V) 423.97 321.35 P
0.08 (iewing Zones) 485.76 321.35 P
-0.17 (\050CVZs\051, which enables them to be observed for long times at high ef) 203.4 309.35 P
-0.17 (\336ciency; see the) 475.9 309.35 P
3 F
(Call for Pr) 203.4 297.35 T
(oposals) 246.93 297.35 T
0 F
( for details on taking advantage of the CVZs.) 277.49 297.35 T
10 11 Q
(\245) 189 282.35 T
0 10 Q
1.32 (The orbit of) 203.4 282.35 P
3 F
1.32 (HST) 257.63 282.35 P
0 F
1.32 ( passes through the South Atlantic Anomaly \050SAA\051, which is a) 275.41 282.35 P
0.81 (region in which the background count rate is very high. At present the scheduling) 203.4 270.35 P
0.69 (software simply stops the counting of photons during times when the spacecraft is) 203.4 258.35 P
(within the SAA.) 203.4 246.35 T
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
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FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (17) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Instrument Summary \321 Why Use the GHRS?) 207 736.18 T
72 671.02 558 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 672.52 558 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 672.52 198 672.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(2.4) 181.32 678.02 T
(GHRS Modes of Operation) 207 678.02 T
0 10 Q
0.47 (GHRS has several operational modes for tar) 207 654.35 P
0.47 (get acquisition and obtaining science data.) 386.25 654.35 P
(See also Section) 207 642.35 T
(4.1 on page) 275.05 642.35 T
(35 for more discussion of acquisitions.) 323.93 642.35 T
2 F
(2.4.1) 175.76 612.35 T
(T) 207 612.35 T
(arget Acquisition Mode) 212.37 612.35 T
2 9 Q
(2.4.1.1) 170.48 589.02 T
(Onboard Acquisitions) 207 589.02 T
0 10 Q
0.75 (Most tar) 207 568.35 P
0.75 (gets observed with the GHRS can be automatically acquired with an onboard) 241.18 568.35 P
-0.02 (acquisition \050) 207 556.35 P
9 F
-0.04 (ONBOARD) 256.7 556.35 P
-0.04 (ACQ) 301.18 556.35 P
0 F
-0.02 (\051. An onboard tar) 319.18 556.35 P
-0.02 (get acquisition observation consists of dis-) 387.82 556.35 P
0.36 (tinct phases, which are executed in ascending numerical order) 207 544.35 P
0.36 (. Phases 1 and 2 perform) 457.33 544.35 P
0.32 (initialization and internal calibration functions, and need not concern the observer) 207 532.35 P
0.32 (. The) 537.13 532.35 P
0.46 (third phase is called T) 207 520.35 P
0.46 (ar) 296.45 520.35 P
0.46 (get Search. A series of small angle maneuvers, called a \322spiral) 304.04 520.35 P
1.86 (search,\323 scans an area of the sky centered on the initial position. The \337ux coming) 207 508.35 P
2.04 (through the Lar) 207 496.35 P
2.04 (ge Science Aperture \050LSA\051 is measured at each dwell point in the) 273.11 496.35 P
0.49 (search. If the) 207 484.35 P
9 F
1.17 (BRIGHT=RETURN) 262.88 484.35 P
0 F
0.49 ( option has been chosen \050and it is recommended\051, the) 340.88 484.35 P
2.43 (telescope returns to that dwell point which had the greatest number of counts. If) 207 472.35 P
9 F
1.65 (BRIGHT) 207 460.35 P
0 F
0.69 ( and) 243 460.35 P
9 F
1.65 (FAINT) 263.81 460.35 P
0 F
0.69 ( limits have instead been speci\336ed, the \337ux is compared to these) 293.81 460.35 P
-0.09 (upper and lower limits at each step in the spiral, and if the measured value falls between) 207 448.35 P
0.48 (these limits the tar) 207 436.35 P
0.48 (get is assumed to be within the aperture and the search immediately) 281.88 436.35 P
-0.21 (stops. Y) 207 424.35 P
-0.21 (ou may request that a \336eld map be generated at the \336nal dwell point by means of) 238.57 424.35 P
0.04 (the) 207 412.35 P
9 F
0.09 (MAP) 221.76 412.35 P
0 F
0.04 ( optional parameter) 239.76 412.35 P
0.04 (. Y) 317.04 412.35 P
0.04 (ou should be aware, though, that approximately two min-) 328.29 412.35 P
0.28 (utes is required for each map, and that many pointings may be made during the search.) 207 400.35 P
1.01 (\050If you intend to analyze the maps in real time, the search phase must be done as an) 207 388.35 P
-0.18 (interactive acquisition.\051 If you wish to con\336rm the spacecraft\325) 207 376.35 P
-0.18 (s pointing, we recommend) 452.45 376.35 P
2.65 (obtaining an) 207 364.35 P
9 F
6.35 (IMAGE) 264.51 364.35 P
3 F
2.65 (after) 299.66 364.35 P
0 F
2.65 ( the acquisition instead of using the) 318.55 364.35 P
9 F
6.35 (MAP) 481.23 364.35 P
0 F
2.65 ( option \320 see) 499.23 364.35 P
(Chapter) 207 352.35 T
(4.) 241.16 352.35 T
1.17 (The fourth phase is tar) 207 332.35 P
1.17 (get locate \050) 301.5 332.35 P
9 F
2.82 (ACQ/PEAKUP) 348.28 332.35 P
0 F
1.17 (\051. This process measures the precise) 408.28 332.35 P
0.23 (location of the tar) 207 320.35 P
0.23 (get within the aperture, and requests a small angle maneuver to move) 278.32 320.35 P
-0.14 (it to the center) 207 308.35 P
-0.14 (. The \336eld map of the LSA may be made) 263.51 308.35 P
3 F
-0.14 (befor) 427.87 308.35 P
-0.14 (e) 448.61 308.35 P
0 F
-0.14 ( the centering maneuver is) 453.05 308.35 P
1.74 (performed by specifying) 207 296.35 P
9 F
4.18 (MAP=END-POINT) 313.03 296.35 P
0 F
1.74 (. If done) 390.29 296.35 P
3 F
1.74 (after) 431.61 296.35 P
0 F
1.74 ( the centering \050in) 450.5 296.35 P
9 F
4.18 (IMAGE) 528 296.35 P
0 F
-0.04 (mode\051, the map can be helpful for con\336rming that the object was placed precisely in the) 207 284.35 P
-0.05 (center of the aperture) 207 272.35 P
0 8 Q
-0.04 (1) 292.1 276.35 P
0 10 Q
-0.05 (. The \336nal phase of an acquisition is a \337ux measurement in which) 296.1 272.35 P
0.88 (the \337ux entering the GHRS through the \336nal tar) 207 260.35 P
0.88 (get aperture is measured and inserted) 405 260.35 P
0.09 (into the data. After centering, a second maneuver will automatically translate the object) 207 248.35 P
0.45 (to the SSA if that is the aperture speci\336ed for the observation. An) 207 236.35 P
9 F
1.08 (ACQ/PEAKUP) 477.27 236.35 P
0 F
0.45 ( with) 537.27 236.35 P
(\322) 207 224.35 T
9 F
(0.25) 211.44 224.35 T
0 F
(\323 as the speci\336ed aperture will also center the object in the SSA.) 235.44 224.35 T
72 120.98 558 150.98 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 128.98 351 128.98 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
-0.07 (1. Please don\325) 207 114.98 P
-0.07 (t get the wrong impression. Getting an image of the aperture to con\336rm pointing is) 259.61 114.98 P
(rarely necessary or useful and we mention it here mostly for completeness. If you are working in) 207 104.98 T
(a crowded \336eld, it might help to know exactly what was in the aperture after the fact.) 207 94.98 T
FMENDPAGE
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[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
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7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Instrument Summary \321 Why Use the GHRS?) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(18) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
-0.23 (For some kinds of dif) 189 679.35 P
-0.23 (\336cult tar) 273.99 679.35 P
-0.23 (gets an onboard acquisition may not work. Possible causes) 307.18 679.35 P
(might be:) 189 667.35 T
10 11 Q
(\245) 189 649.35 T
0 10 Q
-0.02 (The error in the coordinates is greater than a few arcsec in either declination or right) 203.4 649.35 P
-0.01 (ascension, so that the tar) 203.4 637.35 P
-0.01 (get lies outside the lar) 301.21 637.35 P
-0.01 (gest area that the GHRS can search in) 388.74 637.35 P
(its onboard procedure.) 203.4 625.35 T
10 11 Q
(\245) 189 610.35 T
0 10 Q
-0.05 (The object is a moving tar) 203.4 610.35 P
-0.05 (get whose coordinates could not be predicted with) 307.67 610.35 P
13 F
-0.05 (\261) 511.52 610.35 P
0 F
-0.05 (5 arc-) 517.01 610.35 P
0.11 (sec accuracy when the proposal was written. Features in the atmosphere of a planet,) 203.4 598.35 P
(and comets are possible examples.) 203.4 586.35 T
10 11 Q
(\245) 189 571.35 T
0 10 Q
(The object has a poorly known or unpredictably variable ultraviolet \337ux.) 203.4 571.35 T
10 11 Q
(\245) 189 556.35 T
0 10 Q
0.48 (The tar) 203.4 556.35 P
0.48 (get has nearby neighbors of similar brightness \320 the onboard search process) 232.3 556.35 P
(could center up on the wrong object.) 203.4 544.35 T
10 11 Q
(\245) 189 529.35 T
0 10 Q
1.55 (The object has a spatial extent greater than two arcsec. The automatic centering) 203.4 529.35 P
1.74 (algorithms may not produce acceptable results on objects comparable in size or) 203.4 517.35 P
(lar) 203.4 505.35 T
(ger than the Lar) 213.77 505.35 T
(ge Science Aperture.) 277.18 505.35 T
10 11 Q
(\245) 189 490.35 T
0 10 Q
-0.24 (The object is too faint to get adequate counts with the maximum permissible integra-) 203.4 490.35 P
(tion time of 12.75 seconds.) 203.4 478.35 T
-0.16 (In many cases these problems can be worked around by using an onboard acquisition on) 189 458.35 P
0.26 (a nearby star and then of) 189 446.35 P
0.26 (fsetting to the object of interest, or) 288.69 446.35 P
0.26 (, perhaps, by using the FOS) 427.88 446.35 P
(to acquire before slewing the tar) 189 434.35 T
(get to the GHRS.) 317.95 434.35 T
2 9 Q
(2.4.1.2) 152.48 411.02 T
(Early and Interactive Acquisitions) 189 411.02 T
0 10 Q
-0.18 (Y) 189 390.35 P
-0.18 (ou may choose to obtain an early acquisition \050) 195.22 390.35 P
9 F
-0.44 (EARLY) 378.18 390.35 P
-0.44 (ACQ) 410.5 390.35 P
0 F
-0.18 (\051 image with WFPC2, FOC,) 428.5 390.35 P
0.75 (or GHRS itself. In some cases an acquisition image would be helpful, but the \336eld of) 189 378.35 P
-0.13 (view of the WFPC2 is not needed. Stationary point sources in crowded but recognizable) 189 366.35 P
-0.18 (\336elds would be examples. The GHRS has its own \322\336eld map\323 capability which will pro-) 189 354.35 P
0.35 (duce an image of the sky as seen through the LSA. Each map is a square array of 16) 189 342.35 P
13 F
0.35 ( \264) 531.66 342.35 P
0 F
-0.02 (16 pixels, covering) 189 330.35 P
-0.02 ( arcsec with 0.1) 315.29 330.35 P
-0.02 (1 arcsec spatial resolution. A single \336eld) 377.63 330.35 P
0.22 (map requires a minimum of two minutes to take the data and send it to the ground, and) 189 318.35 P
0.27 (much longer if each point in a spiral search is mapped or if a) 189 306.35 P
9 F
0.64 (STEP-TIME) 437.7 306.35 P
0 F
0.27 ( longer than) 491.7 306.35 P
-0.04 (the default \0500.2 sec\051 is used. One WFPC2 image requires from three to \336ve minutes, but) 189 294.35 P
0.51 (covers a much lar) 189 282.35 P
0.51 (ger area of the sky) 261.17 282.35 P
0.51 (. As a practical matter) 336.43 282.35 P
0.51 (, if more than one \336eld map) 426.11 282.35 P
0.06 (would be needed, a WFPC2 image may be a more ef) 189 270.35 P
0.06 (\336cient choice. The FOC could also) 400.25 270.35 P
(be an appropriate choice for ultraviolet-bright objects.) 189 258.35 T
1.5 (If an interactive acquisition \050) 189 238.35 P
9 F
3.6 (INT) 310.53 238.35 P
3.6 (ACQ) 332.53 238.35 P
0 F
1.5 (\051 is required, the observer must be present at) 350.53 238.35 P
0.64 (STScI, prepared to inspect the image and identify the tar) 189 226.35 P
0.64 (get in a timely fashion. Real-) 420.68 226.35 P
0.2 (time observations are subject to many constraints and are dif) 189 214.35 P
0.2 (\336cult to schedule \050they are) 433.1 214.35 P
0.36 (occasionally impossible\051. Early acquisition should therefore be chosen in preference to) 189 202.35 P
1.02 (interactive acquisition whenever possible. The) 189 190.35 P
3 F
1.02 (HST) 382.41 190.35 P
0 F
1.02 ( \050Phase I\051 Proposal Forms require) 400.19 190.35 P
(justi\336cation of requests for real-time observation.) 189 178.35 T
267.83 327.18 315.29 338.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 268.32 330.35 T
(.) 273.32 330.35 T
(7) 275.82 330.35 T
(4) 280.82 330.35 T
(1) 296.3 330.35 T
(.) 301.3 330.35 T
(7) 303.8 330.35 T
(4) 308.8 330.35 T
13 F
(\264) 288.31 330.35 T
0 0 612 792 C
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[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (19) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Instrument Summary \321 Why Use the GHRS?) 207 736.18 T
2 10 Q
(2.4.2) 175.76 679.35 T
(Science Data Acquisition Modes) 207 679.35 T
0 F
1.5 (There are several modes of science data acquisition, including Accumulation Mode,) 207 659.35 P
0.35 (Rapid Readout Mode, and Image Mode. Each of these modes may be used in conjunc-) 207 647.35 P
(tion with any of the optical con\336gurations described earlier) 207 635.35 T
(.) 443.08 635.35 T
1 F
(Accumulation Mode) 207 615.35 T
0 F
1.94 (Accumulation Mode \050) 207 595.35 P
9 F
4.65 (ACCUM) 299.2 595.35 P
0 F
1.94 (\051 is the normal way of obtaining a spectrum with the) 329.2 595.35 P
0.7 (GHRS. The name refers to the fact that data can be accumulated in the onboard com-) 207 583.35 P
0.59 (puter during a long exposure. All of the features of the \337ight software are available in) 207 571.35 P
0.39 (this mode, making it the most powerful, \337exible, and automatic way to use the GHRS.) 207 559.35 P
1.09 (There are two types of bene\336ts which one can expect by using the \337ight software in) 207 547.35 P
(Accumulation Mode.) 207 535.35 T
0.41 (The \336rst is the ability to make long duration observations with ef) 207 515.35 P
0.41 (fective and automatic) 471.08 515.35 P
0.29 (control of the process. The time varying Doppler shift caused by the orbital velocity of) 207 503.35 P
0.16 (the spacecraft is compensated for automatically) 207 491.35 P
0.16 (. The software constantly monitors a set) 397.36 491.35 P
0.28 (of data quality criteria and can \337ag, reject, or reobserve individual integrations that fail) 207 479.35 P
0.79 (the tests. Finally) 207 467.35 P
0.79 (, the software can suspend the observation during scheduled or unex-) 273.77 467.35 P
0.78 (pected interruptions, such as occultation of the tar) 207 455.35 P
0.78 (get by the Earth or passage through) 411.68 455.35 P
0.07 (the South Atlantic Anomaly) 207 443.35 P
0.07 (, and then resume when the interruption ends. The very low) 319.05 443.35 P
0.19 (background count rate and absence of readout noise in the Digicons make exposures of) 207 431.35 P
0.08 (hours duration feasible, though it is strongly suggested that these be broken into shorter) 207 419.35 P
0.47 (segments to aid in scheduling and protect against catastrophic data loss in the event of) 207 407.35 P
(an unexpected problem.) 207 395.35 T
0.35 (The second category of bene\336ts results from the ability of the software to perform pat-) 207 375.35 P
0.04 (terns of integrations at closely spaced positions on the photocathode, a process which is) 207 363.35 P
1.54 (referred to as substepping. There are four purposes for this. At the beginning of an) 207 351.35 P
0.7 (observation, the software executes a procedure called Spectrum Y Balance \050) 207 339.35 P
9 F
1.69 (SPYBAL) 518.67 339.35 P
0 F
0.7 (\051) 554.67 339.35 P
1.05 (to \336nd the optimum centering of the image on the diode array) 207 327.35 P
1.05 (. This compensates for) 464.3 327.35 P
0.37 (minor changes in the image location due to thermal or electrical drifts. The second use) 207 315.35 P
0.79 (is to make multiple \0502 or 4\051 samples per resolution element \0501 diode width\051 to ensure) 207 303.35 P
0.29 (that the digital data satisfy the Nyquist sampling criterion. This is) 207 291.35 P
3 F
0.29 (very) 474.65 291.35 P
0 F
0.29 ( important when) 491.86 291.35 P
1.13 (the ultimate spectral resolution of narrow features is required. Third, the background) 207 279.35 P
0.97 (adjacent to the spectrum or in the echelle interorder region can be measured. Finally) 207 267.35 P
0.97 (,) 555.5 267.35 P
-0.04 (comb addition allows the ef) 207 255.35 P
-0.04 (fect of small diode-to-diode sensitivity variations to be min-) 317.77 255.35 P
1.09 (imized and eliminates the holes in the data due to a few inoperative channels. When) 207 243.35 P
-0.05 (substepping is used to de\336ne the detailed sampling of the spectrum and background, the) 207 231.35 P
0.1 (data obtained at each step are accumulated into one of up to seven distinct \322bins\323 in the) 207 219.35 P
(memory of the onboard computer) 207 207.35 T
(.) 340.87 207.35 T
0.99 (This overview of the \337ight software features is not exhaustive, but summarizes those) 207 187.35 P
0.83 (capabilities which are immediately relevant to the acquisition of spectra in accumula-) 207 175.35 P
3.24 (tion mode. Several items, namely substepping and exposure control, require the) 207 163.35 P
0.81 (observer to specify certain parameters. These will be described in more detail later in) 207 151.35 P
(this) 207 139.35 T
3 F
(Handbook) 223.95 139.35 T
0 F
(.) 265.61 139.35 T
FMENDPAGE
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2 9 Q
(Instrument Summary \321 Why Use the GHRS?) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(20) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
1 F
(Rapid Readout Mode) 189 679.35 T
(\050sometimes called Dir) 283.17 679.35 T
(ect Downlink\051) 375.19 679.35 T
0 F
0.32 (Rapid Readout Mode \050) 189 659.35 P
9 F
0.76 (RAPID) 281.33 659.35 P
0 F
0.32 (\051 is intended to provide very fast time resolution without) 311.33 659.35 P
2.42 (the overhead times associated with Accumulation Mode. The sample time can be) 189 647.35 P
-0.04 (between 50 ms and 12.75 seconds, in increments of 50 milliseconds \050i.e., 1 to 255 times) 189 635.35 P
-0.22 (50 ms\051. At the end of each integration the data are read out, either directly to the TDRSS) 189 623.35 P
0.43 (satellite or to the spacecraft science data tape recorder) 189 611.35 P
0.43 (. The \337ight software cannot exe-) 407.89 611.35 P
0.44 (cute all of its functions and still allow readouts every 50 ms. When the Rapid Readout) 189 599.35 P
1.54 (Mode is entered, substepping, data quality checks and exposure control features are) 189 587.35 P
0.66 (deactivated. The primary factor governing the choice between) 189 575.35 P
9 F
1.57 (ACCUM) 445.01 575.35 P
0 F
0.66 ( and) 475.01 575.35 P
9 F
1.57 ( RAPID) 492.6 575.35 P
0 F
0.66 ( is) 530.17 575.35 P
0.62 (time resolution. In accumulation mode, the time between exposures can be as short as) 189 563.35 P
0.12 (about one minute. If higher time resolution is required, if the source is bright enough to) 189 551.35 P
1.03 (give useful counts in a shorter integration, and if one is willing to sacri\336ce the \337ight) 189 539.35 P
0.29 (software control, then direct downlink is a useful alternative. In) 189 527.35 P
9 F
0.69 (RAPID) 448.48 527.35 P
0 F
0.29 ( mode, a) 478.48 527.35 P
9 F
0.69 (SAM-) 516 527.35 P
5.38 (PLE-TIME) 189 515.35 P
0 F
2.24 ( of less than 0.33 sec requires the use of the 1 Mb data channel \050see) 237 515.35 P
0.17 (Section) 189 503.35 P
0.17 (4.4 on page) 221.5 503.35 P
0.17 (45\051. Such a high data rate stresses) 270.72 503.35 P
3 F
0.17 (HST\325) 409.67 503.35 P
0 F
0.17 (s data-handling capabilities) 430.23 503.35 P
(and means that only about 20 minutes of observations can be stored.) 189 491.35 T
1 F
(Image Mode) 189 471.35 T
0 F
0.23 (Images may be obtained in this mode by de\337ecting the image of the photocathode over) 189 451.35 P
0.41 (the 0.1) 189 439.35 P
0.41 (1) 216.26 439.35 P
13 F
0.41 (\264) 224.17 439.35 P
0 F
0.41 ( 0.1) 229.66 439.35 P
0.41 (1 arcsec focus diodes. The result is a map similar to that obtained during) 244.7 439.35 P
-0.11 (tar) 189 427.35 P
-0.11 (get acquisition, but without an acquisition being performed. Also, a) 199.37 427.35 P
9 F
-0.26 (MAP) 470.78 427.35 P
0 F
-0.11 ( as part of an) 488.78 427.35 P
-0.25 (acquisition can cover more of the sky than the LSA subtends at one time by small move-) 189 415.35 P
0.29 (ments of the telescope, whereas an) 189 403.35 P
9 F
0.7 (IMAGE) 332.11 403.35 P
0 F
0.29 ( is limited to the 1.74 by 1.74 arcsec area of) 362.11 403.35 P
(the LSA; see Section) 189 391.35 T
(4.2 on page) 275.66 391.35 T
(42.) 324.54 391.35 T
1 F
(WSCAN and OSCAN Modes) 189 371.35 T
0 F
-0.22 (These are really modi\336cations of the) 189 351.35 P
9 F
-0.52 (ACCUM) 336.57 351.35 P
0 F
-0.22 (ulation mode designed for higher ef) 366.57 351.35 P
-0.22 (\336ciency) 508.34 351.35 P
-0.18 (in multiple observations, and they may be requested during Phase II of the proposal pro-) 189 339.35 P
0.54 (cess.) 189 327.35 P
9 F
1.3 (WSCAN) 211.2 327.35 P
0 F
0.54 ( obtains a series of spectra within a given order) 241.2 327.35 P
0.54 (, incrementing by a speci-) 434.24 327.35 P
0.76 (\336ed wavelength increment between each. The result is a spectrum spanning a broader) 189 315.35 P
2.24 (wavelength range than is possible with a single exposure.) 189 303.35 P
9 F
5.37 (OSCAN) 441.34 303.35 P
0 F
2.24 ( works with the) 471.34 303.35 P
0.49 (echelle, and uses the magnetic de\337ection of the Digicon to obtain spectra over a range) 189 291.35 P
0.24 (of echelle orders. The grating carrousel is not rotated, and spectra are obtained at equal) 189 279.35 P
0.95 (values of) 189 267.35 P
3 F
0.95 (m) 229.77 267.35 P
13 F
0.95 (l) 236.99 267.35 P
0 F
0.95 (, where) 242.48 267.35 P
3 F
0.95 (m) 276.3 267.35 P
0 F
0.95 ( is the echelle order) 283.52 267.35 P
0.95 (.) 365.07 267.35 P
9 F
2.27 (OSCAN) 371.01 267.35 P
0 F
0.95 ( is not ordinarily used for science) 401.01 267.35 P
(observations.) 189 255.35 T
FMENDPAGE
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0 0 0 1 0 0 0 K
N
72 445.03 558 445.03 2 L
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72 74.02 558 74.02 2 L
0.25 H
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2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (21) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
7 12 Q
1.2 (Chapter 3) 72 677 S
5 24 Q
-0.48 (Phase I:) 207 677 S
-0.48 (What the T) 207 647 S
-0.48 (AC Sees) 309.29 647 S
4 12 Q
(3.1) 144 424 T
( Essential questions) 164.02 424 T
8 F
( 22) 505.32 424 T
4 F
(3.2) 144 406 T
( Creating an Observation Scenario) 164.02 406 T
8 F
( 23) 505.32 406 T
4 10 Q
(3.2.1) 162 389.33 T
( The Simplest Case: One Spectrum for One Star) 187.02 389.33 T
8 F
( 23) 508.1 389.33 T
4 F
(3.2.2) 162 373.33 T
( Several Spectra for One Star) 187.02 373.33 T
8 F
( 23) 508.1 373.33 T
4 F
(3.2.3) 162 357.33 T
( Spectra of Several Stars) 187.02 357.33 T
8 F
( 24) 508.1 357.33 T
4 F
(3.2.4) 162 341.33 T
( RAPID Mode Observations) 187.02 341.33 T
8 F
( 24) 508.1 341.33 T
4 F
(3.2.5) 162 325.33 T
( Adding Calibrations) 187.02 325.33 T
8 F
( 24) 508.1 325.33 T
4 12 Q
(3.3) 144 308 T
( Specifying T) 164.02 308 T
(arget Acquisition) 232.04 308 T
8 F
( 24) 505.32 308 T
4 10 Q
(3.3.1) 162 291.33 T
( V) 187.02 291.33 T
(ery Bright Stars) 195.92 291.33 T
8 F
( 25) 508.1 291.33 T
4 F
(3.3.2) 162 275.33 T
( Moving T) 187.02 275.33 T
(argets) 229.81 275.33 T
8 F
( 25) 508.1 275.33 T
4 F
(3.3.3) 162 259.33 T
( Crowded Fields) 187.02 259.33 T
8 F
( 25) 508.1 259.33 T
4 F
(3.3.4) 162 243.33 T
( Extended and V) 187.02 243.33 T
(ery Faint Objects) 260.41 243.33 T
8 F
( 26) 508.1 243.33 T
4 F
(3.3.5) 162 227.33 T
( V) 187.02 227.33 T
(ariable Objects) 195.73 227.33 T
8 F
( 26) 508.1 227.33 T
4 12 Q
(3.4) 144 210 T
( Calculating the Exposure T) 164.02 210 T
(ime) 310.97 210 T
8 F
( 26) 505.32 210 T
4 10 Q
(3.4.1) 162 193.33 T
( Sensitivity) 187.02 193.33 T
8 F
( 26) 508.1 193.33 T
4 F
(3.4.2) 162 177.33 T
( Reddening) 187.02 177.33 T
8 F
( 27) 508.1 177.33 T
4 F
(3.4.3) 162 161.33 T
( Background) 187.02 161.33 T
8 F
( 27) 508.1 161.33 T
4 F
(3.4.4) 162 145.33 T
( Scattered light) 187.02 145.33 T
8 F
( 28) 508.1 145.33 T
4 F
(3.4.5) 162 129.33 T
( Signal-to-noise) 187.02 129.33 T
8 F
( 29) 508.1 129.33 T
4 F
(3.4.6) 162 113.33 T
( A Simple Example) 187.02 113.33 T
8 F
( 31) 508.1 113.33 T
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7 FrameSetSepColors
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Phase I: What the T) 189 736.18 T
(AC Sees) 271.35 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(22) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
0.09 (A proposal for the) 189 679.35 P
3 F
0.09 (Hubble Space T) 264.9 679.35 P
0.09 (elescope) 328.04 679.35 P
0 F
0.09 ( is written in two phases. In Phase I, you are) 362.47 679.35 P
0.64 (asked to provide the minimum information needed for the T) 189 667.35 P
0.64 (elescope Allocation Com-) 434.29 667.35 P
-0.01 (mittee and STScI to judge the scienti\336c merit and technical feasibility of what you wish) 189 655.35 P
-0.18 (to do. If your proposal is successful, you will be asked in Phase II to provide the speci\336c) 189 643.35 P
0.35 (details and parameters that are needed to turn your proposal into a series of commands) 189 631.35 P
0.73 (that the spacecraft can execute. At the time this) 189 619.35 P
3 F
0.73 (Handbook) 387.2 619.35 P
0 F
0.73 ( is being written the proce-) 428.86 619.35 P
0.04 (dures for submission of) 189 607.35 P
3 F
0.04 (HST) 285.83 607.35 P
0 F
0.04 ( proposals are under review; consult the) 303.61 607.35 P
3 F
0.04 (Call for Pr) 465.82 607.35 P
0.04 (oposals) 509.44 607.35 P
0 F
0.07 (for the procedures in ef) 189 595.35 P
0.07 (fect. In particular) 282.39 595.35 P
0.07 (, Cycle 5 proposals will ask for time in units of) 351.27 595.35 P
1.13 (orbits instead of total spacecraft time and an orbit calculator has been constructed to) 189 583.35 P
(allow for planning.) 189 571.35 T
-0.17 (These instructions for completing a Phase I proposal are meant to work with the Cycle 5) 189 551.35 P
3 F
(Call for Pr) 189 539.35 T
(oposals) 232.53 539.35 T
0 F
(and) 265.59 539.35 T
3 F
(Phase I Pr) 282.53 539.35 T
(oposal Instructions) 324.93 539.35 T
0 F
(.) 401.88 539.35 T
54 496.02 540 499.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 497.52 540 497.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 497.52 180 497.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(3.1) 163.32 503.02 T
(Essential questions) 189 503.02 T
0 10 Q
(The essential questions you must answer in \336lling out an) 189 479.35 T
3 F
(HST) 418.44 479.35 T
0 F
( proposal form are:) 436.22 479.35 T
10 11 Q
(\245) 189 461.35 T
0 10 Q
(Do I need real-time acquisition for my tar) 203.4 461.35 T
(gets?) 370.13 461.35 T
10 11 Q
(\245) 189 446.35 T
0 10 Q
(How long will my exposures take?) 203.4 446.35 T
10 11 Q
(\245) 189 431.35 T
0 10 Q
(Are standard calibrations adequate for my needs?) 203.4 431.35 T
10 11 Q
(\245) 189 416.35 T
0 10 Q
(Does my science call for any special requirements?) 203.4 416.35 T
(All of these lead up to:) 189 396.35 T
10 11 Q
(\245) 189 378.35 T
0 10 Q
(What is the total number of orbits my program asks for?) 203.4 378.35 T
0.87 (The information you provide on the execution of observations is divided into Phase I) 189 358.35 P
0.27 (and Phase II. Phase I proposal processing takes place before the T) 189 346.35 P
0.27 (AC meets and at that) 455.03 346.35 P
0.03 (time you are asked to provide only the information that they need to arrive at a decision) 189 334.35 P
1.49 (on the scienti\336c merit and feasibility of your proposal. The T) 189 322.35 P
1.49 (AC needs to know) 447.21 322.35 P
1.49 (, of) 525.18 322.35 P
0.75 (course, how much telescope time your program is likely to need. Phase II takes place) 189 310.35 P
0.03 (only after your proposal is successful and at that time you are required to specify all the) 189 298.35 P
1.36 (details needed to transform your observational needs into spacecraft commands, and) 189 286.35 P
(you must do so within the total spacecraft time that you have been allotted.) 189 274.35 T
0.55 (The distinction between Phase I and Phase II is somewhat arbitrary and in some cases) 189 254.35 P
-0.2 (the Phase I forms actually prevent you from supplying information \050such as the entrance) 189 242.35 P
1.33 (aperture to be used\051 that could be helpful in assessing the proposal. The intent is to) 189 230.35 P
0.73 (make writing the Phase I proposal easier) 189 218.35 P
0.73 (, but you may \336nd that your proposal will be) 355.14 218.35 P
-0.25 (better if you understand fully the operation and use of the GHRS right from the start. W) 189 206.35 P
-0.25 (e) 535.56 206.35 P
1.23 (encourage you to think in terms of the Phase II requirements even when writing the) 189 194.35 P
0.53 (Phase I proposal because in most cases that will not require much more work and you) 189 182.35 P
0.26 (may be able to save some time later on. Thus there is information in this section that is) 189 170.35 P
-0.21 (only entered on the Phase II forms but which has been included here to provide a picture) 189 158.35 P
(of how the instrument works.) 189 146.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (23) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Phase I: What the T) 207 736.18 T
(AC Sees) 289.35 736.18 T
72 671.02 558 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 672.52 558 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 672.52 198 672.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(3.2) 181.32 678.02 T
(Creating an Observation Scenario) 207 678.02 T
2 10 Q
(3.2.1) 175.76 644.35 T
(The Simplest Case: One Spectrum for One Star) 207 644.35 T
0 F
0.31 (Let us assume that in answering the above questions you have decided that an onboard) 207 624.35 P
0.61 (acquisition will suf) 207 612.35 P
0.61 (\336ce \050more on that in a moment\051, that standard calibrations are ade-) 284.7 612.35 P
0.45 (quate, and that you wish to obtain a single spectrum of a single star) 207 600.35 P
0.45 (. By specifying the) 481.11 600.35 P
0.74 (resolving power you desire for a particular wavelength, you have, in ef) 207 588.35 P
0.74 (fect, chosen to) 498.48 588.35 P
0.36 (observe with either Side 1 or Side 2 and with a particular grating \050see Chapter 7\051. This) 207 576.35 P
2.55 (simplest of observation scenarios then involves one acquisition sequence and one) 207 564.35 P
9 F
3.15 (ACCUM) 207 552.35 P
0 F
1.31 ( observation. \050An) 237 552.35 P
9 F
3.15 (IMAGE) 313.15 552.35 P
0 F
1.31 ( mode observation may be speci\336ed in place of the) 343.15 552.35 P
9 F
1.12 (ACCUM) 207 540.35 P
0 F
0.47 ( with no loss of generality) 237 540.35 P
0.47 (. A) 342.85 540.35 P
9 F
1.12 (WSCAN) 358.51 540.35 P
0 F
0.47 ( or) 388.51 540.35 P
9 F
1.12 (OSCAN) 402.78 540.35 P
0 F
0.47 ( is just a minor variation on an) 432.78 540.35 P
9 F
(ACCUM) 207 528.35 T
0 F
(. See below for) 237 528.35 T
9 F
(RAPID) 300.04 528.35 T
0 F
(s.\051) 330.04 528.35 T
-0.18 (The choice of Side 1 or Side 2 for obtaining the spectrum need not necessarily force you) 207 508.35 P
0.12 (to that Side for the acquisition; for example, you might wish to observe a cool star with) 207 496.35 P
0.92 (grating G140L on Side 1, but the far ultraviolet \337ux would be too low to acquire the) 207 484.35 P
-0.04 (object with mirror N1. In that case you can use mirror N2; it is permissible to mix Sides) 207 472.35 P
-0.09 (in a scenario, but there may be a cost in observing time for doing so \050see Section) 207 460.35 P
-0.09 (4.1.5.1) 530.5 460.35 P
0.54 (on page) 207 448.35 P
0.54 (38\051. Some dif) 241.42 448.35 P
0.54 (\336cult tar) 297.03 448.35 P
0.54 (gets may be best acquired with the FOS before they are) 331 448.35 P
(observed with the GHRS.) 207 436.35 T
0.63 (For this simple case this sequence of events can be compared to the) 207 416.35 P
3 F
0.63 (Phase I Pr) 487.67 416.35 P
0.63 (oposal) 531.33 416.35 P
(Instructions) 207 404.35 T
0 F
(:) 254.78 404.35 T
10 11 Q
(\245) 207 386.35 T
0 10 Q
(A guide star acquisition.) 221.4 386.35 T
10 11 Q
(\245) 207 371.35 T
0 10 Q
(The tar) 221.4 371.35 T
(get acquisition with the GHRS.) 249.82 371.35 T
10 11 Q
(\245) 207 356.35 T
0 10 Q
(The) 221.4 356.35 T
9 F
(ACCUM) 239.45 356.35 T
0 F
( \050or) 269.45 356.35 T
9 F
(IMAGE) 286.11 356.35 T
0 F
(\051.) 316.11 356.35 T
10 11 Q
(\245) 207 341.35 T
0 10 Q
(Some overhead time to read the observation.) 221.4 341.35 T
2 F
(3.2.2) 175.76 311.35 T
(Several Spectra for One Star) 207 311.35 T
0 F
0.24 (If more than one spectrum is desired for the star) 207 291.35 P
0.24 (, the) 400.68 291.35 P
9 F
0.58 (ACCUM) 420.88 291.35 P
0 F
0.24 (s + overheads are repeated) 450.88 291.35 P
-0.11 (as necessary) 207 279.35 P
-0.11 (, bearing in mind the need to reacquire the star at the start of each orbit. The) 255.94 279.35 P
1.47 (multiple spectra could be either an assortment of wavelengths or repeats at a single) 207 267.35 P
0.33 (wavelength to follow an object in time or to improve signal-to-noise. In all cases over-) 207 255.35 P
(head time must be added for each separate exposure:) 207 243.35 T
10 11 Q
(\245) 207 225.35 T
0 10 Q
(A guide star acquisition.) 221.4 225.35 T
10 11 Q
(\245) 207 210.35 T
0 10 Q
(The tar) 221.4 210.35 T
(get acquisition with the GHRS.) 249.82 210.35 T
10 11 Q
(\245) 207 195.35 T
0 10 Q
(The \336rst) 221.4 195.35 T
9 F
(ACCUM) 257.51 195.35 T
0 F
( or) 287.51 195.35 T
9 F
(IMAGE) 300.84 195.35 T
0 F
(.) 330.84 195.35 T
10 11 Q
(\245) 207 180.35 T
0 10 Q
(Some overhead time to read the observation.) 221.4 180.35 T
10 11 Q
(\245) 207 165.35 T
0 10 Q
(The second) 221.4 165.35 T
9 F
(ACCUM) 269.72 165.35 T
0 F
( or) 299.72 165.35 T
9 F
(IMAGE) 313.05 165.35 T
0 F
(, followed by an overhead allowance.) 343.05 165.35 T
10 11 Q
(\245) 207 150.35 T
0 10 Q
(The third) 221.4 150.35 T
9 F
(ACCUM) 260.84 150.35 T
0 F
(\311) 290.84 150.35 T
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Phase I: What the T) 189 736.18 T
(AC Sees) 271.35 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(24) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
(3.2.3) 157.76 679.35 T
(Spectra of Several Stars) 189 679.35 T
0 F
0.02 (This instance is just multiple versions of the previous case since changing stars requires) 189 659.35 P
1.62 (a new visit, meaning a full guide star acquisition, acquisition of the object into the) 189 647.35 P
(GHRS LSA, etc.) 189 635.35 T
2 F
(3.2.4) 157.76 605.35 T
10 F
(RAPID) 189 605.35 T
2 F
( Mode Observations) 219 605.35 T
9 F
2.45 (RAPID) 189 585.35 P
0 F
1.02 ( mode observations can be planned just as for) 219 585.35 P
9 F
2.45 (ACCUM) 412.88 585.35 P
0 F
1.02 (s. The overhead time is) 442.88 585.35 P
(added only once at the very end of the whole) 189 573.35 T
9 F
(RAPID) 371.18 573.35 T
0 F
( sequence.) 401.18 573.35 T
2 F
(3.2.5) 157.76 543.35 T
(Adding Calibrations) 189 543.35 T
0 F
0.05 (The only kind of calibration exposure that an observer will ordinarily need is one of the) 189 523.35 P
-0.14 (wavelength calibration lamp. An exposure of 30 to 60 seconds is adequate for almost all) 189 511.35 P
1.56 (settings with the \336rst-order gratings; otherwise the exposure is just another) 189 499.35 P
9 F
3.74 (ACCUM) 507.5 499.35 P
0 F
1.56 (.) 537.5 499.35 P
-0.09 (Note that for most applications the information contained in the) 189 487.35 P
9 F
-0.21 (SPYBAL) 445.31 487.35 P
0 F
-0.09 ( that accompa-) 481.31 487.35 P
0.32 (nies each \336rst use of a grating is likely to suf) 189 475.35 P
0.32 (\336ce and a separate wavelength calibration) 370.93 475.35 P
(is super\337uous; see Section) 189 463.35 T
(4.5 on page) 297.33 463.35 T
(46.) 346.21 463.35 T
54 420.02 540 423.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 421.52 540 421.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 421.52 180 421.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(3.3) 163.32 427.02 T
(Specifying T) 189 427.02 T
(arget Acquisition) 259.46 427.02 T
0 10 Q
2.69 (For most situations, a standard onboard acquisition that automatically centers the) 189 403.35 P
0.33 (brightest object in the \336eld into the desired aperture is all that is needed. Such a proce-) 189 391.35 P
-0.15 (dure is especially appropriate for isolated point sources that are beyond our solar system) 189 379.35 P
0.35 (and which have fairly predictable ultraviolet \337uxes, i.e., most stars. In other cases, it is) 189 367.35 P
1.58 (possible to use a variation on the automatic procedure to acquire other objects. For) 189 355.35 P
-0.09 (example, an extended object or some moving objects may be acquired by \336rst automati-) 189 343.35 P
0.11 (cally centering on a nearby pointlike source and then of) 189 331.35 P
0.11 (fsetting to the object of interest.) 412.25 331.35 P
(Some potential problem cases are:) 189 319.35 T
10 11 Q
(\245) 189 301.35 T
0 10 Q
(very bright stars, which can saturate the detectors;) 203.4 301.35 T
10 11 Q
(\245) 189 286.35 T
0 10 Q
(moving tar) 203.4 286.35 T
(gets, such as planets and their satellites;) 246.83 286.35 T
10 11 Q
(\245) 189 271.35 T
0 10 Q
(crowded \336elds, in which the automatic centering procedure might) 203.4 271.35 T
(get confused;) 468.91 271.35 T
10 11 Q
(\245) 189 256.35 T
0 10 Q
(extended objects that do not have a sharply peaked source to center on;) 203.4 256.35 T
10 11 Q
(\245) 189 241.35 T
0 10 Q
0.06 (very faint objects for which few counts would be accumulated in the maximum per-) 203.4 241.35 P
(missible integration time \05012.75 sec\051.) 203.4 229.35 T
10 11 Q
(\245) 189 214.35 T
0 10 Q
1 (objects that are so variable that their brightness relative to nearby objects may be) 203.4 214.35 P
(unpredictable.) 203.4 202.35 T
0.8 (These situations may require an interactive \050or real-time\051 acquisition, although an on-) 189 182.35 P
0.1 (board acquisition may still work in many cases. In an interactive acquisition, the space-) 189 170.35 P
0.22 (craft obtains a picture of the tar) 189 158.35 P
0.22 (get\325) 315.64 158.35 P
0.22 (s \336eld with one of the cameras \050WFPC2 or FOC\051 or) 330.64 158.35 P
0.85 (with the \336eld mapping capability of the GHRS itself. This picture is relayed immedi-) 189 146.35 P
0.28 (ately to STScI where the observer is available to study the image and decide where the) 189 134.35 P
1.04 (telescope should be pointed. Interactive acquisitions are obviously helpful in dif) 189 122.35 P
1.04 (\336cult) 519.44 122.35 P
2.26 (situations, but the requirement for real-time contact between the ground and) 189 110.35 P
3 F
2.26 (HST) 520.46 110.35 P
0 F
2.26 (,) 537.5 110.35 P
0.1 (together with the need to set aside a block of telescope time for the pointing decision to) 189 98.35 P
FMENDPAGE
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612 792 0 FMBEGINPAGE
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[ 1 0 1 0 0 1 0]
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[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (25) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Phase I: What the T) 207 736.18 T
(AC Sees) 289.35 736.18 T
0 10 Q
1.26 (be made, makes interactive acquisitions consume much more spacecraft time than is) 207 679.35 P
2.71 (needed for a standard onboard acquisition. Interactive acquisitions require special) 207 667.35 P
1.87 (scheduling and so require greater) 207 655.35 P
1.87 (-than-average work on the part of the planners of) 347.01 655.35 P
3 F
0.29 (HST\325) 207 643.35 P
0 F
0.29 (s time. Real-time contact with) 227.56 643.35 P
3 F
0.29 (HST) 351.79 643.35 P
0 F
0.29 ( is a limited resource \050it cannot exceed 20% of) 369.57 643.35 P
(the total time\051 which must be reserved for genuine need.) 207 631.35 T
0.57 (A variation on this procedure is to get the \336eld image two months or so in advance of) 207 611.35 P
-0.08 (the time the spectrum will be obtained. This is called an early acquisition \050) 207 599.35 P
9 F
-0.19 (EARLY) 504.25 599.35 P
-0.19 (ACQ) 536.67 599.35 P
0 F
-0.08 (\051) 554.67 599.35 P
0.83 (and it takes more time than an on-board acquisition but much less than an interactive) 207 587.35 P
0.2 (acquisition and imposes no burden of real-time contact. The observer must be prepared) 207 575.35 P
0.83 (to analyze the early acquisition image quickly \050within a week or two\051 if the positions) 207 563.35 P
(from it are to be incorporated into the telescope schedule.) 207 551.35 T
0.09 (If you wish to use either WFPC2 or FOC for early- or interactive acquisitions you must) 207 531.35 P
-0.03 (refer to documents speci\336c to those instruments. Details on the use of the GHRS\325 imag-) 207 519.35 P
(ing capability are provided in the next chapter) 207 507.35 T
(.) 390.58 507.35 T
2 F
(3.3.1) 175.76 477.35 T
(V) 207 477.35 T
(ery Bright Stars) 213.12 477.35 T
0 F
0.14 (When is a star too bright for an onboard acquisition? In practice we are unaware of any) 207 457.35 P
0.06 (real need to use interactive acquisition just because a star is very bright. GHRS acquisi-) 207 445.35 P
0.53 (tions are done with ultraviolet light, so it is the UV \337ux of the star that matters. There) 207 433.35 P
0.09 (are no stars too bright to acquire with the attenuated mirror A1, for example. Even with) 207 421.35 P
-0.05 (Side 2 it is not necessary to specify an interactive acquisition for a very bright star if the) 207 409.35 P
9 F
2.33 (BRIGHT=RETURN) 207 397.35 P
0 F
0.97 ( option is used. Since the few very bright stars which could cause) 285 397.35 P
1.49 (problems are always the brightest point sources in their immediate area, there is no) 207 385.35 P
(apparent reason not to use) 207 373.35 T
9 F
(BRIGHT=RETURN) 313.92 373.35 T
0 F
( with an onboard acquisition.) 391.92 373.35 T
2 F
(3.3.2) 175.76 343.35 T
(Moving T) 207 343.35 T
(argets) 250.15 343.35 T
0 F
1.36 (Sophisticated pointing at moving objects \050i.e., objects within the solar system\051 often) 207 323.35 P
0.7 (requires interactive acquisition to be sure the desired portion of the object\325) 207 311.35 P
0.7 (s surface is) 512.17 311.35 P
0.53 (centered in the observing aperture. There are cases where an on-board acquisition will) 207 299.35 P
1.42 (suf) 207 287.35 P
1.42 (\336ce, especially if the object is small \050essentially point-like\051 and has a well-deter-) 219.04 287.35 P
1.72 (mined orbit. An on-board acquisition can often work well even for a lar) 207 275.35 P
1.72 (ge moving) 513.78 275.35 P
0.31 (object like Jupiter by \336rst centering on a small object nearby whose relative position is) 207 263.35 P
0.02 (well known \050one of Jupiter) 207 251.35 P
0.02 (\325) 315.21 251.35 P
0.02 (s moons, for example\051, and then of) 317.99 251.35 P
0.02 (fsetting to the position of) 457.36 251.35 P
1.36 (interest on the planetary disk. Solar system astronomers may wish to consult with a) 207 239.35 P
(moving-tar) 207 227.35 T
(get specialist at STScI before specifying the acquisition mode.) 251.26 227.35 T
2 F
(3.3.3) 175.76 197.35 T
(Crowded Fields) 207 197.35 T
0 F
0.79 (W) 207 177.35 P
0.79 (ork in crowded \336elds can usually be done by obtaining an early acquisition, so that) 215.64 177.35 P
0.09 (you have an image to work from to specify the object to be observed, an image that has) 207 165.35 P
0.02 (been obtained with) 207 153.35 P
3 F
0.02 (HST) 285.65 153.35 P
0 F
0.02 (\325) 303.43 153.35 P
0.02 (s full spatial resolution. The camera observation is usually best) 306.21 153.35 P
(done at about the same wavelength that the spectroscopic observations will be made.) 207 141.35 T
0.21 (The Point Spread Function \050PSF\051 of the GHRS has been restored by the COST) 207 121.35 P
0.21 (AR mir-) 524.18 121.35 P
1.55 (rors, making it possible to separately observe stars that are very close together) 207 109.35 P
1.55 (. For) 537.55 109.35 P
0.34 (example, in an Early Release Observation in April, 1994, two stars in R136a separated) 207 97.35 P
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Phase I: What the T) 189 736.18 T
(AC Sees) 271.35 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(26) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
-0.21 (by only 0.25 arcsec were observed independently) 189 679.35 P
-0.21 (. One of these stars was only 0.1 arcsec) 384.52 679.35 P
0.19 (from a brighter neighbor) 189 667.35 P
0.19 (. This was done by centering on a bright object in the \336eld and) 287.6 667.35 P
0.01 (then of) 189 655.35 P
0.01 (fsetting to the tar) 216.88 655.35 P
0.01 (gets of interest. W) 284.8 655.35 P
0.01 (e suggest that you consult with us if you wish) 357.36 655.35 P
(to work in crowded \336elds. Also, see Section) 189 643.35 T
(8.6.1 on page) 367.87 643.35 T
(94.) 424.25 643.35 T
2 F
(3.3.4) 157.76 613.35 T
(Extended and V) 189 613.35 T
(ery Faint Objects) 263.47 613.35 T
0 F
0.13 (For most extended objects, it may be possible to of) 189 593.35 P
0.13 (fset from a nearby point source or at) 393.86 593.35 P
1.96 (the least the pointing can be speci\336ed from an early acquisition image. Interactive) 189 581.35 P
1 (acquisitions should be necessary only rarely) 189 569.35 P
1 (. Another method is to acquire the object) 369.7 569.35 P
(with the FOS and then of) 189 557.35 T
(fset to the GHRS\325 LSA.) 289.65 557.35 T
-0.22 (In Cycle 5 observers can use a centering option designed expressly for extended objects,) 189 537.35 P
0.29 (especially uniform ones like the Gallilean satellites of Jupiter) 189 525.35 P
0.29 (. Chapter 4 contains more) 435.78 525.35 P
(information on this option, known as) 189 513.35 T
9 F
(LOCATE) 339.28 513.35 T
(=) 377.78 513.35 T
(EXTENDED) 386.28 513.35 T
0 F
(.) 434.28 513.35 T
2 F
(3.3.5) 157.76 483.35 T
(V) 189 483.35 T
(ariable Objects) 195.12 483.35 T
0 F
-0.14 (Objects whose ultraviolet brightness varied often caused acquisitions to fail when it was) 189 463.35 P
-0.21 (necessary to specify both) 189 451.35 P
9 F
-0.5 (BRIGHT) 291.47 451.35 P
0 F
-0.21 ( and) 327.47 451.35 P
9 F
-0.5 (FAINT) 346.49 451.35 P
0 F
-0.21 ( count limits. The advent of software that) 376.49 451.35 P
0.7 (automatically \336nds the brightest object in the \336eld) 189 439.35 P
9 F
1.68 (\050BRIGHT=RETURN) 397.94 439.35 P
0 F
0.7 (\051 obviates that) 481.94 439.35 P
0.11 (problem in most cases. A variable object in a crowded \336eld might bene\336t from an early) 189 427.35 P
0.47 (acquisition to determine precise coordinates, but an interactive acquisition should gen-) 189 415.35 P
(erally be unnecessary) 189 403.35 T
(.) 274.43 403.35 T
54 360.02 540 363.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 361.52 540 361.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 361.52 180 361.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(3.4) 163.32 367.02 T
(Calculating the Exposure T) 189 367.02 T
(ime) 343.49 367.02 T
2 10 Q
(3.4.1) 157.76 333.35 T
(Sensitivity) 189 333.35 T
0 F
1.07 (The sensitivity of the GHRS and) 189 313.35 P
3 F
1.07 (HST) 328.73 313.35 P
0 F
1.07 ( Optical T) 346.52 313.35 P
1.07 (elescope Assembly \050OT) 388.5 313.35 P
1.07 (A\051, using the) 485.92 313.35 P
-0.19 (LSA, has been determined from observations of stars with known ultraviolet \337uxes. The) 189 301.35 P
0.32 (sensitivity is designated as) 189 289.35 P
0.32 (, and has units of \050counts diode) 310.41 289.35 P
0 8 Q
0.26 (-1) 437.07 293.35 P
0 10 Q
0.32 ( sec) 443.73 289.35 P
0 8 Q
0.26 (-1) 459.33 293.35 P
0 10 Q
0.32 (\051 for each incident) 465.99 289.35 P
0.07 (\050er) 189 277.35 P
0.07 (g cm) 199.92 277.35 P
0 8 Q
0.06 (-2) 219.71 281.35 P
0 10 Q
0.07 ( sec) 226.38 277.35 P
0 8 Q
0.06 (-1) 241.72 281.35 P
0 10 Q
0.07 ( \201\051. It varies as a function of wavelength for each grating. Y) 248.38 277.35 P
0.07 (ou must \336rst) 489.85 277.35 P
0.21 (estimate the intrinsic \337ux of your tar) 189 265.35 P
0.21 (get and then multiply that by the appropriate value) 336.15 265.35 P
-0.19 (of) 189 253.35 P
-0.19 ( to yield an estimate of the count rate to be expected for a particular grating con\336g-) 210.86 253.35 P
0.25 (uration at the chosen wavelength. Sensitivity curves for the \336rst-order gratings are pro-) 189 241.35 P
(vided in Section) 189 229.35 T
(8.2.3 on page) 256.5 229.35 T
(85 and for the echelles in Section) 312.88 229.35 T
(8.3.1 on page) 448.69 229.35 T
(87.) 505.07 229.35 T
0.68 (In the echelle con\336gurations, the sensitivity varies with wavelength across each order) 189 209.35 P
0.68 (.) 537.5 209.35 P
-0.17 (This behavior is characteristic of all echelle spectrographs, and is called the Blaze Func-) 189 197.35 P
0.16 (tion. The basic nature of the variation with wavelength is similar for all orders, and can) 189 185.35 P
0.15 (be parameterized in terms of the product) 189 173.35 P
0.15 (, where) 370.01 173.35 P
3 F
0.15 (m) 402.23 173.35 P
0 F
0.15 ( is the order number and) 409.45 173.35 P
13 F
0.15 (l) 510.32 173.35 P
0 F
0.15 ( is the) 515.81 173.35 P
0.66 (wavelength \050\201\051. The shape of the blaze function, normalized to a peak value of unity) 189 161.35 P
0.66 (,) 537.5 161.35 P
0.05 (and plotted as a function of) 189 149.35 P
0.05 ( is shown in Section) 316.23 149.35 P
0.05 (8.3.3 on page) 399.49 149.35 P
0.05 (91. The sensitivity at) 455.96 149.35 P
0.31 (any wavelength in any order can be estimated by multiplying the peak response of that) 189 137.35 P
1.03 (order by the relative response shown. The blaze function, relative to the center of an) 189 125.35 P
-0.25 (order) 189 113.35 P
-0.25 (, falls as low as 0.25 at the end of the free spectral range and its ef) 209.7 113.35 P
-0.25 (fect should not be) 469.36 113.35 P
(omitted in exposure calculations.) 189 101.35 T
299.19 283.26 310.41 297.19 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(S) 299.69 289.35 T
13 7 Q
(l) 305.07 286.25 T
0 0 612 792 C
199.64 247.26 210.86 261.19 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(S) 200.14 253.35 T
13 7 Q
(l) 205.52 250.25 T
0 0 612 792 C
354.72 169.02 370.01 181.19 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(m) 355.21 173.35 T
13 F
(l) 363.02 173.35 T
0 0 612 792 C
300.94 145.02 316.23 157.19 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(m) 301.44 149.35 T
13 F
(l) 309.25 149.35 T
0 0 612 792 C
FMENDPAGE
%%EndPage: "26" 26
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (27) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Phase I: What the T) 207 736.18 T
(AC Sees) 289.35 736.18 T
2 10 Q
(3.4.2) 175.76 672.36 T
(Reddening) 207 672.36 T
0 F
3.66 (Corrections for ultraviolet extinction in the interstellar medium are included in) 207 652.36 P
0.02 (Section) 207 640.36 P
0.02 (8.5 on page) 239.5 640.36 P
0.02 (93. These are standard values, and their applicability in speci\336c sit-) 288.42 640.36 P
(uations is left to the judgment of the observer) 207 628.36 T
(.) 388.1 628.36 T
2 F
(3.4.3) 175.76 598.36 T
(Background) 207 598.36 T
0 F
-0.18 (There are several potential sources of background counts, including detector dark count,) 207 578.36 P
0.7 (electrical interference or cross talk with devices either within the GHRS or the space-) 207 566.36 P
0 (craft, and ef) 207 554.36 P
0 (fects caused by the char) 254.86 554.36 P
0 (ged particle radiation environment of the) 350.22 554.36 P
3 F
0 (HST) 516.33 554.36 P
0 F
0 ( orbit.) 534.1 554.36 P
1.18 (The intrinsic sources of dark count are very small. During \322thermal vacuum\323 testing) 207 542.36 P
0.25 (prior to launch the detector dark count rates were observed to be approximately 0.0004) 207 530.36 P
0.04 (counts per diode per second. On-orbit, the background is caused primarily by Cerenkov) 207 518.36 P
0.17 (radiation bursts induced in the faceplate of the Digicon by cosmic rays. This causes the) 207 506.37 P
1.01 (actual background to range from) 207 494.37 P
1.01 ( to about four times that, depending on the) 380.17 494.37 P
0.42 (orbital position of) 207 482.37 P
3 F
0.42 (HST) 282.44 482.37 P
0 F
0.42 (. For planning purposes these mean values suf) 299.48 482.37 P
0.42 (\336ce: 0.01) 486.69 482.37 P
0.42 (1 counts) 523.97 482.37 P
0.14 (s) 207 470.37 P
0 8 Q
0.11 (-1) 210.89 474.36 P
0 10 Q
0.14 ( for D2 and 0.008 counts s) 217.55 470.37 P
0 8 Q
0.11 (-1) 324.18 474.36 P
0 10 Q
0.14 ( for D1. The counts appear to be randomly distributed in) 330.85 470.37 P
0.13 (time, so that the \322noise\323 in the dark count is the square root of the total counts accumu-) 207 458.37 P
0.25 (lated during the observation. If one is observing very faint objects with low count rates) 207 446.37 P
0.21 (the background can in\337uence the signal to noise ratio of the data. Formulae for making) 207 434.37 P
1.29 (quantitative estimates of S/N are given in Section) 207 422.37 P
1.29 (3.4.5.1 on page) 416.57 422.37 P
1.29 (29. At the present) 483.03 422.37 P
0.53 (time there are no known sources of interference or cross talk which af) 207 410.37 P
0.53 (fect the detector) 492.52 410.37 P
(count rates.) 207 398.37 T
-0.1 (The GHRS is equipped with both hardware \050automatic\051 and software capabilities to rec-) 207 378.37 P
0.05 (ognize and respond to cosmic ray and trapped particle events. Y) 207 366.37 P
0.05 (ou may invoke the soft-) 462.82 366.37 P
2.82 (ware capability by specifying) 207 354.37 P
9 F
6.76 (CENSOR) 338.8 354.37 P
6.76 (=) 380.12 354.37 P
6.76 (YES) 391.44 354.37 P
0 F
2.82 ( on an Exposure Logsheet line in) 409.44 354.37 P
1.93 (Phase) 207 342.37 P
1.93 (II. This causes rejection of individual) 232.83 342.37 P
9 F
4.63 (STEP-TIME) 396.32 342.37 P
0 F
1.93 ( segments of data if they) 450.32 342.37 P
0.64 (included a speci\336ed number of photons arriving within a short \050) 207 330.37 P
13 F
0.64 (8 m) 468.33 330.37 P
0 F
0.64 (s\051 interval, as hap-) 482.22 330.37 P
0.5 (pens with cosmic rays. Any rejected integration is repeated, so there is no loss of total) 207 318.37 P
0.05 (exposure time. Y) 207 306.37 P
0.05 (ou should only use this anticoincidence rejection on faint tar) 274.69 306.37 P
0.05 (gets, since) 516.29 306.37 P
0.01 (on bright tar) 207 294.37 P
0.01 (gets the interval between actual photon events will be small and real counts) 256.28 294.37 P
0.19 (would be rejected. W) 207 282.37 P
0.19 (e recommend using) 292.31 282.37 P
9 F
0.46 (CENSOR) 373.7 282.37 P
0.46 (=) 412.39 282.37 P
0.46 (YES) 421.09 282.37 P
0 F
0.19 ( only for count rates less than) 439.09 282.37 P
0.24 (about 0.1 counts per diode per second. The expected dark count reduction is a few tens) 207 270.37 P
(of per cent \050For more details on) 207 258.37 T
9 F
(CENSOR) 336.14 258.37 T
0 F
(, see Section) 372.14 258.37 T
(8.6.2 on page) 424.91 258.37 T
(95\051.) 481.29 258.37 T
-0.24 (For extremely faint sources for which the expected count rate is well below the expected) 207 238.37 P
1.73 (dark level, it is possible to use a special commanding option called) 207 226.37 P
9 F
4.16 (FLYLIM) 497.49 226.37 P
0 F
1.73 (. This) 533.49 226.37 P
-0.22 (option, if pertinent to your needs, should be explored with a GHRS Instrument Scientist.) 207 214.37 P
(See also Section) 207 202.37 T
(8.6.3 on page) 275.05 202.37 T
(97.) 331.43 202.37 T
0.06 (An external source of background which can potentially be a problem during the acqui-) 207 182.37 P
1.51 (sition \050and sometimes the observation\051 of faint tar) 207 170.37 P
1.51 (gets is geocoronal L) 417.06 170.37 P
1.51 (yman-) 501.85 170.37 P
13 F
1.51 (a) 527.4 170.37 P
0 F
1.51 (. This) 533.71 170.37 P
(problem and what to do about it are discussed in Section) 207 158.37 T
(7.4.2 on page) 435.59 158.37 T
(80.) 491.97 158.37 T
-0.25 (The \336nal cause of background counts is passage through the dip in the Earth\325) 207 138.37 P
-0.25 (s V) 511.83 138.37 P
-0.25 (an Allen) 524.08 138.37 P
-0.22 (radiation belt called the South Atlantic Anomaly \050SAA\051. SAA passage occurs on 7 of 16) 207 126.37 P
0.01 (daily orbits of) 207 114.37 P
3 F
0.01 (HST) 265.64 114.37 P
0 F
0.01 (. During the most central of these passages, dark count rates increase) 282.68 114.37 P
-0.17 (about two orders of magnitude, to about 1 count per diode per second. A contour around) 207 102.37 P
-0.05 (the SSA which corresponds to 0.02 cts/s/diode is known and no GHRS observations are) 207 90.37 P
345.09 491.2 380.17 505.32 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(4) 345.51 494.37 T
(1) 360.99 494.37 T
(0) 365.99 494.37 T
0 7 Q
(3) 375.26 497.24 T
(\320) 371.49 497.24 T
13 10 Q
(\264) 353.01 494.37 T
0 0 612 792 C
FMENDPAGE
%%EndPage: "27" 27
%%Page: "28" 28
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Phase I: What the T) 189 736.18 T
(AC Sees) 271.35 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(28) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
0.6 (scheduled when the) 189 679.35 P
3 F
0.6 (HST) 272.18 679.35 P
0 F
0.6 ( is within this zone. At the time of this writing the SAA con-) 289.96 679.35 P
(tours for the GHRS are being reviewed to allow for more ef) 189 667.35 T
(\336cient usage.) 427.93 667.35 T
2 F
(3.4.4) 157.76 637.35 T
(Scattered light) 189 637.35 T
0 F
0.29 (The presence of stray and scattered light in a spectrograph is an ef) 189 617.35 P
0.29 (fect which can in\337u-) 456.65 617.35 P
-0.18 (ence the planning and execution of an observation, as well as the reduction and interpre-) 189 605.35 P
0.51 (tation of the data. None of the optical con\336gurations which include \336rst order gratings) 189 593.35 P
-0.03 (has any serious problem with scattered light. The high quality of the imaging optics and) 189 581.35 P
1.05 (holographic dif) 189 569.35 P
1.05 (fraction gratings and the ef) 251.25 569.35 P
1.05 (fectiveness of the baf) 363.02 569.35 P
1.05 (\337es have successfully) 451.25 569.35 P
0.66 (minimized the stray light. On-orbit measurements indicate that it amounts to less than) 189 557.35 P
-0.21 (10) 189 545.35 P
0 8 Q
-0.17 (-3) 199 549.35 P
0 10 Q
-0.21 ( when using the SSA, and at most a few times 10) 205.66 545.35 P
0 8 Q
-0.17 (-3) 399.45 549.35 P
0 10 Q
-0.21 (when using the LSA \050these are in) 407.95 545.35 P
(units of the peak intensity\051.) 189 533.35 T
-0 (In the echelle con\336guration, both the echelle and the cross-dispersers are ruled gratings.) 189 513.35 P
0.85 (This fact, plus the presence of light from sixteen orders simultaneously on the photo-) 189 501.35 P
-0.24 (cathode, results in a detectable level of background radiation. The irradiance on the pho-) 189 489.35 P
0.13 (tocathode due to scattered light \050measured as count rate per unit area\051 amounts to a few) 189 477.35 P
0.37 (percent of the signal in the order) 189 465.35 P
0.37 (. T) 320.61 465.35 P
0.37 (wo factors complicate this ef) 331.39 465.35 P
0.37 (fect. The \336rst is a geo-) 448.2 465.35 P
1.37 (metrical ef) 189 453.35 P
1.37 (fect caused by the fact that the science diodes are 400) 233.23 453.35 P
13 F
1.37 (m) 465.14 453.35 P
0 F
1.37 (m tall, while the) 470.9 453.35 P
0.28 (image of the spectrum is only about 55) 189 441.35 P
13 F
0.28 (m) 349.53 441.35 P
0 F
0.28 (m high. Thus about 1/8 of the diode is illumi-) 355.29 441.35 P
0.88 (nated by the spectrum+background, while the rest is measuring background, meaning) 189 429.35 P
0.79 (that a weak background irradiance is multiplied to the point that a signi\336cant fraction) 189 417.35 P
-0.1 (\050anywhere from 2 to 50%\051 of the gross count rate on a diode may be due to background.) 189 405.35 P
3.27 (The measured scattered light background can be calculated from information in) 189 393.35 P
(Section) 189 381.35 T
(8.3.1 on page) 221.5 381.35 T
(87. It varies signi\336cantly with order number) 277.88 381.35 T
(.) 453.7 381.35 T
1.73 (The second complication arises at the short wavelength ends of the echelle format.) 189 361.35 P
0.64 (Below a wavelength of about 1800 \201 with Echelle B \050or 1250 \201 with Echelle A\051, the) 189 349.35 P
0.75 (spacing between orders is comparable to the length of the diodes, and it is dif) 189 337.35 P
0.75 (\336cult to) 508.41 337.35 P
1.26 (make a clean measurement of a single order) 189 325.35 P
1.26 (. The diode array has four lar) 373.07 325.35 P
1.26 (ge \322corner) 496.82 325.35 P
0.57 (diodes\323 which are long \0501 mm\051 in the direction of the echelle\325) 189 313.35 P
0.57 (s dispersion, but narrow) 442.19 313.35 P
1.3 (\050100) 189 301.35 P
13 F
1.3 (m) 211.13 301.35 P
0 F
1.3 (m\051 in the cross-dispersion direction. These diodes may be used to sample the) 216.89 301.35 P
0.25 (interorder background without the problem of contamination by in order light, but they) 189 289.35 P
0.17 (do not provide any spatial resolution. The) 189 277.35 P
3 F
0.17 (HST) 359.64 277.35 P
0 F
0.17 ( scheduling system will default to use of) 377.42 277.35 P
-0 (the corner diodes when that is appropriate. At a minimum, the time spent measuring the) 189 265.35 P
0.99 (background should be about 10% of the time spent on the spectrum. If the goal is to) 189 253.35 P
1.19 (achieve a very high signal to noise ratio in the net spectrum, it may be necessary to) 189 241.35 P
0.39 (devote a greater fraction of time to the background measurement. Suggestions for esti-) 189 229.35 P
(mating signal to noise ratios are made in the next section.) 189 217.35 T
-0.08 (In order to reduce stray light, there is a shutter over the LSA which automatically closes) 189 197.35 P
1.09 (whenever the SSA is being used for an observation. There is no shutter on the SSA.) 189 185.35 P
1.55 (Thus a wavelength calibration exposure obtained with a bright star in the SSA will) 189 173.35 P
0.4 (result in a combined spectrum of the two because the aperture for the wavelength cali-) 189 161.35 P
0.17 (bration lamp \050SC2\051 is displaced from the SSA in the same sense as the direction of dis-) 189 149.35 P
2.77 (persion. Usually you can subtract the stellar spectrum to recover the wavelength) 189 137.35 P
(calibration.) 189 125.35 T
0.32 (More detailed quantitative information on background and scattered light in the GHRS) 189 105.35 P
(is provided in Section) 189 93.35 T
(8.6.1 on page) 279 93.35 T
(94.) 335.38 93.35 T
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (29) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Phase I: What the T) 207 736.18 T
(AC Sees) 289.35 736.18 T
2 10 Q
(3.4.5) 175.76 679.35 T
( Signal-to-noise) 207 679.35 T
0 F
0.16 (There are several factors which in\337uence the signal to noise, including statistical \050Pois-) 207 659.35 P
0.58 (son\051 noise in the detected spectrum, dark count noise in the detector) 207 647.35 P
0.58 (, scattered light in) 484.6 647.35 P
1.23 (the spectrograph, diode to diode gain variations, and granularity in the photocathode) 207 635.35 P
0.74 (sensitivity) 207 623.35 P
0.74 (. For signal to noise ratios up to approximately 50, statistical \337uctuations in) 247.47 623.35 P
-0.19 (the signal and background will dominate. Diode to diode variations are extremely small,) 207 611.35 P
1.31 (and are accounted for in the routine calibration procedures. Cathode granularity will) 207 599.35 P
-0 (become important if signal to noise greater than 50 is required, and must be treated sep-) 207 587.35 P
0.12 (arately) 207 575.35 P
0.12 (. For sources observed through the small aperture the sky background should not) 233.56 575.35 P
(contribute signi\336cantly to the noise, except, perhaps, when observing at L) 207 563.35 T
(yman-) 501.69 563.35 T
13 F
(a) 527.24 563.35 T
0 F
(.) 533.55 563.35 T
2 9 Q
(3.4.5.1) 170.48 540.02 T
(Photon Noise) 207 540.02 T
0 10 Q
-0.03 (The following equations may be used to estimate signal to noise ratio, depending on the) 207 519.35 P
(relative importance of scattered light and dark count.) 207 507.35 T
2 F
(Case 1) 207 487.35 T
4 F
(. Neither scattered light nor dark count are important.) 239.24 487.35 T
0 F
( Let:) 207 467.35 T
3 F
-0.12 (s) 221.4 449.35 P
0 F
-0.12 (= signal strength \050counts per diode per second\051 estimated by multiplying the stellar) 227.67 449.35 P
(\337ux by the sensitivity at the desired wavelength.) 235.8 437.35 T
3 F
0.03 (t) 221.4 422.35 P
0 F
0.03 ( = duration of the observation in seconds. This total time will be divided among the) 224.18 422.35 P
(separate substep bins.) 235.8 410.35 T
0.2 (= the number of adjacent diodes that will be binned together to produce an ef) 231.5 395.35 P
0.2 (fec-) 542.46 395.35 P
0.4 (tive resolution element. Usually) 235.8 383.35 P
3 F
0.4 (n) 367.66 383.35 P
0 8 Q
0.32 (s) 372.66 380.85 P
0 10 Q
0.4 ( = 1. This is not the mer) 375.78 383.35 P
0.4 (ging of substep bins,) 474.02 383.35 P
0.37 (but the deliberate averaging to increase signal to noise at the expense of resolu-) 235.8 371.35 P
(tion.) 235.8 359.35 T
(Then) 207 339.35 T
0.5 (This formula would be appropriate for relatively bright objects observed with any \336rst) 207 282.34 P
(order grating, when substep pattern 1, 2, or 3 is used \050see Section) 207 270.34 T
(8.4 on page) 470.29 270.34 T
(92\051.) 519.17 270.34 T
2 F
(Case 2) 207 250.34 T
4 F
(. Dark count is important, scattered light is not.) 239.24 250.34 T
0 F
( Let:) 207 230.34 T
3 F
(d) 221.4 212.34 T
0 F
( = dark count rate in counts per diode per second.) 226.4 212.34 T
(Then) 207 192.34 T
0.85 (If the signal is less than about ten times the dark count rate, the factor in parentheses) 207 152.34 P
0.14 (should be included in the estimate. This formula would be useful if) 207 140.34 P
9 F
0.35 (STEP-PATT) 479.55 140.34 P
0 F
0.14 ( 5, for) 533.55 140.34 P
0.26 (example, were used with a \336rst order grating to measure a faint source \050see Section) 207 128.34 P
0.26 (8.4) 545.5 128.34 P
(on page) 207 116.34 T
(92\051.) 240.88 116.34 T
221.4 390.02 231.5 403.19 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(n) 221.9 395.35 T
3 7 Q
(s) 227.28 392.25 T
0 0 612 792 C
72 87.98 558 686.02 C
275.83 299.01 354.17 336.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(S) 281.96 311.39 T
(N) 293.62 311.39 T
13 F
(\244) 289.46 311.39 T
(\050) 277.67 311.39 T
(\051) 300.76 311.39 T
0 7 Q
(2) 306.25 314.27 T
3 10 Q
(s) 325.39 311.39 T
(n) 329.87 311.39 T
3 7 Q
(s) 335.25 308.29 T
3 10 Q
(t) 338.56 311.39 T
0 F
(=) 314.75 311.39 T
72 87.98 558 686.02 C
0 0 612 792 C
207 162.5 450 186.4 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(S) 303.68 172.34 T
(N) 315.35 172.34 T
13 F
(\244) 311.18 172.34 T
(\050) 299.39 172.34 T
(\051) 322.48 172.34 T
0 7 Q
(2) 327.98 175.22 T
3 10 Q
(s) 361.09 178.13 T
(d) 371.65 178.13 T
13 F
(\244) 367.48 178.13 T
0 F
(1) 353.27 165.88 T
3 F
(s) 368.91 165.88 T
(d) 379.46 165.88 T
13 F
(\244) 375.3 165.88 T
0 F
(+) 360.77 165.88 T
(-) 353.27 172.57 T
(-) 354.93 172.57 T
(-) 356.6 172.57 T
(-) 358.27 172.57 T
(-) 359.93 172.57 T
(-) 361.6 172.57 T
(-) 363.26 172.57 T
(-) 364.92 172.57 T
(-) 366.59 172.57 T
(-) 368.26 172.57 T
(-) 369.92 172.57 T
(-) 371.58 172.57 T
(-) 373.25 172.57 T
(-) 374.92 172.57 T
(-) 376.58 172.57 T
(-) 378.24 172.57 T
(-) 379.91 172.57 T
(-) 381.13 172.57 T
13 F
(\350) 347.11 168.43 T
(\370) 385.12 168.43 T
(\346) 347.11 177 T
(\366) 385.12 177 T
3 F
(s) 390.71 172.34 T
(n) 395.19 172.34 T
3 7 Q
(s) 400.57 169.24 T
3 10 Q
(t) 403.89 172.34 T
0 F
(=) 336.47 172.34 T
0 0 612 792 C
FMENDPAGE
%%EndPage: "29" 29
%%Page: "30" 30
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Phase I: What the T) 189 736.18 T
(AC Sees) 271.35 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(30) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
(Case 3) 189 679.35 T
4 F
(. Scattered light is important, dark count is not.) 221.24 679.35 T
0 F
(Let:) 189 659.35 T
3 F
(f) 203.4 641.35 T
0 F
(= fraction of time spent measuring the spectrum. \050See Section) 208.68 641.35 T
(8.4 on page) 458.45 641.35 T
(92\051) 507.33 641.35 T
3 F
(b) 203.4 626.35 T
0 F
( = scattered light as a fraction of the signal in the adjacent orders.) 208.4 626.35 T
(Then) 189 606.35 T
0.75 (This formula gives a good estimate of the performance for observations with the ech-) 189 562.45 P
0.43 (elles when stepping patterns 6, 7, 8 or 9 are used. This formula assumes that the back-) 189 550.45 P
0.98 (ground bins are heavily smoothed. Most of the high frequency statistical noise in the) 189 538.45 P
(background bins is thus suppressed.) 189 526.45 T
2 F
(Case 4) 189 506.45 T
4 F
(. Both scattered light and dark count are important.) 221.24 506.45 T
0 F
(Let:) 189 486.45 T
0.01 (= number of adjacent diodes to smooth the background bins over before subtract-) 214.28 468.45 P
1.5 (ing. Experiments with ground-based data indicate that) 217.8 456.45 P
1.5 ( gives the best) 478.55 456.45 P
(results.) 217.8 444.45 T
(Then) 189 424.45 T
0.19 (There are two ways to use these formulae. If you need a certain S/N to do the scienti\336c) 189 358.37 P
0.7 (analysis, use the appropriate equation to solve for the required exposure time) 189 346.37 P
3 F
0.7 (t) 507.64 346.37 P
0 F
0.7 (. Alter-) 510.42 346.37 P
0.66 (nately) 189 334.37 P
0.66 (, you can decide to devote a \336xed length of time to the observation, and use the) 212.79 334.37 P
(equations to estimate what S/N will be achieved.) 189 322.37 T
2 9 Q
(3.4.5.2) 152.48 299.03 T
(Fixed Pattern Noise) 189 299.03 T
0 10 Q
-0.07 (The formulae just presented suggest that the signal to noise ratio increases in proportion) 189 278.37 P
0.13 (to the square root of the exposure time. These relations only hold true until S/N) 189 266.37 P
13 F
0.13 (\273) 510.92 266.37 P
0 F
0.13 ( 50 or) 516.41 266.37 P
3.23 (so is reached. At higher signal levels the photocathode granularity described in) 189 254.37 P
0.04 (Section) 189 242.37 P
0.04 (4.3 on page) 221.5 242.37 P
0.04 (43 will become the limiting factor) 270.46 242.37 P
0.04 (. Observing standard stars to pro-) 406.49 242.37 P
0.39 (vide a precise \322\337at \336eld\323 observation is too inef) 189 230.37 P
0.39 (\336cient, and there is no onboard contin-) 382.98 230.37 P
-0.1 (uum lamp that illuminates the optics and detectors in exactly the same way as the stellar) 189 218.37 P
0.16 (spectrum. The best practice is to use the) 189 206.37 P
9 F
0.39 (FP-SPLIT) 352.76 206.37 P
0 F
0.16 ( option \050Section) 400.76 206.37 P
0.16 (4.3.1 on page) 467.47 206.37 P
0.16 (43\051.) 524.17 206.37 P
-0.17 (Rather than merely averaging the four) 189 194.37 P
9 F
-0.42 (FP-SPLIT) 342.91 194.37 P
0 F
-0.17 ( sub-exposures, the data analysis pro-) 390.91 194.37 P
0.83 (cedure solves for the two vectors representing photocathode granularity and the spec-) 189 182.37 P
(trum. S/N well in excess of 100 has been obtained this way on bright tar) 189 170.37 T
(gets.) 477.4 170.37 T
-0.1 (Achieving extremely high signal-to-noise \050200 or more\051 is possible by obtaining a num-) 189 150.37 P
1.61 (ber of spectra, each with) 189 138.37 P
9 F
3.87 (FP-SPLIT) 297.57 138.37 P
0 F
1.61 ( but at slightly dif) 345.57 138.37 P
1.61 (ferent grating positions. See) 422.96 138.37 P
(Lambert et al. \0501994\051 for a discussion.) 189 126.37 T
54 87.98 540 686.02 C
254.81 579.11 339.19 603.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(S) 261.56 588.96 T
(N) 273.23 588.96 T
13 F
(\244) 269.06 588.96 T
(\050) 257.27 588.96 T
(\051) 280.36 588.96 T
0 7 Q
(2) 285.86 591.84 T
3 10 Q
(f) 308.98 594.75 T
0 F
(1) 300.05 582.5 T
3 F
(b) 315.68 582.5 T
0 F
(+) 307.54 582.5 T
(-) 300.05 589.2 T
(-) 301.71 589.2 T
(-) 303.38 589.2 T
(-) 305.04 589.2 T
(-) 306.7 589.2 T
(-) 308.37 589.2 T
(-) 310.04 589.2 T
(-) 311.7 589.2 T
(-) 313.36 589.2 T
(-) 315.03 589.2 T
(-) 316.7 589.2 T
(-) 317.35 589.2 T
3 F
(s) 321.47 588.96 T
(n) 325.95 588.96 T
3 7 Q
(s) 331.33 585.86 T
3 10 Q
(t) 334.64 588.96 T
13 F
(\273) 291.86 588.96 T
54 87.98 540 686.02 C
0 0 612 792 C
203.4 463.12 214.28 476.28 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(n) 203.9 468.45 T
3 7 Q
(b) 209.28 465.35 T
0 0 612 792 C
447.19 451.12 478.55 464.28 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(n) 447.68 456.45 T
3 7 Q
(b) 453.07 453.35 T
0 10 Q
(1) 467.05 456.45 T
(0) 472.05 456.45 T
13 F
(\273) 459.06 456.45 T
0 0 612 792 C
54 87.98 540 686.02 C
103.51 375.03 490.49 421.11 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(S) 248.12 403.92 T
(N) 259.79 403.92 T
13 F
(\244) 255.62 403.92 T
(\050) 243.83 403.92 T
(\051) 266.92 403.92 T
0 7 Q
(2) 272.41 406.79 T
3 10 Q
(s) 374.05 409.47 T
0 7 Q
(2) 378.44 412.34 T
3 10 Q
(t) 382.53 409.47 T
(s) 291.75 391.67 T
0 F
(1) 302.39 397.22 T
3 F
(b) 318.02 397.22 T
0 F
(+) 309.89 397.22 T
3 F
(n) 306.97 384.97 T
3 7 Q
(s) 312.35 381.87 T
3 10 Q
(f) 315.66 384.97 T
0 F
(-) 302.39 391.67 T
(-) 304.05 391.67 T
(-) 305.72 391.67 T
(-) 307.38 391.67 T
(-) 309.05 391.67 T
(-) 310.71 391.67 T
(-) 312.38 391.67 T
(-) 314.04 391.67 T
(-) 315.71 391.67 T
(-) 317.37 391.67 T
(-) 319.04 391.67 T
(-) 319.69 391.67 T
3 F
(b) 350.89 397.22 T
(n) 334.06 384.97 T
3 7 Q
(b) 339.44 381.87 T
0 10 Q
(1) 349.49 384.97 T
3 F
(f) 364.49 384.97 T
0 F
(\320) 356.99 384.97 T
13 F
(\050) 345.2 384.97 T
(\051) 367.73 384.97 T
0 F
(-) 334.06 391.67 T
(-) 335.73 391.67 T
(-) 337.39 391.67 T
(-) 339.06 391.67 T
(-) 340.72 391.67 T
(-) 342.39 391.67 T
(-) 344.05 391.67 T
(-) 345.72 391.67 T
(-) 347.38 391.67 T
(-) 349.05 391.67 T
(-) 350.71 391.67 T
(-) 352.38 391.67 T
(-) 354.04 391.67 T
(-) 355.71 391.67 T
(-) 357.37 391.67 T
(-) 359.04 391.67 T
(-) 360.7 391.67 T
(-) 362.37 391.67 T
(-) 364.03 391.67 T
(-) 365.7 391.67 T
(-) 367.36 391.67 T
(-) 369.03 391.67 T
(-) 369.4 391.67 T
(+) 325.72 391.67 T
3 F
(d) 389.02 391.67 T
0 F
(1) 404.01 397.22 T
3 F
(n) 400.77 384.97 T
3 7 Q
(s) 406.15 381.87 T
3 10 Q
(f) 409.47 384.97 T
0 F
(-) 400.77 391.67 T
(-) 402.44 391.67 T
(-) 404.1 391.67 T
(-) 405.77 391.67 T
(-) 407.43 391.67 T
(-) 408.92 391.67 T
(1) 440.12 397.22 T
3 F
(n) 423.28 384.97 T
3 7 Q
(b) 428.66 381.87 T
0 10 Q
(1) 438.71 384.97 T
3 F
(f) 453.71 384.97 T
0 F
(\320) 446.21 384.97 T
13 F
(\050) 434.42 384.97 T
(\051) 456.95 384.97 T
0 F
(-) 423.28 391.67 T
(-) 424.95 391.67 T
(-) 426.61 391.67 T
(-) 428.28 391.67 T
(-) 429.94 391.67 T
(-) 431.61 391.67 T
(-) 433.27 391.67 T
(-) 434.94 391.67 T
(-) 436.6 391.67 T
(-) 438.27 391.67 T
(-) 439.93 391.67 T
(-) 441.6 391.67 T
(-) 443.26 391.67 T
(-) 444.93 391.67 T
(-) 446.59 391.67 T
(-) 448.26 391.67 T
(-) 449.92 391.67 T
(-) 451.59 391.67 T
(-) 453.25 391.67 T
(-) 454.92 391.67 T
(-) 456.58 391.67 T
(-) 458.25 391.67 T
(-) 458.62 391.67 T
(+) 414.95 391.67 T
(+) 380.89 391.67 T
(-) 291.75 403.92 T
(-) 293.41 403.92 T
(-) 295.08 403.92 T
(-) 296.74 403.92 T
(-) 298.41 403.92 T
(-) 300.07 403.92 T
(-) 301.74 403.92 T
(-) 303.4 403.92 T
(-) 305.07 403.92 T
(-) 306.73 403.92 T
(-) 308.4 403.92 T
(-) 310.06 403.92 T
(-) 311.73 403.92 T
(-) 313.39 403.92 T
(-) 315.06 403.92 T
(-) 316.72 403.92 T
(-) 318.39 403.92 T
(-) 320.05 403.92 T
(-) 321.72 403.92 T
(-) 323.38 403.92 T
(-) 325.05 403.92 T
(-) 326.71 403.92 T
(-) 328.38 403.92 T
(-) 330.04 403.92 T
(-) 331.71 403.92 T
(-) 333.37 403.92 T
(-) 335.04 403.92 T
(-) 336.7 403.92 T
(-) 338.37 403.92 T
(-) 340.03 403.92 T
(-) 341.7 403.92 T
(-) 343.36 403.92 T
(-) 345.03 403.92 T
(-) 346.69 403.92 T
(-) 348.36 403.92 T
(-) 350.02 403.92 T
(-) 351.69 403.92 T
(-) 353.35 403.92 T
(-) 355.02 403.92 T
(-) 356.68 403.92 T
(-) 358.35 403.92 T
(-) 360.01 403.92 T
(-) 361.68 403.92 T
(-) 363.34 403.92 T
(-) 365.01 403.92 T
(-) 366.67 403.92 T
(-) 368.34 403.92 T
(-) 370 403.92 T
(-) 371.67 403.92 T
(-) 373.33 403.92 T
(-) 375 403.92 T
(-) 376.66 403.92 T
(-) 378.33 403.92 T
(-) 379.99 403.92 T
(-) 381.66 403.92 T
(-) 383.32 403.92 T
(-) 384.99 403.92 T
(-) 386.65 403.92 T
(-) 388.32 403.92 T
(-) 389.98 403.92 T
(-) 391.65 403.92 T
(-) 393.31 403.92 T
(-) 394.98 403.92 T
(-) 396.64 403.92 T
(-) 398.31 403.92 T
(-) 399.97 403.92 T
(-) 401.64 403.92 T
(-) 403.3 403.92 T
(-) 404.97 403.92 T
(-) 406.63 403.92 T
(-) 408.3 403.92 T
(-) 409.96 403.92 T
(-) 411.63 403.92 T
(-) 413.29 403.92 T
(-) 414.96 403.92 T
(-) 416.62 403.92 T
(-) 418.29 403.92 T
(-) 419.95 403.92 T
(-) 421.62 403.92 T
(-) 423.28 403.92 T
(-) 424.95 403.92 T
(-) 426.61 403.92 T
(-) 428.28 403.92 T
(-) 429.94 403.92 T
(-) 431.61 403.92 T
(-) 433.27 403.92 T
(-) 434.94 403.92 T
(-) 436.6 403.92 T
(-) 438.27 403.92 T
(-) 439.93 403.92 T
(-) 441.6 403.92 T
(-) 443.26 403.92 T
(-) 444.93 403.92 T
(-) 446.59 403.92 T
(-) 448.26 403.92 T
(-) 449.92 403.92 T
(-) 451.59 403.92 T
(-) 453.25 403.92 T
(-) 454.92 403.92 T
(-) 456.58 403.92 T
(-) 458.25 403.92 T
(-) 459.91 403.92 T
(-) 461.58 403.92 T
(-) 463.24 403.92 T
(-) 464.28 403.92 T
(=) 280.91 403.92 T
301.23 382.12 298.23 382.12 298.23 402.72 3 L
0.45 H
2 Z
N
298.23 402.72 301.23 402.72 2 L
N
373.39 382.12 376.39 382.12 376.39 402.72 3 L
N
376.39 402.72 373.39 402.72 2 L
N
399.61 382.12 396.61 382.12 396.61 402.72 3 L
N
396.61 402.72 399.61 402.72 2 L
N
462.61 382.12 465.61 382.12 465.61 402.72 3 L
N
465.61 402.72 462.61 402.72 2 L
N
54 87.98 540 686.02 C
0 0 612 792 C
FMENDPAGE
%%EndPage: "30" 30
%%Page: "31" 31
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (31) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Phase I: What the T) 207 736.18 T
(AC Sees) 289.35 736.18 T
2 10 Q
(3.4.6) 175.76 679.35 T
(A Simple Example) 207 679.35 T
0 F
0.57 (Here is a very simple example to illustrate how an integration time may be computed.) 207 663.35 P
0.81 (Suppose that the goal is to obtain a spectrum of a 13th magnitude B0 star at 1900 \201,) 207 651.35 P
0.07 (with the G160M grating and with a signal-to-noise of 25 per diode in the continuum. In) 207 639.35 P
-0.21 (this case we will assume that this star has not been previously observed in the ultraviolet) 207 627.35 P
(so that there is no) 207 615.35 T
3 F
(a priori) 280.05 615.35 T
0 F
( knowledge of the UV \337ux.) 310.89 615.35 T
3.6 (T) 207 595.35 P
3.6 (o be speci\336c, take the star to have a spectral type of B0I,) 212.41 595.35 P
3.6 (, and) 534.96 595.35 P
-0.05 (. The unreddened color for this spectral type is) 276.77 583.35 P
-0.05 (, so) 544.16 583.35 P
0.54 (that) 207 571.35 P
0.54 (. The total visual extinction is then) 301.51 571.35 P
0.54 (, leading) 523.02 571.35 P
1.58 (to a dereddened magnitude of) 207 559.35 P
1.58 (. The dereddened \337ux at 5500 \201 is then) 387.36 559.35 P
(.) 353.56 547.35 T
-0.2 (What \337ux can we anticipate at 1900 \201? The model atmospheres of Kurucz \0501979, ApJS,) 207 527.35 P
-0.03 (40, 1\051 predict) 207 513.35 P
-0.03 ( for a star with) 339.28 513.35 P
-0.03 (K. This leads to a \337ux of) 459.04 513.35 P
0.19 ( at 1900 \201 for the unreddened star) 353.56 499.35 P
0.19 (. Reddening will) 491.23 499.35 P
0.51 (diminish this by a factor of) 207 485.35 P
0.51 (, where the absorption at 1900 \201 can be deter-) 368.42 485.35 P
0.43 (mined from the data in Section) 207 471.35 P
0.43 (8.5 on page) 335.27 471.35 P
0.43 (93; the result in this case is) 385.01 471.35 P
0.43 (.) 555.5 471.35 P
(W) 207 457.35 T
(e therefore predict this star to have a \337ux at 1900 \201 of) 215.64 457.35 T
(.) 545.2 457.35 T
0.31 (The next step is to determine the detected count rate. For G160M at 1900 \201, the sensi-) 207 435.35 P
0.87 (tivity is) 207 423.35 P
0.87 (, in units of counts per second per diode per incident er) 309.75 423.35 P
0.87 (g s) 539.08 423.35 P
0 8 Q
0.69 (-1) 551.34 427.35 P
0 10 Q
0.1 (cm) 207 411.35 P
0 8 Q
0.08 (-2) 219.22 415.35 P
0 10 Q
0.1 ( \201) 225.88 411.35 P
0 8 Q
0.08 (-1) 235.71 415.35 P
0 10 Q
0.1 (. This leads to an expected count rate of) 242.37 411.35 P
0.1 (. An inte-) 519.74 411.35 P
0.59 (gration time of about 2.25 hours would lead to approximately 625 detected counts per) 207 399.35 P
1.34 (diode, or the required signal-to-noise of 25. This neglects the ef) 207 387.35 P
1.34 (fects of dark, which) 474.57 387.35 P
(should be an order) 207 375.35 T
(-of-magnitude below this count rate.) 280.95 375.35 T
487.72 590.85 534.96 603.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(V) 488.72 595.35 T
0 F
(1) 510.46 595.35 T
(2) 515.46 595.35 T
(.) 520.46 595.35 T
(8) 522.96 595.35 T
(9) 527.96 595.35 T
(=) 499.83 595.35 T
0 0 612 792 C
207 578.85 276.77 591.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(B) 213.96 583.35 T
(V) 230.07 583.35 T
0 F
(\320) 222.57 583.35 T
13 F
(\050) 209.67 583.35 T
(\051) 236.64 583.35 T
0 F
(0) 257.27 583.35 T
(.) 262.27 583.35 T
(0) 264.77 583.35 T
(3) 269.77 583.35 T
(=) 246.63 583.35 T
0 0 612 792 C
465.14 576.5 544.16 591.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(B) 472.09 583.35 T
(V) 488.2 583.35 T
0 F
(\320) 480.7 583.35 T
13 F
(\050) 467.8 583.35 T
(\051) 494.77 583.35 T
0 7 Q
(0) 500.15 580.25 T
0 10 Q
(0) 524.66 583.35 T
(.) 529.66 583.35 T
(2) 532.16 583.35 T
(4) 537.16 583.35 T
(\320) 519.28 583.35 T
(=) 508.65 583.35 T
0 0 612 792 C
225.04 566.85 301.51 579.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(E) 226.04 571.35 T
(B) 238.7 571.35 T
(V) 254.81 571.35 T
0 F
(\320) 247.31 571.35 T
13 F
(\050) 234.41 571.35 T
(\051) 261.38 571.35 T
0 F
(0) 282.01 571.35 T
(.) 287.01 571.35 T
(2) 289.51 571.35 T
(7) 294.51 571.35 T
(=) 271.37 571.35 T
0 0 612 792 C
446.4 566.85 523.02 579.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(3) 447.4 571.35 T
(.) 452.4 571.35 T
(1) 454.9 571.35 T
(0) 470.39 571.35 T
(.) 475.39 571.35 T
(2) 477.89 571.35 T
(7) 482.89 571.35 T
13 F
(\264) 462.4 571.35 T
0 F
(0) 503.52 571.35 T
(.) 508.52 571.35 T
(8) 511.02 571.35 T
(4) 516.02 571.35 T
(=) 492.88 571.35 T
0 0 612 792 C
336.24 552.5 387.36 567.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(V) 337.24 559.35 T
0 7 Q
(0) 343.73 556.25 T
0 10 Q
(1) 362.86 559.35 T
(2) 367.86 559.35 T
(.) 372.86 559.35 T
(0) 375.36 559.35 T
(5) 380.36 559.35 T
(=) 352.23 559.35 T
0 0 612 792 C
207 540.5 353.56 559.45 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(F) 208 547.35 T
0 7 Q
(5) 214.49 544.25 T
(5) 217.99 544.25 T
(0) 221.49 544.25 T
(0) 224.99 544.25 T
0 10 Q
(5) 244.12 547.35 T
(.) 249.12 547.35 T
(4) 251.62 547.35 T
(1) 267.11 547.35 T
(0) 272.11 547.35 T
0 7 Q
(1) 281.26 553.2 T
(4) 284.76 553.2 T
(\320) 277.49 553.2 T
0 10 Q
(e) 288.85 547.35 T
(r) 293.29 547.35 T
(g) 296.62 547.35 T
(s) 304.12 547.35 T
0 7 Q
(1) 312.15 553.2 T
(\320) 308.39 553.2 T
0 10 Q
(c) 316.24 547.35 T
(m) 320.68 547.35 T
0 7 Q
(2) 332.61 553.2 T
(\320) 328.84 553.2 T
0 10 Q
(\201) 336.7 547.35 T
0 7 Q
(1) 348.06 553.2 T
(\320) 344.3 553.2 T
13 10 Q
(\264) 259.12 547.35 T
0 F
(=) 233.49 547.35 T
0 0 612 792 C
263 506.5 339.28 521.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(F) 264 513.35 T
0 7 Q
(1) 270.49 510.25 T
(9) 273.99 510.25 T
(0) 277.49 510.25 T
(0) 280.99 510.25 T
3 10 Q
(F) 291.16 513.35 T
0 7 Q
(5) 297.65 510.25 T
(5) 301.15 510.25 T
(0) 304.65 510.25 T
(0) 308.15 510.25 T
13 10 Q
(\244) 286.99 513.35 T
0 F
(2) 327.28 513.35 T
(3) 332.28 513.35 T
(=) 316.65 513.35 T
0 0 612 792 C
399.94 506.5 459.04 521.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(T) 400.94 513.35 T
0 7 Q
(e) 406.88 510.25 T
(f) 409.99 510.25 T
(f) 412.32 510.25 T
0 10 Q
(2) 432.04 513.35 T
(5) 437.04 513.35 T
(0) 442.04 513.35 T
(0) 447.04 513.35 T
(0) 452.04 513.35 T
(=) 421.4 513.35 T
0 0 612 792 C
207 492.5 353.56 511.45 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(F) 208 499.35 T
0 7 Q
(1) 214.49 496.25 T
(9) 217.99 496.25 T
(0) 221.49 496.25 T
(0) 224.99 496.25 T
0 10 Q
(1) 244.12 499.35 T
(.) 249.12 499.35 T
(2) 251.62 499.35 T
(1) 267.11 499.35 T
(0) 272.11 499.35 T
0 7 Q
(1) 281.26 505.2 T
(2) 284.76 505.2 T
(\320) 277.49 505.2 T
0 10 Q
(e) 288.85 499.35 T
(r) 293.29 499.35 T
(g) 296.62 499.35 T
(s) 304.12 499.35 T
0 7 Q
(1) 312.15 505.2 T
(\320) 308.39 505.2 T
0 10 Q
(c) 316.24 499.35 T
(m) 320.68 499.35 T
0 7 Q
(2) 332.61 505.2 T
(\320) 328.84 505.2 T
0 10 Q
(\201) 336.7 499.35 T
0 7 Q
(1) 348.06 505.2 T
(\320) 344.3 505.2 T
13 10 Q
(\264) 259.12 499.35 T
0 F
(=) 233.49 499.35 T
0 0 612 792 C
320.64 480.85 368.42 499.2 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 321.64 485.35 T
(0) 326.64 485.35 T
0 7 Q
(0) 335.79 492.95 T
(.) 339.29 492.95 T
(4) 341.04 492.95 T
3 F
(A) 351.87 492.95 T
0 5 Q
(1) 356.42 490.7 T
(9) 358.92 490.7 T
(0) 361.42 490.7 T
(0) 363.92 490.7 T
13 7 Q
(\264) 346.28 492.95 T
0 F
(\320) 332.02 492.95 T
0 0 612 792 C
498.88 464.5 555.5 479.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(A) 499.88 471.35 T
0 7 Q
(1) 506.36 468.25 T
(9) 509.86 468.25 T
(0) 513.36 468.25 T
(0) 516.86 468.25 T
0 10 Q
(2) 536 471.35 T
(.) 541 471.35 T
(2) 543.5 471.35 T
(6) 548.5 471.35 T
(=) 525.36 471.35 T
0 0 612 792 C
434.76 452.85 545.2 469.45 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 435.76 457.35 T
(.) 440.76 457.35 T
(5) 443.26 457.35 T
(1) 458.75 457.35 T
(0) 463.75 457.35 T
0 7 Q
(1) 472.89 463.2 T
(3) 476.39 463.2 T
(\320) 469.13 463.2 T
0 10 Q
(e) 480.48 457.35 T
(r) 484.92 457.35 T
(g) 488.25 457.35 T
(s) 495.75 457.35 T
0 7 Q
(1) 503.79 463.2 T
(\320) 500.02 463.2 T
0 10 Q
(c) 507.88 457.35 T
(m) 512.32 457.35 T
0 7 Q
(2) 524.24 463.2 T
(\320) 520.48 463.2 T
0 10 Q
(\201) 528.33 457.35 T
0 7 Q
(1) 539.7 463.2 T
(\320) 535.93 463.2 T
13 10 Q
(\264) 450.76 457.35 T
0 0 612 792 C
241.53 416.5 309.75 435.45 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(S) 242.53 423.35 T
13 7 Q
(l) 247.91 420.25 T
0 10 Q
(5) 267.38 423.35 T
(.) 272.38 423.35 T
(2) 274.88 423.35 T
(1) 290.37 423.35 T
(0) 295.37 423.35 T
0 7 Q
(1) 300.75 429.2 T
(1) 304.25 429.2 T
13 10 Q
(\264) 282.38 423.35 T
0 F
(=) 256.75 423.35 T
0 0 612 792 C
404.92 406.85 519.74 423.45 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(7) 405.92 411.35 T
(.) 410.92 411.35 T
(8) 413.42 411.35 T
(1) 428.91 411.35 T
(0) 433.91 411.35 T
0 7 Q
(2) 443.05 417.2 T
(\320) 439.29 417.2 T
0 10 Q
(c) 447.14 411.35 T
(o) 451.58 411.35 T
(u) 456.58 411.35 T
(n) 461.58 411.35 T
(t) 466.58 411.35 T
(s) 469.36 411.35 T
(s) 475.75 411.35 T
0 7 Q
(1) 483.79 417.2 T
(\320) 480.02 417.2 T
0 10 Q
(d) 487.88 411.35 T
(i) 492.88 411.35 T
(o) 495.66 411.35 T
(d) 500.66 411.35 T
(e) 505.66 411.35 T
0 7 Q
(1) 514.24 417.2 T
(\320) 510.48 417.2 T
13 10 Q
(\264) 420.92 411.35 T
0 0 612 792 C
FMENDPAGE
%%EndPage: "31" 31
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Phase I: What the T) 189 736.18 T
(AC Sees) 271.35 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(32) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
FMENDPAGE
%%EndPage: "32" 32
%%Page: "33" 33
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (33) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
7 12 Q
1.2 (Chapter 4) 72 677 S
5 24 Q
-0.48 (Y) 207 677 S
-0.48 (our Phase II Pr) 219.86 677 S
-0.48 (oposal) 359.55 677 S
4 12 Q
(4.1) 144 419 T
( Acquisitions) 164.02 419 T
8 F
( 35) 505.32 419 T
4 10 Q
(4.1.1) 162 402.33 T
( Initial Pointing) 187.02 402.33 T
8 F
( 35) 508.1 402.33 T
4 F
(4.1.2) 162 386.33 T
( Interactive Acquisitions) 187.02 386.33 T
8 F
( 35) 508.1 386.33 T
4 F
(4.1.3) 162 370.33 T
( Early Acquisitions) 187.02 370.33 T
8 F
( 36) 508.1 370.33 T
4 F
(4.1.4) 162 354.33 T
( Onboard Acquisitions) 187.02 354.33 T
8 F
( 36) 508.1 354.33 T
4 F
(4.1.5) 162 338.33 T
( Special Onboard Strategies for Special Situations) 187.02 338.33 T
8 F
( 38) 508.1 338.33 T
4 F
(4.1.6) 162 322.33 T
( MAPs) 187.02 322.33 T
8 F
( 40) 508.1 322.33 T
4 F
(4.1.7) 162 306.33 T
( Acquisition Parameters \321 A Summary) 187.02 306.33 T
8 F
( 40) 508.1 306.33 T
4 12 Q
(4.2) 144 289 T
( Image Mode) 164.02 289 T
8 F
( 42) 505.32 289 T
4 10 Q
(4.2.1) 162 272.33 T
( Image Mode Parameters) 187.02 272.33 T
8 F
( 42) 508.1 272.33 T
4 F
(4.2.2) 162 256.33 T
( The GHRS as a Slitless Spectrograph) 187.02 256.33 T
8 F
( 43) 508.1 256.33 T
4 12 Q
(4.3) 144 239 T
( Accumulation Mode) 164.02 239 T
8 F
( 43) 505.32 239 T
4 10 Q
(4.3.1) 162 222.33 T
( Optimizing Data Quality) 187.02 222.33 T
8 F
( 43) 508.1 222.33 T
4 F
(4.3.2) 162 206.33 T
( Summary of Accumulation Mode Parameters) 187.02 206.33 T
8 F
( 44) 508.1 206.33 T
4 F
(4.3.3) 162 190.33 T
( WSCAN mode) 187.02 190.33 T
8 F
( 45) 508.1 190.33 T
4 F
(4.3.4) 162 174.33 T
( OSCAN mode) 187.02 174.33 T
8 F
( 45) 508.1 174.33 T
4 12 Q
(4.4) 144 157 T
( Rapid Readout Mode) 164.02 157 T
8 F
( 45) 505.32 157 T
4 F
(4.5) 144 139 T
( The Precision and Accuracy of Standard Calibrations) 164.02 139 T
8 F
( 46) 505.32 139 T
4 F
(4.6) 144 121 T
( Other Considerations) 164.02 121 T
8 F
( 47) 505.32 121 T
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Y) 189 736.18 T
(our Phase II Proposal) 194.34 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(34) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
1.64 (This chapter supplements the) 189 560.33 P
3 F
1.64 ( Phase II Pr) 310.86 560.33 P
1.64 (oposal Instructions) 364.02 560.33 P
0 F
1.64 ( that will be issued for) 442.62 560.33 P
-0 (Cycle 5. Y) 189 548.33 P
-0 (ou may also wish to consult) 231.05 548.33 P
3 F
-0 ( Phase II Instructions for the Solar System T) 342.43 548.33 P
-0 (ar) 519.26 548.33 P
-0 (get) 527.78 548.33 P
(List) 189 536.33 T
0 F
(if your program is to observe solar system objects.) 206.51 536.33 T
0.27 (Most users of the GHRS will \336nd that a simple sequence of commands will work most) 189 516.33 P
(of the time to obtain the data they desire:) 189 504.33 T
10 11 Q
(\245) 189 486.33 T
9 10 Q
(ACQ) 203.4 486.33 T
0 F
( in LSA with) 221.4 486.33 T
9 F
(BRIGHT=RETURN) 275.85 486.33 T
0 F
(.) 353.85 486.33 T
10 11 Q
(\245) 189 471.33 T
9 10 Q
-0.31 (ACQ/PEAKUP) 203.4 471.33 P
0 F
-0.13 ( to center star in LSA or SSA, whichever is appropriate to the science) 263.4 471.33 P
(observations that follow) 203.4 459.33 T
(.) 299.41 459.33 T
10 11 Q
(\245) 189 444.33 T
9 10 Q
(IMAGE) 203.4 444.33 T
0 F
(, if you wish to verify tar) 233.4 444.33 T
(get centering or to obtain an image of the object.) 332.93 444.33 T
10 11 Q
(\245) 189 429.33 T
0 10 Q
(W) 203.4 429.33 T
(avelength calibration exposure, if desired.) 212.04 429.33 T
10 11 Q
(\245) 189 414.33 T
9 10 Q
0.94 (ACCUM) 203.4 414.33 P
0 F
0.39 (s at wavelengths of interest.) 233.4 414.33 P
9 F
0.94 (NO) 349.23 414.33 P
0.94 (GAP) 364.12 414.33 P
0 F
0.39 ( is recommended as a Special Require-) 382.12 414.33 P
1.01 (ment in order to ensure the) 203.4 402.33 P
9 F
2.43 (PEAKUP) 319.45 402.33 P
0 F
1.01 ( operation is properly applied to the spectro-) 355.45 402.33 P
(scopic exposures.) 203.4 390.33 T
10 11 Q
(\245) 189 375.33 T
9 10 Q
(ACQ/PEAKUP) 203.4 375.33 T
0 F
( in the SSA if the previous observation was in the LSA.) 263.4 375.33 T
10 11 Q
(\245) 189 360.33 T
9 10 Q
(ACCUM) 203.4 360.33 T
0 F
(s for that dif) 233.4 360.33 T
(ferent aperture, again with) 282.38 360.33 T
9 F
(NO) 390.4 360.33 T
(GAP) 404.9 360.33 T
0 F
(.) 421.79 360.33 T
10 11 Q
(\245) 189 345.33 T
0 10 Q
(Repeat the above as needed for more stars.) 203.4 345.33 T
1.25 (T) 189 325.33 P
1.25 (ar) 194.41 325.33 P
1.25 (get acquisitions always take place with the LSA because the SSA is too small to) 202 325.33 P
0.57 (enable a \336eld to be mapped ef) 189 313.33 P
0.57 (fectively) 312.23 313.33 P
0.57 (. Additional) 346.57 313.33 P
9 F
1.38 (ACCUM) 397.99 313.33 P
0 F
0.57 (s may be speci\336ed after the) 427.99 313.33 P
(\336rst so as to obtain spectra at several wavelengths.) 189 301.33 T
0.67 (One task of the Instrument Scientists at STScI is to check the feasibility of successful) 189 281.33 P
1.18 (proposals after the Phase II proposals have been submitted.) 189 269.33 P
1 F
1.18 ( It is in your inter) 435.33 269.33 P
1.18 (est to) 516.33 269.33 P
-0.19 (help us with that by using standard and consistent formats for the Phase II pr) 189 257.33 P
-0.19 (opos-) 517.22 257.33 P
2.31 (als) 189 245.33 P
0 F
2.31 ( because that can greatly reduce ambiguity about the intentions of the General) 200.67 245.33 P
(Observer) 189 233.33 T
(. W) 225.1 233.33 T
(e suggest the following:) 238.74 233.33 T
10 11 Q
(\245) 189 215.33 T
0 10 Q
2.2 (Follow the examples in the next chapter) 203.4 215.33 P
2.2 (. The examples usually specify all the) 376.01 215.33 P
-0.03 (defaults for clarity) 203.4 203.33 P
-0.03 (, which is not strictly necessary) 276.56 203.33 P
-0.03 (, but, like comments in a computer) 401.3 203.33 P
2.56 (program, can help to con\336rm that a procedure conforms to the intents of the) 203.4 191.33 P
(observer) 203.4 179.33 T
(.) 237.28 179.33 T
10 11 Q
(\245) 189 164.33 T
0 10 Q
0.55 (Although the submission software does not strictly require it, we ask that you give) 203.4 164.33 P
0.53 (the commands in the order just listed: First the acquisition, then embellishments to) 203.4 152.33 P
-0.18 (the acquisition \050) 203.4 140.33 P
9 F
-0.44 (PEAKUP) 267.47 140.33 P
0 F
-0.18 (,) 302.36 140.33 P
9 F
-0.44 (OFFSET) 307.18 140.33 P
0 F
-0.18 (, etc.\051, then an) 342.44 140.33 P
9 F
-0.44 (IMAGE) 400.86 140.33 P
0 F
-0.18 ( and/or wavelength calibra-) 430.86 140.33 P
2.53 (tion exposure \050if desired\051, and then the actual science observation \050usually an) 203.4 128.33 P
9 F
(ACCUM) 203.4 116.33 T
0 F
(\051.) 233.4 116.33 T
54 87.98 540 686.02 C
108 576 540 679.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
108 576 540 679.02 R
5 X
0 0 0 1 0 0 0 K
V
117.83 586.52 530.17 669.18 R
7 X
V
15 14 Q
0 X
(CAUTION) 292.92 651.85 T
11 11 Q
1.54 (The pr) 123.59 632.85 P
1.54 (ocedur) 157.49 632.85 P
1.54 (es for cr) 196.45 632.85 P
1.54 (eating a Phase II pr) 241.39 632.85 P
1.54 (oposal ar) 349.84 632.85 P
1.54 (e being r) 401.1 632.85 P
1.54 (eviewed and) 451.64 632.85 P
2.93 (r) 123.59 619.85 P
2.93 (evised as this is written. W) 126.86 619.85 P
2.93 (e str) 275.37 619.85 P
2.93 (ongly r) 299.76 619.85 P
2.93 (ecommend that users check the) 338.42 619.85 P
1.36 (Phase) 123.59 606.85 P
1.36 (II documentation car) 158.79 606.85 P
1.36 (efully. W) 274.29 606.85 P
1.36 (e also r) 319.38 606.85 P
1.36 (ecommend checking on STEIS) 359.8 606.85 P
(at that time for a r) 123.59 593.85 T
(evised version of this Instrument Handbook.) 219.9 593.85 T
117.83 586.52 530.17 669.18 R
1 H
2 Z
N
108.5 576.5 539.5 678.52 R
0 Z
N
54 87.98 540 686.02 C
0 0 612 792 C
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
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[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (35) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Y) 207 736.18 T
(our Phase II Proposal) 212.34 736.18 T
10 11 Q
(\245) 207 679.35 T
0 10 Q
0.71 (Add plenty of comment lines \050RPSS imposes a limit\051 to explain what you want to) 221.4 679.35 P
0.19 (have happen so that we can see whether or not your proposal actually accomplishes) 221.4 667.35 P
(that. In particular) 221.4 655.35 T
(, please explain brie\337y how the exposure time was determined.) 290.15 655.35 T
72 612.02 558 615.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 613.52 558 613.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 613.52 198 613.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(4.1) 181.32 619.02 T
(Acquisitions) 207 619.02 T
0 10 Q
0.21 (Most objects observed with the GHRS are point sources \050stars\051, and the majority of the) 207 595.35 P
0.53 (remainder can be observed by \336rst centering on a nearby point source and then of) 207 583.35 P
0.53 (fset-) 540.23 583.35 P
0 (ting to the object of interest. Point sources with accurate coordinates are very) 207 571.35 P
0 (, very easy) 514.95 571.35 P
-0.02 (to acquire with the GHRS: just specify) 207 559.35 P
9 F
-0.05 (ACQ) 364.35 559.35 P
0 F
-0.02 ( with) 382.35 559.35 P
9 F
-0.05 (BRIGHT=RETURN) 405.09 559.35 P
0 F
-0.02 ( to have the instru-) 483.09 559.35 P
(ment automatically center on the brightest object found within the LSA.) 207 547.35 T
2 F
(4.1.1) 175.76 517.35 T
(Initial Pointing) 207 517.35 T
0 F
0.17 (A blind pointing with) 207 497.35 P
3 F
0.17 (HST) 296.6 497.35 P
0 F
0.17 ( is likely to place the object of interest within 2 arcsec of the) 314.38 497.35 P
-0 (center of the aperture. That accuracy is limited in part by the quality of coordinates pro-) 207 485.35 P
0.72 (vided by users and partly by errors in the positions of the FGSs relative to the GHRS) 207 473.35 P
0.02 (apertures \050see the) 207 461.35 P
3 F
0.02 ( FOS Instrument Handbook) 277.01 461.35 P
0 F
0.02 ( for a discussion of pointing errors\051. Using) 387.89 461.35 P
0.23 (J2000 coordinates tied to the GSC reference frame can help to reduce the possibility of) 207 449.35 P
1.05 (a failed acquisition. And don\325) 207 437.35 P
1.05 (t for) 330.16 437.35 P
1.05 (get to include proper motions if appropriate and to) 347.97 437.35 P
(check the equinox and epoch of astrometric quantities.) 207 425.35 T
2 F
(4.1.2) 175.76 395.35 T
(Interactive Acquisitions) 207 395.35 T
0 F
0.26 (W) 207 375.35 P
0.26 (e discuss interactive acquisitions \050) 215.64 375.35 P
9 F
0.62 (INT) 353.31 375.35 P
0.62 (ACQ) 374.07 375.35 P
0 F
0.26 (\051 \336rst in the hope of dissuading you from) 392.07 375.35 P
0.78 (using that capability) 207 363.35 P
0.78 (. An) 289.01 363.35 P
9 F
1.86 (INT) 310.29 363.35 P
1.86 (ACQ) 331.56 363.35 P
0 F
0.78 ( requires real-time contact between the ground and) 349.56 363.35 P
3 F
-0.14 (HST) 207 351.35 P
0 F
-0.14 (. Real-time contact is a limited and expensive resource that should only be used as a) 224.04 351.35 P
0.29 (last resort. In almost all cases where an onboard acquisition will not work \050because the) 207 339.35 P
0.52 (object is in a crowded \336eld, or is variable, or is a moving tar) 207 327.35 P
0.52 (get\051, it is suf) 454.45 327.35 P
0.52 (\336cient to use) 505.84 327.35 P
9 F
3.29 (EARLY) 207 315.35 P
3.29 (ACQ) 240.87 315.35 P
0 F
1.37 ( to get a WFPC2 or FOC image a few weeks in advance of the GHRS) 258.87 315.35 P
-0.22 (observation. The image can then be analyzed to pinpoint the source to be observed with-) 207 303.35 P
0.54 (out requiring real-time contact.) 207 291.35 P
9 F
1.3 (INT) 336.08 291.35 P
1.3 (ACQ) 357.13 291.35 P
0 F
0.54 ( may be needed in a few instances where the) 375.13 291.35 P
0.78 (object changes in its ultraviolet brightness unpredictably) 207 279.35 P
0.78 (. W) 437.12 279.35 P
0.78 (e suggest that you consult) 451.55 279.35 P
(with us before requesting) 207 267.35 T
9 F
(INT) 310.87 267.35 T
(ACQ) 331.37 267.35 T
0 F
(.) 349.37 267.35 T
0.69 (If an interactive acquisition with the GHRS has been speci\336ed, a spiral search will be) 207 247.35 P
0.26 (run after) 207 235.35 P
3 F
0.26 (HST) 244.16 235.35 P
0 F
0.26 ( makes its initial pointing. A map of the LSA is made at each dwell point) 261.94 235.35 P
1.5 (and each map is then downlinked to STScI in real time and may be viewed almost) 207 223.35 P
-0.12 (immediately in OSS. After the spiral is complete, the telescope remains at its \336nal dwell) 207 211.35 P
0.59 (point, awaiting instructions. The \336nal 9 \050or 25\051 maps are assembled into a mosaic and) 207 199.35 P
0.82 (displayed for the observer to identify the tar) 207 187.35 P
0.82 (get, either from a cursor position or from) 388.38 187.35 P
0.05 (calculation of a centroid. The motion needed to center the speci\336ed position in the LSA) 207 175.35 P
-0.24 (is computed and uplinked to) 207 163.35 P
3 F
-0.24 (HST) 321.65 163.35 P
0 F
-0.24 (. The recentering of the tar) 338.69 163.35 P
-0.24 (get usually takes place about) 443.96 163.35 P
-0.02 (an orbit after the spiral search, and must be scheduled for a speci\336c time. If you have so) 207 151.35 P
0.52 (requested in your proposal, an image of the LSA will be made after the recentering so) 207 139.35 P
0.14 (that you may con\336rm the position of the tar) 207 127.35 P
0.14 (get \050but additional interaction at that time is) 381.78 127.35 P
(not normally possible\051.) 207 115.35 T
FMENDPAGE
%%EndPage: "35" 35
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Y) 189 736.18 T
(our Phase II Proposal) 194.34 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(36) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
(4.1.3) 157.76 679.35 T
(Early Acquisitions) 189 679.35 T
0 F
0.46 (In an early acquisition \050) 189 659.35 P
9 F
1.11 (EARLY) 285.83 659.35 P
1.11 (ACQ) 318.79 659.35 P
0 F
0.46 (\051, an image of the \336eld of interest is obtained sev-) 336.79 659.35 P
0.16 (eral weeks \0508 or more\051 in advance of the spectroscopic observation that the GHRS is to) 189 647.35 P
0.03 (make. The image may be obtained with WFPC2, with the FOC \050especially if an ultravi-) 189 635.35 P
0.23 (olet image is desired\051, or with the imaging capability of the GHRS itself. The GHRS is) 189 623.35 P
0.23 (relatively slow at getting images, so if you wish to map an area much lar) 189 611.35 P
0.23 (ger than about) 482.32 611.35 P
-0.23 (2) 189 599.35 P
13 F
-0.23 (\264) 196.5 599.35 P
0 F
-0.23 (2 arcsec we recommend that you consider WFPC2 or FOC. However) 204.26 599.35 P
-0.23 (, the GHRS has) 478.46 599.35 P
1.84 (the capability of obtaining a monochromatic map \050see Section) 189 587.35 P
1.84 (4.2.2 on page) 454.5 587.35 P
1.84 (43\051 in) 514.55 587.35 P
9 F
0.09 (IMAGE) 189 575.35 P
0 F
0.04 (mode, which can be useful in some situations. For any) 225.09 575.35 P
9 F
0.09 (EARLY) 445.46 575.35 P
0.09 (ACQ) 478 575.35 P
0 F
0.04 (, be sure to) 496 575.35 P
2.68 (note the relationship of the image to the spectroscopic observations as a Special) 189 563.35 P
0.12 (Requirement \050see the \336rst example in the next chapter\051. Also, you should plan ahead so) 189 551.35 P
-0.24 (that the early acquisition image can be analyzed quickly and the positions measured sent) 189 539.35 P
(back to STScI for incorporation into the telescope observing schedule.) 189 527.35 T
2 F
(4.1.4) 157.76 497.35 T
(Onboard Acquisitions) 189 497.35 T
0 F
-0.04 (After the initial pointing, a GHRS onboard tar) 189 477.35 P
-0.04 (get acquisition begins with a spiral search) 373.01 477.35 P
0.21 (centered on the \336eld of view) 189 465.35 P
0.21 (. The motions are made by the telescope, and at each point) 303.55 465.35 P
0.59 (of the search either a single \337ux measurement \050with 8 science diodes\051 or a map of the) 189 453.35 P
0.66 (LSA is made. The default is a) 189 441.35 P
0.66 ( pattern \050) 337.72 441.35 P
9 F
1.57 (SEARCH-SIZE=3) 375.13 441.35 P
0 F
0.66 (\051 of maps in a square) 453.13 441.35 P
0.67 (4.6 arcsec on a side. Other options available are a) 189 429.35 P
0.67 ( pattern \050) 418.72 429.35 P
9 F
1.62 (SEARCH-SIZE=5) 456.17 429.35 P
0 F
0.67 (\051,) 534.17 429.35 P
1.48 (7.7 arcsec on a side, or a single integration \050) 189 417.35 P
9 F
3.54 (SEARCH-SIZE=1) 378.62 417.35 P
0 F
1.48 (\051 that is 1.74 arcsec) 456.62 417.35 P
0.35 (square \050this latter option can be useful for obtaining a) 189 405.35 P
9 F
0.85 (MAP) 409.16 405.35 P
0 F
0.35 ( after an object is centered\051.) 427.16 405.35 P
0.59 (The telescope motions are made in the) 189 393.35 P
3 F
0.59 (x) 349.47 393.35 P
0 F
0.59 ( and) 353.91 393.35 P
3 F
0.59 (y) 374.52 393.35 P
0 F
0.59 ( coordinate system of the GHRS with a) 378.96 393.35 P
(step-size of 1.53 arcsec, not the U2, U3 system of the telescope.) 189 381.35 T
0.41 (For stars with good coordinates, the default \050) 189 361.35 P
0.41 (\051 acquisition strategy should suf) 393.81 361.35 P
0.41 (\336ce,) 523.06 361.35 P
1.16 (but the) 189 349.35 P
1.16 ( pattern usually costs little more in total time and guards against minor) 243.81 349.35 P
-0.01 (coordinate uncertainties \050the time needed increases in proportion to [) 189 337.35 P
9 F
-0.01 (SEARCH-SIZE) 464.17 337.35 P
0 F
-0.01 (]) 530.17 337.35 P
0 8 Q
-0 (2) 533.5 341.35 P
0 10 Q
-0.01 (,) 537.5 337.35 P
0.37 (but the) 189 325.35 P
9 F
0.9 (STEP-TIME) 219.75 325.35 P
0 F
0.37 ( for an acquisition is usually so low that the total time involved is) 273.75 325.35 P
(small\051.) 189 313.35 T
(Y) 189 293.35 T
(ou should use) 195.22 293.35 T
9 F
(ONBOARD) 252.72 293.35 T
(ACQ) 297.22 293.35 T
0 F
( whenever:) 315.22 293.35 T
10 11 Q
(\245) 189 275.35 T
0 10 Q
(The object is a point source, or) 203.4 275.35 T
10 11 Q
(\245) 189 260.35 T
0 10 Q
0.65 (The object can be reached by of) 203.4 260.35 P
0.65 (fsetting from a nearby object that meets the above) 334.85 260.35 P
(description, or) 203.4 248.35 T
10 11 Q
(\245) 189 233.35 T
0 10 Q
2.38 (An extended object is small enough that) 203.4 233.35 P
9 F
5.72 (LOCATE=EXTENDED) 383.14 233.35 P
0 F
2.38 ( will work \050see) 473.14 233.35 P
(Section) 203.4 221.35 T
(4.1.5.4 on page) 235.9 221.35 T
(39\051.) 299.78 221.35 T
0.69 (Also, the object to be centered should be the brightest object within the area searched) 189 201.35 P
0.13 (\050about) 189 189.35 P
0.13 ( arcsec for a 3) 254.65 189.35 P
13 F
0.13 ( \264) 311.24 189.35 P
0 F
0.13 ( 3 search\051 but with allowance for about 3 arcsec uncer-) 319.36 189.35 P
0.64 (tainty in positioning as well. In other words, you should ensure that your object is the) 189 177.35 P
-0.14 (brightest one that) 189 165.35 P
3 F
-0.14 (HST) 260.52 165.35 P
0 F
-0.14 ( will \336nd within a box whose total size is about 8) 278.3 165.35 P
13 F
-0.14 (\264) 475.51 165.35 P
0 F
-0.14 ( 8 arcsec. Note) 481 165.35 P
(that the \337ux is measured in the ultraviolet \050see Section) 189 153.35 T
(7.4.1 on page) 408.98 153.35 T
(78\051.) 465.36 153.35 T
(The items you must specify for the) 189 133.35 T
9 F
(ONBOARD) 330.93 133.35 T
(ACQ) 375.43 133.35 T
0 F
( are:) 393.43 133.35 T
10 11 Q
(\245) 189 115.35 T
0 10 Q
0.21 (The mirror to use. N2 and A2 should suf) 203.4 115.35 P
0.21 (\336ce for virtually all tar) 367.35 115.35 P
0.21 (gets you might wish) 458.54 115.35 P
0.36 (to observe. Mirrors N1 or A1 may also be used, especially for spectroscopic obser-) 203.4 103.35 P
0.79 (vations that utilize Side 1 \050i.e., detector D1\051. Mirror N2 provides a \337at re\337ectivity) 203.4 91.35 P
315.24 438.18 337.72 449.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(3) 315.74 441.35 T
(3) 331.22 441.35 T
13 F
(\264) 323.23 441.35 T
0 0 612 792 C
396.24 426.18 418.72 437.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(5) 396.74 429.35 T
(5) 412.23 429.35 T
13 F
(\264) 404.24 429.35 T
0 0 612 792 C
371.33 358.18 393.81 369.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(3) 371.82 361.35 T
(3) 387.31 361.35 T
13 F
(\264) 379.32 361.35 T
0 0 612 792 C
221.33 346.18 243.81 357.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(5) 221.83 349.35 T
(5) 237.31 349.35 T
13 F
(\264) 229.33 349.35 T
0 0 612 792 C
217.18 186.18 254.65 197.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(4) 217.67 189.35 T
(.) 222.67 189.35 T
(8) 225.17 189.35 T
(4) 240.66 189.35 T
(.) 245.66 189.35 T
(8) 248.16 189.35 T
13 F
(\264) 232.67 189.35 T
0 0 612 792 C
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (37) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Y) 207 736.18 T
(our Phase II Proposal) 212.34 736.18 T
0 10 Q
0 (over a broad range of ultraviolet wavelengths \050see Section) 221.4 679.35 P
0 (7.4.1 on page) 456.63 679.35 P
0 (78\051. Mirror) 513.01 679.35 P
0.26 (A2 has a similar spectrum response but re\337ects much less light than N2, in order to) 221.4 667.35 P
-0.2 (acquire bright objects. Both detectors may be active at the same time, so it is permis-) 221.4 655.35 P
1.16 (sible to specify mirror N2 for an acquisition to observe with Side 1; this may be) 221.4 643.35 P
1.27 (desirable, for example, when observing cool stars. However) 221.4 631.35 P
1.27 (, doing this may cost) 469.85 631.35 P
(you observing time; see below) 221.4 619.35 T
(.) 342.96 619.35 T
10 11 Q
(\245) 207 604.35 T
9 10 Q
0.88 (BRIGHT) 221.4 604.35 P
0 F
0.37 ( and) 257.4 604.35 P
9 F
0.88 (FAINT) 277.58 604.35 P
0 F
0.37 ( \337ux limits so the instrument knows when the object has been) 307.58 604.35 P
-0.05 (found. However) 221.4 592.35 P
-0.05 (, in almost all cases it is better to use) 285.93 592.35 P
9 F
-0.12 (BRIGHT=RETURN) 434.6 592.35 P
0 F
-0.05 (, which is a) 512.6 592.35 P
0.71 (feature that automatically centers the brightest object found. If) 221.4 580.35 P
9 F
1.72 (BRIGHT=RETURN) 480 580.35 P
0 F
(is speci\336ed, any) 221.4 568.35 T
9 F
(FAINT) 288.06 568.35 T
0 F
( limit given is ignored.) 318.06 568.35 T
10 11 Q
(\245) 207 553.35 T
0 10 Q
0.69 (The size of the spiral search pattern to execute \050) 221.4 553.35 P
9 F
1.66 (SEARCH-SIZE) 418.97 553.35 P
0 F
0.69 (\051. The default is a) 484.97 553.35 P
0.27 (3) 221.4 541.35 P
13 F
0.27 (\264) 228.9 541.35 P
0 F
0.27 ( 3 grid \050which covers about 4.6 arcsec square\051, but you may also request a 5) 234.39 541.35 P
13 F
0.27 (\264) 544.74 541.35 P
0 F
0.27 ( 5) 550.23 541.35 P
(search over a square 7.7 arcsec on a side.) 221.4 529.35 T
10 11 Q
(\245) 207 514.35 T
0 10 Q
0.15 (Whether or not to record a map of the \336eld at the search points so that you can con-) 221.4 514.35 P
1.31 (\336rm the telescope\325) 221.4 502.35 P
1.31 (s pointing after the fact. A) 297.89 502.35 P
9 F
3.13 (MAP) 413.21 502.35 P
0 F
1.31 ( is usually unnecessary and so) 431.21 502.35 P
-0.11 (wastes spacecraft time. At most, a) 221.4 490.35 P
9 F
-0.26 (MAP=END-POINT) 359.62 490.35 P
0 F
-0.11 ( should suf) 437.62 490.35 P
-0.11 (\336ce. Note that such) 481.11 490.35 P
-0.23 (a) 221.4 478.35 P
9 F
-0.54 (MAP) 228.11 478.35 P
0 F
-0.23 ( occurs after the return to the brightest point in the \336eld but before the object is) 246.11 478.35 P
0.23 (centered in the LSA by an) 221.4 466.35 P
9 F
0.54 (ACQ/PEAKUP) 329.96 466.35 P
0 F
0.23 (. T) 388.85 466.35 P
0.23 (o determine the position of an object in) 399.48 466.35 P
0.47 (the LSA before spectroscopic observations are begun, we recommend obtaining an) 221.4 454.35 P
9 F
0.03 (IMAGE) 221.4 442.35 P
0 F
0.01 ( on a separate Exposure Logsheet line. The) 251.4 442.35 P
9 F
0.03 (MAP=ALL-POINTS) 426.19 442.35 P
0 F
0.01 ( option may) 510.19 442.35 P
3 F
(not) 221.4 430.35 T
0 F
( be used with an) 234.18 430.35 T
9 F
(ONBOARD) 301.67 430.35 T
(ACQ) 346.17 430.35 T
0 F
(.) 364.17 430.35 T
10 11 Q
(\245) 207 415.35 T
0 10 Q
(The of) 221.4 415.35 T
(fset to apply once the object is centered \050if appropriate\051.) 247.6 415.35 T
2 9 Q
(4.1.4.1) 170.48 392.02 T
(Explicitly Specifying) 207 392.02 T
10 10 Q
(BRIGHT) 297.04 392.02 T
2 9 Q
(,) 332.04 392.02 T
10 10 Q
( FAINT) 334.54 392.02 T
2 9 Q
(, and) 369.54 392.02 T
10 10 Q
(STEP-TIME) 393.05 392.02 T
0 F
0.02 (Explicit) 207 371.35 P
9 F
0.05 (BRIGHT) 241.19 371.35 P
0 F
0.02 ( and) 277.19 371.35 P
9 F
0.05 (FAINT) 296.67 371.35 P
0 F
0.02 ( limits may be speci\336ed if you desire, although there is an) 326.67 371.35 P
1.49 (increased risk of a failed acquisition unless you are fairly con\336dent of those \337uxes.) 207 359.35 P
1.34 (Also, a few very bright stars cannot be acquired with Side 2 if an explicit) 207 347.35 P
9 F
3.21 (BRIGHT) 522 347.35 P
0 F
(value is given but they can be acquired automatically with) 207 335.35 T
9 F
(BRIGHT=RETURN) 442.52 335.35 T
0 F
(.) 520.52 335.35 T
0.15 (Details on computing) 207 315.35 P
9 F
0.37 (BRIGHT) 296.07 315.35 P
0 F
0.15 (and) 338.44 315.35 P
9 F
0.37 (FAINT) 355.54 315.35 P
0 F
0.15 ( limits are given in Section) 385.54 315.35 P
0.15 (7.1 on page) 496.31 315.35 P
0.15 (68.) 545.5 315.35 P
0.07 (Please note that although we discourage the use of explicit) 207 303.35 P
9 F
0.16 (BRIGHT) 444.31 303.35 P
0 F
0.07 ( and) 480.31 303.35 P
9 F
0.16 (FAINT) 499.88 303.35 P
0 F
0.07 ( values) 529.88 303.35 P
-0.25 (unless they are unavoidable, you still need to estimate the tar) 207 291.35 P
-0.25 (get acquisition count rate in) 447.9 291.35 P
1.3 (order to ensure that you choose the acquisition mirror correctly and that the) 207 279.35 P
9 F
3.12 (STEP-) 528 279.35 P
(TIME) 207 267.35 T
0 F
( is determined properly) 231 267.35 T
(.) 323.39 267.35 T
10 11 Q
(\245) 207 249.35 T
0 10 Q
0.63 (Note that using) 221.4 249.35 P
9 F
1.51 (BRIGHT=RETURN) 286.9 249.35 P
0 F
0.63 ( and explicitly specifying) 364.9 249.35 P
9 F
1.51 (BRIGHT) 471.3 249.35 P
0 F
0.63 ( and) 507.3 249.35 P
9 F
1.51 (FAINT) 528 249.35 P
0 F
2.44 (limits result in fundamentally dif) 221.4 237.35 P
2.44 (ferent acquisition procedures. If) 362.64 237.35 P
9 F
5.85 (BRIGHT) 502.62 237.35 P
0 F
2.44 ( and) 538.62 237.35 P
9 F
1.33 (FAINT) 221.4 225.35 P
0 F
0.55 ( are speci\336ed, the acquisition stops as soon as those conditions are met and) 251.4 225.35 P
3.14 (the point at which that happened is moved to the center of the LSA. W) 221.4 213.35 P
3.14 (ith) 547.44 213.35 P
9 F
5.07 (BRIGHT=RETURN) 221.4 201.35 P
0 F
2.11 (, the entire spiral search region is sampled and the brightest) 299.4 201.35 P
0.67 (object in it determined before any movement is made to center on the tar) 221.4 189.35 P
0.67 (get. Both) 520.66 189.35 P
1.14 (procedures require the same amount of telescope time because the schedule must) 221.4 177.35 P
(allow for the entire region to be sampled.) 221.4 165.35 T
2 9 Q
(4.1.4.2) 170.48 142.02 T
(Peakups) 207 142.02 T
0 10 Q
-0.12 (After the initial acquisition, a peakup helps to precisely center the object in the aperture.) 207 121.35 P
1.08 (Specifying a) 207 109.35 P
9 F
2.59 (ACQ/PEAKUP) 261.93 109.35 P
0 F
1.08 ( before starting LSA observations will help to ensure the) 321.93 109.35 P
FMENDPAGE
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[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Y) 189 736.18 T
(our Phase II Proposal) 194.34 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(38) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
1.58 (reliability of measured \337uxes. A) 189 679.35 P
9 F
3.78 (ACQ/PEAKUP) 328.52 679.35 P
0 F
1.58 ( before starting SSA observations is) 388.52 679.35 P
(vital for achieving the best throughput with the small aperture.) 189 667.35 T
1.19 (In the past we recommended using a) 189 647.35 P
9 F
2.86 (STEP-TIME) 345.92 647.35 P
0 F
1.19 ( value of 1.6 seconds for a) 399.92 647.35 P
9 F
2.86 (ACQ/) 516 647.35 P
-0.46 (PEAKUP) 189 635.35 P
0 F
-0.19 (, but that is unnecessary for the post-Servicing Mission observatory) 223.89 635.35 P
-0.19 (. W) 491.48 635.35 P
-0.19 (e recom-) 504.93 635.35 P
0.35 (mend aiming to achieve 1,000 to 10,000 counts in the peak step, as for the acquisition,) 189 623.35 P
(but levels as low as 100 will suf) 189 611.35 T
(\336ce for faint tar) 316.87 611.35 T
(gets.) 379.17 611.35 T
2 F
(4.1.5) 157.76 581.35 T
(Special Onboard Strategies for Special Situations) 189 581.35 T
2 9 Q
(4.1.5.1) 152.48 558.02 T
(Side 2 Acquisitions for Side 1 Science Observations) 189 558.02 T
0 10 Q
-0.17 (There are situations in which an object can be observed satisfactorily with Side 1 but for) 189 545.35 P
0.02 (which the count rates for acquisition mirrors N1 or A1 are extremely low) 189 533.35 P
0.02 (. One possibil-) 481.34 533.35 P
1.58 (ity is to increase the exposure time for the acquisition, but the maximum permitted) 189 521.35 P
9 F
0.3 (STEP-TIME) 189 509.35 P
0 F
0.12 ( is 12.75 seconds. A better option may be to acquire with mirror N2. Both) 243 509.35 P
-0.08 (detectors, D1 and D2, may be active in the GHRS at the same time, but there is an over-) 189 497.35 P
-0.18 (head involved in making one primary and the other secondary; to go from Side 2 to Side) 189 485.35 P
0.34 (1, that time is approximately 40 minutes. Whether or not that is a \322cost\323 or not to your) 189 473.35 P
0.53 (program depends on speci\336c details. It is often the case that an acquisition takes place) 189 461.35 P
-0.04 (over the \336rst orbit, followed by science observations in later orbits. In that case, most or) 189 449.35 P
0.32 (all of the 40 minutes can take place during the part of the orbit when the tar) 189 437.35 P
0.32 (get is inac-) 495.49 437.35 P
(cessible. But for CVZ viewing the cost can be real.) 189 425.35 T
2 9 Q
(4.1.5.2) 152.48 402.02 T
(Complex T) 189 402.02 T
(argets) 234.34 402.02 T
0 10 Q
-0.04 (Given the centering algorithm for the GHRS, which we will now describe, you can usu-) 189 381.35 P
0.92 (ally predict the results of an onboard tar) 189 369.35 P
0.92 (get acquisition. Stepping, in both the) 354.91 369.35 P
3 F
0.92 (x) 509.85 369.35 P
0 F
0.92 ( and) 514.29 369.35 P
3 F
0.92 (y) 535.56 369.35 P
0 F
0.03 (directions, is done in 0.027 arcsec steps, and on a point source the centering is expected) 189 357.35 P
0.92 (to be good to within two steps. If the tar) 189 345.35 P
0.92 (get is extended enough that the \337uxes in the) 357.1 345.35 P
0.41 (areas which are compared do not change signi\336cantly when a step is made, the center-) 189 333.35 P
0.33 (ing accuracy will be degraded. An example is the case in which there is more than one) 189 321.35 P
(source of light within the LSA.) 189 309.35 T
0.92 (Consider) 189 289.35 P
0.92 (, for instance, two stars which are separated by 1.0 arcsec and for which the) 224.71 289.35 P
-0.12 (second star is 1 magnitude fainter than the primary star) 189 277.35 P
-0.12 (. Exact results will depend on the) 407.65 277.35 P
0.59 (position angle between the two stars. The) 189 265.35 P
3 F
0.59 (x) 361.46 265.35 P
0 F
0.59 (balancing algorithm begins by placing the) 368.99 265.35 P
-0.1 (brightest source on the fourth of the eight diodes that are used during an acquisition \050the) 189 253.35 P
0.58 (LSA is imaged onto eight diodes\051, and moving until the \337ux on diodes 4 and 5 is bal-) 189 241.35 P
0.2 (anced. The second star would not af) 189 229.35 P
0.2 (fect this balance at all unless its light fell on one of) 334.17 229.35 P
-0.22 (the same diodes as the primary star) 189 217.35 P
-0.22 (. In that case it would af) 327.66 217.35 P
-0.22 (fect centering by a fraction of) 422.53 217.35 P
(a diode.) 189 205.35 T
0.55 (In the) 189 185.35 P
3 F
0.55 (y) 215.65 185.35 P
0 F
0.55 ( direction the results are dif) 220.09 185.35 P
0.55 (ferent. If the second star is \322above\323 or \322below\323 the) 332.35 185.35 P
1.33 (primary) 189 173.35 P
1.33 (, it will \322pull\323 the centering in that direction. In the case described, an extra) 220.01 173.35 P
0.01 (source of light 40% as bright as the primary would be present in the upper or lower half) 189 161.35 P
-0.05 (of the LSA. The \337ux-balancing algorithm would divide the primary image 70-30, rather) 189 149.35 P
-0 (than 50-50, with the image displaced towards the half of the LSA which did not contain) 189 137.35 P
-0.17 (the second star) 189 125.35 P
-0.17 (. In this case the centering error should be less than 0.1 arcsec. If the LSA) 247.55 125.35 P
0.08 (acquisition were to be followed by a slew to the SSA,) 189 113.35 P
9 F
0.18 (PEAKUP) 407.04 113.35 P
0 F
0.08 (, and an observation, the) 441.93 113.35 P
3.33 (primary object should be successfully centered and observed. More complicated) 189 101.35 P
FMENDPAGE
%%EndPage: "38" 38
%%Page: "39" 39
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (39) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Y) 207 736.18 T
(our Phase II Proposal) 212.34 736.18 T
0 10 Q
0.42 (images, or sources more similar in brightness may not be suitable for onboard acquisi-) 207 679.35 P
(tion. \050Note that balancing in the) 207 667.35 T
3 F
(y) 336.71 667.35 T
0 F
( direction is done before the) 341.15 667.35 T
3 F
(x) 455.57 667.35 T
0 F
( direction is balanced.\051) 460.01 667.35 T
2 9 Q
(4.1.5.3) 170.48 644.02 T
(Acquiring Faint T) 207 644.02 T
(argets with the GHRS or FOS) 280.34 644.02 T
0 10 Q
0.34 (Sometimes a star may be just plain faint to the point where geocoronal L) 207 623.35 P
0.34 (yman-) 501.64 623.35 P
13 F
0.34 (a) 527.19 623.35 P
0 F
0.34 ( inter-) 533.5 623.35 P
0.75 (feres. Some guidance for when this may be a problem is provided in Section) 207 611.35 P
0.75 (7.4.2 on) 524.75 611.35 P
0.44 (page) 207 599.35 P
0.44 (80. If it is, we recommend that you specify) 228.38 599.35 P
9 F
1.05 (DARK) 406.45 599.35 P
1.05 (TIME) 433.39 599.35 P
0 F
0.44 ( as a special requirement) 457.39 599.35 P
1.16 (on the acquisition line on your Phase II form. Doing so constrains the scheduling of) 207 587.35 P
0.33 (your proposal and is likely to result in greater resource char) 207 575.35 P
0.33 (ges to you, so) 448.37 575.35 P
9 F
0.78 (DARK) 507.17 575.35 P
0.78 (TIME) 534 575.35 P
0 F
(should only be requested when it is necessary) 207 563.35 T
(.) 388.82 563.35 T
1.87 (Another way to acquire very faint tar) 207 543.35 P
1.87 (gets reliably is to use the Faint Object Spec-) 366.36 543.35 P
1.26 (trograph. This can be especially useful for acquiring extragalactic objects to observe) 207 531.35 P
-0 (with grating G140L because the acquisition mirrors for Side 1 of the GHRS re\337ect only) 207 519.35 P
1.12 (far) 207 507.35 P
1.12 (-ultraviolet light and because the maximum permissible integration time per dwell) 217.9 507.35 P
0.74 (point is only 12.75 seconds. FOS-assisted acquisitions for the GHRS will be tested in) 207 495.35 P
(Cycle 4, so we suggest that you consult us if you wish to explore this option.) 207 483.35 T
2 9 Q
(4.1.5.4) 170.48 460.02 T
(Acquiring Extended Sources with the GHRS) 207 460.02 T
0 10 Q
(There are three classes of extended sources we can consider:) 207 439.35 T
10 11 Q
(\245) 207 421.35 T
0 10 Q
(Objects lar) 221.4 421.35 T
(ger than the LSA that have roughly uniform surface brightness.) 264.82 421.35 T
10 11 Q
(\245) 207 406.35 T
0 10 Q
(Objects smaller than the LSA with roughly uniform surface brightness.) 221.4 406.35 T
10 11 Q
(\245) 207 391.35 T
0 10 Q
(Objects with signi\336cant structure, some of which is on scales smaller than the LSA.) 221.4 391.35 T
0.64 (The \336rst class might be typi\336ed by Jupiter) 207 371.35 P
0.64 (, and such objects are impossible to acquire) 379.67 371.35 P
0.77 (directly with the GHRS because there is no clear photometric \322center\323 to align on. In) 207 359.35 P
(such cases it is necessary to of) 207 347.35 T
(fset from a smaller object which can be centered.) 328.46 347.35 T
0.02 (The second class of objects includes the Gallilean satellites of Jupiter) 207 327.35 P
0.02 (, and it is these for) 484.01 327.35 P
0.39 (which the) 207 315.35 P
9 F
0.94 (LOCATE=EXTENDED) 249.44 315.35 P
0 F
0.39 ( acquisition option was written. In a normal) 339.44 315.35 P
9 F
0.94 (LOCATE) 519.5 315.35 P
0 F
0.39 (,) 555.5 315.35 P
0.34 (the object to be observed is moved in the) 207 303.35 P
3 F
0.34 (x) 376.42 303.35 P
0 F
0.34 ( direction until the signal seen by the center) 380.86 303.35 P
6.54 (two diodes \050of the eight onto which the LSA is imaged\051 is balanced.) 207 291.35 P
9 F
3.05 (LOCATE=EXTENDED) 207 279.35 P
0 F
1.27 ( in) 297 279.35 P
9 F
3.05 (ACQUISITION) 312.32 279.35 P
0 F
1.27 ( mode balances the four left diodes against) 378.32 279.35 P
2.26 (the four right-hand ones to roughly center an object. In) 207 267.35 P
9 F
5.43 (ACQ/PEAKUP) 451.53 267.35 P
0 F
2.26 ( mode, the) 511.53 267.35 P
9 F
2.77 (EXTENDED) 207 255.35 P
0 F
1.15 ( option allows you to specify that the balancing be done over the central) 255 255.35 P
(four) 207 243.35 T
(, six, or eight diodes \050speci\336ed as) 223.26 243.35 T
9 F
(EXTENDED=2) 359.08 243.35 T
0 F
(,) 419.08 243.35 T
9 F
(3) 424.08 243.35 T
0 F
(, or) 430.08 243.35 T
9 F
(4) 445.91 243.35 T
0 F
(\051.) 451.91 243.35 T
1.38 (The third class of objects can be the most problematic, especially if the tar) 207 223.35 P
1.38 (get is an) 521.91 223.35 P
0.04 (extragalactic one at high latitude. In such cases there may be no nearby star from which) 207 211.35 P
0.31 (you could of) 207 199.35 P
0.31 (fset, but the source itself often contains point-like sources that can be cen-) 257.98 199.35 P
0.65 (tered on; in these cases an early acquisition or a pre-existing image is invaluable. The) 207 187.35 P
0.66 (problem is then one of predicting acquisition count rates; that is treated in Section) 207 175.35 P
0.66 (7.1) 545.5 175.35 P
0.06 (on page) 207 163.35 P
0.06 (68. Y) 240.94 163.35 P
0.06 (ou may also wish to consider an acquisition with the FOS, as described in) 262.22 163.35 P
(the previous section.) 207 151.35 T
2 9 Q
(4.1.5.5) 170.48 128.02 T
(Offsetting) 207 128.02 T
0 10 Q
0.23 (Even if an) 207 107.35 P
9 F
0.55 (ONBOARD) 251.28 107.35 P
0.55 (ACQ) 296.01 107.35 P
0 F
0.23 (uisition will not work for your tar) 314.01 107.35 P
0.23 (get, it may still be possible) 449.63 107.35 P
0.61 (to acquire a nearby reference star and to then of) 207 95.35 P
0.61 (fset to your tar) 403.03 95.35 P
0.61 (get. Such an of) 463.27 95.35 P
0.61 (fset will) 524.89 95.35 P
FMENDPAGE
%%EndPage: "39" 39
%%Page: "40" 40
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Y) 189 736.18 T
(our Phase II Proposal) 194.34 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(40) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
0.54 (happen automatically if the coordinates given for an acquisition exposure are dif) 189 679.35 P
0.54 (ferent) 516.68 679.35 P
0.6 (from those given for the science exposure. Y) 189 667.35 P
0.6 (ou would normally use two or three lines) 371.62 667.35 P
-0.12 (on the Phase II Exposure Logsheet to achieve this: acquisition of a reference star) 189 655.35 P
-0.12 (, of) 510.03 655.35 P
-0.12 (fset,) 523.06 655.35 P
0.05 (peakup on the tar) 189 643.35 P
0.05 (get \050if desired\051, and a science observation. The \336rst line would request) 258.12 643.35 P
1.76 (an onboard acquisition of the reference star) 189 631.35 P
1.76 (. It should specify) 372.29 631.35 P
9 F
4.22 (ONBOARD) 453.48 631.35 P
4.22 (ACQ) 499.74 631.35 P
4.22 (FOR) 522 631.35 P
0 F
1.64 ( 1.64 (2>. Line 2 should then be an) 212.14 619.35 P
9 F
3.94 (ACQ/PEAKUP) 340.36 619.35 P
0 F
1.64 (, and it should specify) 399.25 619.35 P
9 F
3.94 (ONBOARD) 498 619.35 P
1.79 (ACQ) 189 607.35 P
1.79 (FOR) 210.25 607.35 P
0 F
0.75 ( . The next line would specify an of) 228.25 607.35 P
0.75 (fset to move from the reference) 410.48 607.35 P
(star to the tar) 189 595.35 T
(get, and the \336nal line should be your intended science observation.) 241.31 595.35 T
1.33 (Y) 189 575.35 P
1.33 (ou must, of course, include the reference star as one of the objects on your T) 195.22 575.35 P
1.33 (ar) 520.19 575.35 P
1.33 (get) 527.78 575.35 P
0.5 (Logsheet. It should be designated) 189 563.35 P
16 F
1.19 (xxx) 328.14 563.35 P
9 F
1.19 (-OFFSET) 346.14 563.35 P
0 F
0.5 (, where) 387.4 563.35 P
16 F
1.19 (xxx) 420.32 563.35 P
0 F
0.5 ( is the name of the tar) 438.32 563.35 P
0.5 (get) 527.78 563.35 P
1.04 (object. If desired, you may give the position of your tar) 189 551.35 P
1.04 (get by using) 420.26 551.35 P
9 F
2.49 (RA-OFF) 474.76 551.35 P
0 F
1.04 (,) 509.96 551.35 P
9 F
2.49 (DEC-) 516 551.35 P
4.01 (OFF) 189 539.35 P
0 F
1.67 (, or) 206.2 539.35 P
9 F
4.01 (XI-OFF) 225.37 539.35 P
0 F
1.67 (,) 260.57 539.35 P
9 F
4.01 (ETA-OFF) 267.24 539.35 P
0 F
1.67 ( and) 309.24 539.35 P
9 F
4.01 (FROM) 332.02 539.35 P
0 F
1.67 ( relative to the of) 356.02 539.35 P
1.67 (fset star) 430.83 539.35 P
1.67 (. See the Proposal) 463.33 539.35 P
0.09 (Instructions for details and notes on proper units. On the Exposure Logsheet, the T) 189 527.35 P
0.09 (ar) 520.19 527.35 P
0.09 (get) 527.78 527.35 P
0.31 (Name for lines 1 and 2 are) 189 515.35 P
16 F
0.74 (xxx) 299.74 515.35 P
9 F
0.74 (-OFFSET) 317.74 515.35 P
0 F
0.31 (, and in the example above, the T) 359.01 515.35 P
0.31 (ar) 493.5 515.35 P
0.31 (get Name) 501.09 515.35 P
(for line 3 is) 189 503.35 T
16 F
(xxx) 237.33 503.35 T
9 F
(.) 255.33 503.35 T
0 F
0.6 (T) 189 483.35 P
0.6 (o make a successful of) 194.41 483.35 P
0.6 (fset, the relative positions of the of) 287.15 483.35 P
0.6 (fset star and tar) 429.71 483.35 P
0.6 (get must be) 492.69 483.35 P
0.11 (very well known \320 about as well as 1/4 the size of the aperture. \050e.g., rms errors of 0.05) 189 471.35 P
0.81 (arcsec for the SSA.\051 One way of obtaining such positions is by requesting an) 189 459.35 P
9 F
1.94 (EARLY) 510 459.35 P
0.66 (ACQ) 189 447.35 P
0 F
0.27 (uisition WFPC2 image, and measuring relative positions from it \050at least 2 months) 207 447.35 P
-0.16 (prior to the science observation\051. The of) 189 435.35 P
-0.16 (fset positioning accuracy of the) 348.1 435.35 P
3 F
-0.16 (HST) 475.33 435.35 P
0 F
-0.16 ( is expected) 493.11 435.35 P
-0.02 (to be very good \050of the order of 0.03 to 0.05 arcsec for a 30 arcsec of) 189 423.35 P
-0.02 (fset\051, and the accu-) 463.98 423.35 P
0.72 (racy of the placement will be primarily determined by the accuracy of your positions.) 189 411.35 P
0.38 (An of) 189 399.35 P
0.38 (fset of more than 30 arcsec may require the telescope to acquire new guide stars,) 212.25 399.35 P
(which would worsen the accuracy of the positioning.) 189 387.35 T
2 F
(4.1.6) 157.76 357.35 T
(MAPs) 189 357.35 T
0 F
0.26 (The GHRS has the ability to make a) 189 337.35 P
9 F
0.63 (MAP) 338.3 337.35 P
0 F
0.26 ( of the LSA by raster scanning one or both of) 356.3 337.35 P
0.4 (its small focus diodes over the aperture. Y) 189 325.35 P
0.4 (ou may) 359.68 325.35 P
0.4 (, for example, want a map to con\336rm) 389.15 325.35 P
0.63 (the pointing at the time your spectrum was taken. The default for) 189 313.35 P
9 F
1.52 (ONBOARD) 459.08 313.35 P
1.52 (ACQ) 504.22 313.35 P
0 F
0.63 (uisi-) 522.22 313.35 P
0.11 (tions is to make no map. If you ask for) 189 301.35 P
9 F
0.26 (MAP=END-POINT) 347.01 301.35 P
0 F
0.11 (, you will get a map after the) 424.27 301.35 P
0.71 (spiral search has found your tar) 189 289.35 P
0.71 (get, but before it has been centered \050with) 318.18 289.35 P
9 F
1.71 (LOCATE) 489.68 289.35 P
0 F
0.71 (\051 in) 525.68 289.35 P
1.07 (the LSA. If you want a map after the \336nal centering, you can add a single Exposure) 189 277.35 P
0.01 (Logsheet line in) 189 265.35 P
9 F
0.03 (IMAGE) 255.98 265.35 P
0 F
0.01 ( mode. An) 285.98 265.35 P
9 F
0.03 (IMAGE) 330.46 265.35 P
0 F
0.01 ( may also be obtained of the SSA, which can) 360.46 265.35 P
0.93 (be a useful) 189 253.35 P
3 F
0.93 (a posteriori) 237.61 253.35 P
0 F
0.93 ( means of determining what was observed in a crowded \336eld.) 285.48 253.35 P
(The) 189 241.35 T
9 F
(MAP=ALL-POINTS) 207.05 241.35 T
0 F
( option may) 291.05 241.35 T
3 F
(not) 341.33 241.35 T
0 F
( be used with an onboard acquisition.) 354.11 241.35 T
2 F
(4.1.7) 157.76 211.35 T
(Acquisition Parameters \321 A Summary) 189 211.35 T
1 F
(Step 1:) 189 191.35 T
0 F
( Mode=) 218.72 191.35 T
9 F
(ACQ) 250.19 191.35 T
10 11 Q
(\245) 189 173.35 T
0 10 Q
(Aperture is always LSA \050\322) 203.4 173.35 T
9 F
(2.0) 310.04 173.35 T
0 F
(\323\051.) 328.04 173.35 T
10 11 Q
(\245) 189 158.35 T
9 10 Q
2.73 (MIRROR) 203.4 158.35 P
0 F
1.14 ( is usually) 239.4 158.35 P
9 F
2.73 (N2) 285.87 158.35 P
0 F
1.14 ( or) 297.87 158.35 P
9 F
2.73 (N1) 313.47 158.35 P
0 F
1.14 ( unless object is too bright \050then use) 325.47 158.35 P
9 F
2.73 (A2) 481.21 158.35 P
0 F
1.14 ( or) 493.21 158.35 P
9 F
2.73 (A1) 508.81 158.35 P
0 F
1.14 (; see) 520.81 158.35 P
0.43 (Section) 203.4 146.35 P
0.43 (7.1 on page) 235.9 146.35 P
0.43 (68\051. Mirrors A1 and N1 may also be used and it is permissible) 285.65 146.35 P
-0.18 (to acquire with one side \050mirror) 203.4 134.35 P
9 F
-0.44 (N2) 331.72 134.35 P
0 F
-0.18 (, say\051 and observe with the other \050grating G140L,) 343.72 134.35 P
(perhaps\051, but with a possible cost in time.) 203.4 122.35 T
10 11 Q
(\245) 189 107.35 T
9 10 Q
0.77 (SEARCH-SIZE=3) 203.4 107.35 P
0 F
0.32 ( is the default and adequate almost all the time. V) 281.4 107.35 P
0.32 (alues of 1 or 5) 481.51 107.35 P
(may also be used.) 203.4 95.35 T
FMENDPAGE
%%EndPage: "40" 40
%%Page: "41" 41
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (41) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Y) 207 736.18 T
(our Phase II Proposal) 212.34 736.18 T
10 11 Q
(\245) 207 679.35 T
9 10 Q
2.65 (BRIGHT=RETURN) 221.4 679.35 P
0 F
1.1 ( is the default for \336nding the tar) 299.4 679.35 P
1.1 (get and should be used unless) 433.88 679.35 P
1.01 (you are forced not to. Do not specify) 221.4 667.35 P
9 F
2.42 (FAINT) 379.17 667.35 P
0 F
1.01 ( unless you must specify an explicit) 409.17 667.35 P
9 F
(BRIGHT) 221.4 655.35 T
0 F
( limit. \050) 257.4 655.35 T
9 F
(FAINT) 287.13 655.35 T
0 F
( is ignored if) 317.13 655.35 T
9 F
(BRIGHT=RETURN) 370.46 655.35 T
0 F
( is used.\051) 448.46 655.35 T
10 11 Q
(\245) 207 640.35 T
9 10 Q
2.51 (LOCATE) 221.4 640.35 P
0 F
1.04 (: Default is) 257.4 640.35 P
9 F
2.51 (YES) 307.48 640.35 P
0 F
1.04 ( for an) 325.48 640.35 P
9 F
2.51 (ONBOARD) 357.21 640.35 P
2.51 (ACQ) 402.76 640.35 P
0 F
1.04 ( and) 420.76 640.35 P
9 F
2.51 (NO) 442.29 640.35 P
0 F
1.04 ( for) 454.29 640.35 P
9 F
2.51 (EARLY) 473.04 640.35 P
2.51 (ACQ) 506.58 640.35 P
0 F
1.04 ( or) 524.58 640.35 P
9 F
2.51 (INT) 540 640.35 P
0.32 (ACQ) 221.4 628.35 P
0 F
0.13 (. W) 239.4 628.35 P
0.13 (e recommend these defaults. Note that) 253.17 628.35 P
9 F
0.32 ( LOCATE=EXTENDED) 407.13 628.35 P
0 F
0.13 ( is now avail-) 503.45 628.35 P
-0.22 (able. W) 221.4 616.35 P
-0.22 (ith an) 251.88 616.35 P
9 F
-0.54 (ONBOARD) 276.42 616.35 P
-0.54 (ACQ) 320.7 616.35 P
0 F
-0.22 (,) 338.7 616.35 P
9 F
-0.54 (LOCATE=NO) 343.47 616.35 P
0 F
-0.22 ( may be used only if) 397.47 616.35 P
9 F
-0.54 (MAP=END-POINT) 480 616.35 P
0 F
(is speci\336ed.) 221.4 604.35 T
10 11 Q
(\245) 207 589.35 T
9 10 Q
0.38 (MAP) 221.4 589.35 P
0 F
0.16 (: The defaults provide for an image to be transmitted to the ground if) 239.4 589.35 P
9 F
0.38 (INT) 519.34 589.35 P
0.38 (ACQ) 540 589.35 P
0 F
-0.24 (or) 221.4 577.35 P
9 F
-0.57 (EARLY) 231.99 577.35 P
-0.57 (ACQ) 264.26 577.35 P
0 F
-0.24 ( is speci\336ed. No image is generated by default for an) 282.26 577.35 P
9 F
-0.57 (ONBOARD) 492.95 577.35 P
-0.57 (ACQ) 537.22 577.35 P
0 F
-0.24 (;) 555.22 577.35 P
9 F
1.47 (MAP=END-POINT) 221.4 565.35 P
0 F
0.61 (will provide one with the tar) 306.87 565.35 P
0.61 (get in the LSA, but it will not be) 423.36 565.35 P
-0.06 (centered. As we have pointed out, if you wish to determine the actual position of the) 221.4 553.35 P
-0.21 (object in the LSA before spectroscopic observations are begun, you should obtain an) 221.4 541.35 P
9 F
1.58 (IMAGE) 221.4 529.35 P
0 F
0.66 ( as a separate Exposure Logsheet line and you should not specify a) 251.4 529.35 P
9 F
1.58 (MAP) 529.62 529.35 P
0 F
0.66 ( at) 547.62 529.35 P
(all.) 221.4 517.35 T
9 F
(MAP=ALL-POINTS) 236.4 517.35 T
0 F
( may not be used with an) 320.4 517.35 T
9 F
(ONBOARD) 422.89 517.35 T
(ACQ) 467.39 517.35 T
0 F
(.) 485.39 517.35 T
10 11 Q
(\245) 207 502.35 T
0 10 Q
(The time per exposure can be calculated from) 221.4 502.35 T
0.36 (where) 221.4 440.14 P
0.36 ( \050i.e., 1, 9, or 25\051, and) 383.81 440.14 P
0.36 ( is the number) 499.98 440.14 P
2.36 (of dwell points mapped \050=1 if) 221.4 428.14 P
9 F
5.67 (MAP=END-POINT) 357.31 428.14 P
0 F
2.36 ( is chosen and =) 435.31 428.14 P
2.36 ( if) 547.03 428.14 P
9 F
2.87 (MAP=ALL-POINTS) 221.4 416.14 P
0 F
1.2 (.) 305.4 416.14 P
9 F
2.87 ( MAP=ALL-POINTS) 307.9 416.14 P
0 F
1.2 ( can only be used with) 400.77 416.14 P
9 F
2.87 (INT) 500.17 416.14 P
2.87 (ACQ) 521.86 416.14 P
0 F
1.2 ( and) 539.86 416.14 P
9 F
0.22 (EARLY) 221.4 404.14 P
0.22 (ACQ) 253.99 404.14 P
0 F
0.09 (.\051.) 271.99 404.14 P
1 F
0.09 (Please note the value of) 282.92 404.14 P
10 F
0.22 (STEP-TIME) 385.32 404.14 P
1 F
0.09 ( you want as a) 439.32 404.14 P
10 F
0.22 (COMMENT) 502.85 404.14 P
1 F
0.09 ( on) 544.85 404.14 P
(the Exposur) 221.4 392.14 T
(e Logsheet.) 273.17 392.14 T
10 11 Q
(\245) 207 377.14 T
0 10 Q
(Special Requirements are) 221.4 377.14 T
9 F
(INT) 326.1 377.14 T
(ACQ) 346.6 377.14 T
0 F
(,) 364.6 377.14 T
9 F
(EARLY) 369.6 377.14 T
(ACQ) 402.1 377.14 T
0 F
(, or) 420.1 377.14 T
9 F
(ONBOARD) 435.93 377.14 T
(ACQ) 480.43 377.14 T
0 F
(.) 498.43 377.14 T
1 F
(Step 2:) 207 357.14 T
0 F
( Mode=) 236.72 357.14 T
9 F
(ACQ/PEAKUP) 268.19 357.14 T
10 11 Q
(\245) 207 339.14 T
0 10 Q
-0.11 (The aperture can be either the LSA \050\322) 221.4 339.14 P
9 F
-0.27 (2.0) 371.39 339.14 P
0 F
-0.11 (\323\051 or SSA \050\322) 389.39 339.14 P
9 F
-0.27 (0.25) 438.76 339.14 P
0 F
-0.11 (\323\051; specify the one to be) 462.76 339.14 P
(used for the science observations that immediately follow) 221.4 327.14 T
(.) 451.55 327.14 T
10 11 Q
(\245) 207 312.14 T
0 10 Q
0.02 (Specify the) 221.4 312.14 P
9 F
0.05 (MIRROR) 269.21 312.14 P
0 F
0.02 ( as for Mode=) 305.21 312.14 P
9 F
0.05 (ACQ) 361.73 312.14 P
0 F
0.02 (; i.e.,) 379.73 312.14 P
9 F
0.05 (N1) 402.27 312.14 P
0 F
0.02 (,) 414.27 312.14 P
9 F
0.05 (A1) 419.3 312.14 P
0 F
0.02 (,) 431.3 312.14 P
9 F
0.05 (N2) 436.32 312.14 P
0 F
0.02 (, or) 448.32 312.14 P
9 F
0.05 (A2) 464.19 312.14 P
0 F
0.02 ( depending on tar) 476.19 312.14 P
0.02 (get) 545.78 312.14 P
(brightness.) 221.4 300.14 T
10 11 Q
(\245) 207 285.14 T
0 10 Q
(The time per exposure can be calculated from) 221.4 285.14 T
1.14 (where) 221.4 225.14 P
3 F
1.14 (f) 249.47 225.14 P
3 8 Q
0.92 (Apertur) 255.9 222.64 P
0.92 (e) 280.49 222.64 P
0 10 Q
1.14 ( = 102 if the LSA is used and = \050) 284.04 225.14 P
9 F
2.75 (SEARCH-SIZE) 426.75 225.14 P
0 F
1.14 (\051) 492.75 225.14 P
0 8 Q
0.92 (2) 496.08 229.14 P
0 10 Q
1.14 ( if the SSA is) 500.08 225.14 P
0.69 (used. Note that the throughput of the SSA is half to 2/3 that of the LSA so that in) 221.4 213.14 P
0.17 (general you should specify a) 221.4 201.14 P
9 F
0.41 (STEP-TIME) 339.17 201.14 P
0 F
0.17 ( that is lar) 393.17 201.14 P
0.17 (ger than the one you used for a) 433.23 201.14 P
9 F
(PEAKUP) 221.4 189.14 T
0 F
( in the LSA.) 257.4 189.14 T
10 11 Q
(\245) 207 174.14 T
0 10 Q
0.02 (W) 221.4 174.14 P
0.02 (e ur) 230.04 174.14 P
0.02 (ge you to be precise and explicit about the way in which you specify an) 245.15 174.14 P
9 F
0.05 (ACQ/) 534 174.14 P
-0.51 (PEAKUP) 221.4 162.14 P
0 F
-0.21 ( and the order in which observations are to be made. The defaults that apply) 257.4 162.14 P
0.79 (to) 221.4 150.14 P
9 F
1.89 (ACQ) 232.47 150.14 P
0 F
0.79 ( and) 250.47 150.14 P
9 F
1.89 (ACQ/PEAKUP) 271.48 150.14 P
0 F
0.79 ( modes will usually accomplish what you wish, but the) 331.48 150.14 P
0.07 (way to be sure is to specify the details. Confusion can arise particularly when a pro-) 221.4 138.14 P
0.17 (gram mixes LSA and SSA observations. W) 221.4 126.14 P
0.17 (e would recommend that you do an) 395.22 126.14 P
9 F
0.41 (ACQ) 540 126.14 P
0 F
0.22 (in the \336rst line of the Exposure Logsheet, then on line 2 specify) 221.4 114.14 P
9 F
0.52 (ACQ/PEAKUP) 480.84 114.14 P
0 F
0.22 ( and) 540.84 114.14 P
1.09 (indicate the lines to which it applies \050all of which should use the same aperture\051.) 221.4 102.14 P
72 87.98 558 686.02 C
140.85 466.81 489.15 484.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(t) 276.32 475.6 T
3 7 Q
(e) 279.48 472.5 T
(x) 283.12 472.5 T
(p) 286.77 472.5 T
0 10 Q
(1) 311.86 475.6 T
(2) 316.86 475.6 T
(8) 321.86 475.6 T
3 F
(N) 337.35 475.6 T
3 7 Q
(M) 344.4 472.5 T
(A) 350.77 472.5 T
(P) 355.58 472.5 T
13 10 Q
(\264) 329.36 475.6 T
3 F
(N) 370.5 475.6 T
3 7 Q
(S) 377.55 472.5 T
(E) 381.59 472.5 T
(A) 386.4 472.5 T
(R) 391.22 472.5 T
(C) 396.03 472.5 T
(H) 401.24 472.5 T
0 10 Q
(+) 362.36 475.6 T
13 F
(\050) 307.57 475.6 T
(\051) 406.75 475.6 T
9 F
(S) 422.24 475.6 T
(T) 428.24 475.6 T
(E) 434.24 475.6 T
(P) 440.24 475.6 T
(-) 446.24 475.6 T
(T) 452.24 475.6 T
(I) 458.24 475.6 T
(M) 464.24 475.6 T
(E) 470.24 475.6 T
13 F
(\264) 414.25 475.6 T
0 F
(=) 295.27 475.6 T
72 87.98 558 686.02 C
0 0 612 792 C
248.69 434.81 383.81 450.94 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(N) 249.33 440.14 T
3 7 Q
(S) 256.38 437.04 T
(E) 260.42 437.04 T
(A) 265.23 437.04 T
(R) 270.05 437.04 T
(C) 274.86 437.04 T
(H) 280.07 437.04 T
9 10 Q
(S) 306.71 440.14 T
(E) 312.71 440.14 T
(A) 318.71 440.14 T
(R) 324.71 440.14 T
(C) 330.71 440.14 T
(H) 336.71 440.14 T
(-) 342.71 440.14 T
(S) 348.71 440.14 T
(I) 354.71 440.14 T
(Z) 360.71 440.14 T
(E) 366.71 440.14 T
13 F
(\050) 302.42 440.14 T
(\051) 373.17 440.14 T
0 7 Q
(2) 378.67 443.02 T
0 10 Q
(=) 290.12 440.14 T
0 0 612 792 C
475.49 434.81 499.98 447.98 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(N) 475.98 440.14 T
3 7 Q
(M) 483.03 437.04 T
(A) 489.39 437.04 T
(P) 494.21 437.04 T
0 0 612 792 C
509.27 422.81 547.03 435.98 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(N) 509.75 428.14 T
3 7 Q
(S) 516.8 425.04 T
(E) 520.84 425.04 T
(A) 525.66 425.04 T
(R) 530.47 425.04 T
(C) 535.29 425.04 T
(H) 540.49 425.04 T
0 0 612 792 C
221.4 244 495 271 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(t) 305.09 255.14 T
3 7 Q
(e) 308.25 252.04 T
(x) 311.89 252.04 T
(p) 315.54 252.04 T
3 10 Q
(f) 334.67 255.14 T
3 7 Q
(A) 337.84 252.04 T
(p) 342.65 252.04 T
(e) 346.69 252.04 T
(r) 350.33 252.04 T
(t) 353.6 252.04 T
(u) 356.08 252.04 T
(r) 360.12 252.04 T
(e) 363.38 252.04 T
9 10 Q
(S) 376.98 255.14 T
(T) 382.98 255.14 T
(E) 388.98 255.14 T
(P) 394.98 255.14 T
(-) 400.98 255.14 T
(T) 406.98 255.14 T
(I) 412.98 255.14 T
(M) 418.98 255.14 T
(E) 424.98 255.14 T
13 F
(\264) 368.99 255.14 T
0 F
(=) 324.04 255.14 T
0 0 612 792 C
FMENDPAGE
%%EndPage: "41" 41
%%Page: "42" 42
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Y) 189 736.18 T
(our Phase II Proposal) 194.34 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(42) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
0.68 (Also indicate a) 203.4 679.35 P
9 F
1.64 (NO) 267.94 679.35 P
1.64 (GAP) 283.12 679.35 P
0 F
0.68 ( Special Requirement for that group of lines. Then specify) 301.12 679.35 P
0.36 (another) 203.4 667.35 P
9 F
0.87 (ACQ/PEAKUP) 236.25 667.35 P
0 F
0.36 ( before starting observations in the other aperture, and again) 296.25 667.35 P
(specify) 203.4 655.35 T
9 F
(NO) 234.78 655.35 T
(GAP) 249.28 655.35 T
0 F
( to ensure that they are treated as a group.) 267.28 655.35 T
54 612.02 540 615.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 613.52 540 613.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 613.52 180 613.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(4.2) 163.32 619.02 T
(Image Mode) 189 619.02 T
0 10 Q
0.29 (The GHRS is, of course, primarily a spectrograph, but it includes useful imaging capa-) 189 595.35 P
0.65 (bilities, especially because the detectors of the GHRS are blind to much of the visible) 189 583.35 P
0.25 (light that dominates the \337ux of most stars. Y) 189 571.35 P
0.25 (ou may wish to request an) 368.07 571.35 P
9 F
0.6 (IMAGE) 476.78 571.35 P
0 F
0.25 ( or) 506.78 571.35 P
9 F
0.6 (MAP) 520.61 571.35 P
0 F
0.25 (,) 537.5 571.35 P
-0.02 (for example, to con\336rm that the telescope had your object properly centered in the data-) 189 559.35 P
(taking aperture before the exposure was taken.) 189 547.35 T
(Note the following in using the imaging capability:) 189 527.35 T
10 11 Q
(\245) 189 509.35 T
0 10 Q
1.18 (GHRS) 203.4 509.35 P
9 F
2.84 (IMAGE) 233.75 509.35 P
0 F
1.18 (s and) 263.75 509.35 P
9 F
2.84 (MAP) 289.45 509.35 P
0 F
1.18 (s are obtained with the focus diodes \050see Section) 307.45 509.35 P
1.18 (6.3 on) 513.82 509.35 P
1.87 (page) 203.4 497.35 P
1.87 (62\051 at the ends of the array of main science diodes. The focus diodes are) 224.78 497.35 P
1.47 (smaller and square, making them more useful for focusing, but at the price of a) 203.4 485.35 P
-0.24 (lower count rate. The total count rate over the LSA is, of course, unchanged, and it is) 203.4 473.35 P
0.18 (that which is predicted with the information in Section) 203.4 461.35 P
0.18 (7.1 on page) 425.67 461.35 P
0.18 (68. Multiply the) 474.91 461.35 P
1.24 (count rate estimated for the regular diodes by approximately 0.3 to get the value) 203.4 449.35 P
(appropriate to the focus diodes when they are centered on the star) 203.4 437.35 T
(.) 465.28 437.35 T
10 11 Q
(\245) 189 422.35 T
0 10 Q
0.02 (A) 203.4 422.35 P
9 F
0.05 (MAP) 213.14 422.35 P
0 F
0.02 ( is obtained as an integral part of an acquisition whereas an) 231.14 422.35 P
9 F
0.05 (IMAGE) 470.23 422.35 P
0 F
0.02 ( is a sepa-) 500.23 422.35 P
-0.24 (rate observation that may or may not have anything to do with an acquisition. A) 203.4 410.35 P
9 F
-0.57 (MAP) 522 410.35 P
0 F
0.64 (with) 203.4 398.35 P
9 F
1.53 (SEARCH-SIZE=3) 224.32 398.35 P
0 F
0.64 ( or) 302.32 398.35 P
9 F
1.53 (5) 316.92 398.35 P
0 F
0.64 ( is made as the acquisition procedure causes the tele-) 322.92 398.35 P
0.1 (scope to make small motions in a square spiral pattern, thereby enabling it to record) 203.4 386.35 P
0.2 (a lar) 203.4 374.35 P
0.2 (ger portion of the sky than the LSA itself subtends. An) 220.91 374.35 P
9 F
0.47 (IMAGE) 444.71 374.35 P
0 F
0.2 ( can only record) 474.71 374.35 P
1.47 (the light in the) 203.4 362.35 P
1.47 ( arcsec region of the LSA. A single) 317.32 362.35 P
9 F
3.54 (MAP) 472.7 362.35 P
0 F
1.47 ( \050) 490.7 362.35 P
9 F
3.54 (SEARCH-) 498 362.35 P
3.02 (SIZE=1) 203.4 350.35 P
0 F
1.26 (\051 is equivalent to an) 239.4 350.35 P
9 F
3.02 (IMAGE) 327.07 350.35 P
0 F
1.26 (. Note that) 357.07 350.35 P
9 F
3.02 (MAP=ALL-POINTS) 405.29 350.35 P
0 F
1.26 ( may not be) 489.29 350.35 P
(used with an) 203.4 338.35 T
9 F
(ONBOARD) 256.45 338.35 T
(ACQ) 300.95 338.35 T
0 F
(.) 318.95 338.35 T
10 11 Q
(\245) 189 323.35 T
0 10 Q
1.49 (A standard) 203.4 323.35 P
9 F
3.57 (IMAGE) 252.48 323.35 P
0 F
1.49 ( will have a pixel spacing of 0.109 arcsec and will cover the) 282.48 323.35 P
1.13 (entire LSA aperture of 1.74) 203.4 311.35 P
13 F
1.13 ( \264) 318.16 311.35 P
0 F
1.13 (1.74 arcsec. Y) 330.91 311.35 P
1.13 (ou may also select pixel spacings of) 389.36 311.35 P
1.13 (0.055 or 0.027 arcsec, with proportionately smaller regions of the sky covered in) 203.4 299.35 P
(a) 203.4 287.35 T
( \050the default\051) 240.32 287.35 T
9 F
(IMAGE) 294.47 287.35 T
0 F
(. Y) 324.47 287.35 T
(ou may also use) 335.69 287.35 T
9 F
(IMAGE) 402.35 287.35 T
0 F
( with the SSA.) 432.35 287.35 T
2 F
(4.2.1) 157.76 257.35 T
(Image Mode Parameters) 189 257.35 T
10 11 Q
(\245) 189 241.35 T
0 10 Q
-0.16 (Either the LSA \050\322) 203.4 241.35 P
9 F
-0.39 (2.0) 273.73 241.35 P
0 F
-0.16 (\323\051 or SSA \050\322) 291.73 241.35 P
9 F
-0.39 (0.25) 340.96 241.35 P
0 F
-0.16 (\323\051 may be selected as the aperture. The SSA) 364.96 241.35 P
0.81 (is so small that it is generally pointless to image it, although there may be special) 203.4 229.35 P
2.57 (cases where) 203.4 217.35 P
9 F
6.16 (IMAGE) 259.07 217.35 P
0 F
2.57 ( mode is of use, particularly for con\336rming pointing in a) 289.07 217.35 P
(crowded \336eld.) 203.4 205.35 T
10 11 Q
(\245) 189 190.35 T
0 10 Q
-0.23 (A mirror is the usual choice as optical element. A grating may also be speci\336ed \320 see) 203.4 190.35 P
(below) 203.4 178.35 T
(.) 227.19 178.35 T
10 11 Q
(\245) 189 163.35 T
0 10 Q
1.21 (The number of pixels in the) 203.4 163.35 P
3 F
1.21 (x) 323.95 163.35 P
0 F
1.21 ( and) 328.39 163.35 P
3 F
1.21 (y) 350.24 163.35 P
0 F
1.21 ( directions can be chosen separately and can) 354.68 163.35 P
0 (range from 1 to 512 pixels. However) 203.4 151.35 P
0 (, a lar) 350.48 151.35 P
0 (ge number of pixels only oversamples the) 372.79 151.35 P
0.22 (region of sky subtended by the LSA and does not make the) 203.4 139.35 P
9 F
0.51 (IMAGE) 444.84 139.35 P
0 F
0.22 ( include a lar) 474.84 139.35 P
0.22 (ger) 527.23 139.35 P
-0.12 (area. The parameters to specify are) 203.4 127.35 P
9 F
-0.28 (NX) 345.14 127.35 P
0 F
-0.12 (,) 357.14 127.35 P
9 F
-0.28 (NY) 362.02 127.35 P
0 F
-0.12 (,) 372.73 127.35 P
9 F
-0.28 (DELTA-X) 377.61 127.35 P
0 F
-0.12 (, and) 419.61 127.35 P
9 F
-0.28 (DELTA-Y) 441.32 127.35 P
0 F
-0.12 (, for which the) 482.03 127.35 P
-0.16 (defaults are 16, 16, 4, and 4, respectively) 203.4 115.35 P
-0.16 (. The product of) 365.78 115.35 P
9 F
-0.38 (NX) 432.08 115.35 P
0 F
-0.16 ( and) 444.08 115.35 P
9 F
-0.38 (NY) 463.21 115.35 P
0 F
-0.16 ( may not exceed) 475.21 115.35 P
-0.04 (512. An image that is critically sampled in the) 203.4 103.35 P
3 F
-0.04 (x) 390.26 103.35 P
0 F
-0.04 ( direction may be obtained by speci-) 394.7 103.35 P
(fying) 203.4 91.35 T
9 F
(NX=32) 227.01 91.35 T
0 F
(,) 257.01 91.35 T
9 F
(NY=16) 262.01 91.35 T
0 F
(,) 292.01 91.35 T
9 F
(DELTA-X=2) 297.01 91.35 T
0 F
(, and) 351.01 91.35 T
9 F
(DELTA-Y=4) 372.95 91.35 T
0 F
(.) 426.95 91.35 T
269.86 359.18 317.32 370.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 270.35 362.35 T
(.) 275.35 362.35 T
(7) 277.85 362.35 T
(4) 282.85 362.35 T
(1) 298.33 362.35 T
(.) 303.33 362.35 T
(7) 305.83 362.35 T
(4) 310.83 362.35 T
13 F
(\264) 290.35 362.35 T
0 0 612 792 C
207.84 284.18 240.32 295.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 208.33 287.35 T
(6) 213.33 287.35 T
(1) 228.82 287.35 T
(6) 233.82 287.35 T
13 F
(\264) 220.83 287.35 T
0 0 612 792 C
FMENDPAGE
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612 792 0 FMBEGINPAGE
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0 0 0 1 0 0 0 K
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0 0 0 1 0 0 0 K
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72 750.02 558 750.02 2 L
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0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
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72 74.02 558 74.02 2 L
2 Z
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2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (43) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Y) 207 736.18 T
(our Phase II Proposal) 212.34 736.18 T
0 10 Q
0.93 (Only the N1 mirror intercepts the full beam diameter) 221.4 679.35 P
0.93 (, meaning that images of the) 440.05 679.35 P
-0.15 (LSA with the other acquisition mirrors will not yield an accurate Point Spread Func-) 221.4 667.35 P
(tion \050PSF\051.) 221.4 655.35 T
10 11 Q
(\245) 207 640.35 T
0 10 Q
1.05 (The) 221.4 640.35 P
9 F
2.52 (PRECISION) 240.5 640.35 P
0 F
1.05 ( parameter may be speci\336ed as) 294.5 640.35 P
9 F
2.52 (NORMAL) 426.32 640.35 P
0 F
1.05 ( \050the default\051 or) 462.32 640.35 P
9 F
2.52 (HIGH) 531.5 640.35 P
0 F
1.05 (.) 555.5 640.35 P
9 F
3.63 (PRECISION) 221.4 628.35 P
0 F
1.51 ( may only be speci\336ed if) 275.4 628.35 P
9 F
3.63 (DELTA-Y=4) 385.58 628.35 P
0 F
1.51 (. Using) 439.58 628.35 P
9 F
3.63 (PRECISION=HIGH) 474 628.35 P
0 F
0.59 (causes the image to be obtained with only one focus diode instead of two \050thereby) 221.4 616.35 P
-0.09 (eliminating uncertainty over the relative response of the two\051, but the time per expo-) 221.4 604.35 P
-0.06 (sure you must list is the same in either case \050but using) 221.4 592.35 P
9 F
-0.14 (PRECISION=NORMAL) 439.01 592.35 P
0 F
-0.06 ( takes) 535.01 592.35 P
-0.23 (less actual time to execute and the dif) 221.4 580.35 P
-0.23 (ferences in response of the diodes are known to) 369.87 580.35 P
(be small\051.) 221.4 568.35 T
10 11 Q
(\245) 207 553.35 T
0 10 Q
1.29 (There are two focus diodes available to raster over the LSA. Thus the total time) 221.4 553.35 P
0.59 (needed is the dwell time per pixel \0500.2 seconds is the default\051 times the number of) 221.4 541.35 P
0.35 (pixels in the) 221.4 529.35 P
3 F
0.35 (x) 273.84 529.35 P
0 F
0.35 ( direction \050default is) 278.28 529.35 P
9 F
0.84 (NX=16) 363 529.35 P
0 F
0.35 (\051 times the number of) 393 529.35 P
3 F
0.35 (y) 483.35 529.35 P
0 F
0.35 ( pixels \050default is) 487.79 529.35 P
9 F
1.22 (NY=16) 221.4 517.35 P
0 F
0.51 (\051, all divided by 2. The maximum permissible dwell time per pixel is 12.75) 251.4 517.35 P
0.67 (seconds. \050Note that the) 221.4 505.35 P
3 F
0.67 (Phase II Pr) 318.22 505.35 P
0.67 (oposal Instructions) 365.29 505.35 P
0 F
0.67 ( for Cycle 4 required you to) 442.9 505.35 P
1.84 (calculate the total time without dividing by the factor of two. The situation for) 221.4 493.35 P
(Cycle) 221.4 481.35 T
(5 should be con\336rmed before a value is entered.\051) 247.23 481.35 T
2 F
(4.2.2) 175.76 451.35 T
(The GHRS as a Slitless Spectrograph) 207 451.35 T
0 F
0.24 (In) 207 431.35 P
9 F
0.57 (IMAGE) 218.07 431.35 P
0 F
0.24 ( mode you may specify a grating instead of a mirror as the spectrum element) 248.07 431.35 P
0.58 (\050note that this may) 207 419.35 P
3 F
0.58 (not) 286.54 419.35 P
0 F
0.58 ( be done in Acquisition Mode\051. Doing so for a tar) 299.32 419.35 P
0.58 (get that emits) 502.95 419.35 P
0.79 (primarily in lines can yield the equivalent of using a slitless spectrograph over a very) 207 407.35 P
1.31 (small portion of the sky \050the 1.74 arcsec square region of the LSA\051. Thus the focus) 207 395.35 P
0.59 (diodes would be swept over the image of the line to produce a picture that is resolved) 207 383.35 P
1.01 (spatially in the) 207 371.35 P
3 F
1.01 (y) 271.41 371.35 P
0 F
1.01 ( direction and spectroscopically in the) 275.85 371.35 P
3 F
1.01 (x) 436.31 371.35 P
0 F
1.01 ( direction. This mode of use) 440.75 371.35 P
1.04 (would be very slow if all you wanted was the spatial structure of a small object \050the) 207 359.35 P
0.38 (FOC would probably be better\051, but there might be interesting uses for obtaining spec-) 207 347.35 P
-0.03 (trophotometrically pure, spatially resolved images in the ultraviolet. Please consult us if) 207 335.35 P
(you wish to explore this option.) 207 323.35 T
72 280.02 558 283.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 281.52 558 281.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 281.52 198 281.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(4.3) 181.32 287.02 T
(Accumulation Mode) 207 287.02 T
2 10 Q
(4.3.1) 175.76 253.35 T
(Optimizing Data Quality) 207 253.35 T
0 F
0.5 (The previous chapter provided the information needed to estimate an exposure time to) 207 233.35 P
0.57 (achieve a given level of signal-to-noise. W) 207 221.35 P
0.57 (e reiterate several factors having to do with) 380.98 221.35 P
-0.15 (the detectors that must be taken into account to achieve the best data quality) 207 209.35 P
-0.15 (. Note that it) 508.46 209.35 P
0.2 (is not necessary to explicitly specify these parameters \050except for) 207 197.35 P
9 F
0.49 (FP-SPLIT) 472.32 197.35 P
0 F
0.2 (\051 because) 520.32 197.35 P
-0.13 (the defaults that apply to each mode of operation will automatically invoke them. More-) 207 185.35 P
(over) 207 173.35 T
(, you should not deviate from the defaults without good reason.) 224.37 173.35 T
1.19 (The Digicon detectors have faceplates with some granularity \050uneven response\051. The) 207 153.35 P
0.06 (diodes onto which the faceplate is imaged also have response irregularities and some of) 207 141.35 P
0.58 (them have been turned of) 207 129.35 P
0.58 (f because of misbehavior) 310.79 129.35 P
0.58 (. Both of these ef) 412.23 129.35 P
0.58 (fects are relatively) 482.98 129.35 P
0.05 (small but enough to prevent you from obtaining a spectrum with S/N much in excess of) 207 117.35 P
2.25 (50. They can also produce \322glitches\323 that can mimic spectrum features. The) 207 105.35 P
9 F
5.39 (FP-) 540 105.35 P
-0.19 (SPLIT) 207 93.35 P
0 F
-0.08 ( parameter causes the carrousel to move slightly between each of the two or four) 237 93.35 P
FMENDPAGE
%%EndPage: "43" 43
%%Page: "44" 44
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
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0 X
0 0 0 1 0 0 0 K
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2 9 Q
(Y) 189 736.18 T
(our Phase II Proposal) 194.34 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
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2 10 Q
(44) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
0.5 (separate subexposures. The) 189 679.35 P
9 F
1.21 (COMB) 302.7 679.35 P
0 F
0.5 ( parameter suppresses diode-to-diode gain variations) 326.7 679.35 P
-0.2 (and allows one to work around the dead diodes. Both features should be used, especially) 189 667.35 P
(since they cost little or nothing in exposure time and improve data quality) 189 655.35 T
(.) 483.33 655.35 T
2.09 (The Digicon diodes also undersample the spectrum by about a factor of two. The) 189 635.35 P
0.54 (parameter) 189 623.35 P
9 F
1.3 (STEP-PATT) 232.02 623.35 P
0 F
0.54 ( causes electronic motions of the spectrum so as to sample the) 286.02 623.35 P
0.87 (spectrum fully) 189 611.35 P
0.87 (. It is possible to) 247.26 611.35 P
9 F
2.08 (STEP-PATT) 319.93 611.35 P
0 F
0.87 ( at two samples per diode width, but we) 373.93 611.35 P
0.37 (recommend using four samples per diode to yield optimum results, and again at no net) 189 599.35 P
0.91 (cost. Y) 189 587.35 P
0.91 (ou can always rebin a quarter) 217.24 587.35 P
0.91 (-stepped spectrum into a half-stepped one during) 339.04 587.35 P
1.29 (your data analysis, but the process cannot make a quarter) 189 575.35 P
1.29 (-stepped spectrum out of a) 428.73 575.35 P
2.18 (half-stepped one. Deconvolution has worked best with quarter) 189 563.35 P
2.18 (-stepped spectra \050the) 452.89 563.35 P
0.22 (default\051; see Gilliland et al. \0501992\051.) 189 551.35 P
9 F
0.53 (STEP-PATT) 333.64 551.35 P
0 F
0.22 ( also determines the way in which the) 387.64 551.35 P
(background is measured \050see Section) 189 539.35 T
(8.4 on page) 339.8 539.35 T
(92\051.) 388.68 539.35 T
0.97 (W) 189 519.35 P
0.97 (e also remind you to break up long exposures into subexposures that are no longer) 197.64 519.35 P
-0.03 (than about 5 minutes each, so as to defeat the ef) 189 507.35 P
-0.03 (fects of geomagnetically-induced image) 379.86 507.35 P
1.94 (motion. Bear in mind that a 20 minute exposure, for example, speci\336ed with) 189 495.35 P
9 F
4.66 (FP-) 522 495.35 P
(SPLIT=4) 189 483.35 T
0 F
( will result in four 5-minute exposures.) 231 483.35 T
2 F
(4.3.2) 157.76 453.35 T
(Summary of Accumulation Mode Parameters) 189 453.35 T
10 11 Q
(\245) 189 437.35 T
0 10 Q
0.64 (Specify the aperture as \322) 203.4 437.35 P
9 F
1.54 (2.0) 304.27 437.35 P
0 F
0.64 (\323 \050LSA\051 or \322) 322.27 437.35 P
9 F
1.54 (0.25) 374.46 437.35 P
0 F
0.64 (\323 \050SSA\051. The object will automati-) 398.46 437.35 P
0.12 (cally be moved to the correct aperture even if the acquisition was into the other) 203.4 425.35 P
0.12 (. If a) 521.16 425.35 P
0.62 (SSA spectroscopic observation follows an LSA spectroscopic observation, we rec-) 203.4 413.35 P
-0.19 (ommend an) 203.4 401.35 P
9 F
-0.47 (ACQ/PEAKUP) 252.45 401.35 P
0 F
-0.19 ( in the SSA with) 312.45 401.35 P
9 F
-0.47 (SEARCH-SIZE=5) 380.1 401.35 P
0 F
-0.19 ( before beginning an) 458.1 401.35 P
9 F
(ACCUM) 203.4 389.35 T
0 F
(.) 233.4 389.35 T
10 11 Q
(\245) 189 374.35 T
0 10 Q
2.55 (If wavelength accuracy is needed that exceeds the default \050see Section) 203.4 374.35 P
2.55 (4.5 on) 512.45 374.35 P
1.39 (page) 203.4 362.35 P
1.39 (46\051, then specify) 224.78 362.35 P
9 F
3.34 (WAVE) 298.38 362.35 P
0 F
1.39 ( as the tar) 322.38 362.35 P
1.39 (get with an aperture of) 364.97 362.35 P
9 F
3.34 (SC2) 464.95 362.35 P
0 F
1.39 (. Get a) 482.95 362.35 P
9 F
3.34 (WAVE) 516 362.35 P
3 F
(befor) 203.4 350.35 T
(e) 224.14 350.35 T
0 F
( the) 228.58 350.35 T
9 F
(ACCUM) 245.8 350.35 T
0 F
( to which it is to apply) 275.8 350.35 T
(.) 364.6 350.35 T
10 11 Q
(\245) 189 335.35 T
0 10 Q
0.65 (Specify the grating to be used, either \336rst-order or echelle. If you wish to force an) 203.4 335.35 P
0.33 (echelle observation to be done in an order other than the default, you may do so by) 203.4 323.35 P
(specifying the grating as, for example,) 203.4 311.35 T
9 F
(ECH-B24) 359.48 311.35 T
0 F
(, where 24 was the order chosen.) 401.48 311.35 T
10 11 Q
(\245) 189 296.35 T
9 10 Q
-0.35 (STEP-PATT) 203.4 296.35 P
0 F
-0.15 ( may be chosen as a number from 1 to 15, and speci\336c pattern numbers) 257.4 296.35 P
0.5 (go with speci\336c spectrograph con\336gurations. W) 203.4 284.35 P
0.5 (e recommend using the default that) 396.71 284.35 P
1.05 (pertains to the setup you have chosen. The details of how the substepping is per-) 203.4 272.35 P
(formed and the background measured are given in Section) 203.4 260.35 T
(8.4 on page) 439.18 260.35 T
(92.) 488.06 260.35 T
10 11 Q
(\245) 189 245.35 T
9 10 Q
2.31 (FP-SPLIT=STD) 203.4 245.35 P
0 F
0.96 ( is recommended. The default for) 275.4 245.35 P
9 F
2.31 (FP-SPLIT) 416.98 245.35 P
0 F
0.96 ( is) 464.98 245.35 P
9 F
2.31 (NO) 478.57 245.35 P
0 F
0.96 (, which will) 490.57 245.35 P
3 F
(not) 203.4 233.35 T
0 F
( yield a spectrum with the best signal-to-noise.) 216.18 233.35 T
10 11 Q
(\245) 189 218.35 T
9 10 Q
(COMB=FOUR) 203.4 218.35 T
0 F
( is the default value and is recommended for the best results.) 257.4 218.35 T
10 11 Q
(\245) 189 203.35 T
9 10 Q
6.11 (DOPPLER=DEF) 203.4 203.35 P
0 F
2.55 ( is recommended. This activates compensation for the velocity) 269.4 203.35 P
0.29 (shifts of astronomical spectra over the course of an orbit but turns it of) 203.4 191.35 P
0.29 (f for internal) 488.88 191.35 P
(exposures.) 203.4 179.35 T
10 11 Q
(\245) 189 164.35 T
9 10 Q
3.15 (STEP-TIME) 203.4 164.35 P
0 F
1.32 ( may be speci\336ed as a number from 0.2 to 12.75 seconds, in incre-) 257.4 164.35 P
0.31 (ments of 0.05 seconds.) 203.4 152.35 P
9 F
0.75 (STEP-TIME) 298.54 152.35 P
0 F
0.31 ( speci\336es the length of the individual subspec-) 352.54 152.35 P
0.63 (tra that are accumulated to form the \336nal spectrum, and there is no good reason to) 203.4 140.35 P
(not use the default of 0.2 sec.) 203.4 128.35 T
10 11 Q
(\245) 189 113.35 T
0 10 Q
-0.08 (The) 203.4 113.35 P
9 F
-0.2 (CENSOR) 221.37 113.35 P
0 F
-0.08 ( parameter may also be speci\336ed. The default is) 257.37 113.35 P
9 F
-0.2 (NO) 449.92 113.35 P
0 F
-0.08 (, which is appropri-) 461.92 113.35 P
0.41 (ate in almost all cases. If) 203.4 101.35 P
9 F
0.99 (CENSOR=YES) 307.26 101.35 P
0 F
0.41 ( is used, individual subspectra \050of duration) 367.26 101.35 P
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
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7 FrameSetSepColors
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (45) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Y) 207 736.18 T
(our Phase II Proposal) 212.34 736.18 T
9 10 Q
4.64 (STEP-TIME) 221.4 679.35 P
0 F
1.93 (, which should be used at the default value of 0.2s\051 are examined) 275.4 679.35 P
0.56 (onboard the spacecraft and are discarded if multiple counts have occurred within a) 221.4 667.35 P
0.65 (8) 221.4 655.35 P
13 F
0.65 (m) 228.9 655.35 P
0 F
0.65 (s interval. This allows for the lowering of background noise in cases where the) 234.66 655.35 P
0.89 (object being observed is very faint, i.e., less than about 0.1 counts per second per) 221.4 643.35 P
2.04 (diode. Rejected exposures are repeated by the GHRS, leading to a longer total) 221.4 631.35 P
0.32 (elapsed time for the observation, but only by about 2%. Since the observation must) 221.4 619.35 P
0.5 (end at a speci\336c time that is predetermined in the spacecraft schedule, using) 221.4 607.35 P
9 F
1.21 (CEN-) 534 607.35 P
-0.48 (SOR) 221.4 595.35 P
0 F
-0.2 ( involves a risk of losing all the data if too many subexposures are rejected. This) 239.4 595.35 P
-0.05 (is guarded against by adding some padding time in the observation planning process) 221.4 583.35 P
1.58 (\050that is done at STScI and does not af) 221.4 571.35 P
1.58 (fect the exposure time you estimate\051. See) 383.83 571.35 P
(Section) 221.4 559.35 T
(8.6.2 on page) 253.9 559.35 T
(95 for more information on) 310.28 559.35 T
9 F
(CENSOR) 422.21 559.35 T
0 F
(.) 458.21 559.35 T
10 11 Q
(\245) 207 544.35 T
0 10 Q
1.14 (A special commanding option called) 221.4 544.35 P
9 F
2.73 (FLYLIM) 376.25 544.35 P
0 F
1.14 ( can also be used to reject noise in) 412.25 544.35 P
0.91 (cases where the object is substantially fainter than the background. Please consult) 221.4 532.35 P
(with us if you wish to explore this possibility) 221.4 520.35 T
(.) 401.32 520.35 T
10 11 Q
(\245) 207 505.35 T
0 10 Q
0.75 (If you have any doubts about the manner in which your program will be executed) 221.4 505.35 P
2.13 (\050which spectra \336rst, whether a peakup is done, etc.\051, remove the ambiguity by) 221.4 493.35 P
3.46 (explicitly indicating the nature and order of the exposures on the Exposure) 221.4 481.35 P
(Logsheet.) 221.4 469.35 T
2 F
(4.3.3) 175.76 439.35 T
10 F
(WSCAN) 207 439.35 T
2 F
( mode) 237 439.35 T
0 F
0.16 (Use of) 207 419.35 P
9 F
0.39 (WSCAN) 236.21 419.35 P
0 F
0.16 ( can result in a spectrum covering a broader total bandpass than is possi-) 266.21 419.35 P
0.37 (ble with a single exposure. All the parameters listed above for an) 207 407.35 P
9 F
0.9 (ACCUM) 473.94 407.35 P
0 F
0.37 ( exposure are) 503.94 407.35 P
0.7 (available in) 207 395.35 P
9 F
1.68 (WSCAN) 257.28 395.35 P
0 F
0.7 ( mode. The most important parameter to specify is) 287.28 395.35 P
9 F
1.68 (WAVE-STEP,) 498 395.35 P
0 F
0.5 (which is the spacing \050in \201ngstroms\051 between each subexposure. If) 207 383.35 P
9 F
1.2 (WAVE-STEP=DEF) 480 383.35 P
0 F
0.04 (is speci\336ed, the central wavelengths of the separate exposures will be equally spaced so) 207 371.35 P
0.71 (as to cover the range of wavelengths that you specify) 207 359.35 P
0.71 (, with at least 20% overlap from) 425.17 359.35 P
(one subspectrum to the next.) 207 347.35 T
0.16 (Y) 207 327.35 P
0.16 (ou may also explicitly give a) 213.22 327.35 P
9 F
0.38 (WAVE-STEP) 331.95 327.35 P
0 F
0.16 ( value. If) 385.95 327.35 P
0.16 ( is the central wavelength of) 444.17 327.35 P
1.1 (the shortest-wavelength exposure, and) 207 315.35 P
1.1 ( is the central wavelength of the longest-) 387.8 315.35 P
0.94 (wavelength exposure, then choose these values in concert with) 207 303.35 P
9 F
2.24 (WAVE-STEP) 468.7 303.35 P
0 F
0.94 ( so as to) 522.7 303.35 P
(yield an integral number of) 207 291.35 T
9 F
(WAVE-STEP) 318.37 291.35 T
0 F
(s between) 372.37 291.35 T
( and) 434.01 291.35 T
(.) 474.04 291.35 T
2 F
(4.3.4) 175.76 261.35 T
10 F
(OSCAN) 207 261.35 T
2 F
( mode) 237 261.35 T
0 F
0.12 (This mode makes it possible to scan across echelle orders at a \336xed value of) 207 241.35 P
3 F
0.12 (m) 515.74 241.35 P
13 F
0.12 (l) 522.96 241.35 P
0 F
0.12 (, where) 528.45 241.35 P
3 F
0.3 (m) 207 229.35 P
0 F
0.3 ( is the order number and) 214.22 229.35 P
13 F
0.3 (l) 315.98 229.35 P
0 F
0.3 ( is the wavelength. It is rare that adjacent orders both have) 321.46 229.35 P
0.1 (features of astrophysical interest and so this mode is primarily used for calibrations and) 207 217.35 P
0.57 (not for science observations. If you do use this mode, all the parameters of an) 207 205.35 P
9 F
1.37 (ACCUM) 528 205.35 P
0 F
(observation are available.) 207 193.35 T
72 150.02 558 153.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 151.52 558 151.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 151.52 198 151.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(4.4) 181.32 157.02 T
(Rapid Readout Mode) 207 157.02 T
0 10 Q
0.42 (This mode is sometimes referred to as Direct Downlink. A normal) 207 133.35 P
9 F
1.01 (ACCUM) 479.39 133.35 P
0 F
0.42 ( exposure is) 509.39 133.35 P
1.16 (the best way to get a good spectrum because all the features of the spectrograph are) 207 121.35 P
1.38 (available to you: automatic compensation for the motion of the spacecraft along the) 207 109.35 P
2.35 (line-of-sight, rejection of high-noise subspectra with) 207 97.35 P
9 F
5.63 (CENSOR) 433.54 97.35 P
0 F
2.35 (, use of) 469.54 97.35 P
9 F
5.63 (FP-SPLIT) 508.24 97.35 P
0 F
2.35 (,) 555.5 97.35 P
424.74 321.29 444.17 335.01 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
13 10 Q
0 X
0 0 0 1 0 0 0 K
(l) 425.23 327.35 T
3 7 Q
(m) 431.11 324.25 T
(i) 436.7 324.25 T
(n) 439.18 324.25 T
0 0 612 792 C
367.21 309.29 387.8 323.01 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
13 10 Q
0 X
0 0 0 1 0 0 0 K
(l) 367.71 315.35 T
3 7 Q
(m) 373.58 312.25 T
(a) 379.17 312.25 T
(x) 383.21 312.25 T
0 0 612 792 C
414.58 285.29 434.01 299.01 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
13 10 Q
0 X
0 0 0 1 0 0 0 K
(l) 415.07 291.35 T
3 7 Q
(m) 420.94 288.25 T
(i) 426.53 288.25 T
(n) 429.02 288.25 T
0 0 612 792 C
453.45 285.29 474.04 299.01 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
13 10 Q
0 X
0 0 0 1 0 0 0 K
(l) 453.94 291.35 T
3 7 Q
(m) 459.81 288.25 T
(a) 465.4 288.25 T
(x) 469.44 288.25 T
0 0 612 792 C
FMENDPAGE
%%EndPage: "45" 45
%%Page: "46" 46
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Y) 189 736.18 T
(our Phase II Proposal) 194.34 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(46) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
9 F
1.12 (COMB) 189 679.35 P
0 F
0.47 (, and) 213 679.35 P
9 F
1.12 (STEP-PATT) 235.87 679.35 P
0 F
0.47 ( to optimize data quality) 289.87 679.35 P
0.47 (, and so on. However) 388.3 679.35 P
0.47 (, there are times) 474.74 679.35 P
-0.04 (when) 189 667.35 P
9 F
-0.1 (ACCUM) 213.12 667.35 P
0 F
-0.04 ( cannot obtain successive spectra as quickly as is needed to probe a partic-) 243.12 667.35 P
(ular phenomenon.) 189 655.35 T
0.1 (In those cases you can use) 189 635.35 P
9 F
0.23 (RAPID) 297.33 635.35 P
0 F
0.1 ( mode. The data are read from the detector at the end) 327.33 635.35 P
0.22 (of each short integration, either to the science tape recorder on) 189 623.35 P
3 F
0.22 (HST) 443.52 623.35 P
0 F
0.22 ( or through TDRSS) 461.3 623.35 P
0.51 (to the ground. Data obtained in) 189 611.35 P
9 F
1.22 (RAPID) 318.98 611.35 P
0 F
0.51 ( mode require special handling by the observer) 348.98 611.35 P
0.16 (to correct for some of the ef) 189 599.35 P
0.16 (fects \050especially doppler shifts\051 that are automatically com-) 301.42 599.35 P
(pensated for in) 189 587.35 T
9 F
(ACCUM) 250.93 587.35 T
0 F
( mode.) 280.93 587.35 T
-0.13 (As for an) 189 567.35 P
9 F
-0.31 (ACCUM) 228.32 567.35 P
0 F
-0.13 (, you should specify the science aperture and the spectral element. Y) 258.32 567.35 P
-0.13 (ou) 530 567.35 P
0.85 (may also choose to observe) 189 555.35 P
9 F
2.05 (WAVE) 305.75 555.35 P
0 F
0.85 ( as tar) 329.75 555.35 P
0.85 (get to get a wavelength calibration. The only) 355.16 555.35 P
0.43 (other parameter you may specify is) 189 543.35 P
9 F
1.04 (SAMPLE-TIME) 334.89 543.35 P
0 F
0.43 (, which is the length of each sepa-) 400.89 543.35 P
0.66 (rate exposure that is read to the ground. The default) 189 531.35 P
9 F
1.58 (SAMPLE-TIME) 404.7 531.35 P
0 F
0.66 ( is also the mini-) 470.7 531.35 P
0.07 (mum, 0.05 seconds.) 189 519.35 P
9 F
0.16 (SAMPLE-TIME) 271.42 519.35 P
0 F
0.07 ( may be incremented in 0.05 second values up to a) 337.42 519.35 P
0.28 (maximum of 12.75 seconds. Use of a very short) 189 507.35 P
9 F
0.67 (SAMPLE-TIME) 385.67 507.35 P
0 F
0.28 ( and/or use of) 451.67 507.35 P
9 F
0.67 (RAPID) 510 507.35 P
0 F
-0.15 (mode for extended periods can cause scheduling problems because of the very high data) 189 495.35 P
2.38 (volumes that are generated. In particular) 189 483.35 P
2.38 (, a) 362.1 483.35 P
9 F
5.7 (SAMPLE-TIME) 378.8 483.35 P
0 F
2.38 ( of less than 0.33 sec) 444.8 483.35 P
1 (records data at the 1 Mb rate and so can proceed for no more than about 20 minutes) 189 471.35 P
-0.21 (before \336lling the onboard tape recorder) 189 459.35 P
-0.21 (. A) 344.3 459.35 P
9 F
-0.5 (SAMPLE-TIME) 358.61 459.35 P
0 F
-0.21 ( of 0.33 seconds or more, but) 424.61 459.35 P
0.49 (less than 2.57 seconds, results in a 32k data rate, while a) 189 447.35 P
9 F
1.16 (SAMPLE-TIME) 422.84 447.35 P
0 F
0.49 ( in excess of) 488.84 447.35 P
-0 (2.57 seconds results in a 4k data rate. This latter low rate can be sustained almost indef-) 189 435.35 P
(initely) 189 423.35 T
(.) 213.91 423.35 T
54 380.02 540 383.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 381.52 540 381.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 381.52 180 381.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(4.5) 163.32 387.02 T
(The Precision and Accuracy of Standard Calibrations) 189 387.02 T
0 10 Q
1.14 (Our job of calibrating the GHRS on a routine basis ensures that you can rely on the) 189 363.35 P
-0.02 (wavelength scale and \337ux calibration that you are provided. The quality of the \337ux cali-) 189 351.35 P
0.37 (bration is limited primarily by innate factors that are present in tying together dif) 189 339.35 P
0.37 (ferent) 516.68 339.35 P
0.02 (photometric systems. The GHRS has proved to be a reliable instrument whose response) 189 327.35 P
1.02 (has not been seen to vary with time. Routine calibrations will deliver absolute \337uxes) 189 315.35 P
0.37 (accurate to 10% and photometrically precise to better than 1% with the LSA) 189 303.35 P
0 8 Q
0.29 (1) 498.89 307.35 P
0 10 Q
0.37 (. In other) 502.89 303.35 P
0.12 (words, we monitor the sensitivity of the GHRS on a regular basis \050approximately every) 189 291.35 P
1.05 (four months\051 and have not seen changes in the count rates for the standard stars that) 189 279.35 P
0.64 (exceed 1%, once the ef) 189 267.35 P
0.64 (fects of telescope focus are taken into account. However) 283.86 267.35 P
0.64 (, there) 514.37 267.35 P
-0.12 (are undoubtedly systematic ef) 189 255.35 P
-0.12 (fects present that preclude knowing absolute \337uxes to bet-) 308.18 255.35 P
0.81 (ter than 5 to 10%. The solid performance of the GHRS means that it is impossible to) 189 243.35 P
1.18 (improve substantially on the \337ux-calibration by obtaining observations on your own.) 189 231.35 P
0.18 (The GHRS dark count is so low for most objects as to be irrelevant \050but see the discus-) 189 219.35 P
0.33 (sion on) 189 207.35 P
9 F
0.78 (CENSOR) 221.32 207.35 P
0 F
0.33 ( in Section) 257.32 207.35 P
0.33 (8.6.2 on page) 303.26 207.35 P
0.33 (95\051 and high signal-to-noise can be obtained) 360.29 207.35 P
(without the need for \337at-\336eld exposures.) 189 195.35 T
0.21 (The one area in which you might wish to consider a special calibration is for the wave-) 189 175.35 P
0.22 (length scale. However) 189 163.35 P
0.22 (, even here the default wavelength scale provided by the pipeline) 278.17 163.35 P
54 120.98 540 150.98 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 128.98 333 128.98 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
-0.02 (1. Starting in Cycle 4, the \337uxes from the data reduction pipeline in the ultraviolet can dif) 189 114.98 P
-0.02 (fer sys-) 513.28 114.98 P
(tematically from earlier values by up to 1% because of the use of models of the white dwarf) 189 104.98 T
(G191B2B as the fundamental standard.) 189 94.98 T
FMENDPAGE
%%EndPage: "46" 46
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (47) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Y) 207 736.18 T
(our Phase II Proposal) 212.34 736.18 T
0 10 Q
0.41 (data reduction system has been improved to take account of several systematic ef) 207 679.35 P
0.41 (fects.) 536.62 679.35 P
0.69 (As a result those wavelengths are good to better than 1 km s) 207 667.35 P
0 8 Q
0.55 (-1) 455.82 671.35 P
0 10 Q
0.69 ( for the \336rst-order grat-) 462.48 667.35 P
0.41 (ings, except at the shortest wavelengths \050L) 207 655.35 P
0.41 (y-) 379.14 655.35 P
13 F
0.41 (a) 387.47 655.35 P
0 F
0.41 (\051. For Echelle-B, the rms scatter in \336tted) 393.78 655.35 P
0.1 (wavelengths is about 0.6 km s) 207 643.35 P
0 8 Q
0.08 (-1) 328.07 647.35 P
0 10 Q
0.1 (. These values are uncertainties for the wavelength zero) 334.73 643.35 P
(point of a spectrum; the dispersion of spectra dif) 207 631.35 T
(fer negligibly from the routine values.) 400.68 631.35 T
1.48 (Our) 207 611.35 P
3 F
1.48 (speci\336cations) 226.53 611.35 P
0 F
1.48 ( for routine wavelength calibration are to have them good to only) 280.97 611.35 P
(about one diode rms, estimated as follows:) 207 599.35 T
10 11 Q
(\245) 207 581.35 T
0 10 Q
(First, errors in carrousel positioning can amount to 0.2 diode.) 221.4 581.35 T
10 11 Q
(\245) 207 566.35 T
0 10 Q
-0.12 (Second, if a wavelength calibration is not available for the precise carrousel position) 221.4 566.35 P
0.06 (you select then it is necessary to interpolate in the dispersion constants, and that can) 221.4 554.35 P
(lead to an error of 0.5 diode.) 221.4 542.35 T
10 11 Q
(\245) 207 527.35 T
0 10 Q
0.31 (Third, changing temperatures within the spectrograph can lead to wavelength shifts) 221.4 527.35 P
(of about 0.5 diode over the course of an orbit.) 221.4 515.35 T
10 11 Q
(\245) 207 500.35 T
0 10 Q
0.91 (Finally) 221.4 500.35 P
0.91 (, geomagnetically-induced image motion can lead to oscillations of up to 1) 249.09 500.35 P
(diode peak-to-peak amplitude over half an orbit.) 221.4 488.35 T
10 11 Q
(\245) 207 473.35 T
0 10 Q
(The net result is that about 1 1/4 diode accuracy is what is routinely expected.) 221.4 473.35 T
-0.01 (Precision of about 0.2 diode can be achieved by requesting that an) 207 453.35 P
9 F
-0.03 (ACCUM) 474.31 453.35 P
0 F
-0.01 ( with a) 504.31 453.35 P
9 F
-0.03 (TAR-) 534 453.35 P
-0.1 (GET) 207 441.35 P
0 F
-0.04 ( of) 225 441.35 P
9 F
-0.1 (WAVE) 238.24 441.35 P
0 F
-0.04 ( be made immediately) 262.24 441.35 P
3 F
-0.04 (befor) 353.18 441.35 P
-0.04 (e) 373.92 441.35 P
0 F
-0.04 ( your science exposure. Nearly the same pre-) 378.36 441.35 P
3.34 (cision can be realized by using information in the) 207 429.35 P
9 F
8.01 (SPYBAL) 437.29 429.35 P
0 F
3.34 ( exposures that are) 473.29 429.35 P
0.27 (automatically taken at the start of a sequence of observations with a new grating. Also,) 207 417.35 P
1.4 (you should specify) 207 405.35 P
9 F
3.35 (NO) 289.24 405.35 P
3.35 (GAP) 305.13 405.35 P
0 F
1.4 ( for the exposure lines to which the) 323.13 405.35 P
9 F
3.35 (WAVE) 477.61 405.35 P
0 F
1.4 ( pertains. See) 501.61 405.35 P
-0.04 (Chapter 5 for an example. Bear in mind that the several separate exposures you list may) 207 393.35 P
0.22 (not necessarily be obtained one right after the other \050unless you so specify in Phase II\051,) 207 381.35 P
(so that separate) 207 369.35 T
9 F
(WAVE) 271.15 369.35 T
0 F
( calibrations may be needed.) 295.15 369.35 T
0.2 (W) 207 349.35 P
0.2 (e also recommend breaking long exposures into subexposures that are no longer than) 215.64 349.35 P
2.32 (about 5 minutes each. This is done to ensure that geomagnetically-induced image) 207 337.35 P
0.64 (motion will not degrade the quality of your data. Any shifts in the dif) 207 325.35 P
0.64 (ferent spectra of) 491.76 325.35 P
-0 (the same object can generally be determined by cross-correlating them during your data) 207 313.35 P
(analysis.) 207 301.35 T
72 258.02 558 261.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 259.52 558 259.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 259.52 198 259.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(4.6) 181.32 265.02 T
(Other Considerations) 207 265.02 T
0 10 Q
0.59 (There are many factors that may in\337uence how you specify the manner in which your) 207 241.35 P
1.22 (observations should be obtained. Here we mention two that have arisen in particular) 207 229.35 P
0.99 (instances. The \336rst has to do with T) 207 217.35 P
0.99 (ar) 355.97 217.35 P
0.99 (gets of Opportunity \050T) 363.56 217.35 P
0.99 (OOs\051 and/or coordinated) 456.61 217.35 P
-0.03 (observations. The) 207 205.35 P
3 F
-0.03 (Call for Pr) 280.55 205.35 P
-0.03 (oposals) 324.03 205.35 P
0 F
-0.03 (should be consulted for information about propos-) 357.06 205.35 P
1.54 (ing to observe T) 207 193.35 P
1.54 (ar) 276.19 193.35 P
1.54 (gets of Opportunity with) 283.78 193.35 P
3 F
1.54 (HST) 391.05 193.35 P
0 F
1.54 ( and GHRS. Observations of T) 408.83 193.35 P
1.54 (OOs) 539.67 193.35 P
1.11 (often need to be coordinated with other satellites or ground-based observatories. The) 207 181.35 P
0.8 (long lead times for planning) 207 169.35 P
3 F
0.8 (HST) 326.27 169.35 P
0 F
0.8 ( observations, even for T) 344.05 169.35 P
0.8 (OOs, are an impediment to) 446.76 169.35 P
2.06 (that coordination. W) 207 157.35 P
2.06 (e encourage you to explain in detail exactly what is or is not) 292.8 157.35 P
(required for the successful completion of your program.) 207 145.35 T
-0.01 (Another problem that can occur arises when a science program speci\336es a lar) 207 125.35 P
-0.01 (ge number) 515.52 125.35 P
0.42 (of separate GHRS exposures. The problem is caused by the relatively small amount of) 207 113.35 P
0.33 (memory available on) 207 101.35 P
3 F
0.33 (HST) 294.92 101.35 P
0 F
0.33 ( in which to store GHRS commands. It is usually possible to) 312.7 101.35 P
FMENDPAGE
%%EndPage: "47" 47
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Y) 189 736.18 T
(our Phase II Proposal) 194.34 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(48) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
0.77 (break up such a program so that the separate exposures are not all together) 189 679.35 P
0.77 (, but occa-) 496.54 679.35 P
0.12 (sionally the science goals cannot allow that and some other compromise must be made.) 189 667.35 P
0.41 (Roughly speaking, about 40 total spectra can be scheduled in a single block \050a) 189 655.35 P
9 F
0.99 (WSCAN) 510 655.35 P
0 F
0.21 (with) 189 643.35 P
3 F
0.21 (n) 209.49 643.35 P
0 F
0.21 ( set-points counts as) 214.49 643.35 P
3 F
0.21 (n) 298.65 643.35 P
0 F
0.21 ( exposures and an) 303.65 643.35 P
9 F
0.5 (FP-SPLIT) 378.35 643.35 P
0 F
0.21 ( counts as 2 or 4\051. Once that) 426.35 643.35 P
0.96 (number is exceeded the remaining observations must be scheduled in a new block of) 189 631.35 P
-0.23 (time, and that means a new tar) 189 619.35 P
-0.23 (get acquisition will be needed, with the concomitant over-) 309.36 619.35 P
(head time.) 189 607.35 T
FMENDPAGE
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[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (49) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
7 12 Q
1.2 (Chapter 5) 72 677 S
5 24 Q
-0.48 (Phase II Pr) 207 677 S
-0.48 (oposal) 309.27 677 S
-0.48 (Examples) 207 647 S
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
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[ 1 0 1 0 0 1 0]
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[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Phase II Proposal Examples) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(50) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
1.32 (W) 189 679.35 P
1.32 (e present in this chapter several examples of how to actually execute proposals to) 197.64 679.35 P
0.76 (achieve what you want, since abstract instructions are, at best, dif) 189 667.35 P
0.76 (\336cult to follow) 458.36 667.35 P
0.76 (. The) 518.68 667.35 P
0.24 (examples are shown separately) 189 655.35 P
0.24 (, partly for formatting reasons, since they require a side-) 313.19 655.35 P
0.7 (ways orientation of the page, and partly to assemble them in one place for easy refer-) 189 643.35 P
(ence.) 189 631.35 T
0.01 (W) 189 607.35 P
0.01 (e begin by showing how the \336rst entry on the next page would look as input to RPSS.) 197.64 607.35 P
-0.09 (The remainder of this chapter shows how Phase II proposals look to us. In most of these) 189 595.35 P
1.34 (examples, the various parameters have been explicitly listed for clarity) 189 583.35 P
1.34 (, even though) 483.15 583.35 P
(they often correspond to the defaults that would apply anyway) 189 571.35 T
(.) 438.03 571.35 T
-0.21 (W) 189 547.35 P
-0.21 (e remind you that any if dif) 197.64 547.35 P
-0.21 (ferences exist between this document and, say) 305.64 547.35 P
-0.21 (, the Phase II) 488.42 547.35 P
0.41 (Proposal Instructions, the one with the most recent date of issue should be followed or) 189 535.35 P
(you should consult us to resolve the discrepancy) 189 523.35 T
(.) 381.94 523.35 T
9 8 Q
(exposure_logsheet:) 203.42 482.68 T
(linenum:) 203.42 459.68 T
(1.0) 294.02 459.68 T
(targname:) 203.42 448.68 T
(MU-COL) 294.02 448.68 T
(conf) 203.42 437.68 T
(ig:) 222.62 437.68 T
(HRS) 294.02 437.68 T
(opmode:) 203.42 426.68 T
(ACQ) 294.02 426.68 T
(aperture) 203.42 415.68 T
(2.0) 294.02 415.68 T
(sp_element:) 203.42 404.68 T
(MIRROR-A2) 294.02 404.68 T
(num_exp:) 203.42 393.68 T
(1) 294.02 393.68 T
(time_per_exp:) 203.42 382.68 T
(10.75M) 294.02 382.68 T
(f) 203.42 371.68 T
(luxnum_1:) 208.22 371.68 T
(1) 294.02 371.68 T
(priority:) 203.42 360.68 T
(1) 294.02 360.68 T
(param_1:) 203.42 349.68 T
(SEARCH-SIZE=5,) 294.02 349.68 T
(param_2:) 203.42 338.68 T
(MAP=ALL-POINTS) 294.02 338.68 T
(req_1:) 203.42 327.68 T
(CYCLE 5/ 1-2;) 294.02 327.68 T
(req_2:) 203.42 316.68 T
(EARLY ACQ FOR 2.0) 294.02 316.68 T
(comment_1:) 203.42 305.68 T
(STEP-TIME=0.2S;) 294.02 305.68 T
(comment_2:) 203.42 294.68 T
(EXPECT 21000 COUNTS IN STEP-TIME) 294.02 294.68 T
(!) 203.42 283.68 T
(linenum:) 203.42 272.68 T
(2.0) 294.02 272.68 T
(targname:) 203.42 261.68 T
(MU-COL) 294.02 261.68 T
(conf) 203.42 250.68 T
(ig:) 222.62 250.68 T
(HRS) 294.02 250.68 T
(opmode:) 203.42 239.68 T
(ACCUM) 294.02 239.68 T
(aperture:) 203.42 228.68 T
(2.0) 294.02 228.68 T
(sp_element:) 203.42 217.68 T
(ECH-B) 294.02 217.68 T
(num_exp:) 203.42 206.68 T
(1) 294.02 206.68 T
(time_per_exp:) 203.42 195.68 T
(4.8S) 294.02 195.68 T
(f) 203.42 184.68 T
(luxnum_1:) 208.22 184.68 T
(1) 294.02 184.68 T
(priority:) 203.42 173.68 T
(1) 294.02 173.68 T
(param_1:) 203.42 162.68 T
(STEP-PATT=13) 294.02 162.68 T
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Phase II Proposal Examples) 207 736.18 T
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (51) 546.88 60.29 P
72 90 558 711 R
7 X
V
0 X
-0.13 (1. Example of an observation that speci\336es an early acquisition. Note that the TIME in column \0501) 0 -270 102.67 90 PF
-0.13 (1\051 is 0.2 sec \050the STEP-TIME\051 times) 0 -270 102.67 546.19 PF
0.62 (\050128 x 25\051 + 25, in accord with the formula in Section 4.1.13 . Note also that the expected number of counts for the acquisition is) 0 -270 114.67 90 PF
(mentioned.) 0 -270 126.67 90 TF
9 8 Q
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 167.33 90 TF
-0.13 ( 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15) 0 -270 177.33 90 PF
-0.26 ( LN | SEQ | TARGET |INSTR | OPER. | APER |SPECTRAL|CENTRAL| OPTIONAL |NUM| TIME | S/N |FLX|PR| SPECIAL) 0 -270 187.33 90 PF
-0.24 ( NM | NAME | NAME |CONFIG| MODE |OR FOV |ELEMENT |WAVELN | PARAMETERS |EXP| | |REF| | REQUIREMENTS) 0 -270 197.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 207.33 90 TF
-0.17 (1.0 MU-COL HRS ACQ 2.0 MIRROR- SEARCH-SIZE=5, 1 10.75M 1 1 CYCLE 5/ 1-2;) 0 -270 217.33 90 PF
-0.12 ( A2 MAP=ALL-POINTS EARLY ACQ FOR 2.0) 0 -270 227.33 90 PF
-0.16 ( COMMENTS: STEP-TIME=0.2S; EXPECT 21000 COUNTS IN STEP-TIME) 0 -270 237.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 247.33 90 TF
-0.15 (2.0 MU-COL HRS ACCUM 2.0 ECH-B 1600 STEP-PATT=13 1 4.8S 1 1) 0 -270 257.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 287.33 90 TF
2 10 Q
(2. The same observation as above speci\336ed as an interactive acquisition.) 0 -270 322.67 90 TF
9 8 Q
(--------------------------------------------------------------------------------------------------------------------------------) 0 -270 349.33 90 TF
-0.13 ( 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15) 0 -270 359.33 90 PF
-0.26 ( LN | SEQ | TARGET |INSTR | OPER. | APER |SPECTRAL|CENTRAL| OPTIONAL |NUM| TIME | S/N |FLX|PR| SPECIAL) 0 -270 369.33 90 PF
-0.24 ( NM | NAME | NAME |CONFIG| MODE |OR FOV |ELEMENT |WAVELN | PARAMETERS |EXP| | |REF| | REQUIREMENTS) 0 -270 379.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 389.33 90 TF
(10.0 MU-COL HRS ACQ 2.0 MIRROR- SEARCH-SIZE=5, 1 10.75M 1 1 CYCLE 5/ 10-20;) 0 -270 399.33 90 TF
(00 A2 MAP=ALL-POINT INT ACQ FOR 20;) 0 -270 409.33 90 TF
( S) 0 -270 419.33 90 TF
( COMMENTS: STEP-TIME=0.2S; EXPECT 21000 COUNTS IN STEP-TIME) 0 -270 429.33 90 TF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 439.33 90 TF
-0.15 (20.0 MU-COL HRS ACCUM 2.0 ECH-B 1600 STEP-PATT=13 1 4.8S 1 1) 0 -270 449.33 90 PF
-0.1 (00) 0 -270 459.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 479.33 90 TF
72 90 558 711 R
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
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[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
54 726.98 540 726.98 2 L
0.25 H
N
2 9 Q
(Phase II Proposal Examples) 189 736.18 T
2 10 Q
(52) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 74.02 540 74.02 2 L
2 Z
N
54 90 540 711 R
7 X
V
0 X
(3. A GHRS acquisition speci\336ed with explicit BRIGHT and F) 0 -270 60.67 90 TF
(AINT limits.) 0 -270 60.67 371.74 TF
9 8 Q
(--------------------------------------------------------------------------------------------------------------------------------) 0 -270 87.33 90 TF
-0.13 ( 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15) 0 -270 97.33 90 PF
-0.26 ( LN | SEQ | TARGET |INSTR | OPER. | APER |SPECTRAL|CENTRAL| OPTIONAL |NUM| TIME | S/N |FLX|PR| SPECIAL) 0 -270 107.33 90 PF
-0.24 ( NM | NAME | NAME |CONFIG| MODE |OR FOV |ELEMENT |WAVELN | PARAMETERS |EXP| | |REF| | REQUIREMENTS) 0 -270 117.33 90 PF
(--------------------------------------------------------------------------------------------------------------------------------) 0 -270 127.33 90 TF
-0.18 (100. BD28D4211 HRS ACQ 2.0 MIRROR- BRIGHT=65535, 1 9S 1 1 ONBOARD ACQ FOR 2) 0 -270 137.33 90 PF
-0.11 (000 A2 FAINT=700 00;) 0 -270 147.33 90 PF
-0.29 ( COMMENTS: STEP_TIME=1.0S; EXPECT 1800 COUNTS IN STEP-TIME; FAINT SET TO APPROX. 40% OF EXPECTED COUNTS.) 0 -270 167.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 177.33 90 TF
2 10 Q
(4. Example of an acquisition with an offset.) 0 -270 210.67 90 TF
9 8 Q
(--------------------------------------------------------------------------------------------------------------------------------) 0 -270 237.33 90 TF
-0.13 ( 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15) 0 -270 247.33 90 PF
-0.26 ( LN | SEQ | TARGET |INSTR | OPER. | APER |SPECTRAL|CENTRAL| OPTIONAL |NUM| TIME | S/N |FLX|PR| SPECIAL) 0 -270 257.33 90 PF
-0.24 ( NM | NAME | NAME |CONFIG| MODE |OR FOV |ELEMENT |WAVELN | PARAMETERS |EXP| | |REF| | REQUIREMENTS) 0 -270 267.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 277.33 90 TF
-0.18 (900. HII-POS1 HRS ACQ 2.0 MIRROR- BRIGHT=RETURN 1 1.8S 1 1 ONBOARD ACQ FOR 9) 0 -270 287.33 90 PF
-0.1 (000 N2 10) 0 -270 297.33 90 PF
-0.12 ( COMMENTS: STEP-TIME=0.2S) 0 -270 307.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 317.33 90 TF
-0.14 (910. HII-POS2 HRS ACCUM 2.0 G160M 1500 1 272S 50 1 1) 0 -270 327.33 90 PF
-0.1 (000) 0 -270 337.33 90 PF
-0.19 ( COMMENTS: RA-OFF = +0.227S +/- 0.001S, DEC-OFF = +6.0\323 +/- 0.01\323, FROM HII-POS1) 0 -270 347.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 357.33 90 TF
54 90 540 711 R
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Phase II Proposal Examples) 207 736.18 T
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (53) 546.88 60.29 P
72 90 558 711 R
7 X
V
0 X
0 (5. A fairly typical GHRS observation, starting with an acquisition using BRIGHT=RETURN and proceeding to several spectroscopic) 0 -270 78.67 90 PF
0.25 (exposures that use alternative variants of ACCUM speci\336cations. Not all of these would be used in one program. Note the IMAGE) 0 -270 90.67 90 PF
(\050line 300\051 that is obtained to later con\336rm centering of the target in the LSA.) 0 -270 102.67 90 TF
9 8 Q
(--------------------------------------------------------------------------------------------------------------------------------) 0 -270 129.33 90 TF
-0.13 ( 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15) 0 -270 139.33 90 PF
-0.26 ( LN | SEQ | TARGET |INSTR | OPER. | APER |SPECTRAL|CENTRAL| OPTIONAL |NUM| TIME | S/N |FLX|PR| SPECIAL) 0 -270 149.33 90 PF
-0.24 ( NM | NAME | NAME |CONFIG| MODE |OR FOV |ELEMENT |WAVELN | PARAMETERS |EXP| | |REF| | REQUIREMENTS) 0 -270 159.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 169.33 90 TF
-0.18 (100. BD28D4211 HRS ACQ 2.0 MIRROR- BRIGHT=RETURN, 1 9S 1 1 ONBOARD ACQ FOR 2) 0 -270 179.33 90 PF
-0.1 (000 A2 00;) 0 -270 189.33 90 PF
-0.16 ( COMMENTS: STEP_TIME=1.0S; EXPECT 1800 COUNTS IN STEP-TIME.) 0 -270 199.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 209.33 90 TF
-0.16 (200. BD28D4211 HRS ACQ/PE 2.0 MIRROR- 1 102S 1 1 ONBOARD ACQ FOR 3) 0 -270 219.33 90 PF
-0.11 (000 AKUP A2 00-800;) 0 -270 229.33 90 PF
-0.12 ( COMMENTS: STEP_TIME=1.0S) 0 -270 239.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 249.33 90 TF
-0.16 (300. BD28D4211 HRS IMAGE 2.0 MIRROR- NX=16, NY=16 1 256.0S 1 1) 0 -270 259.33 90 PF
-0.1 (000 A2) 0 -270 269.33 90 PF
( COMMENTS: STEP-TIME=1.0S) 0 -270 279.33 90 TF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 289.33 90 TF
(400. BD28D4211 HRS ACCUM 2.0 G160M 1500 STEP-PATT=5, S 1 217.6S 50 1 1) 0 -270 299.33 90 TF
-0.11 (000 TEP-TIME=0.2,) 0 -270 309.33 90 PF
-0.11 ( FP-SPLIT=NO, C) 0 -270 319.33 90 PF
-0.18 ( OOMB=FOUR) 0 -270 329.33 90 PF
-0.45 ( COMMENTS: EXPOSURE TIME IS A INTEGRAL NUMBER OF MINIMUM EXPOSURE TIME \05027.2S IN THIS CASE\051; S/N IS PER DIODE; STEP-PATT WILL) 0 -270 339.33 90 PF
( RESULT IN 4 PIXELS/DIODE.) 0 -270 349.33 90 TF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 359.33 90 TF
-0.17 (450. BD28D4211 HRS ACCUM 2.0 G160M 1500 STEP-PATT=5, S 1 217.6S 50 1 1) 0 -270 369.33 90 PF
-0.11 (000 TEP-TIME=0.2,) 0 -270 379.33 90 PF
-0.11 ( FP-SPLIT=FOUR,) 0 -270 389.33 90 PF
-0.1 ( COMB=FOUR) 0 -270 399.33 90 PF
( COMMENTS: FP-SPLIT WILL PRODUCE 4 SPECTRA EACH WITH 54.4S EXPOSURE TIME.) 0 -270 409.33 90 TF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 419.33 90 TF
-0.14 (475. BD28D4211 HRS ACCUM 2.0 G160M 1500 10 217.6S 50 1 1) 0 -270 429.33 90 PF
-0.1 (000) 0 -270 439.33 90 PF
-0.28 ( COMMENTS: TOTAL EXPOSURE = 2176S--BREAK UP LONG EXPOSURE TO AVOID DRIFT DUE TO GIMP.) 0 -270 459.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 469.33 90 TF
72 90 558 711 R
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
54 726.98 540 726.98 2 L
0.25 H
N
2 9 Q
(Phase II Proposal Examples) 189 736.18 T
2 10 Q
(54) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 74.02 540 74.02 2 L
2 Z
N
54 90 540 711 R
7 X
V
0 X
(6. A sequence of exposures that could be added to Example 5 if additional SSA observations were desired. The ACCUM, RAPID,) 0 -270 60.67 90 TF
(and WSCAN lines illustrate a range of options. Note the ACQ/PEAKUP with the SSA \050line 550\051 to move the star to that aperture.) 0 -270 72.67 90 TF
(If line 550 were absent the star would still be moved to the SSA, but it would not be as well centered.) 0 -270 84.67 90 TF
9 8 Q
(--------------------------------------------------------------------------------------------------------------------------------) 0 -270 111.33 90 TF
-0.13 ( 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15) 0 -270 121.33 90 PF
-0.26 ( LN | SEQ | TARGET |INSTR | OPER. | APER |SPECTRAL|CENTRAL| OPTIONAL |NUM| TIME | S/N |FLX|PR| SPECIAL) 0 -270 131.33 90 PF
-0.24 ( NM | NAME | NAME |CONFIG| MODE |OR FOV |ELEMENT |WAVELN | PARAMETERS |EXP| | |REF| | REQUIREMENTS) 0 -270 141.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 151.33 90 TF
(550. BD28D4211 HRS ACQ/PE 0.25 MIRROR- SEARCH-SIZE=5 1 25S 1 1 ONBOARD ACQ FOR) 0 -270 161.33 90 TF
( AKUP A2 600.00;) 0 -270 171.33 90 TF
-0.12 ( COMMENTS: STEP_TIME=1.0S) 0 -270 181.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 191.33 90 TF
-0.15 (575. WAVE HRS ACCUM SC2 G160M 1500 1 60S 1 1 CALIB FOR 525;) 0 -270 201.33 90 PF
-0.11 (000 SEQ 500-600 NO GAP) 0 -270 211.33 90 PF
-0.14 ( COMMENTS: STANDARD SPECTRAL CAL LAMP SPECTRUM.) 0 -270 221.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 231.33 90 TF
-0.17 (600. BD28D4211 HRS ACCUM 0.25 G160M 1500 STEP-PATT=5, S 1 326.4S 50 1 1) 0 -270 241.33 90 PF
-0.11 (000 TEP-TIME=0.2,) 0 -270 251.33 90 PF
-0.11 ( FP-SPLIT=NO, C) 0 -270 261.33 90 PF
-0.1 ( OMB=FOUR) 0 -270 271.33 90 PF
-0.15 ( COMMENTS: THROUGHPUT OF SSA APPROX. 0.67 OF LSA AT 1500A.) 0 -270 281.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 291.33 90 TF
-0.17 (700. BD28D4211 HRS RAPID 0.25 G160M 1500 SAMPLE-TIME=1. 1 20M 25 1 1) 0 -270 301.33 90 PF
-0.1 (000 0) 0 -270 311.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 321.33 90 TF
-0.18 (800. BD28D4211 HRS WSCAN 0.25 G160M 1400-1 WAVE-STEP=30.0 1 217.6S 50 1 1) 0 -270 331.33 90 PF
-0.1 (000 610) 0 -270 341.33 90 PF
-0.57 ( COMMENTS: WSCAN TO PRODUCE 7 SPECTRA W/ CENTRAL WAVELENGTHS: W1=1415.0,W2=1445,W3=1475,W4=1505, W5=1535,W6=1565,W7=1595.) 0 -270 351.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 361.33 90 TF
54 90 540 711 R
FMENDPAGE
%%EndPage: "54" 54
%%Page: "55" 55
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (55) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
7 12 Q
1.2 (Chapter 6) 72 677 S
5 24 Q
-0.48 (Design and Construction) 207 677 S
-0.48 (of the GHRS) 207 647 S
4 12 Q
(6.1) 144 424 T
( The HST Focal Plane and the GHRS Apertures) 164.02 424 T
8 F
( 56) 505.32 424 T
4 F
(6.2) 144 406 T
( Gratings and Optical Elements) 164.02 406 T
8 F
( 60) 505.32 406 T
4 F
(6.3) 144 388 T
( The Digicon Detectors) 164.02 388 T
8 F
( 62) 505.32 388 T
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Design and Construction of the GHRS) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(56) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 671.02 540 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 672.52 540 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 672.52 180 672.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(6.1) 163.32 678.02 T
(The HST Focal Plane and the GHRS Apertures) 189 678.02 T
0 10 Q
-0.06 (W) 189 654.35 P
-0.06 (e provide here a description of the instrument in lar) 197.64 654.35 P
-0.06 (gely pictorial terms. More illustra-) 402.19 654.35 P
0.67 (tions and full technical descriptions of the GHRS may be found in the references \050see) 189 642.35 P
(Section) 189 630.35 T
(9.2 on page) 221.5 630.35 T
(102\051.) 270.38 630.35 T
54 87.98 540 686.02 C
54 132.98 540 492.98 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 87.98 540 686.02 C
0 0 612 792 C
54 87.98 540 686.02 C
54 87.98 540 132.98 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
0 X
0 0 0 1 0 0 0 K
(Figure 6-1) 207 109.15 T
4 F
(. The Hubble Space T) 254.79 109.15 T
(elescope and its components, with the) 350.95 109.15 T
(locations of important operational elements shown.) 207 99.15 T
54 87.98 540 686.02 C
0 0 612 792 C
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (57) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Design and Construction of the GHRS) 207 736.18 T
72 87.98 558 686.02 C
72 118.15 558 478.15 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 87.98 558 686.02 C
0 0 612 792 C
72 87.98 558 686.02 C
72 87.98 558 118.15 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
0 X
0 0 0 1 0 0 0 K
(Figure 6-2.) 207 109.15 T
4 F
(The focal plane of HST and the de\336nitions of the V2, V3 and U2,) 260.35 109.15 T
(U3 coordinate systems of the spacecraft.) 207 99.15 T
72 87.98 558 686.02 C
0 0 612 792 C
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Design and Construction of the GHRS) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(58) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 87.98 540 686.02 C
54 168.12 540 480.46 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 87.98 540 686.02 C
0 0 612 792 C
54 87.98 540 686.02 C
54 87.98 540 168.12 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
0 X
0 0 0 1 0 0 0 K
(Figure 6-3.) 189 159.12 T
4 F
( Locations of GHRS apertures relative to spacecraft axes. Note) 239.57 159.12 T
(that the sense of the) 189 149.12 T
8 F
(x) 282.4 149.12 T
4 F
( and) 287.4 149.12 T
8 F
(y) 309.64 149.12 T
4 F
( motions are shown by the arrows, but that the) 314.64 149.12 T
(zero point for each aperture \050SSA and LSA\051 is located at its center) 189 139.12 T
(. COST) 481.37 139.12 T
(AR) 513.97 139.12 T
(does not, of course, change the layout of the entrance apertures, but it does) 189 129.12 T
(alter the way that the sky is imaged onto the focal plane. The sense is easy) 189 119.12 T
(to remember: the COST) 189 109.12 T
(AR mirrors invert the sense of the original image,) 294.96 109.12 T
(which means that the signs of motions in both coordinates, V2 and V3, \050or U2) 189 99.12 T
(and U3\051 are reversed.) 189 89.12 T
54 87.98 540 686.02 C
0 0 612 792 C
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
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[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (59) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Design and Construction of the GHRS) 207 736.18 T
72 90 558 688.03 C
72 116.14 558 428.47 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 90 558 688.03 C
0 0 612 792 C
72 90 558 688.03 C
72 90 558 116.14 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
0 X
0 0 0 1 0 0 0 K
(Figure 6-4.) 207 107.14 T
4 F
( Optical schematic of the GHRS.) 257.57 107.14 T
72 90 558 688.03 C
0 0 612 792 C
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Design and Construction of the GHRS) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(60) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 671.02 540 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 672.52 540 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 672.52 180 672.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(6.2) 163.32 678.02 T
(Gratings and Optical Elements) 189 678.02 T
0 10 Q
1.54 (Note that the \322CD\323 gratings are cross-dispersers for the echelles. CD-A has a focal) 189 433.35 P
0.68 (length of 1460 mm and CD-B has a focal length of 1340 mm. Note also that the \322M\323) 189 421.35 P
-0.11 (gratings are holographic and that the blaze angle quoted formally is that which correctly) 189 409.35 P
1.09 (predicts the center of the wavelength region the grating is optimized for) 189 397.35 P
1.09 (. G140L is a) 487.3 397.35 P
0.41 (ruled grating. \322Ech-A\323 and \322Ech-B\323 refer to two modes of operation that use the same) 189 385.35 P
(echelle grating but dif) 189 373.35 T
(ferent cross-dispersers and detectors.) 276.86 373.35 T
197.42 112.02 486.58 119.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
-0.35 (a. Mirror N2 is actually \322D\323 shaped, being a circle with a small slice of) 197.42 106.02 P
-0.35 (f one) 448.79 106.02 P
(side. It is about 60) 204.62 96.02 T
13 F
(\264) 273.12 96.02 T
0 F
( 80 mm.) 278.06 96.02 T
54 632.02 540 645.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 639.02 540 639.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 639.02 180 639.02 2 L
0 Z
N
0 0 612 792 C
2 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 626.02 T
(ABLE 6-1) 58.83 626.02 T
4 F
(Properties of GHRS Gratings) 189 626.02 T
2 8 Q
(Name) 117.6 593.68 T
(Grooves) 176.37 602.68 T
(per mm) 178.15 593.68 T
(Blaze) 236.15 602.68 T
(Angle) 235.49 593.68 T
(Order of) 284.82 602.68 T
(use) 293.71 593.68 T
(Angle of) 338.6 602.68 T
(Incidence) 336.15 593.68 T
-0.92 (Diffraction) 388.9 602.68 P
(Angle) 397.79 593.68 T
(Deviation) 444.9 602.68 T
(Angle) 451.79 593.68 T
(Detector) 500.38 593.68 T
0 9 Q
(G140L) 117.6 579.02 T
(600) 185.85 579.02 T
(2.6) 240.98 579.02 T
(1) 298.35 579.02 T
(9.0 \320 10.3) 336.6 579.02 T
(-5.3 \320 -4.0) 390.15 579.02 T
(14.25) 452.77 579.02 T
(D1) 511.1 579.02 T
(G140M) 117.6 564.02 T
(6000) 183.6 564.02 T
(23) 242.1 564.02 T
(1) 298.35 564.02 T
(26 \320 38) 341.1 564.02 T
(1) 395.57 564.02 T
(1 \320 24) 399.73 564.02 T
(14.25) 452.77 564.02 T
(D1) 511.1 564.02 T
(G160M) 117.6 549.02 T
(4960) 183.6 549.02 T
(19) 242.1 549.02 T
(1) 298.35 549.02 T
(21 \320 33) 341.1 549.02 T
(14 \320 27) 395.4 549.02 T
(6.25) 455.02 549.02 T
(D2) 511.1 549.02 T
(G200M) 117.6 534.02 T
(4320) 183.6 534.02 T
(26) 242.1 534.02 T
(1) 298.35 534.02 T
(23 \320 34) 341.1 534.02 T
(17 \320 28) 395.4 534.02 T
(6.25) 455.02 534.02 T
(D2) 511.1 534.02 T
(G270M) 117.6 519.02 T
(3600) 183.6 519.02 T
(28) 242.1 519.02 T
(1) 298.35 519.02 T
(27 \320 38) 341.1 519.02 T
(20 \320 32) 395.4 519.02 T
(6.25) 455.02 519.02 T
(D2) 511.1 519.02 T
(Ech-A) 117.6 504.02 T
(316) 185.85 504.02 T
(63.4) 238.73 504.02 T
(33 \320 53) 287.1 504.02 T
(68 \320 74) 341.1 504.02 T
(54 \320 61) 395.4 504.02 T
(13.25) 452.77 504.02 T
(D1) 511.1 504.02 T
(Ech-B) 117.6 489.02 T
(316) 185.85 489.02 T
(63.4) 238.73 489.02 T
(17 \320 33) 287.1 489.02 T
(63 \320 72) 341.1 489.02 T
(58 \320 66) 395.4 489.02 T
(5.75) 455.02 489.02 T
(D2) 511.1 489.02 T
(CD-A) 117.6 474.02 T
(194.6) 182.48 474.02 T
(0.75) 238.73 474.02 T
(1) 298.35 474.02 T
(D1) 511.1 474.02 T
(CD-B) 117.6 459.02 T
(85.7) 184.73 459.02 T
(0.54) 238.73 459.02 T
(1) 298.35 459.02 T
(D2) 511.1 459.02 T
54 327.02 540 340.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 334.02 540 334.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 334.02 180 334.02 2 L
0 Z
N
0 0 612 792 C
2 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 321.02 T
(ABLE 6-2) 58.83 321.02 T
4 F
(Properties of Other GHRS Optical Components) 189 321.02 T
2 8 Q
(Name) 203.42 288.68 T
(Clear Aperture) 283 297.68 T
(\050mm\051) 301.01 288.68 T
(Focal Length) 367.18 297.68 T
(\050mm\051) 382.3 288.68 T
(Detector) 443.35 288.68 T
0 9 Q
(LSA = \322) 203.42 274.02 T
9 F
(2.0) 234 274.02 T
0 F
(\323) 250.2 274.02 T
(0.559) 300.66 274.02 T
(D1, D2) 446.33 274.02 T
(SSA = \322) 203.42 259.02 T
9 F
(0.25) 233.5 259.02 T
0 F
(\323) 255.1 259.02 T
(0.067) 300.66 259.02 T
(D1, D2) 446.33 259.02 T
(Collimator) 203.42 244.02 T
(80) 306.29 244.02 T
(1850) 383.08 244.02 T
(D1, D2) 446.33 244.02 T
(Mirror N2) 203.42 229.02 T
0 7.2 Q
(a) 240.67 232.61 T
0 9 Q
(80) 306.29 229.02 T
(D2) 454.08 229.02 T
(Mirror A2) 203.42 214.02 T
(20) 306.29 214.02 T
(D2) 454.08 214.02 T
(Mirror N1) 203.42 199.02 T
(80) 306.29 199.02 T
(D1) 454.08 199.02 T
(Mirror A1) 203.42 184.02 T
(20) 306.29 184.02 T
(D1) 454.08 184.02 T
(Cam-A) 203.42 169.02 T
(84) 306.29 169.02 T
(1425) 383.08 169.02 T
(D1) 454.08 169.02 T
(Cam-B) 203.42 154.02 T
(86) 306.29 154.02 T
(1350) 383.08 154.02 T
(D2) 454.08 154.02 T
(D1) 203.42 139.02 T
(22) 297.07 139.02 T
13 F
( \264) 306.07 139.02 T
0 F
( 28) 313.26 139.02 T
(D2) 203.42 124.02 T
(22) 297.07 124.02 T
13 F
( \264) 306.07 124.02 T
0 F
( 28) 313.26 124.02 T
111.6 614.89 111.6 454.14 2 L
V
0.25 H
0 Z
N
165.6 615.14 165.6 453.89 2 L
V
0.5 H
N
219.6 615.14 219.6 453.89 2 L
V
0.25 H
N
273.6 615.14 273.6 453.89 2 L
V
N
327.6 615.14 327.6 453.89 2 L
V
N
381.6 615.14 381.6 453.89 2 L
V
N
436.2 615.14 436.2 453.89 2 L
V
N
489.6 615.14 489.6 453.89 2 L
V
N
543.6 614.89 543.6 454.14 2 L
V
N
111.47 615.02 543.72 615.02 2 L
V
N
111.47 589.02 543.72 589.02 2 L
V
0.5 H
N
111.47 574.02 543.72 574.02 2 L
V
0.25 H
N
111.47 559.02 543.72 559.02 2 L
V
N
111.47 544.02 543.72 544.02 2 L
V
N
111.47 529.02 543.72 529.02 2 L
V
N
111.47 514.02 543.72 514.02 2 L
V
N
111.47 499.02 543.72 499.02 2 L
V
N
111.47 484.02 543.72 484.02 2 L
V
N
111.47 469.02 543.72 469.02 2 L
V
N
111.47 454.02 543.72 454.02 2 L
V
N
197.42 309.89 197.42 119.14 2 L
V
N
270 310.14 270 118.89 2 L
V
0.5 H
N
351.58 310.14 351.58 118.89 2 L
V
0.25 H
N
432.58 310.14 432.58 118.89 2 L
V
N
486.58 309.89 486.58 119.14 2 L
V
N
197.3 310.02 486.7 310.02 2 L
V
N
197.3 284.02 486.7 284.02 2 L
V
0.5 H
N
197.3 269.02 486.7 269.02 2 L
V
0.25 H
N
197.3 254.02 486.7 254.02 2 L
V
N
197.3 239.02 486.7 239.02 2 L
V
N
197.3 224.02 486.7 224.02 2 L
V
N
197.3 209.02 486.7 209.02 2 L
V
N
197.3 194.02 486.7 194.02 2 L
V
N
197.3 179.02 486.7 179.02 2 L
V
N
197.3 164.02 486.7 164.02 2 L
V
N
197.3 149.02 486.7 149.02 2 L
V
N
197.3 134.02 486.7 134.02 2 L
V
N
197.3 119.02 486.7 119.02 2 L
V
N
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[0 0 0 1 0 0 0]
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[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (61) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Design and Construction of the GHRS) 207 736.18 T
72 87.98 558 686.02 C
72 118.15 558 427.75 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 87.98 558 686.02 C
0 0 612 792 C
72 87.98 558 686.02 C
72 87.98 558 118.15 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
0 X
0 0 0 1 0 0 0 K
(Figure 6-5.) 207 109.15 T
4 F
( Schematic diagram of GHRS\325 acquisition optics. The \322main) 257.57 109.15 T
(acquisition mirror\323 is N2.) 207 99.15 T
72 87.98 558 686.02 C
0 0 612 792 C
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Design and Construction of the GHRS) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(62) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
72 636.02 558 639.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 637.52 558 637.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 637.52 198 637.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(6.3) 181.32 643.02 T
(The Digicon Detectors) 207 643.02 T
72 87.98 558 686.02 C
72 102.17 558 411.77 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 87.98 558 686.02 C
0 0 612 792 C
72 87.98 558 686.02 C
72 87.98 558 102.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
0 X
0 0 0 1 0 0 0 K
(Figure 6-6.) 207 93.17 T
4 F
( Cutaway view of a Digicon.) 257.57 93.17 T
72 87.98 558 686.02 C
0 0 612 792 C
FMENDPAGE
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[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (63) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Design and Construction of the GHRS) 207 736.18 T
72 87.98 558 686.02 C
72 120.17 558 501.77 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 87.98 558 686.02 C
0 0 612 792 C
72 87.98 558 686.02 C
72 87.98 558 120.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
0 X
0 0 0 1 0 0 0 K
(Figure 6-7.) 207 102.17 T
4 F
( Cross-sectional view of a Digicon and views of its faceplate and) 257.57 102.17 T
(diode arrays.) 207 92.17 T
72 87.98 558 686.02 C
0 0 612 792 C
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Design and Construction of the GHRS) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(64) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
72 87.98 558 686.02 C
72 120.17 558 501.77 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 87.98 558 686.02 C
0 0 612 792 C
72 87.98 558 686.02 C
72 87.98 558 120.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
0 X
0 0 0 1 0 0 0 K
(Figure 6-8.) 207 102.17 T
4 F
( A view from the cross-dispersers toward the Digicon detectors to) 257.57 102.17 T
(illustrate the senses of) 207 92.17 T
8 F
(x) 309.27 92.17 T
4 F
( and) 314.27 92.17 T
8 F
(y) 336.51 92.17 T
4 F
( motions and of increasing wavelength.) 341.51 92.17 T
72 87.98 558 686.02 C
0 0 612 792 C
FMENDPAGE
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[0 0 0 1 0 0 0]
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[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (65) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Design and Construction of the GHRS) 207 736.18 T
54 87.98 540 686.02 C
54 134.14 540 515.74 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 87.98 540 686.02 C
0 0 612 792 C
54 87.98 540 686.02 C
54 87.98 540 134.14 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
0 X
0 0 0 1 0 0 0 K
(Figure 6-9.) 189 116.14 T
4 F
( A detailed layout of the diodes in the Digicon detectors. Note) 239.57 116.14 T
(the 6 large \322corner diodes\323 and the 6 \322focus diodes\323 \050numbers 4, 5, and 6, for) 189 106.14 T
(example\051.) 189 96.14 T
54 87.98 540 686.02 C
0 0 612 792 C
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[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Design and Construction of the GHRS) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(66) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
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[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (67) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
7 12 Q
1.2 (Chapter 7) 72 677 S
5 24 Q
-0.48 (T) 207 677 S
-0.48 (ar) 218.52 677 S
-0.48 (get Acquisition) 237.12 677 S
-0.48 (Refer) 207 647 S
-0.48 (ence Information) 254.86 647 S
4 12 Q
(7.1) 144 415 T
( Predicting T) 164.02 415 T
(arget Acquisition Count Rates for Stars) 230.04 415 T
8 F
( 68) 505.32 415 T
4 10 Q
(7.1.1) 162 398.33 T
( Alternate Method for Predicting T) 187.02 398.33 T
(arget Acquisition Count Rates) 335.42 398.33 T
8 F
( 69) 508.1 398.33 T
4 F
(7.1.2) 162 382.33 T
( T) 187.02 382.33 T
(wo Examples) 195.36 382.33 T
8 F
( 69) 508.1 382.33 T
4 12 Q
(7.2) 144 365 T
( Constraints on the V) 164.02 365 T
(alue of the STEP-TIME Parameter) 275.18 365 T
8 F
( 71) 505.32 365 T
4 F
(7.3) 144 347 T
( Acquisition Count Rates for Extended Objects) 164.02 347 T
8 F
( 76) 505.32 347 T
4 F
(7.4) 144 329 T
( Other Acquisition Information) 164.02 329 T
8 F
( 78) 505.32 329 T
4 10 Q
(7.4.1) 162 312.33 T
( Ef) 187.02 312.33 T
(fective Areas of the Acquisition Mirrors) 199.07 312.33 T
8 F
( 78) 508.1 312.33 T
4 F
(7.4.2) 162 296.33 T
( Geocoronal L) 187.02 296.33 T
(yman-a Background) 249.46 296.33 T
8 F
( 80) 508.1 296.33 T
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(T) 189 736.18 T
(arget Acquisition Reference Information) 193.83 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(68) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 671.02 540 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 672.52 540 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 672.52 180 672.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(7.1) 163.32 678.02 T
(Predicting T) 189 678.02 T
(arget Acquisition Count Rates for Stars) 257.46 678.02 T
0 10 Q
0.78 (W) 189 650.35 P
0.78 (e have calculated GHRS tar) 197.64 650.35 P
0.78 (get acquisition count rates for the spectra of a subset of) 311.67 650.35 P
0.1 (the 175 stars contained in the Bruzual-Persson-Gunn-Stryker \050BPGS\051 Library of Stellar) 189 638.35 P
1.56 (Spectra by using) 189 626.35 P
4 F
1.74 (calcphot) 262.85 626.35 P
0 F
1.56 (, a task in the) 300.09 626.35 P
4 F
1.74 (synphot) 363.46 626.35 P
0 F
1.56 ( package in) 398.48 626.35 P
4 F
1.74 (stsdas) 451.21 626.35 P
0 F
1.56 (. GHRS tar) 480.11 626.35 P
1.56 (get) 527.78 626.35 P
-0 (acquisition count rates for objects similar to those in the BPGS catalog can be predicted) 189 614.35 P
0.79 (by following the procedures described here. Constraints on the value of) 189 602.35 P
9 F
1.9 (STEP-TIME) 486 602.35 P
0 F
-0.05 (are discussed. Please note that the values tabulated are the total count rate for a star) 189 590.35 P
-0.05 (, and) 520.61 590.35 P
0.14 (that the count rate for a particular diode will depend on that portion of the Point Spread) 189 578.35 P
0.02 (Function that strikes it. That can in\337uence the degree, for example, to which the paired-) 189 566.35 P
0.66 (pulse correction applies. However) 189 554.35 P
0.66 (, the acquisition procedure sums the counts over the) 327.22 554.35 P
0.85 (eight science diodes upon which the LSA is imaged, so for most objects these values) 189 542.35 P
(may be used straightforwardly) 189 530.35 T
(.) 310.27 530.35 T
-0.04 (Do not for) 189 506.35 P
-0.04 (get to reduce these values by a factor of 0.3 if the focus diodes are being used) 230.4 506.35 P
-0.11 (for an) 189 494.35 P
9 F
-0.25 (IMAGE) 214.89 494.35 P
0 F
-0.11 (; this is because of the reduced area of the focus diodes compared to using) 244.89 494.35 P
0.03 (eight normal diodes for an acquisition. This factor applies to when a focus diode is cen-) 189 482.35 P
(tered on a point source.) 189 470.35 T
0.64 (The \337ux distributions in the BPGS catalog include ultraviolet wavelengths and can be) 189 446.35 P
0.82 (used for planning GHRS tar) 189 434.35 P
0.82 (get acquisitions. Each spectrum in the catalog was dered-) 304.31 434.35 P
-0.02 (dened and scaled to) 189 422.35 P
3 F
-0.02 (V) 270.02 422.35 P
0 8 Q
-0.01 (0) 276.12 419.85 P
0 10 Q
-0.02 ( = 0.0. The) 280.12 422.35 P
4 F
-0.02 (calcphot) 326.24 422.35 P
0 F
-0.02 ( task in the) 363.48 422.35 P
4 F
-0.02 (synphot) 409.52 422.35 P
0 F
-0.02 ( package of) 444.54 422.35 P
4 F
-0.02 (stsdas) 493.07 422.35 P
0 F
-0.02 ( was) 521.97 422.35 P
-0.05 (used to convolve the catalog \337ux distributions with the ef) 189 410.35 P
-0.05 (fective areas of the acquisition) 418.03 410.35 P
0.44 (mirrors. T) 189 398.35 P
0.44 (able) 229.29 398.35 P
0.44 (7-1 on page) 248.45 398.35 P
0.44 (74 contains columns giving the BPGS catalog object name,) 299.03 398.35 P
0.16 (spectral type,) 189 386.35 P
3 F
0.16 (\050B\320V\051) 245.14 386.35 P
0 8 Q
0.13 (0) 269.02 383.85 P
0 10 Q
0.16 (, count rate for the acquisition mirror with no reddening, and scale) 273.02 386.35 P
-0.19 (factors \050per unit magnitude\051 indicating the relative count rate observed at given amounts) 189 374.35 P
(of reddening compared to the count rate with no reddening.) 189 362.35 T
(T) 189 338.35 T
(o use T) 194.41 338.35 T
(able) 223.15 338.35 T
(7-1 to predict tar) 242.31 338.35 T
(get acquisition count rates:) 309.06 338.35 T
10 11 Q
(\245) 189 320.35 T
0 10 Q
0.1 (Determine the) 203.4 320.35 P
3 F
0.1 (intrinsic) 263.04 320.35 P
0 F
0.1 ( color) 296.38 320.35 P
0.1 (,) 319.13 320.35 P
3 F
0.1 (\050B \320 V\051) 324.23 320.35 P
0 8 Q
0.08 (0) 353.32 317.85 P
0 10 Q
0.1 (, and magnitude,) 357.32 320.35 P
3 F
0.1 (V) 426.79 320.35 P
0 8 Q
0.08 (0) 432.9 317.85 P
0 10 Q
0.1 (, of your object as well as) 436.9 320.35 P
(its color excess,) 203.4 308.35 T
3 F
( E\050B \320 V\051) 267 308.35 T
0 F
(.) 304.49 308.35 T
10 11 Q
(\245) 189 293.35 T
0 10 Q
0.14 (Find an entry in T) 203.4 293.35 P
0.14 (able) 275.47 293.35 P
0.14 (7-1 that has similar spectral characteristics to your object \050by) 294.63 293.35 P
0.53 (spectral type or) 203.4 281.35 P
3 F
0.53 (\050B \320 V\051) 269.13 281.35 P
0 8 Q
0.42 (0) 299.07 278.85 P
0 10 Q
0.53 ( and note that luminosity class is important for the coolest) 303.07 281.35 P
0.38 (stars\051. The table is sorted by increasing) 203.4 269.35 P
3 F
0.38 (\050B \320 V\051) 364.89 269.35 P
0 8 Q
0.3 (0) 394.52 266.85 P
0 10 Q
0.38 (. Make sure you pick from the col-) 398.52 269.35 P
(umn corresponding to the acquisition mirror that you plan to use.) 203.4 257.35 T
10 11 Q
(\245) 189 241.68 T
0 10 Q
1.15 (Scale the predicted count rate found in the previous step by the ratio of apparent) 203.4 241.68 P
(brightness of your object to an object with) 203.4 222.17 T
3 F
(V) 375.05 222.17 T
0 8 Q
(0) 381.16 219.67 T
0 10 Q
( = 0.0, i.e., multiply by) 385.16 222.17 T
(.) 512.9 222.17 T
10 11 Q
(\245) 189 205.33 T
0 10 Q
-0.01 (T) 203.4 205.33 P
-0.01 (o obtain the scale factor by which the unreddened count rate will be reduced for an) 208.81 205.33 P
1.23 (amount of reddening appropriate to your object, multiply the count rate from the) 203.4 193.33 P
(previous step by this factor:) 203.4 181.33 T
10 11 Q
(\245) 189 166.33 T
0 10 Q
0.42 (The GHRS detectors are nonlinear at high count rates: this phenomenon is referred) 203.4 166.33 P
1.42 (to as the \322dead-time\323 or \322paired-pulse\323 ef) 203.4 154.33 P
1.42 (fect. Consequently) 378.34 154.33 P
1.42 (, the predicted count) 454.1 154.33 P
-0.09 (rate from the previous step must be reduced to yield the actual count rate that GHRS) 203.4 142.33 P
0.07 (will measure. Multiply the count rate you just determined by the \322fraction detected\323) 203.4 130.33 P
(value determined from Figure) 203.4 118.33 T
(2 on page) 325.6 118.33 T
(71 to obtain the \336nal predicted count rate.) 366.98 118.33 T
10 11 Q
(\245) 189 103.33 T
0 10 Q
0.29 (This \336nal value is probably reliable to within a factor of two, which is adequate for) 203.4 103.33 P
(acquisition purposes in almost all instances.) 203.4 91.33 T
479.42 217.67 512.9 236.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 480.42 222.17 T
(0) 485.42 222.17 T
0 7 Q
(0) 494.57 229.77 T
(.) 498.07 229.77 T
(4) 499.82 229.77 T
3 F
(V) 503.85 229.77 T
0 5 Q
(0) 508.4 227.52 T
0 7 Q
(\320) 490.8 229.77 T
0 0 612 792 C
317 176.84 398.14 193.43 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 318 181.33 T
(0) 323 181.33 T
0 7 Q
(s) 328.38 187.18 T
(c) 331.1 187.18 T
(a) 334.21 187.18 T
(l) 337.32 187.18 T
(e) 339.27 187.18 T
(f) 344.12 187.18 T
(a) 346.45 187.18 T
(c) 349.56 187.18 T
(t) 352.67 187.18 T
(o) 354.62 187.18 T
(r) 358.12 187.18 T
3 F
(E) 367.78 187.18 T
(B) 376.77 187.18 T
(V) 388.04 187.18 T
0 F
(\320) 382.79 187.18 T
13 F
(\050) 373.77 187.18 T
(\051) 392.64 187.18 T
(\264) 362.19 187.18 T
0 0 612 792 C
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[0 0 0 1 0 0 0]
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[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (69) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(T) 207 736.18 T
(arget Acquisition Reference Information) 211.83 736.18 T
2 10 Q
(7.1.1) 175.76 679.35 T
(Alternate Method for Predicting T) 207 679.35 T
(arget Acquisition Count Rates) 364.61 679.35 T
0 F
1.47 (Figure) 207 655.35 P
1.47 (7-1 on page) 235.61 655.35 P
1.47 (70 shows mean predicted count rates as a function of) 288.25 655.35 P
-0.23 (color for the four acquisition mirrors. Also shown are the \336ts to the predicted count rates) 207 643.35 P
0.28 (for various amounts of reddening. The label for each curve represents the color excess,) 207 631.35 P
3 F
(E\050B \320 V\051) 207 619.35 T
0 F
(, applied to the spectra.) 241.99 619.35 T
(Y) 207 595.35 T
(ou can estimate tar) 213.22 595.35 T
(get acquisition count rates using the plots instead of T) 288.3 595.35 T
(able) 503.42 595.35 T
(7-1:) 522.58 595.35 T
10 11 Q
(\245) 207 577.35 T
0 10 Q
1.9 (Determine the intrinsic color and magnitude of your object as well as its color) 221.4 577.35 P
(excess.) 221.4 565.35 T
10 11 Q
(\245) 207 550.35 T
0 10 Q
(Read from the Figures \050depending on the mirror used\051 the predicted count rate.) 221.4 550.35 T
10 11 Q
(\245) 207 535.35 T
0 10 Q
-0.13 (Scale the predicted count rate by the ratio of apparent brightness of your object to an) 221.4 535.35 P
(object with zero magnitude.) 221.4 523.35 T
10 11 Q
(\245) 207 508.35 T
0 10 Q
(Use Figure) 221.4 508.35 T
(2 on page) 268.06 508.35 T
(71 to correct for the \322paired-pulse\323 ef) 309.44 508.35 T
(fect.) 459.76 508.35 T
2 F
(7.1.2) 175.76 478.35 T
(T) 207 478.35 T
(wo Examples) 212.37 478.35 T
0 F
(First, suppose you want to observe) 207 454.35 T
13 F
(m) 348.38 454.35 T
0 F
( Col, which has the following properties:) 354.14 454.35 T
-0.12 (Using the table, you would see that HR 8023, an O6 star with) 207 388.35 P
-0.12 ( is the) 534.35 388.35 P
0.09 (closest match, giving a predicted count rate for the A2 mirror of 1.3) 207 376.35 P
0.09 (x) 481.66 376.35 P
0.09 (10) 489.16 376.35 P
0 8 Q
0.07 (7) 499.16 380.35 P
0 10 Q
0.09 (counts s) 503.16 376.35 P
0 8 Q
0.07 (\3201) 535.75 380.35 P
0 10 Q
0.09 ( for) 543.75 376.35 P
0.29 (a) 207 364.35 P
3 F
0.29 (V) 214.24 364.35 P
0 8 Q
0.24 (0) 220.35 361.85 P
0 10 Q
0.29 (= 0 star) 227.14 364.35 P
0.29 (. Multiplying this count rate by 10) 257.26 364.35 P
0 8 Q
0.24 (-0.4) 395.98 368.35 P
13 F
0.24 (\264) 408.64 368.35 P
0 F
0.24 (5.13) 413.04 368.35 P
0 10 Q
0.29 (gives 1.2) 429.27 364.35 P
0.29 (x) 468.17 364.35 P
0.29 (10) 475.67 364.35 P
0 8 Q
0.24 (5) 485.67 368.35 P
0 10 Q
0.29 ( counts s) 489.67 364.35 P
0 8 Q
0.24 (\3201) 525.27 368.35 P
0 10 Q
0.29 (. Red-) 533.27 364.35 P
-0.24 (dening will decrease the counts slightly; calculation of the scale factor indicates that you) 207 352.35 P
0.14 (should multiply by 0.93, giving a new count rate of 1.1) 207 340.35 P
0.14 (x) 431.22 340.35 P
0.14 (10) 438.72 340.35 P
0 8 Q
0.12 (5) 448.72 344.35 P
0 10 Q
0.14 ( counts s) 452.72 340.35 P
0 8 Q
0.12 (-1) 488.01 344.35 P
0 10 Q
0.14 (. The dead-time) 494.67 340.35 P
-0.06 (correction factor estimates that only 83% of those counts will be detected, so one would) 207 328.35 P
0.22 (expect approximately 94000 counts s) 207 316.35 P
0 8 Q
0.17 (-1) 356.74 320.35 P
0 10 Q
0.22 (with this star) 365.58 316.35 P
0.22 (. In fact, when) 417.14 316.35 P
13 F
0.22 (m) 477.99 316.35 P
0 F
0.22 ( Col was observed) 483.75 316.35 P
0.09 (early in Cycle) 207 304.35 P
0.09 (4, 19,600 counts were obtained in 0.2) 265.78 304.35 P
0.09 (seconds with the A2 mirror) 419.08 304.35 P
0.09 (, which) 528.47 304.35 P
(works out to 98,000) 207 292.35 T
(counts s) 289.5 292.35 T
0 8 Q
(-1) 322 296.35 T
0 10 Q
(, which is within 5% of the calculated value.) 328.66 292.35 T
(Second, consider a very red star such as Aldebaran:) 207 268.35 T
0.39 (Using the table, you would see that BD\3201) 207 202.35 P
0 8 Q
0.31 (o) 376.95 206.35 P
0 10 Q
0.39 (31) 380.95 202.35 P
0.39 (13 has a similar spectral type \050K5III\051 and) 390.58 202.35 P
0.52 (color \0501.61\051. The calculated count rate for mirror A2 is then) 207 190.35 P
0.52 ( counts per sec-) 493.95 190.35 P
0.02 (ond. The adjustment for apparent magnitude is) 207 178.35 P
0.02 (, which yields a count rate of) 442.06 178.35 P
0.14 (530 per second, or 210 in 0.2 seconds. Early in Cycle 4 a T) 207 166.35 P
0.14 (au was acquired with mirror) 444.7 166.35 P
(A2 and the count rate seen was 246 in 0.2 seconds, within 15% of the predicted value.) 207 154.35 T
2 8 Q
(Name) 214.11 432.68 T
(Sp. T) 279.51 432.68 T
(ype.) 298.48 432.68 T
6 F
(V) 366.33 432.68 T
(B \320 V) 431 432.68 T
(E\050B \320 V\051) 497.66 432.68 T
13 10 Q
(m) 202.5 416.02 T
0 9 Q
( Columbae) 208.26 416.02 T
(O9V) 288.25 416.02 T
(5.16) 361.12 416.02 T
(\3200.29) 430.88 416.02 T
(0.01) 505.12 416.02 T
2 8 Q
(Name) 214.11 246.68 T
(Sp. T) 279.51 246.68 T
(ype.) 298.48 246.68 T
6 F
(V) 366.33 246.68 T
(B \320 V) 431 246.68 T
(E\050B \320 V\051) 497.66 246.68 T
13 10 Q
(a) 211.16 230.02 T
0 9 Q
(T) 219.97 230.02 T
(auri) 224.84 230.02 T
(K5III) 287.01 230.02 T
(0.84) 361.12 230.02 T
(1.54) 433.12 230.02 T
(0.00) 505.12 230.02 T
189 444.89 189 409.14 2 L
V
0 Z
N
261 445.14 261 408.89 2 L
V
N
333 445.14 333 408.89 2 L
V
N
405 445.14 405 408.89 2 L
V
N
477 445.14 477 408.89 2 L
V
N
549 444.89 549 409.14 2 L
V
N
188.88 445.02 549.12 445.02 2 L
V
N
188.88 426.02 549.12 426.02 2 L
V
0.5 H
N
188.88 409.02 549.12 409.02 2 L
V
0.25 H
N
189 258.89 189 223.14 2 L
V
N
261 259.14 261 222.89 2 L
V
N
333 259.14 333 222.89 2 L
V
N
405 259.14 405 222.89 2 L
V
N
477 259.14 477 222.89 2 L
V
N
549 258.89 549 223.14 2 L
V
N
188.88 259.02 549.12 259.02 2 L
V
N
188.88 240.02 549.12 240.02 2 L
V
0.5 H
N
188.88 223.02 549.12 223.02 2 L
V
0.25 H
N
517.3 648.5 558 663.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(B) 524.35 655.35 T
(V) 540.46 655.35 T
0 F
(\320) 532.96 655.35 T
13 F
(\050) 520.06 655.35 T
(\051) 547.03 655.35 T
0 7 Q
(0) 552.41 652.25 T
0 0 612 792 C
454.02 383.85 534.35 396.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
0 X
0 0 0 1 0 0 0 K
(B) 461.07 388.35 T
(V) 477.18 388.35 T
0 F
(\320) 469.68 388.35 T
13 F
(\050) 456.78 388.35 T
(\051) 483.75 388.35 T
0 F
(0) 509.76 388.35 T
(.) 514.76 388.35 T
(3) 517.26 388.35 T
(1) 522.26 388.35 T
(3) 527.26 388.35 T
(\320) 504.38 388.35 T
(=) 493.74 388.35 T
0 0 612 792 C
454.08 185.85 493.95 202.45 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 455.08 190.35 T
(.) 460.08 190.35 T
(6) 462.58 190.35 T
(1) 478.07 190.35 T
(0) 483.07 190.35 T
0 7 Q
(3) 488.45 196.2 T
13 10 Q
(\264) 470.08 190.35 T
0 0 612 792 C
396.58 173.85 442.06 190.45 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 397.58 178.35 T
(0) 402.58 178.35 T
0 7 Q
(0) 411.72 184.2 T
(.) 415.22 184.2 T
(4) 416.97 184.2 T
(0) 427.81 184.2 T
(.) 431.31 184.2 T
(8) 433.06 184.2 T
(4) 436.56 184.2 T
13 F
(\264) 422.22 184.2 T
0 F
(\320) 407.95 184.2 T
0 0 612 792 C
FMENDPAGE
%%EndPage: "69" 69
%%Page: "70" 70
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(T) 189 736.18 T
(arget Acquisition Reference Information) 193.83 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(70) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
63 90 540 711 R
0.01 (Figure 7-1.) 0 -270 517.67 162 PF
4 F
0.01 (Mean target acquisition count rates for stars with the four mirrors of the GHRS. The numbers at) 0 -270 517.67 218.15 PF
(the right indicate the appropriate) 0 -270 529.67 162 TF
8 F
( E\050B \320 V\051) 0 -270 529.67 305.41 TF
4 F
( for each curve.) 0 -270 529.67 345.98 TF
63 90 540 711 R
63 90 540 711 C
70 90 502 711 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 43 29 576 727 213.2 279.2 283.7 425.3 FMBEGINEPSF
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frequency newscreenangle /spotfunction load
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% SP: Set Pattern: pattern -> -
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% FI: Fill with Pattern: - -> -
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%%EndProlog
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%%Page: 1 1
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M ]gE\ D ]dEd SR M ]dEd D ]aEh SR M ]aEh D ][El SR M ^BD_ D ]?D[ SR
M ]?D[ D ^BDW SR M ^BDW D ^ED[ SR M ^ED[ D ^BD_ SR M ^^El D ^XEC SR
M ^XEC D ^^EG SR M ^^EG D ^gEL SR M ^gEL D ^pEL SR M ^pEL D ^yEG SR
M ^yEG D ^?D? SR M ^?D? D _BDs SR M _BDs D _BDo SR M _BDo D ^?Dc SR
M ^?Dc D ^yD[ SR M ^yD[ D ^pDW SR M ^pDW D ^gDW SR M ^gDW D ^^D[ SR
M ^^D[ D ^[D_ SR M ^[D_ D ^XDg SR M ^XDg D ^XDk SR M ^XDk D ^[Do SR
M ^[Do D ^^Dk SR M ^^Dk D ^[Dg SR M ^pEL D ^vEG SR M ^vEG D ^|D? SR
M ^|D? D ^?Ds SR M ^?Ds D ^?Do SR M ^?Do D ^|Dc SR M ^|Dc D ^vD[ SR
M ^vD[ D ^pDW SR M ^^El D ^|El SR M ^^Eh D ^mEh SR M ^mEh D ^|El SR
M j?E\ D kEE` SR M kEE` D kNEl SR M kNEl D kNDW SR M kKEh D kKDW SR
M j?DW D kZDW SR M w]E\ D wcE` SR M wcE` D wlEl SR M wlEl D wlDW SR
M wiEh D wiDW SR M w]DW D wxDW SR M xTD_ D xQD[ SR M xQD[ D xTDW SR
M xTDW D xWD[ SR M xWD[ D xTD_ SR M xoEl D xiEC SR M xiEC D xoEG SR
M xoEG D xxEL SR M xxEL D yAEL SR M yAEL D yKEG SR M yKEG D yQD? SR
M yQD? D yTDs SR M yTDs D yTDo SR M yTDo D yQDc SR M yQDc D yKD[ SR
M yKD[ D yADW SR M yADW D xxDW SR M xxDW D xoD[ SR M xoD[ D xlD_ SR
M xlD_ D xiDg SR M xiDg D xiDk SR M xiDk D xlDo SR M xlDo D xoDk SR
M xoDk D xlDg SR M yAEL D yHEG SR M yHEG D yND? SR M yND? D yQDs SR
M yQDs D yQDo SR M yQDo D yNDc SR M yNDc D yHD[ SR M yHD[ D yADW SR
M xoEl D yNEl SR M xoEh D x~Eh SR M x~Eh D yNEl SR M FY|r D |r|r SR
M FY|r D FY|R SR M IA|r D IA|R SR M Ki|r D Ki|R SR M NQ|r D NQ|R SR
M Pz|r D Pz{r SR M Sb|r D Sb|R SR M VJ|r D VJ|R SR M Xr|r D Xr|R SR
M [Z|r D [Z|R SR M ^B|r D ^B{r SR M `j|r D `j|R SR M cS|r D cS|R SR
M e{|r D e{|R SR M hc|r D hc|R SR M kK|r D kK{r SR M ms|r D ms|R SR
M p[|r D p[|R SR M sC|r D sC|R SR M ul|r D ul|R SR M xT|r D xT{r SR
M z||r D z||R SR M FYFY D FY|r SR M FYFY D FyFY SR M FYFY D GYFY SR
M FYIH D FyIH SR M FYJn D FyJn SR M FYKv D FyKv SR M FYLn D FyLn SR
M FYM\ D FyM\ SR M FYNC D FyNC SR M FYNe D FyNe SR M FYOB D FyOB SR
M FYO] D FyO] SR M FYO] D GYO] SR M FYRL D FyRL SR M FYSr D FySr SR
M FYTz D FyTz SR M FYUr D FyUr SR M FYV` D FyV` SR M FYWG D FyWG SR
M FYWi D FyWi SR M FYXG D FyXG SR M FYXa D FyXa SR M FYXa D GYXa SR
M FY[P D Fy[P SR M FY\v D Fy\v SR M FY]~ D Fy]~ SR M FY^w D Fy^w SR
M FY_e D Fy_e SR M FY`K D Fy`K SR M FY`m D Fy`m SR M FYaK D FyaK SR
M FYae D Fyae SR M FYae D GYae SR M FYdT D FydT SR M FYez D Fyez SR
M FYgB D FygB SR M FYg{ D Fyg{ SR M FYhi D Fyhi SR M FYiO D FyiO SR
M FYiq D Fyiq SR M FYjO D FyjO SR M FYji D Fyji SR M FYji D GYji SR
M FYmX D FymX SR M FYn~ D Fyn~ SR M FYpG D FypG SR M FYp? D Fyp? SR
M FYqm D Fyqm SR M FYrT D FyrT SR M FYru D Fyru SR M FYsS D FysS SR
M FYsm D Fysm SR M FYsm D GYsm SR M FYv\ D Fyv\ SR M FYxB D FyxB SR
M FYyK D FyyK SR M FYzC D FyzC SR M FYzq D Fyzq SR M FY{X D Fy{X SR
M FY{y D Fy{y SR M FY|W D Fy|W SR M FY|r D Fy|r SR M FY|r D GY|r SR
M ByFy D B?F} SR M B?F} D CHGI SR M CHGI D CHEu SR M CEGE D CEEu SR
M ByEu D CTEu SR M C?GI D CvGE SR M CvGE D CpFy SR M CpFy D ClFe SR
M ClFe D ClFY SR M ClFY D CpFE SR M CpFE D CvEy SR M CvEy D C?Eu SR
M C?Eu D DEEu SR M DEEu D DNEy SR M DNEy D DTFE SR M DTFE D DWFY SR
M DWFY D DWFe SR M DWFe D DTFy SR M DTFy D DNGE SR M DNGE D DEGI SR
M DEGI D C?GI SR M C?GI D CyGE SR M CyGE D CvGA SR M CvGA D CsFy SR
M CsFy D CpFe SR M CpFe D CpFY SR M CpFY D CsFE SR M CsFE D CvE} SR
M CvE} D CyEy SR M CyEy D C?Eu SR M DEEu D DKEy SR M DKEy D DNE} SR
M DNE} D DQFE SR M DQFE D DTFY SR M DTFY D DTFe SR M DTFe D DQFy SR
M DQFy D DNGA SR M DNGA D DKGE SR M DKGE D DEGI SR M EIGm D EJGj SR
M EJGj D EIGh SR M EIGh D EGGj SR M EGGj D EGGm SR M EGGm D EIGr SR
M EIGr D EJGt SR M EJGt D EPGw SR M EPGw D EWGw SR M EWGw D E]Gt SR
M E]Gt D E^Gr SR M E^Gr D E`Gm SR M E`Gm D E`Gh SR M E`Gh D E^Gc SR
M E^Gc D EYG^ SR M EYG^ D EPGZ SR M EPGZ D ELGW SR M ELGW D EIGR SR
M EIGR D EGGK SR M EGGK D EGGD SR M EWGw D E[Gt SR M E[Gt D E]Gr SR
M E]Gr D E^Gm SR M E^Gm D E^Gh SR M E^Gh D E]Gc SR M E]Gc D EWG^ SR
M EWG^ D EPGZ SR M EGGI D EIGK SR M EIGK D ELGK SR M ELGK D EUGF SR
M EUGF D E[GF SR M E[GF D E^GI SR M E^GI D E`GK SR M ELGK D EUGD SR
M EUGD D E]GD SR M E]GD D E^GF SR M E^GF D E`GK SR M E`GK D E`GP SR
M ByO} D B?PA SR M B?PA D CHPN SR M CHPN D CHNy SR M CEPI D CENy SR
M ByNy D CTNy SR M C?PN D CvPI SR M CvPI D CpO} SR M CpO} D ClOi SR
M ClOi D ClO] SR M ClO] D CpOI SR M CpOI D CvN} SR M CvN} D C?Ny SR
M C?Ny D DENy SR M DENy D DNN} SR M DNN} D DTOI SR M DTOI D DWO] SR
M DWO] D DWOi SR M DWOi D DTO} SR M DTO} D DNPI SR M DNPI D DEPN SR
M DEPN D C?PN SR M C?PN D CyPI SR M CyPI D CvPE SR M CvPE D CsO} SR
M CsO} D CpOi SR M CpOi D CpO] SR M CpO] D CsOI SR M CsOI D CvOA SR
M CvOA D CyN} SR M CyN} D C?Ny SR M DENy D DKN} SR M DKN} D DNOA SR
M DNOA D DQOI SR M DQOI D DTO] SR M DTO] D DTOi SR M DTOi D DQO} SR
M DQO} D DNPE SR M DNPE D DKPI SR M DKPI D DEPN SR M EIPs D EJPq SR
M EJPq D EIPo SR M EIPo D EGPq SR M EGPq D EGPs SR M EGPs D EJPx SR
M EJPx D EPP{ SR M EPP{ D EWP{ SR M EWP{ D E]Px SR M E]Px D E^Ps SR
M E^Ps D E^Pl SR M E^Pl D E]Pg SR M E]Pg D EWPe SR M EWPe D ERPe SR
M EWP{ D E[Px SR M E[Px D E]Ps SR M E]Ps D E]Pl SR M E]Pl D E[Pg SR
M E[Pg D EWPe SR M EWPe D E[Pb SR M E[Pb D E^P^ SR M E^P^ D E`PY SR
M E`PY D E`PR SR M E`PR D E^PM SR M E^PM D E]PJ SR M E]PJ D EWPH SR
M EWPH D EPPH SR M EPPH D EJPJ SR M EJPJ D EIPM SR M EIPM D EGPR SR
M EGPR D EGPT SR M EGPT D EIPV SR M EIPV D EJPT SR M EJPT D EIPR SR
M E]P` D E^PY SR M E^PY D E^PR SR M E^PR D E]PM SR M E]PM D E[PJ SR
M E[PJ D EWPH SR M ByYA D B?YF SR M B?YF D CHYR SR M CHYR D CHW} SR
M CEYN D CEW} SR M ByW} D CTW} SR M C?YR D CvYN SR M CvYN D CpYA SR
M CpYA D ClXm SR M ClXm D ClXa SR M ClXa D CpXM SR M CpXM D CvXA SR
M CvXA D C?W} SR M C?W} D DEW} SR M DEW} D DNXA SR M DNXA D DTXM SR
M DTXM D DWXa SR M DWXa D DWXm SR M DWXm D DTYA SR M DTYA D DNYN SR
M DNYN D DEYR SR M DEYR D C?YR SR M C?YR D CyYN SR M CyYN D CvYJ SR
M CvYJ D CsYA SR M CsYA D CpXm SR M CpXm D CpXa SR M CpXa D CsXM SR
M CsXM D CvXE SR M CvXE D CyXA SR M CyXA D C?W} SR M DEW} D DKXA SR
M DKXA D DNXE SR M DNXE D DQXM SR M DQXM D DTXa SR M DTXa D DTXm SR
M DTXm D DQYA SR M DQYA D DNYJ SR M DNYJ D DKYN SR M DKYN D DEYR SR
M EWYz D EWYL SR M EYY? D EYYL SR M EYY? D EEY[ SR M EEY[ D EbY[ SR
M ERYL D E^YL SR M BybF D B?bJ SR M B?bJ D CHbV SR M CHbV D CHaA SR
M CEbR D CEaA SR M ByaA D CTaA SR M C?bV D CvbR SR M CvbR D CpbF SR
M CpbF D Claq SR M Claq D Clae SR M Clae D CpaQ SR M CpaQ D CvaE SR
M CvaE D C?aA SR M C?aA D DEaA SR M DEaA D DNaE SR M DNaE D DTaQ SR
M DTaQ D DWae SR M DWae D DWaq SR M DWaq D DTbF SR M DTbF D DNbR SR
M DNbR D DEbV SR M DEbV D C?bV SR M C?bV D CybR SR M CybR D CvbN SR
M CvbN D CsbF SR M CsbF D Cpaq SR M Cpaq D Cpae SR M Cpae D CsaQ SR
M CsaQ D CvaI SR M CvaI D CyaE SR M CyaE D C?aA SR M DEaA D DKaE SR
M DKaE D DNaI SR M DNaI D DQaQ SR M DQaQ D DTae SR M DTae D DTaq SR
M DTaq D DQbF SR M DQbF D DNbN SR M DNbN D DKbR SR M DKbR D DEbV SR
M EJcC D EGbk SR M EGbk D EJbm SR M EJbm D EPbp SR M EPbp D EUbp SR
M EUbp D E[bm SR M E[bm D E^bh SR M E^bh D E`ba SR M E`ba D E`b_ SR
M E`b_ D E^bW SR M E^bW D E[bS SR M E[bS D EUbP SR M EUbP D EPbP SR
M EPbP D EJbS SR M EJbS D EIbU SR M EIbU D EGbZ SR M EGbZ D EGb\ SR
M EGb\ D EIb_ SR M EIb_ D EJb\ SR M EJb\ D EIbZ SR M EUbp D EYbm SR
M EYbm D E]bh SR M E]bh D E^ba SR M E^ba D E^b_ SR M E^b_ D E]bW SR
M E]bW D EYbS SR M EYbS D EUbP SR M EJcC D E]cC SR M EJcA D EScA SR
M EScA D E]cC SR M BykJ D B?kN SR M B?kN D CHkZ SR M CHkZ D CHjE SR
M CEkV D CEjE SR M ByjE D CTjE SR M C?kZ D CvkV SR M CvkV D CpkJ SR
M CpkJ D Cljv SR M Cljv D Clji SR M Clji D CpjU SR M CpjU D CvjI SR
M CvjI D C?jE SR M C?jE D DEjE SR M DEjE D DNjI SR M DNjI D DTjU SR
M DTjU D DWji SR M DWji D DWjv SR M DWjv D DTkJ SR M DTkJ D DNkV SR
M DNkV D DEkZ SR M DEkZ D C?kZ SR M C?kZ D CykV SR M CykV D CvkR SR
M CvkR D CskJ SR M CskJ D Cpjv SR M Cpjv D Cpji SR M Cpji D CsjU SR
M CsjU D CvjM SR M CvjM D CyjI SR M CyjI D C?jE SR M DEjE D DKjI SR
M DKjI D DNjM SR M DNjM D DQjU SR M DQjU D DTji SR M DTji D DTjv SR
M DTjv D DQkJ SR M DQkJ D DNkR SR M DNkR D DKkV SR M DKkV D DEkZ SR
M E]l@ D E[k} SR M E[k} D E]k{ SR M E]k{ D E^k} SR M E^k} D E^l@ SR
M E^l@ D E]lE SR M E]lE D EYlG SR M EYlG D ESlG SR M ESlG D ENlE SR
M ENlE D EJl@ SR M EJl@ D EIk{ SR M EIk{ D EGkq SR M EGkq D EGkc SR
M EGkc D EIk[ SR M EIk[ D ELkW SR M ELkW D ERkT SR M ERkT D EUkT SR
M EUkT D E[kW SR M E[kW D E^k[ SR M E^k[ D E`kc SR M E`kc D E`ke SR
M E`ke D E^kl SR M E^kl D E[kq SR M E[kq D EUkt SR M EUkt D ESkt SR
M ESkt D ENkq SR M ENkq D EJkl SR M EJkl D EIke SR M ESlG D EPlE SR
M EPlE D ELl@ SR M ELl@ D EJk{ SR M EJk{ D EIkq SR M EIkq D EIkc SR
M EIkc D EJk[ SR M EJk[ D ENkW SR M ENkW D ERkT SR M EUkT D EYkW SR
M EYkW D E]k[ SR M E]k[ D E^kc SR M E^kc D E^ke SR M E^ke D E]kl SR
M E]kl D EYkq SR M EYkq D EUkt SR M BytN D B?tR SR M B?tR D CHt^ SR
M CHt^ D CHsI SR M CEtZ D CEsI SR M BysI D CTsI SR M C?t^ D CvtZ SR
M CvtZ D CptN SR M CptN D Clsz SR M Clsz D Clsn SR M Clsn D CpsY SR
M CpsY D CvsM SR M CvsM D C?sI SR M C?sI D DEsI SR M DEsI D DNsM SR
M DNsM D DTsY SR M DTsY D DWsn SR M DWsn D DWsz SR M DWsz D DTtN SR
M DTtN D DNtZ SR M DNtZ D DEt^ SR M DEt^ D C?t^ SR M C?t^ D CytZ SR
M CytZ D CvtV SR M CvtV D CstN SR M CstN D Cpsz SR M Cpsz D Cpsn SR
M Cpsn D CssY SR M CssY D CvsQ SR M CvsQ D CysM SR M CysM D C?sI SR
M DEsI D DKsM SR M DKsM D DNsQ SR M DNsQ D DQsY SR M DQsY D DTsn SR
M DTsn D DTsz SR M DTsz D DQtN SR M DQtN D DNtV SR M DNtV D DKtZ SR
M DKtZ D DEt^ SR M EGuK D EGt} SR M EGuB D EIuF SR M EIuF D ELuK SR
M ELuK D EPuK SR M EPuK D EYuD SR M EYuD D E]uD SR M E]uD D E^uF SR
M E^uF D E`uK SR M EIuF D ELuI SR M ELuI D EPuI SR M EPuI D EYuD SR
M E`uK D E`uD SR M E`uD D E^t} SR M E^t} D EWtq SR M EWtq D EUtl SR
M EUtl D EStd SR M EStd D EStX SR M E^t} D EUtq SR M EUtq D EStl SR
M EStl D ERtd SR M ERtd D ERtX SR M By}R D B?}V SR M B?}V D CH}b SR
M CH}b D CH|M SR M CE}^ D CE|M SR M By|M D CT|M SR M C?}b D Cv}^ SR
M Cv}^ D Cp}R SR M Cp}R D Cl|~ SR M Cl|~ D Cl|r SR M Cl|r D Cp|^ SR
M Cp|^ D Cv|Q SR M Cv|Q D C?|M SR M C?|M D DE|M SR M DE|M D DN|Q SR
M DN|Q D DT|^ SR M DT|^ D DW|r SR M DW|r D DW|~ SR M DW|~ D DT}R SR
M DT}R D DN}^ SR M DN}^ D DE}b SR M DE}b D C?}b SR M C?}b D Cy}^ SR
M Cy}^ D Cv}Z SR M Cv}Z D Cs}R SR M Cs}R D Cp|~ SR M Cp|~ D Cp|r SR
M Cp|r D Cs|^ SR M Cs|^ D Cv|U SR M Cv|U D Cy|Q SR M Cy|Q D C?|M SR
M DE|M D DK|Q SR M DK|Q D DN|U SR M DN|U D DQ|^ SR M DQ|^ D DT|r SR
M DT|r D DT|~ SR M DT|~ D DQ}R SR M DQ}R D DN}Z SR M DN}Z D DK}^ SR
M DK}^ D DE}b SR M EP~O D EJ~M SR M EJ~M D EI~H SR M EI~H D EI~A SR
M EI~A D EJ}| SR M EJ}| D EP}z SR M EP}z D EW}z SR M EW}z D E]}| SR
M E]}| D E^~A SR M E^~A D E^~H SR M E^~H D E]~M SR M E]~M D EW~O SR
M EW~O D EP~O SR M EP~O D EL~M SR M EL~M D EJ~H SR M EJ~H D EJ~A SR
M EJ~A D EL}| SR M EL}| D EP}z SR M EW}z D E[}| SR M E[}| D E]~A SR
M E]~A D E]~H SR M E]~H D E[~M SR M E[~M D EW~O SR M EP}z D EJ}w SR
M EJ}w D EI}u SR M EI}u D EG}p SR M EG}p D EG}f SR M EG}f D EI}a SR
M EI}a D EJ}_ SR M EJ}_ D EP}\ SR M EP}\ D EW}\ SR M EW}\ D E]}_ SR
M E]}_ D E^}a SR M E^}a D E`}f SR M E`}f D E`}p SR M E`}p D E^}u SR
M E^}u D E]}w SR M E]}w D EW}z SR M EP}z D EL}w SR M EL}w D EJ}u SR
M EJ}u D EI}p SR M EI}p D EI}f SR M EI}f D EJ}a SR M EJ}a D EL}_ SR
M EL}_ D EP}\ SR M EW}\ D E[}_ SR M E[}_ D E]}a SR M E]}a D E^}f SR
M E^}f D E^}p SR M E^}p D E]}u SR M E]}u D E[}w SR M E[}w D EW}z SR
M |rFY D |r|r SR M |rFY D |RFY SR M |rFY D {rFY SR M |rIH D |RIH SR
M |rJn D |RJn SR M |rKv D |RKv SR M |rLn D |RLn SR M |rM\ D |RM\ SR
M |rNC D |RNC SR M |rNe D |RNe SR M |rOB D |ROB SR M |rO] D |RO] SR
M |rO] D {rO] SR M |rRL D |RRL SR M |rSr D |RSr SR M |rTz D |RTz SR
M |rUr D |RUr SR M |rV` D |RV` SR M |rWG D |RWG SR M |rWi D |RWi SR
M |rXG D |RXG SR M |rXa D |RXa SR M |rXa D {rXa SR M |r[P D |R[P SR
M |r\v D |R\v SR M |r]~ D |R]~ SR M |r^w D |R^w SR M |r_e D |R_e SR
M |r`K D |R`K SR M |r`m D |R`m SR M |raK D |RaK SR M |rae D |Rae SR
M |rae D {rae SR M |rdT D |RdT SR M |rez D |Rez SR M |rgB D |RgB SR
M |rg{ D |Rg{ SR M |rhi D |Rhi SR M |riO D |RiO SR M |riq D |Riq SR
M |rjO D |RjO SR M |rji D |Rji SR M |rji D {rji SR M |rmX D |RmX SR
M |rn~ D |Rn~ SR M |rpG D |RpG SR M |rp? D |Rp? SR M |rqm D |Rqm SR
M |rrT D |RrT SR M |rru D |Rru SR M |rsS D |RsS SR M |rsm D |Rsm SR
M |rsm D {rsm SR M |rv\ D |Rv\ SR M |rxB D |RxB SR M |ryK D |RyK SR
M |rzC D |RzC SR M |rzq D |Rzq SR M |r{X D |R{X SR M |r{y D |R{y SR
M |r|W D |R|W SR M |r|r D |R|r SR M |r|r D {r|r SR
M @^Ub D @dUf SR M @dUf D @TUf SR M @TUf D @^Ub SR M @^Ub D @WUZ SR
M @WUZ D @TUN SR M @TUN D @TUF SR M @TUF D @WTz SR M @WTz D @^Tq SR
M @^Tq D @dTm SR M @dTm D @mTi SR M @mTi D @|Ti SR M @|Ti D AETm SR
M AETm D AKTq SR M AKTq D AQTz SR M AQTz D ATUF SR M ATUF D ATUN SR
M ATUN D AQUZ SR M AQUZ D AKUb SR M AKUb D AEUf SR M @TUF D @WT~ SR
M @WT~ D @^Tv SR M @^Tv D @dTq SR M @dTq D @mTm SR M @mTm D @|Tm SR
M @|Tm D AETq SR M AETq D AKTv SR M AKTv D AQT~ SR M AQT~ D ATUF SR
M @jVV D @mVJ SR M @mVJ D @sVB SR M @sVB D @|U~ SR M @|U~ D ABU~ SR
M ABU~ D AKVB SR M AKVB D AQVJ SR M AQVJ D ATVV SR M ATVV D ATV^ SR
M ATV^ D AQVk SR M AQVk D AKVs SR M AKVs D ABVw SR M ABVw D @|Vw SR
M @|Vw D @sVs SR M @sVs D @mVk SR M @mVk D @jV^ SR M @jV^ D @jVV SR
M @jVV D @mVN SR M @mVN D @sVF SR M @sVF D @|VB SR M @|VB D ABVB SR
M ABVB D AKVF SR M AKVF D AQVN SR M AQVN D ATVV SR M ATV^ D AQVf SR
M AQVf D AKVo SR M AKVo D ABVs SR M ABVs D @|Vs SR M @|Vs D @sVo SR
M @sVo D @mVf SR M @mVf D @jV^ SR M @jWW D AKWW SR M AKWW D AQW[ SR
M AQW[ D ATWg SR M ATWg D ATWo SR M ATWo D AQW{ SR M AQW{ D AKXC SR
M @jW[ D AKW[ SR M AKW[ D AQW_ SR M AQW_ D ATWg SR M @jXC D ATXC SR
M @jXG D ATXG SR M @jWK D @jW[ SR M @jWw D @jXG SR M ATXC D ATXS SR
M @jXp D ATXp SR M @jXt D ATXt SR M @sXt D @mX| SR M @mX| D @jYH SR
M @jYH D @jYP SR M @jYP D @mY\ SR M @mY\ D @sY` SR M @sY` D ATY` SR
M @jYP D @mYX SR M @mYX D @sY\ SR M @sY\ D ATY\ SR M @jXd D @jXt SR
M ATXd D ATY@ SR M ATYP D ATYl SR M @TZH D AHZH SR M AHZH D AQZM SR
M AQZM D ATZU SR M ATZU D ATZ] SR M ATZ] D AQZe SR M AQZe D AKZi SR
M @TZM D AHZM SR M AHZM D AQZQ SR M AQZQ D ATZU SR M @jY| D @jZ] SR
M @T\N D AT\N SR M @T\R D AT\R SR M @T\A D @T\r SR M @T\r D @W\~ SR
M @W\~ D @Z]B SR M @Z]B D @a]F SR M @a]F D @g]F SR M @g]F D @m]B SR
M @m]B D @p\~ SR M @p\~ D @s\r SR M @s\r D @s\R SR M @T\r D @W\z SR
M @W\z D @Z\~ SR M @Z\~ D @a]B SR M @a]B D @g]B SR M @g]B D @m\~ SR
M @m\~ D @p\z SR M @p\z D @s\r SR M AT\A D AT\^ SR M @s\j D AN\z SR
M AN\z D AT]B SR M AT]B D AT]J SR M AT]J D AN]N SR M @s\j D @y\r SR
M @y\r D AT]B SR M @p]f D @s]f SR M @s]f D @s]b SR M @s]b D @p]b SR
M @p]b D @m]f SR M @m]f D @j]n SR M @j]n D @j]? SR M @j]? D @m^G SR
M @m^G D @p^K SR M @p^K D @v^O SR M @v^O D AK^O SR M AK^O D AQ^S SR
M AQ^S D AT^W SR M @p^K D AK^K SR M AK^K D AQ^O SR M AQ^O D AT^W SR
M AT^W D AT^[ SR M @v^K D @y^G SR M @y^G D @|]n SR M @|]n D @?]b SR
M @?]b D AE]^ SR M AE]^ D AK]^ SR M AK]^ D AQ]b SR M AQ]b D AT]n SR
M AT]n D AT]z SR M AT]z D AQ^C SR M AQ^C D AK^K SR M @|]n D @?]f SR
M @?]f D AE]b SR M AE]b D AK]b SR M AK]b D AQ]f SR M AQ]f D AT]n SR
M @T^w D AH^w SR M AH^w D AQ^{ SR M AQ^{ D AT_C SR M AT_C D AT_K SR
M AT_K D AQ_S SR M AQ_S D AK_W SR M @T^{ D AH^{ SR M AH^{ D AQ^? SR
M AQ^? D AT_C SR M @j^k D @j_K SR M @|_p D @|`` SR M @|`` D @v`` SR
M @v`` D @p`\ SR M @p`\ D @m`X SR M @m`X D @j`P SR M @j`P D @j`D SR
M @j`D D @m_x SR M @m_x D @s_p SR M @s_p D @|_k SR M @|_k D AB_k SR
M AB_k D AK_p SR M AK_p D AQ_x SR M AQ_x D AT`D SR M AT`D D AT`L SR
M AT`L D AQ`X SR M AQ`X D AK`` SR M @|`\ D @s`\ SR M @s`\ D @m`X SR
M @j`D D @m_| SR M @m_| D @s_t SR M @s_t D @|_p SR M @|_p D AB_p SR
M AB_p D AK_t SR M AK_t D AQ_| SR M AQ_| D AT`D SR M @Hba D @NbY SR
M @NbY D @WbQ SR M @WbQ D @dbI SR M @dbI D @sbE SR M @sbE D @?bE SR
M @?bE D ANbI SR M ANbI D AZbQ SR M AZbQ D AdbY SR M AdbY D Ajba SR
M @NbY D @ZbQ SR M @ZbQ D @dbM SR M @dbM D @sbI SR M @sbI D @?bI SR
M @?bI D ANbM SR M ANbM D AWbQ SR M AWbQ D AdbY SR M @scj D @vcf SR
M @vcf D @ycj SR M @ycj D @vcn SR M @vcn D @scn SR M @scn D @mcf SR
M @mcf D @jc^ SR M @jc^ D @jcQ SR M @jcQ D @mcE SR M @mcE D @sb} SR
M @sb} D @|by SR M @|by D ABby SR M ABby D AKb} SR M AKb} D AQcE SR
M AQcE D ATcQ SR M ATcQ D ATcZ SR M ATcZ D AQcf SR M AQcf D AKcn SR
M @jcQ D @mcI SR M @mcI D @scA SR M @scA D @|b} SR M @|b} D ABb} SR
M ABb} D AKcA SR M AKcA D AQcI SR M AQcI D ATcQ SR M @jd^ D @mdR SR
M @mdR D @sdJ SR M @sdJ D @|dF SR M @|dF D ABdF SR M ABdF D AKdJ SR
M AKdJ D AQdR SR M AQdR D ATd^ SR M ATd^ D ATdf SR M ATdf D AQdr SR
M AQdr D AKdz SR M AKdz D ABd~ SR M ABd~ D @|d~ SR M @|d~ D @sdz SR
M @sdz D @mdr SR M @mdr D @jdf SR M @jdf D @jd^ SR M @jd^ D @mdV SR
M @mdV D @sdN SR M @sdN D @|dJ SR M @|dJ D ABdJ SR M ABdJ D AKdN SR
M AKdN D AQdV SR M AQdV D ATd^ SR M ATdf D AQdn SR M AQdn D AKdv SR
M AKdv D ABdz SR M ABdz D @|dz SR M @|dz D @sdv SR M @sdv D @mdn SR
M @mdn D @jdf SR M @je_ D AKe_ SR M AKe_ D AQec SR M AQec D ATeo SR
M ATeo D ATew SR M ATew D AQfC SR M AQfC D AKfK SR M @jec D AKec SR
M AKec D AQeg SR M AQeg D ATeo SR M @jfK D ATfK SR M @jfO D ATfO SR
M @jeR D @jec SR M @je? D @jfO SR M ATfK D ATf[ SR M @jfw D ATfw SR
M @jf{ D ATf{ SR M @sf{ D @mgC SR M @mgC D @jgP SR M @jgP D @jgX SR
M @jgX D @mgd SR M @mgd D @sgh SR M @sgh D ATgh SR M @jgX D @mg` SR
M @mg` D @sgd SR M @sgd D ATgd SR M @jfk D @jf{ SR M ATfk D ATgH SR
M ATgX D ATgt SR M @ThP D AHhP SR M AHhP D AQhT SR M AQhT D ATh\ SR
M ATh\ D AThd SR M AThd D AQhl SR M AQhl D AKhp SR M @ThT D AHhT SR
M AHhT D AQhX SR M AQhX D ATh\ SR M @jhD D @jhd SR M @mim D @jiq SR
M @jiq D @siq SR M @siq D @mim SR M @mim D @jia SR M @jia D @jiU SR
M @jiU D @miI SR M @miI D @piE SR M @piE D @siE SR M @siE D @yiI SR
M @yiI D @|iQ SR M @|iQ D ABie SR M ABie D AEim SR M AEim D AHiq SR
M @siE D @viI SR M @viI D @yiQ SR M @yiQ D @?ie SR M @?ie D ABim SR
M ABim D AHiq SR M AHiq D ANiq SR M ANiq D AQim SR M AQim D ATia SR
M ATia D ATiU SR M ATiU D AQiI SR M AQiI D AKiE SR M AKiE D ATiE SR
M ATiE D AQiI SR M @mkz D @jk~ SR M @jk~ D @sk~ SR M @sk~ D @mkz SR
M @mkz D @jkn SR M @jkn D @jkb SR M @jkb D @mkV SR M @mkV D @pkR SR
M @pkR D @skR SR M @skR D @ykV SR M @ykV D @|k^ SR M @|k^ D ABkr SR
M ABkr D AEkz SR M AEkz D AHk~ SR M @skR D @vkV SR M @vkV D @yk^ SR
M @yk^ D @?kr SR M @?kr D ABkz SR M ABkz D AHk~ SR M AHk~ D ANk~ SR
M ANk~ D AQkz SR M AQkz D ATkn SR M ATkn D ATkb SR M ATkb D AQkV SR
M AQkV D AKkR SR M AKkR D ATkR SR M ATkR D AQkV SR M @HlR D @Hl} SR
M @@mS D @@mX SR M @@mX D @@m_ SR M @@m_ D @Ym_ SR M @@m] D @Ym] SR
M @YmS D @Ymi SR M @HnA D @NnI SR M @NnI D @WnQ SR M @WnQ D @dnY SR
M @dnY D @sn] SR M @sn] D @?n] SR M @?n] D ANnY SR M ANnY D AZnQ SR
M AZnQ D AdnI SR M AdnI D AjnA SR M @NnI D @ZnQ SR M @ZnQ D @dnU SR
M @dnU D @snY SR M @snY D @?nY SR M @?nY D ANnU SR M ANnU D AWnQ SR
M AWnQ D AdnI SR
M _bBo D _\Bg SR M _\Bg D _VB[ SR M _VB[ D _PBK SR M _PBK D _MAw SR
M _MAw D _MAg SR M _MAg D _PAR SR M _PAR D _VAB SR M _VAB D _\@v SR
M _\@v D _b@n SR M _\Bg D _VBW SR M _VBW D _SBK SR M _SBK D _PAw SR
M _PAw D _PAg SR M _PAg D _SAR SR M _SAR D _VAF SR M _VAF D _\@v SR
M _{B_ D _{AJ SR M _~B_ D _~AJ SR M _rB_ D `VB_ SR M `VB_ D `_B[ SR
M `_B[ D `bBW SR M `bBW D `eBO SR M `eBO D `eBG SR M `eBG D `bA? SR
M `bA? D `_A{ SR M `_A{ D `VAw SR M `VB_ D `\B[ SR M `\B[ D `_BW SR
M `_BW D `bBO SR M `bBO D `bBG SR M `bBG D `_A? SR M `_A? D `\A{ SR
M `\A{ D `VAw SR M _~Aw D `VAw SR M `VAw D `_As SR M `_As D `bAo SR
M `bAo D `eAg SR M `eAg D `eAZ SR M `eAZ D `bAR SR M `bAR D `_AN SR
M `_AN D `VAJ SR M `VAJ D _rAJ SR M `VAw D `\As SR M `\As D `_Ao SR
M `_Ao D `bAg SR M `bAg D `bAZ SR M `bAZ D `_AR SR M `_AR D `\AN SR
M `\AN D `VAJ SR M `xAo D anAo SR M bDB_ D bYAJ SR M bGB_ D bYAV SR
M bnB_ D bYAJ SR M a{B_ D bPB_ SR M beB_ D bxB_ SR M cDBo D cJBg SR
M cJBg D cPB[ SR M cPB[ D cVBK SR M cVBK D cYAw SR M cYAw D cYAg SR
M cYAg D cVAR SR M cVAR D cPAB SR M cPAB D cJ@v SR M cJ@v D cD@n SR
M cJBg D cPBW SR M cPBW D cSBK SR M cSBK D cVAw SR M cVAw D cVAg SR
M cVAg D cSAR SR M cSAR D cPAF SR M cPAF D cJ@v SR M cvAe D cpAb SR
M cpAb D cmA[ SR M cmA[ D ckAO SR M ckAO D ckAH SR M ckAH D cm@| SR
M cm@| D cp@t SR M cp@t D cv@r SR M cv@r D cy@r SR M cy@r D c?@t SR
M c?@t D dC@| SR M dC@| D dDAH SR M dDAH D dDAO SR M dDAO D dCA[ SR
M dCA[ D c?Ab SR M c?Ab D cyAe SR M cyAe D cvAe SR M cvAe D crAb SR
M crAb D cpA` SR M cpA` D cnA[ SR M cnA[ D cmAO SR M cmAO D cmAH SR
M cmAH D cn@| SR M cn@| D cp@w SR M cp@w D cr@t SR M cr@t D cv@r SR
M cy@r D c}@t SR M c}@t D c?@w SR M c?@w D dA@| SR M dA@| D dCAH SR
M dCAH D dCAO SR M dCAO D dAA[ SR M dAA[ D c?A` SR M c?A` D c}Ab SR
M c}Ab D cyAe SR
M kppF D kVn` SR M kppF D lIn` SR M kpow D lFn` SR M k]nx D lBnx SR
M kKn` D kan` SR M k{n` D lTn` SR M lcor D lgom SR M lgom D lcoi SR
M lcoi D l_om SR M l_om D l_or SR M l_or D lco| SR M lco| D lgpA SR
M lgpA D lqpF SR M lqpF D m@pF SR M m@pF D mKpA SR M mKpA D mOo| SR
M mOo| D mRor SR M mRor D mRoi SR M mRoi D mOo_ SR M mOo_ D mDoU SR
M mDoU D lqoK SR M lqoK D ljoG SR M ljoG D lcn} SR M lcn} D l_nn SR
M l_nn D l_n` SR M m@pF D mGpA SR M mGpA D mKo| SR M mKo| D mOor SR
M mOor D mOoi SR M mOoi D mKo_ SR M mKo_ D m@oU SR M m@oU D lqoK SR
M l_nj D lcnn SR M lcnn D ljnn SR M ljnn D l|ne SR M l|ne D mGne SR
M mGne D mOnj SR M mOnj D mRnn SR M ljnn D l|n` SR M l|n` D mKn` SR
M mKn` D mOne SR M mOne D mRnn SR M mRnn D mRnx SR
M Gmza D IAwT D JUtb D KirH D L}pC D NQnP D Oeln D PzkZ D RNjR D SbiS
D Tvh\ D VJgl D W^g@ D XrfX D ZFeq D [ZeK D \nde D ^Bc~ D _VcU D `jbj
D a~a| D cSaJ D dg`U D e{_] D gO^a D hc]b D iw\a D kK[] D l_ZX D msYR
D oGXL D p[WH D qoVF D sCUH D tXTO D ulS^ D w@Ru D xTRW SR
M y~R} D ywRz SR M ywRz D yrRp SR M yrRp D yoR` SR M yoR` D yoRW SR
M yoRW D yrRG SR M yrRG D ywQ} SR M ywQ} D y~Qz SR M y~Qz D zCQz SR
M zCQz D zJQ} SR M zJQ} D zORG SR M zORG D zQRW SR M zQRW D zQR` SR
M zQR` D zORp SR M zORp D zJRz SR M zJRz D zCR} SR M zCR} D y~R} SR
M y~R} D yyRz SR M yyRz D ywRw SR M ywRw D ytRp SR M ytRp D yrR` SR
M yrR` D yrRW SR M yrRW D ytRG SR M ytRG D ywR@ SR M ywR@ D yyQ} SR
M yyQ} D y~Qz SR M zCQz D zHQ} SR M zHQ} D zJR@ SR M zJR@ D zLRG SR
M zLRG D zORW SR M zORW D zOR` SR M zOR` D zLRp SR M zLRp D zJRw SR
M zJRw D zHRz SR M zHRz D zCR} SR M zbR@ D z`Q} SR M z`Q} D zbQz SR
M zbQz D zeQ} SR M zeQ} D zbR@ SR M {BR} D z{Rz SR M z{Rz D zvRp SR
M zvRp D zsR` SR M zsR` D zsRW SR M zsRW D zvRG SR M zvRG D z{Q} SR
M z{Q} D {BQz SR M {BQz D {GQz SR M {GQz D {NQ} SR M {NQ} D {SRG SR
M {SRG D {VRW SR M {VRW D {VR` SR M {VR` D {SRp SR M {SRp D {NRz SR
M {NRz D {GR} SR M {GR} D {BR} SR M {BR} D z}Rz SR M z}Rz D z{Rw SR
M z{Rw D zxRp SR M zxRp D zvR` SR M zvR` D zvRW SR M zvRW D zxRG SR
M zxRG D z{R@ SR M z{R@ D z}Q} SR M z}Q} D {BQz SR M {GQz D {LQ} SR
M {LQ} D {NR@ SR M {NR@ D {QRG SR M {QRG D {SRW SR M {SRW D {SR` SR
M {SR` D {QRp SR M {QRp D {NRw SR M {NRw D {LRz SR M {LRz D {GR} SR
M Gmwl D IAt` D JUqo D KioU D L}mR D NQka D OejA D Pzho D RNgi D Sbfm
D Tvex D VJeJ D W^da D Xrc{ D ZFcW D [Zbt D \nbP D ^Bak D _VaE D `j`[
D a~_o D cS^? D dg^K D e{]T D gO\Z D hc[\ D iwZ\ D kKYY D l_XT D msWO
D oGVI D p[UE D qoTD D sCSF D tXRN D ulQ\ D w@Pt D xTPV SR
M y~P~ D ywP{ SR M ywP{ D yrPq SR M yrPq D yoPa SR M yoPa D yoPW SR
M yoPW D yrPG SR M yrPG D ywO} SR M ywO} D y~Oz SR M y~Oz D zCOz SR
M zCOz D zJO} SR M zJO} D zOPG SR M zOPG D zQPW SR M zQPW D zQPa SR
M zQPa D zOPq SR M zOPq D zJP{ SR M zJP{ D zCP~ SR M zCP~ D y~P~ SR
M y~P~ D yyP{ SR M yyP{ D ywPw SR M ywPw D ytPq SR M ytPq D yrPa SR
M yrPa D yrPW SR M yrPW D ytPG SR M ytPG D ywPA SR M ywPA D yyO} SR
M yyO} D y~Oz SR M zCOz D zHO} SR M zHO} D zJPA SR M zJPA D zLPG SR
M zLPG D zOPW SR M zOPW D zOPa SR M zOPa D zLPq SR M zLPq D zJPw SR
M zJPw D zHP{ SR M zHP{ D zCP~ SR M zbPA D z`O} SR M z`O} D zbOz SR
M zbOz D zeO} SR M zeO} D zbPA SR M z{Pq D {@Pt SR M {@Pt D {GP~ SR
M {GP~ D {GOz SR M {EP{ D {EOz SR M z{Oz D {QOz SR
M Gmt{ D IAqo D JUn? D Kilg D L}je D NQhv D OegX D PzfH D RNeD D SbdJ
D TvcX D VJbm D W^bF D Xrac D ZFaA D [Z`` D \n_~ D ^B_[ D _V^v D `j^O
D a~]d D cS\u D dg\C D e{[N D gOZT D hcYW D iwXW D kKWU D l_VQ D msUL
D oGTG D p[SC D qoRB D sCQE D tXPM D ulO\ D w@Nt D xTNW SR
M y~N~ D ywN{ SR M ywN{ D yrNq SR M yrNq D yoNa SR M yoNa D yoNW SR
M yoNW D yrNG SR M yrNG D ywM~ SR M ywM~ D y~Mz SR M y~Mz D zCMz SR
M zCMz D zJM~ SR M zJM~ D zONG SR M zONG D zQNW SR M zQNW D zQNa SR
M zQNa D zONq SR M zONq D zJN{ SR M zJN{ D zCN~ SR M zCN~ D y~N~ SR
M y~N~ D yyN{ SR M yyN{ D ywNx SR M ywNx D ytNq SR M ytNq D yrNa SR
M yrNa D yrNW SR M yrNW D ytNG SR M ytNG D ywNA SR M ywNA D yyM~ SR
M yyM~ D y~Mz SR M zCMz D zHM~ SR M zHM~ D zJNA SR M zJNA D zLNG SR
M zLNG D zONW SR M zONW D zONa SR M zONa D zLNq SR M zLNq D zJNx SR
M zJNx D zHN{ SR M zHN{ D zCN~ SR M zbNA D z`M~ SR M z`M~ D zbMz SR
M zbMz D zeM~ SR M zeM~ D zbNA SR M zvNq D zxNn SR M zxNn D zvNk SR
M zvNk D zsNn SR M zsNn D zsNq SR M zsNq D zvNx SR M zvNx D zxN{ SR
M zxN{ D {@N~ SR M {@N~ D {IN~ SR M {IN~ D {QN{ SR M {QN{ D {SNx SR
M {SNx D {VNq SR M {VNq D {VNk SR M {VNk D {SNd SR M {SNd D {LN^ SR
M {LN^ D {@NW SR M {@NW D z{NT SR M z{NT D zvNN SR M zvNN D zsND SR
M zsND D zsMz SR M {IN~ D {NN{ SR M {NN{ D {QNx SR M {QNx D {SNq SR
M {SNq D {SNk SR M {SNk D {QNd SR M {QNd D {IN^ SR M {IN^ D {@NW SR
M zsNA D zvND SR M zvND D z{ND SR M z{ND D {GM~ SR M {GM~ D {NM~ SR
M {NM~ D {SNA SR M {SNA D {VND SR M z{ND D {GMz SR M {GMz D {QMz SR
M {QMz D {SM~ SR M {SM~ D {VND SR M {VND D {VNK SR
M GmrM D IAoA D JUlR D Kii| D L}g| D NQfO D Oedr D Pzce D RNbc D Sbak
D Tv`| D VJ`S D W^_n D Xr_M D ZF^m D [Z^N D \n]n D ^B]M D _V\j D `j\D
D a~[[ D cSZm D dgY| D e{YH D gOXO D hcWS D iwVT D kKUR D l_TO D msSJ
D oGRF D p[QB D qoPA D sCOD D tXNL D ulM\ D w@Lt D xTLX SR
M y~L? D ywL{ SR M ywL{ D yrLr SR M yrLr D yoLa SR M yoLa D yoLX SR
M yoLX D yrLH SR M yrLH D ywK~ SR M ywK~ D y~K{ SR M y~K{ D zCK{ SR
M zCK{ D zJK~ SR M zJK~ D zOLH SR M zOLH D zQLX SR M zQLX D zQLa SR
M zQLa D zOLr SR M zOLr D zJL{ SR M zJL{ D zCL? SR M zCL? D y~L? SR
M y~L? D yyL{ SR M yyL{ D ywLx SR M ywLx D ytLr SR M ytLr D yrLa SR
M yrLa D yrLX SR M yrLX D ytLH SR M ytLH D ywLA SR M ywLA D yyK~ SR
M yyK~ D y~K{ SR M zCK{ D zHK~ SR M zHK~ D zJLA SR M zJLA D zLLH SR
M zLLH D zOLX SR M zOLX D zOLa SR M zOLa D zLLr SR M zLLr D zJLx SR
M zJLx D zHL{ SR M zHL{ D zCL? SR M zbLA D z`K~ SR M z`K~ D zbK{ SR
M zbK{ D zeK~ SR M zeK~ D zbLA SR M zvLu D zxLr SR M zxLr D zvLn SR
M zvLn D zsLr SR M zsLr D zsLu SR M zsLu D zxL{ SR M zxL{ D {@L? SR
M {@L? D {IL? SR M {IL? D {QL{ SR M {QL{ D {SLu SR M {SLu D {SLk SR
M {SLk D {QLe SR M {QLe D {ILa SR M {ILa D {BLa SR M {IL? D {NL{ SR
M {NL{ D {QLu SR M {QLu D {QLk SR M {QLk D {NLe SR M {NLe D {ILa SR
M {ILa D {NL^ SR M {NL^ D {SLX SR M {SLX D {VLQ SR M {VLQ D {VLH SR
M {VLH D {SLA SR M {SLA D {QK~ SR M {QK~ D {IK{ SR M {IK{ D {@K{ SR
M {@K{ D zxK~ SR M zxK~ D zvLA SR M zvLA D zsLH SR M zsLH D zsLK SR
M zsLK D zvLN SR M zvLN D zxLK SR M zxLK D zvLH SR M {QL[ D {SLQ SR
M {SLQ D {SLH SR M {SLH D {QLA SR M {QLA D {NK~ SR M {NK~ D {IK{ SR
M Gmoa D IAlW D JUij D KigU D L}eV D NQck D OebQ D PzaE D RN`F D Sb_P
D Tv^c D VJ]| D W^]Y D Xr\z D ZF\\ D [Z[? D \n[a D ^B[A D _VZ` D `jY{
D a~YS D cSXg D dgWw D e{WC D gOVK D hcUP D iwTQ D kKSP D l_RM D msQI
D oGPD D p[OA D qoN@ D sCMD D tXLL D ulK\ D w@Ju D xTJY SR
M y~J? D ywJ| SR M ywJ| D yrJr SR M yrJr D yoJb SR M yoJb D yoJX SR
M yoJX D yrJH SR M yrJH D ywI~ SR M ywI~ D y~I{ SR M y~I{ D zCI{ SR
M zCI{ D zJI~ SR M zJI~ D zOJH SR M zOJH D zQJX SR M zQJX D zQJb SR
M zQJb D zOJr SR M zOJr D zJJ| SR M zJJ| D zCJ? SR M zCJ? D y~J? SR
M y~J? D yyJ| SR M yyJ| D ywJx SR M ywJx D ytJr SR M ytJr D yrJb SR
M yrJb D yrJX SR M yrJX D ytJH SR M ytJH D ywJB SR M ywJB D yyI~ SR
M yyI~ D y~I{ SR M zCI{ D zHI~ SR M zHI~ D zJJB SR M zJJB D zLJH SR
M zLJH D zOJX SR M zOJX D zOJb SR M zOJb D zLJr SR M zLJr D zJJx SR
M zJJx D zHJ| SR M zHJ| D zCJ? SR M zbJB D z`I~ SR M z`I~ D zbI{ SR
M zbI{ D zeI~ SR M zeI~ D zbJB SR M {IJx D {II{ SR M {LJ? D {LI{ SR
M {LJ? D zqJN SR M zqJN D {XJN SR M {BI{ D {SI{ SR
M Gmly D IAiq D JUgE D Kidq D L}bu D NQaL D Oe_s D Pz^i D RN]l D Sb\x
D Tv\M D VJ[h D W^[G D XrZi D ZFZM D [ZYq D \nYU D ^BXw D _VXW D `jWs
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%PSKOpenWorkStation
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FMENDEPSF
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%%BeginDocument: /pongo/data2/drs/ghrs/handbook/ih5/figs/mirror_a1.epsi
%!PS-Adobe-2.0 EPSF-1.2
%%BoundingBox: 43 29 576 730
%!PS-Adobe-1.0
%%Creator: PSIKern - An IRAF GKI Translator
%%CreationDate: Thu 15:35:52 28-Apr-94
%%DocumentFonts: (atend)
%%Pages: (atend)
%%BoundingBox: 28 28 583 763
%%EndComments
/MAXNDC 4095 def /PageSizeXMeter 0.2594 def /PageSizeYMeter 0.1959 def
/PageOffXMeter 0.01 def /PageOffYMeter 0.01 def
/PortraitMode false def /PortraitRotation 0. def
/LandScapeRotation 90. def /GT_LEFT 2 def /GT_RIGHT 3 def
/GT_TOP 6 def /GT_BOTTOM 7 def /GT_UP 4 def /GT_DOWN 5 def
/GT_CENTER 1 def /RF /Times-Roman def /GF /Symbol def
/IF /Times-Italic def /BF /Times-Bold def /DASH 49 def /DOT 4 def
/SPACE 24 def

% How to define things.
/BD { bind def } bind def
/LD { load def } bind def

% Constants
/yes true def
/no false def

% Define some shorthand instructions.
/GRS /grestore LD
/GS /gsave LD
/MK /mark LD
/R /restore LD
/S /save LD
/SH /showpage LD
/SW /setlinewidth LD

% Measurement conversions.
/PointperMeter 2834.64 def
/MonoScale .7 def

% SR: Set current path to page: - -> -
/SR { currentpoint stroke moveto } BD

% CL: CLear the page: - -> -
/CL { restore showpage grestore gsave save } BD

% RC: Read Coordinates: string -> x y
/RC {
currentfile read pop 8#77 and 6 bitshift
currentfile read pop 8#77 and or
currentfile read pop 8#77 and 6 bitshift
currentfile read pop 8#77 and or
} BD

% DO - Determine Offset: length -> offset
/DO { DS dup 0 eq { pop pop 0 } { mod } ifelse } BD

% M: Move: M string -> -
% Move to a point and clear length of path.
/M { RC moveto CT OF setdash } BD

% D: Draw: D string -> -
% This also calculates the length of the current path.
/OF 0 def
/D { RC DS 0 ne { 2 copy currentpoint exch 4 1 roll sub dup mul 3 1 roll
sub dup mul add sqrt round OF add cvi DO /OF exch store } if lineto
} BD

% Character/Font definitions.

% FS -- Define the current font size: xsize ysize FS -
/FontXSize 0 def /FontYSize 0 def /NewFont true def
/FS { /FontYSize exch MonoScale mul store /FontXSize exch MonoScale mul store
/NewFont true store } BD

% PH -- Set the current path: path PH -
/Path 0 def
/PH { /Path exch store } BD

% PA -- Set the path angle of the text: angle PA -
/Angle 0 def
/PA { 360 mod dup 0 lt { 360 add } if /Angle exch store /NewFont true store } BD

% HJ, VJ -- Set Horizontal/Verticle Justification: just HJ/VJ -
/HorzJust 0 def /VertJust 0 def
/HJ { /HorzJust exch store } BD /VJ { /VertJust exch store } BD

% VT -- Use mono- or variable-spaced fonts: flag VT -
/VT true def
/VT { /Variable exch store } BD

% SetFont -- Make the required font the default: font SetFont -
% Note scale factor- This is to fill out monospaced better and match other
% IRAF output.
/Font () def
/FontMatrix matrix def
/SetFont {
dup Font ne NewFont or
{ dup /Font exch store findfont
Angle matrix rotate FontXSize MonoScale div FontYSize MonoScale div
matrix scale matrix concatmatrix makefont setfont Angle matrix rotate
FontXSize FontYSize matrix scale matrix concatmatrix /FontMatrix exch
store
}
{ pop } ifelse /NewFont false store
} BD

% StringWidth -- Determine path length of string: string StringWidth - xs ys
/StringWidth { Path GT_RIGHT eq Variable and { stringwidth }
{ Path GT_RIGHT eq { length } { pop 1 } ifelse 0 FontMatrix transform }
ifelse
} BD

% MonoShow -- Write the string out in mono-spaced: string MonoShow -
/MonoShow {
/t 1 string def 1 0 FontMatrix transform
/dy exch def /dx exch def Path GT_RIGHT eq { /mx dx def /my dy def }
{ 0 1 FontMatrix transform /my exch def /mx exch def } ifelse
{ t 0 3 -1 roll put t dup stringwidth dy exch sub 2 div exch dx exch
sub 2 div exch gsave rmoveto show grestore mx my rmoveto
} forall
} BD

% WS -- Draw the string: string font string ... DS -
/*WSDict 13 dict def
/WS { *WSDict begin
counttomark 2 idiv dup dup array /FontArray exch def
array /StringArray exch def 1 sub /NStrings exch def

NStrings -1 0 {
dup 4 1 roll exch StringArray 3 1 roll put FontArray 3 1 roll put
} for
pop

/XSize 0 def /YSize 0 def /NChars 0 def
0 1 NStrings {
dup FontArray exch get SetFont StringArray exch get dup
length NChars add /NChars exch def StringWidth
YSize add /YSize exch def XSize add /XSize exch def
} for

/TAngle HorzJust GT_RIGHT eq
{ Angle 180 add dup 360 ge { 360 sub } if } { Angle } ifelse def
0 TAngle 180 le HorzJust GT_CENTER eq or
{ Angle sin FontYSize mul Path GT_UP eq { NChars mul } if add } if
TAngle 90 ge TAngle 270 le and HorzJust GT_CENTER eq or
{ Path GT_RIGHT eq { XSize } { Angle cos FontXSize mul } ifelse sub } if
HorzJust GT_CENTER eq { .5 mul } if

/TAngle
VertJust GT_TOP eq { Angle 180 sub dup 0 lt { 360 add } if } { Angle } ifelse
def
0 TAngle 90 ge TAngle 270 le and VertJust GT_CENTER eq or
{ Angle cos FontYSize mul Path GT_UP eq { NChars mul } if sub } if
TAngle 180 ge TAngle 360 le and VertJust GT_CENTER eq or
{ Path GT_RIGHT eq { YSize } { Angle sin FontXSize mul } ifelse sub } if
VertJust GT_CENTER eq { .5 mul } if
rmoveto

0 1 NStrings {
dup FontArray exch get SetFont StringArray exch get
Path GT_RIGHT eq Variable and { show } { MonoShow } ifelse
} for

end
} BD

% Define the DASHED, DOTTED, DOTDASH patterns.
/DS 0 def
/LPS {
/OF 0 store /DS 0 store 0 array
} BD
/LPD {
/OF 0 store DASH SPACE 2 copy add /DS exch store 2 array astore
} BD
/LPP {
/OF 0 store DOT SPACE 2 copy add /DS exch store 2 array astore
} BD
/LDD {
/OF 0 store DOT SPACE DASH SPACE 4 copy add add add /DS exch store
4 array astore
} BD

% LT - Set Line Type - array -> -
/CT { currentdash pop } BD
/LT { /CT exch store /OF 0 store } BD

% SC - Set Color: color -> -
/*SCDict 1 dict def
/SC { *SCDict begin
1 sub /color exch def
GR color get 255 div GG color get 255 div GB color get 255 div setrgbcolor
end
} BD

% MI - Make Image LUT: table-name size MI hexstring -> -
/MI { currentfile exch string readhexstring pop def } BD

% Define the graphics color lookup table.
/GR 16 MI 00FFFF0000FF00FFFFB0FFF0D940F0F5
/GG 16 MI 00FF00FF00FFFF0080D0A6E670E082DE
/GB 16 MI 00FF0000FF00FFFF4F61008CD6D1EFB3

% Render an image when no image LUT has been define.
/DefaultGrey {
{ currentfile inarr readhexstring pop } image
} BD

% ColorImage - Produce an image by indexing into the Image Lookup Table.
% There are two versions of this code- one for PostScript that has
% the colorimage operator and one that doesn't. If the PostScript doesn't
% have colorimage, it is assumed that it can only produce black & white,
% in which the Image LUT is combined to produce a single grey which is
% then used as the image for the image operator.
/colorimage where
{ pop
/ColorImage {
{ currentfile inarr readhexstring pop dup /inarr exch def
length 3 mul string /oarr exch def
0 1 inarr length 1 sub
{ /iindex exch def
/oindex iindex 3 mul def
oarr oindex IR inarr iindex get get put
oarr oindex 1 add IG inarr iindex get get put
oarr oindex 2 add IB inarr iindex get get put
} for
oarr
}
false 3 colorimage
} BD
}
{ /ColorImage {
{ currentfile inarr readhexstring pop dup /inarr exch def
length string /oarr exch def
0 1 inarr length 1 sub
{ /iindex exch def
oarr iindex
IR inarr iindex get get 0.3 mul
IG inarr iindex get get 0.59 mul
IB inarr iindex get get 0.11 mul
add add round cvi dup 255 gt { pop 255 } if
put
} for
oarr
}
image
} BD
}
ifelse

% PC: Put Cellarray: width height bitspersample matrix -> -
/*PCdict 10 dict def
/PC {
*PCdict begin
4 -1 roll dup /inarr exch string def 4 1 roll
/IR where {pop ColorImage} {DefaultGrey} ifelse
end
} BD

% Define the Hatch (fill area) styles. H1 and H2 are handled internally
% by PSIKern. Feel free to define more; there is no limit.
/H3 <8888888888888888> def
/H4 def
/H5 <8844221188442211> def
/H6 <1122448811224488> def

% Setup for fill patterns. This whole section of code is taken almost
% directly from _PostScript Language: Tutorial and Cookbook_, Adobe Systems,
% 1986 (the blue book).
/setuserscreendict 22 dict def
setuserscreendict begin
/tempctm matrix def
/temprot matrix def
/tempscale matrix def

/concatprocs
{ /proc2 exch cvlit def
/proc1 exch cvlit def
/newproc proc1 length proc2 length add
array def
newproc 0 proc1 putinterval
newproc proc1 length proc2 putinterval
newproc cvx
} def

/resmatrix matrix def
/findresolution
{ 72 0 resmatrix defaultmatrix dtransform
/yres exch def /xres exch def
xres dup mul yres dup mul add sqrt
} def
end

/setuserscreen
{ setuserscreendict begin
/spotfunction exch def
/screenangle exch def
/cellsize exch def

/m tempctm currentmatrix def
/rm screenangle temprot rotate def
/sm cellsize dup tempscale scale def

sm rm m m concatmatrix m concatmatrix pop
1 0 m dtransform /y1 exch def /x1 exch def

/veclength x1 dup mul y1 dup mul add sqrt def
/frequency findresolution veclength div def

/newscreenangle y1 x1 atan def

m 2 get m 1 get mul m 0 get m 3 get mul sub
0 gt
{ {neg} /spotfunction load concatprocs
/spotfunction exch def
} if

frequency newscreenangle /spotfunction load
setscreen
end
} def

/setpatterndict 18 dict def
setpatterndict begin
/bitison
{ /ybit exch def /xbit exch def
/bytevalue bstring ybit bwidth mul xbit 8 idiv
add get def

/mask 1 7 xbit 8 mod sub bitshift def
bytevalue mask and 0 ne
} def
end

/bitpatternspotfunction
{ setpatterndict begin
/y exch def /x exch def

/xindex x 1 add 2 div bpside mul cvi def
/yindex y 1 add 2 div bpside mul cvi def

xindex yindex bitison
{ /onbits onbits 1 add def 1 }
{ /offbits offbits 1 add def 0 }
ifelse
end
} def

/setpattern
{ setpatterndict begin
/cellsz exch def
/angle exch def
/bwidth exch def
/bpside exch def
/bstring exch def

/onbits 0 def /offbits 0 def
cellsz angle /bitpatternspotfunction load
setuserscreen
{ } settransfer
offbits offbits onbits add div setgray
end
} def

% SP: Set Pattern: pattern -> -
/SP { 8 1 0 MAXNDC 100 div setpattern } BD

% FI: Fill with Pattern: - -> -
/FI { fill grestore } BD

% Set the transformation matrix.
PointperMeter dup scale
PageOffXMeter
PortraitMode not
{ PageSizeYMeter add }
if
PageOffYMeter translate
PortraitMode
{ PortraitRotation rotate }
{ LandScapeRotation rotate}
ifelse
PageSizeXMeter MAXNDC div PageSizeYMeter MAXNDC div scale
1 setlinejoin 1 setlinecap

% Save the current graphics state (to restore after showpage) and the
% VM state to recover after a showpage.
GS S

%%EndProlog
%PSKOpenWorkStation
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M NoDW D NrD[ SR M NrD[ D NoD_ SR M OGE\ D OJEX SR M OJEX D OGET SR
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M OJEh D OSEl SR M OSEl D O`El SR M O`El D OiEh SR M OiEh D OlEd SR
M OlEd D OoE\ SR M OoE\ D OoET SR M OoET D OlEL SR M OlEL D OcEC SR
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M ODDc D ODDW SR M O`El D OfEh SR M OfEh D OiEd SR M OiEd D OlE\ SR
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M VHD[ D VNDg SR M VNDg D VQD{ SR M VQD{ D VQEG SR M VQEG D VNE\ SR
M VNE\ D VHEh SR M VHEh D U~El SR M U~El D UxEl SR M UxEl D UrEh SR
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M UiD{ D UlDg SR M UlDg D UoD_ SR M UoD_ D UrD[ SR M UrD[ D UxDW SR
M U~DW D VED[ SR M VED[ D VHD_ SR M VHD_ D VKDg SR M VKDg D VND{ SR
M VND{ D VNEG SR M VNEG D VKE\ SR M VKE\ D VHEd SR M VHEd D VEEh SR
M VEEh D U~El SR M \?El D \vEh SR M \vEh D \pE\ SR M \pE\ D \mEG SR
M \mEG D \mD{ SR M \mD{ D \pDg SR M \pDg D \vD[ SR M \vD[ D \?DW SR
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M ]WD{ D ]WEG SR M ]WEG D ]TE\ SR M ]TE\ D ]NEh SR M ]NEh D ]EEl SR
M ]EEl D \?El SR M \?El D \yEh SR M \yEh D \vEd SR M \vEd D \sE\ SR
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M mwDW D m}DW SR M m}DW D nFD[ SR M nFD[ D nLDc SR M nLDc D nODo SR
M nODo D nODs SR M nODs D nLD? SR M nLD? D nFEG SR M nFEG D m}EL SR
M m}EL D mzEL SR M mzEL D mqEG SR M mqEG D mkD? SR M mkD? D mhDs SR
M mzEl D mtEh SR M mtEh D mnE` SR M mnE` D mkEX SR M mkEX D mhEG SR
M mhEG D mhDo SR M mhDo D mkDc SR M mkDc D mqD[ SR M mqD[ D mwDW SR
M m}DW D nCD[ SR M nCD[ D nIDc SR M nIDc D nLDo SR M nLDo D nLDs SR
M nLDs D nID? SR M nID? D nCEG SR M nCEG D m}EL SR M tSEl D tJEh SR
M tJEh D tDE\ SR M tDE\ D t@EG SR M t@EG D t@D{ SR M t@D{ D tDDg SR
M tDDg D tJD[ SR M tJD[ D tSDW SR M tSDW D tYDW SR M tYDW D tbD[ SR
M tbD[ D thDg SR M thDg D tkD{ SR M tkD{ D tkEG SR M tkEG D thE\ SR
M thE\ D tbEh SR M tbEh D tYEl SR M tYEl D tSEl SR M tSEl D tMEh SR
M tMEh D tJEd SR M tJEd D tGE\ SR M tGE\ D tDEG SR M tDEG D tDD{ SR
M tDD{ D tGDg SR M tGDg D tJD_ SR M tJD_ D tMD[ SR M tMD[ D tSDW SR
M tYDW D t_D[ SR M t_D[ D tbD_ SR M tbD_ D teDg SR M teDg D thD{ SR
M thD{ D thEG SR M thEG D teE\ SR M teE\ D tbEd SR M tbEd D t_Eh SR
M t_Eh D tYEl SR M u@D_ D t}D[ SR M t}D[ D u@DW SR M u@DW D uDD[ SR
M uDD[ D u@D_ SR M ueEl D u\Eh SR M u\Eh D uYE` SR M uYE` D uYET SR
M uYET D u\EL SR M u\EL D ueEG SR M ueEG D uqEG SR M uqEG D uzEL SR
M uzEL D u}ET SR M u}ET D u}E` SR M u}E` D uzEh SR M uzEh D uqEl SR
M uqEl D ueEl SR M ueEl D u_Eh SR M u_Eh D u\E` SR M u\E` D u\ET SR
M u\ET D u_EL SR M u_EL D ueEG SR M uqEG D uwEL SR M uwEL D uzET SR
M uzET D uzE` SR M uzE` D uwEh SR M uwEh D uqEl SR M ueEG D u\EC SR
M u\EC D uYD? SR M uYD? D uVDw SR M uVDw D uVDg SR M uVDg D uYD_ SR
M uYD_ D u\D[ SR M u\D[ D ueDW SR M ueDW D uqDW SR M uqDW D uzD[ SR
M uzD[ D u}D_ SR M u}D_ D v@Dg SR M v@Dg D v@Dw SR M v@Dw D u}D? SR
M u}D? D uzEC SR M uzEC D uqEG SR M ueEG D u_EC SR M u_EC D u\D? SR
M u\D? D uYDw SR M uYDw D uYDg SR M uYDg D u\D_ SR M u\D_ D u_D[ SR
M u_D[ D ueDW SR M uqDW D uwD[ SR M uwD[ D uzD_ SR M uzD_ D u}Dg SR
M u}Dg D u}Dw SR M u}Dw D uzD? SR M uzD? D uwEC SR M uwEC D uqEG SR
M |fE\ D |lE` SR M |lE` D |uEl SR M |uEl D |uDW SR M |rEh D |rDW SR
M |fDW D }ADW SR M FY|r D |r|r SR M FY|r D FY{r SR M HU|r D HU|R SR
M JQ|r D JQ|R SR M LN|r D LN|R SR M NJ|r D NJ{r SR M PF|r D PF|R SR
M RC|r D RC|R SR M S?|r D S?|R SR M U{|r D U{{r SR M Wx|r D Wx|R SR
M Yt|r D Yt|R SR M [p|r D [p|R SR M ]m|r D ]m{r SR M _i|r D _i|R SR
M ae|r D ae|R SR M cb|r D cb|R SR M e^|r D e^{r SR M gZ|r D gZ|R SR
M iV|r D iV|R SR M kS|r D kS|R SR M mO|r D mO{r SR M oK|r D oK|R SR
M qH|r D qH|R SR M sD|r D sD|R SR M u@|r D u@{r SR M v}|r D v}|R SR
M xy|r D xy|R SR M zu|r D zu|R SR M |r|r D |r{r SR M FYFY D FY|r SR
M FYFY D FyFY SR M FYFY D GYFY SR M FYH\ D FyH\ SR M FYIh D FyIh SR
M FYJ_ D FyJ_ SR M FYKI D FyKI SR M FYKk D FyKk SR M FYLI D FyLI SR
M FYLb D FyLb SR M FYLx D FyLx SR M FYML D FyML SR M FYML D GYML SR
M FYOO D FyOO SR M FYP\ D FyP\ SR M FYQR D FyQR SR M FYQ| D FyQ| SR
M FYR^ D FyR^ SR M FYR| D FyR| SR M FYSU D FySU SR M FYSk D FySk SR
M FYS? D FyS? SR M FYS? D GYS? SR M FYVB D FyVB SR M FYWO D FyWO SR
M FYXE D FyXE SR M FYXo D FyXo SR M FYYR D FyYR SR M FYYo D FyYo SR
M FYZH D FyZH SR M FYZ^ D FyZ^ SR M FYZr D FyZr SR M FYZr D GYZr SR
M FY\u D Fy\u SR M FY^B D Fy^B SR M FY^x D Fy^x SR M FY_b D Fy_b SR
M FY`E D Fy`E SR M FY`b D Fy`b SR M FY`{ D Fy`{ SR M FYaQ D FyaQ SR
M FYae D Fyae SR M FYae D GYae SR M FYch D Fych SR M FYdu D Fydu SR
M FYek D Fyek SR M FYfU D FyfU SR M FYfx D Fyfx SR M FYgU D FygU SR
M FYgn D Fygn SR M FYhD D FyhD SR M FYhX D FyhX SR M FYhX D GYhX SR
M FYj[ D Fyj[ SR M FYkh D Fykh SR M FYl^ D Fyl^ SR M FYmH D FymH SR
M FYmk D Fymk SR M FYnH D FynH SR M FYna D Fyna SR M FYnw D Fynw SR
M FYoK D FyoK SR M FYoK D GYoK SR M FYqN D FyqN SR M FYr[ D Fyr[ SR
M FYsQ D FysQ SR M FYs| D Fys| SR M FYt^ D Fyt^ SR M FYt{ D Fyt{ SR
M FYuT D FyuT SR M FYuk D Fyuk SR M FYu? D Fyu? SR M FYu? D GYu? SR
M FYxA D FyxA SR M FYyN D FyyN SR M FYzD D FyzD SR M FYzo D Fyzo SR
M FY{Q D Fy{Q SR M FY{n D Fy{n SR M FY|G D Fy|G SR M FY|^ D Fy|^ SR
M FY|r D Fy|r SR M FY|r D GY|r SR M BnFy D BtF} SR M BtF} D B}GI SR
M B}GI D B}Eu SR M BzGE D BzEu SR M BnEu D CIEu SR M CtGI D CkGE SR
M CkGE D CeFy SR M CeFy D CbFe SR M CbFe D CbFY SR M CbFY D CeFE SR
M CeFE D CkEy SR M CkEy D CtEu SR M CtEu D CzEu SR M CzEu D DCEy SR
M DCEy D DIFE SR M DIFE D DLFY SR M DLFY D DLFe SR M DLFe D DIFy SR
M DIFy D DCGE SR M DCGE D CzGI SR M CzGI D CtGI SR M CtGI D CnGE SR
M CnGE D CkGA SR M CkGA D ChFy SR M ChFy D CeFe SR M CeFe D CeFY SR
M CeFY D ChFE SR M ChFE D CkE} SR M CkE} D CnEy SR M CnEy D CtEu SR
M CzEu D D@Ey SR M D@Ey D DCE} SR M DCE} D DFFE SR M DFFE D DIFY SR
M DIFY D DIFe SR M DIFe D DFFy SR M DFFy D DCGA SR M DCGA D D@GE SR
M D@GE D CzGI SR M D[GZ D D|GZ SR M EIGm D EJGj SR M EJGj D EIGh SR
M EIGh D EGGj SR M EGGj D EGGm SR M EGGm D EIGr SR M EIGr D EJGt SR
M EJGt D EPGw SR M EPGw D EWGw SR M EWGw D E]Gt SR M E]Gt D E^Gr SR
M E^Gr D E`Gm SR M E`Gm D E`Gh SR M E`Gh D E^Gc SR M E^Gc D EYG^ SR
M EYG^ D EPGZ SR M EPGZ D ELGW SR M ELGW D EIGR SR M EIGR D EGGK SR
M EGGK D EGGD SR M EWGw D E[Gt SR M E[Gt D E]Gr SR M E]Gr D E^Gm SR
M E^Gm D E^Gh SR M E^Gh D E]Gc SR M E]Gc D EWG^ SR M EWG^ D EPGZ SR
M EGGI D EIGK SR M EIGK D ELGK SR M ELGK D EUGF SR M EUGF D E[GF SR
M E[GF D E^GI SR M E^GI D E`GK SR M ELGK D EUGD SR M EUGD D E]GD SR
M E]GD D E^GF SR M E^GF D E`GK SR M E`GK D E`GP SR M BnMl D BtMp SR
M BtMp D B}M| SR M B}M| D B}Lh SR M BzMx D BzLh SR M BnLh D CILh SR
M CtM| D CkMx SR M CkMx D CeMl SR M CeMl D CbMX SR M CbMX D CbML SR
M CbML D CeLx SR M CeLx D CkLl SR M CkLl D CtLh SR M CtLh D CzLh SR
M CzLh D DCLl SR M DCLl D DILx SR M DILx D DLML SR M DLML D DLMX SR
M DLMX D DIMl SR M DIMl D DCMx SR M DCMx D CzM| SR M CzM| D CtM| SR
M CtM| D CnMx SR M CnMx D CkMt SR M CkMt D ChMl SR M ChMl D CeMX SR
M CeMX D CeML SR M CeML D ChLx SR M ChLx D CkLp SR M CkLp D CnLl SR
M CnLl D CtLh SR M CzLh D D@Ll SR M D@Ll D DCLp SR M DCLp D DFLx SR
M DFLx D DIML SR M DIML D DIMX SR M DIMX D DFMl SR M DFMl D DCMt SR
M DCMt D D@Mx SR M D@Mx D CzM| SR M D[NM D D|NM SR M ELN` D EPNb SR
M EPNb D EUNj SR M EUNj D EUMw SR M ESNg D ESMw SR M ELMw D E]Mw SR
M ByT_ D B?Tc SR M B?Tc D CHTp SR M CHTp D CHS[ SR M CETk D CES[ SR
M ByS[ D CTS[ SR M C?Tp D CvTk SR M CvTk D CpT_ SR M CpT_ D ClTK SR
M ClTK D ClS? SR M ClS? D CpSk SR M CpSk D CvS_ SR M CvS_ D C?S[ SR
M C?S[ D DES[ SR M DES[ D DNS_ SR M DNS_ D DTSk SR M DTSk D DWS? SR
M DWS? D DWTK SR M DWTK D DTT_ SR M DTT_ D DNTk SR M DNTk D DETp SR
M DETp D C?Tp SR M C?Tp D CyTk SR M CyTk D CvTg SR M CvTg D CsT_ SR
M CsT_ D CpTK SR M CpTK D CpS? SR M CpS? D CsSk SR M CsSk D CvSc SR
M CvSc D CyS_ SR M CyS_ D C?S[ SR M DES[ D DKS_ SR M DKS_ D DNSc SR
M DNSc D DQSk SR M DQSk D DTS? SR M DTS? D DTTK SR M DTTK D DQT_ SR
M DQT_ D DNTg SR M DNTg D DKTk SR M DKTk D DETp SR M ERU] D ELUZ SR
M ELUZ D EIUS SR M EIUS D EGUG SR M EGUG D EGU@ SR M EGU@ D EITt SR
M EITt D ELTl SR M ELTl D ERTj SR M ERTj D EUTj SR M EUTj D E[Tl SR
M E[Tl D E^Tt SR M E^Tt D E`U@ SR M E`U@ D E`UG SR M E`UG D E^US SR
M E^US D E[UZ SR M E[UZ D EUU] SR M EUU] D ERU] SR M ERU] D ENUZ SR
M ENUZ D ELUX SR M ELUX D EJUS SR M EJUS D EIUG SR M EIUG D EIU@ SR
M EIU@ D EJTt SR M EJTt D ELTo SR M ELTo D ENTl SR M ENTl D ERTj SR
M EUTj D EYTl SR M EYTl D E[To SR M E[To D E]Tt SR M E]Tt D E^U@ SR
M E^U@ D E^UG SR M E^UG D E]US SR M E]US D E[UX SR M E[UX D EYUZ SR
M EYUZ D EUU] SR M By[S D B?[W SR M B?[W D CH[c SR M CH[c D CHZN SR
M CE[_ D CEZN SR M ByZN D CTZN SR M C?[c D Cv[_ SR M Cv[_ D Cp[S SR
M Cp[S D ClZ~ SR M ClZ~ D ClZr SR M ClZr D CpZ^ SR M CpZ^ D CvZR SR
M CvZR D C?ZN SR M C?ZN D DEZN SR M DEZN D DNZR SR M DNZR D DTZ^ SR
M DTZ^ D DWZr SR M DWZr D DWZ~ SR M DWZ~ D DT[S SR M DT[S D DN[_ SR
M DN[_ D DE[c SR M DE[c D C?[c SR M C?[c D Cy[_ SR M Cy[_ D Cv[[ SR
M Cv[[ D Cs[S SR M Cs[S D CpZ~ SR M CpZ~ D CpZr SR M CpZr D CsZ^ SR
M CsZ^ D CvZV SR M CvZV D CyZR SR M CyZR D C?ZN SR M DEZN D DKZR SR
M DKZR D DNZV SR M DNZV D DQZ^ SR M DQZ^ D DTZr SR M DTZr D DTZ~ SR
M DTZ~ D DQ[S SR M DQ[S D DN[[ SR M DN[[ D DK[_ SR M DK[_ D DE[c SR
M EL\F D EP\I SR M EP\I D EU\P SR M EU\P D EU[] SR M ES\M D ES[] SR
M EL[] D E][] SR M BybF D B?bJ SR M B?bJ D CHbV SR M CHbV D CHaA SR
M CEbR D CEaA SR M ByaA D CTaA SR M C?bV D CvbR SR M CvbR D CpbF SR
M CpbF D Claq SR M Claq D Clae SR M Clae D CpaQ SR M CpaQ D CvaE SR
M CvaE D C?aA SR M C?aA D DEaA SR M DEaA D DNaE SR M DNaE D DTaQ SR
M DTaQ D DWae SR M DWae D DWaq SR M DWaq D DTbF SR M DTbF D DNbR SR
M DNbR D DEbV SR M DEbV D C?bV SR M C?bV D CybR SR M CybR D CvbN SR
M CvbN D CsbF SR M CsbF D Cpaq SR M Cpaq D Cpae SR M Cpae D CsaQ SR
M CsaQ D CvaI SR M CvaI D CyaE SR M CyaE D C?aA SR M DEaA D DKaE SR
M DKaE D DNaI SR M DNaI D DQaQ SR M DQaQ D DTae SR M DTae D DTaq SR
M DTaq D DQbF SR M DQbF D DNbN SR M DNbN D DKbR SR M DKbR D DEbV SR
M EIby D EJbw SR M EJbw D EIbt SR M EIbt D EGbw SR M EGbw D EGby SR
M EGby D EIb~ SR M EIb~ D EJcA SR M EJcA D EPcC SR M EPcC D EWcC SR
M EWcC D E]cA SR M E]cA D E^b~ SR M E^b~ D E`by SR M E`by D E`bt SR
M E`bt D E^bp SR M E^bp D EYbk SR M EYbk D EPbf SR M EPbf D ELbc SR
M ELbc D EIb_ SR M EIb_ D EGbW SR M EGbW D EGbP SR M EWcC D E[cA SR
M E[cA D E]b~ SR M E]b~ D E^by SR M E^by D E^bt SR M E^bt D E]bp SR
M E]bp D EWbk SR M EWbk D EPbf SR M EGbU D EIbW SR M EIbW D ELbW SR
M ELbW D EUbS SR M EUbS D E[bS SR M E[bS D E^bU SR M E^bU D E`bW SR
M ELbW D EUbP SR M EUbP D E]bP SR M E]bP D E^bS SR M E^bS D E`bW SR
M E`bW D E`b\ SR M Byhy D B?h} SR M B?h} D CHiI SR M CHiI D CHgt SR
M CEiE D CEgt SR M Bygt D CTgt SR M C?iI D CviE SR M CviE D Cphy SR
M Cphy D Clhe SR M Clhe D ClhX SR M ClhX D CphD SR M CphD D Cvgx SR
M Cvgx D C?gt SR M C?gt D DEgt SR M DEgt D DNgx SR M DNgx D DThD SR
M DThD D DWhX SR M DWhX D DWhe SR M DWhe D DThy SR M DThy D DNiE SR
M DNiE D DEiI SR M DEiI D C?iI SR M C?iI D CyiE SR M CyiE D CviA SR
M CviA D Cshy SR M Cshy D Cphe SR M Cphe D CphX SR M CphX D CshD SR
M CshD D Cvg| SR M Cvg| D Cygx SR M Cygx D C?gt SR M DEgt D DKgx SR
M DKgx D DNg| SR M DNg| D DQhD SR M DQhD D DThX SR M DThX D DThe SR
M DThe D DQhy SR M DQhy D DNiA SR M DNiA D DKiE SR M DKiE D DEiI SR
M EIio D EJil SR M EJil D EIij SR M EIij D EGil SR M EGil D EGio SR
M EGio D EJit SR M EJit D EPiv SR M EPiv D EWiv SR M EWiv D E]it SR
M E]it D E^io SR M E^io D E^ig SR M E^ig D E]ic SR M E]ic D EWi` SR
M EWi` D ERi` SR M EWiv D E[it SR M E[it D E]io SR M E]io D E]ig SR
M E]ig D E[ic SR M E[ic D EWi` SR M EWi` D E[i^ SR M E[i^ D E^iY SR
M E^iY D E`iT SR M E`iT D E`iM SR M E`iM D E^iH SR M E^iH D E]iF SR
M E]iF D EWiC SR M EWiC D EPiC SR M EPiC D EJiF SR M EJiF D EIiH SR
M EIiH D EGiM SR M EGiM D EGiO SR M EGiO D EIiR SR M EIiR D EJiO SR
M EJiO D EIiM SR M E]i[ D E^iT SR M E^iT D E^iM SR M E^iM D E]iH SR
M E]iH D E[iF SR M E[iF D EWiC SR M Byol D B?op SR M B?op D CHo| SR
M CHo| D CHng SR M CEox D CEng SR M Byng D CTng SR M C?o| D Cvox SR
M Cvox D Cpol SR M Cpol D CloX SR M CloX D CloK SR M CloK D Cpnw SR
M Cpnw D Cvnk SR M Cvnk D C?ng SR M C?ng D DEng SR M DEng D DNnk SR
M DNnk D DTnw SR M DTnw D DWoK SR M DWoK D DWoX SR M DWoX D DTol SR
M DTol D DNox SR M DNox D DEo| SR M DEo| D C?o| SR M C?o| D Cyox SR
M Cyox D Cvot SR M Cvot D Csol SR M Csol D CpoX SR M CpoX D CpoK SR
M CpoK D Csnw SR M Csnw D Cvno SR M Cvno D Cynk SR M Cynk D C?ng SR
M DEng D DKnk SR M DKnk D DNno SR M DNno D DQnw SR M DQnw D DToK SR
M DToK D DToX SR M DToX D DQol SR M DQol D DNot SR M DNot D DKox SR
M DKox D DEo| SR M EWpd D EWov SR M EYpi D EYov SR M EYpi D EEpE SR
M EEpE D EbpE SR M ERov D E^ov SR M Byv_ D B?vc SR M B?vc D CHvo SR
M CHvo D CHuZ SR M CEvk D CEuZ SR M ByuZ D CTuZ SR M C?vo D Cvvk SR
M Cvvk D Cpv_ SR M Cpv_ D ClvK SR M ClvK D Clu? SR M Clu? D Cpuj SR
M Cpuj D Cvu^ SR M Cvu^ D C?uZ SR M C?uZ D DEuZ SR M DEuZ D DNu^ SR
M DNu^ D DTuj SR M DTuj D DWu? SR M DWu? D DWvK SR M DWvK D DTv_ SR
M DTv_ D DNvk SR M DNvk D DEvo SR M DEvo D C?vo SR M C?vo D Cyvk SR
M Cyvk D Cvvg SR M Cvvg D Csv_ SR M Csv_ D CpvK SR M CpvK D Cpu? SR
M Cpu? D Csuj SR M Csuj D Cvub SR M Cvub D Cyu^ SR M Cyu^ D C?uZ SR
M DEuZ D DKu^ SR M DKu^ D DNub SR M DNub D DQuj SR M DQuj D DTu? SR
M DTu? D DTvK SR M DTvK D DQv_ SR M DQv_ D DNvg SR M DNvg D DKvk SR
M DKvk D DEvo SR M EJw\ D EGwD SR M EGwD D EJwF SR M EJwF D EPwI SR
M EPwI D EUwI SR M EUwI D E[wF SR M E[wF D E^wB SR M E^wB D E`vz SR
M E`vz D E`vx SR M E`vx D E^vq SR M E^vq D E[vl SR M E[vl D EUvi SR
M EUvi D EPvi SR M EPvi D EJvl SR M EJvl D EIvn SR M EIvn D EGvs SR
M EGvs D EGvv SR M EGvv D EIvx SR M EIvx D EJvv SR M EJvv D EIvs SR
M EUwI D EYwF SR M EYwF D E]wB SR M E]wB D E^vz SR M E^vz D E^vx SR
M E^vx D E]vq SR M E]vq D EYvl SR M EYvl D EUvi SR M EJw\ D E]w\ SR
M EJwZ D ESwZ SR M ESwZ D E]w\ SR M By}R D B?}V SR M B?}V D CH}b SR
M CH}b D CH|M SR M CE}^ D CE|M SR M By|M D CT|M SR M C?}b D Cv}^ SR
M Cv}^ D Cp}R SR M Cp}R D Cl|~ SR M Cl|~ D Cl|r SR M Cl|r D Cp|^ SR
M Cp|^ D Cv|Q SR M Cv|Q D C?|M SR M C?|M D DE|M SR M DE|M D DN|Q SR
M DN|Q D DT|^ SR M DT|^ D DW|r SR M DW|r D DW|~ SR M DW|~ D DT}R SR
M DT}R D DN}^ SR M DN}^ D DE}b SR M DE}b D C?}b SR M C?}b D Cy}^ SR
M Cy}^ D Cv}Z SR M Cv}Z D Cs}R SR M Cs}R D Cp|~ SR M Cp|~ D Cp|r SR
M Cp|r D Cs|^ SR M Cs|^ D Cv|U SR M Cv|U D Cy|Q SR M Cy|Q D C?|M SR
M DE|M D DK|Q SR M DK|Q D DN|U SR M DN|U D DQ|^ SR M DQ|^ D DT|r SR
M DT|r D DT|~ SR M DT|~ D DQ}R SR M DQ}R D DN}Z SR M DN}Z D DK}^ SR
M DK}^ D DE}b SR M E]~H D E[~F SR M E[~F D E]~C SR M E]~C D E^~F SR
M E^~F D E^~H SR M E^~H D E]~M SR M E]~M D EY~O SR M EY~O D ES~O SR
M ES~O D EN~M SR M EN~M D EJ~H SR M EJ~H D EI~C SR M EI~C D EG}z SR
M EG}z D EG}k SR M EG}k D EI}d SR M EI}d D EL}_ SR M EL}_ D ER}\ SR
M ER}\ D EU}\ SR M EU}\ D E[}_ SR M E[}_ D E^}d SR M E^}d D E`}k SR
M E`}k D E`}m SR M E`}m D E^}u SR M E^}u D E[}z SR M E[}z D EU}| SR
M EU}| D ES}| SR M ES}| D EN}z SR M EN}z D EJ}u SR M EJ}u D EI}m SR
M ES~O D EP~M SR M EP~M D EL~H SR M EL~H D EJ~C SR M EJ~C D EI}z SR
M EI}z D EI}k SR M EI}k D EJ}d SR M EJ}d D EN}_ SR M EN}_ D ER}\ SR
M EU}\ D EY}_ SR M EY}_ D E]}d SR M E]}d D E^}k SR M E^}k D E^}m SR
M E^}m D E]}u SR M E]}u D EY}z SR M EY}z D EU}| SR M |rFY D |r|r SR
M |rFY D |RFY SR M |rFY D {rFY SR M |rH\ D |RH\ SR M |rIh D |RIh SR
M |rJ_ D |RJ_ SR M |rKI D |RKI SR M |rKk D |RKk SR M |rLI D |RLI SR
M |rLb D |RLb SR M |rLx D |RLx SR M |rML D |RML SR M |rML D {rML SR
M |rOO D |ROO SR M |rP\ D |RP\ SR M |rQR D |RQR SR M |rQ| D |RQ| SR
M |rR^ D |RR^ SR M |rR| D |RR| SR M |rSU D |RSU SR M |rSk D |RSk SR
M |rS? D |RS? SR M |rS? D {rS? SR M |rVB D |RVB SR M |rWO D |RWO SR
M |rXE D |RXE SR M |rXo D |RXo SR M |rYR D |RYR SR M |rYo D |RYo SR
M |rZH D |RZH SR M |rZ^ D |RZ^ SR M |rZr D |RZr SR M |rZr D {rZr SR
M |r\u D |R\u SR M |r^B D |R^B SR M |r^x D |R^x SR M |r_b D |R_b SR
M |r`E D |R`E SR M |r`b D |R`b SR M |r`{ D |R`{ SR M |raQ D |RaQ SR
M |rae D |Rae SR M |rae D {rae SR M |rch D |Rch SR M |rdu D |Rdu SR
M |rek D |Rek SR M |rfU D |RfU SR M |rfx D |Rfx SR M |rgU D |RgU SR
M |rgn D |Rgn SR M |rhD D |RhD SR M |rhX D |RhX SR M |rhX D {rhX SR
M |rj[ D |Rj[ SR M |rkh D |Rkh SR M |rl^ D |Rl^ SR M |rmH D |RmH SR
M |rmk D |Rmk SR M |rnH D |RnH SR M |rna D |Rna SR M |rnw D |Rnw SR
M |roK D |RoK SR M |roK D {roK SR M |rqN D |RqN SR M |rr[ D |Rr[ SR
M |rsQ D |RsQ SR M |rs| D |Rs| SR M |rt^ D |Rt^ SR M |rt{ D |Rt{ SR
M |ruT D |RuT SR M |ruk D |Ruk SR M |ru? D |Ru? SR M |ru? D {ru? SR
M |rxA D |RxA SR M |ryN D |RyN SR M |rzD D |RzD SR M |rzo D |Rzo SR
M |r{Q D |R{Q SR M |r{n D |R{n SR M |r|G D |R|G SR M |r|^ D |R|^ SR
M |r|r D |R|r SR M |r|r D {r|r SR
M @^Ub D @dUf SR M @dUf D @TUf SR M @TUf D @^Ub SR M @^Ub D @WUZ SR
M @WUZ D @TUN SR M @TUN D @TUF SR M @TUF D @WTz SR M @WTz D @^Tq SR
M @^Tq D @dTm SR M @dTm D @mTi SR M @mTi D @|Ti SR M @|Ti D AETm SR
M AETm D AKTq SR M AKTq D AQTz SR M AQTz D ATUF SR M ATUF D ATUN SR
M ATUN D AQUZ SR M AQUZ D AKUb SR M AKUb D AEUf SR M @TUF D @WT~ SR
M @WT~ D @^Tv SR M @^Tv D @dTq SR M @dTq D @mTm SR M @mTm D @|Tm SR
M @|Tm D AETq SR M AETq D AKTv SR M AKTv D AQT~ SR M AQT~ D ATUF SR
M @jVV D @mVJ SR M @mVJ D @sVB SR M @sVB D @|U~ SR M @|U~ D ABU~ SR
M ABU~ D AKVB SR M AKVB D AQVJ SR M AQVJ D ATVV SR M ATVV D ATV^ SR
M ATV^ D AQVk SR M AQVk D AKVs SR M AKVs D ABVw SR M ABVw D @|Vw SR
M @|Vw D @sVs SR M @sVs D @mVk SR M @mVk D @jV^ SR M @jV^ D @jVV SR
M @jVV D @mVN SR M @mVN D @sVF SR M @sVF D @|VB SR M @|VB D ABVB SR
M ABVB D AKVF SR M AKVF D AQVN SR M AQVN D ATVV SR M ATV^ D AQVf SR
M AQVf D AKVo SR M AKVo D ABVs SR M ABVs D @|Vs SR M @|Vs D @sVo SR
M @sVo D @mVf SR M @mVf D @jV^ SR M @jWW D AKWW SR M AKWW D AQW[ SR
M AQW[ D ATWg SR M ATWg D ATWo SR M ATWo D AQW{ SR M AQW{ D AKXC SR
M @jW[ D AKW[ SR M AKW[ D AQW_ SR M AQW_ D ATWg SR M @jXC D ATXC SR
M @jXG D ATXG SR M @jWK D @jW[ SR M @jWw D @jXG SR M ATXC D ATXS SR
M @jXp D ATXp SR M @jXt D ATXt SR M @sXt D @mX| SR M @mX| D @jYH SR
M @jYH D @jYP SR M @jYP D @mY\ SR M @mY\ D @sY` SR M @sY` D ATY` SR
M @jYP D @mYX SR M @mYX D @sY\ SR M @sY\ D ATY\ SR M @jXd D @jXt SR
M ATXd D ATY@ SR M ATYP D ATYl SR M @TZH D AHZH SR M AHZH D AQZM SR
M AQZM D ATZU SR M ATZU D ATZ] SR M ATZ] D AQZe SR M AQZe D AKZi SR
M @TZM D AHZM SR M AHZM D AQZQ SR M AQZQ D ATZU SR M @jY| D @jZ] SR
M @T\N D AT\N SR M @T\R D AT\R SR M @T\A D @T\r SR M @T\r D @W\~ SR
M @W\~ D @Z]B SR M @Z]B D @a]F SR M @a]F D @g]F SR M @g]F D @m]B SR
M @m]B D @p\~ SR M @p\~ D @s\r SR M @s\r D @s\R SR M @T\r D @W\z SR
M @W\z D @Z\~ SR M @Z\~ D @a]B SR M @a]B D @g]B SR M @g]B D @m\~ SR
M @m\~ D @p\z SR M @p\z D @s\r SR M AT\A D AT\^ SR M @s\j D AN\z SR
M AN\z D AT]B SR M AT]B D AT]J SR M AT]J D AN]N SR M @s\j D @y\r SR
M @y\r D AT]B SR M @p]f D @s]f SR M @s]f D @s]b SR M @s]b D @p]b SR
M @p]b D @m]f SR M @m]f D @j]n SR M @j]n D @j]? SR M @j]? D @m^G SR
M @m^G D @p^K SR M @p^K D @v^O SR M @v^O D AK^O SR M AK^O D AQ^S SR
M AQ^S D AT^W SR M @p^K D AK^K SR M AK^K D AQ^O SR M AQ^O D AT^W SR
M AT^W D AT^[ SR M @v^K D @y^G SR M @y^G D @|]n SR M @|]n D @?]b SR
M @?]b D AE]^ SR M AE]^ D AK]^ SR M AK]^ D AQ]b SR M AQ]b D AT]n SR
M AT]n D AT]z SR M AT]z D AQ^C SR M AQ^C D AK^K SR M @|]n D @?]f SR
M @?]f D AE]b SR M AE]b D AK]b SR M AK]b D AQ]f SR M AQ]f D AT]n SR
M @T^w D AH^w SR M AH^w D AQ^{ SR M AQ^{ D AT_C SR M AT_C D AT_K SR
M AT_K D AQ_S SR M AQ_S D AK_W SR M @T^{ D AH^{ SR M AH^{ D AQ^? SR
M AQ^? D AT_C SR M @j^k D @j_K SR M @|_p D @|`` SR M @|`` D @v`` SR
M @v`` D @p`\ SR M @p`\ D @m`X SR M @m`X D @j`P SR M @j`P D @j`D SR
M @j`D D @m_x SR M @m_x D @s_p SR M @s_p D @|_k SR M @|_k D AB_k SR
M AB_k D AK_p SR M AK_p D AQ_x SR M AQ_x D AT`D SR M AT`D D AT`L SR
M AT`L D AQ`X SR M AQ`X D AK`` SR M @|`\ D @s`\ SR M @s`\ D @m`X SR
M @j`D D @m_| SR M @m_| D @s_t SR M @s_t D @|_p SR M @|_p D AB_p SR
M AB_p D AK_t SR M AK_t D AQ_| SR M AQ_| D AT`D SR M @Hba D @NbY SR
M @NbY D @WbQ SR M @WbQ D @dbI SR M @dbI D @sbE SR M @sbE D @?bE SR
M @?bE D ANbI SR M ANbI D AZbQ SR M AZbQ D AdbY SR M AdbY D Ajba SR
M @NbY D @ZbQ SR M @ZbQ D @dbM SR M @dbM D @sbI SR M @sbI D @?bI SR
M @?bI D ANbM SR M ANbM D AWbQ SR M AWbQ D AdbY SR M @scj D @vcf SR
M @vcf D @ycj SR M @ycj D @vcn SR M @vcn D @scn SR M @scn D @mcf SR
M @mcf D @jc^ SR M @jc^ D @jcQ SR M @jcQ D @mcE SR M @mcE D @sb} SR
M @sb} D @|by SR M @|by D ABby SR M ABby D AKb} SR M AKb} D AQcE SR
M AQcE D ATcQ SR M ATcQ D ATcZ SR M ATcZ D AQcf SR M AQcf D AKcn SR
M @jcQ D @mcI SR M @mcI D @scA SR M @scA D @|b} SR M @|b} D ABb} SR
M ABb} D AKcA SR M AKcA D AQcI SR M AQcI D ATcQ SR M @jd^ D @mdR SR
M @mdR D @sdJ SR M @sdJ D @|dF SR M @|dF D ABdF SR M ABdF D AKdJ SR
M AKdJ D AQdR SR M AQdR D ATd^ SR M ATd^ D ATdf SR M ATdf D AQdr SR
M AQdr D AKdz SR M AKdz D ABd~ SR M ABd~ D @|d~ SR M @|d~ D @sdz SR
M @sdz D @mdr SR M @mdr D @jdf SR M @jdf D @jd^ SR M @jd^ D @mdV SR
M @mdV D @sdN SR M @sdN D @|dJ SR M @|dJ D ABdJ SR M ABdJ D AKdN SR
M AKdN D AQdV SR M AQdV D ATd^ SR M ATdf D AQdn SR M AQdn D AKdv SR
M AKdv D ABdz SR M ABdz D @|dz SR M @|dz D @sdv SR M @sdv D @mdn SR
M @mdn D @jdf SR M @je_ D AKe_ SR M AKe_ D AQec SR M AQec D ATeo SR
M ATeo D ATew SR M ATew D AQfC SR M AQfC D AKfK SR M @jec D AKec SR
M AKec D AQeg SR M AQeg D ATeo SR M @jfK D ATfK SR M @jfO D ATfO SR
M @jeR D @jec SR M @je? D @jfO SR M ATfK D ATf[ SR M @jfw D ATfw SR
M @jf{ D ATf{ SR M @sf{ D @mgC SR M @mgC D @jgP SR M @jgP D @jgX SR
M @jgX D @mgd SR M @mgd D @sgh SR M @sgh D ATgh SR M @jgX D @mg` SR
M @mg` D @sgd SR M @sgd D ATgd SR M @jfk D @jf{ SR M ATfk D ATgH SR
M ATgX D ATgt SR M @ThP D AHhP SR M AHhP D AQhT SR M AQhT D ATh\ SR
M ATh\ D AThd SR M AThd D AQhl SR M AQhl D AKhp SR M @ThT D AHhT SR
M AHhT D AQhX SR M AQhX D ATh\ SR M @jhD D @jhd SR M @mim D @jiq SR
M @jiq D @siq SR M @siq D @mim SR M @mim D @jia SR M @jia D @jiU SR
M @jiU D @miI SR M @miI D @piE SR M @piE D @siE SR M @siE D @yiI SR
M @yiI D @|iQ SR M @|iQ D ABie SR M ABie D AEim SR M AEim D AHiq SR
M @siE D @viI SR M @viI D @yiQ SR M @yiQ D @?ie SR M @?ie D ABim SR
M ABim D AHiq SR M AHiq D ANiq SR M ANiq D AQim SR M AQim D ATia SR
M ATia D ATiU SR M ATiU D AQiI SR M AQiI D AKiE SR M AKiE D ATiE SR
M ATiE D AQiI SR M @mkz D @jk~ SR M @jk~ D @sk~ SR M @sk~ D @mkz SR
M @mkz D @jkn SR M @jkn D @jkb SR M @jkb D @mkV SR M @mkV D @pkR SR
M @pkR D @skR SR M @skR D @ykV SR M @ykV D @|k^ SR M @|k^ D ABkr SR
M ABkr D AEkz SR M AEkz D AHk~ SR M @skR D @vkV SR M @vkV D @yk^ SR
M @yk^ D @?kr SR M @?kr D ABkz SR M ABkz D AHk~ SR M AHk~ D ANk~ SR
M ANk~ D AQkz SR M AQkz D ATkn SR M ATkn D ATkb SR M ATkb D AQkV SR
M AQkV D AKkR SR M AKkR D ATkR SR M ATkR D AQkV SR M @HlR D @Hl} SR
M @@mS D @@mX SR M @@mX D @@m_ SR M @@m_ D @Ym_ SR M @@m] D @Ym] SR
M @YmS D @Ymi SR M @HnA D @NnI SR M @NnI D @WnQ SR M @WnQ D @dnY SR
M @dnY D @sn] SR M @sn] D @?n] SR M @?n] D ANnY SR M ANnY D AZnQ SR
M AZnQ D AdnI SR M AdnI D AjnA SR M @NnI D @ZnQ SR M @ZnQ D @dnU SR
M @dnU D @snY SR M @snY D @?nY SR M @?nY D ANnU SR M ANnU D AWnQ SR
M AWnQ D AdnI SR
M _bBo D _\Bg SR M _\Bg D _VB[ SR M _VB[ D _PBK SR M _PBK D _MAw SR
M _MAw D _MAg SR M _MAg D _PAR SR M _PAR D _VAB SR M _VAB D _\@v SR
M _\@v D _b@n SR M _\Bg D _VBW SR M _VBW D _SBK SR M _SBK D _PAw SR
M _PAw D _PAg SR M _PAg D _SAR SR M _SAR D _VAF SR M _VAF D _\@v SR
M _{B_ D _{AJ SR M _~B_ D _~AJ SR M _rB_ D `VB_ SR M `VB_ D `_B[ SR
M `_B[ D `bBW SR M `bBW D `eBO SR M `eBO D `eBG SR M `eBG D `bA? SR
M `bA? D `_A{ SR M `_A{ D `VAw SR M `VB_ D `\B[ SR M `\B[ D `_BW SR
M `_BW D `bBO SR M `bBO D `bBG SR M `bBG D `_A? SR M `_A? D `\A{ SR
M `\A{ D `VAw SR M _~Aw D `VAw SR M `VAw D `_As SR M `_As D `bAo SR
M `bAo D `eAg SR M `eAg D `eAZ SR M `eAZ D `bAR SR M `bAR D `_AN SR
M `_AN D `VAJ SR M `VAJ D _rAJ SR M `VAw D `\As SR M `\As D `_Ao SR
M `_Ao D `bAg SR M `bAg D `bAZ SR M `bAZ D `_AR SR M `_AR D `\AN SR
M `\AN D `VAJ SR M `xAo D anAo SR M bDB_ D bYAJ SR M bGB_ D bYAV SR
M bnB_ D bYAJ SR M a{B_ D bPB_ SR M beB_ D bxB_ SR M cDBo D cJBg SR
M cJBg D cPB[ SR M cPB[ D cVBK SR M cVBK D cYAw SR M cYAw D cYAg SR
M cYAg D cVAR SR M cVAR D cPAB SR M cPAB D cJ@v SR M cJ@v D cD@n SR
M cJBg D cPBW SR M cPBW D cSBK SR M cSBK D cVAw SR M cVAw D cVAg SR
M cVAg D cSAR SR M cSAR D cPAF SR M cPAF D cJ@v SR M cvAe D cpAb SR
M cpAb D cmA[ SR M cmA[ D ckAO SR M ckAO D ckAH SR M ckAH D cm@| SR
M cm@| D cp@t SR M cp@t D cv@r SR M cv@r D cy@r SR M cy@r D c?@t SR
M c?@t D dC@| SR M dC@| D dDAH SR M dDAH D dDAO SR M dDAO D dCA[ SR
M dCA[ D c?Ab SR M c?Ab D cyAe SR M cyAe D cvAe SR M cvAe D crAb SR
M crAb D cpA` SR M cpA` D cnA[ SR M cnA[ D cmAO SR M cmAO D cmAH SR
M cmAH D cn@| SR M cn@| D cp@w SR M cp@w D cr@t SR M cr@t D cv@r SR
M cy@r D c}@t SR M c}@t D c?@w SR M c?@w D dA@| SR M dA@| D dCAH SR
M dCAH D dCAO SR M dCAO D dAA[ SR M dAA[ D c?A` SR M c?A` D c}Ab SR
M c}Ab D cyAe SR
M mtpF D mZn` SR M mtpF D nMn` SR M mtow D nJn` SR M mbnx D nFnx SR
M mOn` D men` SR M m?n` D nXn` SR M nnor D nvow SR M nvow D o@pF SR
M o@pF D o@n` SR M n}pA D n}n` SR M nnn` D oOn` SR
M HUxr D JQwi D LNv^ D NJuQ D PFtB D RCrq D S?q^ D U{pJ D Wxns D YtmZ
D [pk? D ]mjc D _iiD D aegc D cbf@ D e^d\ D gZbu D iVaL D kS_b D mO]u
D oK\G D qHZV D sDXc D u@Vo D v}Tx SR
M yOU^ D yHU[ SR M yHU[ D yCUQ SR M yCUQ D y@UA SR M y@UA D y@Tx SR
M y@Tx D yCTh SR M yCTh D yHT^ SR M yHT^ D yOT[ SR M yOT[ D yTT[ SR
M yTT[ D y[T^ SR M y[T^ D y`Th SR M y`Th D ybTx SR M ybTx D ybUA SR
M ybUA D y`UQ SR M y`UQ D y[U[ SR M y[U[ D yTU^ SR M yTU^ D yOU^ SR
M yOU^ D yJU[ SR M yJU[ D yHUX SR M yHUX D yEUQ SR M yEUQ D yCUA SR
M yCUA D yCTx SR M yCTx D yETh SR M yETh D yHTa SR M yHTa D yJT^ SR
M yJT^ D yOT[ SR M yTT[ D yYT^ SR M yYT^ D y[Ta SR M y[Ta D y^Th SR
M y^Th D y`Tx SR M y`Tx D y`UA SR M y`UA D y^UQ SR M y^UQ D y[UX SR
M y[UX D yYU[ SR M yYU[ D yTU^ SR M ytTa D yqT^ SR M yqT^ D ytT[ SR
M ytT[ D yvT^ SR M yvT^ D ytTa SR M zSU^ D zLU[ SR M zLU[ D zGUQ SR
M zGUQ D zEUA SR M zEUA D zETx SR M zETx D zGTh SR M zGTh D zLT^ SR
M zLT^ D zST[ SR M zST[ D zXT[ SR M zXT[ D z_T^ SR M z_T^ D zdTh SR
M zdTh D zgTx SR M zgTx D zgUA SR M zgUA D zdUQ SR M zdUQ D z_U[ SR
M z_U[ D zXU^ SR M zXU^ D zSU^ SR M zSU^ D zNU[ SR M zNU[ D zLUX SR
M zLUX D zIUQ SR M zIUQ D zGUA SR M zGUA D zGTx SR M zGTx D zITh SR
M zITh D zLTa SR M zLTa D zNT^ SR M zNT^ D zST[ SR M zXT[ D z]T^ SR
M z]T^ D z_Ta SR M z_Ta D zbTh SR M zbTh D zdTx SR M zdTx D zdUA SR
M zdUA D zbUQ SR M zbUQ D z_UX SR M z_UX D z]U[ SR M z]U[ D zXU^ SR
M HUvi D JQu` D LNtU D NJsH D PFqz D RCpi D S?oV D U{nA D Wxlj D YtkQ
D [piw D ]mhZ D _if{ D aeeZ D cbcx D e^bS D gZ`l D iV_C D kS]Y D mO[l
D oKY~ D qHXM D sDVZ D u@Tf D v}Ro SR
M yOSW D yHST SR M yHST D yCSK SR M yCSK D y@Rz SR M y@Rz D y@Rq SR
M y@Rq D yCRa SR M yCRa D yHRW SR M yHRW D yORT SR M yORT D yTRT SR
M yTRT D y[RW SR M y[RW D y`Ra SR M y`Ra D ybRq SR M ybRq D ybRz SR
M ybRz D y`SK SR M y`SK D y[ST SR M y[ST D yTSW SR M yTSW D yOSW SR
M yOSW D yJST SR M yJST D yHSQ SR M yHSQ D yESK SR M yESK D yCRz SR
M yCRz D yCRq SR M yCRq D yERa SR M yERa D yHRZ SR M yHRZ D yJRW SR
M yJRW D yORT SR M yTRT D yYRW SR M yYRW D y[RZ SR M y[RZ D y^Ra SR
M y^Ra D y`Rq SR M y`Rq D y`Rz SR M y`Rz D y^SK SR M y^SK D y[SQ SR
M y[SQ D yYST SR M yYST D yTSW SR M ytRZ D yqRW SR M yqRW D ytRT SR
M ytRT D yvRW SR M yvRW D ytRZ SR M zLSK D zQSN SR M zQSN D zXSW SR
M zXSW D zXRT SR M zVST D zVRT SR M zLRT D zbRT SR
M HUta D JQsX D LNrM D NJq@ D PFoq D RCn` D S?mM D U{kx D Wxja D YtiI
D [pgn D ]mfQ D _idr D aecQ D cbao D e^`J D gZ^c D iV\z D kS[P D mOYc
D oKWu D qHVD D sDTQ D u@R] D v}Pf SR
M yOQQ D yHQM SR M yHQM D yCQD SR M yCQD D y@Pt SR M y@Pt D y@Pj SR
M y@Pj D yCPZ SR M yCPZ D yHPP SR M yHPP D yOPM SR M yOPM D yTPM SR
M yTPM D y[PP SR M y[PP D y`PZ SR M y`PZ D ybPj SR M ybPj D ybPt SR
M ybPt D y`QD SR M y`QD D y[QM SR M y[QM D yTQQ SR M yTQQ D yOQQ SR
M yOQQ D yJQM SR M yJQM D yHQJ SR M yHQJ D yEQD SR M yEQD D yCPt SR
M yCPt D yCPj SR M yCPj D yEPZ SR M yEPZ D yHPS SR M yHPS D yJPP SR
M yJPP D yOPM SR M yTPM D yYPP SR M yYPP D y[PS SR M y[PS D y^PZ SR
M y^PZ D y`Pj SR M y`Pj D y`Pt SR M y`Pt D y^QD SR M y^QD D y[QJ SR
M y[QJ D yYQM SR M yYQM D yTQQ SR M ytPS D yqPP SR M yqPP D ytPM SR
M ytPM D yvPP SR M yvPP D ytPS SR M zGQD D zIQA SR M zIQA D zGP} SR
M zGP} D zEQA SR M zEQA D zEQD SR M zEQD D zGQJ SR M zGQJ D zIQM SR
M zIQM D zQQQ SR M zQQQ D z[QQ SR M z[QQ D zbQM SR M zbQM D zdQJ SR
M zdQJ D zgQD SR M zgQD D zgP} SR M zgP} D zdPw SR M zdPw D z]Pp SR
M z]Pp D zQPj SR M zQPj D zLPg SR M zLPg D zGP` SR M zGP` D zEPW SR
M zEPW D zEPM SR M z[QQ D z_QM SR M z_QM D zbQJ SR M zbQJ D zdQD SR
M zdQD D zdP} SR M zdP} D zbPw SR M zbPw D z[Pp SR M z[Pp D zQPj SR
M zEPS D zGPW SR M zGPW D zLPW SR M zLPW D zXPP SR M zXPP D z_PP SR
M z_PP D zdPS SR M zdPS D zgPW SR M zLPW D zXPM SR M zXPM D zbPM SR
M zbPM D zdPP SR M zdPP D zgPW SR M zgPW D zgP] SR
M HUrY D JQqO D LNpD D NJnw D PFmi D RClX D S?kE D U{ip D WxhY D Ytg@
D [pee D ]mdH D _ibi D aeaI D cb_f D e^^A D gZ\Z D iVZr D kSYG D mOWZ
D oKUk D qHS{ D sDRH D u@PT D v}N] SR
M yOOE D yHOB SR M yHOB D yCNy SR M yCNy D y@Nh SR M y@Nh D y@N_ SR
M y@N_ D yCNO SR M yCNO D yHNE SR M yHNE D yONB SR M yONB D yTNB SR
M yTNB D y[NE SR M y[NE D y`NO SR M y`NO D ybN_ SR M ybN_ D ybNh SR
M ybNh D y`Ny SR M y`Ny D y[OB SR M y[OB D yTOE SR M yTOE D yOOE SR
M yOOE D yJOB SR M yJOB D yHN? SR M yHN? D yENy SR M yENy D yCNh SR
M yCNh D yCN_ SR M yCN_ D yENO SR M yENO D yHNH SR M yHNH D yJNE SR
M yJNE D yONB SR M yTNB D yYNE SR M yYNE D y[NH SR M y[NH D y^NO SR
M y^NO D y`N_ SR M y`N_ D y`Nh SR M y`Nh D y^Ny SR M y^Ny D y[N? SR
M y[N? D yYOB SR M yYOB D yTOE SR M ytNH D yqNE SR M yqNE D ytNB SR
M ytNB D yvNE SR M yvNE D ytNH SR M zGN| D zINy SR M zINy D zGNu SR
M zGNu D zENy SR M zENy D zEN| SR M zEN| D zIOB SR M zIOB D zQOE SR
M zQOE D z[OE SR M z[OE D zbOB SR M zbOB D zdN| SR M zdN| D zdNr SR
M zdNr D zbNl SR M zbNl D z[Nh SR M z[Nh D zSNh SR M z[OE D z_OB SR
M z_OB D zbN| SR M zbN| D zbNr SR M zbNr D z_Nl SR M z_Nl D z[Nh SR
M z[Nh D z_Ne SR M z_Ne D zdN_ SR M zdN_ D zgNX SR M zgNX D zgNO SR
M zgNO D zdNH SR M zdNH D zbNE SR M zbNE D z[NB SR M z[NB D zQNB SR
M zQNB D zINE SR M zINE D zGNH SR M zGNH D zENO SR M zENO D zENR SR
M zENR D zGNU SR M zGNU D zINR SR M zINR D zGNO SR M zbNb D zdNX SR
M zdNX D zdNO SR M zdNO D zbNH SR M zbNH D z_NE SR M z_NE D z[NB SR
M HUpP D JQoG D LNm| D NJlo D PFk` D RCjO D S?h| D U{gg D WxfP D Ytdw
D [pc\ D ]ma? D _i`a D ae_@ D cb]] D e^[x D gZZQ D iVXi D kSV~ D mOUQ
D oKSb D qHQr D sDO? D u@NK D v}LT SR
M yOLz D yHLw SR M yHLw D yCLm SR M yCLm D y@L] SR M y@L] D y@LS SR
M y@LS D yCLC SR M yCLC D yHKz SR M yHKz D yOKv SR M yOKv D yTKv SR
M yTKv D y[Kz SR M y[Kz D y`LC SR M y`LC D ybLS SR M ybLS D ybL] SR
M ybL] D y`Lm SR M y`Lm D y[Lw SR M y[Lw D yTLz SR M yTLz D yOLz SR
M yOLz D yJLw SR M yJLw D yHLt SR M yHLt D yELm SR M yELm D yCL] SR
M yCL] D yCLS SR M yCLS D yELC SR M yELC D yHK} SR M yHK} D yJKz SR
M yJKz D yOKv SR M yTKv D yYKz SR M yYKz D y[K} SR M y[K} D y^LC SR
M y^LC D y`LS SR M y`LS D y`L] SR M y`L] D y^Lm SR M y^Lm D y[Lt SR
M y[Lt D yYLw SR M yYLw D yTLz SR M ytK} D yqKz SR M yqKz D ytKv SR
M ytKv D yvKz SR M yvKz D ytK} SR M z[Lt D z[Kv SR M z]Lz D z]Kv SR
M z]Lz D zBLJ SR M zBLJ D ziLJ SR M zSKv D zdKv SR
M HUnH D JQl? D LNkt D NJjg D PFiX D RChF D S?fs D U{e^ D WxdH D Ytbo
D [paT D ]m_w D _i^X D ae\w D cb[T D e^Yo D gZXI D iVV` D kSTu D mOSH
D oKQZ D qHOi D sDMv D u@LB D v}JK SR
M yOJs D yHJp SR M yHJp D yCJf SR M yCJf D y@JV SR M y@JV D y@JM SR
M y@JM D yCI| SR M yCI| D yHIs SR M yHIs D yOIo SR M yOIo D yTIo SR
M yTIo D y[Is SR M y[Is D y`I| SR M y`I| D ybJM SR M ybJM D ybJV SR
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M yOJs D yJJp SR M yJJp D yHJm SR M yHJm D yEJf SR M yEJf D yCJV SR
M yCJV D yCJM SR M yCJM D yEI| SR M yEI| D yHIv SR M yHIv D yJIs SR
M yJIs D yOIo SR M yTIo D yYIs SR M yYIs D y[Iv SR M y[Iv D y^I| SR
M y^I| D y`JM SR M y`JM D y`JV SR M y`JV D y^Jf SR M y^Jf D y[Jm SR
M y[Jm D yYJp SR M yYJp D yTJs SR M ytIv D yqIs SR M yqIs D ytIo SR
M ytIo D yvIs SR M yvIs D ytIv SR M zIJs D zEJS SR M zEJS D zIJV SR
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M zdJP D zgJF SR M zgJF D zgJC SR M zgJC D zdIy SR M zdIy D z_Is SR
M z_Is D zXIo SR M zXIo D zQIo SR M zQIo D zIIs SR M zIIs D zGIv SR
M zGIv D zEI| SR M zEI| D zEJ@ SR M zEJ@ D zGJC SR M zGJC D zIJ@ SR
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M zdJF D zdJC SR M zdJC D zbIy SR M zbIy D z]Is SR M z]Is D zXIo SR
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%PSKCloseWorkStation
%PSKOpenWorkStation
CL
%%Trailer
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%DocumentFonts: Times-Bold Times-Italic Symbol Times-Roman
%%Pages: 1
%%EOF

%%EndDocument
FMENDEPSF
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%%BeginDocument: /pongo/data2/drs/ghrs/handbook/ih5/figs/mirror_n1.epsi
%!PS-Adobe-2.0 EPSF-1.2
%%BoundingBox: 56 29 576 730
%!PS-Adobe-1.0
%%Creator: PSIKern - An IRAF GKI Translator
%%CreationDate: Thu 15:33:07 28-Apr-94
%%DocumentFonts: (atend)
%%Pages: (atend)
%%BoundingBox: 28 28 583 763
%%EndComments
/MAXNDC 4095 def /PageSizeXMeter 0.2594 def /PageSizeYMeter 0.1959 def
/PageOffXMeter 0.01 def /PageOffYMeter 0.01 def
/PortraitMode false def /PortraitRotation 0. def
/LandScapeRotation 90. def /GT_LEFT 2 def /GT_RIGHT 3 def
/GT_TOP 6 def /GT_BOTTOM 7 def /GT_UP 4 def /GT_DOWN 5 def
/GT_CENTER 1 def /RF /Times-Roman def /GF /Symbol def
/IF /Times-Italic def /BF /Times-Bold def /DASH 49 def /DOT 4 def
/SPACE 24 def

% How to define things.
/BD { bind def } bind def
/LD { load def } bind def

% Constants
/yes true def
/no false def

% Define some shorthand instructions.
/GRS /grestore LD
/GS /gsave LD
/MK /mark LD
/R /restore LD
/S /save LD
/SH /showpage LD
/SW /setlinewidth LD

% Measurement conversions.
/PointperMeter 2834.64 def
/MonoScale .7 def

% SR: Set current path to page: - -> -
/SR { currentpoint stroke moveto } BD

% CL: CLear the page: - -> -
/CL { restore showpage grestore gsave save } BD

% RC: Read Coordinates: string -> x y
/RC {
currentfile read pop 8#77 and 6 bitshift
currentfile read pop 8#77 and or
currentfile read pop 8#77 and 6 bitshift
currentfile read pop 8#77 and or
} BD

% DO - Determine Offset: length -> offset
/DO { DS dup 0 eq { pop pop 0 } { mod } ifelse } BD

% M: Move: M string -> -
% Move to a point and clear length of path.
/M { RC moveto CT OF setdash } BD

% D: Draw: D string -> -
% This also calculates the length of the current path.
/OF 0 def
/D { RC DS 0 ne { 2 copy currentpoint exch 4 1 roll sub dup mul 3 1 roll
sub dup mul add sqrt round OF add cvi DO /OF exch store } if lineto
} BD

% Character/Font definitions.

% FS -- Define the current font size: xsize ysize FS -
/FontXSize 0 def /FontYSize 0 def /NewFont true def
/FS { /FontYSize exch MonoScale mul store /FontXSize exch MonoScale mul store
/NewFont true store } BD

% PH -- Set the current path: path PH -
/Path 0 def
/PH { /Path exch store } BD

% PA -- Set the path angle of the text: angle PA -
/Angle 0 def
/PA { 360 mod dup 0 lt { 360 add } if /Angle exch store /NewFont true store } BD

% HJ, VJ -- Set Horizontal/Verticle Justification: just HJ/VJ -
/HorzJust 0 def /VertJust 0 def
/HJ { /HorzJust exch store } BD /VJ { /VertJust exch store } BD

% VT -- Use mono- or variable-spaced fonts: flag VT -
/VT true def
/VT { /Variable exch store } BD

% SetFont -- Make the required font the default: font SetFont -
% Note scale factor- This is to fill out monospaced better and match other
% IRAF output.
/Font () def
/FontMatrix matrix def
/SetFont {
dup Font ne NewFont or
{ dup /Font exch store findfont
Angle matrix rotate FontXSize MonoScale div FontYSize MonoScale div
matrix scale matrix concatmatrix makefont setfont Angle matrix rotate
FontXSize FontYSize matrix scale matrix concatmatrix /FontMatrix exch
store
}
{ pop } ifelse /NewFont false store
} BD

% StringWidth -- Determine path length of string: string StringWidth - xs ys
/StringWidth { Path GT_RIGHT eq Variable and { stringwidth }
{ Path GT_RIGHT eq { length } { pop 1 } ifelse 0 FontMatrix transform }
ifelse
} BD

% MonoShow -- Write the string out in mono-spaced: string MonoShow -
/MonoShow {
/t 1 string def 1 0 FontMatrix transform
/dy exch def /dx exch def Path GT_RIGHT eq { /mx dx def /my dy def }
{ 0 1 FontMatrix transform /my exch def /mx exch def } ifelse
{ t 0 3 -1 roll put t dup stringwidth dy exch sub 2 div exch dx exch
sub 2 div exch gsave rmoveto show grestore mx my rmoveto
} forall
} BD

% WS -- Draw the string: string font string ... DS -
/*WSDict 13 dict def
/WS { *WSDict begin
counttomark 2 idiv dup dup array /FontArray exch def
array /StringArray exch def 1 sub /NStrings exch def

NStrings -1 0 {
dup 4 1 roll exch StringArray 3 1 roll put FontArray 3 1 roll put
} for
pop

/XSize 0 def /YSize 0 def /NChars 0 def
0 1 NStrings {
dup FontArray exch get SetFont StringArray exch get dup
length NChars add /NChars exch def StringWidth
YSize add /YSize exch def XSize add /XSize exch def
} for

/TAngle HorzJust GT_RIGHT eq
{ Angle 180 add dup 360 ge { 360 sub } if } { Angle } ifelse def
0 TAngle 180 le HorzJust GT_CENTER eq or
{ Angle sin FontYSize mul Path GT_UP eq { NChars mul } if add } if
TAngle 90 ge TAngle 270 le and HorzJust GT_CENTER eq or
{ Path GT_RIGHT eq { XSize } { Angle cos FontXSize mul } ifelse sub } if
HorzJust GT_CENTER eq { .5 mul } if

/TAngle
VertJust GT_TOP eq { Angle 180 sub dup 0 lt { 360 add } if } { Angle } ifelse
def
0 TAngle 90 ge TAngle 270 le and VertJust GT_CENTER eq or
{ Angle cos FontYSize mul Path GT_UP eq { NChars mul } if sub } if
TAngle 180 ge TAngle 360 le and VertJust GT_CENTER eq or
{ Path GT_RIGHT eq { YSize } { Angle sin FontXSize mul } ifelse sub } if
VertJust GT_CENTER eq { .5 mul } if
rmoveto

0 1 NStrings {
dup FontArray exch get SetFont StringArray exch get
Path GT_RIGHT eq Variable and { show } { MonoShow } ifelse
} for

end
} BD

% Define the DASHED, DOTTED, DOTDASH patterns.
/DS 0 def
/LPS {
/OF 0 store /DS 0 store 0 array
} BD
/LPD {
/OF 0 store DASH SPACE 2 copy add /DS exch store 2 array astore
} BD
/LPP {
/OF 0 store DOT SPACE 2 copy add /DS exch store 2 array astore
} BD
/LDD {
/OF 0 store DOT SPACE DASH SPACE 4 copy add add add /DS exch store
4 array astore
} BD

% LT - Set Line Type - array -> -
/CT { currentdash pop } BD
/LT { /CT exch store /OF 0 store } BD

% SC - Set Color: color -> -
/*SCDict 1 dict def
/SC { *SCDict begin
1 sub /color exch def
GR color get 255 div GG color get 255 div GB color get 255 div setrgbcolor
end
} BD

% MI - Make Image LUT: table-name size MI hexstring -> -
/MI { currentfile exch string readhexstring pop def } BD

% Define the graphics color lookup table.
/GR 16 MI 00FFFF0000FF00FFFFB0FFF0D940F0F5
/GG 16 MI 00FF00FF00FFFF0080D0A6E670E082DE
/GB 16 MI 00FF0000FF00FFFF4F61008CD6D1EFB3

% Render an image when no image LUT has been define.
/DefaultGrey {
{ currentfile inarr readhexstring pop } image
} BD

% ColorImage - Produce an image by indexing into the Image Lookup Table.
% There are two versions of this code- one for PostScript that has
% the colorimage operator and one that doesn't. If the PostScript doesn't
% have colorimage, it is assumed that it can only produce black & white,
% in which the Image LUT is combined to produce a single grey which is
% then used as the image for the image operator.
/colorimage where
{ pop
/ColorImage {
{ currentfile inarr readhexstring pop dup /inarr exch def
length 3 mul string /oarr exch def
0 1 inarr length 1 sub
{ /iindex exch def
/oindex iindex 3 mul def
oarr oindex IR inarr iindex get get put
oarr oindex 1 add IG inarr iindex get get put
oarr oindex 2 add IB inarr iindex get get put
} for
oarr
}
false 3 colorimage
} BD
}
{ /ColorImage {
{ currentfile inarr readhexstring pop dup /inarr exch def
length string /oarr exch def
0 1 inarr length 1 sub
{ /iindex exch def
oarr iindex
IR inarr iindex get get 0.3 mul
IG inarr iindex get get 0.59 mul
IB inarr iindex get get 0.11 mul
add add round cvi dup 255 gt { pop 255 } if
put
} for
oarr
}
image
} BD
}
ifelse

% PC: Put Cellarray: width height bitspersample matrix -> -
/*PCdict 10 dict def
/PC {
*PCdict begin
4 -1 roll dup /inarr exch string def 4 1 roll
/IR where {pop ColorImage} {DefaultGrey} ifelse
end
} BD

% Define the Hatch (fill area) styles. H1 and H2 are handled internally
% by PSIKern. Feel free to define more; there is no limit.
/H3 <8888888888888888> def
/H4 def
/H5 <8844221188442211> def
/H6 <1122448811224488> def

% Setup for fill patterns. This whole section of code is taken almost
% directly from _PostScript Language: Tutorial and Cookbook_, Adobe Systems,
% 1986 (the blue book).
/setuserscreendict 22 dict def
setuserscreendict begin
/tempctm matrix def
/temprot matrix def
/tempscale matrix def

/concatprocs
{ /proc2 exch cvlit def
/proc1 exch cvlit def
/newproc proc1 length proc2 length add
array def
newproc 0 proc1 putinterval
newproc proc1 length proc2 putinterval
newproc cvx
} def

/resmatrix matrix def
/findresolution
{ 72 0 resmatrix defaultmatrix dtransform
/yres exch def /xres exch def
xres dup mul yres dup mul add sqrt
} def
end

/setuserscreen
{ setuserscreendict begin
/spotfunction exch def
/screenangle exch def
/cellsize exch def

/m tempctm currentmatrix def
/rm screenangle temprot rotate def
/sm cellsize dup tempscale scale def

sm rm m m concatmatrix m concatmatrix pop
1 0 m dtransform /y1 exch def /x1 exch def

/veclength x1 dup mul y1 dup mul add sqrt def
/frequency findresolution veclength div def

/newscreenangle y1 x1 atan def

m 2 get m 1 get mul m 0 get m 3 get mul sub
0 gt
{ {neg} /spotfunction load concatprocs
/spotfunction exch def
} if

frequency newscreenangle /spotfunction load
setscreen
end
} def

/setpatterndict 18 dict def
setpatterndict begin
/bitison
{ /ybit exch def /xbit exch def
/bytevalue bstring ybit bwidth mul xbit 8 idiv
add get def

/mask 1 7 xbit 8 mod sub bitshift def
bytevalue mask and 0 ne
} def
end

/bitpatternspotfunction
{ setpatterndict begin
/y exch def /x exch def

/xindex x 1 add 2 div bpside mul cvi def
/yindex y 1 add 2 div bpside mul cvi def

xindex yindex bitison
{ /onbits onbits 1 add def 1 }
{ /offbits offbits 1 add def 0 }
ifelse
end
} def

/setpattern
{ setpatterndict begin
/cellsz exch def
/angle exch def
/bwidth exch def
/bpside exch def
/bstring exch def

/onbits 0 def /offbits 0 def
cellsz angle /bitpatternspotfunction load
setuserscreen
{ } settransfer
offbits offbits onbits add div setgray
end
} def

% SP: Set Pattern: pattern -> -
/SP { 8 1 0 MAXNDC 100 div setpattern } BD

% FI: Fill with Pattern: - -> -
/FI { fill grestore } BD

% Set the transformation matrix.
PointperMeter dup scale
PageOffXMeter
PortraitMode not
{ PageSizeYMeter add }
if
PageOffYMeter translate
PortraitMode
{ PortraitRotation rotate }
{ LandScapeRotation rotate}
ifelse
PageSizeXMeter MAXNDC div PageSizeYMeter MAXNDC div scale
1 setlinejoin 1 setlinecap

% Save the current graphics state (to restore after showpage) and the
% VM state to recover after a showpage.
GS S

%%EndProlog
%PSKOpenWorkStation
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M F~DW D GAD[ SR M GAD[ D F~D_ SR M GnEd D GnDW SR M GqEl D GqDW SR
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M MoD{ D MrDg SR M MrDg D MxD[ SR M MxD[ D NADW SR M NADW D NGDW SR
M NGDW D NPD[ SR M NPD[ D NVDg SR M NVDg D NYD{ SR M NYD{ D NYEG SR
M NYEG D NVE\ SR M NVE\ D NPEh SR M NPEh D NGEl SR M NGEl D NAEl SR
M NAEl D M{Eh SR M M{Eh D MxEd SR M MxEd D MuE\ SR M MuE\ D MrEG SR
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M NSDg D NVD{ SR M NVD{ D NVEG SR M NVEG D NSE\ SR M NSE\ D NPEd SR
M NPEd D NMEh SR M NMEh D NGEl SR M NoD_ D NlD[ SR M NlD[ D NoDW SR
M NoDW D NrD[ SR M NrD[ D NoD_ SR M OGE\ D OJEX SR M OJEX D OGET SR
M OGET D ODEX SR M ODEX D ODE\ SR M ODE\ D OGEd SR M OGEd D OJEh SR
M OJEh D OSEl SR M OSEl D O`El SR M O`El D OiEh SR M OiEh D OlEd SR
M OlEd D OoE\ SR M OoE\ D OoET SR M OoET D OlEL SR M OlEL D OcEC SR
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M ODDc D ODDW SR M O`El D OfEh SR M OfEh D OiEd SR M OiEd D OlE\ SR
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M ODD_ D OGDc SR M OGDc D OMDc SR M OMDc D O\D[ SR M O\D[ D OfD[ SR
M OfD[ D OlD_ SR M OlD_ D OoDc SR M OMDc D O\DW SR M O\DW D OiDW SR
M OiDW D OlD[ SR M OlD[ D OoDc SR M OoDc D OoDk SR M UxEl D UoEh SR
M UoEh D UiE\ SR M UiE\ D UfEG SR M UfEG D UfD{ SR M UfD{ D UiDg SR
M UiDg D UoD[ SR M UoD[ D UxDW SR M UxDW D U~DW SR M U~DW D VHD[ SR
M VHD[ D VNDg SR M VNDg D VQD{ SR M VQD{ D VQEG SR M VQEG D VNE\ SR
M VNE\ D VHEh SR M VHEh D U~El SR M U~El D UxEl SR M UxEl D UrEh SR
M UrEh D UoEd SR M UoEd D UlE\ SR M UlE\ D UiEG SR M UiEG D UiD{ SR
M UiD{ D UlDg SR M UlDg D UoD_ SR M UoD_ D UrD[ SR M UrD[ D UxDW SR
M U~DW D VED[ SR M VED[ D VHD_ SR M VHD_ D VKDg SR M VKDg D VND{ SR
M VND{ D VNEG SR M VNEG D VKE\ SR M VKE\ D VHEd SR M VHEd D VEEh SR
M VEEh D U~El SR M \?El D \vEh SR M \vEh D \pE\ SR M \pE\ D \mEG SR
M \mEG D \mD{ SR M \mD{ D \pDg SR M \pDg D \vD[ SR M \vD[ D \?DW SR
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M ]WD{ D ]WEG SR M ]WEG D ]TE\ SR M ]TE\ D ]NEh SR M ]NEh D ]EEl SR
M ]EEl D \?El SR M \?El D \yEh SR M \yEh D \vEd SR M \vEd D \sE\ SR
M \sE\ D \pEG SR M \pEG D \pD{ SR M \pD{ D \sDg SR M \sDg D \vD_ SR
M \vD_ D \yD[ SR M \yD[ D \?DW SR M ]EDW D ]KD[ SR M ]KD[ D ]ND_ SR
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M ]QE\ D ]NEd SR M ]NEd D ]KEh SR M ]KEh D ]EEl SR M ]mD_ D ]jD[ SR
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M dpEl D dgEh SR M dgEh D daE\ SR M daE\ D d^EG SR M d^EG D d^D{ SR
M d^D{ D daDg SR M daDg D dgD[ SR M dgD[ D dpDW SR M dpDW D dvDW SR
M dvDW D d?D[ SR M d?D[ D eFDg SR M eFDg D eID{ SR M eID{ D eIEG SR
M eIEG D eFE\ SR M eFE\ D d?Eh SR M d?Eh D dvEl SR M dvEl D dpEl SR
M dpEl D djEh SR M djEh D dgEd SR M dgEd D ddE\ SR M ddE\ D daEG SR
M daEG D daD{ SR M daD{ D ddDg SR M ddDg D dgD_ SR M dgD_ D djD[ SR
M djD[ D dpDW SR M dvDW D d|D[ SR M d|D[ D d?D_ SR M d?D_ D eBDg SR
M eBDg D eFD{ SR M eFD{ D eFEG SR M eFEG D eBE\ SR M eBE\ D d?Ed SR
M d?Ed D d|Eh SR M d|Eh D dvEl SR M e^D_ D e[D[ SR M e[D[ D e^DW SR
M e^DW D eaD[ SR M eaD[ D e^D_ SR M fOEd D fODW SR M fREl D fRDW SR
M fREl D epDo SR M epDo D faDo SR M fFDW D f[DW SR M lbEl D lXEh SR
M lXEh D lRE\ SR M lRE\ D lOEG SR M lOEG D lOD{ SR M lOD{ D lRDg SR
M lRDg D lXD[ SR M lXD[ D lbDW SR M lbDW D lhDW SR M lhDW D lqD[ SR
M lqD[ D lwDg SR M lwDg D lzD{ SR M lzD{ D lzEG SR M lzEG D lwE\ SR
M lwE\ D lqEh SR M lqEh D lhEl SR M lhEl D lbEl SR M lbEl D l[Eh SR
M l[Eh D lXEd SR M lXEd D lUE\ SR M lUE\ D lREG SR M lREG D lRD{ SR
M lRD{ D lUDg SR M lUDg D lXD_ SR M lXD_ D l[D[ SR M l[D[ D lbDW SR
M lhDW D lnD[ SR M lnD[ D lqD_ SR M lqD_ D ltDg SR M ltDg D lwD{ SR
M lwD{ D lwEG SR M lwEG D ltE\ SR M ltE\ D lqEd SR M lqEd D lnEh SR
M lnEh D lhEl SR M mOD_ D mLD[ SR M mLD[ D mODW SR M mODW D mRD[ SR
M mRD[ D mOD_ SR M nIE` D nFE\ SR M nFE\ D nIEX SR M nIEX D nLE\ SR
M nLE\ D nLE` SR M nLE` D nIEh SR M nIEh D nCEl SR M nCEl D mzEl SR
M mzEl D mqEh SR M mqEh D mkE` SR M mkE` D mhEX SR M mhEX D meEG SR
M meEG D meDo SR M meDo D mhDc SR M mhDc D mnD[ SR M mnD[ D mwDW SR
M mwDW D m}DW SR M m}DW D nFD[ SR M nFD[ D nLDc SR M nLDc D nODo SR
M nODo D nODs SR M nODs D nLD? SR M nLD? D nFEG SR M nFEG D m}EL SR
M m}EL D mzEL SR M mzEL D mqEG SR M mqEG D mkD? SR M mkD? D mhDs SR
M mzEl D mtEh SR M mtEh D mnE` SR M mnE` D mkEX SR M mkEX D mhEG SR
M mhEG D mhDo SR M mhDo D mkDc SR M mkDc D mqD[ SR M mqD[ D mwDW SR
M m}DW D nCD[ SR M nCD[ D nIDc SR M nIDc D nLDo SR M nLDo D nLDs SR
M nLDs D nID? SR M nID? D nCEG SR M nCEG D m}EL SR M tSEl D tJEh SR
M tJEh D tDE\ SR M tDE\ D t@EG SR M t@EG D t@D{ SR M t@D{ D tDDg SR
M tDDg D tJD[ SR M tJD[ D tSDW SR M tSDW D tYDW SR M tYDW D tbD[ SR
M tbD[ D thDg SR M thDg D tkD{ SR M tkD{ D tkEG SR M tkEG D thE\ SR
M thE\ D tbEh SR M tbEh D tYEl SR M tYEl D tSEl SR M tSEl D tMEh SR
M tMEh D tJEd SR M tJEd D tGE\ SR M tGE\ D tDEG SR M tDEG D tDD{ SR
M tDD{ D tGDg SR M tGDg D tJD_ SR M tJD_ D tMD[ SR M tMD[ D tSDW SR
M tYDW D t_D[ SR M t_D[ D tbD_ SR M tbD_ D teDg SR M teDg D thD{ SR
M thD{ D thEG SR M thEG D teE\ SR M teE\ D tbEd SR M tbEd D t_Eh SR
M t_Eh D tYEl SR M u@D_ D t}D[ SR M t}D[ D u@DW SR M u@DW D uDD[ SR
M uDD[ D u@D_ SR M ueEl D u\Eh SR M u\Eh D uYE` SR M uYE` D uYET SR
M uYET D u\EL SR M u\EL D ueEG SR M ueEG D uqEG SR M uqEG D uzEL SR
M uzEL D u}ET SR M u}ET D u}E` SR M u}E` D uzEh SR M uzEh D uqEl SR
M uqEl D ueEl SR M ueEl D u_Eh SR M u_Eh D u\E` SR M u\E` D u\ET SR
M u\ET D u_EL SR M u_EL D ueEG SR M uqEG D uwEL SR M uwEL D uzET SR
M uzET D uzE` SR M uzE` D uwEh SR M uwEh D uqEl SR M ueEG D u\EC SR
M u\EC D uYD? SR M uYD? D uVDw SR M uVDw D uVDg SR M uVDg D uYD_ SR
M uYD_ D u\D[ SR M u\D[ D ueDW SR M ueDW D uqDW SR M uqDW D uzD[ SR
M uzD[ D u}D_ SR M u}D_ D v@Dg SR M v@Dg D v@Dw SR M v@Dw D u}D? SR
M u}D? D uzEC SR M uzEC D uqEG SR M ueEG D u_EC SR M u_EC D u\D? SR
M u\D? D uYDw SR M uYDw D uYDg SR M uYDg D u\D_ SR M u\D_ D u_D[ SR
M u_D[ D ueDW SR M uqDW D uwD[ SR M uwD[ D uzD_ SR M uzD_ D u}Dg SR
M u}Dg D u}Dw SR M u}Dw D uzD? SR M uzD? D uwEC SR M uwEC D uqEG SR
M |fE\ D |lE` SR M |lE` D |uEl SR M |uEl D |uDW SR M |rEh D |rDW SR
M |fDW D }ADW SR M FY|r D |r|r SR M FY|r D FY{r SR M HU|r D HU|R SR
M JQ|r D JQ|R SR M LN|r D LN|R SR M NJ|r D NJ{r SR M PF|r D PF|R SR
M RC|r D RC|R SR M S?|r D S?|R SR M U{|r D U{{r SR M Wx|r D Wx|R SR
M Yt|r D Yt|R SR M [p|r D [p|R SR M ]m|r D ]m{r SR M _i|r D _i|R SR
M ae|r D ae|R SR M cb|r D cb|R SR M e^|r D e^{r SR M gZ|r D gZ|R SR
M iV|r D iV|R SR M kS|r D kS|R SR M mO|r D mO{r SR M oK|r D oK|R SR
M qH|r D qH|R SR M sD|r D sD|R SR M u@|r D u@{r SR M v}|r D v}|R SR
M xy|r D xy|R SR M zu|r D zu|R SR M |r|r D |r{r SR M FYFY D FY|r SR
M FYFY D FyFY SR M FYFY D GYFY SR M FYHG D FyHG SR M FYIH D FyIH SR
M FYIu D FyIu SR M FYJY D FyJY SR M FYJv D FyJv SR M FYKN D FyKN SR
M FYKd D FyKd SR M FYKv D FyKv SR M FYLG D FyLG SR M FYLG D GYLG SR
M FYMv D FyMv SR M FYNv D FyNv SR M FYOd D FyOd SR M FYPG D FyPG SR
M FYPd D FyPd SR M FYP} D FyP} SR M FYQR D FyQR SR M FYQe D FyQe SR
M FYQv D FyQv SR M FYQv D GYQv SR M FYSd D FySd SR M FYTd D FyTd SR
M FYUR D FyUR SR M FYUv D FyUv SR M FYVS D FyVS SR M FYVk D FyVk SR
M FYWA D FyWA SR M FYWS D FyWS SR M FYWd D FyWd SR M FYWd D GYWd SR
M FYYR D FyYR SR M FYZS D FyZS SR M FY[A D Fy[A SR M FY[d D Fy[d SR
M FY\A D Fy\A SR M FY\Z D Fy\Z SR M FY\o D Fy\o SR M FY]B D Fy]B SR
M FY]R D Fy]R SR M FY]R D GY]R SR M FY_A D Fy_A SR M FY`A D Fy`A SR
M FY`o D Fy`o SR M FYaS D FyaS SR M FYap D Fyap SR M FYbH D FybH SR
M FYb] D Fyb] SR M FYbp D Fybp SR M FYcA D FycA SR M FYcA D GYcA SR
M FYdo D Fydo SR M FYep D Fyep SR M FYf] D Fyf] SR M FYgA D FygA SR
M FYg^ D Fyg^ SR M FYgv D Fygv SR M FYhL D FyhL SR M FYh^ D Fyh^ SR
M FYho D Fyho SR M FYho D GYho SR M FYj^ D Fyj^ SR M FYk^ D Fyk^ SR
M FYlL D FylL SR M FYlo D Fylo SR M FYmL D FymL SR M FYme D Fyme SR
M FYmz D Fymz SR M FYnM D FynM SR M FYn^ D Fyn^ SR M FYn^ D GYn^ SR
M FYpL D FypL SR M FYqL D FyqL SR M FYqz D Fyqz SR M FYr^ D Fyr^ SR
M FYr{ D Fyr{ SR M FYsS D FysS SR M FYsi D Fysi SR M FYs{ D Fys{ SR
M FYtL D FytL SR M FYtL D GYtL SR M FYuz D Fyuz SR M FYv{ D Fyv{ SR
M FYwi D Fywi SR M FYxL D FyxL SR M FYxi D Fyxi SR M FYyB D FyyB SR
M FYyW D FyyW SR M FYyj D Fyyj SR M FYyz D Fyyz SR M FYyz D GYyz SR
M FY{i D Fy{i SR M FY|i D Fy|i SR M ByFy D B?F} SR M B?F} D CHGI SR
M CHGI D CHEu SR M CEGE D CEEu SR M ByEu D CTEu SR M C?GI D CvGE SR
M CvGE D CpFy SR M CpFy D ClFe SR M ClFe D ClFY SR M ClFY D CpFE SR
M CpFE D CvEy SR M CvEy D C?Eu SR M C?Eu D DEEu SR M DEEu D DNEy SR
M DNEy D DTFE SR M DTFE D DWFY SR M DWFY D DWFe SR M DWFe D DTFy SR
M DTFy D DNGE SR M DNGE D DEGI SR M DEGI D C?GI SR M C?GI D CyGE SR
M CyGE D CvGA SR M CvGA D CsFy SR M CsFy D CpFe SR M CpFe D CpFY SR
M CpFY D CsFE SR M CsFE D CvE} SR M CvE} D CyEy SR M CyEy D C?Eu SR
M DEEu D DKEy SR M DKEy D DNE} SR M DNE} D DQFE SR M DQFE D DTFY SR
M DTFY D DTFe SR M DTFe D DQFy SR M DQFy D DNGA SR M DNGA D DKGE SR
M DKGE D DEGI SR M ERGw D ELGt SR M ELGt D EIGm SR M EIGm D EGGa SR
M EGGa D EGGZ SR M EGGZ D EIGM SR M EIGM D ELGF SR M ELGF D ERGD SR
M ERGD D EUGD SR M EUGD D E[GF SR M E[GF D E^GM SR M E^GM D E`GZ SR
M E`GZ D E`Ga SR M E`Ga D E^Gm SR M E^Gm D E[Gt SR M E[Gt D EUGw SR
M EUGw D ERGw SR M ERGw D ENGt SR M ENGt D ELGr SR M ELGr D EJGm SR
M EJGm D EIGa SR M EIGa D EIGZ SR M EIGZ D EJGM SR M EJGM D ELGI SR
M ELGI D ENGF SR M ENGF D ERGD SR M EUGD D EYGF SR M EYGF D E[GI SR
M E[GI D E]GM SR M E]GM D E^GZ SR M E^GZ D E^Ga SR M E^Ga D E]Gm SR
M E]Gm D E[Gr SR M E[Gr D EYGt SR M EYGt D EUGw SR M ByLh D B?Ll SR
M B?Ll D CHLx SR M CHLx D CHKc SR M CELt D CEKc SR M ByKc D CTKc SR
M C?Lx D CvLt SR M CvLt D CpLh SR M CpLh D ClLS SR M ClLS D ClLG SR
M ClLG D CpKs SR M CpKs D CvKg SR M CvKg D C?Kc SR M C?Kc D DEKc SR
M DEKc D DNKg SR M DNKg D DTKs SR M DTKs D DWLG SR M DWLG D DWLS SR
M DWLS D DTLh SR M DTLh D DNLt SR M DNLt D DELx SR M DELx D C?Lx SR
M C?Lx D CyLt SR M CyLt D CvLp SR M CvLp D CsLh SR M CsLh D CpLS SR
M CpLS D CpLG SR M CpLG D CsKs SR M CsKs D CvKk SR M CvKk D CyKg SR
M CyKg D C?Kc SR M DEKc D DKKg SR M DKKg D DNKk SR M DNKk D DQKs SR
M DQKs D DTLG SR M DTLG D DTLS SR M DTLS D DQLh SR M DQLh D DNLp SR
M DNLp D DKLt SR M DKLt D DELx SR M ELM[ D EPM^ SR M EPM^ D EUMe SR
M EUMe D EULr SR M ESMc D ESLr SR M ELLr D E]Lr SR M ByRV D B?RZ SR
M B?RZ D CHRf SR M CHRf D CHQQ SR M CERb D CEQQ SR M ByQQ D CTQQ SR
M C?Rf D CvRb SR M CvRb D CpRV SR M CpRV D ClRB SR M ClRB D ClQv SR
M ClQv D CpQb SR M CpQb D CvQV SR M CvQV D C?QQ SR M C?QQ D DEQQ SR
M DEQQ D DNQV SR M DNQV D DTQb SR M DTQb D DWQv SR M DWQv D DWRB SR
M DWRB D DTRV SR M DTRV D DNRb SR M DNRb D DERf SR M DERf D C?Rf SR
M C?Rf D CyRb SR M CyRb D CvR^ SR M CvR^ D CsRV SR M CsRV D CpRB SR
M CpRB D CpQv SR M CpQv D CsQb SR M CsQb D CvQZ SR M CvQZ D CyQV SR
M CyQV D C?QQ SR M DEQQ D DKQV SR M DKQV D DNQZ SR M DNQZ D DQQb SR
M DQQb D DTQv SR M DTQv D DTRB SR M DTRB D DQRV SR M DQRV D DNR^ SR
M DNR^ D DKRb SR M DKRb D DERf SR M EISJ D EJSG SR M EJSG D EISE SR
M EISE D EGSG SR M EGSG D EGSJ SR M EGSJ D EISN SR M EISN D EJSQ SR
M EJSQ D EPSS SR M EPSS D EWSS SR M EWSS D E]SQ SR M E]SQ D E^SN SR
M E^SN D E`SJ SR M E`SJ D E`SE SR M E`SE D E^S@ SR M E^S@ D EYR{ SR
M EYR{ D EPRv SR M EPRv D ELRt SR M ELRt D EIRo SR M EIRo D EGRh SR
M EGRh D EGR` SR M EWSS D E[SQ SR M E[SQ D E]SN SR M E]SN D E^SJ SR
M E^SJ D E^SE SR M E^SE D E]S@ SR M E]S@ D EWR{ SR M EWR{ D EPRv SR
M EGRe D EIRh SR M EIRh D ELRh SR M ELRh D EURc SR M EURc D E[Rc SR
M E[Rc D E^Re SR M E^Re D E`Rh SR M ELRh D EUR` SR M EUR` D E]R` SR
M E]R` D E^Rc SR M E^Rc D E`Rh SR M E`Rh D E`Rm SR M ByXD D B?XH SR
M B?XH D CHXU SR M CHXU D CHW@ SR M CEXQ D CEW@ SR M ByW@ D CTW@ SR
M C?XU D CvXQ SR M CvXQ D CpXD SR M CpXD D ClWp SR M ClWp D ClWd SR
M ClWd D CpWP SR M CpWP D CvWD SR M CvWD D C?W@ SR M C?W@ D DEW@ SR
M DEW@ D DNWD SR M DNWD D DTWP SR M DTWP D DWWd SR M DWWd D DWWp SR
M DWWp D DTXD SR M DTXD D DNXQ SR M DNXQ D DEXU SR M DEXU D C?XU SR
M C?XU D CyXQ SR M CyXQ D CvXL SR M CvXL D CsXD SR M CsXD D CpWp SR
M CpWp D CpWd SR M CpWd D CsWP SR M CsWP D CvWH SR M CvWH D CyWD SR
M CyWD D C?W@ SR M DEW@ D DKWD SR M DKWD D DNWH SR M DNWH D DQWP SR
M DQWP D DTWd SR M DTWd D DTWp SR M DTWp D DQXD SR M DQXD D DNXL SR
M DNXL D DKXQ SR M DKXQ D DEXU SR M EIXz D EJXx SR M EJXx D EIXv SR
M EIXv D EGXx SR M EGXx D EGXz SR M EGXz D EJX? SR M EJX? D EPYB SR
M EPYB D EWYB SR M EWYB D E]X? SR M E]X? D E^Xz SR M E^Xz D E^Xs SR
M E^Xs D E]Xn SR M E]Xn D EWXl SR M EWXl D ERXl SR M EWYB D E[X? SR
M E[X? D E]Xz SR M E]Xz D E]Xs SR M E]Xs D E[Xn SR M E[Xn D EWXl SR
M EWXl D E[Xj SR M E[Xj D E^Xe SR M E^Xe D E`X` SR M E`X` D E`XY SR
M E`XY D E^XT SR M E^XT D E]XQ SR M E]XQ D EWXO SR M EWXO D EPXO SR
M EPXO D EJXQ SR M EJXQ D EIXT SR M EIXT D EGXY SR M EGXY D EGX[ SR
M EGX[ D EIX] SR M EIX] D EJX[ SR M EJX[ D EIXY SR M E]Xg D E^X` SR
M E^X` D E^XY SR M E^XY D E]XT SR M E]XT D E[XQ SR M E[XQ D EWXO SR
M By]s D B?]w SR M B?]w D CH^C SR M CH^C D CH\n SR M CE]? D CE\n SR
M By\n D CT\n SR M C?^C D Cv]? SR M Cv]? D Cp]s SR M Cp]s D Cl]_ SR
M Cl]_ D Cl]R SR M Cl]R D Cp\~ SR M Cp\~ D Cv\r SR M Cv\r D C?\n SR
M C?\n D DE\n SR M DE\n D DN\r SR M DN\r D DT\~ SR M DT\~ D DW]R SR
M DW]R D DW]_ SR M DW]_ D DT]s SR M DT]s D DN]? SR M DN]? D DE^C SR
M DE^C D C?^C SR M C?^C D Cy]? SR M Cy]? D Cv]{ SR M Cv]{ D Cs]s SR
M Cs]s D Cp]_ SR M Cp]_ D Cp]R SR M Cp]R D Cs\~ SR M Cs\~ D Cv\v SR
M Cv\v D Cy\r SR M Cy\r D C?\n SR M DE\n D DK\r SR M DK\r D DN\v SR
M DN\v D DQ\~ SR M DQ\~ D DT]R SR M DT]R D DT]_ SR M DT]_ D DQ]s SR
M DQ]s D DN]{ SR M DN]{ D DK]? SR M DK]? D DE^C SR M EW^k D EW]} SR
M EY^p D EY]} SR M EY^p D EE^L SR M EE^L D Eb^L SR M ER]} D E^]} SR
M Byca D B?ce SR M B?ce D CHcq SR M CHcq D CHb] SR M CEcm D CEb] SR
M Byb] D CTb] SR M C?cq D Cvcm SR M Cvcm D Cpca SR M Cpca D ClcM SR
M ClcM D ClcA SR M ClcA D Cpbm SR M Cpbm D Cvba SR M Cvba D C?b] SR
M C?b] D DEb] SR M DEb] D DNba SR M DNba D DTbm SR M DTbm D DWcA SR
M DWcA D DWcM SR M DWcM D DTca SR M DTca D DNcm SR M DNcm D DEcq SR
M DEcq D C?cq SR M C?cq D Cycm SR M Cycm D Cvci SR M Cvci D Csca SR
M Csca D CpcM SR M CpcM D CpcA SR M CpcA D Csbm SR M Csbm D Cvbe SR
M Cvbe D Cyba SR M Cyba D C?b] SR M DEb] D DKba SR M DKba D DNbe SR
M DNbe D DQbm SR M DQbm D DTcA SR M DTcA D DTcM SR M DTcM D DQca SR
M DQca D DNci SR M DNci D DKcm SR M DKcm D DEcq SR M EJd_ D EGdF SR
M EGdF D EJdI SR M EJdI D EPdK SR M EPdK D EUdK SR M EUdK D E[dI SR
M E[dI D E^dD SR M E^dD D E`c} SR M E`c} D E`cz SR M E`cz D E^cs SR
M E^cs D E[cn SR M E[cn D EUcl SR M EUcl D EPcl SR M EPcl D EJcn SR
M EJcn D EIcq SR M EIcq D EGcu SR M EGcu D EGcx SR M EGcx D EIcz SR
M EIcz D EJcx SR M EJcx D EIcu SR M EUdK D EYdI SR M EYdI D E]dD SR
M E]dD D E^c} SR M E^c} D E^cz SR M E^cz D E]cs SR M E]cs D EYcn SR
M EYcn D EUcl SR M EJd_ D E]d_ SR M EJd\ D ESd\ SR M ESd\ D E]d_ SR
M ByiP D B?iT SR M B?iT D CHi` SR M CHi` D CHhK SR M CEi\ D CEhK SR
M ByhK D CThK SR M C?i` D Cvi\ SR M Cvi\ D CpiP SR M CpiP D Clh{ SR
M Clh{ D Clho SR M Clho D Cph[ SR M Cph[ D CvhO SR M CvhO D C?hK SR
M C?hK D DEhK SR M DEhK D DNhO SR M DNhO D DTh[ SR M DTh[ D DWho SR
M DWho D DWh{ SR M DWh{ D DTiP SR M DTiP D DNi\ SR M DNi\ D DEi` SR
M DEi` D C?i` SR M C?i` D Cyi\ SR M Cyi\ D CviX SR M CviX D CsiP SR
M CsiP D Cph{ SR M Cph{ D Cpho SR M Cpho D Csh[ SR M Csh[ D CvhS SR
M CvhS D CyhO SR M CyhO D C?hK SR M DEhK D DKhO SR M DKhO D DNhS SR
M DNhS D DQh[ SR M DQh[ D DTho SR M DTho D DTh{ SR M DTh{ D DQiP SR
M DQiP D DNiX SR M DNiX D DKi\ SR M DKi\ D DEi` SR M E]jF D E[jC SR
M E[jC D E]jA SR M E]jA D E^jC SR M E^jC D E^jF SR M E^jF D E]jJ SR
M E]jJ D EYjM SR M EYjM D ESjM SR M ESjM D ENjJ SR M ENjJ D EJjF SR
M EJjF D EIjA SR M EIjA D EGiw SR M EGiw D EGii SR M EGii D EIia SR
M EIia D ELi\ SR M ELi\ D ERiZ SR M ERiZ D EUiZ SR M EUiZ D E[i\ SR
M E[i\ D E^ia SR M E^ia D E`ii SR M E`ii D E`ik SR M E`ik D E^ir SR
M E^ir D E[iw SR M E[iw D EUiz SR M EUiz D ESiz SR M ESiz D ENiw SR
M ENiw D EJir SR M EJir D EIik SR M ESjM D EPjJ SR M EPjJ D ELjF SR
M ELjF D EJjA SR M EJjA D EIiw SR M EIiw D EIii SR M EIii D EJia SR
M EJia D ENi\ SR M ENi\ D ERiZ SR M EUiZ D EYi\ SR M EYi\ D E]ia SR
M E]ia D E^ii SR M E^ii D E^ik SR M E^ik D E]ir SR M E]ir D EYiw SR
M EYiw D EUiz SR M Byn~ D B?oB SR M B?oB D CHoN SR M CHoN D CHmy SR
M CEoJ D CEmy SR M Bymy D CTmy SR M C?oN D CvoJ SR M CvoJ D Cpn~ SR
M Cpn~ D Clnj SR M Clnj D Cln^ SR M Cln^ D CpnI SR M CpnI D Cvm} SR
M Cvm} D C?my SR M C?my D DEmy SR M DEmy D DNm} SR M DNm} D DTnI SR
M DTnI D DWn^ SR M DWn^ D DWnj SR M DWnj D DTn~ SR M DTn~ D DNoJ SR
M DNoJ D DEoN SR M DEoN D C?oN SR M C?oN D CyoJ SR M CyoJ D CvoF SR
M CvoF D Csn~ SR M Csn~ D Cpnj SR M Cpnj D Cpn^ SR M Cpn^ D CsnI SR
M CsnI D CvnA SR M CvnA D Cym} SR M Cym} D C?my SR M DEmy D DKm} SR
M DKm} D DNnA SR M DNnA D DQnI SR M DQnI D DTn^ SR M DTn^ D DTnj SR
M DTnj D DQn~ SR M DQn~ D DNoF SR M DNoF D DKoJ SR M DKoJ D DEoN SR
M EGo{ D EGom SR M EGor D EIov SR M EIov D ELo{ SR M ELo{ D EPo{ SR
M EPo{ D EYot SR M EYot D E]ot SR M E]ot D E^ov SR M E^ov D E`o{ SR
M EIov D ELoy SR M ELoy D EPoy SR M EPoy D EYot SR M E`o{ D E`ot SR
M E`ot D E^om SR M E^om D EWoa SR M EWoa D EUo\ SR M EUo\ D ESoU SR
M ESoU D ESoH SR M E^om D EUoa SR M EUoa D ESo\ SR M ESo\ D ERoU SR
M ERoU D ERoH SR M Bytl D B?tp SR M B?tp D CHt} SR M CHt} D CHsh SR
M CEty D CEsh SR M Bysh D CTsh SR M C?t} D Cvty SR M Cvty D Cptl SR
M Cptl D CltX SR M CltX D CltL SR M CltL D Cpsx SR M Cpsx D Cvsl SR
M Cvsl D C?sh SR M C?sh D DEsh SR M DEsh D DNsl SR M DNsl D DTsx SR
M DTsx D DWtL SR M DWtL D DWtX SR M DWtX D DTtl SR M DTtl D DNty SR
M DNty D DEt} SR M DEt} D C?t} SR M C?t} D Cyty SR M Cyty D Cvtt SR
M Cvtt D Cstl SR M Cstl D CptX SR M CptX D CptL SR M CptL D Cssx SR
M Cssx D Cvsp SR M Cvsp D Cysl SR M Cysl D C?sh SR M DEsh D DKsl SR
M DKsl D DNsp SR M DNsp D DQsx SR M DQsx D DTtL SR M DTtL D DTtX SR
M DTtX D DQtl SR M DQtl D DNtt SR M DNtt D DKty SR M DKty D DEt} SR
M EPuj D EJug SR M EJug D EIub SR M EIub D EIu[ SR M EIu[ D EJuV SR
M EJuV D EPuT SR M EPuT D EWuT SR M EWuT D E]uV SR M E]uV D E^u[ SR
M E^u[ D E^ub SR M E^ub D E]ug SR M E]ug D EWuj SR M EWuj D EPuj SR
M EPuj D ELug SR M ELug D EJub SR M EJub D EJu[ SR M EJu[ D ELuV SR
M ELuV D EPuT SR M EWuT D E[uV SR M E[uV D E]u[ SR M E]u[ D E]ub SR
M E]ub D E[ug SR M E[ug D EWuj SR M EPuT D EJuR SR M EJuR D EIuO SR
M EIuO D EGuJ SR M EGuJ D EGuA SR M EGuA D EIt| SR M EIt| D EJty SR
M EJty D EPtw SR M EPtw D EWtw SR M EWtw D E]ty SR M E]ty D E^t| SR
M E^t| D E`uA SR M E`uA D E`uJ SR M E`uJ D E^uO SR M E^uO D E]uR SR
M E]uR D EWuT SR M EPuT D ELuR SR M ELuR D EJuO SR M EJuO D EIuJ SR
M EIuJ D EIuA SR M EIuA D EJt| SR M EJt| D ELty SR M ELty D EPtw SR
M EWtw D E[ty SR M E[ty D E]t| SR M E]t| D E^uA SR M E^uA D E^uJ SR
M E^uJ D E]uO SR M E]uO D E[uR SR M E[uR D EWuT SR M Byz[ D B?z_ SR
M B?z_ D CHzk SR M CHzk D CHyV SR M CEzg D CEyV SR M ByyV D CTyV SR
M C?zk D Cvzg SR M Cvzg D Cpz[ SR M Cpz[ D ClzG SR M ClzG D Clyz SR
M Clyz D Cpyf SR M Cpyf D CvyZ SR M CvyZ D C?yV SR M C?yV D DEyV SR
M DEyV D DNyZ SR M DNyZ D DTyf SR M DTyf D DWyz SR M DWyz D DWzG SR
M DWzG D DTz[ SR M DTz[ D DNzg SR M DNzg D DEzk SR M DEzk D C?zk SR
M C?zk D Cyzg SR M Cyzg D Cvzc SR M Cvzc D Csz[ SR M Csz[ D CpzG SR
M CpzG D Cpyz SR M Cpyz D Csyf SR M Csyf D Cvy^ SR M Cvy^ D CyyZ SR
M CyyZ D C?yV SR M DEyV D DKyZ SR M DKyZ D DNy^ SR M DNy^ D DQyf SR
M DQyf D DTyz SR M DTyz D DTzG SR M DTzG D DQz[ SR M DQz[ D DNzc SR
M DNzc D DKzg SR M DKzg D DEzk SR M E^{G D E]{@ SR M E]{@ D EYz{ SR
M EYz{ D ESzy SR M ESzy D ERzy SR M ERzy D ELz{ SR M ELz{ D EI{@ SR
M EI{@ D EG{G SR M EG{G D EG{J SR M EG{J D EI{Q SR M EI{Q D EL{V SR
M EL{V D ER{X SR M ER{X D EU{X SR M EU{X D E[{V SR M E[{V D E^{Q SR
M E^{Q D E`{J SR M E`{J D E`z{ SR M E`z{ D E^zq SR M E^zq D E]zm SR
M E]zm D EYzh SR M EYzh D ESze SR M ESze D ENze SR M ENze D EJzh SR
M EJzh D EIzm SR M EIzm D EIzo SR M EIzo D EJzq SR M EJzq D ELzo SR
M ELzo D EJzm SR M ERzy D ENz{ SR M ENz{ D EJ{@ SR M EJ{@ D EI{G SR
M EI{G D EI{J SR M EI{J D EJ{Q SR M EJ{Q D EN{V SR M EN{V D ER{X SR
M EU{X D EY{V SR M EY{V D E]{Q SR M E]{Q D E^{J SR M E^{J D E^z{ SR
M E^z{ D E]zq SR M E]zq D E[zm SR M E[zm D EWzh SR M EWzh D ESze SR
M |rFY D |r|r SR M |rFY D |RFY SR M |rFY D {rFY SR M |rHG D |RHG SR
M |rIH D |RIH SR M |rIu D |RIu SR M |rJY D |RJY SR M |rJv D |RJv SR
M |rKN D |RKN SR M |rKd D |RKd SR M |rKv D |RKv SR M |rLG D |RLG SR
M |rLG D {rLG SR M |rMv D |RMv SR M |rNv D |RNv SR M |rOd D |ROd SR
M |rPG D |RPG SR M |rPd D |RPd SR M |rP} D |RP} SR M |rQR D |RQR SR
M |rQe D |RQe SR M |rQv D |RQv SR M |rQv D {rQv SR M |rSd D |RSd SR
M |rTd D |RTd SR M |rUR D |RUR SR M |rUv D |RUv SR M |rVS D |RVS SR
M |rVk D |RVk SR M |rWA D |RWA SR M |rWS D |RWS SR M |rWd D |RWd SR
M |rWd D {rWd SR M |rYR D |RYR SR M |rZS D |RZS SR M |r[A D |R[A SR
M |r[d D |R[d SR M |r\A D |R\A SR M |r\Z D |R\Z SR M |r\o D |R\o SR
M |r]B D |R]B SR M |r]R D |R]R SR M |r]R D {r]R SR M |r_A D |R_A SR
M |r`A D |R`A SR M |r`o D |R`o SR M |raS D |RaS SR M |rap D |Rap SR
M |rbH D |RbH SR M |rb] D |Rb] SR M |rbp D |Rbp SR M |rcA D |RcA SR
M |rcA D {rcA SR M |rdo D |Rdo SR M |rep D |Rep SR M |rf] D |Rf] SR
M |rgA D |RgA SR M |rg^ D |Rg^ SR M |rgv D |Rgv SR M |rhL D |RhL SR
M |rh^ D |Rh^ SR M |rho D |Rho SR M |rho D {rho SR M |rj^ D |Rj^ SR
M |rk^ D |Rk^ SR M |rlL D |RlL SR M |rlo D |Rlo SR M |rmL D |RmL SR
M |rme D |Rme SR M |rmz D |Rmz SR M |rnM D |RnM SR M |rn^ D |Rn^ SR
M |rn^ D {rn^ SR M |rpL D |RpL SR M |rqL D |RqL SR M |rqz D |Rqz SR
M |rr^ D |Rr^ SR M |rr{ D |Rr{ SR M |rsS D |RsS SR M |rsi D |Rsi SR
M |rs{ D |Rs{ SR M |rtL D |RtL SR M |rtL D {rtL SR M |ruz D |Ruz SR
M |rv{ D |Rv{ SR M |rwi D |Rwi SR M |rxL D |RxL SR M |rxi D |Rxi SR
M |ryB D |RyB SR M |ryW D |RyW SR M |ryj D |Ryj SR M |ryz D |Ryz SR
M |ryz D {ryz SR M |r{i D |R{i SR M |r|i D |R|i SR
M @^Ub D @dUf SR M @dUf D @TUf SR M @TUf D @^Ub SR M @^Ub D @WUZ SR
M @WUZ D @TUN SR M @TUN D @TUF SR M @TUF D @WTz SR M @WTz D @^Tq SR
M @^Tq D @dTm SR M @dTm D @mTi SR M @mTi D @|Ti SR M @|Ti D AETm SR
M AETm D AKTq SR M AKTq D AQTz SR M AQTz D ATUF SR M ATUF D ATUN SR
M ATUN D AQUZ SR M AQUZ D AKUb SR M AKUb D AEUf SR M @TUF D @WT~ SR
M @WT~ D @^Tv SR M @^Tv D @dTq SR M @dTq D @mTm SR M @mTm D @|Tm SR
M @|Tm D AETq SR M AETq D AKTv SR M AKTv D AQT~ SR M AQT~ D ATUF SR
M @jVV D @mVJ SR M @mVJ D @sVB SR M @sVB D @|U~ SR M @|U~ D ABU~ SR
M ABU~ D AKVB SR M AKVB D AQVJ SR M AQVJ D ATVV SR M ATVV D ATV^ SR
M ATV^ D AQVk SR M AQVk D AKVs SR M AKVs D ABVw SR M ABVw D @|Vw SR
M @|Vw D @sVs SR M @sVs D @mVk SR M @mVk D @jV^ SR M @jV^ D @jVV SR
M @jVV D @mVN SR M @mVN D @sVF SR M @sVF D @|VB SR M @|VB D ABVB SR
M ABVB D AKVF SR M AKVF D AQVN SR M AQVN D ATVV SR M ATV^ D AQVf SR
M AQVf D AKVo SR M AKVo D ABVs SR M ABVs D @|Vs SR M @|Vs D @sVo SR
M @sVo D @mVf SR M @mVf D @jV^ SR M @jWW D AKWW SR M AKWW D AQW[ SR
M AQW[ D ATWg SR M ATWg D ATWo SR M ATWo D AQW{ SR M AQW{ D AKXC SR
M @jW[ D AKW[ SR M AKW[ D AQW_ SR M AQW_ D ATWg SR M @jXC D ATXC SR
M @jXG D ATXG SR M @jWK D @jW[ SR M @jWw D @jXG SR M ATXC D ATXS SR
M @jXp D ATXp SR M @jXt D ATXt SR M @sXt D @mX| SR M @mX| D @jYH SR
M @jYH D @jYP SR M @jYP D @mY\ SR M @mY\ D @sY` SR M @sY` D ATY` SR
M @jYP D @mYX SR M @mYX D @sY\ SR M @sY\ D ATY\ SR M @jXd D @jXt SR
M ATXd D ATY@ SR M ATYP D ATYl SR M @TZH D AHZH SR M AHZH D AQZM SR
M AQZM D ATZU SR M ATZU D ATZ] SR M ATZ] D AQZe SR M AQZe D AKZi SR
M @TZM D AHZM SR M AHZM D AQZQ SR M AQZQ D ATZU SR M @jY| D @jZ] SR
M @T\N D AT\N SR M @T\R D AT\R SR M @T\A D @T\r SR M @T\r D @W\~ SR
M @W\~ D @Z]B SR M @Z]B D @a]F SR M @a]F D @g]F SR M @g]F D @m]B SR
M @m]B D @p\~ SR M @p\~ D @s\r SR M @s\r D @s\R SR M @T\r D @W\z SR
M @W\z D @Z\~ SR M @Z\~ D @a]B SR M @a]B D @g]B SR M @g]B D @m\~ SR
M @m\~ D @p\z SR M @p\z D @s\r SR M AT\A D AT\^ SR M @s\j D AN\z SR
M AN\z D AT]B SR M AT]B D AT]J SR M AT]J D AN]N SR M @s\j D @y\r SR
M @y\r D AT]B SR M @p]f D @s]f SR M @s]f D @s]b SR M @s]b D @p]b SR
M @p]b D @m]f SR M @m]f D @j]n SR M @j]n D @j]? SR M @j]? D @m^G SR
M @m^G D @p^K SR M @p^K D @v^O SR M @v^O D AK^O SR M AK^O D AQ^S SR
M AQ^S D AT^W SR M @p^K D AK^K SR M AK^K D AQ^O SR M AQ^O D AT^W SR
M AT^W D AT^[ SR M @v^K D @y^G SR M @y^G D @|]n SR M @|]n D @?]b SR
M @?]b D AE]^ SR M AE]^ D AK]^ SR M AK]^ D AQ]b SR M AQ]b D AT]n SR
M AT]n D AT]z SR M AT]z D AQ^C SR M AQ^C D AK^K SR M @|]n D @?]f SR
M @?]f D AE]b SR M AE]b D AK]b SR M AK]b D AQ]f SR M AQ]f D AT]n SR
M @T^w D AH^w SR M AH^w D AQ^{ SR M AQ^{ D AT_C SR M AT_C D AT_K SR
M AT_K D AQ_S SR M AQ_S D AK_W SR M @T^{ D AH^{ SR M AH^{ D AQ^? SR
M AQ^? D AT_C SR M @j^k D @j_K SR M @|_p D @|`` SR M @|`` D @v`` SR
M @v`` D @p`\ SR M @p`\ D @m`X SR M @m`X D @j`P SR M @j`P D @j`D SR
M @j`D D @m_x SR M @m_x D @s_p SR M @s_p D @|_k SR M @|_k D AB_k SR
M AB_k D AK_p SR M AK_p D AQ_x SR M AQ_x D AT`D SR M AT`D D AT`L SR
M AT`L D AQ`X SR M AQ`X D AK`` SR M @|`\ D @s`\ SR M @s`\ D @m`X SR
M @j`D D @m_| SR M @m_| D @s_t SR M @s_t D @|_p SR M @|_p D AB_p SR
M AB_p D AK_t SR M AK_t D AQ_| SR M AQ_| D AT`D SR M @Hba D @NbY SR
M @NbY D @WbQ SR M @WbQ D @dbI SR M @dbI D @sbE SR M @sbE D @?bE SR
M @?bE D ANbI SR M ANbI D AZbQ SR M AZbQ D AdbY SR M AdbY D Ajba SR
M @NbY D @ZbQ SR M @ZbQ D @dbM SR M @dbM D @sbI SR M @sbI D @?bI SR
M @?bI D ANbM SR M ANbM D AWbQ SR M AWbQ D AdbY SR M @scj D @vcf SR
M @vcf D @ycj SR M @ycj D @vcn SR M @vcn D @scn SR M @scn D @mcf SR
M @mcf D @jc^ SR M @jc^ D @jcQ SR M @jcQ D @mcE SR M @mcE D @sb} SR
M @sb} D @|by SR M @|by D ABby SR M ABby D AKb} SR M AKb} D AQcE SR
M AQcE D ATcQ SR M ATcQ D ATcZ SR M ATcZ D AQcf SR M AQcf D AKcn SR
M @jcQ D @mcI SR M @mcI D @scA SR M @scA D @|b} SR M @|b} D ABb} SR
M ABb} D AKcA SR M AKcA D AQcI SR M AQcI D ATcQ SR M @jd^ D @mdR SR
M @mdR D @sdJ SR M @sdJ D @|dF SR M @|dF D ABdF SR M ABdF D AKdJ SR
M AKdJ D AQdR SR M AQdR D ATd^ SR M ATd^ D ATdf SR M ATdf D AQdr SR
M AQdr D AKdz SR M AKdz D ABd~ SR M ABd~ D @|d~ SR M @|d~ D @sdz SR
M @sdz D @mdr SR M @mdr D @jdf SR M @jdf D @jd^ SR M @jd^ D @mdV SR
M @mdV D @sdN SR M @sdN D @|dJ SR M @|dJ D ABdJ SR M ABdJ D AKdN SR
M AKdN D AQdV SR M AQdV D ATd^ SR M ATdf D AQdn SR M AQdn D AKdv SR
M AKdv D ABdz SR M ABdz D @|dz SR M @|dz D @sdv SR M @sdv D @mdn SR
M @mdn D @jdf SR M @je_ D AKe_ SR M AKe_ D AQec SR M AQec D ATeo SR
M ATeo D ATew SR M ATew D AQfC SR M AQfC D AKfK SR M @jec D AKec SR
M AKec D AQeg SR M AQeg D ATeo SR M @jfK D ATfK SR M @jfO D ATfO SR
M @jeR D @jec SR M @je? D @jfO SR M ATfK D ATf[ SR M @jfw D ATfw SR
M @jf{ D ATf{ SR M @sf{ D @mgC SR M @mgC D @jgP SR M @jgP D @jgX SR
M @jgX D @mgd SR M @mgd D @sgh SR M @sgh D ATgh SR M @jgX D @mg` SR
M @mg` D @sgd SR M @sgd D ATgd SR M @jfk D @jf{ SR M ATfk D ATgH SR
M ATgX D ATgt SR M @ThP D AHhP SR M AHhP D AQhT SR M AQhT D ATh\ SR
M ATh\ D AThd SR M AThd D AQhl SR M AQhl D AKhp SR M @ThT D AHhT SR
M AHhT D AQhX SR M AQhX D ATh\ SR M @jhD D @jhd SR M @mim D @jiq SR
M @jiq D @siq SR M @siq D @mim SR M @mim D @jia SR M @jia D @jiU SR
M @jiU D @miI SR M @miI D @piE SR M @piE D @siE SR M @siE D @yiI SR
M @yiI D @|iQ SR M @|iQ D ABie SR M ABie D AEim SR M AEim D AHiq SR
M @siE D @viI SR M @viI D @yiQ SR M @yiQ D @?ie SR M @?ie D ABim SR
M ABim D AHiq SR M AHiq D ANiq SR M ANiq D AQim SR M AQim D ATia SR
M ATia D ATiU SR M ATiU D AQiI SR M AQiI D AKiE SR M AKiE D ATiE SR
M ATiE D AQiI SR M @mkz D @jk~ SR M @jk~ D @sk~ SR M @sk~ D @mkz SR
M @mkz D @jkn SR M @jkn D @jkb SR M @jkb D @mkV SR M @mkV D @pkR SR
M @pkR D @skR SR M @skR D @ykV SR M @ykV D @|k^ SR M @|k^ D ABkr SR
M ABkr D AEkz SR M AEkz D AHk~ SR M @skR D @vkV SR M @vkV D @yk^ SR
M @yk^ D @?kr SR M @?kr D ABkz SR M ABkz D AHk~ SR M AHk~ D ANk~ SR
M ANk~ D AQkz SR M AQkz D ATkn SR M ATkn D ATkb SR M ATkb D AQkV SR
M AQkV D AKkR SR M AKkR D ATkR SR M ATkR D AQkV SR M @HlR D @Hl} SR
M @@mS D @@mX SR M @@mX D @@m_ SR M @@m_ D @Ym_ SR M @@m] D @Ym] SR
M @YmS D @Ymi SR M @HnA D @NnI SR M @NnI D @WnQ SR M @WnQ D @dnY SR
M @dnY D @sn] SR M @sn] D @?n] SR M @?n] D ANnY SR M ANnY D AZnQ SR
M AZnQ D AdnI SR M AdnI D AjnA SR M @NnI D @ZnQ SR M @ZnQ D @dnU SR
M @dnU D @snY SR M @snY D @?nY SR M @?nY D ANnU SR M ANnU D AWnQ SR
M AWnQ D AdnI SR
M _bBo D _\Bg SR M _\Bg D _VB[ SR M _VB[ D _PBK SR M _PBK D _MAw SR
M _MAw D _MAg SR M _MAg D _PAR SR M _PAR D _VAB SR M _VAB D _\@v SR
M _\@v D _b@n SR M _\Bg D _VBW SR M _VBW D _SBK SR M _SBK D _PAw SR
M _PAw D _PAg SR M _PAg D _SAR SR M _SAR D _VAF SR M _VAF D _\@v SR
M _{B_ D _{AJ SR M _~B_ D _~AJ SR M _rB_ D `VB_ SR M `VB_ D `_B[ SR
M `_B[ D `bBW SR M `bBW D `eBO SR M `eBO D `eBG SR M `eBG D `bA? SR
M `bA? D `_A{ SR M `_A{ D `VAw SR M `VB_ D `\B[ SR M `\B[ D `_BW SR
M `_BW D `bBO SR M `bBO D `bBG SR M `bBG D `_A? SR M `_A? D `\A{ SR
M `\A{ D `VAw SR M _~Aw D `VAw SR M `VAw D `_As SR M `_As D `bAo SR
M `bAo D `eAg SR M `eAg D `eAZ SR M `eAZ D `bAR SR M `bAR D `_AN SR
M `_AN D `VAJ SR M `VAJ D _rAJ SR M `VAw D `\As SR M `\As D `_Ao SR
M `_Ao D `bAg SR M `bAg D `bAZ SR M `bAZ D `_AR SR M `_AR D `\AN SR
M `\AN D `VAJ SR M `xAo D anAo SR M bDB_ D bYAJ SR M bGB_ D bYAV SR
M bnB_ D bYAJ SR M a{B_ D bPB_ SR M beB_ D bxB_ SR M cDBo D cJBg SR
M cJBg D cPB[ SR M cPB[ D cVBK SR M cVBK D cYAw SR M cYAw D cYAg SR
M cYAg D cVAR SR M cVAR D cPAB SR M cPAB D cJ@v SR M cJ@v D cD@n SR
M cJBg D cPBW SR M cPBW D cSBK SR M cSBK D cVAw SR M cVAw D cVAg SR
M cVAg D cSAR SR M cSAR D cPAF SR M cPAF D cJ@v SR M cvAe D cpAb SR
M cpAb D cmA[ SR M cmA[ D ckAO SR M ckAO D ckAH SR M ckAH D cm@| SR
M cm@| D cp@t SR M cp@t D cv@r SR M cv@r D cy@r SR M cy@r D c?@t SR
M c?@t D dC@| SR M dC@| D dDAH SR M dDAH D dDAO SR M dDAO D dCA[ SR
M dCA[ D c?Ab SR M c?Ab D cyAe SR M cyAe D cvAe SR M cvAe D crAb SR
M crAb D cpA` SR M cpA` D cnA[ SR M cnA[ D cmAO SR M cmAO D cmAH SR
M cmAH D cn@| SR M cn@| D cp@w SR M cp@w D cr@t SR M cr@t D cv@r SR
M cy@r D c}@t SR M c}@t D c?@w SR M c?@w D dA@| SR M dA@| D dCAH SR
M dCAH D dCAO SR M dCAO D dAA[ SR M dAA[ D c?A` SR M c?A` D c}Ab SR
M c}Ab D cyAe SR
M mboX D mbmr SR M meoX D nQm| SR M meoN D nQmr SR M nQoX D nQmr SR
M mWoX D meoX SR M nFoX D n\oX SR M mWmr D mmmr SR M nyoD D o@oI SR
M o@oI D oKoX SR M oKoX D oKmr SR M oHoS D oHmr SR M nymr D oZmr SR
M HUyS D JQwo D LNvK D NJth D PFsE D RCqb D S?o? D U{n] D Wxl{ D YtkY
D [piw D ]mhV D _ifu D aeeT D cbct D e^bT D gZ`t D iV_U D kS]u D mO\V
D oKZx D qHYY D sDW{ D u@V] D v}U@ SR
M yOUf D yHUc SR M yHUc D yCUY SR M yCUY D y@UI SR M y@UI D y@T? SR
M y@T? D yCTo SR M yCTo D yHTe SR M yHTe D yOTb SR M yOTb D yTTb SR
M yTTb D y[Te SR M y[Te D y`To SR M y`To D ybT? SR M ybT? D ybUI SR
M ybUI D y`UY SR M y`UY D y[Uc SR M y[Uc D yTUf SR M yTUf D yOUf SR
M yOUf D yJUc SR M yJUc D yHU` SR M yHU` D yEUY SR M yEUY D yCUI SR
M yCUI D yCT? SR M yCT? D yETo SR M yETo D yHTi SR M yHTi D yJTe SR
M yJTe D yOTb SR M yTTb D yYTe SR M yYTe D y[Ti SR M y[Ti D y^To SR
M y^To D y`T? SR M y`T? D y`UI SR M y`UI D y^UY SR M y^UY D y[U` SR
M y[U` D yYUc SR M yYUc D yTUf SR M ytTi D yqTe SR M yqTe D ytTb SR
M ytTb D yvTe SR M yvTe D ytTi SR M zSUf D zLUc SR M zLUc D zGUY SR
M zGUY D zEUI SR M zEUI D zET? SR M zET? D zGTo SR M zGTo D zLTe SR
M zLTe D zSTb SR M zSTb D zXTb SR M zXTb D z_Te SR M z_Te D zdTo SR
M zdTo D zgT? SR M zgT? D zgUI SR M zgUI D zdUY SR M zdUY D z_Uc SR
M z_Uc D zXUf SR M zXUf D zSUf SR M zSUf D zNUc SR M zNUc D zLU` SR
M zLU` D zIUY SR M zIUY D zGUI SR M zGUI D zGT? SR M zGT? D zITo SR
M zITo D zLTi SR M zLTi D zNTe SR M zNTe D zSTb SR M zXTb D z]Te SR
M z]Te D z_Ti SR M z_Ti D zbTo SR M zbTo D zdT? SR M zdT? D zdUI SR
M zdUI D zbUY SR M zbUY D z_U` SR M z_U` D z]Uc SR M z]Uc D zXUf SR
M HUwS D JQup D LNtN D NJrl D PFqJ D RCoh D S?nF D U{le D WxkD D Ytib
D [phB D ]mfa D _ie@ D aec` D cbb@ D e^`` D gZ_@ D iV]` D kS\A D mOZb
D oKYC D qHWd D sDVE D u@Tf D v}SH SR
M yOSm D yHSj SR M yHSj D yCS` SR M yCS` D y@SP SR M y@SP D y@SF SR
M y@SF D yCRv SR M yCRv D yHRl SR M yHRl D yORi SR M yORi D yTRi SR
M yTRi D y[Rl SR M y[Rl D y`Rv SR M y`Rv D ybSF SR M ybSF D ybSP SR
M ybSP D y`S` SR M y`S` D y[Sj SR M y[Sj D yTSm SR M yTSm D yOSm SR
M yOSm D yJSj SR M yJSj D yHSg SR M yHSg D yES` SR M yES` D yCSP SR
M yCSP D yCSF SR M yCSF D yERv SR M yERv D yHRp SR M yHRp D yJRl SR
M yJRl D yORi SR M yTRi D yYRl SR M yYRl D y[Rp SR M y[Rp D y^Rv SR
M y^Rv D y`SF SR M y`SF D y`SP SR M y`SP D y^S` SR M y^S` D y[Sg SR
M y[Sg D yYSj SR M yYSj D yTSm SR M ytRp D yqRl SR M yqRl D ytRi SR
M ytRi D yvRl SR M yvRl D ytRp SR M zLS` D zQSc SR M zQSc D zXSm SR
M zXSm D zXRi SR M zVSj D zVRi SR M zLRi D zbRi SR
M HUuQ D JQsp D LNrO D NJpo D PFoN D RCmn D S?lN D U{jn D WxiN D Ytgo
D [pfO D ]mdp D _icQ D aeaq D cb`R D e^^t D gZ]U D iV[v D kSZX D mOXy
D oKW[ D qHU} D sDT_ D u@SA D v}Qd SR
M yORJ D yHRG SR M yHRG D yCQ} SR M yCQ} D y@Qm SR M y@Qm D y@Qc SR
M y@Qc D yCQS SR M yCQS D yHQJ SR M yHQJ D yOQF SR M yOQF D yTQF SR
M yTQF D y[QJ SR M y[QJ D y`QS SR M y`QS D ybQc SR M ybQc D ybQm SR
M ybQm D y`Q} SR M y`Q} D y[RG SR M y[RG D yTRJ SR M yTRJ D yORJ SR
M yORJ D yJRG SR M yJRG D yHRD SR M yHRD D yEQ} SR M yEQ} D yCQm SR
M yCQm D yCQc SR M yCQc D yEQS SR M yEQS D yHQM SR M yHQM D yJQJ SR
M yJQJ D yOQF SR M yTQF D yYQJ SR M yYQJ D y[QM SR M y[QM D y^QS SR
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M zIRG D zQRJ SR M zQRJ D z[RJ SR M z[RJ D zbRG SR M zbRG D zdRD SR
M zdRD D zgQ} SR M zgQ} D zgQw SR M zgQw D zdQp SR M zdQp D z]Qj SR
M z]Qj D zQQc SR M zQQc D zLQ` SR M zLQ` D zGQZ SR M zGQZ D zEQP SR
M zEQP D zEQF SR M z[RJ D z_RG SR M z_RG D zbRD SR M zbRD D zdQ} SR
M zdQ} D zdQw SR M zdQw D zbQp SR M zbQp D z[Qj SR M z[Qj D zQQc SR
M zEQM D zGQP SR M zGQP D zLQP SR M zLQP D zXQJ SR M zXQJ D z_QJ SR
M z_QJ D zdQM SR M zdQM D zgQP SR M zLQP D zXQF SR M zXQF D zbQF SR
M zbQF D zdQJ SR M zdQJ D zgQP SR M zgQP D zgQW SR
M HUsR D JQqs D LNpS D NJnt D PFmU D RCku D S?jV D U{hw D WxgX D Ytey
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M yOPU D yHPR SR M yHPR D yCPH SR M yCPH D y@Ox SR M y@Ox D y@On SR
M y@On D yCO^ SR M yCO^ D yHOT SR M yHOT D yOOQ SR M yOOQ D yTOQ SR
M yTOQ D y[OT SR M y[OT D y`O^ SR M y`O^ D ybOn SR M ybOn D ybOx SR
M ybOx D y`PH SR M y`PH D y[PR SR M y[PR D yTPU SR M yTPU D yOPU SR
M yOPU D yJPR SR M yJPR D yHPN SR M yHPN D yEPH SR M yEPH D yCOx SR
M yCOx D yCOn SR M yCOn D yEO^ SR M yEO^ D yHOX SR M yHOX D yJOT SR
M yJOT D yOOQ SR M yTOQ D yYOT SR M yYOT D y[OX SR M y[OX D y^O^ SR
M y^O^ D y`On SR M y`On D y`Ox SR M y`Ox D y^PH SR M y^PH D y[PN SR
M y[PN D yYPR SR M yYPR D yTPU SR M ytOX D yqOT SR M yqOT D ytOQ SR
M ytOQ D yvOT SR M yvOT D ytOX SR M zGPK D zIPH SR M zIPH D zGPE SR
M zGPE D zEPH SR M zEPH D zEPK SR M zEPK D zIPR SR M zIPR D zQPU SR
M zQPU D z[PU SR M z[PU D zbPR SR M zbPR D zdPK SR M zdPK D zdPB SR
M zdPB D zbO{ SR M zbO{ D z[Ox SR M z[Ox D zSOx SR M z[PU D z_PR SR
M z_PR D zbPK SR M zbPK D zbPB SR M zbPB D z_O{ SR M z_O{ D z[Ox SR
M z[Ox D z_Ou SR M z_Ou D zdOn SR M zdOn D zgOh SR M zgOh D zgO^ SR
M zgO^ D zdOX SR M zdOX D zbOT SR M zbOT D z[OQ SR M z[OQ D zQOQ SR
M zQOQ D zIOT SR M zIOT D zGOX SR M zGOX D zEO^ SR M zEO^ D zEOa SR
M zEOa D zGOe SR M zGOe D zIOa SR M zIOa D zGO^ SR M zbOq D zdOh SR
M zdOh D zdO^ SR M zdO^ D zbOX SR M zbOX D z_OT SR M z_OT D z[OQ SR
M HUqT D JQov D LNnX D NJly D PFk[ D RCi} D S?h^ D U{g@ D Wxea D YtdC
D [pbe D ]maF D _i_g D ae^I D cb\j D e^[L D gZYm D iVXN D kSVp D mOUQ
D oKSr D qHRS D sDPt D u@OV D v}Mw SR
M yON\ D yHNY SR M yHNY D yCNO SR M yCNO D y@M? SR M y@M? D y@Mu SR
M y@Mu D yCMe SR M yCMe D yHM[ SR M yHM[ D yOMX SR M yOMX D yTMX SR
M yTMX D y[M[ SR M y[M[ D y`Me SR M y`Me D ybMu SR M ybMu D ybM? SR
M ybM? D y`NO SR M y`NO D y[NY SR M y[NY D yTN\ SR M yTN\ D yON\ SR
M yON\ D yJNY SR M yJNY D yHNV SR M yHNV D yENO SR M yENO D yCM? SR
M yCM? D yCMu SR M yCMu D yEMe SR M yEMe D yHM_ SR M yHM_ D yJM[ SR
M yJM[ D yOMX SR M yTMX D yYM[ SR M yYM[ D y[M_ SR M y[M_ D y^Me SR
M y^Me D y`Mu SR M y`Mu D y`M? SR M y`M? D y^NO SR M y^NO D y[NV SR
M y[NV D yYNY SR M yYNY D yTN\ SR M ytM_ D yqM[ SR M yqM[ D ytMX SR
M ytMX D yvM[ SR M yvM[ D ytM_ SR M z[NV D z[MX SR M z]N\ D z]MX SR
M z]N\ D zBMl SR M zBMl D ziMl SR M zSMX D zdMX SR
M HUoW D JQmz D LNl] D NJj? D PFib D RChD D S?fg D U{eI D Wxck D YtbM
D [p`o D ]m_Q D _i]s D ae\U D cbZv D e^YX D gZWy D iVVZ D kST| D mOS]
D oKQ~ D qHP_ D sDN? D u@M` D v}LA SR
M yOLg D yHLc SR M yHLc D yCLZ SR M yCLZ D y@LJ SR M y@LJ D y@L@ SR
M y@L@ D yCKp SR M yCKp D yHKf SR M yHKf D yOKc SR M yOKc D yTKc SR
M yTKc D y[Kf SR M y[Kf D y`Kp SR M y`Kp D ybL@ SR M ybL@ D ybLJ SR
M ybLJ D y`LZ SR M y`LZ D y[Lc SR M y[Lc D yTLg SR M yTLg D yOLg SR
M yOLg D yJLc SR M yJLc D yHL` SR M yHL` D yELZ SR M yELZ D yCLJ SR
M yCLJ D yCL@ SR M yCL@ D yEKp SR M yEKp D yHKi SR M yHKi D yJKf SR
M yJKf D yOKc SR M yTKc D yYKf SR M yYKf D y[Ki SR M y[Ki D y^Kp SR
M y^Kp D y`L@ SR M y`L@ D y`LJ SR M y`LJ D y^LZ SR M y^LZ D y[L` SR
M y[L` D yYLc SR M yYLc D yTLg SR M ytKi D yqKf SR M yqKf D ytKc SR
M ytKc D yvKf SR M yvKf D ytKi SR M zILg D zELF SR M zELF D zILJ SR
M zILJ D zQLM SR M zQLM D zXLM SR M zXLM D z_LJ SR M z_LJ D zdLC SR
M zdLC D zgKz SR M zgKz D zgKv SR M zgKv D zdKm SR M zdKm D z_Kf SR
M z_Kf D zXKc SR M zXKc D zQKc SR M zQKc D zIKf SR M zIKf D zGKi SR
M zGKi D zEKp SR M zEKp D zEKs SR M zEKs D zGKv SR M zGKv D zIKs SR
M zIKs D zGKp SR M zXLM D z]LJ SR M z]LJ D zbLC SR M zbLC D zdKz SR
M zdKz D zdKv SR M zdKv D zbKm SR M zbKm D z]Kf SR M z]Kf D zXKc SR
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%PSKCloseWorkStation
%PSKOpenWorkStation
CL
%%Trailer
R
%DocumentFonts: Times-Bold Times-Italic Symbol Times-Roman
%%Pages: 1
%%EOF

%%EndDocument
FMENDEPSF
0 56 29 576 727 208 279.2 74 424.4 FMBEGINEPSF
%%BeginDocument: /pongo/data2/drs/ghrs/handbook/ih5/figs/mirror_n2.epsi
%!PS-Adobe-2.0 EPSF-1.2
%%BoundingBox: 56 29 576 727
%!PS-Adobe-1.0
%%Creator: PSIKern - An IRAF GKI Translator
%%CreationDate: Thu 15:08:26 28-Apr-94
%%DocumentFonts: (atend)
%%Pages: (atend)
%%BoundingBox: 28 28 583 763
%%EndComments
/MAXNDC 4095 def /PageSizeXMeter 0.2594 def /PageSizeYMeter 0.1959 def
/PageOffXMeter 0.01 def /PageOffYMeter 0.01 def
/PortraitMode false def /PortraitRotation 0. def
/LandScapeRotation 90. def /GT_LEFT 2 def /GT_RIGHT 3 def
/GT_TOP 6 def /GT_BOTTOM 7 def /GT_UP 4 def /GT_DOWN 5 def
/GT_CENTER 1 def /RF /Times-Roman def /GF /Symbol def
/IF /Times-Italic def /BF /Times-Bold def /DASH 49 def /DOT 4 def
/SPACE 24 def

% How to define things.
/BD { bind def } bind def
/LD { load def } bind def

% Constants
/yes true def
/no false def

% Define some shorthand instructions.
/GRS /grestore LD
/GS /gsave LD
/MK /mark LD
/R /restore LD
/S /save LD
/SH /showpage LD
/SW /setlinewidth LD

% Measurement conversions.
/PointperMeter 2834.64 def
/MonoScale .7 def

% SR: Set current path to page: - -> -
/SR { currentpoint stroke moveto } BD

% CL: CLear the page: - -> -
/CL { restore showpage grestore gsave save } BD

% RC: Read Coordinates: string -> x y
/RC {
currentfile read pop 8#77 and 6 bitshift
currentfile read pop 8#77 and or
currentfile read pop 8#77 and 6 bitshift
currentfile read pop 8#77 and or
} BD

% DO - Determine Offset: length -> offset
/DO { DS dup 0 eq { pop pop 0 } { mod } ifelse } BD

% M: Move: M string -> -
% Move to a point and clear length of path.
/M { RC moveto CT OF setdash } BD

% D: Draw: D string -> -
% This also calculates the length of the current path.
/OF 0 def
/D { RC DS 0 ne { 2 copy currentpoint exch 4 1 roll sub dup mul 3 1 roll
sub dup mul add sqrt round OF add cvi DO /OF exch store } if lineto
} BD

% Character/Font definitions.

% FS -- Define the current font size: xsize ysize FS -
/FontXSize 0 def /FontYSize 0 def /NewFont true def
/FS { /FontYSize exch MonoScale mul store /FontXSize exch MonoScale mul store
/NewFont true store } BD

% PH -- Set the current path: path PH -
/Path 0 def
/PH { /Path exch store } BD

% PA -- Set the path angle of the text: angle PA -
/Angle 0 def
/PA { 360 mod dup 0 lt { 360 add } if /Angle exch store /NewFont true store } BD

% HJ, VJ -- Set Horizontal/Verticle Justification: just HJ/VJ -
/HorzJust 0 def /VertJust 0 def
/HJ { /HorzJust exch store } BD /VJ { /VertJust exch store } BD

% VT -- Use mono- or variable-spaced fonts: flag VT -
/VT true def
/VT { /Variable exch store } BD

% SetFont -- Make the required font the default: font SetFont -
% Note scale factor- This is to fill out monospaced better and match other
% IRAF output.
/Font () def
/FontMatrix matrix def
/SetFont {
dup Font ne NewFont or
{ dup /Font exch store findfont
Angle matrix rotate FontXSize MonoScale div FontYSize MonoScale div
matrix scale matrix concatmatrix makefont setfont Angle matrix rotate
FontXSize FontYSize matrix scale matrix concatmatrix /FontMatrix exch
store
}
{ pop } ifelse /NewFont false store
} BD

% StringWidth -- Determine path length of string: string StringWidth - xs ys
/StringWidth { Path GT_RIGHT eq Variable and { stringwidth }
{ Path GT_RIGHT eq { length } { pop 1 } ifelse 0 FontMatrix transform }
ifelse
} BD

% MonoShow -- Write the string out in mono-spaced: string MonoShow -
/MonoShow {
/t 1 string def 1 0 FontMatrix transform
/dy exch def /dx exch def Path GT_RIGHT eq { /mx dx def /my dy def }
{ 0 1 FontMatrix transform /my exch def /mx exch def } ifelse
{ t 0 3 -1 roll put t dup stringwidth dy exch sub 2 div exch dx exch
sub 2 div exch gsave rmoveto show grestore mx my rmoveto
} forall
} BD

% WS -- Draw the string: string font string ... DS -
/*WSDict 13 dict def
/WS { *WSDict begin
counttomark 2 idiv dup dup array /FontArray exch def
array /StringArray exch def 1 sub /NStrings exch def

NStrings -1 0 {
dup 4 1 roll exch StringArray 3 1 roll put FontArray 3 1 roll put
} for
pop

/XSize 0 def /YSize 0 def /NChars 0 def
0 1 NStrings {
dup FontArray exch get SetFont StringArray exch get dup
length NChars add /NChars exch def StringWidth
YSize add /YSize exch def XSize add /XSize exch def
} for

/TAngle HorzJust GT_RIGHT eq
{ Angle 180 add dup 360 ge { 360 sub } if } { Angle } ifelse def
0 TAngle 180 le HorzJust GT_CENTER eq or
{ Angle sin FontYSize mul Path GT_UP eq { NChars mul } if add } if
TAngle 90 ge TAngle 270 le and HorzJust GT_CENTER eq or
{ Path GT_RIGHT eq { XSize } { Angle cos FontXSize mul } ifelse sub } if
HorzJust GT_CENTER eq { .5 mul } if

/TAngle
VertJust GT_TOP eq { Angle 180 sub dup 0 lt { 360 add } if } { Angle } ifelse
def
0 TAngle 90 ge TAngle 270 le and VertJust GT_CENTER eq or
{ Angle cos FontYSize mul Path GT_UP eq { NChars mul } if sub } if
TAngle 180 ge TAngle 360 le and VertJust GT_CENTER eq or
{ Path GT_RIGHT eq { YSize } { Angle sin FontXSize mul } ifelse sub } if
VertJust GT_CENTER eq { .5 mul } if
rmoveto

0 1 NStrings {
dup FontArray exch get SetFont StringArray exch get
Path GT_RIGHT eq Variable and { show } { MonoShow } ifelse
} for

end
} BD

% Define the DASHED, DOTTED, DOTDASH patterns.
/DS 0 def
/LPS {
/OF 0 store /DS 0 store 0 array
} BD
/LPD {
/OF 0 store DASH SPACE 2 copy add /DS exch store 2 array astore
} BD
/LPP {
/OF 0 store DOT SPACE 2 copy add /DS exch store 2 array astore
} BD
/LDD {
/OF 0 store DOT SPACE DASH SPACE 4 copy add add add /DS exch store
4 array astore
} BD

% LT - Set Line Type - array -> -
/CT { currentdash pop } BD
/LT { /CT exch store /OF 0 store } BD

% SC - Set Color: color -> -
/*SCDict 1 dict def
/SC { *SCDict begin
1 sub /color exch def
GR color get 255 div GG color get 255 div GB color get 255 div setrgbcolor
end
} BD

% MI - Make Image LUT: table-name size MI hexstring -> -
/MI { currentfile exch string readhexstring pop def } BD

% Define the graphics color lookup table.
/GR 16 MI 00FFFF0000FF00FFFFB0FFF0D940F0F5
/GG 16 MI 00FF00FF00FFFF0080D0A6E670E082DE
/GB 16 MI 00FF0000FF00FFFF4F61008CD6D1EFB3

% Render an image when no image LUT has been define.
/DefaultGrey {
{ currentfile inarr readhexstring pop } image
} BD

% ColorImage - Produce an image by indexing into the Image Lookup Table.
% There are two versions of this code- one for PostScript that has
% the colorimage operator and one that doesn't. If the PostScript doesn't
% have colorimage, it is assumed that it can only produce black & white,
% in which the Image LUT is combined to produce a single grey which is
% then used as the image for the image operator.
/colorimage where
{ pop
/ColorImage {
{ currentfile inarr readhexstring pop dup /inarr exch def
length 3 mul string /oarr exch def
0 1 inarr length 1 sub
{ /iindex exch def
/oindex iindex 3 mul def
oarr oindex IR inarr iindex get get put
oarr oindex 1 add IG inarr iindex get get put
oarr oindex 2 add IB inarr iindex get get put
} for
oarr
}
false 3 colorimage
} BD
}
{ /ColorImage {
{ currentfile inarr readhexstring pop dup /inarr exch def
length string /oarr exch def
0 1 inarr length 1 sub
{ /iindex exch def
oarr iindex
IR inarr iindex get get 0.3 mul
IG inarr iindex get get 0.59 mul
IB inarr iindex get get 0.11 mul
add add round cvi dup 255 gt { pop 255 } if
put
} for
oarr
}
image
} BD
}
ifelse

% PC: Put Cellarray: width height bitspersample matrix -> -
/*PCdict 10 dict def
/PC {
*PCdict begin
4 -1 roll dup /inarr exch string def 4 1 roll
/IR where {pop ColorImage} {DefaultGrey} ifelse
end
} BD

% Define the Hatch (fill area) styles. H1 and H2 are handled internally
% by PSIKern. Feel free to define more; there is no limit.
/H3 <8888888888888888> def
/H4 def
/H5 <8844221188442211> def
/H6 <1122448811224488> def

% Setup for fill patterns. This whole section of code is taken almost
% directly from _PostScript Language: Tutorial and Cookbook_, Adobe Systems,
% 1986 (the blue book).
/setuserscreendict 22 dict def
setuserscreendict begin
/tempctm matrix def
/temprot matrix def
/tempscale matrix def

/concatprocs
{ /proc2 exch cvlit def
/proc1 exch cvlit def
/newproc proc1 length proc2 length add
array def
newproc 0 proc1 putinterval
newproc proc1 length proc2 putinterval
newproc cvx
} def

/resmatrix matrix def
/findresolution
{ 72 0 resmatrix defaultmatrix dtransform
/yres exch def /xres exch def
xres dup mul yres dup mul add sqrt
} def
end

/setuserscreen
{ setuserscreendict begin
/spotfunction exch def
/screenangle exch def
/cellsize exch def

/m tempctm currentmatrix def
/rm screenangle temprot rotate def
/sm cellsize dup tempscale scale def

sm rm m m concatmatrix m concatmatrix pop
1 0 m dtransform /y1 exch def /x1 exch def

/veclength x1 dup mul y1 dup mul add sqrt def
/frequency findresolution veclength div def

/newscreenangle y1 x1 atan def

m 2 get m 1 get mul m 0 get m 3 get mul sub
0 gt
{ {neg} /spotfunction load concatprocs
/spotfunction exch def
} if

frequency newscreenangle /spotfunction load
setscreen
end
} def

/setpatterndict 18 dict def
setpatterndict begin
/bitison
{ /ybit exch def /xbit exch def
/bytevalue bstring ybit bwidth mul xbit 8 idiv
add get def

/mask 1 7 xbit 8 mod sub bitshift def
bytevalue mask and 0 ne
} def
end

/bitpatternspotfunction
{ setpatterndict begin
/y exch def /x exch def

/xindex x 1 add 2 div bpside mul cvi def
/yindex y 1 add 2 div bpside mul cvi def

xindex yindex bitison
{ /onbits onbits 1 add def 1 }
{ /offbits offbits 1 add def 0 }
ifelse
end
} def

/setpattern
{ setpatterndict begin
/cellsz exch def
/angle exch def
/bwidth exch def
/bpside exch def
/bstring exch def

/onbits 0 def /offbits 0 def
cellsz angle /bitpatternspotfunction load
setuserscreen
{ } settransfer
offbits offbits onbits add div setgray
end
} def

% SP: Set Pattern: pattern -> -
/SP { 8 1 0 MAXNDC 100 div setpattern } BD

% FI: Fill with Pattern: - -> -
/FI { fill grestore } BD

% Set the transformation matrix.
PointperMeter dup scale
PageOffXMeter
PortraitMode not
{ PageSizeYMeter add }
if
PageOffYMeter translate
PortraitMode
{ PortraitRotation rotate }
{ LandScapeRotation rotate}
ifelse
PageSizeXMeter MAXNDC div PageSizeYMeter MAXNDC div scale
1 setlinejoin 1 setlinecap

% Save the current graphics state (to restore after showpage) and the
% VM state to recover after a showpage.
GS S

%%EndProlog
%PSKOpenWorkStation
%%Page: 1 1
LPS LT 3 SW 1 SC M FYFY D |rFY SR M FYFY D FYFy SR M IAFY D IAFy SR
M KiFY D KiFy SR M NQFY D NQFy SR M PzFY D PzGY SR M SbFY D SbFy SR
M VJFY D VJFy SR M XrFY D XrFy SR M [ZFY D [ZFy SR M ^BFY D ^BGY SR
M `jFY D `jFy SR M cSFY D cSFy SR M e{FY D e{Fy SR M hcFY D hcFy SR
M kKFY D kKGY SR M msFY D msFy SR M p[FY D p[Fy SR M sCFY D sCFy SR
M ulFY D ulFy SR M xTFY D xTGY SR M z|FY D z|Fy SR M PwEl D PmEh SR
M PmEh D PgE\ SR M PgE\ D PdEG SR M PdEG D PdD{ SR M PdD{ D PgDg SR
M PgDg D PmD[ SR M PmD[ D PwDW SR M PwDW D P}DW SR M P}DW D QFD[ SR
M QFD[ D QLDg SR M QLDg D QOD{ SR M QOD{ D QOEG SR M QOEG D QLE\ SR
M QLE\ D QFEh SR M QFEh D P}El SR M P}El D PwEl SR M PwEl D PpEh SR
M PpEh D PmEd SR M PmEd D PjE\ SR M PjE\ D PgEG SR M PgEG D PgD{ SR
M PgD{ D PjDg SR M PjDg D PmD_ SR M PmD_ D PpD[ SR M PpD[ D PwDW SR
M P}DW D QCD[ SR M QCD[ D QFD_ SR M QFD_ D QIDg SR M QIDg D QLD{ SR
M QLD{ D QLEG SR M QLEG D QIE\ SR M QIE\ D QFEd SR M QFEd D QCEh SR
M QCEh D P}El SR M ]UEl D ]KEh SR M ]KEh D ]EE\ SR M ]EE\ D ]BEG SR
M ]BEG D ]BD{ SR M ]BD{ D ]EDg SR M ]EDg D ]KD[ SR M ]KD[ D ]UDW SR
M ]UDW D ][DW SR M ][DW D ]dD[ SR M ]dD[ D ]jDg SR M ]jDg D ]mD{ SR
M ]mD{ D ]mEG SR M ]mEG D ]jE\ SR M ]jE\ D ]dEh SR M ]dEh D ][El SR
M ][El D ]UEl SR M ]UEl D ]NEh SR M ]NEh D ]KEd SR M ]KEd D ]HE\ SR
M ]HE\ D ]EEG SR M ]EEG D ]ED{ SR M ]ED{ D ]HDg SR M ]HDg D ]KD_ SR
M ]KD_ D ]ND[ SR M ]ND[ D ]UDW SR M ][DW D ]aD[ SR M ]aD[ D ]dD_ SR
M ]dD_ D ]gDg SR M ]gDg D ]jD{ SR M ]jD{ D ]jEG SR M ]jEG D ]gE\ SR
M ]gE\ D ]dEd SR M ]dEd D ]aEh SR M ]aEh D ][El SR M ^BD_ D ]?D[ SR
M ]?D[ D ^BDW SR M ^BDW D ^ED[ SR M ^ED[ D ^BD_ SR M ^^El D ^XEC SR
M ^XEC D ^^EG SR M ^^EG D ^gEL SR M ^gEL D ^pEL SR M ^pEL D ^yEG SR
M ^yEG D ^?D? SR M ^?D? D _BDs SR M _BDs D _BDo SR M _BDo D ^?Dc SR
M ^?Dc D ^yD[ SR M ^yD[ D ^pDW SR M ^pDW D ^gDW SR M ^gDW D ^^D[ SR
M ^^D[ D ^[D_ SR M ^[D_ D ^XDg SR M ^XDg D ^XDk SR M ^XDk D ^[Do SR
M ^[Do D ^^Dk SR M ^^Dk D ^[Dg SR M ^pEL D ^vEG SR M ^vEG D ^|D? SR
M ^|D? D ^?Ds SR M ^?Ds D ^?Do SR M ^?Do D ^|Dc SR M ^|Dc D ^vD[ SR
M ^vD[ D ^pDW SR M ^^El D ^|El SR M ^^Eh D ^mEh SR M ^mEh D ^|El SR
M j?E\ D kEE` SR M kEE` D kNEl SR M kNEl D kNDW SR M kKEh D kKDW SR
M j?DW D kZDW SR M w]E\ D wcE` SR M wcE` D wlEl SR M wlEl D wlDW SR
M wiEh D wiDW SR M w]DW D wxDW SR M xTD_ D xQD[ SR M xQD[ D xTDW SR
M xTDW D xWD[ SR M xWD[ D xTD_ SR M xoEl D xiEC SR M xiEC D xoEG SR
M xoEG D xxEL SR M xxEL D yAEL SR M yAEL D yKEG SR M yKEG D yQD? SR
M yQD? D yTDs SR M yTDs D yTDo SR M yTDo D yQDc SR M yQDc D yKD[ SR
M yKD[ D yADW SR M yADW D xxDW SR M xxDW D xoD[ SR M xoD[ D xlD_ SR
M xlD_ D xiDg SR M xiDg D xiDk SR M xiDk D xlDo SR M xlDo D xoDk SR
M xoDk D xlDg SR M yAEL D yHEG SR M yHEG D yND? SR M yND? D yQDs SR
M yQDs D yQDo SR M yQDo D yNDc SR M yNDc D yHD[ SR M yHD[ D yADW SR
M xoEl D yNEl SR M xoEh D x~Eh SR M x~Eh D yNEl SR M FY|r D |r|r SR
M FY|r D FY|R SR M IA|r D IA|R SR M Ki|r D Ki|R SR M NQ|r D NQ|R SR
M Pz|r D Pz{r SR M Sb|r D Sb|R SR M VJ|r D VJ|R SR M Xr|r D Xr|R SR
M [Z|r D [Z|R SR M ^B|r D ^B{r SR M `j|r D `j|R SR M cS|r D cS|R SR
M e{|r D e{|R SR M hc|r D hc|R SR M kK|r D kK{r SR M ms|r D ms|R SR
M p[|r D p[|R SR M sC|r D sC|R SR M ul|r D ul|R SR M xT|r D xT{r SR
M z||r D z||R SR M FYFY D FY|r SR M FYGT D FyGT SR M FYHL D FyHL SR
M FYHz D FyHz SR M FYIa D FyIa SR M FYJC D FyJC SR M FYJ` D FyJ` SR
M FYJ{ D FyJ{ SR M FYJ{ D GYJ{ SR M FYMj D FyMj SR M FYOP D FyOP SR
M FYPX D FyPX SR M FYQP D FyQP SR M FYQ~ D FyQ~ SR M FYRe D FyRe SR
M FYSG D FySG SR M FYSd D FySd SR M FYS? D FyS? SR M FYS? D GYS? SR
M FYVn D FyVn SR M FYXT D FyXT SR M FYY\ D FyY\ SR M FYZU D FyZU SR
M FY[C D Fy[C SR M FY[i D Fy[i SR M FY\K D Fy\K SR M FY\i D Fy\i SR
M FY]C D Fy]C SR M FY]C D GY]C SR M FY_r D Fy_r SR M FYaX D FyaX SR
M FYb` D Fyb` SR M FYcY D FycY SR M FYdG D FydG SR M FYdm D Fydm SR
M FYeO D FyeO SR M FYem D Fyem SR M FYfG D FyfG SR M FYfG D GYfG SR
M FYhv D Fyhv SR M FYj\ D Fyj\ SR M FYke D Fyke SR M FYl] D Fyl] SR
M FYmK D FymK SR M FYmq D Fymq SR M FYnS D FynS SR M FYnq D Fynq SR
M FYoK D FyoK SR M FYoK D GYoK SR M FYqz D Fyqz SR M FYs` D Fys` SR
M FYti D Fyti SR M FYua D Fyua SR M FYvO D FyvO SR M FYvv D Fyvv SR
M FYwW D FywW SR M FYwu D Fywu SR M FYxO D FyxO SR M FYxO D GYxO SR
M FYz~ D Fyz~ SR M FY|d D Fy|d SR M ByK[ D B?K_ SR M B?K_ D CHKk SR
M CHKk D CHJW SR M CEKg D CEJW SR M ByJW D CTJW SR M C?Kk D CvKg SR
M CvKg D CpK[ SR M CpK[ D ClKG SR M ClKG D ClJ{ SR M ClJ{ D CpJg SR
M CpJg D CvJ[ SR M CvJ[ D C?JW SR M C?JW D DEJW SR M DEJW D DNJ[ SR
M DNJ[ D DTJg SR M DTJg D DWJ{ SR M DWJ{ D DWKG SR M DWKG D DTK[ SR
M DTK[ D DNKg SR M DNKg D DEKk SR M DEKk D C?Kk SR M C?Kk D CyKg SR
M CyKg D CvKc SR M CvKc D CsK[ SR M CsK[ D CpKG SR M CpKG D CpJ{ SR
M CpJ{ D CsJg SR M CsJg D CvJ_ SR M CvJ_ D CyJ[ SR M CyJ[ D C?JW SR
M DEJW D DKJ[ SR M DKJ[ D DNJ_ SR M DNJ_ D DQJg SR M DQJg D DTJ{ SR
M DTJ{ D DTKG SR M DTKG D DQK[ SR M DQK[ D DNKc SR M DNKc D DKKg SR
M DKKg D DEKk SR M EJLY D EGL@ SR M EGL@ D EJLC SR M EJLC D EPLE SR
M EPLE D EULE SR M EULE D E[LC SR M E[LC D E^K~ SR M E^K~ D E`Kw SR
M E`Kw D E`Kt SR M E`Kt D E^Km SR M E^Km D E[Kh SR M E[Kh D EUKf SR
M EUKf D EPKf SR M EPKf D EJKh SR M EJKh D EIKk SR M EIKk D EGKo SR
M EGKo D EGKr SR M EGKr D EIKt SR M EIKt D EJKr SR M EJKr D EIKo SR
M EULE D EYLC SR M EYLC D E]K~ SR M E]K~ D E^Kw SR M E^Kw D E^Kt SR
M E^Kt D E]Km SR M E]Km D EYKh SR M EYKh D EUKf SR M EJLY D E]LY SR
M EJLV D ESLV SR M ESLV D E]LY SR M ByT_ D B?Tc SR M B?Tc D CHTp SR
M CHTp D CHS[ SR M CETk D CES[ SR M ByS[ D CTS[ SR M C?Tp D CvTk SR
M CvTk D CpT_ SR M CpT_ D ClTK SR M ClTK D ClS? SR M ClS? D CpSk SR
M CpSk D CvS_ SR M CvS_ D C?S[ SR M C?S[ D DES[ SR M DES[ D DNS_ SR
M DNS_ D DTSk SR M DTSk D DWS? SR M DWS? D DWTK SR M DWTK D DTT_ SR
M DTT_ D DNTk SR M DNTk D DETp SR M DETp D C?Tp SR M C?Tp D CyTk SR
M CyTk D CvTg SR M CvTg D CsT_ SR M CsT_ D CpTK SR M CpTK D CpS? SR
M CpS? D CsSk SR M CsSk D CvSc SR M CvSc D CyS_ SR M CyS_ D C?S[ SR
M DES[ D DKS_ SR M DKS_ D DNSc SR M DNSc D DQSk SR M DQSk D DTS? SR
M DTS? D DTTK SR M DTTK D DQT_ SR M DQT_ D DNTg SR M DNTg D DKTk SR
M DKTk D DETp SR M E]UU D E[US SR M E[US D E]UQ SR M E]UQ D E^US SR
M E^US D E^UU SR M E^UU D E]UZ SR M E]UZ D EYU] SR M EYU] D ESU] SR
M ESU] D ENUZ SR M ENUZ D EJUU SR M EJUU D EIUQ SR M EIUQ D EGUG SR
M EGUG D EGTx SR M EGTx D EITq SR M EITq D ELTl SR M ELTl D ERTj SR
M ERTj D EUTj SR M EUTj D E[Tl SR M E[Tl D E^Tq SR M E^Tq D E`Tx SR
M E`Tx D E`T{ SR M E`T{ D E^UB SR M E^UB D E[UG SR M E[UG D EUUI SR
M EUUI D ESUI SR M ESUI D ENUG SR M ENUG D EJUB SR M EJUB D EIT{ SR
M ESU] D EPUZ SR M EPUZ D ELUU SR M ELUU D EJUQ SR M EJUQ D EIUG SR
M EIUG D EITx SR M EITx D EJTq SR M EJTq D ENTl SR M ENTl D ERTj SR
M EUTj D EYTl SR M EYTl D E]Tq SR M E]Tq D E^Tx SR M E^Tx D E^T{ SR
M E^T{ D E]UB SR M E]UB D EYUG SR M EYUG D EUUI SR M By]c D B?]h SR
M B?]h D CH]t SR M CH]t D CH\_ SR M CE]p D CE\_ SR M By\_ D CT\_ SR
M C?]t D Cv]p SR M Cv]p D Cp]c SR M Cp]c D Cl]O SR M Cl]O D Cl]C SR
M Cl]C D Cp\o SR M Cp\o D Cv\c SR M Cv\c D C?\_ SR M C?\_ D DE\_ SR
M DE\_ D DN\c SR M DN\c D DT\o SR M DT\o D DW]C SR M DW]C D DW]O SR
M DW]O D DT]c SR M DT]c D DN]p SR M DN]p D DE]t SR M DE]t D C?]t SR
M C?]t D Cy]p SR M Cy]p D Cv]l SR M Cv]l D Cs]c SR M Cs]c D Cp]O SR
M Cp]O D Cp]C SR M Cp]C D Cs\o SR M Cs\o D Cv\g SR M Cv\g D Cy\c SR
M Cy\c D C?\_ SR M DE\_ D DK\c SR M DK\c D DN\g SR M DN\g D DQ\o SR
M DQ\o D DT]C SR M DT]C D DT]O SR M DT]O D DQ]c SR M DQ]c D DN]l SR
M DN]l D DK]p SR M DK]p D DE]t SR M EG^a D EG^R SR M EG^W D EI^\ SR
M EI^\ D EL^a SR M EL^a D EP^a SR M EP^a D EY^Z SR M EY^Z D E]^Z SR
M E]^Z D E^^\ SR M E^^\ D E`^a SR M EI^\ D EL^^ SR M EL^^ D EP^^ SR
M EP^^ D EY^Z SR M E`^a D E`^Z SR M E`^Z D E^^R SR M E^^R D EW^F SR
M EW^F D EU^A SR M EU^A D ES]z SR M ES]z D ES]n SR M E^^R D EU^F SR
M EU^F D ES^A SR M ES^A D ER]z SR M ER]z D ER]n SR M Byfh D B?fl SR
M B?fl D CHfx SR M CHfx D CHec SR M CEft D CEec SR M Byec D CTec SR
M C?fx D Cvft SR M Cvft D Cpfh SR M Cpfh D ClfS SR M ClfS D ClfG SR
M ClfG D Cpes SR M Cpes D Cveg SR M Cveg D C?ec SR M C?ec D DEec SR
M DEec D DNeg SR M DNeg D DTes SR M DTes D DWfG SR M DWfG D DWfS SR
M DWfS D DTfh SR M DTfh D DNft SR M DNft D DEfx SR M DEfx D C?fx SR
M C?fx D Cyft SR M Cyft D Cvfp SR M Cvfp D Csfh SR M Csfh D CpfS SR
M CpfS D CpfG SR M CpfG D Cses SR M Cses D Cvek SR M Cvek D Cyeg SR
M Cyeg D C?ec SR M DEec D DKeg SR M DKeg D DNek SR M DNek D DQes SR
M DQes D DTfG SR M DTfG D DTfS SR M DTfS D DQfh SR M DQfh D DNfp SR
M DNfp D DKft SR M DKft D DEfx SR M EPge D EJgc SR M EJgc D EIg^ SR
M EIg^ D EIgV SR M EIgV D EJgR SR M EJgR D EPgO SR M EPgO D EWgO SR
M EWgO D E]gR SR M E]gR D E^gV SR M E^gV D E^g^ SR M E^g^ D E]gc SR
M E]gc D EWge SR M EWge D EPge SR M EPge D ELgc SR M ELgc D EJg^ SR
M EJg^ D EJgV SR M EJgV D ELgR SR M ELgR D EPgO SR M EWgO D E[gR SR
M E[gR D E]gV SR M E]gV D E]g^ SR M E]g^ D E[gc SR M E[gc D EWge SR
M EPgO D EJgM SR M EJgM D EIgJ SR M EIgJ D EGgE SR M EGgE D EGf| SR
M EGf| D EIfw SR M EIfw D EJfu SR M EJfu D EPfr SR M EPfr D EWfr SR
M EWfr D E]fu SR M E]fu D E^fw SR M E^fw D E`f| SR M E`f| D E`gE SR
M E`gE D E^gJ SR M E^gJ D E]gM SR M E]gM D EWgO SR M EPgO D ELgM SR
M ELgM D EJgJ SR M EJgJ D EIgE SR M EIgE D EIf| SR M EIf| D EJfw SR
M EJfw D ELfu SR M ELfu D EPfr SR M EWfr D E[fu SR M E[fu D E]fw SR
M E]fw D E^f| SR M E^f| D E^gE SR M E^gE D E]gJ SR M E]gJ D E[gM SR
M E[gM D EWgO SR M Byol D B?op SR M B?op D CHo| SR M CHo| D CHng SR
M CEox D CEng SR M Byng D CTng SR M C?o| D Cvox SR M Cvox D Cpol SR
M Cpol D CloX SR M CloX D CloK SR M CloK D Cpnw SR M Cpnw D Cvnk SR
M Cvnk D C?ng SR M C?ng D DEng SR M DEng D DNnk SR M DNnk D DTnw SR
M DTnw D DWoK SR M DWoK D DWoX SR M DWoX D DTol SR M DTol D DNox SR
M DNox D DEo| SR M DEo| D C?o| SR M C?o| D Cyox SR M Cyox D Cvot SR
M Cvot D Csol SR M Csol D CpoX SR M CpoX D CpoK SR M CpoK D Csnw SR
M Csnw D Cvno SR M Cvno D Cynk SR M Cynk D C?ng SR M DEng D DKnk SR
M DKnk D DNno SR M DNno D DQnw SR M DQnw D DToK SR M DToK D DToX SR
M DToX D DQol SR M DQol D DNot SR M DNot D DKox SR M DKox D DEo| SR
M E^pX D E]pQ SR M E]pQ D EYpL SR M EYpL D ESpJ SR M ESpJ D ERpJ SR
M ERpJ D ELpL SR M ELpL D EIpQ SR M EIpQ D EGpX SR M EGpX D EGp[ SR
M EGp[ D EIpb SR M EIpb D ELpg SR M ELpg D ERpi SR M ERpi D EUpi SR
M EUpi D E[pg SR M E[pg D E^pb SR M E^pb D E`p[ SR M E`p[ D E`pL SR
M E`pL D E^pB SR M E^pB D E]o} SR M E]o} D EYoy SR M EYoy D ESov SR
M ESov D ENov SR M ENov D EJoy SR M EJoy D EIo} SR M EIo} D EIp@ SR
M EIp@ D EJpB SR M EJpB D ELp@ SR M ELp@ D EJo} SR M ERpJ D ENpL SR
M ENpL D EJpQ SR M EJpQ D EIpX SR M EIpX D EIp[ SR M EIp[ D EJpb SR
M EJpb D ENpg SR M ENpg D ERpi SR M EUpi D EYpg SR M EYpg D E]pb SR
M E]pb D E^p[ SR M E^p[ D E^pL SR M E^pL D E]pB SR M E]pB D E[o} SR
M E[o} D EWoy SR M EWoy D ESov SR M Buxp D B{xt SR M B{xt D CDy@ SR
M CDy@ D CDwk SR M CAx| D CAwk SR M Buwk D CPwk SR M C{y@ D Crx| SR
M Crx| D Clxp SR M Clxp D Cix\ SR M Cix\ D CixP SR M CixP D Clw{ SR
M Clw{ D Crwo SR M Crwo D C{wk SR M C{wk D DAwk SR M DAwk D DJwo SR
M DJwo D DPw{ SR M DPw{ D DSxP SR M DSxP D DSx\ SR M DSx\ D DPxp SR
M DPxp D DJx| SR M DJx| D DAy@ SR M DAy@ D C{y@ SR M C{y@ D Cux| SR
M Cux| D Crxx SR M Crxx D Coxp SR M Coxp D Clx\ SR M Clx\ D ClxP SR
M ClxP D Cow{ SR M Cow{ D Crws SR M Crws D Cuwo SR M Cuwo D C{wk SR
M DAwk D DGwo SR M DGwo D DJws SR M DJws D DMw{ SR M DMw{ D DPxP SR
M DPxP D DPx\ SR M DPx\ D DMxp SR M DMxp D DJxx SR M DJxx D DGx| SR
M DGx| D DAy@ SR M Dhyd D Dkyf SR M Dkyf D Dqym SR M Dqym D Dqxz SR
M Doyk D Doxz SR M Dhxz D Dxxz SR M ERym D ELyk SR M ELyk D EIyd SR
M EIyd D EGyW SR M EGyW D EGyP SR M EGyP D EIyD SR M EIyD D ELx} SR
M ELx} D ERxz SR M ERxz D EUxz SR M EUxz D E[x} SR M E[x} D E^yD SR
M E^yD D E`yP SR M E`yP D E`yW SR M E`yW D E^yd SR M E^yd D E[yk SR
M E[yk D EUym SR M EUym D ERym SR M ERym D ENyk SR M ENyk D ELyh SR
M ELyh D EJyd SR M EJyd D EIyW SR M EIyW D EIyP SR M EIyP D EJyD SR
M EJyD D ELx? SR M ELx? D ENx} SR M ENx} D ERxz SR M EUxz D EYx} SR
M EYx} D E[x? SR M E[x? D E]yD SR M E]yD D E^yP SR M E^yP D E^yW SR
M E^yW D E]yd SR M E]yd D E[yh SR M E[yh D EYyk SR M EYyk D EUym SR
M |rFY D |r|r SR M |rGT D |RGT SR M |rHL D |RHL SR M |rHz D |RHz SR
M |rIa D |RIa SR M |rJC D |RJC SR M |rJ` D |RJ` SR M |rJ{ D |RJ{ SR
M |rJ{ D {rJ{ SR M |rMj D |RMj SR M |rOP D |ROP SR M |rPX D |RPX SR
M |rQP D |RQP SR M |rQ~ D |RQ~ SR M |rRe D |RRe SR M |rSG D |RSG SR
M |rSd D |RSd SR M |rS? D |RS? SR M |rS? D {rS? SR M |rVn D |RVn SR
M |rXT D |RXT SR M |rY\ D |RY\ SR M |rZU D |RZU SR M |r[C D |R[C SR
M |r[i D |R[i SR M |r\K D |R\K SR M |r\i D |R\i SR M |r]C D |R]C SR
M |r]C D {r]C SR M |r_r D |R_r SR M |raX D |RaX SR M |rb` D |Rb` SR
M |rcY D |RcY SR M |rdG D |RdG SR M |rdm D |Rdm SR M |reO D |ReO SR
M |rem D |Rem SR M |rfG D |RfG SR M |rfG D {rfG SR M |rhv D |Rhv SR
M |rj\ D |Rj\ SR M |rke D |Rke SR M |rl] D |Rl] SR M |rmK D |RmK SR
M |rmq D |Rmq SR M |rnS D |RnS SR M |rnq D |Rnq SR M |roK D |RoK SR
M |roK D {roK SR M |rqz D |Rqz SR M |rs` D |Rs` SR M |rti D |Rti SR
M |rua D |Rua SR M |rvO D |RvO SR M |rvv D |Rvv SR M |rwW D |RwW SR
M |rwu D |Rwu SR M |rxO D |RxO SR M |rxO D {rxO SR M |rz~ D |Rz~ SR
M |r|d D |R|d SR
M @^Ub D @dUf SR M @dUf D @TUf SR M @TUf D @^Ub SR M @^Ub D @WUZ SR
M @WUZ D @TUN SR M @TUN D @TUF SR M @TUF D @WTz SR M @WTz D @^Tq SR
M @^Tq D @dTm SR M @dTm D @mTi SR M @mTi D @|Ti SR M @|Ti D AETm SR
M AETm D AKTq SR M AKTq D AQTz SR M AQTz D ATUF SR M ATUF D ATUN SR
M ATUN D AQUZ SR M AQUZ D AKUb SR M AKUb D AEUf SR M @TUF D @WT~ SR
M @WT~ D @^Tv SR M @^Tv D @dTq SR M @dTq D @mTm SR M @mTm D @|Tm SR
M @|Tm D AETq SR M AETq D AKTv SR M AKTv D AQT~ SR M AQT~ D ATUF SR
M @jVV D @mVJ SR M @mVJ D @sVB SR M @sVB D @|U~ SR M @|U~ D ABU~ SR
M ABU~ D AKVB SR M AKVB D AQVJ SR M AQVJ D ATVV SR M ATVV D ATV^ SR
M ATV^ D AQVk SR M AQVk D AKVs SR M AKVs D ABVw SR M ABVw D @|Vw SR
M @|Vw D @sVs SR M @sVs D @mVk SR M @mVk D @jV^ SR M @jV^ D @jVV SR
M @jVV D @mVN SR M @mVN D @sVF SR M @sVF D @|VB SR M @|VB D ABVB SR
M ABVB D AKVF SR M AKVF D AQVN SR M AQVN D ATVV SR M ATV^ D AQVf SR
M AQVf D AKVo SR M AKVo D ABVs SR M ABVs D @|Vs SR M @|Vs D @sVo SR
M @sVo D @mVf SR M @mVf D @jV^ SR M @jWW D AKWW SR M AKWW D AQW[ SR
M AQW[ D ATWg SR M ATWg D ATWo SR M ATWo D AQW{ SR M AQW{ D AKXC SR
M @jW[ D AKW[ SR M AKW[ D AQW_ SR M AQW_ D ATWg SR M @jXC D ATXC SR
M @jXG D ATXG SR M @jWK D @jW[ SR M @jWw D @jXG SR M ATXC D ATXS SR
M @jXp D ATXp SR M @jXt D ATXt SR M @sXt D @mX| SR M @mX| D @jYH SR
M @jYH D @jYP SR M @jYP D @mY\ SR M @mY\ D @sY` SR M @sY` D ATY` SR
M @jYP D @mYX SR M @mYX D @sY\ SR M @sY\ D ATY\ SR M @jXd D @jXt SR
M ATXd D ATY@ SR M ATYP D ATYl SR M @TZH D AHZH SR M AHZH D AQZM SR
M AQZM D ATZU SR M ATZU D ATZ] SR M ATZ] D AQZe SR M AQZe D AKZi SR
M @TZM D AHZM SR M AHZM D AQZQ SR M AQZQ D ATZU SR M @jY| D @jZ] SR
M @T\N D AT\N SR M @T\R D AT\R SR M @T\A D @T\r SR M @T\r D @W\~ SR
M @W\~ D @Z]B SR M @Z]B D @a]F SR M @a]F D @g]F SR M @g]F D @m]B SR
M @m]B D @p\~ SR M @p\~ D @s\r SR M @s\r D @s\R SR M @T\r D @W\z SR
M @W\z D @Z\~ SR M @Z\~ D @a]B SR M @a]B D @g]B SR M @g]B D @m\~ SR
M @m\~ D @p\z SR M @p\z D @s\r SR M AT\A D AT\^ SR M @s\j D AN\z SR
M AN\z D AT]B SR M AT]B D AT]J SR M AT]J D AN]N SR M @s\j D @y\r SR
M @y\r D AT]B SR M @p]f D @s]f SR M @s]f D @s]b SR M @s]b D @p]b SR
M @p]b D @m]f SR M @m]f D @j]n SR M @j]n D @j]? SR M @j]? D @m^G SR
M @m^G D @p^K SR M @p^K D @v^O SR M @v^O D AK^O SR M AK^O D AQ^S SR
M AQ^S D AT^W SR M @p^K D AK^K SR M AK^K D AQ^O SR M AQ^O D AT^W SR
M AT^W D AT^[ SR M @v^K D @y^G SR M @y^G D @|]n SR M @|]n D @?]b SR
M @?]b D AE]^ SR M AE]^ D AK]^ SR M AK]^ D AQ]b SR M AQ]b D AT]n SR
M AT]n D AT]z SR M AT]z D AQ^C SR M AQ^C D AK^K SR M @|]n D @?]f SR
M @?]f D AE]b SR M AE]b D AK]b SR M AK]b D AQ]f SR M AQ]f D AT]n SR
M @T^w D AH^w SR M AH^w D AQ^{ SR M AQ^{ D AT_C SR M AT_C D AT_K SR
M AT_K D AQ_S SR M AQ_S D AK_W SR M @T^{ D AH^{ SR M AH^{ D AQ^? SR
M AQ^? D AT_C SR M @j^k D @j_K SR M @|_p D @|`` SR M @|`` D @v`` SR
M @v`` D @p`\ SR M @p`\ D @m`X SR M @m`X D @j`P SR M @j`P D @j`D SR
M @j`D D @m_x SR M @m_x D @s_p SR M @s_p D @|_k SR M @|_k D AB_k SR
M AB_k D AK_p SR M AK_p D AQ_x SR M AQ_x D AT`D SR M AT`D D AT`L SR
M AT`L D AQ`X SR M AQ`X D AK`` SR M @|`\ D @s`\ SR M @s`\ D @m`X SR
M @j`D D @m_| SR M @m_| D @s_t SR M @s_t D @|_p SR M @|_p D AB_p SR
M AB_p D AK_t SR M AK_t D AQ_| SR M AQ_| D AT`D SR M @Hba D @NbY SR
M @NbY D @WbQ SR M @WbQ D @dbI SR M @dbI D @sbE SR M @sbE D @?bE SR
M @?bE D ANbI SR M ANbI D AZbQ SR M AZbQ D AdbY SR M AdbY D Ajba SR
M @NbY D @ZbQ SR M @ZbQ D @dbM SR M @dbM D @sbI SR M @sbI D @?bI SR
M @?bI D ANbM SR M ANbM D AWbQ SR M AWbQ D AdbY SR M @scj D @vcf SR
M @vcf D @ycj SR M @ycj D @vcn SR M @vcn D @scn SR M @scn D @mcf SR
M @mcf D @jc^ SR M @jc^ D @jcQ SR M @jcQ D @mcE SR M @mcE D @sb} SR
M @sb} D @|by SR M @|by D ABby SR M ABby D AKb} SR M AKb} D AQcE SR
M AQcE D ATcQ SR M ATcQ D ATcZ SR M ATcZ D AQcf SR M AQcf D AKcn SR
M @jcQ D @mcI SR M @mcI D @scA SR M @scA D @|b} SR M @|b} D ABb} SR
M ABb} D AKcA SR M AKcA D AQcI SR M AQcI D ATcQ SR M @jd^ D @mdR SR
M @mdR D @sdJ SR M @sdJ D @|dF SR M @|dF D ABdF SR M ABdF D AKdJ SR
M AKdJ D AQdR SR M AQdR D ATd^ SR M ATd^ D ATdf SR M ATdf D AQdr SR
M AQdr D AKdz SR M AKdz D ABd~ SR M ABd~ D @|d~ SR M @|d~ D @sdz SR
M @sdz D @mdr SR M @mdr D @jdf SR M @jdf D @jd^ SR M @jd^ D @mdV SR
M @mdV D @sdN SR M @sdN D @|dJ SR M @|dJ D ABdJ SR M ABdJ D AKdN SR
M AKdN D AQdV SR M AQdV D ATd^ SR M ATdf D AQdn SR M AQdn D AKdv SR
M AKdv D ABdz SR M ABdz D @|dz SR M @|dz D @sdv SR M @sdv D @mdn SR
M @mdn D @jdf SR M @je_ D AKe_ SR M AKe_ D AQec SR M AQec D ATeo SR
M ATeo D ATew SR M ATew D AQfC SR M AQfC D AKfK SR M @jec D AKec SR
M AKec D AQeg SR M AQeg D ATeo SR M @jfK D ATfK SR M @jfO D ATfO SR
M @jeR D @jec SR M @je? D @jfO SR M ATfK D ATf[ SR M @jfw D ATfw SR
M @jf{ D ATf{ SR M @sf{ D @mgC SR M @mgC D @jgP SR M @jgP D @jgX SR
M @jgX D @mgd SR M @mgd D @sgh SR M @sgh D ATgh SR M @jgX D @mg` SR
M @mg` D @sgd SR M @sgd D ATgd SR M @jfk D @jf{ SR M ATfk D ATgH SR
M ATgX D ATgt SR M @ThP D AHhP SR M AHhP D AQhT SR M AQhT D ATh\ SR
M ATh\ D AThd SR M AThd D AQhl SR M AQhl D AKhp SR M @ThT D AHhT SR
M AHhT D AQhX SR M AQhX D ATh\ SR M @jhD D @jhd SR M @mim D @jiq SR
M @jiq D @siq SR M @siq D @mim SR M @mim D @jia SR M @jia D @jiU SR
M @jiU D @miI SR M @miI D @piE SR M @piE D @siE SR M @siE D @yiI SR
M @yiI D @|iQ SR M @|iQ D ABie SR M ABie D AEim SR M AEim D AHiq SR
M @siE D @viI SR M @viI D @yiQ SR M @yiQ D @?ie SR M @?ie D ABim SR
M ABim D AHiq SR M AHiq D ANiq SR M ANiq D AQim SR M AQim D ATia SR
M ATia D ATiU SR M ATiU D AQiI SR M AQiI D AKiE SR M AKiE D ATiE SR
M ATiE D AQiI SR M @mkz D @jk~ SR M @jk~ D @sk~ SR M @sk~ D @mkz SR
M @mkz D @jkn SR M @jkn D @jkb SR M @jkb D @mkV SR M @mkV D @pkR SR
M @pkR D @skR SR M @skR D @ykV SR M @ykV D @|k^ SR M @|k^ D ABkr SR
M ABkr D AEkz SR M AEkz D AHk~ SR M @skR D @vkV SR M @vkV D @yk^ SR
M @yk^ D @?kr SR M @?kr D ABkz SR M ABkz D AHk~ SR M AHk~ D ANk~ SR
M ANk~ D AQkz SR M AQkz D ATkn SR M ATkn D ATkb SR M ATkb D AQkV SR
M AQkV D AKkR SR M AKkR D ATkR SR M ATkR D AQkV SR M @HlR D @Hl} SR
M @@mS D @@mX SR M @@mX D @@m_ SR M @@m_ D @Ym_ SR M @@m] D @Ym] SR
M @YmS D @Ymi SR M @HnA D @NnI SR M @NnI D @WnQ SR M @WnQ D @dnY SR
M @dnY D @sn] SR M @sn] D @?n] SR M @?n] D ANnY SR M ANnY D AZnQ SR
M AZnQ D AdnI SR M AdnI D AjnA SR M @NnI D @ZnQ SR M @ZnQ D @dnU SR
M @dnU D @snY SR M @snY D @?nY SR M @?nY D ANnU SR M ANnU D AWnQ SR
M AWnQ D AdnI SR
M _bBo D _\Bg SR M _\Bg D _VB[ SR M _VB[ D _PBK SR M _PBK D _MAw SR
M _MAw D _MAg SR M _MAg D _PAR SR M _PAR D _VAB SR M _VAB D _\@v SR
M _\@v D _b@n SR M _\Bg D _VBW SR M _VBW D _SBK SR M _SBK D _PAw SR
M _PAw D _PAg SR M _PAg D _SAR SR M _SAR D _VAF SR M _VAF D _\@v SR
M _{B_ D _{AJ SR M _~B_ D _~AJ SR M _rB_ D `VB_ SR M `VB_ D `_B[ SR
M `_B[ D `bBW SR M `bBW D `eBO SR M `eBO D `eBG SR M `eBG D `bA? SR
M `bA? D `_A{ SR M `_A{ D `VAw SR M `VB_ D `\B[ SR M `\B[ D `_BW SR
M `_BW D `bBO SR M `bBO D `bBG SR M `bBG D `_A? SR M `_A? D `\A{ SR
M `\A{ D `VAw SR M _~Aw D `VAw SR M `VAw D `_As SR M `_As D `bAo SR
M `bAo D `eAg SR M `eAg D `eAZ SR M `eAZ D `bAR SR M `bAR D `_AN SR
M `_AN D `VAJ SR M `VAJ D _rAJ SR M `VAw D `\As SR M `\As D `_Ao SR
M `_Ao D `bAg SR M `bAg D `bAZ SR M `bAZ D `_AR SR M `_AR D `\AN SR
M `\AN D `VAJ SR M `xAo D anAo SR M bDB_ D bYAJ SR M bGB_ D bYAV SR
M bnB_ D bYAJ SR M a{B_ D bPB_ SR M beB_ D bxB_ SR M cDBo D cJBg SR
M cJBg D cPB[ SR M cPB[ D cVBK SR M cVBK D cYAw SR M cYAw D cYAg SR
M cYAg D cVAR SR M cVAR D cPAB SR M cPAB D cJ@v SR M cJ@v D cD@n SR
M cJBg D cPBW SR M cPBW D cSBK SR M cSBK D cVAw SR M cVAw D cVAg SR
M cVAg D cSAR SR M cSAR D cPAF SR M cPAF D cJ@v SR M cvAe D cpAb SR
M cpAb D cmA[ SR M cmA[ D ckAO SR M ckAO D ckAH SR M ckAH D cm@| SR
M cm@| D cp@t SR M cp@t D cv@r SR M cv@r D cy@r SR M cy@r D c?@t SR
M c?@t D dC@| SR M dC@| D dDAH SR M dDAH D dDAO SR M dDAO D dCA[ SR
M dCA[ D c?Ab SR M c?Ab D cyAe SR M cyAe D cvAe SR M cvAe D crAb SR
M crAb D cpA` SR M cpA` D cnA[ SR M cnA[ D cmAO SR M cmAO D cmAH SR
M cmAH D cn@| SR M cn@| D cp@w SR M cp@w D cr@t SR M cr@t D cv@r SR
M cy@r D c}@t SR M c}@t D c?@w SR M c?@w D dA@| SR M dA@| D dCAH SR
M dCAH D dCAO SR M dCAO D dAA[ SR M dAA[ D c?A` SR M c?A` D c}Ab SR
M c}Ab D cyAe SR
M k]pF D k]n` SR M kapF D lMnj SR M kao| D lMn` SR M lMpF D lMn` SR
M kRpF D kapF SR M lBpF D lXpF SR M kRn` D khn` SR M lnor D lqom SR
M lqom D lnoi SR M lnoi D ljom SR M ljom D ljor SR M ljor D lno| SR
M lno| D lqpA SR M lqpA D l|pF SR M l|pF D mKpF SR M mKpF D mVpA SR
M mVpA D mZo| SR M mZo| D m]or SR M m]or D m]oi SR M m]oi D mZo_ SR
M mZo_ D mOoU SR M mOoU D l|oK SR M l|oK D luoG SR M luoG D lnn} SR
M lnn} D ljnn SR M ljnn D ljn` SR M mKpF D mRpA SR M mRpA D mVo| SR
M mVo| D mZor SR M mZor D mZoi SR M mZoi D mVo_ SR M mVo_ D mKoU SR
M mKoU D l|oK SR M ljnj D lnnn SR M lnnn D lunn SR M lunn D mGne SR
M mGne D mRne SR M mRne D mZnj SR M mZnj D m]nn SR M lunn D mGn` SR
M mGn` D mVn` SR M mVn` D mZne SR M mZne D m]nn SR M m]nn D m]nx SR
M Gm{b D IAxX D JUui D KisQ D L}qO D NQo` D Oen@ D Pzlo D RNki D Sbjm
D Tviy D VJiK D W^hb D Xrg| D ZFgW D [Zft D \nfP D ^Bek D _VeC D `jdZ
D a~cm D cSb} D dgbI D e{aR D gO`W D hc_Z D iw^Y D kK]V D l_\Q D ms[L
D oGZG D p[YC D qoXA D sCWD D tXVK D ulUZ D w@Tq D xTTS SR
M y~T} D ywTz SR M ywTz D yrTp SR M yrTp D yoT` SR M yoT` D yoTV SR
M yoTV D yrTF SR M yrTF D ywS| SR M ywS| D y~Sy SR M y~Sy D zCSy SR
M zCSy D zJS| SR M zJS| D zOTF SR M zOTF D zQTV SR M zQTV D zQT` SR
M zQT` D zOTp SR M zOTp D zJTz SR M zJTz D zCT} SR M zCT} D y~T} SR
M y~T} D yyTz SR M yyTz D ywTw SR M ywTw D ytTp SR M ytTp D yrT` SR
M yrT` D yrTV SR M yrTV D ytTF SR M ytTF D ywT@ SR M ywT@ D yyS| SR
M yyS| D y~Sy SR M zCSy D zHS| SR M zHS| D zJT@ SR M zJT@ D zLTF SR
M zLTF D zOTV SR M zOTV D zOT` SR M zOT` D zLTp SR M zLTp D zJTw SR
M zJTw D zHTz SR M zHTz D zCT} SR M zbT@ D z`S| SR M z`S| D zbSy SR
M zbSy D zeS| SR M zeS| D zbT@ SR M {BT} D z{Tz SR M z{Tz D zvTp SR
M zvTp D zsT` SR M zsT` D zsTV SR M zsTV D zvTF SR M zvTF D z{S| SR
M z{S| D {BSy SR M {BSy D {GSy SR M {GSy D {NS| SR M {NS| D {STF SR
M {STF D {VTV SR M {VTV D {VT` SR M {VT` D {STp SR M {STp D {NTz SR
M {NTz D {GT} SR M {GT} D {BT} SR M {BT} D z}Tz SR M z}Tz D z{Tw SR
M z{Tw D zxTp SR M zxTp D zvT` SR M zvT` D zvTV SR M zvTV D zxTF SR
M zxTF D z{T@ SR M z{T@ D z}S| SR M z}S| D {BSy SR M {GSy D {LS| SR
M {LS| D {NT@ SR M {NT@ D {QTF SR M {QTF D {STV SR M {STV D {ST` SR
M {ST` D {QTp SR M {QTp D {NTw SR M {NTw D {LTz SR M {LTz D {GT} SR
M Gmxr D IAuh D JUry D Kipc D L}nb D NQlt D OekV D PzjG D RNiC D SbhJ
D TvgX D VJfm D W^fF D Xreb D ZFe@ D [Zd_ D \nc} D ^BcZ D _Vbu D `jbM
D a~ab D cS`s D dg`A D e{_K D gO^Q D hc]T D iw\U D kK[R D l_ZN D msYI
D oGXE D p[WA D qoV@ D sCUB D tXTJ D ulSY D w@Rq D xTRT SR
M y~Rx D ywRt SR M ywRt D yrRk SR M yrRk D yoR[ SR M yoR[ D yoRQ SR
M yoRQ D yrRA SR M yrRA D ywQw SR M ywQw D y~Qt SR M y~Qt D zCQt SR
M zCQt D zJQw SR M zJQw D zORA SR M zORA D zQRQ SR M zQRQ D zQR[ SR
M zQR[ D zORk SR M zORk D zJRt SR M zJRt D zCRx SR M zCRx D y~Rx SR
M y~Rx D yyRt SR M yyRt D ywRq SR M ywRq D ytRk SR M ytRk D yrR[ SR
M yrR[ D yrRQ SR M yrRQ D ytRA SR M ytRA D ywQz SR M ywQz D yyQw SR
M yyQw D y~Qt SR M zCQt D zHQw SR M zHQw D zJQz SR M zJQz D zLRA SR
M zLRA D zORQ SR M zORQ D zOR[ SR M zOR[ D zLRk SR M zLRk D zJRq SR
M zJRq D zHRt SR M zHRt D zCRx SR M zbQz D z`Qw SR M z`Qw D zbQt SR
M zbQt D zeQw SR M zeQw D zbQz SR M z{Rk D {@Rn SR M {@Rn D {GRx SR
M {GRx D {GQt SR M {ERt D {EQt SR M z{Qt D {QQt SR
M GmvE D IAr{ D JUpM D Kimx D L}ky D NQjL D Oehq D Pzgc D RNfb D Sbej
D Tvd{ D VJdR D W^cm D XrcL D ZFbl D [ZbL D \nam D ^BaK D _V`h D `j`B
D a~_X D cS^k D dg]z D e{]E D gO\L D hc[P D iwZQ D kKYO D l_XL D msWG
D oGVC D p[T? D qoS~ D sCSA D tXRJ D ulQY D w@Pq D xTPU SR
M y~P~ D ywP{ SR M ywP{ D yrPq SR M yrPq D yoPa SR M yoPa D yoPW SR
M yoPW D yrPG SR M yrPG D ywO} SR M ywO} D y~Oz SR M y~Oz D zCOz SR
M zCOz D zJO} SR M zJO} D zOPG SR M zOPG D zQPW SR M zQPW D zQPa SR
M zQPa D zOPq SR M zOPq D zJP{ SR M zJP{ D zCP~ SR M zCP~ D y~P~ SR
M y~P~ D yyP{ SR M yyP{ D ywPw SR M ywPw D ytPq SR M ytPq D yrPa SR
M yrPa D yrPW SR M yrPW D ytPG SR M ytPG D ywPA SR M ywPA D yyO} SR
M yyO} D y~Oz SR M zCOz D zHO} SR M zHO} D zJPA SR M zJPA D zLPG SR
M zLPG D zOPW SR M zOPW D zOPa SR M zOPa D zLPq SR M zLPq D zJPw SR
M zJPw D zHP{ SR M zHP{ D zCP~ SR M zbPA D z`O} SR M z`O} D zbOz SR
M zbOz D zeO} SR M zeO} D zbPA SR M zvPq D zxPn SR M zxPn D zvPj SR
M zvPj D zsPn SR M zsPn D zsPq SR M zsPq D zvPw SR M zvPw D zxP{ SR
M zxP{ D {@P~ SR M {@P~ D {IP~ SR M {IP~ D {QP{ SR M {QP{ D {SPw SR
M {SPw D {VPq SR M {VPq D {VPj SR M {VPj D {SPd SR M {SPd D {LP^ SR
M {LP^ D {@PW SR M {@PW D z{PT SR M z{PT D zvPM SR M zvPM D zsPD SR
M zsPD D zsOz SR M {IP~ D {NP{ SR M {NP{ D {QPw SR M {QPw D {SPq SR
M {SPq D {SPj SR M {SPj D {QPd SR M {QPd D {IP^ SR M {IP^ D {@PW SR
M zsPA D zvPD SR M zvPD D z{PD SR M z{PD D {GO} SR M {GO} D {NO} SR
M {NO} D {SPA SR M {SPA D {VPD SR M z{PD D {GOz SR M {GOz D {QOz SR
M {QOz D {SO} SR M {SO} D {VPD SR M {VPD D {VPJ SR
M GmsZ D IApR D JUme D KikQ D L}iS D NQgi D OefO D PzeC D RNdD D SbcO
D Tvba D VJaz D W^aX D Xr`x D ZF`Z D [Z_} D \n__ D ^B^? D _V^] D `j]x
D a~]P D cS\d D dg[t D e{[@ D gOZH D hcYM D iwXN D kKWM D l_VJ D msUF
D oGTB D p[R? D qoQ~ D sCQA D tXPJ D ulOZ D w@Nr D xTNV SR
M y~Nx D ywNu SR M ywNu D yrNk SR M yrNk D yoN[ SR M yoN[ D yoNR SR
M yoNR D yrNB SR M yrNB D ywMx SR M ywMx D y~Mu SR M y~Mu D zCMu SR
M zCMu D zJMx SR M zJMx D zONB SR M zONB D zQNR SR M zQNR D zQN[ SR
M zQN[ D zONk SR M zONk D zJNu SR M zJNu D zCNx SR M zCNx D y~Nx SR
M y~Nx D yyNu SR M yyNu D ywNr SR M ywNr D ytNk SR M ytNk D yrN[ SR
M yrN[ D yrNR SR M yrNR D ytNB SR M ytNB D ywM{ SR M ywM{ D yyMx SR
M yyMx D y~Mu SR M zCMu D zHMx SR M zHMx D zJM{ SR M zJM{ D zLNB SR
M zLNB D zONR SR M zONR D zON[ SR M zON[ D zLNk SR M zLNk D zJNr SR
M zJNr D zHNu SR M zHNu D zCNx SR M zbM{ D z`Mx SR M z`Mx D zbMu SR
M zbMu D zeMx SR M zeMx D zbM{ SR M zvNo D zxNk SR M zxNk D zvNh SR
M zvNh D zsNk SR M zsNk D zsNo SR M zsNo D zxNu SR M zxNu D {@Nx SR
M {@Nx D {INx SR M {INx D {QNu SR M {QNu D {SNo SR M {SNo D {SNe SR
M {SNe D {QN_ SR M {QN_ D {IN[ SR M {IN[ D {BN[ SR M {INx D {NNu SR
M {NNu D {QNo SR M {QNo D {QNe SR M {QNe D {NN_ SR M {NN_ D {IN[ SR
M {IN[ D {NNX SR M {NNX D {SNR SR M {SNR D {VNK SR M {VNK D {VNB SR
M {VNB D {SM{ SR M {SM{ D {QMx SR M {QMx D {IMu SR M {IMu D {@Mu SR
M {@Mu D zxMx SR M zxMx D zvM{ SR M zvM{ D zsNB SR M zsNB D zsNE SR
M zsNE D zvNH SR M zvNH D zxNE SR M zxNE D zvNB SR M {QNU D {SNK SR
M {SNK D {SNB SR M {SNB D {QM{ SR M {QM{ D {NMx SR M {NMx D {IMu SR
M Gmps D IAmk D JUk@ D Kihn D L}fq D NQeI D Oecq D Pzbg D RNaj D Sb`v
D Tv`K D VJ_f D W^_E D Xr^g D ZF^K D [Z]o D \n]S D ^B\t D _V\T D `j[p
D a~[I D cSZ^ D dgYo D e{X| D gOXE D hcWJ D iwVL D kKUK D l_TI D msSE
D oGRA D p[P~ D qoO~ D sCOA D tXNJ D ulM[ D w@Lt D xTLY SR
M y~L? D ywL{ SR M ywL{ D yrLr SR M yrLr D yoLa SR M yoLa D yoLX SR
M yoLX D yrLH SR M yrLH D ywK~ SR M ywK~ D y~K{ SR M y~K{ D zCK{ SR
M zCK{ D zJK~ SR M zJK~ D zOLH SR M zOLH D zQLX SR M zQLX D zQLa SR
M zQLa D zOLr SR M zOLr D zJL{ SR M zJL{ D zCL? SR M zCL? D y~L? SR
M y~L? D yyL{ SR M yyL{ D ywLx SR M ywLx D ytLr SR M ytLr D yrLa SR
M yrLa D yrLX SR M yrLX D ytLH SR M ytLH D ywLA SR M ywLA D yyK~ SR
M yyK~ D y~K{ SR M zCK{ D zHK~ SR M zHK~ D zJLA SR M zJLA D zLLH SR
M zLLH D zOLX SR M zOLX D zOLa SR M zOLa D zLLr SR M zLLr D zJLx SR
M zJLx D zHL{ SR M zHL{ D zCL? SR M zbLA D z`K~ SR M z`K~ D zbK{ SR
M zbK{ D zeK~ SR M zeK~ D zbLA SR M {ILx D {IK{ SR M {LL? D {LK{ SR
M {LL? D zqLN SR M zqLN D {XLN SR M {BK{ D {SK{ SR
M GmnN D IAkH D JUh^ D KifN D L}dS D NQbl D OeaV D Pz`N D RN_R D Sb^a
D Tv]w D VJ]S D W^\t D Xr\X D ZF[~ D [Z[c D \n[H D ^BZk D _VZL D `jYi
D a~YC D cSXY D dgWk D e{Vy D gOVB D hcUH D iwTJ D kKSJ D l_RH D msQD
D oGPA D p[N~ D qoM~ D sCMB D tXLK D ulK\ D w@Jv D xTJ[ SR
M y~J? D ywJ| SR M ywJ| D yrJr SR M yrJr D yoJb SR M yoJb D yoJX SR
M yoJX D yrJH SR M yrJH D ywI~ SR M ywI~ D y~I{ SR M y~I{ D zCI{ SR
M zCI{ D zJI~ SR M zJI~ D zOJH SR M zOJH D zQJX SR M zQJX D zQJb SR
M zQJb D zOJr SR M zOJr D zJJ| SR M zJJ| D zCJ? SR M zCJ? D y~J? SR
M y~J? D yyJ| SR M yyJ| D ywJx SR M ywJx D ytJr SR M ytJr D yrJb SR
M yrJb D yrJX SR M yrJX D ytJH SR M ytJH D ywJB SR M ywJB D yyI~ SR
M yyI~ D y~I{ SR M zCI{ D zHI~ SR M zHI~ D zJJB SR M zJJB D zLJH SR
M zLJH D zOJX SR M zOJX D zOJb SR M zOJb D zLJr SR M zLJr D zJJx SR
M zJJx D zHJ| SR M zHJ| D zCJ? SR M zbJB D z`I~ SR M z`I~ D zbI{ SR
M zbI{ D zeI~ SR M zeI~ D zbJB SR M zxJ? D zsJ_ SR M zsJ_ D zxJb SR
M zxJb D {@Je SR M {@Je D {GJe SR M {GJe D {NJb SR M {NJb D {SJ[ SR
M {SJ[ D {VJR SR M {VJR D {VJN SR M {VJN D {SJE SR M {SJE D {NI~ SR
M {NI~ D {GI{ SR M {GI{ D {@I{ SR M {@I{ D zxI~ SR M zxI~ D zvJB SR
M zvJB D zsJH SR M zsJH D zsJK SR M zsJK D zvJN SR M zvJN D zxJK SR
M zxJK D zvJH SR M {GJe D {LJb SR M {LJb D {QJ[ SR M {QJ[ D {SJR SR
M {SJR D {SJN SR M {SJN D {QJE SR M {QJE D {LI~ SR M {LI~ D {GI{ SR
M zxJ? D {QJ? SR M zxJ| D {EJ| SR M {EJ| D {QJ? SR
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FMENDEPSF
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (71) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(T) 207 736.18 T
(arget Acquisition Reference Information) 211.83 736.18 T
2 10 Q
0.57 (Figure 7-2.) 126 434.33 P
4 F
0.57 (Fraction of counts detected as a function of the true count rate,) 183.83 434.33 P
(i.e., before the paired pulse correction.) 126 422.33 T
54 379 540 382 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 380.5 540 380.5 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 380.5 180 380.5 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(7.2) 163.32 386 T
(Constraints on the V) 189 386 T
(alue of the) 305.69 386 T
10 F
(STEP-TIME) 369.04 386 T
2 F
( Parameter) 433.84 386 T
0 10 Q
-0.22 (Once you have the predicted countrate, you then need to extract the piece of information) 189 358.33 P
-0.02 (required to plan your tar) 189 346.33 P
-0.02 (get acquisition:) 285.93 346.33 P
9 F
-0.05 (STEP-TIME) 349.77 346.33 P
0 F
-0.02 (. This is necessary to calculate the) 403.77 346.33 P
0.7 (time per exposure that is entered on the proposal logsheet. The goal is to have GHRS) 189 334.33 P
-0.2 (see 10) 189 322.33 P
0 8 Q
-0.16 (3) 214.07 326.33 P
0 10 Q
-0.2 ( to 10) 218.07 322.33 P
0 8 Q
-0.16 (4) 240.46 326.33 P
0 10 Q
-0.2 ( counts at the peak dwell point of the spiral search for either an acquisition) 244.46 322.33 P
0.16 (or a peakup. A minimum of 100 counts are needed to have a chance at a successful tar-) 189 310.33 P
0.13 (get acquisition. The) 189 298.33 P
9 F
0.31 (STEP-TIME) 271.05 298.33 P
0 F
0.13 ( then is just the number of counts desired \05010) 325.05 298.33 P
0 8 Q
0.1 (3) 506.46 302.33 P
0 10 Q
0.13 ( to 10) 510.46 298.33 P
0 8 Q
0.1 (5) 533.5 302.33 P
0 10 Q
0.13 (,) 537.5 298.33 P
-0.09 (but at least 100\051 divided by the predicted count rate. Remember) 189 286.33 P
-0.09 (, however) 442.42 286.33 P
-0.09 (, that the mini-) 481.37 286.33 P
0.76 (mum) 189 274.33 P
9 F
1.82 (STEP-TIME) 212.82 274.33 P
0 F
0.76 ( permitted is 0.2 seconds. Also bear in mind that the) 266.82 274.33 P
9 F
1.82 (STEP-TIME) 486 274.33 P
0 F
(may not exceed 12.75 seconds.) 189 262.33 T
-0.24 (T) 189 238.33 P
-0.24 (o avoid the possibility of a failed tar) 194.41 238.33 P
-0.24 (get acquisition, it is important that the combination) 337.24 238.33 P
0.21 (of your tar) 189 226.33 P
0.21 (get \337ux and the acquisition mirror used should not result in the eight science) 231.45 226.33 P
0.82 (diodes used for the tar) 189 214.33 P
0.82 (get acquisition seeing more than a total of about 65,000 counts) 280.98 214.33 P
-0.23 (\050the number accommodated in a 16 bit register\051 in a given) 189 202.33 P
9 F
-0.55 (STEP-TIME) 421.17 202.33 P
0 F
-0.23 (. Counting more) 475.17 202.33 P
0.98 (than 65,000 counts ef) 189 190.33 P
0.98 (fectively causes the register to wrap back to zero and thus con-) 277.87 190.33 P
-0.03 (founds the tar) 189 178.33 P
-0.03 (get acquisition algorithm.) 243.76 178.33 P
1 F
-0.03 (This pr) 348.68 178.33 P
-0.03 (oblem is avoided if) 379.87 178.33 P
10 F
-0.06 (BRIGHT=RETURN) 462 178.33 P
1 F
0.62 (is speci\336ed) 189 166.33 P
0 F
0.62 (because a 32-bit on-board register is used. If a) 238.57 166.33 P
9 F
1.48 (BRIGHT) 431.3 166.33 P
0 F
0.62 ( limit is explicitly) 467.3 166.33 P
(given, the register that holds it is limited to 16 bits.) 189 154.33 T
-0.11 (Figure) 189 130.33 P
-0.11 (7-3 and Figure) 217.61 130.33 P
-0.11 (7-4 are provided to allow for a visual check of potential problems) 278.77 130.33 P
0.38 (arising from the choice of) 189 118.33 P
9 F
0.91 (STEP-TIME) 296.71 118.33 P
0 F
0.38 (. These Figures show the constraints placed on) 350.71 118.33 P
0.35 (using a particular mirror and) 189 106.33 P
9 F
0.84 (STEP-TIME) 307.67 106.33 P
0 F
0.35 (. Figure) 361.67 106.33 P
0.35 (7-4 is analogous for the Side 1 mir-) 395.62 106.33 P
(rors.) 189 94.33 T
54 87.98 540 686.02 C
54 450 540 679.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 92 210 534 484 353.6 219.2 120.2 456.41 FMBEGINEPSF
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54 726.98 540 726.98 2 L
0.25 H
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54 74.02 540 74.02 2 L
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(72) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
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54 74.02 540 74.02 2 L
2 Z
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54 726.98 540 726.98 2 L
0 Z
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54 74.02 540 74.02 2 L
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(Figure 7-3.) 126 326.33 T
4 F
(T) 182.13 326.33 T
(arget acquisition constraints for the Side 2 mirrors N2 and A2.) 187.13 326.33 T
0 0 0 1 0 0 0 K
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(N2R:) 114 299 T
(Constraints and Restrictions Document \050CARD\051 upper limit for use of Mirror) 186 299 T
(-N2. Observing) 465.3 299 T
(objects that are bluer and brighter than indicated by this line would result in degraded perfor-) 186 288 T
-0.33 (mance and possible damage to the instrument. Brighter and bluer objects should be acquired with) 186 277 P
(mirrors A2 or A1.) 186 266 T
(N2-0.2:) 114 247 T
-0.17 (GHRS will count 65,000 counts in 0.2 seconds with the N2 mirror for objects on this contour) 186 247 P
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(the left of this curve, more than 65,000 counts will be detected leading to a probable failure to) 186 236 T
(acquire the object if a) 186 225 T
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(BRIGHT) 266.23 225 T
0 F
( value is speci\336ed. However) 298.63 225 T
(, use of) 399.99 225 T
9 F
(BRIGHT=RETURN) 428.49 225 T
0 F
( will) 498.69 225 T
(result in a satisfactory acquisition.) 186 214 T
(A2-0.2:) 114 195 T
-0.17 (GHRS will count 65,000 counts in 0.2 seconds with the A2 mirror for objects on this contour) 186 195 P
-0.17 (. T) 518.23 195 P
-0.17 (o) 527.42 195 P
(the left of this curve, more than 65,000 counts will be detected leading to a probable failure to) 186 184 T
(acquire the object if a) 186 173 T
9 F
(BRIGHT) 266.23 173 T
0 F
( value is speci\336ed. However) 298.63 173 T
(, use of) 399.99 173 T
9 F
(BRIGHT=RETURN) 428.49 173 T
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( will) 498.69 173 T
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180 311.12 180 154.88 2 L
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72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
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2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (73) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
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72 726.98 558 726.98 2 L
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72 74.02 558 74.02 2 L
2 Z
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2 9 Q
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(arget Acquisition Reference Information) 211.83 736.18 T
2 10 Q
(Figure 7-4.) 144 335.33 T
4 F
(T) 200.13 335.33 T
(arget acquisition constraints for the Side 1 mirrors N1 and A1.) 205.13 335.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
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(-N1. Observing) 483.3 308 T
(objects that are bluer and brighter than indicated by this line would result in degraded perfor-) 204 297 T
-0.33 (mance and possible damage to the instrument. Brighter and bluer objects should be acquired with) 204 286 P
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(N1-0.2:) 132 256 T
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(acquire the object if a) 204 234 T
9 F
(BRIGHT) 284.23 234 T
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( value is speci\336ed. However) 316.63 234 T
(, use of) 417.99 234 T
9 F
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0 F
( will) 516.69 234 T
(result in a satisfactory acquisition.!) 204 223 T
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%+ prolog.ps -- Prolog for IDL generated PostScript files
%+ Copyright (c) 1988-1993 Research Systems, Inc. All Rights Reserved.
%v 3
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setlinewidth 1 setlinecap stroke grestore} bdef /L0 {[] 0 setdash} bdef /L1
{[40 100] 0 setdash} bdef /L2 {[200 200] 0 setdash} bdef /L3 {[200 100 50
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FMENDEPSF
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2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(T) 189 736.18 T
(arget Acquisition Reference Information) 193.83 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(74) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
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0 Z
N
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(T) 0 -270 74 152.01 TF
(ABLE 7-1) 0 -270 74 156.84 TF
4 F
(Predicted target acquisition count rates for stars, reduced to) 0 -270 74 287.01 TF
8 F
(V) 0 -270 74 527.62 TF
8 7.2 Q
(0) 0 -270 76.25 533.62 TF
4 9 Q
(= 0.) 0 -270 74 540.13 TF
2 8 Q
(Star Name) 0 -270 100.33 161.69 TF
(Spectral) 0 -270 95.33 221.97 TF
(T) 0 -270 105.33 228.71 TF
(ype) 0 -270 105.33 233.01 TF
6 F
(\050B\320V\051) 0 -270 100.33 270.82 TF
6 6.4 Q
(0) 0 -270 102.33 291.71 TF
2 8 Q
(count rate for mirror) 0 -270 92.33 365.08 TF
(reddening reduction factor) 0 -270 92.33 530.82 TF
2 6.4 Q
(a) 0 -270 89.13 632.61 TF
2 8 Q
(N2) 0 -270 108.33 321.96 TF
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(A1) 0 -270 108.33 475.33 TF
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(A2) 0 -270 108.33 559.01 TF
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(A1) 0 -270 108.33 636.51 TF
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(8.595E9) 0 -270 123 311.95 TF
(2.098E7) 0 -270 123 363.07 TF
(4.598E8) 0 -270 123 414.19 TF
(2.657E5) 0 -270 123 465.32 TF
(-3.034) 0 -270 123 513.75 TF
(-3.108) 0 -270 123 552.5 TF
(-3.428) 0 -270 123 591.25 TF
(-3.130) 0 -270 123 630 TF
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(O6) 0 -270 136 232.25 TF
(-0.313) 0 -270 136 271.42 TF
(5.684E9) 0 -270 136 311.95 TF
(1.348E7) 0 -270 136 363.07 TF
(2.545E8) 0 -270 136 414.19 TF
(1.690E5) 0 -270 136 465.32 TF
(-2.955) 0 -270 136 513.75 TF
(-3.021) 0 -270 136 552.5 TF
(-3.382) 0 -270 136 591.25 TF
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(-0.269) 0 -270 149 271.42 TF
(5.367E9) 0 -270 149 311.95 TF
(1.293E7) 0 -270 149 363.07 TF
(2.794E8) 0 -270 149 414.19 TF
(1.767E5) 0 -270 149 465.32 TF
(-3.002) 0 -270 149 513.75 TF
(-3.070) 0 -270 149 552.5 TF
(-3.393) 0 -270 149 591.25 TF
(-3.123) 0 -270 149 630 TF
(69 Cyg) 0 -270 162 178.68 TF
(B0IB) 0 -270 162 228 TF
(-0.234) 0 -270 162 271.42 TF
(4.192E9) 0 -270 162 311.95 TF
(9.901E6) 0 -270 162 363.07 TF
(1.869E8) 0 -270 162 414.19 TF
(1.209E5) 0 -270 162 465.32 TF
(-2.935) 0 -270 162 513.75 TF
(-3.003) 0 -270 162 552.5 TF
(-3.384) 0 -270 162 591.25 TF
(-3.1) 0 -270 162 630.16 TF
(10) 0 -270 162 644.08 TF
13 10 Q
(i) 0 -270 175 185.65 TF
0 9 Q
(Her) 0 -270 175 191.44 TF
(B3V) 0 -270 175 229.25 TF
(-0.203) 0 -270 175 271.42 TF
(2.764E9) 0 -270 175 311.95 TF
(6.529E6) 0 -270 175 363.07 TF
(1.232E8) 0 -270 175 414.19 TF
(7.970E4) 0 -270 175 465.32 TF
(-2.935) 0 -270 175 513.75 TF
(-3.003) 0 -270 175 552.5 TF
(-3.384) 0 -270 175 591.25 TF
(-3.1) 0 -270 175 630.16 TF
(10) 0 -270 175 644.08 TF
(HR 7467) 0 -270 188 172.18 TF
(B3III) 0 -270 188 228.01 TF
(-0.182) 0 -270 188 271.42 TF
(2.436E9) 0 -270 188 311.95 TF
(5.755E6) 0 -270 188 363.07 TF
(1.087E8) 0 -270 188 414.19 TF
(7.028E4) 0 -270 188 465.32 TF
(-2.936) 0 -270 188 513.75 TF
(-3.004) 0 -270 188 552.5 TF
(-3.384) 0 -270 188 591.25 TF
(-3.1) 0 -270 188 630.16 TF
(10) 0 -270 188 644.08 TF
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(B3IV) 0 -270 201 227.75 TF
(-0.156) 0 -270 201 271.42 TF
(2.268E9) 0 -270 201 311.95 TF
(5.357E6) 0 -270 201 363.07 TF
(1.012E8) 0 -270 201 414.19 TF
(6.542E4) 0 -270 201 465.32 TF
(-2.936) 0 -270 201 513.75 TF
(-3.004) 0 -270 201 552.5 TF
(-3.384) 0 -270 201 591.25 TF
(-3.1) 0 -270 201 630.16 TF
(10) 0 -270 201 644.08 TF
(38 Oph) 0 -270 214 178.19 TF
(A1V) 0 -270 214 229 TF
(-0.139) 0 -270 214 271.42 TF
(1.776E9) 0 -270 214 311.95 TF
(4.108E6) 0 -270 214 363.07 TF
(6.421E7) 0 -270 214 414.19 TF
(4.582E4) 0 -270 214 465.32 TF
(-2.891) 0 -270 214 513.75 TF
(-2.953) 0 -270 214 552.5 TF
(-3.347) 0 -270 214 591.25 TF
(-3.101) 0 -270 214 630 TF
(HR 7346) 0 -270 227 172.18 TF
(B7III) 0 -270 227 228.01 TF
(-0.108) 0 -270 227 271.42 TF
(1.368E9) 0 -270 227 311.95 TF
(3.165E6) 0 -270 227 363.07 TF
(4.948E7) 0 -270 227 414.19 TF
(3.531E4) 0 -270 227 465.32 TF
(-2.892) 0 -270 227 513.75 TF
(-2.953) 0 -270 227 552.5 TF
(-3.347) 0 -270 227 591.25 TF
(-3.101) 0 -270 227 630 TF
(HD 189689) 0 -270 240 162.69 TF
(B9V) 0 -270 240 229.25 TF
(-0.081) 0 -270 240 271.42 TF
(1.008E9) 0 -270 240 311.95 TF
(2.303E6) 0 -270 240 363.07 TF
(2.763E7) 0 -270 240 414.19 TF
(2.306E4) 0 -270 240 465.32 TF
(-2.864) 0 -270 240 513.75 TF
(-2.921) 0 -270 240 552.5 TF
(-3.317) 0 -270 240 591.25 TF
(-3.097) 0 -270 240 630 TF
(59 Her) 0 -270 253 180.19 TF
(A3III) 0 -270 253 227.76 TF
(-0.045) 0 -270 253 271.42 TF
(5.948E8) 0 -270 253 311.95 TF
(1.363E6) 0 -270 253 363.07 TF
(1.700E7) 0 -270 253 414.19 TF
(1.407E4) 0 -270 253 465.32 TF
(-2.873) 0 -270 253 513.75 TF
(-2.932) 0 -270 253 552.5 TF
(-3.320) 0 -270 253 591.25 TF
(-3.099) 0 -270 253 630 TF
(1) 0 -270 266 180.52 TF
(1 Sge) 0 -270 266 184.68 TF
(B9IV) 0 -270 266 227.75 TF
(-0.027) 0 -270 266 271.42 TF
(5.745E8) 0 -270 266 311.95 TF
(1.293E6) 0 -270 266 363.07 TF
(1.168E7) 0 -270 266 414.19 TF
(1.182E4) 0 -270 266 465.32 TF
(-2.819) 0 -270 266 513.75 TF
(-2.873) 0 -270 266 552.5 TF
(-3.281) 0 -270 266 591.25 TF
(-3.088) 0 -270 266 630 TF
(69 Her) 0 -270 279 180.19 TF
(A2V) 0 -270 279 229 TF
(0.000) 0 -270 279 272.92 TF
(4.918E8) 0 -270 279 311.95 TF
(1.107E6) 0 -270 279 363.07 TF
(9.997E6) 0 -270 279 414.19 TF
(1.01) 0 -270 279 465.48 TF
(1E4) 0 -270 279 480.9 TF
(-2.819) 0 -270 279 513.75 TF
(-2.873) 0 -270 279 552.5 TF
(-3.281) 0 -270 279 591.25 TF
(-3.088) 0 -270 279 630 TF
(HR 8020) 0 -270 292 172.18 TF
(B8IA) 0 -270 292 227.75 TF
(0.027) 0 -270 292 272.92 TF
(1.063E9) 0 -270 292 311.95 TF
(2.386E6) 0 -270 292 363.07 TF
(1.940E7) 0 -270 292 414.19 TF
(2.154E4) 0 -270 292 465.32 TF
(-2.820) 0 -270 292 513.75 TF
(-2.872) 0 -270 292 552.5 TF
(-3.255) 0 -270 292 591.25 TF
(-3.089) 0 -270 292 630 TF
(78 Her) 0 -270 305 180.19 TF
(B9V) 0 -270 305 229.25 TF
(0.036) 0 -270 305 272.92 TF
(4.532E8) 0 -270 305 311.95 TF
(1.018E6) 0 -270 305 363.07 TF
(8.272E6) 0 -270 305 414.19 TF
(9.187E3) 0 -270 305 465.32 TF
(-2.820) 0 -270 305 513.75 TF
(-2.872) 0 -270 305 552.5 TF
(-3.255) 0 -270 305 591.25 TF
(-3.089) 0 -270 305 630 TF
(58 Aql) 0 -270 318 180.18 TF
(A0V) 0 -270 318 229 TF
(0.057) 0 -270 318 272.92 TF
(4.291E8) 0 -270 318 311.95 TF
(9.634E5) 0 -270 318 363.07 TF
(7.830E6) 0 -270 318 414.19 TF
(8.696E3) 0 -270 318 465.32 TF
(-2.820) 0 -270 318 513.75 TF
(-2.872) 0 -270 318 552.5 TF
(-3.255) 0 -270 318 591.25 TF
(-3.089) 0 -270 318 630 TF
(60 Her) 0 -270 331 180.19 TF
(A3IV) 0 -270 331 227.51 TF
(0.085) 0 -270 331 272.92 TF
(3.197E8) 0 -270 331 311.95 TF
(7.086E5) 0 -270 331 363.07 TF
(3.280E6) 0 -270 331 414.19 TF
(5.497E3) 0 -270 331 465.32 TF
(-2.758) 0 -270 331 513.75 TF
(-2.810) 0 -270 331 552.5 TF
(-3.217) 0 -270 331 591.25 TF
(-3.077) 0 -270 331 630 TF
(HR 6570) 0 -270 344 172.18 TF
(A7V) 0 -270 344 229 TF
(0.107) 0 -270 344 272.92 TF
(2.999E8) 0 -270 344 311.95 TF
(6.647E5) 0 -270 344 363.07 TF
(3.079E6) 0 -270 344 414.19 TF
(5.161E3) 0 -270 344 465.32 TF
(-2.759) 0 -270 344 513.75 TF
(-2.81) 0 -270 344 552.67 TF
(1) 0 -270 344 571.08 TF
(-3.217) 0 -270 344 591.25 TF
(-3.077) 0 -270 344 630 TF
(HD192285) 0 -270 357 164.94 TF
(A4IV) 0 -270 357 227.51 TF
(0.124) 0 -270 357 272.92 TF
(2.628E8) 0 -270 357 311.95 TF
(5.771E5) 0 -270 357 363.07 TF
(1.444E6) 0 -270 357 414.19 TF
(3.569E3) 0 -270 357 465.32 TF
(-2.719) 0 -270 357 513.75 TF
(-2.771) 0 -270 357 552.5 TF
(-3.184) 0 -270 357 591.25 TF
(-3.071) 0 -270 357 630 TF
13 10 Q
(q) 0 -270 370 182.33 TF
0 7.2 Q
(1) 0 -270 366.4 187.54 TF
0 9 Q
(Ser) 0 -270 370 192.94 TF
(A5V) 0 -270 370 229 TF
(0.143) 0 -270 370 272.92 TF
(2.669E8) 0 -270 370 311.95 TF
(5.862E5) 0 -270 370 363.07 TF
(1.466E6) 0 -270 370 414.19 TF
(3.623E3) 0 -270 370 465.32 TF
(-2.718) 0 -270 370 513.75 TF
(-2.770) 0 -270 370 552.5 TF
(-3.184) 0 -270 370 591.25 TF
(-3.071) 0 -270 370 630 TF
(KW 1) 0 -270 383 174.52 TF
(14) 0 -270 383 195.93 TF
(0.175) 0 -270 383 272.92 TF
(2.395E8) 0 -270 383 311.95 TF
(5.240E5) 0 -270 383 363.07 TF
(9.954E5) 0 -270 383 414.19 TF
(2.843E3) 0 -270 383 465.32 TF
(-2.703) 0 -270 383 513.75 TF
(-2.755) 0 -270 383 552.5 TF
(-3.168) 0 -270 383 591.25 TF
(-3.069) 0 -270 383 630 TF
(KW 154) 0 -270 396 174.19 TF
(0.219) 0 -270 396 272.92 TF
(2.050E8) 0 -270 396 311.95 TF
(4.439E5) 0 -270 396 363.07 TF
(4.497E5) 0 -270 396 414.19 TF
(1.636E3) 0 -270 396 465.32 TF
(-2.666) 0 -270 396 513.75 TF
(-2.715) 0 -270 396 552.5 TF
(-3.166) 0 -270 396 591.25 TF
(-3.063) 0 -270 396 630 TF
13 10 Q
(c) 0 -270 409 184.95 TF
0 9 Q
(Ser) 0 -270 409 192.94 TF
(F0IV) 0 -270 409 228.25 TF
(0.240) 0 -270 409 272.92 TF
(1.829E8) 0 -270 409 311.95 TF
(3.958E5) 0 -270 409 363.07 TF
(4.004E5) 0 -270 409 414.19 TF
(1.457E3) 0 -270 409 465.32 TF
(-2.665) 0 -270 409 513.75 TF
(-2.714) 0 -270 409 552.5 TF
(-3.166) 0 -270 409 591.25 TF
(-3.062) 0 -270 409 630 TF
(HD5132) 0 -270 422 173.94 TF
(F0IV) 0 -270 422 228.25 TF
(0.287) 0 -270 422 272.92 TF
(2.01) 0 -270 422 312.12 TF
(1E8) 0 -270 422 327.53 TF
(4.354E5) 0 -270 422 363.07 TF
(4.412E5) 0 -270 422 414.19 TF
(1.605E3) 0 -270 422 465.32 TF
(-2.666) 0 -270 422 513.75 TF
(-2.715) 0 -270 422 552.5 TF
(-3.166) 0 -270 422 591.25 TF
(-3.063) 0 -270 422 630 TF
(HD508) 0 -270 435 178.44 TF
(A9IV) 0 -270 435 227.51 TF
(0.305) 0 -270 435 272.92 TF
(1.718E8) 0 -270 435 311.95 TF
(3.720E5) 0 -270 435 363.07 TF
(3.771E5) 0 -270 435 414.19 TF
(1.372E3) 0 -270 435 465.32 TF
(-2.666) 0 -270 435 513.75 TF
(-2.716) 0 -270 435 552.5 TF
(-3.166) 0 -270 435 591.25 TF
(-3.063) 0 -270 435 630 TF
13 10 Q
(r) 0 -270 448 182.45 TF
0 9 Q
(Cap) 0 -270 448 190.43 TF
(F2IV) 0 -270 448 228.25 TF
(0.339) 0 -270 448 272.92 TF
(1.125E8) 0 -270 448 311.95 TF
(2.322E5) 0 -270 448 363.07 TF
(2.619E4) 0 -270 448 414.19 TF
(1.014E2) 0 -270 448 465.32 TF
(-2.484) 0 -270 448 513.75 TF
(-2.517) 0 -270 448 552.5 TF
(-3.181) 0 -270 448 591.25 TF
(-3.023) 0 -270 448 630 TF
(KW 332) 0 -270 461 174.19 TF
(0.389) 0 -270 461 272.92 TF
(1.177E8) 0 -270 461 311.95 TF
(2.431E5) 0 -270 461 363.07 TF
(2.751E4) 0 -270 461 414.19 TF
(1.065E2) 0 -270 461 465.32 TF
(-2.486) 0 -270 461 513.75 TF
(-2.519) 0 -270 461 552.5 TF
(-3.181) 0 -270 461 591.25 TF
(-3.023) 0 -270 461 630 TF
(HD7331) 0 -270 474 173.94 TF
(F7IV) 0 -270 474 228.25 TF
(0.427) 0 -270 474 272.92 TF
(9.807E7) 0 -270 474 311.95 TF
(2.012E5) 0 -270 474 363.07 TF
(2.256E4) 0 -270 474 414.19 TF
(8.772E1) 0 -270 474 465.32 TF
(-2.451) 0 -270 474 513.75 TF
(-2.482) 0 -270 474 552.5 TF
(-3.179) 0 -270 474 591.25 TF
(-3.015) 0 -270 474 630 TF
(BD+63) 0 -270 487 165.76 TF
0 7.2 Q
(o) 0 -270 483.4 192.33 TF
0 9 Q
(13) 0 -270 487 195.93 TF
(F5IV) 0 -270 487 228.25 TF
(0.444) 0 -270 487 272.92 TF
(1.139E8) 0 -270 487 311.95 TF
(2.362E5) 0 -270 487 363.07 TF
(6.070E4) 0 -270 487 414.19 TF
(2.395E2) 0 -270 487 465.32 TF
(-2.488) 0 -270 487 513.75 TF
(-2.523) 0 -270 487 552.5 TF
(-3.171) 0 -270 487 591.25 TF
(-3.024) 0 -270 487 630 TF
(HD35296) 0 -270 500 169.44 TF
(F8V) 0 -270 500 229.75 TF
(0.489) 0 -270 500 272.92 TF
(1.089E8) 0 -270 500 311.95 TF
(2.259E5) 0 -270 500 363.07 TF
(5.804E4) 0 -270 500 414.19 TF
(2.290E2) 0 -270 500 465.32 TF
(-2.488) 0 -270 500 513.75 TF
(-2.523) 0 -270 500 552.5 TF
(-3.171) 0 -270 500 591.25 TF
(-3.024) 0 -270 500 630 TF
(vB 1) 0 -270 513 187.68 TF
(0.530) 0 -270 513 272.92 TF
(6.757E7) 0 -270 513 311.95 TF
(1.374E5) 0 -270 513 363.07 TF
(2.147E4) 0 -270 513 414.19 TF
(8.448E1) 0 -270 513 465.32 TF
(-2.407) 0 -270 513 513.75 TF
(-2.437) 0 -270 513 552.5 TF
(-3.175) 0 -270 513 591.25 TF
(-3.006) 0 -270 513 630 TF
(HD154760) 0 -270 526 164.94 TF
(G2V) 0 -270 526 229 TF
(0.586) 0 -270 526 272.92 TF
(6.393E7) 0 -270 526 311.95 TF
(1.285E5) 0 -270 526 363.07 TF
(3.1) 0 -270 526 414.36 TF
(15E3) 0 -270 526 425.28 TF
(1.151E1) 0 -270 526 465.32 TF
(-2.365) 0 -270 526 513.75 TF
(-2.386) 0 -270 526 552.5 TF
(-3.206) 0 -270 526 591.25 TF
(-2.998) 0 -270 526 630 TF
83.12 152.01 530.88 152.01 2 L
V
0.25 H
0 Z
N
82.88 210.93 531.12 210.93 2 L
V
N
82.88 264.57 531.12 264.57 2 L
V
N
82.88 301.51 531.12 301.51 2 L
V
2 H
N
98.88 352.64 531.12 352.64 2 L
V
0.25 H
N
98.88 403.76 531.12 403.76 2 L
V
N
98.88 454.88 531.12 454.88 2 L
V
N
82.88 506 531.12 506 2 L
V
N
98.88 544.75 531.12 544.75 2 L
V
N
98.88 583.5 531.12 583.5 2 L
V
N
98.88 622.24 531.12 622.24 2 L
V
N
83.12 660.99 530.88 660.99 2 L
V
N
83 151.88 83 661.12 2 L
V
N
99 300.51 99 661.12 2 L
V
N
115 151.88 115 661.12 2 L
V
0.5 H
N
180 151.88 180 661.12 2 L
V
0.25 H
N
245 151.88 245 661.12 2 L
V
N
310 151.88 310 661.12 2 L
V
N
375 151.88 375 661.12 2 L
V
N
440 151.88 440 661.12 2 L
V
N
505 151.88 505 661.12 2 L
V
N
531 151.88 531 661.12 2 L
V
N
FMENDPAGE
%%EndPage: "74" 74
%%Page: "75" 75
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (75) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(T) 207 736.18 T
(arget Acquisition Reference Information) 211.83 736.18 T
30.49 78 563.51 699 R
519.49 134.01 526.49 642.99 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(a. use factor) 0 -270 532.49 281.01 TF
3 F
(f) 0 -270 532.49 326.99 TF
0 F
( to reduce count rate by) 0 -270 532.49 329.49 TF
(.) 0 -270 532.49 466.45 TF
30.49 78 563.51 699 R
(HD139777A) 0 -270 98.49 140.44 TF
(K0V) 0 -270 98.49 211 TF
(0.631) 0 -270 98.49 254.92 TF
(6.040E7) 0 -270 98.49 293.95 TF
(1.215E5) 0 -270 98.49 345.07 TF
(2.954E3) 0 -270 98.49 396.19 TF
(1.091E1) 0 -270 98.49 447.32 TF
(-2.367) 0 -270 98.49 495.75 TF
(-2.387) 0 -270 98.49 534.5 TF
(-3.206) 0 -270 98.49 573.25 TF
(-2.998) 0 -270 98.49 612 TF
(HR 6516) 0 -270 111.49 154.18 TF
(G6IV) 0 -270 111.49 209.51 TF
(0.651) 0 -270 111.49 254.92 TF
(5.167E7) 0 -270 111.49 293.95 TF
(1.039E5) 0 -270 111.49 345.07 TF
(2.518E3) 0 -270 111.49 396.19 TF
(9.301E0) 0 -270 111.49 447.32 TF
(-2.365) 0 -270 111.49 495.75 TF
(-2.386) 0 -270 111.49 534.5 TF
(-3.206) 0 -270 111.49 573.25 TF
(-2.998) 0 -270 111.49 612 TF
(HD136274) 0 -270 124.49 146.94 TF
(G8V) 0 -270 124.49 211 TF
(0.672) 0 -270 124.49 254.92 TF
(4.901E7) 0 -270 124.49 293.95 TF
(9.855E4) 0 -270 124.49 345.07 TF
(2.392E3) 0 -270 124.49 396.19 TF
(8.837E0) 0 -270 124.49 447.32 TF
(-2.366) 0 -270 124.49 495.75 TF
(-2.387) 0 -270 124.49 534.5 TF
(-3.206) 0 -270 124.49 573.25 TF
(-2.998) 0 -270 124.49 612 TF
(HD150205) 0 -270 137.49 146.94 TF
(G5V) 0 -270 137.49 211 TF
(0.700) 0 -270 137.49 254.92 TF
(4.650E7) 0 -270 137.49 293.95 TF
(9.352E4) 0 -270 137.49 345.07 TF
(2.275E3) 0 -270 137.49 396.19 TF
(8.404E0) 0 -270 137.49 447.32 TF
(-2.367) 0 -270 137.49 495.75 TF
(-2.388) 0 -270 137.49 534.5 TF
(-3.206) 0 -270 137.49 573.25 TF
(-2.998) 0 -270 137.49 612 TF
(31 Aql) 0 -270 150.49 162.18 TF
(G8IV) 0 -270 150.49 209.51 TF
(0.732) 0 -270 150.49 254.92 TF
(4.042E7) 0 -270 150.49 293.95 TF
(8.123E4) 0 -270 150.49 345.07 TF
(1.960E3) 0 -270 150.49 396.19 TF
(7.242E0) 0 -270 150.49 447.32 TF
(-2.364) 0 -270 150.49 495.75 TF
(-2.384) 0 -270 150.49 534.5 TF
(-3.206) 0 -270 150.49 573.25 TF
(-2.997) 0 -270 150.49 612 TF
(vB 21) 0 -270 163.49 165.18 TF
(0.766) 0 -270 163.49 254.92 TF
(3.890E7) 0 -270 163.49 293.95 TF
(7.818E4) 0 -270 163.49 345.07 TF
(1.887E3) 0 -270 163.49 396.19 TF
(6.972E0) 0 -270 163.49 447.32 TF
(-2.364) 0 -270 163.49 495.75 TF
(-2.385) 0 -270 163.49 534.5 TF
(-3.206) 0 -270 163.49 573.25 TF
(-2.997) 0 -270 163.49 612 TF
(BD\3202) 0 -270 176.49 143.83 TF
0 7.2 Q
(o) 0 -270 172.89 165.33 TF
0 9 Q
(4018) 0 -270 176.49 168.93 TF
(G5IV) 0 -270 176.49 209.51 TF
(0.791) 0 -270 176.49 254.92 TF
(3.516E7) 0 -270 176.49 293.95 TF
(7.068E4) 0 -270 176.49 345.07 TF
(1.713E3) 0 -270 176.49 396.19 TF
(6.328E0) 0 -270 176.49 447.32 TF
(-2.365) 0 -270 176.49 495.75 TF
(-2.386) 0 -270 176.49 534.5 TF
(-3.206) 0 -270 176.49 573.25 TF
(-2.998) 0 -270 176.49 612 TF
(HD190571) 0 -270 189.49 146.94 TF
(G8V) 0 -270 189.49 211 TF
(0.816) 0 -270 189.49 254.92 TF
(1.587E7) 0 -270 189.49 293.95 TF
(3.086E4) 0 -270 189.49 345.07 TF
(1.165E1) 0 -270 189.49 396.19 TF
(4.76E-4) 0 -270 189.49 448.07 TF
(-2.233) 0 -270 189.49 495.75 TF
(-2.244) 0 -270 189.49 534.5 TF
(-3.719) 0 -270 189.49 573.25 TF
(-3.247) 0 -270 189.49 612 TF
(HD1) 0 -270 202.49 151.77 TF
(1004) 0 -270 202.49 168.93 TF
(G5IV) 0 -270 202.49 209.51 TF
(0.825) 0 -270 202.49 254.92 TF
(1.587E7) 0 -270 202.49 293.95 TF
(3.086E4) 0 -270 202.49 345.07 TF
(1.169E1) 0 -270 202.49 396.19 TF
(4.78E-4) 0 -270 202.49 448.07 TF
(-2.234) 0 -270 202.49 495.75 TF
(-2.244) 0 -270 202.49 534.5 TF
(-3.719) 0 -270 202.49 573.25 TF
(-3.247) 0 -270 202.49 612 TF
(HD56176) 0 -270 215.49 151.44 TF
(G7IV) 0 -270 215.49 209.51 TF
(0.857) 0 -270 215.49 254.92 TF
(1.510E7) 0 -270 215.49 293.95 TF
(2.937E4) 0 -270 215.49 345.07 TF
(1.109E1) 0 -270 215.49 396.19 TF
(4.54E-4) 0 -270 215.49 448.07 TF
(-2.233) 0 -270 215.49 495.75 TF
(-2.244) 0 -270 215.49 534.5 TF
(-3.719) 0 -270 215.49 573.25 TF
(-3.247) 0 -270 215.49 612 TF
(HD190470) 0 -270 228.49 146.94 TF
(K3V) 0 -270 228.49 211 TF
(0.895) 0 -270 228.49 254.92 TF
(1.237E7) 0 -270 228.49 293.95 TF
(2.403E4) 0 -270 228.49 345.07 TF
(8.968E0) 0 -270 228.49 396.19 TF
(3.67E-4) 0 -270 228.49 448.07 TF
(-2.230) 0 -270 228.49 495.75 TF
(-2.241) 0 -270 228.49 534.5 TF
(-3.719) 0 -270 228.49 573.25 TF
(-3.246) 0 -270 228.49 612 TF
13 10 Q
(q) 0 -270 241.49 162.96 TF
0 7.2 Q
(1) 0 -270 237.89 168.17 TF
0 9 Q
(T) 0 -270 241.49 173.57 TF
(au) 0 -270 241.49 178.44 TF
(G8III) 0 -270 241.49 209.76 TF
(0.904) 0 -270 241.49 254.92 TF
(1.950E7) 0 -270 241.49 293.95 TF
(3.862E4) 0 -270 241.49 345.07 TF
(2.639E1) 0 -270 241.49 396.19 TF
(2.67E-4) 0 -270 241.49 448.07 TF
(-2.306) 0 -270 241.49 495.75 TF
(-2.320) 0 -270 241.49 534.5 TF
(-3.750) 0 -270 241.49 573.25 TF
(-3.262) 0 -270 241.49 612 TF
(HD170527) 0 -270 254.49 146.94 TF
(G5IV) 0 -270 254.49 209.51 TF
(0.918) 0 -270 254.49 254.92 TF
(2.157E7) 0 -270 254.49 293.95 TF
(4.277E4) 0 -270 254.49 345.07 TF
(2.944E1) 0 -270 254.49 396.19 TF
(2.98E-4) 0 -270 254.49 448.07 TF
(-2.309) 0 -270 254.49 495.75 TF
(-2.323) 0 -270 254.49 534.5 TF
(-3.750) 0 -270 254.49 573.25 TF
(-3.263) 0 -270 254.49 612 TF
(HD191615) 0 -270 267.49 146.94 TF
(G8IV) 0 -270 267.49 209.51 TF
(0.947) 0 -270 267.49 254.92 TF
(1.596E7) 0 -270 267.49 293.95 TF
(3.159E4) 0 -270 267.49 345.07 TF
(2.136E1) 0 -270 267.49 396.19 TF
(2.16E-4) 0 -270 267.49 448.07 TF
(-2.303) 0 -270 267.49 495.75 TF
(-2.317) 0 -270 267.49 534.5 TF
(-3.750) 0 -270 267.49 573.25 TF
(-3.261) 0 -270 267.49 612 TF
(HD4744) 0 -270 280.49 155.94 TF
(G8IV) 0 -270 280.49 209.51 TF
(0.989) 0 -270 280.49 254.92 TF
(1.087E7) 0 -270 280.49 293.95 TF
(2.1) 0 -270 280.49 345.24 TF
(19E4) 0 -270 280.49 356.15 TF
(8.241E0) 0 -270 280.49 396.19 TF
(3.37E-4) 0 -270 280.49 448.07 TF
(-2.240) 0 -270 280.49 495.75 TF
(-2.250) 0 -270 280.49 534.5 TF
(-3.719) 0 -270 280.49 573.25 TF
(-3.248) 0 -270 280.49 612 TF
(91 Aqr) 0 -270 293.49 161.69 TF
(K0III) 0 -270 293.49 209.76 TF
(1.010) 0 -270 293.49 254.92 TF
(8.535E6) 0 -270 293.49 293.95 TF
(1.662E4) 0 -270 293.49 345.07 TF
(6.381E0) 0 -270 293.49 396.19 TF
(2.61E-4) 0 -270 293.49 448.07 TF
(-2.237) 0 -270 293.49 495.75 TF
(-2.247) 0 -270 293.49 534.5 TF
(-3.719) 0 -270 293.49 573.25 TF
(-3.247) 0 -270 293.49 612 TF
(HD95272) 0 -270 306.49 151.44 TF
(K0III) 0 -270 306.49 209.76 TF
(1.041) 0 -270 306.49 254.92 TF
(8.184E6) 0 -270 306.49 293.95 TF
(1.593E4) 0 -270 306.49 345.07 TF
(6.086E0) 0 -270 306.49 396.19 TF
(2.49E-4) 0 -270 306.49 448.07 TF
(-2.236) 0 -270 306.49 495.75 TF
(-2.246) 0 -270 306.49 534.5 TF
(-3.719) 0 -270 306.49 573.25 TF
(-3.247) 0 -270 306.49 612 TF
13 10 Q
(y) 0 -270 319.49 159.08 TF
0 9 Q
(UMa) 0 -270 319.49 168.44 TF
(K1III) 0 -270 319.49 209.76 TF
(1.081) 0 -270 319.49 254.92 TF
(6.894E6) 0 -270 319.49 293.95 TF
(1.342E4) 0 -270 319.49 345.07 TF
(5.143E0) 0 -270 319.49 396.19 TF
(2.10E-4) 0 -270 319.49 448.07 TF
(-2.237) 0 -270 319.49 495.75 TF
(-2.247) 0 -270 319.49 534.5 TF
(-3.719) 0 -270 319.49 573.25 TF
(-3.247) 0 -270 319.49 612 TF
(BD+1) 0 -270 332.49 143.26 TF
0 7.2 Q
(o) 0 -270 328.89 165.33 TF
0 9 Q
(3131) 0 -270 332.49 168.93 TF
(K0III) 0 -270 332.49 209.76 TF
(1.143) 0 -270 332.49 254.92 TF
(4.403E6) 0 -270 332.49 293.95 TF
(8.51) 0 -270 332.49 345.24 TF
(1E3) 0 -270 332.49 360.65 TF
(7.928E0) 0 -270 332.49 396.19 TF
(2.54E-4) 0 -270 332.49 448.07 TF
(-2.210) 0 -270 332.49 495.75 TF
(-2.221) 0 -270 332.49 534.5 TF
(-3.718) 0 -270 332.49 573.25 TF
(-3.242) 0 -270 332.49 612 TF
(vB 173) 0 -270 345.49 160.68 TF
(1.202) 0 -270 345.49 254.92 TF
(6.753E6) 0 -270 345.49 293.95 TF
(1.337E4) 0 -270 345.49 345.07 TF
(2.396E1) 0 -270 345.49 396.19 TF
(7.80E-4) 0 -270 345.49 448.07 TF
(-2.296) 0 -270 345.49 495.75 TF
(-2.31) 0 -270 345.49 534.67 TF
(1) 0 -270 345.49 553.08 TF
(-3.721) 0 -270 345.49 573.25 TF
(-3.260) 0 -270 345.49 612 TF
(HD166780) 0 -270 358.49 146.94 TF
(K5III) 0 -270 358.49 209.76 TF
(1.323) 0 -270 358.49 254.92 TF
(2.059E6) 0 -270 358.49 293.95 TF
(3.986E3) 0 -270 358.49 345.07 TF
(3.791E0) 0 -270 358.49 396.19 TF
(1.21E-4) 0 -270 358.49 448.07 TF
(-2.214) 0 -270 358.49 495.75 TF
(-2.225) 0 -270 358.49 534.5 TF
(-3.718) 0 -270 358.49 573.25 TF
(-3.243) 0 -270 358.49 612 TF
(RZ Her) 0 -270 371.49 159.69 TF
(M6III) 0 -270 371.49 209.01 TF
(1.380) 0 -270 371.49 254.92 TF
(5.352E6) 0 -270 371.49 293.95 TF
(1.042E4) 0 -270 371.49 345.07 TF
(1.057E1) 0 -270 371.49 396.19 TF
(3.39E-4) 0 -270 371.49 448.07 TF
(-2.228) 0 -270 371.49 495.75 TF
(-2.239) 0 -270 371.49 534.5 TF
(-3.718) 0 -270 371.49 573.25 TF
(-3.246) 0 -270 371.49 612 TF
(HD1) 0 -270 384.49 147.27 TF
(16870) 0 -270 384.49 164.43 TF
(M0III) 0 -270 384.49 209.01 TF
(1.413) 0 -270 384.49 254.92 TF
(1.414E6) 0 -270 384.49 293.95 TF
(2.734E3) 0 -270 384.49 345.07 TF
(2.228E0) 0 -270 384.49 396.19 TF
(7.87E-5) 0 -270 384.49 448.07 TF
(-2.207) 0 -270 384.49 495.75 TF
(-2.218) 0 -270 384.49 534.5 TF
(-3.717) 0 -270 384.49 573.25 TF
(-3.241) 0 -270 384.49 612 TF
(M67 IV) 0 -270 397.49 142.52 TF
(-202) 0 -270 397.49 170.44 TF
(1.463) 0 -270 397.49 254.92 TF
(1.170E6) 0 -270 397.49 293.95 TF
(2.263E3) 0 -270 397.49 345.07 TF
(1.857E0) 0 -270 397.49 396.19 TF
(6.56E-5) 0 -270 397.49 448.07 TF
(-2.208) 0 -270 397.49 495.75 TF
(-2.219) 0 -270 397.49 534.5 TF
(-3.717) 0 -270 397.49 573.25 TF
(-3.242) 0 -270 397.49 612 TF
(HD104216) 0 -270 410.49 146.94 TF
(M2III) 0 -270 410.49 209.01 TF
(1.523) 0 -270 410.49 254.92 TF
(1.423E6) 0 -270 410.49 293.95 TF
(2.795E3) 0 -270 410.49 345.07 TF
(4.603E0) 0 -270 410.49 396.19 TF
(1.50E-4) 0 -270 410.49 448.07 TF
(-2.271) 0 -270 410.49 495.75 TF
(-2.287) 0 -270 410.49 534.5 TF
(-3.721) 0 -270 410.49 573.25 TF
(-3.255) 0 -270 410.49 612 TF
(BD\3201) 0 -270 423.49 144.17 TF
0 7.2 Q
(o) 0 -270 419.89 165.67 TF
0 9 Q
(31) 0 -270 423.49 169.27 TF
(13) 0 -270 423.49 177.93 TF
(K5III) 0 -270 423.49 209.76 TF
(1.609) 0 -270 423.49 254.92 TF
(8.070E5) 0 -270 423.49 293.95 TF
(1.588E3) 0 -270 423.49 345.07 TF
(2.681E0) 0 -270 423.49 396.19 TF
(8.72E-5) 0 -270 423.49 448.07 TF
(-2.277) 0 -270 423.49 495.75 TF
(-2.293) 0 -270 423.49 534.5 TF
(-3.721) 0 -270 423.49 573.25 TF
(-3.256) 0 -270 423.49 612 TF
(HD142804) 0 -270 436.49 146.94 TF
(M1III) 0 -270 436.49 209.01 TF
(1.694) 0 -270 436.49 254.92 TF
(7.419E5) 0 -270 436.49 293.95 TF
(1.463E3) 0 -270 436.49 345.07 TF
(2.517E0) 0 -270 436.49 396.19 TF
(8.19E-5) 0 -270 436.49 448.07 TF
(-2.283) 0 -270 436.49 495.75 TF
(-2.299) 0 -270 436.49 534.5 TF
(-3.721) 0 -270 436.49 573.25 TF
(-3.258) 0 -270 436.49 612 TF
(Gl 15B) 0 -270 449.49 160.68 TF
(M6V) 0 -270 449.49 210.25 TF
(1.707) 0 -270 449.49 254.92 TF
(2.391E6) 0 -270 449.49 293.95 TF
(4.742E3) 0 -270 449.49 345.07 TF
(8.704E0) 0 -270 449.49 396.19 TF
(2.83E-4) 0 -270 449.49 448.07 TF
(-2.303) 0 -270 449.49 495.75 TF
(-2.318) 0 -270 449.49 534.5 TF
(-3.721) 0 -270 449.49 573.25 TF
(-3.262) 0 -270 449.49 612 TF
(Gl 65) 0 -270 462.49 166.68 TF
(M5V) 0 -270 462.49 210.25 TF
(1.768) 0 -270 462.49 254.92 TF
(1.075E7) 0 -270 462.49 293.95 TF
(2.122E4) 0 -270 462.49 345.07 TF
(3.642E1) 0 -270 462.49 396.19 TF
(1.18E-3) 0 -270 462.49 448.07 TF
(-2.284) 0 -270 462.49 495.75 TF
(-2.300) 0 -270 462.49 534.5 TF
(-3.721) 0 -270 462.49 573.25 TF
(-3.258) 0 -270 462.49 612 TF
(HD 151658) 0 -270 475.49 144.69 TF
(M2III) 0 -270 475.49 209.01 TF
(1.770) 0 -270 475.49 254.92 TF
(7.242E5) 0 -270 475.49 293.95 TF
(1.423E3) 0 -270 475.49 345.07 TF
(2.359E0) 0 -270 475.49 396.19 TF
(7.67E-5) 0 -270 475.49 448.07 TF
(-2.272) 0 -270 475.49 495.75 TF
(-2.288) 0 -270 475.49 534.5 TF
(-3.721) 0 -270 475.49 573.25 TF
(-3.255) 0 -270 475.49 612 TF
(R Leo) 0 -270 488.49 164.69 TF
(1.918) 0 -270 488.49 254.92 TF
(4.550E6) 0 -270 488.49 293.95 TF
(8.879E3) 0 -270 488.49 345.07 TF
(1.308E1) 0 -270 488.49 396.19 TF
(4.26E-4) 0 -270 488.49 448.07 TF
(-2.245) 0 -270 488.49 495.75 TF
(-2.260) 0 -270 488.49 534.5 TF
(-3.721) 0 -270 488.49 573.25 TF
(-3.250) 0 -270 488.49 612 TF
(WZ Cas) 0 -270 501.49 157.19 TF
(N) 0 -270 501.49 216.5 TF
(2.636) 0 -270 501.49 254.92 TF
(1.987E5) 0 -270 501.49 293.95 TF
(3.867E2) 0 -270 501.49 345.07 TF
(5.89E-1) 0 -270 501.49 396.95 TF
(1.92E-5) 0 -270 501.49 448.07 TF
(-2.246) 0 -270 501.49 495.75 TF
(-2.263) 0 -270 501.49 534.5 TF
(-3.721) 0 -270 501.49 573.25 TF
(-3.250) 0 -270 501.49 612 TF
(A) 0 -270 514.49 155.41 TF
(W Cyg) 0 -270 514.49 161.18 TF
(N) 0 -270 514.49 216.5 TF
(3.790) 0 -270 514.49 254.92 TF
(1.951E5) 0 -270 514.49 293.95 TF
(3.796E2) 0 -270 514.49 345.07 TF
(5.70E-1) 0 -270 514.49 396.95 TF
(1.85E-5) 0 -270 514.49 448.07 TF
(-2.243) 0 -270 514.49 495.75 TF
(-2.260) 0 -270 514.49 534.5 TF
(-3.721) 0 -270 514.49 573.25 TF
(-3.249) 0 -270 514.49 612 TF
30.49 134.01 43.49 699 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
36.49 269.01 36.49 620.01 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
36.49 134.01 36.49 260.01 2 L
0 Z
N
0 0 612 792 C
2 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 0 -270 49.49 134.01 TF
(ABLE 7-1) 0 -270 49.49 138.84 TF
4 F
(Predicted target acquisition count rates for stars, reduced to) 0 -270 49.49 269.01 TF
8 F
(V) 0 -270 49.49 509.62 TF
8 7.2 Q
(0) 0 -270 51.74 515.62 TF
4 9 Q
(= 0. \050Continued\051) 0 -270 49.49 522.13 TF
2 8 Q
(Star Name) 0 -270 75.83 143.69 TF
(Spectral) 0 -270 70.83 203.97 TF
(T) 0 -270 80.83 210.71 TF
(ype) 0 -270 80.83 215.01 TF
6 F
(\050B\320V\051) 0 -270 75.83 252.82 TF
6 6.4 Q
(0) 0 -270 77.83 273.71 TF
2 8 Q
(count rate for mirror) 0 -270 67.83 347.08 TF
(reddening reduction factor) 0 -270 67.83 512.82 TF
2 6.4 Q
(a) 0 -270 64.63 614.61 TF
2 8 Q
(N2) 0 -270 83.83 303.96 TF
(A2) 0 -270 83.83 355.08 TF
(N1) 0 -270 83.83 406.21 TF
(A1) 0 -270 83.83 457.33 TF
(N2) 0 -270 83.83 502.26 TF
(A2) 0 -270 83.83 541.01 TF
(N1) 0 -270 83.83 579.76 TF
(A1) 0 -270 83.83 618.51 TF
58.62 134.01 519.37 134.01 2 L
V
0.25 H
0 Z
N
58.37 192.93 519.62 192.93 2 L
V
N
58.37 246.57 519.62 246.57 2 L
V
N
58.37 283.51 519.62 283.51 2 L
V
2 H
N
74.37 334.64 519.62 334.64 2 L
V
0.25 H
N
74.37 385.76 519.62 385.76 2 L
V
N
74.37 436.88 519.62 436.88 2 L
V
N
58.37 488 519.62 488 2 L
V
N
74.37 526.75 519.62 526.75 2 L
V
N
74.37 565.5 519.62 565.5 2 L
V
N
74.37 604.24 519.62 604.24 2 L
V
N
58.62 642.99 519.37 642.99 2 L
V
N
58.49 133.88 58.49 643.12 2 L
V
N
74.49 282.51 74.49 643.12 2 L
V
N
90.49 133.88 90.49 643.12 2 L
V
0.5 H
N
129.49 133.88 129.49 643.12 2 L
V
0.25 H
N
194.49 133.88 194.49 643.12 2 L
V
N
259.49 133.88 259.49 643.12 2 L
V
N
324.49 133.88 324.49 643.12 2 L
V
N
389.49 133.88 389.49 643.12 2 L
V
N
454.49 133.88 454.49 643.12 2 L
V
N
519.49 133.88 519.49 643.12 2 L
V
N
520.77 416.46 536.74 466.45 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 9 Q
0 X
0 0 0 1 0 0 0 K
(1) 0 -270 532.49 417.47 TF
(0) 0 -270 532.49 421.97 TF
3 7 Q
(f) 0 -270 527.02 426.81 TF
(E) 0 -270 527.02 436.09 TF
(B) 0 -270 527.02 445.08 TF
(V) 0 -270 527.02 456.35 TF
0 F
(\320) 0 -270 527.02 451.1 TF
13 F
(\050) 0 -270 527.02 442.08 TF
(\051) 0 -270 527.02 460.95 TF
(\264) 0 -270 527.02 430.5 TF
0 0 612 792 C
FMENDPAGE
%%EndPage: "75" 75
%%Page: "76" 76
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(T) 189 736.18 T
(arget Acquisition Reference Information) 193.83 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(76) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
72 669 558 672 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 670.5 558 670.5 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 670.5 198 670.5 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(7.3) 181.32 676 T
(Acquisition Count Rates for Extended Objects) 207 676 T
0 10 Q
0.62 (Chapter 4 mentions acquisition methodologies for extended objects, and, in particular) 207 648.33 P
0.62 (,) 555.5 648.33 P
-0.06 (the use of the) 207 636.33 P
9 F
-0.16 (EXTENDED) 262.84 636.33 P
0 F
-0.06 ( optional parameter) 310.84 636.33 P
-0.06 (. In this section we provide some guidance) 387.92 636.33 P
-0.06 (on predicting the count rates to be expected during an acquisition of an extended object,) 207 624.33 P
-0.14 (especially one beyond our own Galaxy) 207 612.33 P
-0.14 (. The renewed availability of Side 1 of the GHRS) 361.47 612.33 P
0.48 (and its G140L grating make it possible to get high-quality spectra of faint objects ef) 207 600.33 P
0.48 (\336-) 549.11 600.33 P
(ciently) 207 588.33 T
(.) 233.57 588.33 T
0.68 (Whenever possible, we recommend that faint objects be acquired by of) 207 564.33 P
0.68 (fsetting from a) 497.75 564.33 P
-0.09 (nearby and brighter point source. If accurate coordinates are used this method should be) 207 552.33 P
0.74 (reliable. However) 207 540.33 P
0.74 (, such objects are not always present next to tar) 278.98 540.33 P
0.74 (gets of astrophysical) 474.31 540.33 P
0.49 (interest. Also, obtaining a good astrometric position of an extended source can be pre-) 207 528.33 P
0.13 (vented by its lar) 207 516.33 P
0.13 (ge saturated area on the photographic plates upon which the Guide Star) 271.37 516.33 P
-0.08 (Catalog is based. In these cases a direct tar) 207 504.33 P
-0.08 (get acquisition will need to be attempted, and) 376.94 504.33 P
2.02 (it should succeed if the object provides enough ultraviolet photons. The procedure) 207 492.33 P
(closely follows that for point sources just described:) 207 480.33 T
10 11 Q
(\245) 207 462.33 T
0 10 Q
-0.15 (Find a star in T) 221.4 462.33 P
-0.15 (able) 281.22 462.33 P
-0.15 (7-1 with a spectral ener) 300.38 462.33 P
-0.15 (gy distribution like that of your object, or) 393.48 462.33 P
0.52 (consult the IUE Atlas of Star) 221.4 450.33 P
0.52 (-Forming Galaxies, by Kinney et al. \0501993, ApJS, 86,) 339.65 450.33 P
0.25 (5\051. This publication provides representative spectra of many classes of galaxies and) 221.4 438.33 P
(compares their shapes to ones of stellar spectra \050whence the \322spectral types\323 listed\051.) 221.4 426.33 T
10 11 Q
(\245) 207 411.33 T
0 10 Q
0.14 (Estimate the \337ux that will fall within the LSA from either T) 221.4 411.33 P
0.14 (able) 461.37 411.33 P
0.14 (7-1 or T) 480.53 411.33 P
0.14 (able) 512.87 411.33 P
0.14 (7-2 on) 532.03 411.33 P
(page) 221.4 399.33 T
(77, as appropriate.) 242.78 399.33 T
10 11 Q
(\245) 207 384.33 T
0 10 Q
0.62 (Calculate) 221.4 384.33 P
9 F
1.48 (STEP-TIME) 262.29 384.33 P
0 F
0.62 ( in the same manner as for stars. If necessary) 316.29 384.33 P
0.62 (, you may use) 500.59 384.33 P
-0.12 (mirror N2 on Side 2 for your acquisition, even if Side 1 is being used to observe, but) 221.4 372.33 P
(doing so will add about 40 minutes of overhead time.) 221.4 360.33 T
10 11 Q
(\245) 207 345.33 T
0 10 Q
(If your object does not fall within these categories, please consult us.) 221.4 345.33 T
FMENDPAGE
%%EndPage: "76" 76
%%Page: "77" 77
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (77) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(T) 207 736.18 T
(arget Acquisition Reference Information) 211.83 736.18 T
88.7 104.02 505.3 111.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(a. use factor) 235.7 98.02 T
3 F
(f) 281.68 98.02 T
0 F
( to reduce count rate by) 284.18 98.02 T
(.) 421.14 98.02 T
88.7 665.02 540 678.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
223.7 672.02 574.7 672.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
88.7 672.02 214.7 672.02 2 L
0 Z
N
0 0 612 792 C
2 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 88.7 659.02 T
(ABLE 7-2) 93.53 659.02 T
4 F
(Predicted count rates for non-stellar objects) 223.7 659.02 T
2 8 Q
(\322Spectral) 99.48 637.68 T
(T) 106.22 627.68 T
(ype\323) 110.52 627.68 T
(count rate for mirror) 209.4 640.68 T
(reddening reduction factor) 375.13 640.68 T
2 6.4 Q
(a) 476.92 643.88 T
2 8 Q
(N2) 166.27 624.68 T
(A2) 217.39 624.68 T
(N1) 268.52 624.68 T
(A1) 319.64 624.68 T
(N2) 364.57 624.68 T
(A2) 403.32 624.68 T
(N1) 442.07 624.68 T
(A1) 480.82 624.68 T
0 9 Q
(o3_6v) 106.01 610.02 T
(8.843E9) 156.26 610.02 T
(2.1) 207.55 610.02 T
(16E7) 218.46 610.02 T
(3.990E8) 258.5 610.02 T
(2.726E5) 309.62 610.02 T
(-3.059) 358.06 610.02 T
(-3.1) 396.98 610.02 T
(12) 410.89 610.02 T
(-3.362) 435.56 610.02 T
(-3.134) 474.31 610.02 T
(o4_9i) 107.01 597.02 T
(8.047E9) 156.26 597.02 T
(1.934E7) 207.38 597.02 T
(3.731E8) 258.5 597.02 T
(2.427E5) 309.62 597.02 T
(-3.054) 358.06 597.02 T
(-3.109) 396.81 597.02 T
(-3.380) 435.56 597.02 T
(-3.133) 474.31 597.02 T
(o5_6iii) 104.51 584.02 T
(8.935E9) 156.26 584.02 T
(2.140E7) 207.38 584.02 T
(3.961E8) 258.5 584.02 T
(2.687E5) 309.62 584.02 T
(-3.068) 358.06 584.02 T
(-3.121) 396.81 584.02 T
(-3.364) 435.56 584.02 T
(-3.136) 474.31 584.02 T
(o7_b0v) 103.76 571.02 T
(7.407E9) 156.26 571.02 T
(1.771E7) 207.38 571.02 T
(3.282E8) 258.5 571.02 T
(2.065E5) 309.62 571.02 T
(-3.028) 358.06 571.02 T
(-3.086) 396.81 571.02 T
(-3.388) 435.56 571.02 T
(-3.129) 474.31 571.02 T
(o9_b0iv) 102.51 558.02 T
(6.413E9) 156.26 558.02 T
(1.533E7) 207.38 558.02 T
(2.931E8) 258.5 558.02 T
(1.784E5) 309.62 558.02 T
(-3.012) 358.06 558.02 T
(-3.072) 396.81 558.02 T
(-3.396) 435.56 558.02 T
(-3.125) 474.31 558.02 T
(b0_2i) 107.01 545.02 T
(4.314E9) 156.26 545.02 T
(1.005E7) 207.38 545.02 T
(1.372E8) 258.5 545.02 T
(9.530E4) 309.62 545.02 T
(-2.949) 358.06 545.02 T
(-3.005) 396.81 545.02 T
(-3.378) 435.56 545.02 T
(-3.1) 474.47 545.02 T
(13) 488.39 545.02 T
(b0_2iii) 104.51 532.02 T
(5.144E9) 156.26 532.02 T
(1.214E7) 207.38 532.02 T
(1.908E8) 258.5 532.02 T
(1.231E5) 309.62 532.02 T
(-2.994) 358.06 532.02 T
(-3.051) 396.81 532.02 T
(-3.388) 435.56 532.02 T
(-3.122) 474.31 532.02 T
(b2_4v) 106.01 519.02 T
(2.889E9) 156.26 519.02 T
(6.765E6) 207.38 519.02 T
(1.037E8) 258.5 519.02 T
(7.131E4) 309.62 519.02 T
(-2.964) 358.06 519.02 T
(-3.021) 396.81 519.02 T
(-3.364) 435.56 519.02 T
(-3.1) 474.47 519.02 T
(16) 488.39 519.02 T
(b2_5iv) 104.76 506.02 T
(2.754E9) 156.26 506.02 T
(6.444E6) 207.38 506.02 T
(9.673E7) 258.5 506.02 T
(6.712E4) 309.62 506.02 T
(-2.960) 358.06 506.02 T
(-3.017) 396.81 506.02 T
(-3.367) 435.56 506.02 T
(-3.1) 474.47 506.02 T
(15) 488.39 506.02 T
(b3_5i) 107.01 493.02 T
(1.694E9) 156.26 493.02 T
(3.836E6) 207.38 493.02 T
(3.581E7) 258.5 493.02 T
(3.042E4) 309.62 493.02 T
(-2.859) 358.06 493.02 T
(-2.910) 396.81 493.02 T
(-3.328) 435.56 493.02 T
(-3.095) 474.31 493.02 T
(b3_6iii) 104.51 480.02 T
(2.344E9) 156.26 480.02 T
(5.448E6) 207.38 480.02 T
(7.404E7) 258.5 480.02 T
(5.400E4) 309.62 480.02 T
(-2.943) 358.06 480.02 T
(-2.998) 396.81 480.02 T
(-3.353) 435.56 480.02 T
(-3.1) 474.47 480.02 T
(12) 488.39 480.02 T
(b5_8v) 106.01 467.02 T
(1.713E9) 156.26 467.02 T
(3.952E6) 207.38 467.02 T
(4.849E7) 258.5 467.02 T
(3.716E4) 309.62 467.02 T
(-2.922) 358.06 467.02 T
(-2.976) 396.81 467.02 T
(-3.337) 435.56 467.02 T
(-3.108) 474.31 467.02 T
(b6_9i) 107.01 454.02 T
(9.689E8) 156.26 454.02 T
(2.187E6) 207.38 454.02 T
(2.021E7) 258.5 454.02 T
(1.765E4) 309.62 454.02 T
(-2.831) 358.06 454.02 T
(-2.882) 396.81 454.02 T
(-3.313) 435.56 454.02 T
(-3.089) 474.31 454.02 T
(b7_9iii) 104.51 441.02 T
(8.700E8) 156.26 441.02 T
(1.975E6) 207.38 441.02 T
(1.845E7) 258.5 441.02 T
(1.663E4) 309.62 441.02 T
(-2.867) 358.06 441.02 T
(-2.918) 396.81 441.02 T
(-3.305) 435.56 441.02 T
(-3.098) 474.31 441.02 T
(b8_9iv) 104.76 428.02 T
(9.701E8) 156.26 428.02 T
(2.216E6) 207.38 428.02 T
(2.337E7) 258.5 428.02 T
(1.984E4) 309.62 428.02 T
(-2.889) 358.06 428.02 T
(-2.941) 396.81 428.02 T
(-3.316) 435.56 428.02 T
(-3.102) 474.31 428.02 T
(f2_7iv) 105.51 415.02 T
(1.007E8) 156.26 415.02 T
(2.108E5) 207.38 415.02 T
(2.968E4) 258.5 415.02 T
(1.206E2) 309.62 415.02 T
(-2.547) 358.06 415.02 T
(-2.580) 396.81 415.02 T
(-3.201) 435.56 415.02 T
(-3.043) 474.31 415.02 T
(f2_8i) 107.76 402.02 T
(4.536E7) 156.26 402.02 T
(9.480E4) 207.38 402.02 T
(1.403E4) 258.5 402.02 T
(5.634E1) 309.62 402.02 T
(-2.535) 358.06 402.02 T
(-2.569) 396.81 402.02 T
(-3.201) 435.56 402.02 T
(-3.041) 474.31 402.02 T
(f5_7v) 106.76 389.02 T
(1.079E8) 156.26 389.02 T
(2.254E5) 207.38 389.02 T
(1.782E4) 258.5 389.02 T
(-2.538) 358.06 389.02 T
(-2.571) 396.81 389.02 T
(-3.238) 435.56 389.02 T
(f6iii) 109.76 376.02 T
(9.009E7) 156.26 376.02 T
(1.862E5) 207.38 376.02 T
(8.586E2) 258.5 376.02 T
(-2.499) 358.06 376.02 T
(-2.526) 396.81 376.02 T
(-3.830) 435.56 376.02 T
(f8_9v) 106.76 363.02 T
(6.664E7) 156.26 363.02 T
(1.367E5) 207.38 363.02 T
(3.996E3) 258.5 363.02 T
(-2.460) 358.06 363.02 T
(-2.484) 396.81 363.02 T
(-3.245) 435.56 363.02 T
(g0_2iv) 104.76 350.02 T
(4.451E7) 156.26 350.02 T
(9.041E4) 207.38 350.02 T
(3.614E2) 258.5 350.02 T
(-2.415) 358.06 350.02 T
(-2.434) 396.81 350.02 T
(-3.604) 435.56 350.02 T
(g0_3i) 107.01 337.02 T
(1.971E7) 156.26 337.02 T
(4.015E4) 207.38 337.02 T
(-2.429) 358.06 337.02 T
(-2.444) 396.81 337.02 T
(g0_5iii) 104.51 324.02 T
(3.349E7) 156.26 324.02 T
(6.822E4) 207.38 324.02 T
(-2.431) 358.06 324.02 T
(-2.450) 396.81 324.02 T
(g0_5v) 106.01 311.02 T
(5.372E7) 156.26 311.02 T
(1.095E5) 207.38 311.02 T
(-2.428) 358.06 311.02 T
(-2.449) 396.81 311.02 T
(g5_8i) 107.01 298.02 T
(4.802E6) 156.26 298.02 T
(9.721E3) 207.38 298.02 T
(-2.399) 358.06 298.02 T
(-2.414) 396.81 298.02 T
(g5_8iv) 104.76 285.02 T
(2.123E7) 156.26 285.02 T
(4.242E4) 207.38 285.02 T
(-2.344) 358.06 285.02 T
(-2.354) 396.81 285.02 T
(g5_k0iii) 102.26 272.02 T
(6.969E6) 156.26 272.02 T
(1.384E4) 207.38 272.02 T
(-2.320) 358.06 272.02 T
(-2.330) 396.81 272.02 T
(g6_9v) 106.01 259.02 T
(2.588E7) 156.26 259.02 T
(5.189E4) 207.38 259.02 T
(-2.360) 358.06 259.02 T
(-2.372) 396.81 259.02 T
(g8_k1iv) 102.51 246.02 T
(8.008E6) 156.26 246.02 T
(1.583E4) 207.38 246.02 T
(-2.297) 358.06 246.02 T
(-2.304) 396.81 246.02 T
(k0_1v) 106.01 233.02 T
(1.307E7) 156.26 233.02 T
(2.606E4) 207.38 233.02 T
(-2.337) 358.06 233.02 T
(-2.348) 396.81 233.02 T
(k0_2iii) 104.51 220.02 T
(5.918E6) 156.26 220.02 T
(1.165E4) 207.38 220.02 T
(-2.285) 358.06 220.02 T
(-2.290) 396.81 220.02 T
(k1_3i) 107.01 207.02 T
(2.497E6) 156.26 207.02 T
(5.057E3) 207.38 207.02 T
(-2.397) 358.06 207.02 T
(-2.41) 396.98 207.02 T
(1) 415.39 207.02 T
(k2_3v) 106.01 194.02 T
(9.035E6) 156.26 194.02 T
(1.800E4) 207.38 194.02 T
(-2.327) 358.06 194.02 T
(-2.336) 396.81 194.02 T
(k2iii) 109.01 181.02 T
(2.092E6) 156.26 181.02 T
(4.107E3) 207.38 181.02 T
(-2.268) 358.06 181.02 T
(-2.273) 396.81 181.02 T
(k3iii) 109.01 168.02 T
(1.157E6) 156.26 168.02 T
(2.266E3) 207.38 168.02 T
(-2.259) 358.06 168.02 T
(-2.264) 396.81 168.02 T
(k4_5iii) 104.51 155.02 T
(5.490E5) 156.26 155.02 T
(1.085E3) 207.38 155.02 T
(-2.290) 358.06 155.02 T
(-2.296) 396.81 155.02 T
(k5_m0v) 102.51 142.02 T
(2.607E6) 156.26 142.02 T
(5.167E3) 207.38 142.02 T
(-2.304) 358.06 142.02 T
(-2.31) 396.98 142.02 T
(1) 415.39 142.02 T
(k5_m5i) 103.51 129.02 T
(9.714E5) 156.26 129.02 T
(1.976E3) 207.38 129.02 T
(-2.413) 358.06 129.02 T
(-2.426) 396.81 129.02 T
(k7_m3iii) 101.01 116.02 T
(5.420E5) 156.26 116.02 T
(1.081E3) 207.38 116.02 T
(-2.323) 358.06 116.02 T
(-2.330) 396.81 116.02 T
88.7 649.89 88.7 111.14 2 L
V
0.25 H
0 Z
N
145.82 650.14 145.82 110.89 2 L
V
N
196.95 634.14 196.95 110.89 2 L
V
N
248.07 634.14 248.07 110.89 2 L
V
N
299.19 634.14 299.19 110.89 2 L
V
N
350.31 650.14 350.31 110.89 2 L
V
N
389.06 634.14 389.06 110.89 2 L
V
N
427.81 634.14 427.81 110.89 2 L
V
N
466.55 634.14 466.55 110.89 2 L
V
N
505.3 649.89 505.3 111.14 2 L
V
N
88.57 650.02 505.43 650.02 2 L
V
N
145.7 634.02 505.43 634.02 2 L
V
N
88.57 618.02 505.43 618.02 2 L
V
0.5 H
N
88.57 553.02 505.43 553.02 2 L
V
0.25 H
N
88.57 488.02 505.43 488.02 2 L
V
N
88.57 423.02 505.43 423.02 2 L
V
N
88.57 358.02 505.43 358.02 2 L
V
N
88.57 293.02 505.43 293.02 2 L
V
N
88.57 228.02 505.43 228.02 2 L
V
N
88.57 163.02 505.43 163.02 2 L
V
N
88.57 111.02 505.43 111.02 2 L
V
N
371.16 93.77 421.14 109.74 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 9 Q
0 X
0 0 0 1 0 0 0 K
(1) 372.16 98.02 T
(0) 376.66 98.02 T
3 7 Q
(f) 381.5 103.49 T
(E) 390.78 103.49 T
(B) 399.77 103.49 T
(V) 411.04 103.49 T
0 F
(\320) 405.79 103.49 T
13 F
(\050) 396.77 103.49 T
(\051) 415.64 103.49 T
(\264) 385.19 103.49 T
0 0 612 792 C
FMENDPAGE
%%EndPage: "77" 77
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(T) 189 736.18 T
(arget Acquisition Reference Information) 193.83 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(78) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
72 671.02 558 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 672.52 558 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 672.52 198 672.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(7.4) 181.32 678.02 T
(Other Acquisition Information) 207 678.02 T
2 10 Q
(7.4.1) 175.76 644.35 T
(Effective Areas of the Acquisition Mirrors) 207 644.35 T
0 F
0.04 (T) 207 620.35 P
0.04 (able) 212.41 620.35 P
0.04 (7-3 on page) 231.57 620.35 P
0.04 (79 lists the ef) 281.35 620.35 P
0.04 (fective areas of the four acquisition mirrors \050in) 334.89 620.35 P
0.04 (\051 as) 543.8 620.35 P
1.38 (a function of wavelength, to use to predict acquisition count rates. These values are) 207 608.35 P
-0.17 (those from the Science V) 207 596.35 P
-0.17 (eri\336cation Report for the GHRS, adjusted by the observed ratio) 306.28 596.35 P
-0.09 (of post- to pre-COST) 207 584.35 P
-0.09 (AR sensitivities \050see Section) 291.19 584.35 P
-0.09 (8.1 on page) 408.13 584.35 P
-0.09 (82\051. Note that A1 and N1) 456.82 584.35 P
(may only be used with detector D1 and A2 and N2 with detector D2.) 207 572.35 T
0.33 (Also note that the proper use of this table requires compensation for the dif) 207 548.35 P
0.33 (ferent ener-) 511.31 548.35 P
-0.18 (gies of photons of dif) 207 536.35 P
-0.18 (ferent wavelengths, hence the last column, which is in picoer) 291.66 536.35 P
-0.18 (gs per) 534.02 536.35 P
(photon.) 207 524.35 T
2 F
0.19 (Figure 7-5.) 144 179.33 P
4 F
0.19 (Relative sensitivities of the GHRS acquisition mirrors. The ef) 200.7 179.33 P
0.19 (fec-) 469.33 179.33 P
(tive areas shown are from T) 144 167.33 T
(able) 266.82 167.33 T
(7-3 on page) 288.5 167.33 T
(79.) 344.65 167.33 T
524.58 615.85 543.8 629.47 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(c) 525.58 620.35 T
(m) 530.02 620.35 T
0 7 Q
(2) 538.3 623.22 T
0 0 612 792 C
72 87.98 558 686.02 C
72 195 558 506.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
270 29 38 538 744 285.03 395.35 172.48 152.83 FMBEGINEPSF
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2194 1574 d 2199 1569 d 2206 1567 d 2211 1567 d 2218 1569 d 2223 1574 d
2226 1579 d 2226 1586 d 2223 1591 d 2218 1596 d 2192 1612 r 2226 1612 d
2202 1612 r 2194 1620 d 2192 1624 d 2192 1632 d 2194 1636 d 2202 1639 d
2226 1639 d 2192 1682 r 2230 1682 d 2238 1680 d 2240 1677 d 2242 1672 d
2242 1665 d 2240 1660 d 2199 1682 r 2194 1677 d 2192 1672 d 2192 1665 d
2194 1660 d 2199 1656 d 2206 1653 d 2211 1653 d 2218 1656 d 2223 1660 d
2226 1665 d 2226 1672 d 2223 1677 d 2218 1682 d 2175 1701 r 2216 1701 d
2223 1704 d 2226 1708 d 2226 1713 d 2192 1694 r 2192 1711 d 2175 1723 r
2226 1723 d 2202 1723 r 2194 1730 d 2192 1735 d 2192 1742 d 2194 1747 d
2202 1749 d 2226 1749 d 2166 1821 r 2170 1816 d 2178 1812 d 2187 1807 d
2199 1804 d 2209 1804 d 2221 1807 d 2230 1812 d 2238 1816 d 2242 1821 d
2175 1850 r 2226 1831 d 2175 1850 r 2226 1869 d 2209 1838 r 2209 1862 d
2192 1881 r 2226 1881 d 2202 1881 r 2194 1888 d 2192 1893 d 2192 1900 d
2194 1905 d 2202 1908 d 2226 1908 d 2192 1951 r 2230 1951 d 2238 1948 d
2240 1946 d 2242 1941 d 2242 1934 d 2240 1929 d 2199 1951 r 2194 1946 d
2192 1941 d 2192 1934 d 2194 1929 d 2199 1924 d 2206 1922 d 2211 1922 d
2218 1924 d 2223 1929 d 2226 1934 d 2226 1941 d 2223 1946 d 2218 1951 d
2199 1992 r 2194 1989 d 2192 1982 d 2192 1975 d 2194 1968 d 2199 1965 d
2204 1968 d 2206 1972 d 2209 1984 d 2211 1989 d 2216 1992 d 2218 1992 d
2223 1989 d 2226 1982 d 2226 1975 d 2223 1968 d 2218 1965 d 2175 2008 r
2216 2008 d 2223 2011 d 2226 2016 d 2226 2020 d 2192 2001 r 2192 2018 d
2192 2030 r 2226 2030 d 2206 2030 r 2199 2032 d 2194 2037 d 2192 2042 d
2192 2049 d 2192 2073 r 2194 2068 d 2199 2064 d 2206 2061 d 2211 2061 d
2218 2064 d 2223 2068 d 2226 2073 d 2226 2080 d 2223 2085 d 2218 2090 d
2211 2092 d 2206 2092 d 2199 2090 d 2194 2085 d 2192 2080 d 2192 2073 d
2192 2107 r 2226 2107 d 2202 2107 r 2194 2114 d 2192 2119 d 2192 2126 d
2194 2131 d 2202 2133 d 2226 2133 d 2202 2133 r 2194 2140 d 2192 2145 d
2192 2152 d 2194 2157 d 2202 2160 d 2226 2160 d 2199 2203 r 2194 2200 d
2192 2193 d 2192 2186 d 2194 2179 d 2199 2176 d 2204 2179 d 2206 2184 d
2209 2196 d 2211 2200 d 2216 2203 d 2218 2203 d 2223 2200 d 2226 2193 d
2226 2186 d 2223 2179 d 2218 2176 d 2166 2215 r 2170 2220 d 2178 2224 d
2187 2229 d 2199 2232 d 2209 2232 d 2221 2229 d 2230 2224 d 2238 2220 d
2242 2215 d 1986 1042 r 1650 1096 d 1371 1150 d 1256 1204 d 1245 1258 d
1281 1313 d 1394 1367 d 1514 1421 d 1691 1475 d 1671 554 r 777 608 d
632 663 d 569 717 d 548 771 d 540 825 d 542 879 d 544 933 d
544 988 d 547 1042 d 563 1096 d 566 1150 d 581 1204 d 623 1258 d
673 1313 d 729 1367 d 833 1421 d 960 1475 d 1035 1529 d 1106 1583 d
1180 1638 d 1798 554 r 1214 608 d 1110 663 d 1091 717 d 1081 771 d
1091 825 d 1114 879 d 1114 933 d 1119 988 d 1110 1042 d 1102 1096 d
1081 1150 d 1061 1204 d 1033 1258 d 1010 1313 d 1000 1367 d 992 1421 d
960 1475 d 960 1529 d 955 1583 d 950 1638 d 922 1746 d 913 1854 d
898 1963 d 891 2071 d 892 2179 d 893 2288 d 903 2396 d 916 2504 d
997 2613 d 1028 2721 d 1078 2829 d 1148 2938 d 1196 3046 d 1170 554 r
593 608 d 494 663 d 453 717 d 426 771 d 425 825 d 425 879 d
415 933 d 407 988 d 387 1042 d 369 1096 d 362 1150 d 355 1204 d
330 1258 d 309 1313 d 299 1367 d 291 1421 d 270 1475 d 269 1529 d
256 1583 d 244 1638 d 211 1746 d 198 1854 d 180 1963 d 169 2071 d
169 2179 d 167 2288 d 174 2396 d 183 2504 d 258 2613 d 288 2721 d
343 2829 d 403 2938 d 448 3046 d 1242 1356 r 1293 1336 d 1242 1356 r
1293 1375 d 1276 1344 r 1276 1368 d 1252 1392 r 1249 1396 d 1242 1404 d
1293 1404 d 960 2264 r 1011 2244 d 960 2264 r 1011 2283 d 994 2252 r
994 2276 d 972 2295 r 970 2295 d 965 2297 d 963 2300 d 960 2304 d
960 2314 d 963 2319 d 965 2321 d 970 2324 d 975 2324 d 979 2321 d
987 2316 d 1011 2292 d 1011 2326 d 783 1453 r 834 1453 d 783 1453 r
834 1486 d 783 1486 r 834 1486 d 793 1510 r 790 1515 d 783 1522 d
834 1522 d 230 2248 r 281 2248 d 230 2248 r 281 2281 d 230 2281 r
281 2281 d 242 2300 r 240 2300 d 235 2303 d 233 2305 d 230 2310 d
230 2320 d 233 2324 d 235 2327 d 240 2329 d 245 2329 d 249 2327 d
257 2322 d 281 2298 d 281 2332 d
e
%%Trailer
EndPSPlot

%%EndDocument
FMENDEPSF
72 87.98 558 686.02 C
0 0 612 792 C
FMENDPAGE
%%EndPage: "78" 78
%%Page: "79" 79
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (79) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(T) 207 736.18 T
(arget Acquisition Reference Information) 211.83 736.18 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 660.02 540 673.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 667.02 540 667.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 667.02 180 667.02 2 L
0 Z
N
0 0 612 792 C
2 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 654.02 T
(ABLE 7-3.) 58.83 654.02 T
4 F
(Ef) 189 654.02 T
(fective areas of the four GHRS acquisition mirrors) 197.34 654.02 T
2 8 Q
(W) 203.14 613.68 T
(avelength) 210.39 613.68 T
(\050\201\051) 249.96 613.68 T
(Effective Area \050cm) 342.89 630.68 T
2 6.4 Q
(2) 412.69 633.88 T
2 8 Q
(\051) 416.25 630.68 T
(perg) 504.33 622.68 T
(photon) 496.6 613.68 T
2 6.4 Q
(-1) 523.71 616.88 T
2 8 Q
(A1) 294.79 613.68 T
(N1) 345.89 613.68 T
(A2) 399.89 613.68 T
(N2) 453.89 613.68 T
0 9 Q
(1) 223.27 599.02 T
(100) 227.43 599.02 T
(0.0025) 338.62 599.02 T
(0.00085) 390.38 599.02 T
(0.175) 448.88 599.02 T
(18.1) 505.12 599.02 T
(1) 223.27 584.02 T
(150) 227.43 584.02 T
(4.89) 343.12 584.02 T
(0.12) 397.12 584.02 T
(23.36) 448.88 584.02 T
(17.3) 505.12 584.02 T
(1200) 223.1 569.02 T
(16.79) 340.88 569.02 T
(0.29) 397.12 569.02 T
(54.18) 448.88 569.02 T
(16.6) 505.12 569.02 T
(1250) 223.1 554.02 T
(28.54) 340.88 554.02 T
(0.34) 397.12 554.02 T
(76.50) 448.88 554.02 T
(15.9) 505.12 554.02 T
(1300) 223.1 539.02 T
(34.10) 340.88 539.02 T
(0.37) 397.12 539.02 T
(96.22) 448.88 539.02 T
(15.3) 505.12 539.02 T
(1350) 223.1 524.02 T
(36.64) 340.88 524.02 T
(0.34) 397.12 524.02 T
(97.03) 448.88 524.02 T
(14.7) 505.12 524.02 T
(1400) 223.1 509.02 T
(36.05) 340.88 509.02 T
(0.28) 397.12 509.02 T
(96.88) 448.88 509.02 T
(14.2) 505.12 509.02 T
(1450) 223.1 494.02 T
(35.35) 340.88 494.02 T
(0.28) 397.12 494.02 T
(105.46) 446.62 494.02 T
(13.7) 505.12 494.02 T
(1500) 223.1 479.02 T
(35.49) 340.88 479.02 T
(0.27) 397.12 479.02 T
(1) 446.79 479.02 T
(13.43) 450.96 479.02 T
(13.2) 505.12 479.02 T
(1550) 223.1 464.02 T
(0.000172) 283.02 464.02 T
(34.43) 340.88 464.02 T
(0.29) 397.12 464.02 T
(133.84) 446.62 464.02 T
(12.8) 505.12 464.02 T
(1600) 223.1 449.02 T
(0.00298) 285.27 449.02 T
(30.18) 340.88 449.02 T
(0.31) 397.12 449.02 T
(155.76) 446.62 449.02 T
(12.4) 505.12 449.02 T
(1650) 223.1 434.02 T
(0.0317) 287.52 434.02 T
(29.37) 340.88 434.02 T
(0.37) 397.12 434.02 T
(165.92) 446.62 434.02 T
(12.0) 505.12 434.02 T
(1700) 223.1 419.02 T
(0.0843) 287.52 419.02 T
(25.91) 340.88 419.02 T
(0.44) 397.12 419.02 T
(176.10) 446.62 419.02 T
(1) 505.29 419.02 T
(1.7) 509.46 419.02 T
(1750) 223.1 404.02 T
(0.0923) 287.52 404.02 T
(18.1) 341.04 404.02 T
(1) 356.46 404.02 T
(0.56) 397.12 404.02 T
(216.91) 446.62 404.02 T
(1) 505.29 404.02 T
(1.4) 509.46 404.02 T
(1800) 223.1 389.02 T
(0.0680) 287.52 389.02 T
(1) 341.04 389.02 T
(1.82) 345.21 389.02 T
(0.68) 397.12 389.02 T
(259.65) 446.62 389.02 T
(1) 505.29 389.02 T
(1.0) 509.46 389.02 T
(1850) 223.1 374.02 T
(0.0261) 287.52 374.02 T
(7.38) 343.12 374.02 T
(0.74) 397.12 374.02 T
(281.80) 446.62 374.02 T
(10.7) 505.12 374.02 T
(1900) 223.1 359.02 T
(0.0094) 287.52 359.02 T
(3.04) 343.12 359.02 T
(0.79) 397.12 359.02 T
(302.40) 446.62 359.02 T
(10.5) 505.12 359.02 T
(1950) 223.1 344.02 T
(0.0021) 287.52 344.02 T
(1.04) 343.12 344.02 T
(1.04) 397.12 344.02 T
(362.78) 446.62 344.02 T
(10.2) 505.12 344.02 T
(2000) 223.1 329.02 T
(0.55) 343.12 329.02 T
(1.04) 397.12 329.02 T
(363.32) 446.62 329.02 T
(9.93) 505.12 329.02 T
(2050) 223.1 314.02 T
(0.30) 343.12 314.02 T
(1.08) 397.12 314.02 T
(406.51) 446.62 314.02 T
(9.69) 505.12 314.02 T
(2100) 223.1 299.02 T
(0.16) 343.12 299.02 T
(1.13) 397.12 299.02 T
(449.71) 446.62 299.02 T
(9.46) 505.12 299.02 T
(2200) 223.1 284.02 T
(1.43) 397.12 284.02 T
(594.61) 446.62 284.02 T
(9.03) 505.12 284.02 T
(2300) 223.1 269.02 T
(1.55) 397.12 269.02 T
(663.74) 446.62 269.02 T
(8.64) 505.12 269.02 T
(2400) 223.1 254.02 T
(1.75) 397.12 254.02 T
(776.52) 446.62 254.02 T
(8.28) 505.12 254.02 T
(2500) 223.1 239.02 T
(1.87) 397.12 239.02 T
(847.76) 446.62 239.02 T
(7.95) 505.12 239.02 T
(2600) 223.1 224.02 T
(1.85) 397.12 224.02 T
(854.42) 446.62 224.02 T
(7.64) 505.12 224.02 T
(2700) 223.1 209.02 T
(1.83) 397.12 209.02 T
(866.65) 446.62 209.02 T
(7.36) 505.12 209.02 T
(2800) 223.1 194.02 T
(1.68) 397.12 194.02 T
(813.29) 446.62 194.02 T
(7.09) 505.12 194.02 T
(2900) 223.1 179.02 T
(1.50) 397.12 179.02 T
(754.81) 446.62 179.02 T
(6.85) 505.12 179.02 T
(3000) 223.1 164.02 T
(0.76) 397.12 164.02 T
(398.89) 446.62 164.02 T
(6.62) 505.12 164.02 T
(3100) 223.1 149.02 T
(0.58) 397.12 149.02 T
(309.31) 446.62 149.02 T
(6.41) 505.12 149.02 T
(3200) 223.1 134.02 T
(0.38) 397.12 134.02 T
(194.15) 446.62 134.02 T
(6.21) 505.12 134.02 T
(3300) 223.1 119.02 T
(0.21) 397.12 119.02 T
(1) 446.79 119.02 T
(16.67) 450.96 119.02 T
(6.02) 505.12 119.02 T
(3400) 223.1 104.02 T
(0.14) 397.12 104.02 T
(80.) 453.38 104.02 T
(5.84) 505.12 104.02 T
188.4 642.89 188.4 99.14 2 L
V
0.25 H
0 Z
N
275.8 643.14 275.8 98.89 2 L
V
N
324 626.14 324 98.89 2 L
V
N
378 626.14 378 98.89 2 L
V
N
432 626.14 432 98.89 2 L
V
N
486 643.14 486 98.89 2 L
V
N
540 642.89 540 99.14 2 L
V
N
188.27 643.02 540.12 643.02 2 L
V
N
275.68 626.02 486.12 626.02 2 L
V
N
188.27 609.02 540.12 609.02 2 L
V
0.5 H
N
188.27 594.02 540.12 594.02 2 L
V
0.25 H
N
188.27 579.02 540.12 579.02 2 L
V
N
188.27 564.02 540.12 564.02 2 L
V
N
188.27 549.02 540.12 549.02 2 L
V
N
188.27 534.02 540.12 534.02 2 L
V
N
188.27 519.02 540.12 519.02 2 L
V
N
188.27 504.02 540.12 504.02 2 L
V
N
188.27 489.02 540.12 489.02 2 L
V
N
188.27 474.02 540.12 474.02 2 L
V
N
188.27 459.02 540.12 459.02 2 L
V
N
188.27 444.02 540.12 444.02 2 L
V
N
188.27 429.02 540.12 429.02 2 L
V
N
188.27 414.02 540.12 414.02 2 L
V
N
188.27 399.02 540.12 399.02 2 L
V
N
188.27 384.02 540.12 384.02 2 L
V
N
188.27 369.02 540.12 369.02 2 L
V
N
188.27 354.02 540.12 354.02 2 L
V
N
188.27 339.02 540.12 339.02 2 L
V
N
188.27 324.02 540.12 324.02 2 L
V
N
188.27 309.02 540.12 309.02 2 L
V
N
188.27 294.02 540.12 294.02 2 L
V
N
188.27 279.02 540.12 279.02 2 L
V
N
188.27 264.02 540.12 264.02 2 L
V
N
188.27 249.02 540.12 249.02 2 L
V
N
188.27 234.02 540.12 234.02 2 L
V
N
188.27 219.02 540.12 219.02 2 L
V
N
188.27 204.02 540.12 204.02 2 L
V
N
188.27 189.02 540.12 189.02 2 L
V
N
188.27 174.02 540.12 174.02 2 L
V
N
188.27 159.02 540.12 159.02 2 L
V
N
188.27 144.02 540.12 144.02 2 L
V
N
188.27 129.02 540.12 129.02 2 L
V
N
188.27 114.02 540.12 114.02 2 L
V
N
188.27 99.02 540.12 99.02 2 L
V
N
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(T) 189 736.18 T
(arget Acquisition Reference Information) 193.83 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(80) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
(7.4.2) 157.76 679.35 T
(Geocoronal L) 189 679.35 T
(yman-) 253.09 679.35 T
13 F
(a) 282.54 679.35 T
2 F
( Background) 288.85 679.35 T
0 F
1.33 (The acquisition mirror sensitivity curves illustrated above show that the mirrors still) 189 655.35 P
0.28 (re\337ect well at the L) 189 643.35 P
0.28 (yman-) 267.34 643.35 P
13 F
0.28 (a) 292.89 643.35 P
0 F
0.28 ( line at 1216 \201. Note that L) 299.2 643.35 P
0.28 (y-) 410.62 643.35 P
13 F
0.28 (a) 418.95 643.35 P
0 F
0.28 ( is suppressed by mirror A1.) 425.26 643.35 P
0.98 (T) 189 631.35 P
0.98 (ests have shown that the count rate from geocoronal L) 194.41 631.35 P
0.98 (yman-) 419.53 631.35 P
13 F
0.98 (a) 445.08 631.35 P
0 F
0.98 ( can be as high as 12) 451.39 631.35 P
0.95 (counts per second per diode. If you wish to acquire a faint tar) 189 619.35 P
0.95 (get with the least L) 445.45 619.35 P
0.95 (y-) 525.36 619.35 P
13 F
0.95 (a) 533.69 619.35 P
0 F
0.92 (contamination, we suggest that you specify) 189 607.35 P
9 F
2.22 (DARK) 369.8 607.35 P
2.22 (TIME) 397.23 607.35 P
0 F
0.92 ( as a Special Requirement in) 421.23 607.35 P
(Phase II.) 189 595.35 T
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (81) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
7 12 Q
1.2 (Chapter 8) 72 677 S
5 24 Q
-0.48 (Refer) 207 677 S
-0.48 (ence T) 254.86 677 S
-0.48 (ables for) 311.76 677 S
-0.48 (Instrument Performance) 207 647 S
4 12 Q
(8.1) 144 415 T
( The Ef) 164.02 415 T
(fect of COST) 202.49 415 T
(AR on the GHRS) 270.96 415 T
8 F
( 82) 505.32 415 T
4 F
(8.2) 144 397 T
( Properties of the First-Order Gratings) 164.02 397 T
8 F
( 83) 505.32 397 T
4 10 Q
(8.2.1) 162 380.33 T
( Useful W) 187.02 380.33 T
(avelength Ranges) 229.99 380.33 T
8 F
( 83) 508.1 380.33 T
4 F
(8.2.2) 162 364.33 T
( Resolving Power) 187.02 364.33 T
8 F
( 83) 508.1 364.33 T
4 F
(8.2.3) 162 348.33 T
( Sensitivity Functions for the First-Order Gratings) 187.02 348.33 T
8 F
( 85) 508.1 348.33 T
4 12 Q
(8.3) 144 331 T
( Properties of the Echelle Gratings) 164.02 331 T
8 F
( 87) 505.32 331 T
4 10 Q
(8.3.1) 162 314.33 T
( W) 187.02 314.33 T
(avelength Coverage, Bandpass, and Sensitivity) 198.87 314.33 T
8 F
( 87) 508.1 314.33 T
4 F
(8.3.2) 162 298.33 T
( Echelle W) 187.02 298.33 T
(avelength Formats) 234.44 298.33 T
8 F
( 89) 508.1 298.33 T
4 F
(8.3.3) 162 282.33 T
( Echelle Blaze Function) 187.02 282.33 T
8 F
( 91) 508.1 282.33 T
4 12 Q
(8.4) 144 265 T
( Standard Patterns for Substepping and Background Measurement) 164.02 265 T
8 F
( 92) 525.54 265 T
4 F
(8.5) 144 247 T
( The Ef) 164.02 247 T
(fects of Reddening in the Ultraviolet) 202.49 247 T
8 F
( 93) 505.32 247 T
4 F
(8.6) 144 229 T
( Instrumental Properties) 164.02 229 T
8 F
( 94) 505.32 229 T
4 10 Q
(8.6.1) 162 212.33 T
( The Point Spread Function) 187.02 212.33 T
8 F
( 94) 508.1 212.33 T
4 F
(8.6.2) 162 196.33 T
( Detector Dark Count and the CENSOR Option) 187.02 196.33 T
8 F
( 95) 508.1 196.33 T
4 F
(8.6.3) 162 180.33 T
( Noise Rejection with FL) 187.02 180.33 T
(YLIM) 294.09 180.33 T
8 F
( 97) 508.1 180.33 T
4 F
(8.6.4) 162 164.33 T
( Count Rate Linearity) 187.02 164.33 T
8 F
( 98) 508.1 164.33 T
4 F
(8.6.5) 162 148.33 T
( Image Stability) 187.02 148.33 T
8 F
( 98) 508.1 148.33 T
4 F
(8.6.6) 162 132.33 T
( W) 187.02 132.33 T
(avelength Calibrations) 198.87 132.33 T
8 F
( 98) 508.1 132.33 T
FMENDPAGE
%%EndPage: "81" 81
%%Page: "82" 82
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(82) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
72 671.02 558 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 672.52 558 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 672.52 198 672.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(8.1) 181.32 678.02 T
(The Effect of COST) 207 678.02 T
(AR on the GHRS) 315.46 678.02 T
0 10 Q
-0.21 (Prior to the Servicing Mission, it was believed that the COST) 207 654.35 P
-0.21 (AR mirrors would have lit-) 449.95 654.35 P
1.02 (tle ef) 207 642.35 P
1.02 (fect on the throughput of the GHRS. It was known that the magnesium \337uoride) 228.11 642.35 P
1.16 (coatings would severely attenuate light below 1) 207 630.35 P
1.16 (150 \201, but at longer wavelengths we) 404.12 630.35 P
0.62 (anticipated that the light lost from the extra two re\337ections would be compensated for) 207 618.35 P
(by the improved throughput of the restored Point Spread Function.) 207 606.35 T
0.5 (The actual situation is more complex, as shown below) 207 586.35 P
0.5 (. What is plotted is a mean rela-) 427.29 586.35 P
-0.11 (tion that was \336tted to observations of the same star that were made both before and after) 207 574.35 P
0.27 (the Servicing Mission. The most prominent feature is the dip at 2000 \201. The high ratio) 207 562.35 P
0.34 (at longer wavelengths is just due to the improved PSF) 207 550.35 P
0.34 (, but the peak near 1300 \201 is not) 425.05 550.35 P
(understood.) 207 538.35 T
2 F
0.44 (Figure 8-1.) 144 187.35 P
4 F
0.44 (The observed ratio of counts for) 201.44 187.35 P
13 F
0.39 (m) 348.01 187.35 P
4 F
0.44 ( Col, made before the Servic-) 353.77 187.35 P
(ing Mission \050in Cycle 2\051 and after the deployment of the COST) 144 175.35 T
(AR mirrors.) 418.37 175.35 T
72 87.98 558 686.02 C
126 203.02 558 520.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 87.98 558 686.02 C
0 0 612 792 C
270 35 25 549 744 287.83 402.63 192.08 164.68 FMBEGINEPSF
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%%Page: 1 1
3 lw lt0 2050 500 r 2050 3100 d 2050 557 r 2018 557 d 2050 670 r
2018 670 d 2050 783 r 2018 783 d 2050 896 r 2018 896 d 2050 1009 r
1986 1009 d 2050 1122 r 2018 1122 d 2050 1235 r 2018 1235 d 2050 1348 r
2018 1348 d 2050 1461 r 2018 1461 d 2050 1574 r 1986 1574 d 2050 1687 r
2018 1687 d 2050 1800 r 2018 1800 d 2050 1913 r 2018 1913 d 2050 2026 r
2018 2026 d 2050 2139 r 1986 2139 d 2050 2252 r 2018 2252 d 2050 2365 r
2018 2365 d 2050 2478 r 2018 2478 d 2050 2591 r 2018 2591 d 2050 2704 r
1986 2704 d 2050 2817 r 2018 2817 d 2050 2930 r 2018 2930 d 2050 3043 r
2018 3043 d 2098 941 r 2096 945 d 2090 951 d 2132 951 d 2090 999 r
2090 979 d 2108 977 d 2106 979 d 2104 985 d 2104 991 d 2106 997 d
2110 1001 d 2116 1003 d 2120 1003 d 2126 1001 d 2130 997 d 2132 991 d
2132 985 d 2130 979 d 2128 977 d 2124 975 d 2090 1027 r 2092 1021 d
2098 1017 d 2108 1015 d 2114 1015 d 2124 1017 d 2130 1021 d 2132 1027 d
2132 1031 d 2130 1037 d 2124 1041 d 2114 1043 d 2108 1043 d 2098 1041 d
2092 1037 d 2090 1031 d 2090 1027 d 2090 1067 r 2092 1061 d 2098 1057 d
2108 1055 d 2114 1055 d 2124 1057 d 2130 1061 d 2132 1067 d 2132 1071 d
2130 1077 d 2124 1081 d 2114 1083 d 2108 1083 d 2098 1081 d 2092 1077 d
2090 1071 d 2090 1067 d 2100 1502 r 2098 1502 d 2094 1504 d 2092 1506 d
2090 1510 d 2090 1518 d 2092 1522 d 2094 1524 d 2098 1526 d 2102 1526 d
2106 1524 d 2112 1520 d 2132 1500 d 2132 1528 d 2090 1552 r 2092 1546 d
2098 1542 d 2108 1540 d 2114 1540 d 2124 1542 d 2130 1546 d 2132 1552 d
2132 1556 d 2130 1562 d 2124 1566 d 2114 1568 d 2108 1568 d 2098 1566 d
2092 1562 d 2090 1556 d 2090 1552 d 2090 1592 r 2092 1586 d 2098 1582 d
2108 1580 d 2114 1580 d 2124 1582 d 2130 1586 d 2132 1592 d 2132 1596 d
2130 1602 d 2124 1606 d 2114 1608 d 2108 1608 d 2098 1606 d 2092 1602 d
2090 1596 d 2090 1592 d 2090 1632 r 2092 1626 d 2098 1622 d 2108 1620 d
2114 1620 d 2124 1622 d 2130 1626 d 2132 1632 d 2132 1636 d 2130 1642 d
2124 1646 d 2114 1648 d 2108 1648 d 2098 1646 d 2092 1642 d 2090 1636 d
2090 1632 d 2100 2067 r 2098 2067 d 2094 2069 d 2092 2071 d 2090 2075 d
2090 2083 d 2092 2087 d 2094 2089 d 2098 2091 d 2102 2091 d 2106 2089 d
2112 2085 d 2132 2065 d 2132 2093 d 2090 2129 r 2090 2109 d 2108 2107 d
2106 2109 d 2104 2115 d 2104 2121 d 2106 2127 d 2110 2131 d 2116 2133 d
2120 2133 d 2126 2131 d 2130 2127 d 2132 2121 d 2132 2115 d 2130 2109 d
2128 2107 d 2124 2105 d 2090 2157 r 2092 2151 d 2098 2147 d 2108 2145 d
2114 2145 d 2124 2147 d 2130 2151 d 2132 2157 d 2132 2161 d 2130 2167 d
2124 2171 d 2114 2173 d 2108 2173 d 2098 2171 d 2092 2167 d 2090 2161 d
2090 2157 d 2090 2197 r 2092 2191 d 2098 2187 d 2108 2185 d 2114 2185 d
2124 2187 d 2130 2191 d 2132 2197 d 2132 2201 d 2130 2207 d 2124 2211 d
2114 2213 d 2108 2213 d 2098 2211 d 2092 2207 d 2090 2201 d 2090 2197 d
2090 2634 r 2090 2656 d 2106 2644 d 2106 2650 d 2108 2654 d 2110 2656 d
2116 2658 d 2120 2658 d 2126 2656 d 2130 2652 d 2132 2646 d 2132 2640 d
2130 2634 d 2128 2632 d 2124 2630 d 2090 2682 r 2092 2676 d 2098 2672 d
2108 2670 d 2114 2670 d 2124 2672 d 2130 2676 d 2132 2682 d 2132 2686 d
2130 2692 d 2124 2696 d 2114 2698 d 2108 2698 d 2098 2696 d 2092 2692 d
2090 2686 d 2090 2682 d 2090 2722 r 2092 2716 d 2098 2712 d 2108 2710 d
2114 2710 d 2124 2712 d 2130 2716 d 2132 2722 d 2132 2726 d 2130 2732 d
2124 2736 d 2114 2738 d 2108 2738 d 2098 2736 d 2092 2732 d 2090 2726 d
2090 2722 d 2090 2762 r 2092 2756 d 2098 2752 d 2108 2750 d 2114 2750 d
2124 2752 d 2130 2756 d 2132 2762 d 2132 2766 d 2130 2772 d 2124 2776 d
2114 2778 d 2108 2778 d 2098 2776 d 2092 2772 d 2090 2766 d 2090 2762 d
150 500 r 150 3100 d 150 557 r 182 557 d 150 670 r 182 670 d
150 783 r 182 783 d 150 896 r 182 896 d 150 1009 r 214 1009 d
150 1122 r 182 1122 d 150 1235 r 182 1235 d 150 1348 r 182 1348 d
150 1461 r 182 1461 d 150 1574 r 214 1574 d 150 1687 r 182 1687 d
150 1800 r 182 1800 d 150 1913 r 182 1913 d 150 2026 r 182 2026 d
150 2139 r 214 2139 d 150 2252 r 182 2252 d 150 2365 r 182 2365 d
150 2478 r 182 2478 d 150 2591 r 182 2591 d 150 2704 r 214 2704 d
150 2817 r 182 2817 d 150 2930 r 182 2930 d 150 3043 r 182 3043 d
2050 500 r 150 500 d 2050 500 r 2050 564 d 1898 500 r 1898 532 d
1746 500 r 1746 532 d 1594 500 r 1594 532 d 1442 500 r 1442 532 d
1290 500 r 1290 564 d 1138 500 r 1138 532 d 986 500 r 986 532 d
834 500 r 834 532 d 682 500 r 682 532 d 530 500 r 530 564 d
378 500 r 378 532 d 226 500 r 226 532 d 2026 386 r 2028 380 d
2034 376 d 2044 374 d 2050 374 d 2060 376 d 2066 380 d 2068 386 d
2068 390 d 2066 396 d 2060 400 d 2050 402 d 2044 402 d 2034 400 d
2028 396 d 2026 390 d 2026 386 d 2064 418 r 2066 416 d 2068 418 d
2066 420 d 2064 418 d 2026 446 r 2028 440 d 2034 436 d 2044 434 d
2050 434 d 2060 436 d 2066 440 d 2068 446 d 2068 450 d 2066 456 d
2060 460 d 2050 462 d 2044 462 d 2034 460 d 2028 456 d 2026 450 d
2026 446 d 1266 386 r 1268 380 d 1274 376 d 1284 374 d 1290 374 d
1300 376 d 1306 380 d 1308 386 d 1308 390 d 1306 396 d 1300 400 d
1290 402 d 1284 402 d 1274 400 d 1268 396 d 1266 390 d 1266 386 d
1304 418 r 1306 416 d 1308 418 d 1306 420 d 1304 418 d 1266 458 r
1266 438 d 1284 436 d 1282 438 d 1280 444 d 1280 450 d 1282 456 d
1286 460 d 1292 462 d 1296 462 d 1302 460 d 1306 456 d 1308 450 d
1308 444 d 1306 438 d 1304 436 d 1300 434 d 514 380 r 512 384 d
506 390 d 548 390 d 544 418 r 546 416 d 548 418 d 546 420 d
544 418 d 506 446 r 508 440 d 514 436 d 524 434 d 530 434 d
540 436 d 546 440 d 548 446 d 548 450 d 546 456 d 540 460 d
530 462 d 524 462 d 514 460 d 508 456 d 506 450 d 506 446 d
2050 3100 r 150 3100 d 2050 3100 r 2050 3036 d 1898 3100 r 1898 3068 d
1746 3100 r 1746 3068 d 1594 3100 r 1594 3068 d 1442 3100 r 1442 3068 d
1290 3100 r 1290 3036 d 1138 3100 r 1138 3068 d 986 3100 r 986 3068 d
834 3100 r 834 3068 d 682 3100 r 682 3068 d 530 3100 r 530 3036 d
378 3100 r 378 3068 d 226 3100 r 226 3068 d 2227 1260 r 2269 1272 d
2227 1284 r 2269 1272 d 2227 1284 r 2269 1296 d 2227 1308 r 2269 1296 d
2227 1362 r 2269 1362 d 2236 1362 r 2230 1356 d 2227 1350 d 2227 1341 d
2230 1335 d 2236 1329 d 2245 1326 d 2251 1326 d 2260 1329 d 2266 1335 d
2269 1341 d 2269 1350 d 2266 1356 d 2260 1362 d 2227 1377 r 2269 1395 d
2227 1413 r 2269 1395 d 2245 1428 r 2245 1464 d 2239 1464 d 2233 1461 d
2230 1458 d 2227 1452 d 2227 1443 d 2230 1437 d 2236 1431 d 2245 1428 d
2251 1428 d 2260 1431 d 2266 1437 d 2269 1443 d 2269 1452 d 2266 1458 d
2260 1464 d 2206 1485 r 2269 1485 d 2245 1506 r 2245 1542 d 2239 1542 d
2233 1539 d 2230 1536 d 2227 1530 d 2227 1521 d 2230 1515 d 2236 1509 d
2245 1506 d 2251 1506 d 2260 1509 d 2266 1515 d 2269 1521 d 2269 1530 d
2266 1536 d 2260 1542 d 2227 1563 r 2269 1563 d 2239 1563 r 2230 1572 d
2227 1578 d 2227 1587 d 2230 1593 d 2239 1596 d 2269 1596 d 2227 1650 r
2275 1650 d 2284 1647 d 2287 1644 d 2290 1638 d 2290 1629 d 2287 1623 d
2236 1650 r 2230 1644 d 2227 1638 d 2227 1629 d 2230 1623 d 2236 1617 d
2245 1614 d 2251 1614 d 2260 1617 d 2266 1623 d 2269 1629 d 2269 1638 d
2266 1644 d 2260 1650 d 2206 1674 r 2257 1674 d 2266 1677 d 2269 1683 d
2269 1689 d 2227 1665 r 2227 1686 d 2206 1701 r 2269 1701 d 2239 1701 r
2230 1710 d 2227 1716 d 2227 1725 d 2230 1731 d 2239 1734 d 2269 1734 d
2194 1824 r 2200 1818 d 2209 1812 d 2221 1806 d 2236 1803 d 2248 1803 d
2263 1806 d 2275 1812 d 2284 1818 d 2290 1824 d 2206 1860 r 2269 1836 d
2206 1860 r 2269 1884 d 2248 1845 r 2248 1875 d 2227 1899 r 2269 1899 d
2239 1899 r 2230 1908 d 2227 1914 d 2227 1923 d 2230 1929 d 2239 1932 d
2269 1932 d 2227 1986 r 2275 1986 d 2284 1983 d 2287 1980 d 2290 1974 d
2290 1965 d 2287 1959 d 2236 1986 r 2230 1980 d 2227 1974 d 2227 1965 d
2230 1959 d 2236 1953 d 2245 1950 d 2251 1950 d 2260 1953 d 2266 1959 d
2269 1965 d 2269 1974 d 2266 1980 d 2260 1986 d 2236 2037 r 2230 2034 d
2227 2025 d 2227 2016 d 2230 2007 d 2236 2004 d 2242 2007 d 2245 2013 d
2248 2028 d 2251 2034 d 2257 2037 d 2260 2037 d 2266 2034 d 2269 2025 d
2269 2016 d 2266 2007 d 2260 2004 d 2206 2058 r 2257 2058 d 2266 2061 d
2269 2067 d 2269 2073 d 2227 2049 r 2227 2070 d 2227 2085 r 2269 2085 d
2245 2085 r 2236 2088 d 2230 2094 d 2227 2100 d 2227 2109 d 2227 2139 r
2230 2133 d 2236 2127 d 2245 2124 d 2251 2124 d 2260 2127 d 2266 2133 d
2269 2139 d 2269 2148 d 2266 2154 d 2260 2160 d 2251 2163 d 2245 2163 d
2236 2160 d 2230 2154 d 2227 2148 d 2227 2139 d 2227 2181 r 2269 2181 d
2239 2181 r 2230 2190 d 2227 2196 d 2227 2205 d 2230 2211 d 2239 2214 d
2269 2214 d 2239 2214 r 2230 2223 d 2227 2229 d 2227 2238 d 2230 2244 d
2239 2247 d 2269 2247 d 2236 2301 r 2230 2298 d 2227 2289 d 2227 2280 d
2230 2271 d 2236 2268 d 2242 2271 d 2245 2277 d 2248 2292 d 2251 2298 d
2257 2301 d 2260 2301 d 2266 2298 d 2269 2289 d 2269 2280 d 2266 2271 d
2260 2268 d 2194 2316 r 2200 2322 d 2209 2328 d 2221 2334 d 2236 2337 d
2248 2337 d 2263 2334 d 2275 2328 d 2284 2322 d 2290 2316 d 1496 125 r
1496 167 d 1496 143 r 1493 134 d 1487 128 d 1481 125 d 1472 125 d
1421 125 r 1421 167 d 1421 134 r 1427 128 d 1433 125 d 1442 125 d
1448 128 d 1454 134 d 1457 143 d 1457 149 d 1454 158 d 1448 164 d
1442 167 d 1433 167 d 1427 164 d 1421 158 d 1397 104 r 1397 155 d
1394 164 d 1388 167 d 1382 167 d 1406 125 r 1385 125 d 1373 104 r
1370 107 d 1367 104 d 1370 101 d 1373 104 d 1370 125 r 1370 167 d
1334 125 r 1340 128 d 1346 134 d 1349 143 d 1349 149 d 1346 158 d
1340 164 d 1334 167 d 1325 167 d 1319 164 d 1313 158 d 1310 149 d
1310 143 d 1313 134 d 1319 128 d 1325 125 d 1334 125 d 1232 125 r
1238 128 d 1244 134 d 1247 143 d 1247 149 d 1244 158 d 1238 164 d
1232 167 d 1223 167 d 1217 164 d 1211 158 d 1208 149 d 1208 143 d
1211 134 d 1217 128 d 1223 125 d 1232 125 d 1172 104 r 1178 104 d
1184 107 d 1187 116 d 1187 167 d 1196 125 r 1175 125 d 1082 134 r
1085 128 d 1094 125 d 1103 125 d 1112 128 d 1115 134 d 1112 140 d
1106 143 d 1091 146 d 1085 149 d 1082 155 d 1082 158 d 1085 164 d
1094 167 d 1103 167 d 1112 164 d 1115 158 d 1067 143 r 1031 143 d
1031 137 d 1034 131 d 1037 128 d 1043 125 d 1052 125 d 1058 128 d
1064 134 d 1067 143 d 1067 149 d 1064 158 d 1058 164 d 1052 167 d
1043 167 d 1037 164 d 1031 158 d 1010 125 r 1010 167 d 1010 137 r
1001 128 d 995 125 d 986 125 d 980 128 d 977 137 d 977 167 d
926 134 r 929 128 d 938 125 d 947 125 d 956 128 d 959 134 d
956 140 d 950 143 d 935 146 d 929 149 d 926 155 d 926 158 d
929 164 d 938 167 d 947 167 d 956 164 d 959 158 d 911 104 r
908 107 d 905 104 d 908 101 d 911 104 d 908 125 r 908 167 d
881 104 r 881 155 d 878 164 d 872 167 d 866 167 d 890 125 r
869 125 d 857 104 r 854 107 d 851 104 d 854 101 d 857 104 d
854 125 r 854 167 d 836 125 r 818 167 d 800 125 r 818 167 d
785 104 r 782 107 d 779 104 d 782 101 d 785 104 d 782 125 r
782 167 d 755 104 r 755 155 d 752 164 d 746 167 d 740 167 d
764 125 r 743 125 d 734 125 r 716 167 d 698 125 r 716 167 d
722 179 d 728 185 d 734 188 d 737 188 d 2037 557 r 1072 613 d
538 670 d 315 726 d 284 783 d 327 839 d 389 896 d 457 952 d
521 1009 d 569 1065 d 598 1122 d 614 1178 d 627 1235 d 647 1291 d
682 1348 d 725 1404 d 766 1461 d 791 1517 d 789 1574 d 758 1630 d
708 1687 d 650 1743 d 596 1800 d 554 1857 d 523 1913 d 500 1970 d
482 2026 d 465 2083 d 448 2139 d 431 2196 d 414 2252 d 396 2309 d
378 2365 d 359 2422 d 341 2478 d 323 2535 d 306 2591 d 290 2648 d
273 2704 d 255 2761 d 236 2817 d 219 2874 d 211 2930 d 223 2987 d
263 3043 d
e
%%Trailer
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%%EndDocument
FMENDEPSF
FMENDPAGE
%%EndPage: "82" 82
%%Page: "83" 83
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (83) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Reference T) 207 736.18 T
(ables for Instrument Performance) 257.85 736.18 T
54 671.02 540 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 672.52 540 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 672.52 180 672.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(8.2) 163.32 678.02 T
(Properties of the First-Order Gratings) 189 678.02 T
2 10 Q
(8.2.1) 157.76 644.35 T
(Useful W) 189 644.35 T
(avelength Ranges) 231.41 644.35 T
0 F
0.32 (The following table summarizes the useful wavelength range for each of the \336rst-order) 189 624.35 P
0.28 (gratings of GHRS. More precise sensitivity values are enumerated below) 189 612.35 P
0.28 (. Note that lit-) 483.05 612.35 P
-0.24 (tle or no \337ux below 1) 189 600.35 P
-0.24 (150 \201 is re\337ected by the COST) 273.24 600.35 P
-0.24 (AR mirrors because of their magne-) 397.09 600.35 P
(sium \337uoride coatings.) 189 588.35 T
1.64 (The last three gratings are used with detector D2, which admits some second-order) 189 429.35 P
0.08 (light, hence the comments. For example, L) 189 417.35 P
0.08 (yman-) 360.3 417.35 P
13 F
0.08 (a) 385.85 417.35 P
0 F
0.08 ( light \0501216 \201\051 can appear at 2432 \201) 392.16 417.35 P
1.58 (in second order) 189 405.35 P
1.58 (. Except for this possibility of geocoronal contamination, many cool) 253.27 405.35 P
0.51 (stars have very little short-wavelength \337ux, so that the best resolution can be achieved) 189 393.35 P
1.48 (without undue extraneous light by observing in \336rst order near the high-wavelength) 189 381.35 P
(limit.) 189 369.35 T
1.08 (Note that the G270M grating has an order) 189 349.35 P
1.08 (-sorting \336lter which eliminates light below) 363.8 349.35 P
(about 1650 \201 so that no cross-order contamination occurs below 3300 \201.) 189 337.35 T
2 F
(8.2.2) 157.76 307.35 T
(Resolving Power) 189 307.35 T
0 F
1.25 (The following \336gures illustrate the resolving power as measured for each of GHRS\325) 189 287.35 P
0.38 (gratings. In this case the resolving power was computed as) 189 275.35 P
14 F
0.33 (R) 430.21 275.35 P
0 F
0.38 ( =) 436.21 275.35 P
13 F
0.38 ( l) 444.73 275.35 P
0 F
0.38 (/) 453.09 275.35 P
13 F
0.38 (Dl) 455.87 275.35 P
0 F
0.38 (, where) 467.48 275.35 P
0.38 ( is the) 515.36 275.35 P
1.05 (measured full-width-at-half-maximum \050FWHM\051 of lines from an exposure of a spec-) 189 263.35 P
-0.17 (trum calibration lamp. T) 189 251.35 P
-0.17 (ests have shown that the measured FWHM does not change sig-) 285.58 251.35 P
0.73 (ni\336cantly with wavelength \050for the \336rst-order gratings\051 or with) 189 239.35 P
3 F
0.73 (m) 448.56 239.35 P
13 F
0.73 (l) 455.78 239.35 P
0 F
0.73 (, the product of the) 461.27 239.35 P
0.45 (wavelength and order number \050for the echelle gratings\051. The nominal design speci\336ca-) 189 227.35 P
-0.15 (tion for the GHRS was) 189 215.35 P
14 F
-0.13 (R) 282.42 215.35 P
0 F
-0.15 ( = 20,000 for the \336rst-order gratings, but in fact one can exceed) 288.42 215.35 P
0.61 (a resolving power of 25,000 at virtually all wavelengths. Similarly) 189 203.35 P
0.61 (, the low-dispersion) 459.62 203.35 P
0.42 (grating G140L has R in excess of 2,000 over most of its useful wavelength range. The) 189 191.35 P
1.45 (true resolving powers for the echelle gratings are closer to 80,000 than the nominal) 189 179.35 P
(100,000.) 189 167.35 T
0.27 (By providing a sharper image of a point source, COST) 189 147.35 P
0.27 (AR restores the resolving power) 409.5 147.35 P
0.36 (achieved with the LSA to within about 20% of that possible with the SSA. There is no) 189 135.35 P
(ef) 189 123.35 T
(fective change for the SSA, however) 196.59 123.35 T
(.) 343.22 123.35 T
54 566.02 540 579.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 573.02 540 573.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 573.02 180 573.02 2 L
0 Z
N
0 0 612 792 C
2 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 560.02 T
(ABLE 8-1) 58.83 560.02 T
4 F
(Useful wavelength ranges for \336rst-order gratings.) 189 549.02 T
2 8 Q
(Grating) 115.12 525.68 T
(Useful Range \050\201\051) 172.05 525.68 T
(\201 per diode) 266.19 525.68 T
(Bandpass \050\201\051) 340.06 525.68 T
(Comment) 410.4 525.68 T
0 9 Q
(G140L) 115.12 511.02 T
(1) 185.25 511.02 T
(100 \320 1900) 189.41 511.02 T
(0.572 \320 0.573) 263.45 511.02 T
(286 \320 287) 347.84 511.02 T
(G140M) 115.12 496.02 T
(1) 185.25 496.02 T
(100 \320 1900) 189.41 496.02 T
(0.056 \320 0.052) 263.45 496.02 T
(28 \320 26) 352.34 496.02 T
(G160M) 115.12 481.02 T
(1) 185.25 481.02 T
(150 \320 2300) 189.41 481.02 T
(0.072 \320 0.066) 263.45 481.02 T
(36 \320 33) 352.34 481.02 T
(2nd order overlap above 2300 \201) 410.4 481.02 T
(G200M) 115.12 466.02 T
(1600 \320 2300) 185.08 466.02 T
(0.081 \320 0.075) 263.45 466.02 T
(41 \320 38) 352.34 466.02 T
(2nd order overlap above 2300 \201) 410.4 466.02 T
(G270M) 115.12 451.02 T
(2000 \320 3300) 185.08 451.02 T
(0.096 \320 0.087) 263.45 451.02 T
(48 \320 44) 352.34 451.02 T
(2nd order overlap above 3300 \201) 410.4 451.02 T
109.12 537.89 109.12 446.14 2 L
V
0.25 H
0 Z
N
166.05 538.14 166.05 445.89 2 L
V
N
249.11 538.14 249.11 445.89 2 L
V
N
327.29 538.14 327.29 445.89 2 L
V
N
404.4 538.14 404.4 445.89 2 L
V
N
540 537.89 540 446.14 2 L
V
N
109 538.02 540.12 538.02 2 L
V
N
109 521.02 540.12 521.02 2 L
V
0.5 H
N
109 506.02 540.12 506.02 2 L
V
0.25 H
N
109 491.02 540.12 491.02 2 L
V
N
109 476.02 540.12 476.02 2 L
V
N
109 461.02 540.12 461.02 2 L
V
N
109 446.02 540.12 446.02 2 L
V
N
500.16 270.85 515.36 283.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
13 10 Q
0 X
0 0 0 1 0 0 0 K
(D) 501.16 275.35 T
(l) 507.87 275.35 T
0 0 612 792 C
FMENDPAGE
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7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(84) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
1.27 (Figure 8-2.) 144 414.32 P
4 F
1.27 (Spectrum resolving power as a function of wavelength for the) 203.93 414.32 P
0.15 (GHRS medium-resolution \050holographic\051 gratings. From left to right the curves) 144 402.32 P
(are for G140M, G160M, G200M, and G270M, respectively) 144 390.32 T
(.) 400.59 390.32 T
2 F
(Figure 8-3.) 144 108.32 T
4 F
(Resolving power for grating G140L.) 200.13 108.32 T
72 85.97 558 684 C
72 429.98 558 677 C
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819 1589 d 800 1617 r 819 1617 d 800 1644 r 838 1644 d 800 1672 r
819 1672 d 800 1700 r 819 1700 d 692 1238 r 695 1239 d 698 1242 d
698 1217 d 727 1242 r 715 1242 d 714 1232 d 715 1233 d 719 1234 d
722 1234 d 726 1233 d 728 1230 d 729 1227 d 729 1224 d 728 1221 d
726 1218 d 722 1217 d 719 1217 d 715 1218 d 714 1220 d 713 1222 d
744 1242 r 740 1241 d 738 1238 d 737 1232 d 737 1228 d 738 1222 d
740 1218 d 744 1217 d 746 1217 d 750 1218 d 752 1222 d 753 1228 d
753 1232 d 752 1238 d 750 1241 d 746 1242 d 744 1242 d 768 1242 r
764 1241 d 762 1238 d 761 1232 d 761 1228 d 762 1222 d 764 1218 d
768 1217 d 770 1217 d 774 1218 d 776 1222 d 777 1228 d 777 1232 d
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691 1379 d 692 1380 d 695 1381 d 699 1381 d 702 1380 d 703 1379 d
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744 1356 d 746 1356 d 750 1357 d 752 1361 d 753 1367 d 753 1371 d
752 1377 d 750 1380 d 746 1381 d 744 1381 d 768 1381 r 764 1380 d
762 1377 d 761 1371 d 761 1367 d 762 1361 d 764 1357 d 768 1356 d
770 1356 d 774 1357 d 776 1361 d 777 1367 d 777 1371 d 776 1377 d
774 1380 d 770 1381 d 768 1381 d 690 1514 r 690 1516 d 691 1518 d
692 1519 d 695 1520 d 699 1520 d 702 1519 d 703 1518 d 704 1516 d
704 1513 d 703 1511 d 701 1507 d 689 1495 d 705 1495 d 727 1520 r
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728 1508 d 729 1505 d 729 1502 d 728 1499 d 726 1496 d 722 1495 d
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738 1516 d 737 1510 d 737 1506 d 738 1500 d 740 1496 d 744 1495 d
746 1495 d 750 1496 d 752 1500 d 753 1506 d 753 1510 d 752 1516 d
750 1519 d 746 1520 d 744 1520 d 768 1520 r 764 1519 d 762 1516 d
761 1510 d 761 1506 d 762 1500 d 764 1496 d 768 1495 d 770 1495 d
774 1496 d 776 1500 d 777 1506 d 777 1510 d 776 1516 d 774 1519 d
770 1520 d 768 1520 d 691 1658 r 704 1658 d 697 1649 d 701 1649 d
703 1648 d 704 1646 d 705 1643 d 705 1640 d 704 1637 d 702 1634 d
698 1633 d 695 1633 d 691 1634 d 690 1636 d 689 1638 d 720 1658 r
716 1657 d 714 1654 d 713 1648 d 713 1644 d 714 1638 d 716 1634 d
720 1633 d 722 1633 d 726 1634 d 728 1638 d 729 1644 d 729 1648 d
728 1654 d 726 1657 d 722 1658 d 720 1658 d 744 1658 r 740 1657 d
738 1654 d 737 1648 d 737 1644 d 738 1638 d 740 1634 d 744 1633 d
746 1633 d 750 1634 d 752 1638 d 753 1644 d 753 1648 d 752 1654 d
750 1657 d 746 1658 d 744 1658 d 768 1658 r 764 1657 d 762 1654 d
761 1648 d 761 1644 d 762 1638 d 764 1634 d 768 1633 d 770 1633 d
774 1634 d 776 1638 d 777 1644 d 777 1648 d 776 1654 d 774 1657 d
770 1658 d 768 1658 d 2000 1200 r 2000 1700 d 2000 1200 r 1981 1200 d
2000 1228 r 1962 1228 d 2000 1256 r 1981 1256 d 2000 1283 r 1981 1283 d
2000 1311 r 1981 1311 d 2000 1339 r 1981 1339 d 2000 1367 r 1962 1367 d
2000 1394 r 1981 1394 d 2000 1422 r 1981 1422 d 2000 1450 r 1981 1450 d
2000 1478 r 1981 1478 d 2000 1506 r 1962 1506 d 2000 1533 r 1981 1533 d
2000 1561 r 1981 1561 d 2000 1589 r 1981 1589 d 2000 1617 r 1981 1617 d
2000 1644 r 1962 1644 d 2000 1672 r 1981 1672 d 2000 1700 r 1981 1700 d
1109 1117 r 1117 1084 d 1125 1117 r 1117 1084 d 1125 1117 r 1133 1084 d
1141 1117 r 1133 1084 d 1168 1106 r 1168 1084 d 1168 1101 r 1165 1104 d
1162 1106 d 1157 1106 d 1154 1104 d 1151 1101 d 1149 1096 d 1149 1093 d
1151 1088 d 1154 1085 d 1157 1084 d 1162 1084 d 1165 1085 d 1168 1088 d
1176 1106 r 1186 1084 d 1196 1106 r 1186 1084 d 1204 1096 r 1223 1096 d
1223 1100 d 1221 1103 d 1220 1104 d 1216 1106 d 1212 1106 d 1208 1104 d
1205 1101 d 1204 1096 d 1204 1093 d 1205 1088 d 1208 1085 d 1212 1084 d
1216 1084 d 1220 1085 d 1223 1088 d 1234 1117 r 1234 1084 d 1245 1096 r
1264 1096 d 1264 1100 d 1263 1103 d 1261 1104 d 1258 1106 d 1253 1106 d
1250 1104 d 1247 1101 d 1245 1096 d 1245 1093 d 1247 1088 d 1250 1085 d
1253 1084 d 1258 1084 d 1261 1085 d 1264 1088 d 1276 1106 r 1276 1084 d
1276 1100 r 1280 1104 d 1284 1106 d 1288 1106 d 1292 1104 d 1293 1100 d
1293 1084 d 1322 1106 r 1322 1080 d 1320 1076 d 1319 1074 d 1316 1072 d
1311 1072 d 1308 1074 d 1322 1101 r 1319 1104 d 1316 1106 d 1311 1106 d
1308 1104 d 1304 1101 d 1303 1096 d 1303 1093 d 1304 1088 d 1308 1085 d
1311 1084 d 1316 1084 d 1319 1085 d 1322 1088 d 1335 1117 r 1335 1090 d
1336 1085 d 1340 1084 d 1343 1084 d 1330 1106 r 1341 1106 d 1349 1117 r
1349 1084 d 1349 1100 r 1354 1104 d 1357 1106 d 1362 1106 d 1365 1104 d
1367 1100 d 1367 1084 d 1415 1124 r 1412 1120 d 1408 1116 d 1405 1109 d
1404 1101 d 1404 1095 d 1405 1087 d 1408 1080 d 1412 1076 d 1415 1072 d
1434 1117 r 1421 1084 d 1434 1117 r 1447 1084 d 1426 1095 r 1442 1095 d
1455 1106 r 1455 1084 d 1455 1100 r 1460 1104 d 1463 1106 d 1468 1106 d
1471 1104 d 1472 1100 d 1472 1084 d 1501 1106 r 1501 1080 d 1500 1076 d
1498 1074 d 1495 1072 d 1490 1072 d 1487 1074 d 1501 1101 r 1498 1104 d
1495 1106 d 1490 1106 d 1487 1104 d 1484 1101 d 1482 1096 d 1482 1093 d
1484 1088 d 1487 1085 d 1490 1084 d 1495 1084 d 1498 1085 d 1501 1088 d
1528 1101 r 1527 1104 d 1522 1106 d 1517 1106 d 1512 1104 d 1511 1101 d
1512 1098 d 1516 1096 d 1524 1095 d 1527 1093 d 1528 1090 d 1528 1088 d
1527 1085 d 1522 1084 d 1517 1084 d 1512 1085 d 1511 1088 d 1540 1117 r
1540 1090 d 1541 1085 d 1544 1084 d 1548 1084 d 1535 1106 r 1546 1106 d
1554 1106 r 1554 1084 d 1554 1096 r 1556 1101 d 1559 1104 d 1562 1106 d
1567 1106 d 1583 1106 r 1580 1104 d 1576 1101 d 1575 1096 d 1575 1093 d
1576 1088 d 1580 1085 d 1583 1084 d 1588 1084 d 1591 1085 d 1594 1088 d
1596 1093 d 1596 1096 d 1594 1101 d 1591 1104 d 1588 1106 d 1583 1106 d
1605 1106 r 1605 1084 d 1605 1100 r 1610 1104 d 1613 1106 d 1618 1106 d
1621 1104 d 1623 1100 d 1623 1084 d 1623 1100 r 1628 1104 d 1631 1106 d
1636 1106 d 1639 1104 d 1640 1100 d 1640 1084 d 1669 1101 r 1668 1104 d
1663 1106 d 1658 1106 d 1653 1104 d 1652 1101 d 1653 1098 d 1656 1096 d
1664 1095 d 1668 1093 d 1669 1090 d 1669 1088 d 1668 1085 d 1663 1084 d
1658 1084 d 1653 1085 d 1652 1088 d 1677 1124 r 1680 1120 d 1684 1116 d
1687 1109 d 1688 1101 d 1688 1095 d 1687 1087 d 1684 1080 d 1680 1076 d
1677 1072 d 589 1254 r 622 1254 d 589 1254 r 589 1269 d 590 1274 d
592 1275 d 595 1277 d 598 1277 d 602 1275 d 603 1274 d 605 1269 d
605 1254 d 605 1266 r 622 1277 d 610 1288 r 610 1307 d 606 1307 d
603 1306 d 602 1304 d 600 1301 d 600 1296 d 602 1293 d 605 1290 d
610 1288 d 613 1288 d 618 1290 d 621 1293 d 622 1296 d 622 1301 d
621 1304 d 618 1307 d 605 1334 r 602 1333 d 600 1328 d 600 1323 d
602 1318 d 605 1317 d 608 1318 d 610 1322 d 611 1330 d 613 1333 d
616 1334 d 618 1334 d 621 1333 d 622 1328 d 622 1323 d 621 1318 d
618 1317 d 600 1350 r 602 1347 d 605 1344 d 610 1342 d 613 1342 d
618 1344 d 621 1347 d 622 1350 d 622 1355 d 621 1358 d 618 1362 d
613 1363 d 610 1363 d 605 1362 d 602 1358 d 600 1355 d 600 1350 d
589 1373 r 622 1373 d 600 1382 r 622 1392 d 600 1402 r 622 1392 d
589 1410 r 590 1411 d 589 1413 d 587 1411 d 589 1410 d 600 1411 r
622 1411 d 600 1424 r 622 1424 d 606 1424 r 602 1429 d 600 1432 d
600 1437 d 602 1440 d 606 1442 d 622 1442 d 600 1470 r 626 1470 d
630 1469 d 632 1467 d 634 1464 d 634 1459 d 632 1456 d 605 1470 r
602 1467 d 600 1464 d 600 1459 d 602 1456 d 605 1453 d 610 1451 d
613 1451 d 618 1453 d 621 1456 d 622 1459 d 622 1464 d 621 1467 d
618 1470 d 589 1507 r 622 1507 d 589 1507 r 589 1522 d 590 1526 d
592 1528 d 595 1530 d 600 1530 d 603 1528 d 605 1526 d 606 1522 d
606 1507 d 600 1549 r 602 1546 d 605 1542 d 610 1541 d 613 1541 d
618 1542 d 621 1546 d 622 1549 d 622 1554 d 621 1557 d 618 1560 d
613 1562 d 610 1562 d 605 1560 d 602 1557 d 600 1554 d 600 1549 d
600 1570 r 622 1576 d 600 1582 r 622 1576 d 600 1582 r 622 1589 d
600 1595 r 622 1589 d 610 1605 r 610 1624 d 606 1624 d 603 1622 d
602 1621 d 600 1618 d 600 1613 d 602 1610 d 605 1606 d 610 1605 d
613 1605 d 618 1606 d 621 1610 d 622 1613 d 622 1618 d 621 1621 d
618 1624 d 600 1635 r 622 1635 d 610 1635 r 605 1637 d 602 1640 d
600 1643 d 600 1648 d 867 1283 r 933 1303 d 1067 1346 d 1200 1388 d
1333 1431 d 1467 1475 d 1600 1518 d 1733 1562 d 1867 1604 d 1973 1632 d
e
%%Trailer
EndPSPlot

%%EndDocument
FMENDEPSF
72 85.97 558 684 C
0 0 612 792 C
FMENDPAGE
%%EndPage: "84" 84
%%Page: "85" 85
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (85) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Reference T) 207 736.18 T
(ables for Instrument Performance) 257.85 736.18 T
2 10 Q
(8.2.3) 157.76 679.35 T
(Sensitivity Functions for the First-Order Gratings) 189 679.35 T
0 F
0.27 (Below are given sensitivities for the \336rst-order gratings, using the Lar) 189 659.35 P
0.27 (ge Science Aper-) 470.61 659.35 P
0.43 (ture, in units of) 189 647.35 P
0.43 (. These) 510.69 647.35 P
0.83 (values will be updated with precise numbers determined in Cycle 4 but what is listed) 189 635.35 P
-0.11 (here has been adjusted for the known ef) 189 623.35 P
-0.11 (fects of the COST) 347.14 623.35 P
-0.11 (AR mirrors. SSA sensitivity is) 418.49 623.35 P
(about 50 to 70% of these values, with the lar) 189 611.35 T
(ger value applying at longer wavelengths.) 367.13 611.35 T
54 589.02 540 602.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 596.02 540 596.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 596.02 180 596.02 2 L
0 Z
N
0 0 612 792 C
2 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 583.02 T
(ABLE 8-2) 58.83 583.02 T
4 F
(Sensitivities for \336rst-order gratings.) 189 572.02 T
2 8 Q
(Grating) 277.48 548.68 T
(W) 200.4 531.68 T
(avelength \050\201\051) 207.66 531.68 T
(G140L) 277.48 531.68 T
(G140M) 331.48 531.68 T
(G160M) 385.48 531.68 T
(G200M) 439.48 531.68 T
(G270M) 493.48 531.68 T
0 9 Q
(1) 224.1 517.02 T
(100) 228.27 517.02 T
(0.20) 303.73 517.02 T
(0.006) 331.48 517.02 T
(1) 224.1 502.02 T
(150) 228.27 502.02 T
(20.9) 303.73 502.02 T
(0.75) 331.48 502.02 T
(0.64) 411.73 502.02 T
(1200) 223.94 487.02 T
(82.3) 303.73 487.02 T
(2.27) 331.48 487.02 T
(2.87) 411.73 487.02 T
(1250) 223.94 472.02 T
(152.) 303.73 472.02 T
(4.95) 331.48 472.02 T
(5.77) 411.73 472.02 T
(1300) 223.94 457.02 T
(168.) 303.73 457.02 T
(7.13) 331.48 457.02 T
(7.96) 411.73 457.02 T
(1350) 223.94 442.02 T
(166.) 303.73 442.02 T
(5.89) 331.48 442.02 T
(7.33) 411.73 442.02 T
(1400) 223.94 427.02 T
(146.) 303.73 427.02 T
(5.23) 331.48 427.02 T
(6.41) 411.73 427.02 T
(1450) 223.94 412.02 T
(1) 304.06 412.02 T
(14.) 308.23 412.02 T
(4.74) 331.48 412.02 T
(6.08) 411.73 412.02 T
(1500) 223.94 397.02 T
(89.3) 303.73 397.02 T
(3.41) 331.48 397.02 T
(4.34) 411.73 397.02 T
(1550) 223.94 382.02 T
(67.0) 303.73 382.02 T
(2.34) 331.48 382.02 T
(4.87) 411.73 382.02 T
(1600) 223.94 367.02 T
(43.9) 303.73 367.02 T
(1.36) 331.48 367.02 T
(5.17) 411.73 367.02 T
(4.48) 465.73 367.02 T
(1650) 223.94 352.02 T
(40.0) 303.73 352.02 T
(1.14) 331.48 352.02 T
(4.89) 411.73 352.02 T
(4.63) 465.73 352.02 T
(1700) 223.94 337.02 T
(32.0) 303.73 337.02 T
(0.88) 331.48 337.02 T
(4.74) 411.73 337.02 T
(5.56) 465.73 337.02 T
(1750) 223.94 322.02 T
(20.7) 303.73 322.02 T
(4.80) 411.73 322.02 T
(6.53) 465.73 322.02 T
(1800) 223.94 307.02 T
(10.8) 303.73 307.02 T
(4.78) 411.73 307.02 T
(7.42) 465.73 307.02 T
(1850) 223.94 292.02 T
(4.03) 303.73 292.02 T
(5.02) 411.73 292.02 T
(8.21) 465.73 292.02 T
(1900) 223.94 277.02 T
(1.09) 303.73 277.02 T
(5.20) 411.73 277.02 T
(8.61) 465.73 277.02 T
(1950) 223.94 262.02 T
(5.20) 411.73 262.02 T
(8.40) 465.73 262.02 T
(3.64) 519.73 262.02 T
(2000) 223.94 247.02 T
(5.00) 411.73 247.02 T
(8.23) 465.73 247.02 T
(4.72) 519.73 247.02 T
(2050) 223.94 232.02 T
(4.75) 411.73 232.02 T
(8.57) 465.73 232.02 T
(6.72) 519.73 232.02 T
(2100) 223.94 217.02 T
(4.68) 411.73 217.02 T
(8.92) 465.73 217.02 T
(9.25) 519.73 217.02 T
(2150) 223.94 202.02 T
(9.18) 465.73 202.02 T
(12.31) 515.23 202.02 T
(2200) 223.94 187.02 T
(9.35) 465.73 187.02 T
(16.19) 515.23 187.02 T
(2250) 223.94 172.02 T
(9.02) 465.73 172.02 T
(20.87) 515.23 172.02 T
(2300) 223.94 157.02 T
(8.57) 465.73 157.02 T
(23.82) 515.23 157.02 T
(2350) 223.94 142.02 T
(8.14) 465.73 142.02 T
(23.98) 515.23 142.02 T
(2400) 223.94 127.02 T
(8.70) 465.73 127.02 T
(26.29) 515.23 127.02 T
(2450) 223.94 112.02 T
(9.24) 465.73 112.02 T
(32.34) 515.23 112.02 T
(2500) 223.94 97.02 T
(9.76) 465.73 97.02 T
(41.63) 515.23 97.02 T
194.4 560.89 194.4 92.14 2 L
V
0.25 H
0 Z
N
271.48 561.14 271.48 91.89 2 L
V
N
325.48 544.27 325.48 91.89 2 L
V
N
379.48 544.27 379.48 91.89 2 L
V
N
433.48 544.27 433.48 91.89 2 L
V
N
487.48 544.27 487.48 91.89 2 L
V
N
541.48 560.89 541.48 92.14 2 L
V
N
194.27 561.02 541.6 561.02 2 L
V
N
194.27 544.02 271.6 544.02 2 L
V
N
271.35 544.02 541.6 544.02 2 L
V
0.5 H
N
194.27 527.02 541.6 527.02 2 L
V
N
194.27 512.02 541.6 512.02 2 L
V
0.25 H
N
194.27 497.02 541.6 497.02 2 L
V
N
194.27 482.02 541.6 482.02 2 L
V
N
194.27 467.02 541.6 467.02 2 L
V
N
194.27 452.02 541.6 452.02 2 L
V
N
194.27 437.02 541.6 437.02 2 L
V
N
194.27 422.02 541.6 422.02 2 L
V
N
194.27 407.02 541.6 407.02 2 L
V
N
194.27 392.02 541.6 392.02 2 L
V
N
194.27 377.02 541.6 377.02 2 L
V
N
194.27 362.02 541.6 362.02 2 L
V
N
194.27 347.02 541.6 347.02 2 L
V
N
194.27 332.02 541.6 332.02 2 L
V
N
194.27 317.02 541.6 317.02 2 L
V
N
194.27 302.02 541.6 302.02 2 L
V
N
194.27 287.02 541.6 287.02 2 L
V
N
194.27 272.02 541.6 272.02 2 L
V
N
194.27 257.02 541.6 257.02 2 L
V
N
194.27 242.02 541.6 242.02 2 L
V
N
194.27 227.02 541.6 227.02 2 L
V
N
194.27 212.02 541.6 212.02 2 L
V
N
194.27 197.02 541.6 197.02 2 L
V
N
194.27 182.02 541.6 182.02 2 L
V
N
194.27 167.02 541.6 167.02 2 L
V
N
194.27 152.02 541.6 152.02 2 L
V
N
194.27 137.02 541.6 137.02 2 L
V
N
194.27 122.02 541.6 122.02 2 L
V
N
194.27 107.02 541.6 107.02 2 L
V
N
194.27 92.02 541.6 92.02 2 L
V
N
254.33 644.18 510.69 658.31 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 259.88 647.35 T
(0) 264.88 647.35 T
0 7 Q
(1) 270.38 650.22 T
(1) 273.88 650.22 T
0 10 Q
(\050) 277.97 647.35 T
(c) 281.3 647.35 T
(o) 285.74 647.35 T
(u) 290.74 647.35 T
(n) 295.74 647.35 T
(t) 300.74 647.35 T
(s) 303.52 647.35 T
(s) 309.91 647.35 T
(e) 313.8 647.35 T
(c) 318.24 647.35 T
0 7 Q
(1) 326.95 650.22 T
(\320) 323.18 650.22 T
0 10 Q
(d) 333.54 647.35 T
(i) 338.54 647.35 T
(o) 341.32 647.35 T
(d) 346.32 647.35 T
(e) 351.32 647.35 T
0 7 Q
(1) 360.02 650.22 T
(\320) 356.26 650.22 T
0 10 Q
(\051) 364.11 647.35 T
(p) 369.94 647.35 T
(e) 374.94 647.35 T
(r) 379.38 647.35 T
(i) 385.21 647.35 T
(n) 387.99 647.35 T
(c) 392.99 647.35 T
(i) 397.43 647.35 T
(d) 400.21 647.35 T
(e) 405.21 647.35 T
(n) 409.65 647.35 T
(t) 414.65 647.35 T
(\050) 419.93 647.35 T
(e) 423.26 647.35 T
(r) 427.7 647.35 T
(g) 431.03 647.35 T
(c) 438.53 647.35 T
(m) 442.97 647.35 T
0 7 Q
(2) 455.02 650.22 T
(\320) 451.25 650.22 T
0 10 Q
(s) 461.61 647.35 T
(e) 465.5 647.35 T
(c) 469.94 647.35 T
0 7 Q
(1) 478.64 650.22 T
(\320) 474.88 650.22 T
0 10 Q
(\201) 485.23 647.35 T
0 7 Q
(1) 496.72 650.22 T
(\320) 492.95 650.22 T
0 10 Q
(\051) 500.81 647.35 T
0 0 612 792 C
FMENDPAGE
%%EndPage: "85" 85
%%Page: "86" 86
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(86) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
0 9 Q
(2550) 241.94 601.02 T
(49.06) 533.23 601.02 T
(2600) 241.94 586.02 T
(53.21) 533.23 586.02 T
(2650) 241.94 571.02 T
(54.37) 533.23 571.02 T
(2700) 241.94 556.02 T
(53.01) 533.23 556.02 T
(2750) 241.94 541.02 T
(50.28) 533.23 541.02 T
(2800) 241.94 526.02 T
(46.73) 533.23 526.02 T
(2850) 241.94 511.02 T
(42.44) 533.23 511.02 T
(2900) 241.94 496.02 T
(37.71) 533.23 496.02 T
(2950) 241.94 481.02 T
(32.19) 533.23 481.02 T
(3000) 241.94 466.02 T
(25.76) 533.23 466.02 T
(3050) 241.94 451.02 T
(19.46) 533.23 451.02 T
(3100) 241.94 436.02 T
(14.14) 533.23 436.02 T
(3150) 241.94 421.02 T
(10.07) 533.23 421.02 T
(3200) 241.94 406.02 T
(6.53) 537.73 406.02 T
(3250) 241.94 391.02 T
(3.83) 537.73 391.02 T
(3300) 241.94 376.02 T
(2.64) 537.73 376.02 T
72 673.02 558 686.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 680.02 558 680.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 680.02 198 680.02 2 L
0 Z
N
0 0 612 792 C
2 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 72 667.02 T
(ABLE 8-2) 76.83 667.02 T
4 F
( \050Continued\051) 207 667.02 T
(Sensitivities for \336rst-order gratings.) 207 656.02 T
2 8 Q
(Grating) 295.48 632.68 T
(W) 218.4 615.68 T
(avelength \050\201\051) 225.66 615.68 T
(G140L) 295.48 615.68 T
(G140M) 349.48 615.68 T
(G160M) 403.48 615.68 T
(G200M) 457.48 615.68 T
(G270M) 511.48 615.68 T
212.4 644.89 212.4 371.14 2 L
V
0.25 H
0 Z
N
289.48 645.14 289.48 370.89 2 L
V
N
343.48 628.27 343.48 370.89 2 L
V
N
397.48 628.27 397.48 370.89 2 L
V
N
451.48 628.27 451.48 370.89 2 L
V
N
505.48 628.27 505.48 370.89 2 L
V
N
559.48 644.89 559.48 371.14 2 L
V
N
212.27 645.02 559.6 645.02 2 L
V
N
212.27 628.02 289.6 628.02 2 L
V
N
289.35 628.02 559.6 628.02 2 L
V
0.5 H
N
212.27 611.02 559.6 611.02 2 L
V
N
212.27 596.02 559.6 596.02 2 L
V
0.25 H
N
212.27 581.02 559.6 581.02 2 L
V
N
212.27 566.02 559.6 566.02 2 L
V
N
212.27 551.02 559.6 551.02 2 L
V
N
212.27 536.02 559.6 536.02 2 L
V
N
212.27 521.02 559.6 521.02 2 L
V
N
212.27 506.02 559.6 506.02 2 L
V
N
212.27 491.02 559.6 491.02 2 L
V
N
212.27 476.02 559.6 476.02 2 L
V
N
212.27 461.02 559.6 461.02 2 L
V
N
212.27 446.02 559.6 446.02 2 L
V
N
212.27 431.02 559.6 431.02 2 L
V
N
212.27 416.02 559.6 416.02 2 L
V
N
212.27 401.02 559.6 401.02 2 L
V
N
212.27 386.02 559.6 386.02 2 L
V
N
212.27 371.02 559.6 371.02 2 L
V
N
FMENDPAGE
%%EndPage: "86" 86
%%Page: "87" 87
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (87) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Reference T) 207 736.18 T
(ables for Instrument Performance) 257.85 736.18 T
54 671.02 540 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 672.52 540 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 672.52 180 672.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(8.3) 163.32 678.02 T
(Properties of the Echelle Gratings) 189 678.02 T
2 10 Q
(8.3.1) 157.76 644.35 T
(W) 189 644.35 T
(avelength Coverage, Bandpass, and Sensitivity) 198.07 644.35 T
0 F
0.81 (The following tables summarize basic properties of the two echelle gratings. The dis-) 189 624.35 P
0.14 (persion in each order has not been listed but does not change if it is computed in veloc-) 189 612.35 P
0.17 (ity units. At the center of each order) 189 600.35 P
0.17 (, the dispersion is 3.0 km s) 334.22 600.35 P
0 8 Q
0.14 (-1) 441.93 604.35 P
0 10 Q
0.17 ( per diode, at the long-) 448.59 600.35 P
-0.04 (wavelength end of each order it is 2.9 km s) 189 588.35 P
0 8 Q
-0.03 (-1) 360.86 592.35 P
0 10 Q
-0.04 ( per diode, and at the short-wavelength end) 367.52 588.35 P
(of each order it is 3.1 km s) 189 576.35 T
0 8 Q
(-1) 295.65 580.35 T
0 10 Q
( per diode.) 302.31 576.35 T
135.06 208.02 540 215.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
-0.08 (a.) 135.06 202.02 P
3 F
-0.08 (\322d\323) 143.48 202.02 P
0 F
-0.08 ( coef) 157.99 202.02 P
-0.08 (\336cient of Cardelli, Ebbets, and Savage \0501993; see Section) 175.48 202.02 P
-0.08 (9.2 on page) 384.07 202.02 P
-0.08 (102\051. These apply only to) 427.9 202.02 P
(the SSA.) 171.06 192.02 T
-0.08 (b. Sensitivity function at blaze peak, in units of 10) 135.06 179.02 P
0 7.2 Q
-0.07 (1) 315.55 182.62 P
-0.07 (1) 318.88 182.62 P
0 9 Q
-0.08 ( \050counts diode) 322.48 179.02 P
0 7.2 Q
-0.07 (-1) 373.3 182.62 P
0 9 Q
-0.08 ( sec) 379.3 179.02 P
0 7.2 Q
-0.07 (-1) 392.96 182.62 P
0 9 Q
-0.08 (\051 per incident \050er) 398.96 179.02 P
-0.08 (g cm) 458.77 179.02 P
0 7.2 Q
-0.07 (-2) 476.44 182.62 P
0 9 Q
-0.08 ( sec) 482.43 179.02 P
0 7.2 Q
-0.07 (-1) 496.09 182.62 P
0 9 Q
-0.08 ( \201) 502.09 179.02 P
0 7.2 Q
-0.07 (-1) 510.76 182.62 P
0 9 Q
-0.08 (\051.) 516.75 179.02 P
54 554.02 540 567.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 561.02 540 561.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 561.02 180 561.02 2 L
0 Z
N
0 0 612 792 C
2 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 548.02 T
(ABLE 8-3) 58.83 548.02 T
4 F
(Properties of Grating Echelle-A) 189 537.02 T
2 8 Q
(Order) 150.99 504.68 T
(Central) 215.57 513.68 T
(W) 200.39 504.68 T
(avelength \050\201\051) 207.64 504.68 T
(Order) 295.11 513.68 T
(Coverage \050\201\051) 281.11 504.68 T
(Bandpass per) 360.55 513.68 T
(exposure \050\201\051) 362.55 504.68 T
(Scattered) 440.77 513.68 T
(Light) 447.45 504.68 T
2 6.4 Q
(a) 467 507.88 T
2 8 Q
(S) 506.18 504.68 T
13 F
(l) 511.52 502.18 T
2 6.4 Q
(b) 515.91 507.88 T
0 9 Q
(51) 157.38 490.02 T
(1) 220.52 490.02 T
(102) 224.68 490.02 T
(1091 \320 1) 283.83 490.02 T
(1) 315 490.02 T
(13) 319.17 490.02 T
(5.90 \320 5.55) 366.75 490.02 T
432.25 485.27 485.75 499.77 R
7 X
V
0 X
(50) 157.38 475.02 T
(1) 220.52 475.02 T
(124) 224.68 475.02 T
(1) 284 475.02 T
(1) 288.17 475.02 T
(13 \320 1) 292.33 475.02 T
(135) 314.5 475.02 T
(6.05 \320 5.65) 366.75 475.02 T
432.25 470.27 485.75 484.77 R
7 X
V
0 X
(49) 157.38 460.02 T
(1) 220.52 460.02 T
(147) 224.68 460.02 T
(1) 283.83 460.02 T
(135 \320 1) 288 460.02 T
(159) 314.67 460.02 T
(6.15 \320 5.75) 366.75 460.02 T
432.25 455.27 485.75 469.77 R
7 X
V
0 X
(0.061) 448.88 460.02 T
(0.12) 505.12 460.02 T
(48) 157.38 445.02 T
(1) 220.52 445.02 T
(171) 224.68 445.02 T
(1) 283.83 445.02 T
(159 \320 1) 288 445.02 T
(183) 314.67 445.02 T
(6.25 \320 5.90) 366.75 445.02 T
432.25 440.27 485.75 454.77 R
7 X
V
0 X
(0.058) 448.88 445.02 T
(0.27) 505.12 445.02 T
(47) 157.38 430.02 T
(1) 220.52 430.02 T
(196) 224.68 430.02 T
(1) 283.67 430.02 T
(183 \320 1209) 287.83 430.02 T
(6.40 \320 6.00) 366.75 430.02 T
432.25 425.27 485.75 439.77 R
7 X
V
0 X
(0.055) 448.88 430.02 T
(0.46) 505.12 430.02 T
(46) 157.38 415.02 T
(1222) 220.35 415.02 T
(1209 \320 1235) 283.5 415.02 T
(6.55 \320 6.10) 366.75 415.02 T
432.25 410.27 485.75 424.77 R
7 X
V
0 X
(0.052) 448.88 415.02 T
(0.8) 507.38 415.02 T
(45) 157.38 400.02 T
(1249) 220.35 400.02 T
(1235 \320 1263) 283.5 400.02 T
(6.70 \320 6.25) 366.75 400.02 T
432.25 395.27 485.75 409.77 R
7 X
V
0 X
(0.049) 448.88 400.02 T
(0.92) 505.12 400.02 T
(44) 157.38 385.02 T
(1277) 220.35 385.02 T
(1263 \320 1292) 283.5 385.02 T
(6.85 \320 6.40) 366.75 385.02 T
432.25 380.27 485.75 394.77 R
7 X
V
0 X
(0.046) 448.88 385.02 T
(1.15) 505.12 385.02 T
(43) 157.38 370.02 T
(1307) 220.35 370.02 T
(1292 \320 1322) 283.5 370.02 T
(7.05 \320 6.55) 366.75 370.02 T
432.25 365.27 485.75 379.77 R
7 X
V
0 X
(0.044) 448.88 370.02 T
(1.16) 505.12 370.02 T
(42) 157.38 355.02 T
(1338) 220.35 355.02 T
(1322 \320 1354) 283.5 355.02 T
(7.20 \320 6.70) 366.75 355.02 T
432.25 350.27 485.75 364.77 R
7 X
V
0 X
(0.041) 448.88 355.02 T
(1.34) 505.12 355.02 T
(41) 157.38 340.02 T
(1371) 220.35 340.02 T
(1354 \320 1387) 283.5 340.02 T
(7.40 \320 6.85) 366.75 340.02 T
432.25 335.27 485.75 349.77 R
7 X
V
0 X
(0.039) 448.88 340.02 T
(1.23) 505.12 340.02 T
(40) 157.38 325.02 T
(1405) 220.35 325.02 T
(1387 \320 1423) 283.5 325.02 T
(7.55 \320 7.00) 366.75 325.02 T
432.25 320.27 485.75 334.77 R
7 X
V
0 X
(0.037) 448.88 325.02 T
(1.47) 505.12 325.02 T
(39) 157.38 310.02 T
(1441) 220.35 310.02 T
(1423 \320 1460) 283.5 310.02 T
(7.80 \320 7.20) 366.75 310.02 T
432.25 305.27 485.75 319.77 R
7 X
V
0 X
(0.035) 448.88 310.02 T
(1.04) 505.12 310.02 T
(38) 157.38 295.02 T
(1479) 220.35 295.02 T
(1460 \320 1498) 283.5 295.02 T
(8.00 \320 7.40) 366.75 295.02 T
432.25 290.27 485.75 304.77 R
7 X
V
0 X
(0.034) 448.88 295.02 T
(0.91) 505.12 295.02 T
(37) 157.38 280.02 T
(1519) 220.35 280.02 T
(1498 \320 1539) 283.5 280.02 T
(8.25 \320 7.55) 366.75 280.02 T
432.25 275.27 485.75 289.77 R
7 X
V
0 X
(0.032) 448.88 280.02 T
(0.77) 505.12 280.02 T
(36) 157.38 265.02 T
(1561) 220.35 265.02 T
(1539 \320 1583) 283.5 265.02 T
(8.45 \320 7.75) 366.75 265.02 T
432.25 260.27 485.75 274.77 R
7 X
V
0 X
(0.031) 448.88 265.02 T
(0.64) 505.12 265.02 T
(35) 157.38 250.02 T
(1606) 220.35 250.02 T
(1583 \320 1629) 283.5 250.02 T
(8.70 \320 7.95) 366.75 250.02 T
432.25 245.27 485.75 259.77 R
7 X
V
0 X
(0.030) 448.88 250.02 T
(0.56) 505.12 250.02 T
(34) 157.38 235.02 T
(1653) 220.35 235.02 T
(1629 \320 1677) 283.5 235.02 T
(8.95 \320 8.20) 366.75 235.02 T
432.25 230.27 485.75 244.77 R
7 X
V
0 X
(0.030) 448.88 235.02 T
(0.44) 505.12 235.02 T
(33) 157.38 220.02 T
(1703) 220.35 220.02 T
(1677 \320 1729) 283.5 220.02 T
(9.25 \320 8.40) 366.75 220.02 T
432.25 215.27 485.75 229.77 R
7 X
V
0 X
(0.029) 448.88 220.02 T
(0.40) 505.12 220.02 T
135.06 525.89 135.06 215.14 2 L
V
0.25 H
0 Z
N
188.7 526.14 188.7 214.89 2 L
V
N
270 526.14 270 214.89 2 L
V
N
342 526.14 342 214.89 2 L
V
N
432 526.14 432 499.77 2 L
V
N
432 500.27 432 214.77 2 L
V
0.5 H
N
486 526.14 486 499.77 2 L
V
0.25 H
N
486 500.27 486 214.77 2 L
V
0.5 H
N
540 525.89 540 215.14 2 L
V
0.25 H
N
134.93 526.02 540.12 526.02 2 L
V
N
134.93 500.02 540.12 500.02 2 L
V
0.5 H
N
134.93 485.02 432.25 485.02 2 L
V
0.25 H
N
431.75 485.02 486.25 485.02 2 L
V
0.5 H
N
485.75 485.02 540.12 485.02 2 L
V
0.25 H
N
134.93 470.02 432.25 470.02 2 L
V
N
431.75 470.02 486.25 470.02 2 L
V
0.5 H
N
485.75 470.02 540.12 470.02 2 L
V
0.25 H
N
134.93 455.02 432.25 455.02 2 L
V
N
431.75 455.02 486.25 455.02 2 L
V
0.5 H
N
485.75 455.02 540.12 455.02 2 L
V
0.25 H
N
134.93 440.02 432.25 440.02 2 L
V
N
431.75 440.02 486.25 440.02 2 L
V
0.5 H
N
485.75 440.02 540.12 440.02 2 L
V
0.25 H
N
134.93 425.02 432.25 425.02 2 L
V
N
431.75 425.02 486.25 425.02 2 L
V
0.5 H
N
485.75 425.02 540.12 425.02 2 L
V
0.25 H
N
134.93 410.02 432.25 410.02 2 L
V
N
431.75 410.02 486.25 410.02 2 L
V
0.5 H
N
485.75 410.02 540.12 410.02 2 L
V
0.25 H
N
134.93 395.02 432.25 395.02 2 L
V
N
431.75 395.02 486.25 395.02 2 L
V
0.5 H
N
485.75 395.02 540.12 395.02 2 L
V
0.25 H
N
134.93 380.02 432.25 380.02 2 L
V
N
431.75 380.02 486.25 380.02 2 L
V
0.5 H
N
485.75 380.02 540.12 380.02 2 L
V
0.25 H
N
134.93 365.02 432.25 365.02 2 L
V
N
431.75 365.02 486.25 365.02 2 L
V
0.5 H
N
485.75 365.02 540.12 365.02 2 L
V
0.25 H
N
134.93 350.02 432.25 350.02 2 L
V
N
431.75 350.02 486.25 350.02 2 L
V
0.5 H
N
485.75 350.02 540.12 350.02 2 L
V
0.25 H
N
134.93 335.02 432.25 335.02 2 L
V
N
431.75 335.02 486.25 335.02 2 L
V
0.5 H
N
485.75 335.02 540.12 335.02 2 L
V
0.25 H
N
134.93 320.02 432.25 320.02 2 L
V
N
431.75 320.02 486.25 320.02 2 L
V
0.5 H
N
485.75 320.02 540.12 320.02 2 L
V
0.25 H
N
134.93 305.02 432.25 305.02 2 L
V
N
431.75 305.02 486.25 305.02 2 L
V
0.5 H
N
485.75 305.02 540.12 305.02 2 L
V
0.25 H
N
134.93 290.02 432.25 290.02 2 L
V
N
431.75 290.02 486.25 290.02 2 L
V
0.5 H
N
485.75 290.02 540.12 290.02 2 L
V
0.25 H
N
134.93 275.02 432.25 275.02 2 L
V
N
431.75 275.02 486.25 275.02 2 L
V
0.5 H
N
485.75 275.02 540.12 275.02 2 L
V
0.25 H
N
134.93 260.02 432.25 260.02 2 L
V
N
431.75 260.02 486.25 260.02 2 L
V
0.5 H
N
485.75 260.02 540.12 260.02 2 L
V
0.25 H
N
134.93 245.02 432.25 245.02 2 L
V
N
431.75 245.02 486.25 245.02 2 L
V
0.5 H
N
485.75 245.02 540.12 245.02 2 L
V
0.25 H
N
134.93 230.02 432.25 230.02 2 L
V
N
431.75 230.02 486.25 230.02 2 L
V
0.5 H
N
485.75 230.02 540.12 230.02 2 L
V
0.25 H
N
134.93 215.02 431.75 215.02 2 L
V
N
432.25 215.02 485.75 215.02 2 L
V
0.5 H
N
486.25 215.02 540.12 215.02 2 L
V
0.25 H
N
FMENDPAGE
%%EndPage: "87" 87
%%Page: "88" 88
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(88) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
135.06 356.02 540 363.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
-0.08 (a.) 135.06 350.02 P
3 F
-0.08 (\322d\323) 143.48 350.02 P
0 F
-0.08 ( coef) 157.99 350.02 P
-0.08 (\336cient of Cardelli, Ebbets, and Savage \0501993; see Section) 175.48 350.02 P
-0.08 (9.2 on page) 384.07 350.02 P
-0.08 (102\051. These apply only to) 427.9 350.02 P
(the SSA.) 171.06 340.02 T
-0.08 (b. Sensitivity function at blaze peak, in units of 10) 135.06 327.02 P
0 7.2 Q
-0.07 (1) 315.55 330.62 P
-0.07 (1) 318.88 330.62 P
0 9 Q
-0.08 ( \050counts diode) 322.48 327.02 P
0 7.2 Q
-0.07 (-1) 373.3 330.62 P
0 9 Q
-0.08 ( sec) 379.3 327.02 P
0 7.2 Q
-0.07 (-1) 392.96 330.62 P
0 9 Q
-0.08 (\051 per incident \050er) 398.96 327.02 P
-0.08 (g cm) 458.77 327.02 P
0 7.2 Q
-0.07 (-2) 476.44 330.62 P
0 9 Q
-0.08 ( sec) 482.43 327.02 P
0 7.2 Q
-0.07 (-1) 496.09 330.62 P
0 9 Q
-0.08 ( \201) 502.09 327.02 P
0 7.2 Q
-0.07 (-1) 510.76 330.62 P
0 9 Q
-0.08 (\051.) 516.75 327.02 P
54 657.02 540 670.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 664.02 540 664.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 664.02 180 664.02 2 L
0 Z
N
0 0 612 792 C
2 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 651.02 T
(ABLE 8-4) 58.83 651.02 T
4 F
(Properties of Grating Echelle-B) 189 640.02 T
2 8 Q
(Order) 150.99 607.68 T
(Central) 215.57 616.68 T
(W) 200.39 607.68 T
(avelength \050\201\051) 207.64 607.68 T
(Order) 295.11 616.68 T
(Coverage \050\201\051) 281.11 607.68 T
(Bandpass per) 360.55 616.68 T
(exposure \050\201\051) 362.55 607.68 T
(Scattered) 440.77 616.68 T
(Light) 447.45 607.68 T
2 6.4 Q
(a) 467 610.88 T
2 8 Q
(S) 506.18 616.68 T
13 F
(l) 511.52 614.18 T
2 6.4 Q
(b) 515.91 619.88 T
0 9 Q
(33) 157.38 593.02 T
(1703) 220.35 593.02 T
(1677 \320 1729) 283.5 593.02 T
(9.3 \320 8.4) 371.25 593.02 T
432.25 588.27 485.75 602.77 R
7 X
V
0 X
(0.045) 448.88 593.02 T
(0.35) 505.12 593.02 T
(32) 157.38 578.02 T
(1756) 220.35 578.02 T
(1729 \320 1784) 283.5 578.02 T
(9.6 \320 8.6) 371.25 578.02 T
432.25 573.27 485.75 587.77 R
7 X
V
0 X
(0.043) 448.88 578.02 T
(0.74) 505.12 578.02 T
(31) 157.38 563.02 T
(1813) 220.35 563.02 T
(1784 \320 1842) 283.5 563.02 T
(9.9 \320 8.9) 371.25 563.02 T
432.25 558.27 485.75 572.77 R
7 X
V
0 X
(0.041) 448.88 563.02 T
(1.06) 505.12 563.02 T
(30) 157.38 548.02 T
(1873) 220.35 548.02 T
(1842 \320 1905) 283.5 548.02 T
(10.3 \320 9.2) 369 548.02 T
432.25 543.27 485.75 557.77 R
7 X
V
0 X
(0.039) 448.88 548.02 T
(1.62) 505.12 548.02 T
(29) 157.38 533.02 T
(1938) 220.35 533.02 T
(1905 \320 1971) 283.5 533.02 T
(10.7 \320 9.5) 369 533.02 T
432.25 528.27 485.75 542.77 R
7 X
V
0 X
(0.037) 448.88 533.02 T
(2.26) 505.12 533.02 T
(28) 157.38 518.02 T
(2007) 220.35 518.02 T
(1971 \320 2043) 283.5 518.02 T
(1) 369.17 518.02 T
(1.1 \320 9.8) 373.33 518.02 T
432.25 513.27 485.75 527.77 R
7 X
V
0 X
(0.035) 448.88 518.02 T
(3.04) 505.12 518.02 T
(27) 157.38 503.02 T
(2082) 220.35 503.02 T
(2043 \320 2120) 283.5 503.02 T
(1) 366.92 503.02 T
(1.5 \320 10.1) 371.08 503.02 T
432.25 498.27 485.75 512.77 R
7 X
V
0 X
(0.033) 448.88 503.02 T
(4.29) 505.12 503.02 T
(26) 157.38 488.02 T
(2162) 220.35 488.02 T
(2120 \320 2203) 283.5 488.02 T
(1) 366.92 488.02 T
(1.9 \320 10.5) 371.08 488.02 T
432.25 483.27 485.75 497.77 R
7 X
V
0 X
(0.031) 448.88 488.02 T
(6.18) 505.12 488.02 T
(25) 157.38 473.02 T
(2248) 220.35 473.02 T
(2203 \320 2293) 283.5 473.02 T
(12.4 \320 10.9) 366.75 473.02 T
432.25 468.27 485.75 482.77 R
7 X
V
0 X
(0.030) 448.88 473.02 T
(8.59) 505.12 473.02 T
(24) 157.38 458.02 T
(2342) 220.35 458.02 T
(2293 \320 2391) 283.5 458.02 T
(13.0 \320 1) 366.92 458.02 T
(1.3) 395.83 458.02 T
432.25 453.27 485.75 467.77 R
7 X
V
0 X
(0.028) 448.88 458.02 T
(9.96) 505.12 458.02 T
(23) 157.38 443.02 T
(2444) 220.35 443.02 T
(2390 \320 2497) 283.5 443.02 T
(13.6 \320 1) 366.92 443.02 T
(1.7) 395.83 443.02 T
432.25 438.27 485.75 452.77 R
7 X
V
0 X
(0.026) 448.88 443.02 T
(1) 505.29 443.02 T
(1.2) 509.46 443.02 T
(22) 157.38 428.02 T
(2555) 220.35 428.02 T
(2497 \320 2613) 283.5 428.02 T
(14.2 \320 12.2) 366.75 428.02 T
432.25 423.27 485.75 437.77 R
7 X
V
0 X
(0.024) 448.88 428.02 T
(13.0) 505.12 428.02 T
(21) 157.38 413.02 T
(2676) 220.35 413.02 T
(2613 \320 2740) 283.5 413.02 T
(14.9 \320 12.7) 366.75 413.02 T
432.25 408.27 485.75 422.77 R
7 X
V
0 X
(0.022) 448.88 413.02 T
(13.4) 505.12 413.02 T
(20) 157.38 398.02 T
(2810) 220.35 398.02 T
(2740 \320 2880) 283.5 398.02 T
(15.8 \320 13.3) 366.75 398.02 T
432.25 393.27 485.75 407.77 R
7 X
V
0 X
(0.020) 448.88 398.02 T
(12.8) 505.12 398.02 T
(19) 157.38 383.02 T
(2958) 220.35 383.02 T
(2880 \320 3036) 283.5 383.02 T
(16.7 \320 13.9) 366.75 383.02 T
432.25 378.27 485.75 392.77 R
7 X
V
0 X
(0.018) 448.88 383.02 T
(9.57) 505.12 383.02 T
(18) 157.38 368.02 T
(3122) 220.35 368.02 T
(3036 \320 3209) 283.5 368.02 T
(17.6 \320 14.6) 366.75 368.02 T
432.25 363.27 485.75 377.77 R
7 X
V
0 X
(0.016) 448.88 368.02 T
(4.20) 505.12 368.02 T
135.06 628.89 135.06 363.14 2 L
V
0.25 H
0 Z
N
188.7 629.14 188.7 362.89 2 L
V
N
270 629.14 270 362.89 2 L
V
N
342 629.14 342 362.89 2 L
V
N
432 629.14 432 602.77 2 L
V
N
432 603.27 432 362.77 2 L
V
0.5 H
N
486 629.14 486 602.77 2 L
V
0.25 H
N
486 603.27 486 362.77 2 L
V
0.5 H
N
540 628.89 540 363.14 2 L
V
0.25 H
N
134.93 629.02 540.12 629.02 2 L
V
N
134.93 603.02 540.12 603.02 2 L
V
0.5 H
N
134.93 588.02 432.25 588.02 2 L
V
0.25 H
N
431.75 588.02 486.25 588.02 2 L
V
0.5 H
N
485.75 588.02 540.12 588.02 2 L
V
0.25 H
N
134.93 573.02 432.25 573.02 2 L
V
N
431.75 573.02 486.25 573.02 2 L
V
0.5 H
N
485.75 573.02 540.12 573.02 2 L
V
0.25 H
N
134.93 558.02 432.25 558.02 2 L
V
N
431.75 558.02 486.25 558.02 2 L
V
0.5 H
N
485.75 558.02 540.12 558.02 2 L
V
0.25 H
N
134.93 543.02 432.25 543.02 2 L
V
N
431.75 543.02 486.25 543.02 2 L
V
0.5 H
N
485.75 543.02 540.12 543.02 2 L
V
0.25 H
N
134.93 528.02 432.25 528.02 2 L
V
N
431.75 528.02 486.25 528.02 2 L
V
0.5 H
N
485.75 528.02 540.12 528.02 2 L
V
0.25 H
N
134.93 513.02 432.25 513.02 2 L
V
N
431.75 513.02 486.25 513.02 2 L
V
0.5 H
N
485.75 513.02 540.12 513.02 2 L
V
0.25 H
N
134.93 498.02 432.25 498.02 2 L
V
N
431.75 498.02 486.25 498.02 2 L
V
0.5 H
N
485.75 498.02 540.12 498.02 2 L
V
0.25 H
N
134.93 483.02 432.25 483.02 2 L
V
N
431.75 483.02 486.25 483.02 2 L
V
0.5 H
N
485.75 483.02 540.12 483.02 2 L
V
0.25 H
N
134.93 468.02 432.25 468.02 2 L
V
N
431.75 468.02 486.25 468.02 2 L
V
0.5 H
N
485.75 468.02 540.12 468.02 2 L
V
0.25 H
N
134.93 453.02 432.25 453.02 2 L
V
N
431.75 453.02 486.25 453.02 2 L
V
0.5 H
N
485.75 453.02 540.12 453.02 2 L
V
0.25 H
N
134.93 438.02 432.25 438.02 2 L
V
N
431.75 438.02 486.25 438.02 2 L
V
0.5 H
N
485.75 438.02 540.12 438.02 2 L
V
0.25 H
N
134.93 423.02 432.25 423.02 2 L
V
N
431.75 423.02 486.25 423.02 2 L
V
0.5 H
N
485.75 423.02 540.12 423.02 2 L
V
0.25 H
N
134.93 408.02 432.25 408.02 2 L
V
N
431.75 408.02 486.25 408.02 2 L
V
0.5 H
N
485.75 408.02 540.12 408.02 2 L
V
0.25 H
N
134.93 393.02 432.25 393.02 2 L
V
N
431.75 393.02 486.25 393.02 2 L
V
0.5 H
N
485.75 393.02 540.12 393.02 2 L
V
0.25 H
N
134.93 378.02 432.25 378.02 2 L
V
N
431.75 378.02 486.25 378.02 2 L
V
0.5 H
N
485.75 378.02 540.12 378.02 2 L
V
0.25 H
N
134.93 363.02 431.75 363.02 2 L
V
N
432.25 363.02 485.75 363.02 2 L
V
0.5 H
N
486.25 363.02 540.12 363.02 2 L
V
0.25 H
N
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (89) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Reference T) 207 736.18 T
(ables for Instrument Performance) 257.85 736.18 T
2 10 Q
(8.3.2) 157.76 679.35 T
(Echelle W) 189 679.35 T
(avelength Formats) 235.87 679.35 T
0 F
-0.03 (The illustrations below provide a means of estimating where particular wavelengths fall) 189 663.35 P
0.22 (within the echelle formats and where they lie relative to the blaze peak. Note that these) 189 651.35 P
0.53 (layouts are purely schematic; the actual length of the free spectral range changes from) 189 639.35 P
(order to order) 189 627.35 T
(. The center of each order is at) 243.43 627.35 T
3 F
(m) 367.55 627.35 T
13 F
(l) 374.77 627.35 T
0 F
( = 56200.) 380.26 627.35 T
2 F
(Figure 8-4.) 126 129.33 T
4 F
(Schematic format of wavelengths for Echelle-B.) 182.13 129.33 T
54 87.98 540 686.02 C
54 145 540 609.02 C
0 0 0 1 0 0 0 K
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805 1651 d 807 1651 d 811 1652 d 813 1656 d 814 1662 d 814 1666 d
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1410 1661 d 1406 1662 d 1404 1664 d 1403 1668 d 1403 1669 d 1404 1673 d
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512 556 534 627 R
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2 9 Q
(Reference T) 189 736.18 T
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54 726.98 540 726.98 2 L
0.25 H
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54 74.02 540 74.02 2 L
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(90) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
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54 74.02 540 74.02 2 L
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54 726.98 540 726.98 2 L
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54 74.02 540 74.02 2 L
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(Figure 8-5.) 126 128.33 T
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(Schematic format of wavelengths for Echelle-A.) 182.13 128.33 T
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1840 2556 d 1842 2552 d 1846 2551 d 1848 2551 d 1852 2552 d 1854 2556 d
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100 653 123 666 R
7 X
V
1 H
2 Z
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101 174 122 195 R
V
N
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V
N
509 659 530 680 R
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N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (91) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
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72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Reference T) 207 736.18 T
(ables for Instrument Performance) 257.85 736.18 T
2 10 Q
(8.3.3) 157.76 679.35 T
(Echelle Blaze Function) 189 679.35 T
0 F
1.04 (The \336gure below shows the echelle blaze function \050also known as the \322Ripple Func-) 189 659.35 P
0.11 (tion\323\051 in the form of sensitivity relative to the peak of the blaze as the product of wave-) 189 647.35 P
(length and order number) 189 635.35 T
(.) 287.04 635.35 T
2 F
(Figure 8-6.) 126 330.33 T
4 F
(Normalized blaze function for the GHRS echelle gratings.) 182.13 330.33 T
54 87.98 540 686.02 C
54 346 540 617.02 C
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2210 962 d 2206 967 d 2202 968 d 2198 968 d 2230 968 r 2226 967 d
2222 962 d 2221 954 d 2221 949 d 2222 941 d 2226 936 d 2230 935 d
2234 935 d 2238 936 d 2242 941 d 2243 949 d 2243 954 d 2242 962 d
2238 967 d 2234 968 d 2230 968 d 2262 968 r 2258 967 d 2254 962 d
2253 954 d 2253 949 d 2254 941 d 2258 936 d 2262 935 d 2266 935 d
2270 936 d 2274 941 d 2275 949 d 2275 954 d 2274 962 d 2270 967 d
2266 968 d 2262 968 d 600 1800 r 2200 1800 d 600 1800 r 600 1749 d
653 1800 r 653 1774 d 707 1800 r 707 1774 d 760 1800 r 760 1774 d
813 1800 r 813 1774 d 867 1800 r 867 1774 d 920 1800 r 920 1774 d
973 1800 r 973 1774 d 1027 1800 r 1027 1774 d 1080 1800 r 1080 1774 d
1133 1800 r 1133 1749 d 1187 1800 r 1187 1774 d 1240 1800 r 1240 1774 d
1293 1800 r 1293 1774 d 1347 1800 r 1347 1774 d 1400 1800 r 1400 1774 d
1453 1800 r 1453 1774 d 1507 1800 r 1507 1774 d 1560 1800 r 1560 1774 d
1613 1800 r 1613 1774 d 1667 1800 r 1667 1749 d 1720 1800 r 1720 1774 d
1773 1800 r 1773 1774 d 1827 1800 r 1827 1774 d 1880 1800 r 1880 1774 d
1933 1800 r 1933 1774 d 1987 1800 r 1987 1774 d 2040 1800 r 2040 1774 d
2093 1800 r 2093 1774 d 2147 1800 r 2147 1774 d 2200 1800 r 2200 1749 d
600 1000 r 600 1800 d 600 1000 r 651 1000 d 600 1080 r 626 1080 d
600 1160 r 626 1160 d 600 1240 r 626 1240 d 600 1320 r 626 1320 d
600 1400 r 651 1400 d 600 1480 r 626 1480 d 600 1560 r 626 1560 d
600 1640 r 626 1640 d 600 1720 r 626 1720 d 600 1800 r 651 1800 d
508 1019 r 504 1018 d 500 1013 d 499 1005 d 499 1000 d 500 992 d
504 987 d 508 986 d 512 986 d 516 987 d 520 992 d 521 1000 d
521 1005 d 520 1013 d 516 1018 d 512 1019 d 508 1019 d 534 989 r
532 987 d 534 986 d 536 987 d 534 989 d 556 1019 r 552 1018 d
548 1013 d 547 1005 d 547 1000 d 548 992 d 552 987 d 556 986 d
560 986 d 564 987 d 568 992 d 569 1000 d 569 1005 d 568 1013 d
564 1018 d 560 1019 d 556 1019 d 508 1419 r 504 1418 d 500 1413 d
499 1405 d 499 1400 d 500 1392 d 504 1387 d 508 1386 d 512 1386 d
516 1387 d 520 1392 d 521 1400 d 521 1405 d 520 1413 d 516 1418 d
512 1419 d 508 1419 d 534 1389 r 532 1387 d 534 1386 d 536 1387 d
534 1389 d 566 1419 r 550 1419 d 548 1405 d 550 1406 d 555 1408 d
560 1408 d 564 1406 d 568 1403 d 569 1398 d 569 1395 d 568 1390 d
564 1387 d 560 1386 d 555 1386 d 550 1387 d 548 1389 d 547 1392 d
504 1813 r 507 1814 d 512 1819 d 512 1786 d 534 1789 r 532 1787 d
534 1786 d 536 1787 d 534 1789 d 556 1819 r 552 1818 d 548 1813 d
547 1805 d 547 1800 d 548 1792 d 552 1787 d 556 1786 d 560 1786 d
564 1787 d 568 1792 d 569 1800 d 569 1805 d 568 1813 d 564 1818 d
560 1819 d 556 1819 d 2200 1000 r 2200 1800 d 2200 1000 r 2149 1000 d
2200 1080 r 2174 1080 d 2200 1160 r 2174 1160 d 2200 1240 r 2174 1240 d
2200 1320 r 2174 1320 d 2200 1400 r 2149 1400 d 2200 1480 r 2174 1480 d
2200 1560 r 2174 1560 d 2200 1640 r 2174 1640 d 2200 1720 r 2174 1720 d
2200 1800 r 2149 1800 d 336 1126 r 378 1126 d 336 1126 r 336 1144 d
338 1150 d 340 1152 d 344 1154 d 348 1154 d 352 1152 d 354 1150 d
356 1144 d 356 1126 d 356 1140 r 378 1154 d 362 1168 r 362 1192 d
358 1192 d 354 1190 d 352 1188 d 350 1184 d 350 1178 d 352 1174 d
356 1170 d 362 1168 d 366 1168 d 372 1170 d 376 1174 d 378 1178 d
378 1184 d 376 1188 d 372 1192 d 336 1206 r 378 1206 d 350 1244 r
378 1244 d 356 1244 r 352 1240 d 350 1236 d 350 1230 d 352 1226 d
356 1222 d 362 1220 d 366 1220 d 372 1222 d 376 1226 d 378 1230 d
378 1236 d 376 1240 d 372 1244 d 336 1260 r 370 1260 d 376 1262 d
378 1266 d 378 1270 d 350 1254 r 350 1268 d 336 1276 r 338 1278 d
336 1280 d 334 1278 d 336 1276 d 350 1278 r 378 1278 d 350 1290 r
378 1302 d 350 1314 r 378 1302 d 362 1324 r 362 1348 d 358 1348 d
354 1346 d 352 1344 d 350 1340 d 350 1334 d 352 1330 d 356 1326 d
362 1324 d 366 1324 d 372 1326 d 376 1330 d 378 1334 d 378 1340 d
376 1344 d 372 1348 d 342 1420 r 338 1416 d 336 1410 d 336 1402 d
338 1396 d 342 1392 d 346 1392 d 350 1394 d 352 1396 d 354 1400 d
358 1412 d 360 1416 d 362 1418 d 366 1420 d 372 1420 d 376 1416 d
378 1410 d 378 1402 d 376 1396 d 372 1392 d 362 1432 r 362 1456 d
358 1456 d 354 1454 d 352 1452 d 350 1448 d 350 1442 d 352 1438 d
356 1434 d 362 1432 d 366 1432 d 372 1434 d 376 1438 d 378 1442 d
378 1448 d 376 1452 d 372 1456 d 350 1470 r 378 1470 d 358 1470 r
352 1476 d 350 1480 d 350 1486 d 352 1490 d 358 1492 d 378 1492 d
356 1526 r 352 1524 d 350 1518 d 350 1512 d 352 1506 d 356 1504 d
360 1506 d 362 1510 d 364 1520 d 366 1524 d 370 1526 d 372 1526 d
376 1524 d 378 1518 d 378 1512 d 376 1506 d 372 1504 d 336 1536 r
338 1538 d 336 1540 d 334 1538 d 336 1536 d 350 1538 r 378 1538 d
336 1556 r 370 1556 d 376 1558 d 378 1562 d 378 1566 d 350 1550 r
350 1564 d 336 1572 r 338 1574 d 336 1576 d 334 1574 d 336 1572 d
350 1574 r 378 1574 d 350 1586 r 378 1598 d 350 1610 r 378 1598 d
336 1620 r 338 1622 d 336 1624 d 334 1622 d 336 1620 d 350 1622 r
378 1622 d 336 1640 r 370 1640 d 376 1642 d 378 1646 d 378 1650 d
350 1634 r 350 1648 d 350 1654 r 378 1666 d 350 1678 r 378 1666 d
386 1662 d 390 1658 d 392 1654 d 392 1652 d 1156 882 r 1156 854 d
1156 874 r 1162 880 d 1166 882 d 1172 882 d 1176 880 d 1178 874 d
1178 854 d 1178 874 r 1184 880 d 1188 882 d 1194 882 d 1198 880 d
1200 874 d 1200 854 d 1214 896 r 1218 896 d 1222 894 d 1224 892 d
1228 882 d 1240 856 d 1242 854 d 1218 896 r 1222 892 d 1226 882 d
1238 856 d 1242 854 d 1244 854 d 1226 882 r 1212 854 d 1226 882 r
1214 854 d 1302 904 r 1298 900 d 1294 894 d 1290 886 d 1288 876 d
1288 868 d 1290 858 d 1294 850 d 1298 844 d 1302 840 d 1326 896 r
1310 854 d 1326 896 r 1342 854 d 1316 868 r 1336 868 d 1352 882 r
1352 854 d 1352 874 r 1358 880 d 1362 882 d 1368 882 d 1372 880 d
1374 874 d 1374 854 d 1410 882 r 1410 850 d 1408 844 d 1406 842 d
1402 840 d 1396 840 d 1392 842 d 1410 876 r 1406 880 d 1402 882 d
1396 882 d 1392 880 d 1388 876 d 1386 870 d 1386 866 d 1388 860 d
1392 856 d 1396 854 d 1402 854 d 1406 856 d 1410 860 d 1444 876 r
1442 880 d 1436 882 d 1430 882 d 1424 880 d 1422 876 d 1424 872 d
1428 870 d 1438 868 d 1442 866 d 1444 862 d 1444 860 d 1442 856 d
1436 854 d 1430 854 d 1424 856 d 1422 860 d 1458 896 r 1458 862 d
1460 856 d 1464 854 d 1468 854 d 1452 882 r 1466 882 d 1476 882 r
1476 854 d 1476 870 r 1478 876 d 1482 880 d 1486 882 d 1492 882 d
1512 882 r 1508 880 d 1504 876 d 1502 870 d 1502 866 d 1504 860 d
1508 856 d 1512 854 d 1518 854 d 1522 856 d 1526 860 d 1528 866 d
1528 870 d 1526 876 d 1522 880 d 1518 882 d 1512 882 d 1540 882 r
1540 854 d 1540 874 r 1546 880 d 1550 882 d 1556 882 d 1560 880 d
1562 874 d 1562 854 d 1562 874 r 1568 880 d 1572 882 d 1578 882 d
1582 880 d 1584 874 d 1584 854 d 1620 876 r 1618 880 d 1612 882 d
1606 882 d 1600 880 d 1598 876 d 1600 872 d 1604 870 d 1614 868 d
1618 866 d 1620 862 d 1620 860 d 1618 856 d 1612 854 d 1606 854 d
1600 856 d 1598 860 d 1630 904 r 1634 900 d 1638 894 d 1642 886 d
1644 876 d 1644 868 d 1642 858 d 1638 850 d 1634 844 d 1630 840 d
747 1266 r 813 1378 d 867 1474 d 920 1550 d 973 1616 d 1027 1672 d
1080 1728 d 1133 1762 d 1187 1786 d 1240 1797 d 1256 1800 d 1293 1794 d
1347 1773 d 1400 1741 d 1453 1700 d 1507 1646 d 1560 1584 d 1613 1522 d
1667 1471 d 1720 1408 d 1773 1354 d 1827 1300 d 1880 1248 d 1933 1200 d
e
%%Trailer
EndPSPlot

%%EndDocument
FMENDEPSF
54 87.98 540 686.02 C
0 0 612 792 C
FMENDPAGE
%%EndPage: "91" 91
%%Page: "92" 92
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(92) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
2 12 Q
(8.4) 163.32 678.02 T
(Standard Patterns for Substepping and Background) 189 678.02 T
54 657.02 540 660.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 658.52 540 658.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 658.52 180 658.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(Measurement) 189 664.02 T
0 10 Q
-0.06 (This table shows how each) 189 640.35 P
9 F
-0.14 (STEP-PATT) 298.97 640.35 P
0 F
-0.06 ( pattern measures the background for a science) 352.97 640.35 P
0.48 (exposure. Listed are the) 189 628.35 P
9 F
1.16 (STEP-PATT) 288.96 628.35 P
0 F
0.48 ( number) 342.96 628.35 P
0.48 (, the number of spectrum bins for which) 376.09 628.35 P
0.37 (substepping occurs, the number of background bins measured, the diodes used to mea-) 189 616.35 P
0.57 (sure the background, the fraction of the total time spent measuring \337ux on the science) 189 604.35 P
-0.25 (diodes, the gratings for which the) 189 592.35 P
9 F
-0.59 (STEP-PATT) 323.89 592.35 P
0 F
-0.25 ( is appropriate, and the shortest exposure) 377.89 592.35 P
0.98 (that can be used for that pattern. The shortest exposure has been computed assuming) 189 580.35 P
9 F
0.68 (COMB=4) 189 568.35 P
0 F
0.28 (, which is the recommended value. These minimum exposures can be reduced) 225 568.35 P
(by half if) 189 556.35 T
9 F
(COMB=2) 228.16 556.35 T
0 F
( is used and by a factor of four for) 264.16 556.35 T
9 F
(COMB=NO) 403.01 556.35 T
0 F
(.) 445.01 556.35 T
54 519.02 540 532.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 526.02 540 526.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 526.02 180 526.02 2 L
0 Z
N
0 0 612 792 C
2 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 513.02 T
(ABLE 8-5) 58.83 513.02 T
4 F
(STEP-P) 189 502.02 T
(A) 220.84 502.02 T
(TT speci\336cations) 226.18 502.02 T
10 F
(STEP-) 67.46 478.68 T
(PATT) 70.16 469.68 T
2 8 Q
(number) 66.29 460.68 T
(Bins Measured) 136.11 478.68 T
(Spectrum/) 236.94 478.68 T
(Backgr) 242.94 469.68 T
(Ratio) 246.5 460.68 T
(Diodes used for) 298.27 474.18 T
(Background) 305.16 465.18 T
(On-target) 380.25 474.18 T
(Ef\336ciency) 379.35 465.18 T
(Appropriate) 434.08 474.18 T
( Gratings) 439.19 465.18 T
(Minimum) 495.44 478.68 T
(Exposure) 494.77 469.68 T
(T) 493.29 460.68 T
(ime \050sec\051) 498.03 460.68 T
(Spectrum) 114.61 460.68 T
(Background) 170.16 460.68 T
9 9 Q
(1) 78.26 446.02 T
0 F
(1) 130.81 446.02 T
(0) 191.25 446.02 T
(1) 254.25 446.02 T
(1.00) 390.38 446.02 T
(all) 452.25 446.02 T
(0.8) 507.38 446.02 T
9 F
(2) 78.26 431.02 T
0 F
(2) 130.81 431.02 T
(0) 191.25 431.02 T
(1) 254.25 431.02 T
(1.00) 390.38 431.02 T
(all) 452.25 431.02 T
(1.6) 507.38 431.02 T
9 F
(3) 78.26 416.02 T
0 F
(4) 130.81 416.02 T
(0) 191.25 416.02 T
(1) 254.25 416.02 T
(1.00) 390.38 416.02 T
(all) 452.25 416.02 T
(3.2) 507.38 416.02 T
9 F
(4) 78.26 401.02 T
0 F
(2) 130.81 401.02 T
(2) 191.25 401.02 T
(8) 254.25 401.02 T
(science) 315.26 401.02 T
(0.89) 390.38 401.02 T
(\336rst-order) 438.76 401.02 T
(14.4) 505.12 401.02 T
9 F
(5) 78.26 386.02 T
0 F
(4) 130.81 386.02 T
(2) 191.25 386.02 T
(8) 254.25 386.02 T
(science) 315.26 386.02 T
(0.94) 390.38 386.02 T
(\336rst-order) 438.76 386.02 T
(27.2) 505.12 386.02 T
9 F
(6) 78.26 371.02 T
0 F
(2) 130.81 371.02 T
(2) 191.25 371.02 T
(8) 254.25 371.02 T
(science) 315.26 371.02 T
(0.89) 390.38 371.02 T
(echelle) 444.01 371.02 T
(14.4) 505.12 371.02 T
9 F
(7) 78.26 356.02 T
0 F
(4) 130.81 356.02 T
(2) 191.25 356.02 T
(8) 254.25 356.02 T
(science) 315.26 356.02 T
(0.94) 390.38 356.02 T
(echelle) 444.01 356.02 T
(27.2) 505.12 356.02 T
9 F
(8) 78.26 341.02 T
0 F
(2) 130.81 341.02 T
(2) 191.25 341.02 T
(8) 254.25 341.02 T
(corner) 317.01 341.02 T
(0.89) 390.38 341.02 T
(echelle) 444.01 341.02 T
(14.4) 505.12 341.02 T
9 F
(9) 78.26 326.02 T
0 F
(4) 130.81 326.02 T
(2) 191.25 326.02 T
(8) 254.25 326.02 T
(corner) 317.01 326.02 T
(0.94) 390.38 326.02 T
(echelle) 444.01 326.02 T
(27.2) 505.12 326.02 T
9 F
(10) 75.56 311.02 T
0 F
(2) 130.81 311.02 T
(2) 191.25 311.02 T
(1) 254.25 311.02 T
(science) 315.26 311.02 T
(0.50) 390.38 311.02 T
(\336rst-order) 438.76 311.02 T
(3.2) 507.38 311.02 T
9 F
(11) 75.56 296.02 T
0 F
(4) 130.81 296.02 T
(2) 191.25 296.02 T
(1) 254.25 296.02 T
(science) 315.26 296.02 T
(0.67) 390.38 296.02 T
(\336rst-order) 438.76 296.02 T
(4.8) 507.38 296.02 T
9 F
(12) 75.56 281.02 T
0 F
(2) 130.81 281.02 T
(2) 191.25 281.02 T
(1) 254.25 281.02 T
(science) 315.26 281.02 T
(0.50) 390.38 281.02 T
(echelle) 444.01 281.02 T
(3.2) 507.38 281.02 T
9 F
(13) 75.56 266.02 T
0 F
(4) 130.81 266.02 T
(2) 191.25 266.02 T
(1) 254.25 266.02 T
(science) 315.26 266.02 T
(0.67) 390.38 266.02 T
(echelle) 444.01 266.02 T
(4.8) 507.38 266.02 T
9 F
(14) 75.56 251.02 T
0 F
(2) 130.81 251.02 T
(2) 191.25 251.02 T
(1) 254.25 251.02 T
(corner) 317.01 251.02 T
(0.50) 390.38 251.02 T
(echelle) 444.01 251.02 T
(3.2) 507.38 251.02 T
9 F
(15) 75.56 236.02 T
0 F
(4) 130.81 236.02 T
(2) 191.25 236.02 T
(1) 254.25 236.02 T
(corner) 317.01 236.02 T
(0.67) 390.38 236.02 T
(echelle) 444.01 236.02 T
(4.8) 507.38 236.02 T
54 195.02 540 208.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 202.02 540 202.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 202.02 180 202.02 2 L
0 Z
N
0 0 612 792 C
2 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 189.02 T
(ABLE 8-6) 58.83 189.02 T
4 F
(Default STEP-P) 189 189.02 T
(A) 251.86 189.02 T
(TT for science modes) 257.19 189.02 T
4 8 Q
(Grating) 326.62 172.68 T
(Order) 407.15 172.68 T
9 9 Q
(STEP-PATT) 466.76 172.02 T
0 F
(First-order) 326.62 159.02 T
(1) 415.12 159.02 T
9 F
(5) 488.36 159.02 T
0 F
(Ech-A) 326.62 146.02 T
13 10 Q
(\263) 409.01 146.02 T
0 9 Q
( 51) 414.49 146.02 T
9 F
(9) 488.36 146.02 T
0 F
(< 51) 409.21 133.02 T
9 F
(7) 488.36 133.02 T
0 F
(Ech-B) 326.62 120.02 T
13 10 Q
(\263) 409.01 120.02 T
0 9 Q
( 31) 414.49 120.02 T
9 F
(9) 488.36 120.02 T
0 F
(< 31) 409.21 107.02 T
9 F
(7) 488.36 107.02 T
57.8 490.89 57.8 231.14 2 L
V
0.25 H
0 Z
N
104.12 491.14 104.12 230.89 2 L
V
N
162 474.14 162 230.89 2 L
V
N
225 491.14 225 230.89 2 L
V
N
288 491.14 288 230.89 2 L
V
N
369 491.14 369 230.89 2 L
V
N
427.5 491.14 427.5 230.89 2 L
V
N
486 491.14 486 230.89 2 L
V
N
540 490.89 540 231.14 2 L
V
N
57.67 491.02 540.12 491.02 2 L
V
N
104 474.02 225.12 474.02 2 L
V
N
57.67 456.02 540.12 456.02 2 L
V
0.5 H
N
57.67 441.02 540.12 441.02 2 L
V
0.25 H
N
57.67 426.02 540.12 426.02 2 L
V
N
57.67 411.02 540.12 411.02 2 L
V
N
57.67 396.02 540.12 396.02 2 L
V
N
57.67 381.02 540.12 381.02 2 L
V
N
57.67 366.02 540.12 366.02 2 L
V
N
57.67 351.02 540.12 351.02 2 L
V
N
57.67 336.02 540.12 336.02 2 L
V
N
57.67 321.02 540.12 321.02 2 L
V
N
57.67 306.02 540.12 306.02 2 L
V
N
57.67 291.02 540.12 291.02 2 L
V
N
57.67 276.02 540.12 276.02 2 L
V
N
57.67 261.02 540.12 261.02 2 L
V
N
57.67 246.02 540.12 246.02 2 L
V
N
57.67 231.02 540.12 231.02 2 L
V
N
320.62 179.89 320.62 102.14 2 L
V
N
392.62 180.14 392.62 101.89 2 L
V
N
442.12 180.14 442.12 101.89 2 L
V
N
540 179.89 540 102.14 2 L
V
N
320.5 180.02 540.12 180.02 2 L
V
N
320.5 167.02 540.12 167.02 2 L
V
N
320.5 154.02 540.12 154.02 2 L
V
N
392.5 141.02 540.12 141.02 2 L
V
N
320.5 128.02 540.12 128.02 2 L
V
N
392.5 115.02 540.12 115.02 2 L
V
N
320.5 102.02 540.12 102.02 2 L
V
N
FMENDPAGE
%%EndPage: "92" 92
%%Page: "93" 93
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
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[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (93) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Reference T) 207 736.18 T
(ables for Instrument Performance) 257.85 736.18 T
54 671.02 540 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 672.52 540 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 672.52 180 672.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(8.5) 163.32 678.02 T
(The Effects of Reddening in the Ultraviolet) 189 678.02 T
0 10 Q
0.8 (The table above lists extinction from interstellar reddening at ultraviolet wavelengths.) 189 423.35 P
-0.23 (More information on the ef) 189 411.35 P
-0.23 (fects of reddening may be found in the bibliography in Chap-) 296.77 411.35 P
0.11 (ter 9. The above values are from Code et al. \0501976\051. Seaton \0501979\051 has provided conve-) 189 399.35 P
(nient \336ts to ultraviolet extinction for) 189 387.35 T
3 F
(x) 336.78 387.35 T
0 F
( =) 341.22 387.35 T
13 F
(1/l) 351.86 387.35 T
0 F
(, with) 365.13 387.35 T
13 F
(l) 390.41 387.35 T
0 F
( in microns:) 395.9 387.35 T
54 650.02 540 663.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 657.02 540 657.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 657.02 180 657.02 2 L
0 Z
N
0 0 612 792 C
2 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 644.02 T
(ABLE 8-7) 58.83 644.02 T
4 F
(A) 189 633.02 T
(verage normalized ultraviolet extinction as a function of wavelength.) 194.84 633.02 T
2 8 Q
(W) 231.77 609.68 T
(avelength \050\201\051) 239.02 609.68 T
8 9 Q
(A) 318.82 609.68 T
13 8 Q
(l) 324.82 607.18 T
6 F
(/E\050B-V\051) 329.22 609.68 T
2 F
(W) 385.04 609.68 T
(avelength \050\201\051) 392.29 609.68 T
8 9 Q
(A) 476.47 609.68 T
13 8 Q
(l) 482.47 607.18 T
6 F
(/E\050B-V\051) 486.86 609.68 T
0 9 Q
(1) 251.9 595.02 T
(100) 256.06 595.02 T
(1) 327.39 595.02 T
(1.70) 331.56 595.02 T
(2160) 405 595.02 T
(10.10) 484.88 595.02 T
(1200) 251.73 580.02 T
(10.20) 327.23 580.02 T
(2200) 405 580.02 T
(9.85) 487.12 580.02 T
(1300) 251.73 565.02 T
(9.19) 329.48 565.02 T
(2300) 405 565.02 T
(8.75) 487.12 565.02 T
(1400) 251.73 550.02 T
(8.54) 329.48 550.02 T
(2400) 405 550.02 T
(7.92) 487.12 550.02 T
(1500) 251.73 535.02 T
(8.29) 329.48 535.02 T
(2500) 405 535.02 T
(7.30) 487.12 535.02 T
(1600) 251.73 520.02 T
(8.03) 329.48 520.02 T
(2600) 405 520.02 T
(6.82) 487.12 520.02 T
(1700) 251.73 505.02 T
(7.85) 329.48 505.02 T
(2700) 405 505.02 T
(6.41) 487.12 505.02 T
(1800) 251.73 490.02 T
(7.90) 329.48 490.02 T
(2800) 405 490.02 T
(6.10) 487.12 490.02 T
(1900) 251.73 475.02 T
(8.38) 329.48 475.02 T
(2900) 405 475.02 T
(5.85) 487.12 475.02 T
(2000) 251.73 460.02 T
(9.05) 329.48 460.02 T
(3000) 405 460.02 T
(5.65) 487.12 460.02 T
(2100) 251.73 445.02 T
(9.90) 329.48 445.02 T
(3300) 405 445.02 T
(5.16) 487.12 445.02 T
3 10 Q
(x) 205.93 342.35 T
0 F
( range) 210.37 342.35 T
3 F
(X\050x\051 = A) 372.26 342.35 T
13 8 Q
(l) 407.33 339.85 T
3 10 Q
(/E\050B\320V\051) 411.72 342.35 T
0 9 Q
(2.70) 170.25 321.02 T
13 F
(\243) 188.25 321.02 T
3 F
(x) 195.44 321.02 T
13 F
(\243) 201.69 321.02 T
0 F
( 3.65) 206.63 321.02 T
(3.65) 170.25 299.02 T
13 F
( \243) 186 299.02 T
3 F
(x) 195.44 299.02 T
13 F
(\243) 201.69 299.02 T
0 F
( 7.14) 206.63 299.02 T
(7.14) 170.25 277.02 T
13 F
(\243) 188.25 277.02 T
3 F
(x) 195.44 277.02 T
13 F
(\243) 201.69 277.02 T
0 F
( 10) 206.63 277.02 T
224.76 621.89 224.76 440.14 2 L
V
0.25 H
0 Z
N
296.7 622.14 296.7 559.89 2 L
V
N
296.7 560.14 296.7 544.89 2 L
V
0.5 H
N
296.7 545.14 296.7 439.89 2 L
V
0.25 H
N
378 622.14 378 439.77 2 L
V
2 H
N
450 622.14 450 439.77 2 L
V
0.25 H
N
540 621.89 540 440.14 2 L
V
N
224.63 622.02 540.12 622.02 2 L
V
N
224.63 605.02 540.12 605.02 2 L
V
0.5 H
N
224.63 590.02 540.12 590.02 2 L
V
0.25 H
N
224.63 575.02 540.12 575.02 2 L
V
N
224.63 560.02 540.12 560.02 2 L
V
N
224.63 545.02 540.12 545.02 2 L
V
N
224.63 530.02 540.12 530.02 2 L
V
N
224.63 515.02 540.12 515.02 2 L
V
N
224.63 500.02 540.12 500.02 2 L
V
N
224.63 485.02 540.12 485.02 2 L
V
N
224.63 470.02 540.12 470.02 2 L
V
N
224.63 455.02 379 455.02 2 L
V
N
377 455.02 450.12 455.02 2 L
V
0.5 H
N
449.88 455.02 540.12 455.02 2 L
V
0.25 H
N
224.63 440.02 377 440.02 2 L
V
N
379 440.02 449.88 440.02 2 L
V
0.5 H
N
450.12 440.02 540.12 440.02 2 L
V
0.25 H
N
164.25 356.89 164.25 267.14 2 L
V
N
276.75 357.14 276.75 266.89 2 L
V
N
540 356.89 540 267.14 2 L
V
N
164.12 357.02 540.12 357.02 2 L
V
N
164.12 333.02 540.12 333.02 2 L
V
0.5 H
N
164.12 311.02 540.12 311.02 2 L
V
0.25 H
N
164.12 289.02 540.12 289.02 2 L
V
N
164.12 267.02 540.12 267.02 2 L
V
N
282.75 314.77 449.78 328.03 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 9 Q
0 X
0 0 0 1 0 0 0 K
(1) 283.53 319.02 T
(.) 288.03 319.02 T
(5) 290.28 319.02 T
(6) 294.78 319.02 T
(1) 308.85 319.02 T
(.) 313.35 319.02 T
(0) 315.6 319.02 T
(4) 320.1 319.02 T
(8) 324.6 319.02 T
3 F
(x) 329.63 319.02 T
0 F
(1) 343.2 319.02 T
(.) 347.7 319.02 T
(0) 349.95 319.02 T
(1) 354.45 319.02 T
3 F
(x) 375.67 319.02 T
0 F
(4) 388.66 319.02 T
(.) 393.16 319.02 T
(6) 395.41 319.02 T
(0) 399.91 319.02 T
(\320) 381.91 319.02 T
13 F
(\050) 371.81 319.02 T
(\051) 404.82 319.02 T
0 7 Q
(2) 409.77 321.78 T
0 9 Q
(0) 422.84 319.02 T
(.) 427.34 319.02 T
(2) 429.59 319.02 T
(8) 434.09 319.02 T
(0) 438.59 319.02 T
(+) 415.52 319.02 T
13 F
([) 366.45 319.02 T
(]) 443.5 319.02 T
(\244) 361.2 319.02 T
0 F
(+) 301.53 319.02 T
(+) 335.88 319.02 T
0 0 612 792 C
282.75 292.77 449.78 306.03 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 9 Q
0 X
0 0 0 1 0 0 0 K
(2) 283.53 297.02 T
(.) 288.03 297.02 T
(2) 290.28 297.02 T
(9) 294.78 297.02 T
(0) 308.85 297.02 T
(.) 313.35 297.02 T
(8) 315.6 297.02 T
(4) 320.1 297.02 T
(8) 324.6 297.02 T
3 F
(x) 329.63 297.02 T
0 F
(1) 343.2 297.02 T
(.) 347.7 297.02 T
(0) 349.95 297.02 T
(1) 354.45 297.02 T
3 F
(x) 375.67 297.02 T
0 F
(4) 388.66 297.02 T
(.) 393.16 297.02 T
(6) 395.41 297.02 T
(0) 399.91 297.02 T
(\320) 381.91 297.02 T
13 F
(\050) 371.81 297.02 T
(\051) 404.82 297.02 T
0 7 Q
(2) 409.77 299.78 T
0 9 Q
(0) 422.84 297.02 T
(.) 427.34 297.02 T
(2) 429.59 297.02 T
(8) 434.09 297.02 T
(0) 438.59 297.02 T
(+) 415.52 297.02 T
13 F
([) 366.45 297.02 T
(]) 443.5 297.02 T
(\244) 361.2 297.02 T
0 F
(+) 301.53 297.02 T
(+) 335.88 297.02 T
0 0 612 792 C
282.75 270.77 377.63 284.03 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 9 Q
0 X
0 0 0 1 0 0 0 K
(1) 283.53 275.02 T
(6) 288.03 275.02 T
(.) 292.53 275.02 T
(1) 294.78 275.02 T
(7) 299.28 275.02 T
(3) 312.78 275.02 T
(.) 317.28 275.02 T
(2) 319.53 275.02 T
(0) 324.03 275.02 T
3 F
(x) 329.06 275.02 T
0 F
(\320) 306.03 275.02 T
(0) 342.62 275.02 T
(.) 347.12 275.02 T
(2) 349.37 275.02 T
(9) 353.87 275.02 T
(7) 358.37 275.02 T
(5) 362.87 275.02 T
3 F
(x) 367.9 275.02 T
0 7 Q
(2) 372.35 277.78 T
0 9 Q
(+) 335.3 275.02 T
0 0 612 792 C
FMENDPAGE
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7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(94) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 671.02 540 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 672.52 540 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 672.52 180 672.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(8.6) 163.32 678.02 T
(Instrumental Properties) 189 678.02 T
2 10 Q
(8.6.1) 157.76 644.35 T
(The Point Spread Function) 189 644.35 T
0 F
0.71 (The illustration below shows the PSF for the GHRS after the installation of the COS-) 189 624.35 P
0.24 (T) 189 612.35 P
0.24 (AR mirrors, to allow for estimation of the degree of scattered light in the vicinity of a) 194.31 612.35 P
0.95 (bright object. Note that this PSF is only one-dimensional, and was only measured on) 189 600.35 P
0.59 (one side of the center of the aperture at that; in fact the true PSF has two-dimensional) 189 588.35 P
0.34 (structure. The relative throughput of the SSA at the wavelength at which this measure-) 189 576.35 P
(ment was done \0501450 \201\051 is 0.55.) 189 564.35 T
2 F
1.79 (Figure 8-7.) 126 228.33 P
4 F
1.79 (Normalized Point Spread Function for the GHRS. The upper) 187.49 228.33 P
0.36 (curve is for the LSA and the lower for the SSA, both normalized to 1.0 at the) 126 216.33 P
(origin.) 126 204.33 T
54 87.98 540 686.02 C
54 244 540 546.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
270 35 25 549 744 287.83 402.63 153.08 193.69 FMBEGINEPSF
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1986 2947 d 2050 3100 r 2018 3100 d 2090 498 r 2092 492 d 2098 488 d
2108 486 d 2114 486 d 2124 488 d 2130 492 d 2132 498 d 2132 502 d
2130 508 d 2124 512 d 2114 514 d 2108 514 d 2098 512 d 2092 508 d
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2100 1100 r 2098 1100 d 2094 1102 d 2092 1104 d 2090 1108 d 2090 1116 d
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214 2641 d 150 2794 r 182 2794 d 150 2947 r 214 2947 d 150 3100 r
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1898 418 d 1896 420 d 1894 418 d 1856 446 r 1858 440 d 1864 436 d
1874 434 d 1880 434 d 1890 436 d 1896 440 d 1898 446 d 1898 450 d
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1856 450 d 1856 446 d 1541 324 r 1541 360 d 1517 394 r 1545 374 d
1545 404 d 1517 394 r 1559 394 d 1555 418 r 1557 416 d 1559 418 d
1557 420 d 1555 418 d 1517 446 r 1519 440 d 1525 436 d 1535 434 d
1541 434 d 1551 436 d 1557 440 d 1559 446 d 1559 450 d 1557 456 d
1551 460 d 1541 462 d 1535 462 d 1525 460 d 1519 456 d 1517 450 d
1517 446 d 1202 324 r 1202 360 d 1178 378 r 1178 400 d 1194 388 d
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1218 396 d 1220 390 d 1220 384 d 1218 378 d 1216 376 d 1212 374 d
1216 418 r 1218 416 d 1220 418 d 1218 420 d 1216 418 d 1178 446 r
1180 440 d 1186 436 d 1196 434 d 1202 434 d 1212 436 d 1218 440 d
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1186 460 d 1180 456 d 1178 450 d 1178 446 d 863 324 r 863 360 d
849 376 r 847 376 d 843 378 d 841 380 d 839 384 d 839 392 d
841 396 d 843 398 d 847 400 d 851 400 d 855 398 d 861 394 d
881 374 d 881 402 d 877 418 r 879 416 d 881 418 d 879 420 d
877 418 d 839 446 r 841 440 d 847 436 d 857 434 d 863 434 d
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863 462 d 857 462 d 847 460 d 841 456 d 839 450 d 839 446 d
523 324 r 523 360 d 507 380 r 505 384 d 499 390 d 541 390 d
537 418 r 539 416 d 541 418 d 539 420 d 537 418 d 499 446 r
501 440 d 507 436 d 517 434 d 523 434 d 533 436 d 539 440 d
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507 460 d 501 456 d 499 450 d 499 446 d 160 386 r 162 380 d
168 376 d 178 374 d 184 374 d 194 376 d 200 380 d 202 386 d
202 390 d 200 396 d 194 400 d 184 402 d 178 402 d 168 400 d
162 396 d 160 390 d 160 386 d 198 418 r 200 416 d 202 418 d
200 420 d 198 418 d 160 446 r 162 440 d 168 436 d 178 434 d
184 434 d 194 436 d 200 440 d 202 446 d 202 450 d 200 456 d
194 460 d 184 462 d 178 462 d 168 460 d 162 456 d 160 450 d
160 446 d 2050 3100 r 150 3100 d 2050 3100 r 2050 3068 d 1880 3100 r
1880 3036 d 1711 3100 r 1711 3068 d 1541 3100 r 1541 3036 d 1371 3100 r
1371 3068 d 1202 3100 r 1202 3036 d 1032 3100 r 1032 3068 d 863 3100 r
863 3036 d 693 3100 r 693 3068 d 523 3100 r 523 3036 d 354 3100 r
354 3068 d 184 3100 r 184 3036 d 2206 1479 r 2209 1473 d 2215 1467 d
2221 1464 d 2230 1461 d 2245 1461 d 2254 1464 d 2260 1467 d 2266 1473 d
2269 1479 d 2269 1491 d 2266 1497 d 2260 1503 d 2254 1506 d 2245 1509 d
2230 1509 d 2221 1506 d 2215 1503 d 2209 1497 d 2206 1491 d 2206 1479 d
2206 1548 r 2206 1542 d 2209 1536 d 2218 1533 d 2269 1533 d 2227 1524 r
2227 1545 d 2206 1578 r 2206 1572 d 2209 1566 d 2218 1563 d 2269 1563 d
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2260 1638 d 2266 1644 d 2269 1650 d 2269 1659 d 2266 1665 d 2260 1671 d
2206 1695 r 2257 1695 d 2266 1698 d 2269 1704 d 2269 1710 d 2227 1686 r
2227 1707 d 2194 1791 r 2200 1785 d 2209 1779 d 2221 1773 d 2236 1770 d
2248 1770 d 2263 1773 d 2275 1779 d 2284 1785 d 2290 1791 d 2227 1845 r
2269 1845 d 2236 1845 r 2230 1839 d 2227 1833 d 2227 1824 d 2230 1818 d
2236 1812 d 2245 1809 d 2251 1809 d 2260 1812 d 2266 1818 d 2269 1824 d
2269 1833 d 2266 1839 d 2260 1845 d 2227 1866 r 2269 1866 d 2245 1866 r
2236 1869 d 2230 1875 d 2227 1881 d 2227 1890 d 2236 1941 r 2230 1935 d
2227 1929 d 2227 1920 d 2230 1914 d 2236 1908 d 2245 1905 d 2251 1905 d
2260 1908 d 2266 1914 d 2269 1920 d 2269 1929 d 2266 1935 d 2260 1941 d
2236 1992 r 2230 1989 d 2227 1980 d 2227 1971 d 2230 1962 d 2236 1959 d
2242 1962 d 2245 1968 d 2248 1983 d 2251 1989 d 2257 1992 d 2260 1992 d
2266 1989 d 2269 1980 d 2269 1971 d 2266 1962 d 2260 1959 d 2245 2007 r
2245 2043 d 2239 2043 d 2233 2040 d 2230 2037 d 2227 2031 d 2227 2022 d
2230 2016 d 2236 2010 d 2245 2007 d 2251 2007 d 2260 2010 d 2266 2016 d
2269 2022 d 2269 2031 d 2266 2037 d 2260 2043 d 2236 2097 r 2230 2091 d
2227 2085 d 2227 2076 d 2230 2070 d 2236 2064 d 2245 2061 d 2251 2061 d
2260 2064 d 2266 2070 d 2269 2076 d 2269 2085 d 2266 2091 d 2260 2097 d
2194 2115 r 2200 2121 d 2209 2127 d 2221 2133 d 2236 2136 d 2248 2136 d
2263 2133 d 2275 2127 d 2284 2121 d 2290 2115 d 1550 104 r 1550 167 d
1514 125 r 1520 128 d 1526 134 d 1529 143 d 1529 149 d 1526 158 d
1520 164 d 1514 167 d 1505 167 d 1499 164 d 1493 158 d 1490 149 d
1490 143 d 1493 134 d 1499 128 d 1505 125 d 1514 125 d 1439 125 r
1439 173 d 1442 182 d 1445 185 d 1451 188 d 1460 188 d 1466 185 d
1439 134 r 1445 128 d 1451 125 d 1460 125 d 1466 128 d 1472 134 d
1475 143 d 1475 149 d 1472 158 d 1466 164 d 1460 167 d 1451 167 d
1445 164 d 1439 158 d 1370 125 r 1370 167 d 1370 143 r 1367 134 d
1361 128 d 1355 125 d 1346 125 d 1331 143 r 1295 143 d 1295 137 d
1298 131 d 1301 128 d 1307 125 d 1316 125 d 1322 128 d 1328 134 d
1331 143 d 1331 149 d 1328 158 d 1322 164 d 1316 167 d 1307 167 d
1301 164 d 1295 158 d 1274 104 r 1274 167 d 1217 125 r 1217 167 d
1217 134 r 1223 128 d 1229 125 d 1238 125 d 1244 128 d 1250 134 d
1253 143 d 1253 149 d 1250 158 d 1244 164 d 1238 167 d 1229 167 d
1223 164 d 1217 158 d 1193 104 r 1193 155 d 1190 164 d 1184 167 d
1178 167 d 1202 125 r 1181 125 d 1169 104 r 1166 107 d 1163 104 d
1166 101 d 1169 104 d 1166 125 r 1166 167 d 1148 125 r 1130 167 d
1112 125 r 1130 167 d 1097 143 r 1061 143 d 1061 137 d 1064 131 d
1067 128 d 1073 125 d 1082 125 d 1088 128 d 1094 134 d 1097 143 d
1097 149 d 1094 158 d 1088 164 d 1082 167 d 1073 167 d 1067 164 d
1061 158 d 995 104 r 992 107 d 989 104 d 992 101 d 995 104 d
992 125 r 992 167 d 968 125 r 968 167 d 968 137 r 959 128 d
953 125 d 944 125 d 938 128 d 935 137 d 935 167 d 911 104 r
911 155 d 908 164 d 902 167 d 896 167 d 920 125 r 899 125 d
887 143 r 851 143 d 851 137 d 854 131 d 857 128 d 863 125 d
872 125 d 878 128 d 884 134 d 887 143 d 887 149 d 884 158 d
878 164 d 872 167 d 863 167 d 857 164 d 851 158 d 830 125 r
830 167 d 830 137 r 821 128 d 815 125 d 806 125 d 800 128 d
797 137 d 797 167 d 746 134 r 749 128 d 758 125 d 767 125 d
776 128 d 779 134 d 776 140 d 770 143 d 755 146 d 749 149 d
746 155 d 746 158 d 749 164 d 758 167 d 767 167 d 776 164 d
779 158 d 731 104 r 728 107 d 725 104 d 728 101 d 731 104 d
728 125 r 728 167 d 701 104 r 701 155 d 698 164 d 692 167 d
686 167 d 710 125 r 689 125 d 680 125 r 662 167 d 644 125 r
662 167 d 668 179 d 674 185 d 680 188 d 683 188 d 201 505 r
201 500 d 200 507 r 200 500 d 199 510 r 199 500 d 198 511 r
198 500 d 197 512 r 197 500 d 196 513 r 196 500 d 195 514 r
195 500 d 194 515 r 194 500 d 193 516 r 193 500 d 192 516 r
192 500 d 191 516 r 191 500 d 190 517 r 190 500 d 189 517 r
189 500 d 188 517 r 188 500 d 187 518 r 187 500 d 186 518 r
186 500 d 185 518 r 185 500 d 184 518 r 184 500 d 183 518 r
183 500 d 182 517 r 182 500 d 181 517 r 181 500 d 180 517 r
180 500 d 179 517 r 179 500 d 178 517 r 178 500 d 177 516 r
177 500 d 176 516 r 176 500 d 175 515 r 175 500 d 174 515 r
174 500 d 173 514 r 173 500 d 172 513 r 172 500 d 171 512 r
171 500 d 170 511 r 170 500 d 169 509 r 169 500 d 168 508 r
168 500 d 167 505 r 167 500 d 166 500 p 588 811 r 588 801 d
587 813 r 587 799 d 586 816 r 586 796 d 585 817 r 585 795 d
584 818 r 584 794 d 583 819 r 583 793 d 582 820 r 582 792 d
581 821 r 581 791 d 580 822 r 580 790 d 579 822 r 579 790 d
578 822 r 578 790 d 577 823 r 577 789 d 576 823 r 576 789 d
575 823 r 575 789 d 574 824 r 574 788 d 573 824 r 573 788 d
572 824 r 572 788 d 571 824 r 571 788 d 570 824 r 570 788 d
569 823 r 569 789 d 568 823 r 568 789 d 567 823 r 567 789 d
566 823 r 566 789 d 565 823 r 565 789 d 564 822 r 564 790 d
563 822 r 563 790 d 562 821 r 562 791 d 561 821 r 561 791 d
560 820 r 560 792 d 559 819 r 559 793 d 558 818 r 558 794 d
557 817 r 557 795 d 556 815 r 556 797 d 555 814 r 555 798 d
554 811 r 554 801 d 553 806 p 1088 1117 r 1088 1107 d 1087 1119 r
1087 1105 d 1086 1122 r 1086 1102 d 1085 1123 r 1085 1101 d 1084 1124 r
1084 1100 d 1083 1125 r 1083 1099 d 1082 1126 r 1082 1098 d 1081 1127 r
1081 1097 d 1080 1128 r 1080 1096 d 1079 1128 r 1079 1096 d 1078 1128 r
1078 1096 d 1077 1129 r 1077 1095 d 1076 1129 r 1076 1095 d 1075 1129 r
1075 1095 d 1074 1130 r 1074 1094 d 1073 1130 r 1073 1094 d 1072 1130 r
1072 1094 d 1071 1130 r 1071 1094 d 1070 1130 r 1070 1094 d 1069 1129 r
1069 1095 d 1068 1129 r 1068 1095 d 1067 1129 r 1067 1095 d 1066 1129 r
1066 1095 d 1065 1129 r 1065 1095 d 1064 1128 r 1064 1096 d 1063 1128 r
1063 1096 d 1062 1127 r 1062 1097 d 1061 1127 r 1061 1097 d 1060 1126 r
1060 1098 d 1059 1125 r 1059 1099 d 1058 1124 r 1058 1100 d 1057 1123 r
1057 1101 d 1056 1121 r 1056 1103 d 1055 1120 r 1055 1104 d 1054 1117 r
1054 1107 d 1053 1112 p 1425 1729 r 1425 1719 d 1424 1731 r 1424 1717 d
1423 1734 r 1423 1714 d 1422 1735 r 1422 1713 d 1421 1736 r 1421 1712 d
1420 1737 r 1420 1711 d 1419 1738 r 1419 1710 d 1418 1739 r 1418 1709 d
1417 1740 r 1417 1708 d 1416 1740 r 1416 1708 d 1415 1740 r 1415 1708 d
1414 1741 r 1414 1707 d 1413 1741 r 1413 1707 d 1412 1741 r 1412 1707 d
1411 1742 r 1411 1706 d 1410 1742 r 1410 1706 d 1409 1742 r 1409 1706 d
1408 1742 r 1408 1706 d 1407 1742 r 1407 1706 d 1406 1741 r 1406 1707 d
1405 1741 r 1405 1707 d 1404 1741 r 1404 1707 d 1403 1741 r 1403 1707 d
1402 1741 r 1402 1707 d 1401 1740 r 1401 1708 d 1400 1740 r 1400 1708 d
1399 1739 r 1399 1709 d 1398 1739 r 1398 1709 d 1397 1738 r 1397 1710 d
1396 1737 r 1396 1711 d 1395 1736 r 1395 1712 d 1394 1735 r 1394 1713 d
1393 1733 r 1393 1715 d 1392 1732 r 1392 1716 d 1391 1729 r 1391 1719 d
1390 1724 p 1650 2952 r 1650 2942 d 1649 2954 r 1649 2940 d 1648 2957 r
1648 2937 d 1647 2958 r 1647 2936 d 1646 2959 r 1646 2935 d 1645 2960 r
1645 2934 d 1644 2961 r 1644 2933 d 1643 2962 r 1643 2932 d 1642 2963 r
1642 2931 d 1641 2963 r 1641 2931 d 1640 2963 r 1640 2931 d 1639 2964 r
1639 2930 d 1638 2964 r 1638 2930 d 1637 2964 r 1637 2930 d 1636 2965 r
1636 2929 d 1635 2965 r 1635 2929 d 1634 2965 r 1634 2929 d 1633 2965 r
1633 2929 d 1632 2965 r 1632 2929 d 1631 2964 r 1631 2930 d 1630 2964 r
1630 2930 d 1629 2964 r 1629 2930 d 1628 2964 r 1628 2930 d 1627 2964 r
1627 2930 d 1626 2963 r 1626 2931 d 1625 2963 r 1625 2931 d 1624 2962 r
1624 2932 d 1623 2962 r 1623 2932 d 1622 2961 r 1622 2933 d 1621 2960 r
1621 2934 d 1620 2959 r 1620 2935 d 1619 2958 r 1619 2936 d 1618 2956 r
1618 2938 d 1617 2955 r 1617 2939 d 1616 2952 r 1616 2942 d 1615 2947 p
184 500 r 571 806 d 1071 1112 d 1408 1724 d 1633 2947 d 197 513 r
171 513 d 171 500 d 197 500 r 197 513 d 714 574 r 688 574 d
688 548 d 714 548 d 714 574 d 865 635 r 839 635 d 839 609 d
865 609 d 865 635 d 1244 758 r 1218 758 d 1218 732 d 1244 732 d
1244 758 d 1558 1002 r 1532 1002 d 1532 976 d 1558 976 d 1558 1002 d
2032 1492 r 2006 1492 d 2006 1466 d 2032 1466 d 2032 1492 d 184 500 r
701 561 d 852 622 d 1231 745 d 1545 989 d 2019 1479 d
e
%%Trailer
EndPSPlot

%%EndDocument
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54 87.98 540 686.02 C
0 0 612 792 C
FMENDPAGE
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%%Page: "95" 95
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (95) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Reference T) 207 736.18 T
(ables for Instrument Performance) 257.85 736.18 T
2 10 Q
(8.6.2) 157.76 679.35 T
(Detector Dark Count and the CENSOR Option) 189 679.35 T
0 F
-0.24 (Each Digicon diode has its own discriminator) 189 659.35 P
-0.24 (, and if they are properly set the dark count) 369.94 659.35 P
0.3 (rate measured is very low) 189 647.35 P
0.3 (. On-orbit measurement has shown that both GHRS detectors) 292.32 647.35 P
0.61 (have a dark rate less than the design goal of 0.01 counts diode) 189 635.35 P
0 8 Q
0.48 (-1) 444.27 639.35 P
0 10 Q
0.61 ( sec) 450.93 635.35 P
0 8 Q
0.48 (-1) 466.81 639.35 P
0 10 Q
0.61 ( at low geomag-) 473.47 635.35 P
0.19 (netic latitudes and that the dominant noise source is cosmic rays. During SAA passage,) 189 623.35 P
0.53 (the noise increases to a maximum of about 1 count diode) 189 611.35 P
0 8 Q
0.43 (-1) 422.07 615.35 P
0 10 Q
0.53 ( sec) 428.73 611.35 P
0 8 Q
0.43 (-1) 444.53 615.35 P
0 10 Q
0.53 (. The scheduling soft-) 451.2 611.35 P
0.63 (ware for) 189 599.35 P
3 F
0.63 (HST) 226.35 599.35 P
0 F
0.63 ( uses known contours of the SAA and does not accumulate counts when) 244.13 599.35 P
(the spacecraft is within those contours.) 189 587.35 T
1.08 (Even outside the SAA, observations show that \322dark\323 counts tend to come in bursts.) 189 567.35 P
-0.06 (Approximately 15% of dark counts are produced by events that occur within a time of) 189 555.35 P
-0.06 (8) 535 555.35 P
13 F
0.48 (m) 189 543.35 P
0 F
0.48 (s or less. The) 194.76 543.35 P
9 F
1.15 ( CENSOR) 248.97 543.35 P
0 F
0.48 ( feature in Accumulation Mode allows you to ignore integra-) 292.12 543.35 P
1.09 (tions with such high dark rates.) 189 531.35 P
9 F
2.62 (CENSOR) 323.05 531.35 P
0 F
1.09 ( works by summing all 512 channels of the) 359.05 531.35 P
0.3 (Digicon every 8) 189 519.35 P
13 F
0.3 (m) 256.83 519.35 P
0 F
0.3 (s, and if that sum exceeds a threshold a coincident event is recorded.) 262.59 519.35 P
-0.05 (The \337ight software maintains a record of how many coincidence events occurred within) 189 507.35 P
-0.16 (a given) 189 495.35 P
9 F
-0.38 (STEP-TIME) 220.34 495.35 P
0 F
-0.16 ( and can reject and repeat a subexposure for which the coincidence) 274.34 495.35 P
0.38 (sum exceeds a speci\336ed level. The coincidence circuit reacts only to strong events that) 189 483.35 P
1.69 (trigger about 8 diodes simultaneously) 189 471.35 P
1.69 (, so that only the high-amplitude tail of back-) 345.66 471.35 P
1.1 (ground events can be rejected, even if the speci\336cation is to reject any) 189 459.35 P
9 F
2.64 (STEP-TIME) 486 459.35 P
0 F
1.06 (with a non-zero coincidence sum. It is estimated that use of) 189 447.35 P
9 F
2.54 (CENSOR) 440.58 447.35 P
0 F
1.06 ( can reduce the) 476.58 447.35 P
0.29 (dark count rate by about 20%. Using) 189 435.35 P
9 F
0.71 (CENSOR=YES) 340.48 435.35 P
0 F
0.29 ( is unlikely to degrade an observa-) 400.48 435.35 P
0.33 (tion \050unless the object is bright enough to cause a consistently high count rate\051, but the) 189 423.35 P
(bene\336t is also low: only about a 10% gain in S/N in favorable cases.) 189 411.35 T
0.19 (The dark count rate is highly uniform over the diodes, so that a mean dark count rate is) 189 391.35 P
(an excellent representation of what happens at the detector) 189 379.35 T
(.) 422.83 379.35 T
(Summary:) 189 359.35 T
10 11 Q
(\245) 189 341.35 T
0 10 Q
0.73 (The pre-\337ight noise speci\336cation was 0.01 counts diode) 203.4 341.35 P
0 8 Q
0.59 (-1) 431.84 345.35 P
0 10 Q
0.73 ( sec) 438.5 341.35 P
0 8 Q
0.59 (-1) 454.51 345.35 P
0 10 Q
0.73 (. The average mea-) 461.17 341.35 P
(sured value is 0.005 for D1 and 0.008 for D2.) 203.4 329.35 T
10 11 Q
(\245) 189 314.35 T
0 10 Q
(The background is sensibly constant between \32020 and +20) 203.4 314.35 T
0 8 Q
(o) 437.34 318.35 T
0 10 Q
( geomagnetic latitude.) 441.34 314.35 T
10 11 Q
(\245) 189 299.35 T
0 10 Q
-0.17 (At) 203.4 299.35 P
13 F
-0.17 (\261) 215.73 299.35 P
0 F
-0.17 (40) 221.22 299.35 P
0 8 Q
-0.14 (o) 231.22 303.35 P
0 10 Q
-0.17 ( geomagnetic latitude, the extrema of) 235.22 299.35 P
3 F
-0.17 (HST) 385.55 299.35 P
0 F
-0.17 (\325) 403.33 299.35 P
-0.17 (s orbit, the rate is twice that at the) 406.11 299.35 P
0.9 (geomagnetic equator) 203.4 287.35 P
0.9 (. T) 287.34 287.35 P
0.9 (ypical average rates are 0.007 counts per diode per second) 298.65 287.35 P
(for D1 and 0.01) 203.4 275.35 T
(1 for D2.) 266.35 275.35 T
10 11 Q
(\245) 189 260.35 T
0 10 Q
-0.09 (The background rate is correlated with the cosmic ray and trapped particle \337ux. Cal-) 203.4 260.35 P
0.05 (culations show that the dark noise can be accounted for by cosmic-ray-induced Cer-) 203.4 248.35 P
(enkov radiation in the faceplates of the Digicons.) 203.4 236.35 T
10 11 Q
(\245) 189 221.35 T
0 10 Q
0.16 (The background due to the direct penetration of cosmic rays into diodes is very low) 203.4 221.35 P
(\0500.0004 counts diode) 203.4 209.35 T
0 8 Q
(-1) 287.56 213.35 T
0 10 Q
( sec) 294.22 209.35 T
0 8 Q
(-1) 309.49 213.35 T
0 10 Q
(\051.) 316.16 209.35 T
(When using) 189 189.35 T
9 F
(CENSOR) 239.55 189.35 T
0 F
(:) 275.55 189.35 T
10 11 Q
(\245) 189 171.35 T
0 10 Q
(Use the default) 203.4 171.35 T
9 F
(STEP-TIME) 266.44 171.35 T
0 F
(of 0.2 sec.) 326.44 171.35 T
10 11 Q
(\245) 189 156.35 T
0 10 Q
0.05 (Do not use) 203.4 156.35 P
9 F
0.12 (CENSOR) 249.37 156.35 P
0 F
0.05 ( if the expected count rate exceeds about 100 counts per second) 285.37 156.35 P
0.54 (per diode because real photon events will be rejected. In a severe case, all the data) 203.4 144.35 P
(could be lost.) 203.4 132.35 T
10 11 Q
(\245) 189 117.35 T
0 10 Q
1.06 (Using) 203.4 117.35 P
9 F
2.54 (CENSOR) 230.85 117.35 P
0 F
1.06 ( can drop the noise level by about 20%. The nominal Side 2 dark) 266.85 117.35 P
0.9 (count rate is 0.01) 203.4 105.35 P
0.9 (1 counts per second per diode, so) 274.6 105.35 P
9 F
2.15 (CENSOR=YES) 416.42 105.35 P
0 F
0.9 ( can lower it to) 476.42 105.35 P
(0.0088.) 203.4 93.35 T
FMENDPAGE
%%EndPage: "95" 95
%%Page: "96" 96
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
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[ 1 0 1 0 0 1 0]
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[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(96) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
10 11 Q
(\245) 189 679.35 T
0 10 Q
-0.01 (The following table shows the expected ef) 203.4 679.35 P
-0.01 (fects of using) 372.58 679.35 P
9 F
-0.02 (CENSOR) 428.93 679.35 P
0 F
-0.01 (.) 464.93 679.35 P
4 F
-0.01 (Rate) 469.92 679.35 P
0 F
-0.01 ( is the tar) 491.05 679.35 P
-0.01 (get) 527.78 679.35 P
0.2 (count rate per diode per second; the second column shows the standard S/N and the) 203.4 667.35 P
1.19 (third column lists the S/N achieved with) 203.4 655.35 P
9 F
2.85 (CENSOR=YES) 375.32 655.35 P
0 F
1.19 ( if the dark is 80% of its) 435.32 655.35 P
1.1 (value without) 203.4 643.35 P
9 F
2.63 (CENSOR) 262.81 643.35 P
0 F
1.1 (. Signal-to-noise was calculated on a per diode basis for a) 298.81 643.35 P
0.37 (nominal exposure time of 10,000 seconds \050which is reduced to 9,800 if) 203.4 415.35 P
9 F
0.89 (CENSOR) 494.46 415.35 P
0 F
0.37 ( is) 530.46 415.35 P
(used because of the loss of 2% of the exposures\051.) 203.4 403.35 T
-0.1 (Note that for rates exceeding one per second the ef) 203.4 388.35 P
-0.1 (fective loss of exposure time \050due) 405.27 388.35 P
0.15 (to 2% of the exposures being rejected\051 more than of) 203.4 376.35 P
0.15 (fsets any reduction of the noise.) 412.04 376.35 P
0.41 (At a rate of 0.1) 203.4 364.35 P
9 F
0.98 (CENSOR) 268.21 364.35 P
0 F
0.41 ( has essentially no ef) 304.21 364.35 P
0.41 (fect on S/N but for lower rates) 388.99 364.35 P
9 F
0.98 (CEN-) 516 364.35 P
(SOR) 203.4 352.35 T
0 F
( can help.) 221.4 352.35 T
54 615.02 540 628.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 622.02 540 622.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 622.02 180 622.02 2 L
0 Z
N
0 0 612 792 C
2 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 609.02 T
(ABLE 8-8) 58.83 609.02 T
4 F
(Ef) 189 609.02 T
(fects of CENSOR) 197.34 609.02 T
(Rate) 249.25 586.02 T
(Standard S/N) 335.24 586.02 T
(S/N with CENSOR=YES) 428.11 586.02 T
0 F
(100) 252 565.02 T
(999.94) 349.88 565.02 T
(989.91) 464.62 565.02 T
(10) 254.25 546.02 T
(316.05) 349.88 546.02 T
(312.91) 464.62 546.02 T
(1) 256.5 527.02 T
(99.45) 352.12 527.02 T
(98.56) 466.88 527.02 T
(0.1) 253.12 508.02 T
(30.02) 352.12 508.02 T
(30.01) 466.88 508.02 T
(0.01) 250.88 489.02 T
(6.90) 354.38 489.02 T
(7.22) 469.12 489.02 T
(0.005) 248.62 470.02 T
(3.95) 354.38 470.02 T
(4.21) 469.12 470.02 T
(0.001) 248.62 451.02 T
(0.91) 354.38 451.02 T
(1.00) 469.12 451.02 T
207 599.89 207 444.14 2 L
V
0.25 H
0 Z
N
310.5 600.14 310.5 443.89 2 L
V
N
414 600.14 414 443.89 2 L
V
N
540 599.89 540 444.14 2 L
V
N
206.88 600.02 540.12 600.02 2 L
V
N
206.88 577.02 540.12 577.02 2 L
V
0.5 H
N
206.88 558.02 540.12 558.02 2 L
V
0.25 H
N
206.88 539.02 540.12 539.02 2 L
V
N
206.88 520.02 540.12 520.02 2 L
V
N
206.88 501.02 540.12 501.02 2 L
V
N
206.88 482.02 540.12 482.02 2 L
V
N
206.88 463.02 540.12 463.02 2 L
V
N
206.88 444.02 540.12 444.02 2 L
V
N
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
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[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (97) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Reference T) 207 736.18 T
(ables for Instrument Performance) 257.85 736.18 T
2 10 Q
(8.6.3) 157.76 679.35 T
(Noise Rejection with FL) 189 679.35 T
(YLIM) 300.88 679.35 T
9 F
1.19 (FLYLIM) 189 659.35 P
0 F
0.5 ( is a special commanding option for rejecting noise in cases where the source) 225 659.35 P
0.52 (signal is much weaker than the noise level. The idea is that as) 189 647.35 P
3 F
0.52 (HST) 444.6 647.35 P
0 F
0.52 ( circles the Earth it) 462.38 647.35 P
0.31 (\336nds itself in dif) 189 635.35 P
0.31 (ferent noise environments due to the changing magnetic \336eld, and that) 255.58 635.35 P
-0.08 (in\337uences the detected noise background. Also, the background noise occurs as discrete) 189 623.35 P
0.37 (events from radiation in the space environment. If the source count level is well below) 189 611.35 P
0.17 (the background noise, then spectra integrated over a suf) 189 599.35 P
0.17 (\336ciently short interval that con-) 413.21 599.35 P
1.25 (tain multiple counts are probably just noise, and should be rejected, whereas spectra) 189 587.35 P
0.43 (with single counts are more likely to contain real information. The rejected spectra are) 189 575.35 P
-0.22 (discarded, which wastes observing time, but there is a net gain in signal-to-noise. A test-) 189 563.35 P
-0.06 (in-principle run in 1993 showed that the net background rate could be reduced to as low) 189 551.35 P
2.3 (as 0.002 counts sec) 189 539.35 P
0 8 Q
1.84 (-1) 273.12 543.35 P
0 10 Q
2.3 ( diode) 279.78 539.35 P
0 8 Q
1.84 (-1) 306.8 543.35 P
0 10 Q
2.3 ( for the Side 2 detector) 313.47 539.35 P
2.3 (, which was a factor of four) 415.95 539.35 P
0.29 (improvement over the mean dark rate. This gain was achieved at the cost of the loss of) 189 527.35 P
(about 25% of the individual 0.2 second) 189 515.35 T
9 F
(STEP-TIME) 348.43 515.35 T
0 F
( integrations.) 402.43 515.35 T
1.26 (By \322special commanding\323 we mean that) 189 495.35 P
9 F
3.04 (FLYLIM) 360.45 495.35 P
0 F
1.26 ( is requested as a comment on the) 396.45 495.35 P
0.55 (Phase) 189 483.35 P
0.55 (II proposal, rather than as an optional parameter) 214.83 483.35 P
0.55 (. The normal scheduling system) 410.31 483.35 P
1.93 (cannot automatically invoke) 189 471.35 P
9 F
4.63 (FLYLIM) 310.61 471.35 P
0 F
1.93 (; manual intervention is necessary) 346.61 471.35 P
1.93 (. A detailed) 489.76 471.35 P
0.14 (description of) 189 459.35 P
9 F
0.34 (FLYLIM) 247.05 459.35 P
0 F
0.14 ( cannot be provided here, but if users believe that) 283.05 459.35 P
9 F
0.34 (FLYLIM) 484.14 459.35 P
0 F
0.14 ( may) 520.14 459.35 P
(be of help in their science program they should note the following:) 189 447.35 T
10 11 Q
(\245) 189 429.35 T
0 10 Q
0.28 (The use of the) 203.4 429.35 P
9 F
0.68 (FLYLIM) 263.97 429.35 P
0 F
0.28 ( parameter may not be assumed by the proposer but instead) 299.97 429.35 P
-0.13 (must be arranged in advance, i.e., before the Phase I proposal deadline, through con-) 203.4 417.35 P
1.89 (sultation with a GHRS Instrument Scientist. The T) 203.4 405.35 P
1.89 (AC will be made aware that) 418.62 405.35 P
9 F
(FLYLIM) 203.4 393.35 T
0 F
( may require additional resources to implement.) 239.4 393.35 T
10 11 Q
(\245) 189 378.35 T
0 10 Q
0.67 (If your program that uses) 203.4 378.35 P
9 F
1.61 (FLYLIM) 310.35 378.35 P
0 F
0.67 ( is approved, we will attempt to execute it on a) 346.35 378.35 P
(best ef) 203.4 366.35 T
(forts basis, but limited resources may prevent that.) 229.6 366.35 T
10 11 Q
(\245) 189 351.35 T
0 10 Q
1.07 (At the time this is written) 203.4 351.35 P
9 F
2.56 (FLYLIM) 314.24 351.35 P
0 F
1.07 ( has not been fully tested and its use is at the) 350.24 351.35 P
(observer) 203.4 339.35 T
(\325) 238.2 339.35 T
(s risk.) 240.98 339.35 T
FMENDPAGE
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(98) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
(8.6.4) 157.76 679.35 T
(Count Rate Linearity) 189 679.35 T
0 F
0.35 (Deviations from linearity in the way in which the Digicons count photons at high rates) 189 659.35 P
0.54 (were illustrated above in Figure) 189 647.35 P
0.54 (7-2 on page) 320.88 647.35 P
0.54 (71. The ef) 371.67 647.35 P
0.54 (fective deadtime for the GHRS) 413.4 647.35 P
0.93 (detectors has been measured to be 10.2) 189 635.35 P
13 F
0.93 (m) 354.36 635.35 P
0 F
0.93 (s for detector D1. The same value has been) 360.11 635.35 P
0.16 (assumed to hold for D2. Deviations from linearity are imperceptible below 10) 189 623.35 P
0 8 Q
0.13 (3) 502.36 627.35 P
0 10 Q
0.16 ( and can) 506.36 623.35 P
0.88 (be corrected to an accuracy of 1% up to a measured count rate of 20,000 \050in units of) 189 611.35 P
(counts diode) 189 599.35 T
0 8 Q
(-1) 239.83 603.35 T
0 10 Q
( s) 246.49 599.35 T
0 8 Q
(-1) 252.88 603.35 T
0 10 Q
(\051.) 259.55 599.35 T
2 F
(8.6.5) 157.76 569.35 T
(Image Stability) 189 569.35 T
0 F
-0.11 (The images formed by the Digicons are vulnerable to the ef) 189 549.35 P
-0.11 (fects of the Earth\325) 426.01 549.35 P
-0.11 (s magnetic) 497.06 549.35 P
-0.18 (\336eld. Over the course of a full orbit, the amplitude of the motion is about 50 microns per) 189 537.35 P
0.61 (Gauss for D2 \050about 15 microns peak-to-peak\051 and 10 microns per Gauss for D1. The) 189 525.35 P
0.21 (50 micron motion seen in D2 corresponds to the size of a diode. This geomagnetically-) 189 513.35 P
-0.22 (induced image motion \050\322GIMP\323\051, together with thermal ef) 189 501.35 P
-0.22 (fects, is the underlying reason) 421.16 501.35 P
(for breaking up long exposures into segments of no more than about 5 minutes each.) 189 489.35 T
2 F
(8.6.6) 157.76 459.35 T
(W) 189 459.35 T
(avelength Calibrations) 198.07 459.35 T
0 F
0.13 (The GHRS has two spectrum calibration lamps, although only lamp SC2 now operates.) 189 439.35 P
1.11 (Lamp SC1 should not be speci\336ed under any circumstances. Both are platinum-neon) 189 427.35 P
0.68 (hollow cathode lamps manufactured by W) 189 415.35 P
0.68 (estinghouse, providing a rich array of emis-) 361.26 415.35 P
-0.14 (sion lines throughout the ultraviolet region that the GHRS observes. The lines are bright) 189 403.35 P
0.51 (enough so that a 30 second exposure will yield a good comparison spectrum at almost) 189 391.35 P
0.5 (any wavelength, although longer times are needed at some echelle settings. The lamps) 189 379.35 P
0.17 (are designated) 189 367.35 P
9 F
0.41 (SC1) 249.32 367.35 P
0 F
0.17 ( and) 267.32 367.35 P
9 F
0.41 (SC2) 287.09 367.35 P
0 F
0.17 ( and are selected by using) 305.09 367.35 P
9 F
0.41 (WAVE) 411.64 367.35 P
0 F
0.17 ( as the tar) 435.64 367.35 P
0.17 (get speci\336cation) 474.56 367.35 P
0.5 (with) 189 355.35 P
9 F
1.2 (SC1) 209.78 355.35 P
0 F
0.5 ( or) 227.78 355.35 P
9 F
1.2 (SC2) 242.12 355.35 P
0 F
0.5 ( as the aperture. Each lamp, in fact, has its own aperture, of) 260.12 355.35 P
0.5 (fset from) 503.12 355.35 P
-0 (the two science apertures of the GHRS. SC2 forms its spectrum at the same) 189 343.35 P
3 F
-0 (y) 493.62 343.35 P
0 F
-0 ( de\337ection) 498.06 343.35 P
0.46 (as the SSA, but displaced in) 189 331.35 P
3 F
0.46 (x) 306.46 331.35 P
0 F
0.46 ( \050the direction of dispersion\051. SC1 is nearly aligned with) 310.9 331.35 P
0.17 (the SSA in) 189 319.35 P
3 F
0.17 (x) 235.35 319.35 P
0 F
0.17 ( but dif) 239.79 319.35 P
0.17 (fers in) 268.85 319.35 P
3 F
0.17 (y) 296.96 319.35 P
0 F
0.17 ( by about 130 de\337ection steps. The lamp apertures are each) 301.4 319.35 P
1.35 (67 microns square and they form Gaussian-shaped images with FWHM = 1.1 diode) 189 307.35 P
(widths.) 189 295.35 T
0.1 (A wavelength calibration exposure made with the star in the SSA may be contaminated) 189 275.35 P
-0.04 (by the stellar spectrum. This is because the SSA has no shutter and the fact that the SC2) 189 263.35 P
0.63 (aperture is in line with the SSA. This contamination is rarely a serious problem, how-) 189 251.35 P
0.58 (ever) 189 239.35 P
0.58 (, because it is possible to subtract the stellar component. Also, such exposures are) 205.81 239.35 P
1.38 (usually used to only con\336rm the zero-point of the spectrum and not to obtain a full) 189 227.35 P
(wavelength solution.) 189 215.35 T
(For a comprehensive listing of the platinum lines, see Reader et al. \0501990\051.) 189 195.35 T
2 9 Q
(8.6.6.1) 152.48 172.02 T
(Aperture Offsets) 189 172.02 T
0 10 Q
0.02 (The light from the spectrum calibration lamps does not enter the spectrograph along the) 189 151.35 P
0.08 (same path that starlight takes. This introduces a wavelength shift that must be corrected) 189 139.35 P
-0.21 (for in solving for the wavelength solution. The data reduction software incorporates cor-) 189 127.35 P
1.28 (rections that were determined during pre-\337ight ground testing \050new values are being) 189 115.35 P
(measured in Cycle 4\051.) 189 103.35 T
FMENDPAGE
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(99) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
2 9 Q
(8.6.6.2) 152.48 680.02 T
(Thermal Effects) 189 680.02 T
0 10 Q
0.59 (The image formed by the Digicons is also af) 189 659.35 P
0.59 (fected by the thermal environment within) 371.26 659.35 P
-0.04 (the GHRS, which in turn is in\337uenced by whatever electronics happen to be on or of) 189 647.35 P
-0.04 (f in) 526.43 647.35 P
0.76 (the GHRS and the other instruments. The temperature inside the GHRS can be moni-) 189 635.35 P
0.65 (tored and the image motion calibrated. This correction is also provided for in the data) 189 623.35 P
0.63 (reduction software. However) 189 611.35 P
0.63 (, this correction is applied only once to a given Exposure) 306.21 611.35 P
-0.23 (Logsheet line. W) 189 599.35 P
-0.23 (e recommend that the exposure times for individual Exposure Logsheet) 256.33 599.35 P
-0.07 (lines be kept shorter than about one hour as long as you do not encounter problems with) 189 587.35 P
(using too much on-board memory \050see Section) 189 575.35 T
(4.6 on page) 378.7 575.35 T
(47\051.) 427.58 575.35 T
2 9 Q
(8.6.6.3) 152.48 552.02 T
(Geomagnetic Effects) 189 552.02 T
0 10 Q
0.14 (As for overall image stability) 189 531.35 P
0.14 (, geomagnetic ef) 306.13 531.35 P
0.14 (fects in\337uence wavelength stability) 372.6 531.35 P
0.14 (. Long) 513.75 531.35 P
-0 (exposures should be divided into units of about 5 minutes each, the time over which the) 189 519.35 P
(wavelength scale does not change measurably) 189 507.35 T
(.) 372.47 507.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(100) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
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2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (101) 541.32 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
7 12 Q
1.2 (Chapter 9) 72 677 S
5 24 Q
-0.48 (GHRS Bibliography) 207 677 S
4 12 Q
(9.1) 144 424 T
( Ultraviolet Extinction) 164.02 424 T
8 F
( 102) 498.65 424 T
4 F
(9.2) 144 406 T
( GHRS-Related T) 164.02 406 T
(echnical Papers) 256.7 406 T
8 F
( 102) 498.65 406 T
4 F
(9.3) 144 388 T
( GHRS Scienti\336c Papers) 164.02 388 T
8 F
( 104) 498.65 388 T
4 F
(9.4) 144 370 T
( Acknowledgments) 164.02 370 T
8 F
( 109) 498.65 370 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(GHRS Bibliography) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(102) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
1.45 (W) 189 679.35 P
1.45 (e have tried to make this) 197.64 679.35 P
3 F
1.45 (Handbook) 306.86 679.35 P
0 F
1.45 ( a comprehensive guide to using the Goddard) 348.52 679.35 P
0.39 (High Resolution Spectrograph, but some of the best information on the instrument and) 189 667.35 P
-0.2 (the uses to which it can be put can be found in the open literature. Here we provide three) 189 655.35 P
0.45 (lists. The \336rst provides additional information on interstellar reddening in the ultravio-) 189 643.35 P
0.32 (let. The next is technically oriented, and gives papers that provide detailed information) 189 631.35 P
1.29 (on speci\336c aspects of the GHRS. The \336nal list is of scienti\336c papers that have used) 189 619.35 P
(GHRS data.) 189 607.35 T
54 564.02 540 567.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 565.52 540 565.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 565.52 180 565.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(9.1) 163.32 571.02 T
(Ultraviolet Extinction) 189 571.02 T
3 10 Q
1.26 (\322Ultraviolet Photometry fr) 189 547.35 P
1.26 (om the Orbiting Astr) 298.93 547.35 P
1.26 (onomical Observatory) 385.4 547.35 P
1.26 (. II. Interstellar) 475.82 547.35 P
(Extinction.\323) 198 535.35 T
4 9 Q
(Bless, R.C., and Savage, B.D. 1972, ApJ, 171, 293\320308.) 207 518.02 T
3 10 Q
-0.15 (\322Studies of Ultraviolet Interstellar Extinction with the Sky-survey T) 189 498.35 P
-0.15 (elescope of the TD-1) 457.42 498.35 P
(Satellite.\323) 198 486.35 T
4 9 Q
0.77 (Nandy) 207 469.02 P
0.77 (, K., Thompson, G.I., Jamar) 232.34 469.02 P
0.77 (, C., Mon\336ls, A., and Wilson, R. 1976, A&A, 51,) 345.48 469.02 P
(63\32069.) 216 458.02 T
3 10 Q
(\322Empirical Effective T) 189 438.35 T
(emperatur) 279.19 438.35 T
(es and Bolometric Corr) 320.48 438.35 T
(ections for Early-T) 414.83 438.35 T
(ype Stars.\323) 490.2 438.35 T
4 9 Q
0.99 (Code, A.D., Davis, J., Bless, R.C., and Hanbury Brown, R. 1976, ApJ, 203, 417\320) 207 421.02 P
(434.) 216 410.02 T
3 10 Q
(\322Interstellar Extinction in the UV\323) 189 390.35 T
4 9 Q
(Seaton, M.J. 1979, MNRAS, 187, 73P\32076P) 207 373.02 T
(.) 378.43 373.02 T
3 10 Q
(\322Observed Pr) 189 353.35 T
(operties of Interstellar Dust\323) 245.01 353.35 T
4 9 Q
(Savage, B.D., and Mathis, J.S. 1979, ARA&A, 17, 73\3201) 207 336.02 T
(12.) 426.96 336.02 T
54 293.02 540 296.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 294.52 540 294.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 294.52 180 294.52 2 L
0 Z
N
0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(9.2) 163.32 300.02 T
(GHRS-Related T) 189 300.02 T
(echnical Papers) 280.79 300.02 T
3 10 Q
(\322Ultraviolet High-Resolution Spectr) 189 276.35 T
(oscopy fr) 334.74 276.35 T
(om the Space T) 371.31 276.35 T
(elescope.\323) 431.77 276.35 T
4 9 Q
0.29 (Ebbets, D.C., Brandt, J.C., and the HRS Investigation De\336nition T) 207 259.02 P
0.29 (eam 1983, P) 469.71 259.02 P
0.29 (ASP) 520.65 259.02 P
0.29 (,) 537.5 259.02 P
(95, 543\320549.) 216 248.02 T
3 10 Q
0.35 (\322W) 189 228.35 P
0.35 (avelengths and Intensities of a Platinum/Neon Hollow Cathode Lamp in the Region) 201.97 228.35 P
(1) 198 215.35 T
(100\3204000 \201\323) 202.26 215.35 T
4 9 Q
1.62 (Reader) 207 198.02 P
1.62 (, J., Acquista, N., Sansonetti, C.J., and Sansonetti, J.E. 1990, ApJS, 72,) 236.02 198.02 P
(831\320866.) 216 187.02 T
3 10 Q
(\322Status of the Goddar) 189 167.35 T
(d High Resolution Spectr) 277.25 167.35 T
(ograph in May 1991.\323) 377.71 167.35 T
4 9 Q
1.28 (Ebbets, D.C., Brandt, J., Heap, S. 1991, in The First Y) 207 150.02 P
1.28 (ear of) 434.61 150.02 P
8 F
1.28 (HST) 462.69 150.02 P
4 F
1.28 ( Observations,) 480.69 150.02 P
(edited by A.L. Kinney and J.C. Blades, p. 1) 216 139.02 T
(10-122,) 386.43 139.02 T
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0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (103) 541.32 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(GHRS Bibliography) 207 736.18 T
3 10 Q
0.93 (\322Scatter) 189 679.35 P
0.93 (ed Light in the Echelle Modes of the Goddar) 222.52 679.35 P
0.93 (d High Resolution Spectr) 407.87 679.35 P
0.93 (ograph) 511.11 679.35 P
(Aboar) 198 667.35 T
(d the) 222.63 667.35 T
0 F
(Hubble Space T) 244.85 667.35 T
(elescope) 308.58 667.35 T
3 F
(. I. Analysis of Pr) 343.01 667.35 T
(elaunch Calibration Data.\323) 412.64 667.35 T
4 9 Q
(Cardelli, J.A., Ebbets, D.C., and Savage, B.D. 1990, 365, 789\320802.) 207 650.02 T
3 10 Q
0.93 (\322Scatter) 189 630.35 P
0.93 (ed Light in the Echelle Modes of the Goddar) 222.52 630.35 P
0.93 (d High Resolution Spectr) 407.87 630.35 P
0.93 (ograph) 511.11 630.35 P
0.68 (Aboar) 198 618.35 P
0.68 (d the) 222.63 618.35 P
0 F
0.68 (Hubble Space T) 246.22 618.35 P
0.68 (elescope) 311.31 618.35 P
3 F
0.68 (. II. Analysis of In\337ight Spectr) 345.74 618.35 P
0.68 (oscopic Observa-) 469.06 618.35 P
(tions.\323) 198 606.35 T
4 9 Q
(Cardelli, J.A., Ebbets, D.C., and Savage, B.D. 1993, ApJ, 413, 401\320415.) 207 589.02 T
3 10 Q
(\322Resolution and Noise Pr) 189 569.35 T
(operties of the Goddar) 292.25 569.35 T
(d High Resolution Spectr) 382.71 569.35 T
(ograph\323) 483.17 569.35 T
4 9 Q
1 (Gilliland, R.L., Morris, S.L., W) 207 552.02 P
1 (eymann, R.J., Ebbets, D.C., and Lindler) 328.88 552.02 P
1 (, D.J. 1992,) 491.97 552.02 P
(P) 216 541.02 T
(ASP) 221.34 541.02 T
(, 104, 367\320382.) 238.18 541.02 T
0 10 Q
-0.26 (This last paper is especially recommended for its discussion of the deconvolution of) 207 523.35 P
0.4 (the ef) 207 511.35 P
0.4 (fects of the Point Spread Function \050PSF\051 and Line Spread Function \050LSF\051 of) 229.71 511.35 P
3 F
(HST) 207 499.35 T
0 F
( and the GHRS.) 224.78 499.35 T
3 F
1.29 (\322Final Report of the Science V) 189 479.35 P
1.29 (eri\336cation Pr) 317.97 479.35 P
1.29 (ogram for the Goddar) 372.5 479.35 P
1.29 (d High Resolution) 464.63 479.35 P
(Spectr) 198 467.35 T
(ograph for the Hubble Space T) 223.18 467.35 T
(elescope\323) 346.42 467.35 T
4 9 Q
0.44 (Ebbets, D.C. 1992, prepared for NASA/Goddard Space Flight Center by Ball Aero-) 207 450.02 P
(space Systems Group.) 216 439.02 T
0 10 Q
-0.11 (This is a technical document prepared by Ball to ful\336ll a contractual requirement. It) 207 421.35 P
1.01 (provides a detailed description of the tests and calibrations performed during the) 207 409.35 P
0.62 (Science V) 207 397.35 P
0.62 (eri\336cation phase that occurred immediately after the launch of) 247.33 397.35 P
3 F
0.62 (HST) 504.26 397.35 P
0 F
0.62 (. W) 521.3 397.35 P
0.62 (e) 535.56 397.35 P
0.4 (cite it here for completeness, but a General Observer should usually be able to get) 207 385.35 P
(the information that he or she needs from this) 207 373.35 T
3 F
(Handbook) 391.7 373.35 T
0 F
( or by consulting us.) 433.36 373.35 T
FMENDPAGE
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2 9 Q
(GHRS Bibliography) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
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54 74.02 540 74.02 2 L
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2 10 Q
(104) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
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54 726.98 540 726.98 2 L
0.25 H
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54 750.02 540 750.02 2 L
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54 726.98 540 726.98 2 L
0.25 H
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189 672.52 540 672.52 2 L
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0 0 0 1 0 0 0 K
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54 672.52 180 672.52 2 L
0 Z
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0 0 612 792 C
2 12 Q
0 X
0 0 0 1 0 0 0 K
(9.3) 163.32 678.02 T
(GHRS Scienti\336c Papers) 189 678.02 T
0 10 Q
1.44 (A number of GHRS-related papers are concentrated in three special volumes whose) 189 650.35 P
(contents will not be itemized here:) 189 638.35 T
10 11 Q
(\245) 189 620.35 T
3 10 Q
(The First Y) 203.4 620.35 T
(ear of HST Observations) 247.49 620.35 T
0 F
(, 1991, edited by A.L. Kinney and J.C. Blades,) 347.21 620.35 T
(and published by STScI.) 203.4 608.35 T
10 11 Q
(\245) 189 593.35 T
3 10 Q
(Astr) 203.4 593.35 T
(ophysical Journal Letters) 219.7 593.35 T
0 F
(, volume 377, number 1, 1991.) 321.92 593.35 T
10 11 Q
(\245) 189 578.35 T
3 10 Q
(Science with the Hubble Space T) 203.4 578.35 T
(elescope) 333.85 578.35 T
0 F
(, 1992, edited by P) 368.28 578.35 T
(. Benvenuti and E.) 442.17 578.35 T
(Schreier) 203.4 566.35 T
(, and published by ESO.) 236.32 566.35 T
12 12 Q
(1992:) 162 539.02 T
3 10 Q
(\322The Abundance of Bor) 189 518.35 T
(on in Thr) 284.46 518.35 T
(ee Halo Stars\323) 321.32 518.35 T
4 9 Q
(Duncan, D.K., Lambert, D.L., and Lemke, M. 1992, ApJ, 401, 584\320595.) 207 501.02 T
3 10 Q
0.38 (\322Ultraviolet Observations of the Gas Phase Abundances in the Diffuse Clouds T) 189 481.35 P
0.38 (owar) 514.81 481.35 P
0.38 (d) 535 481.35 P
(Zeta Ophiuchi at 3.5 Kilometers per Second Resolution\323) 198 469.35 T
4 9 Q
(Savage, B.D., Cardelli, J.A., and So\336a, U.J. 1992, ApJ, 401, 706\320723.) 207 452.02 T
3 10 Q
(\322Fractionation of CO in the Diffuse Clouds T) 189 432.35 T
(owar) 371.16 432.35 T
(d Zeta Ophiuchi\323) 391.35 432.35 T
4 9 Q
0.22 (Shef) 207 415.02 P
0.22 (fer) 225.35 415.02 P
0.22 (, Y) 235.36 415.02 P
0.22 (., Federman, S.R., Lambert, D.L., and Cardelli, J.A. 1992, ApJ, 397, 482\320) 245.43 415.02 P
(491.) 216 404.02 T
3 10 Q
(\322Highly Ionized Atoms T) 189 384.35 T
(owar) 288.36 384.35 T
(d HD 93521.\323) 308.55 384.35 T
4 9 Q
(Spitzer) 207 367.02 T
(, L., and Fitzpatrick, E.L. 1992, ApJ, 391, L41\320L44.) 234.51 367.02 T
3 10 Q
1.58 (\322Ultraviolet and Optical Spectral Morphology of Melnick 42 and Radcliffe 136a in) 189 347.35 P
(30) 198 335.35 T
(Doradus\323) 210.5 335.35 T
4 9 Q
0.06 (W) 207 318.02 P
0.06 (alborn, N.R., Ebbets, D.C., Parker) 215.16 318.02 P
0.06 (, J.W) 350.47 318.02 P
0.06 (., Nichols-Bohlin, J., and White, R.L. 1992,) 370.54 318.02 P
(ApJ, 393, L13\320L16.) 216 307.02 T
3 10 Q
(\322Detection of a Pr) 189 287.35 T
(oton Beam During the Impulsive Phase of a Stellar Flar) 263.35 287.35 T
(e\323) 487.69 287.35 T
4 9 Q
1.62 (W) 207 270.02 P
1.62 (oodgate, B.E., Robinson, R.D., Carpenter) 215.33 270.02 P
1.62 (, K.G., Maran, S.P) 386.89 270.02 P
1.62 (., and Shore, S.N.) 463.61 270.02 P
(1992, ApJ, 397, L95\320-L98.) 216 259.02 T
12 12 Q
(1993:) 162 232.02 T
3 10 Q
0.12 (\322Interstellar Mg) 189 211.35 P
3 9 Q
0.11 (II) 258.13 211.35 P
3 10 Q
0.12 ( and C) 264.12 211.35 P
3 9 Q
0.11 (IV) 293.66 211.35 P
3 10 Q
0.12 ( Absorption T) 302.15 211.35 P
0.12 (owar) 356.48 211.35 P
0.12 (d Mrk 205 by NGC 4319: An \324Optically-) 376.67 211.35 P
(Thick\325 QSO Absorption System\323) 198 199.35 T
4 9 Q
(Bowen D.V) 207 182.02 T
(., and Blades, J.C. ApJ, 403, L55\320L58.) 251.19 182.02 T
3 10 Q
0.24 (\322Observations of 3C 273 with the Goddar) 189 162.35 P
0.24 (d High Resolution Spectr) 358.95 162.35 P
0.24 (ograph on the Hub-) 460.13 162.35 P
(ble Space T) 198 150.35 T
(elescope\323) 243.74 150.35 T
4 9 Q
(Brandt, J.C., et al. 1993, AJ, 105, 831\320846.) 207 133.02 T
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0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (105) 541.32 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(GHRS Bibliography) 207 736.18 T
3 10 Q
(\322The Galactic Halo and Local Inter) 189 679.35 T
(galactic Medium towar) 333.35 679.35 T
(d PKS 2155\320304\323) 426.31 679.35 T
4 9 Q
0.49 (Bruweiler) 207 662.02 P
0.49 (, F) 244.01 662.02 P
0.49 (.C., Boggess, A., Norman, D.J., Grady) 254 662.02 P
0.49 (, C.A., Urry) 408.34 662.02 P
0.49 (, C.M., and Kondo, Y) 453.16 662.02 P
0.49 (.) 537.5 662.02 P
(1993, ApJ, 409, 199\320204.) 216 651.02 T
3 10 Q
0.9 (\322Ultraviolet T) 189 631.35 P
0.9 (ransitions of Low Condensation T) 246.86 631.35 P
0.9 (emperatur) 385.68 631.35 P
0.9 (e Heavy Elements and New) 426.98 631.35 P
(Data for Interstellar Arsenic, Selenium, T) 198 619.35 T
(ellurium, and Lead\323) 364.02 619.35 T
4 9 Q
0.35 (Cardelli, J.A., Federman, S.R., Lambert, D., and Theodosiou, C.E. 1993, ApJ, 416,) 207 602.02 P
(L41\320L44.) 216 591.02 T
3 10 Q
(\322Abundance of Interstellar Carbon T) 189 571.35 T
(owar) 337.53 571.35 T
(d Zeta Ophiuchi\323) 357.72 571.35 T
4 9 Q
0.86 (Cardelli, J.A., Mathis, J.S., Ebbets, D.C., and Savage, B.D. 1993, ApJ, 403, L17\320) 207 554.02 P
(L20.) 216 543.02 T
3 10 Q
(\322Detection of Bor) 189 523.35 T
(on, Cobalt, and other W) 260.85 523.35 T
(eak Interstellar Lines towar) 356.6 523.35 T
(d) 467.62 523.35 T
13 F
(z) 475.12 523.35 T
3 F
( Ophiuchi\323) 480.06 523.35 T
4 9 Q
1.14 (Federman, S.R., Shef) 207 506.02 P
1.14 (fer) 296.15 506.02 P
1.14 (, Lambert, D.L., and Gilliland, R.L. 1993, ApJ, 413, L51\320) 306.16 506.02 P
(L54.) 216 495.02 T
3 10 Q
(\322Quantitative Spectr) 189 475.35 T
(oscopy of K647 \321 the PNN of Ps1 in the Globular Cluster M15\323) 272.24 475.35 T
4 9 Q
(Heber) 207 458.02 T
(, U., Dreizler) 231.01 458.02 T
(, S., and W) 280.52 458.02 T
(erner) 324.88 458.02 T
(, K. 1993, Acta Astron., 43, 337\320342.) 345.39 458.02 T
3 10 Q
(\322The Interstellar Abundances of T) 189 438.35 T
(in and Four Other Heavy Elements\323) 326.23 438.35 T
4 9 Q
0.44 (Hobbs, L.M., W) 207 421.02 P
0.44 (elty) 269.73 421.02 P
0.44 (, D.E., Morton, D.C., Spitzer) 283.07 421.02 P
0.44 (, L., and Y) 395.85 421.02 P
0.44 (ork, D.G. 1993, ApJ, 41) 437.36 421.02 P
0.44 (1,) 532.49 421.02 P
(750\320755.) 216 410.02 T
3 10 Q
1 (\322T) 189 390.35 P
1 (ime-Series Observations of O Stars. III. IUE and HST Spectr) 199.57 390.35 P
1 (oscopy of) 451.79 390.35 P
13 F
1 (z) 494.34 390.35 P
3 F
1 ( Ophiuchi) 499.28 390.35 P
(and Implications for the \324Photospheric Connection\325\323) 198 378.35 T
4 9 Q
(Howarth, I.D. et al., 1993, ApJ, 417, 338\320346.) 207 361.02 T
3 10 Q
1.36 (\322Hubble Space T) 189 341.35 P
1.36 (elescope Spectra of the Phase-Modulated W) 260.23 341.35 P
1.36 (ind in the SMC O+WR) 443.38 341.35 P
(Binary R31\323) 198 329.35 T
4 9 Q
(Hutchings, J.B., Morris, S.C., and Bianchi, L. 1993, ApJ, 410, 803\320807.) 207 312.02 T
3 10 Q
(\322Deceleration of Interstellar Hydr) 189 292.35 T
(ogen at the Heliospheric Interface\323) 327.23 292.35 T
4 9 Q
(Lallement, R., Bertaux, J.-L., and Clarke, J.T) 207 275.02 T
(. 1993, Science, 260, 1095\3201098.) 383.57 275.02 T
0 10 Q
(Provides a good illustration of geocoronal L) 207 257.35 T
(y-) 383.1 257.35 T
13 F
(a) 391.43 257.35 T
0 F
( with the LSA and Echelle-A.) 397.74 257.35 T
3 F
3.24 (\322High Resolution UV Stellar Spectr) 189 237.35 P
3.24 (oscopy with the HST/GHRS, Challenges and) 345.48 237.35 P
(Opportunities for Atomic Physics\323) 198 225.35 T
4 9 Q
0.62 (Leckrone, D.S., Johansson, S., W) 207 208.02 P
0.62 (ahlgren, G.M., and Adelman, S.J. 1993, Physica) 344.2 208.02 P
(Scripta, T47, 149\320156.) 216 197.02 T
3 10 Q
3.97 (\322Goddar) 189 177.35 P
3.97 (d High Resolution Spectr) 225.3 177.35 P
3.97 (ograph Observations of the Local Interstellar) 337.66 177.35 P
-0.15 (Medium and the Deuterium/Hydr) 198 165.35 P
-0.15 (ogen Ratio Along the Line of Sight T) 330.78 165.35 P
-0.15 (owar) 475.23 165.35 P
-0.15 (d Capella\323) 495.42 165.35 P
4 9 Q
-0.1 (Linsky) 207 148.02 P
-0.1 (, J.L., Brown, A., Gayley) 231.84 148.02 P
-0.1 (, K., Diplas, A., Savage, B.D., A) 327.33 148.02 P
-0.1 (yres, T) 452.66 148.02 P
-0.1 (.R., Landsman,) 479.07 148.02 P
(W) 216 137.02 T
(., Shore, S.N., and Heap, S.R. 1993, ApJ, 402, 694\320709.) 224 137.02 T
3 10 Q
(\322The Bor) 189 117.35 T
(on Abundance of Pr) 226.69 117.35 T
(ocyon\323) 306.59 117.35 T
4 9 Q
(Lemke, M., Lambert, D.L., and Edvardsson, B. 1993, P) 207 100.02 T
(ASP) 424.94 100.02 T
(, 105, 468\320475.) 441.79 100.02 T
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0 0 0 1 0 0 0 K
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54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(GHRS Bibliography) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(106) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
3 F
(\322Detection of [O II]) 189 679.35 T
13 F
(l) 272.88 679.35 T
3 F
(2471 fr) 278.37 679.35 T
(om the Io Plasma T) 307.17 679.35 T
(orus\323) 384.58 679.35 T
4 9 Q
0.23 (McGrath, M.A., Feldman, P) 207 662.02 P
0.23 (.D., Strobel, D.F) 315.56 662.02 P
0.23 (., Moos, H.W) 379.54 662.02 P
0.23 (., and Ballester) 431.52 662.02 P
0.23 (, G.E. 1993,) 491.51 662.02 P
(ApJ, 415, L55\320L58.) 216 651.02 T
3 10 Q
(\322A Sear) 189 631.35 T
(ch for Pr) 221.13 631.35 T
(oton Beams During Flar) 256.87 631.35 T
(es on AU Micr) 355.11 631.35 T
(oscopii\323) 413.34 631.35 T
4 9 Q
0.19 (Robinson, R.D., Carpenter) 207 614.02 P
0.19 (, K.G., W) 312.93 614.02 P
0.19 (oodgate, B.E., and Maran, S.P) 349.67 614.02 P
0.19 (. 1993, ApJ, 414,) 471.37 614.02 P
(872\320876.) 216 603.02 T
3 10 Q
1.28 (\322Observations of the Gaseous Galactic Halo T) 189 583.35 P
1.28 (owar) 384.07 583.35 P
1.28 (d 3C273 with the Goddar) 404.26 583.35 P
1.28 (d High) 511.22 583.35 P
(Resolution Spectr) 198 571.35 T
(ograph\323) 268.46 571.35 T
4 9 Q
(Savage, B.D., Lu, L., W) 207 554.02 T
(eymann, R.J., and Morris, S.L. 1993, ApJ, 404, 124\320143.) 300.89 554.02 T
3 10 Q
-0.25 (\322Goddar) 189 534.35 P
-0.25 (d High Resolution Spectr) 225.3 534.35 P
-0.25 (ograph Observations of Narr) 325.01 534.35 P
-0.25 (ow Discr) 440.84 534.35 P
-0.25 (ete Stellar W) 476.61 534.35 P
-0.25 (ind) 527.22 534.35 P
(Absorption Featur) 198 522.35 T
(es in the Ultraviolet Spectrum of the O7.5III Star) 271.8 522.35 T
13 F
(z) 470.67 522.35 T
3 F
( Persei\323) 475.61 522.35 T
4 9 Q
-0.08 (Shore, S.N., Altner) 207 505.02 P
-0.08 (, B., Bolton, C.T) 281.38 505.02 P
-0.08 (., Cardelli, J.A., and Ebbets, D.C. 1993, ApJ, 41) 343.68 505.02 P
-0.08 (1,) 532.49 505.02 P
(864\320868.) 216 494.02 T
3 10 Q
(\322The Early Ultraviolet Spectral Evolution of Nova Cygni 1992\323) 189 474.35 T
4 9 Q
2.14 (Shore, S.N., Sonneborn, G., Starr\336eld, S., Gonzalez-Riestra, R., and Ake, T) 207 457.02 P
2.14 (.B.) 528.99 457.02 P
(1993, AJ, 106, 2408\3202428.) 216 446.02 T
3 10 Q
1.49 (\322High-Resolution Ultraviolet Observations of the Interstellar Diffuse Clouds towar) 189 426.35 P
1.49 (d) 535 426.35 P
13 F
(m) 198 414.35 T
3 F
(Columbae\323) 206.26 414.35 T
4 9 Q
(So\336a, U.J., Savage, B.D., and Cardelli, J.A. 1993, ApJ, 413, 251\320267.) 207 397.02 T
3 10 Q
(\322Composition of Interstellar Clouds in the Disk and Halo. I. HD 93521\323) 189 377.35 T
4 9 Q
(Spitzer) 207 360.02 T
(, L., and Fitzpatrick, E.L. 1993, ApJ,409, 299\320318.) 234.51 360.02 T
12 12 Q
(1994:) 162 333.02 T
3 10 Q
(\322Interstellar and Inter) 189 312.35 T
(galactic Magnesium and Sodium Absorption towar) 278.63 312.35 T
(d SN 1993J\323) 482.43 312.35 T
4 9 Q
(Bowen, D.V) 207 295.02 T
(., Roth, K.C., Blades, J.C., and Meyer) 253.69 295.02 T
(, D.M. 1994, ApJ, 420, L71\320L74.) 403.26 295.02 T
3 10 Q
(\322Interstellar Detection of the Intersystem Line Si II] l 2335 towar) 189 275.35 T
(d) 451.4 275.35 T
13 F
(z) 458.9 275.35 T
3 F
( Ophiuchi\323) 463.84 275.35 T
4 9 Q
0.64 (Cardelli, J.A., So\336a, U.J., Savage, B.D., Keenan, F) 207 258.02 P
0.64 (.P) 412.55 258.02 P
0.64 (., and Dufton, P) 419.9 258.02 P
0.64 (.L. 1994, ApJ,) 483.19 258.02 P
(420, L29\320L32.) 216 247.02 T
3 10 Q
0.04 (\322GHRS Observations of Cool, Low-Gravity Stars. I. The Far) 189 227.35 P
0.04 (-Ultraviolet Spectrum of) 433.3 227.35 P
13 F
0.04 (a) 533.69 227.35 P
3 F
(Orionis \050M2Iab\051\323) 198 215.35 T
4 9 Q
0.08 (Carpenter) 207 198.02 P
0.08 (, K.G., Robinson, R.D., W) 246.52 198.02 P
0.08 (ahlgren, G.M., Linsky) 349.03 198.02 P
0.08 (, J.L., and Brown, A. 1994,) 433.55 198.02 P
(ApJ, in press.) 216 187.02 T
3 10 Q
(\322Composition of Interstellar Clouds in the Disk and Halo. II.) 189 167.35 T
13 F
(g) 436.79 167.35 T
3 8 Q
(2) 440.9 171.35 T
3 10 Q
( V) 444.9 167.35 T
(elorum\323) 452.4 167.35 T
4 9 Q
(Fitzpatrick, E.L., and Spitzer) 207 150.02 T
(, L. 1994, ApJ, in press.) 319.05 150.02 T
3 10 Q
(\322Sear) 189 130.35 T
(ch for CO Absorption Bands in IUE Far) 212.52 130.35 T
(-Ultraviolet Spectra of Cool Stars\323) 373.71 130.35 T
4 9 Q
(Gessner) 207 113.02 T
(, S.E., Carpenter) 240.52 113.02 T
(, K.G., and Robinson, R.D. 1994, AJ, 107, 747\320750.) 307.05 113.02 T
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[ 0 0 1 0 1 1 0]
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0 0 0 1 0 0 0 K
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72 750.02 558 750.02 2 L
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0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (107) 541.32 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(GHRS Bibliography) 207 736.18 T
3 10 Q
1.13 (\322Comparison of New Experimental and Astr) 207 679.35 P
1.13 (ophysical f-values for Some Ru II Lines,) 390.93 679.35 P
(Observed in HST Spectra of) 216 667.35 T
13 F
(c) 330.71 667.35 T
3 F
(Lupi\323) 338.7 667.35 T
4 9 Q
(Johansson, S.G., et al. 1994, ApJ, 421, 809\320815.) 225 650.02 T
3 10 Q
(\322Is Ther) 207 630.35 T
(e Primor) 240.8 630.35 T
(dial Gas in IZw 18?\323) 276.26 630.35 T
4 9 Q
0.79 (Kunth, D., Lequeux, J., Sargent, W) 225 613.02 P
0.79 (.L.W) 367.52 613.02 P
0.79 (., and V) 385.53 613.02 P
0.79 (iallefond, F) 417.97 613.02 P
0.79 (. 1994, A&A, 282, 709\320) 461.78 613.02 P
(716.) 234 602.02 T
3 10 Q
0.58 (\322Interstellar Clouds towar) 207 582.35 P
0.58 (d Sirius and Local Cloud Ionization. I. GHRS Observations) 315.03 582.35 P
(of Sirius A\323) 216 570.35 T
4 9 Q
-0.14 (Lallement, R., Bertin, P) 225 553.02 P
-0.14 (., Ferlet, R., V) 315.95 553.02 P
-0.14 (idal-Madjar) 370.89 553.02 P
-0.14 (, A., and Bertaux, J.L. 1994, A&A, in) 414.9 553.02 P
(press.) 234 542.02 T
3 10 Q
(\322Interstellar Carbon Monoxide towar) 207 522.35 T
(d) 358.58 522.35 T
13 F
(z) 366.08 522.35 T
3 F
( Ophiuchi.\323) 371.02 522.35 T
4 9 Q
0.01 (Lambert, D.L., Shef) 225 505.02 P
0.01 (fer) 302.9 505.02 P
0.01 (, Y) 312.91 505.02 P
0.01 (., Gilliland, R.L., and Federman, S.R. 1994, ApJ, 420, 756\320) 322.77 505.02 P
(771.) 234 494.02 T
0 10 Q
0.02 (An especially good discussion of how to achieve very high signal-to-noise with the) 225 476.35 P
(GHRS.) 225 464.35 T
3 F
0.35 (\322High V) 207 444.35 P
0.35 (elocity Plasma in the T) 240.41 444.35 P
0.35 (ransition Region of Au Micr) 333.46 444.35 P
0.35 (oscopii: Evidence for Mag-) 447.26 444.35 P
2.05 (netic Reconnection and saturated Heating During Quiescent and Flaring Condi-) 216 432.35 P
(tions\323) 216 420.35 T
4 9 Q
(Linsky) 225 403.02 T
(, J.L., and W) 249.84 403.02 T
(ood, B.E. 1994, ApJ, in press.) 300.2 403.02 T
3 10 Q
(\322Pr) 207 383.35 T
(obing the Galactic Disk and Halo. I. The NGC 3783 Sight Line\323) 222.19 383.35 T
4 9 Q
(Lu, L., Savage, B.D., and Sembach, K.R. 1994, ApJ, in press.) 225 366.02 T
3 10 Q
(\322Observing Stellar Cor) 207 346.35 T
(onae with the Goddar) 301.08 346.35 T
(d High Resolution Spectr) 388.21 346.35 T
(ograph.) 488.67 346.35 T
(I. The dMe Star AU Micr) 216 334.35 T
(oscopii\323) 316.17 334.35 T
4 9 Q
1.27 (Maran, S.P) 225 317.02 P
1.27 (., Robinson, R.D., Shore, S.N., Brosius, J.W) 270.13 317.02 P
1.27 (., Carpenter) 452.81 317.02 P
1.27 (, K.G., W) 501.1 317.02 P
1.27 (ood-) 539.99 317.02 P
0.93 (gate, B.E., Linsky) 234 306.02 P
0.93 (, J.L., Brown, A., Byrne, P) 305.23 306.02 P
0.93 (.B., Kundu, M.R., White, S., Brandt,) 411.78 306.02 P
(J.C., Shine, R.A., and W) 234 295.02 T
(alter) 331.21 295.02 T
(, F) 348.22 295.02 T
(.M. 1994, ApJ, 421, 800\320808.) 357.72 295.02 T
3 10 Q
0.51 (\322Highly Ionized Gas Absorption in the Disk and Halo towar) 207 275.35 P
0.51 (d HD) 453.18 275.35 P
0.51 (167756 at 3.5 Kilo-) 478.13 275.35 P
(meters per Second Resolution\323) 216 263.35 T
4 9 Q
(Savage, B.D., Sembach, K.R., and Cardelli, J.A., 1994, ApJ, 420, 183\320196.) 225 246.02 T
3 10 Q
0.39 (\322Al III, Si IV) 207 226.35 P
0.39 (, and C IV Absorption towar) 258.55 226.35 P
0.39 (d) 374.05 226.35 P
13 F
0.39 (z) 381.94 226.35 P
3 F
0.39 ( Ophiuchi: Evidence for Photoionized and) 386.88 226.35 P
(Collisionally Ionized Gas\323) 216 214.35 T
4 9 Q
(Sembach, K.R., Savage, B.D., and Jenkins, E.B. 1994, ApJ, 421, 585\320599.) 225 197.02 T
3 10 Q
0.22 (\322A Sear) 207 177.35 P
0.22 (ch for Chr) 239.35 177.35 P
0.22 (omospheric Emission in A-type Stars Using the Goddar) 281.1 177.35 P
0.22 (d High Reso-) 504.78 177.35 P
(lution Spectr) 216 165.35 T
(ograph\323) 267.02 165.35 T
4 9 Q
(Simon, T) 225 148.02 T
(., Landsman, W) 260.01 148.02 T
(.B., and Gilliland, R.L. 1994, ApJ, in press.) 322.54 148.02 T
3 10 Q
(\322The Abundant Elements in Interstellar Dust\323) 207 128.35 T
4 9 Q
(So\336a, U.J., Cardelli, J.A., and Savage, B.D. 1994, ApJ, in press.) 225 111.02 T
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2 9 Q
(GHRS Bibliography) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(108) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
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54 74.02 540 74.02 2 L
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54 750.02 540 750.02 2 L
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0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
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0.65 (\322High-Resolution Spectra of Jupiter) 189 679.35 P
0.65 (\325) 337.16 679.35 P
0.65 (s Northern Aur) 339.2 679.35 P
0.65 (oral Ultraviolet Emission with the) 400.7 679.35 P
(Hubble Space T) 198 667.35 T
(elescope\323) 260.96 667.35 T
4 9 Q
1.04 (T) 207 650.02 P
1.04 (rafton, L.M., Gerard, J.C., Munhoven, G., and W) 212.17 650.02 P
1.04 (aite, J.H. 1994, ApJ, 421, 816\320) 411.21 650.02 P
(827.) 216 639.02 T
3 10 Q
(\322A W) 189 619.35 T
(eak Diffuse Interstellar Band in the Far) 210.58 619.35 T
(-Ultraviolet Spectrum of) 369.26 619.35 T
13 F
(z) 469.53 619.35 T
3 F
( Ophiuchi?\323) 474.47 619.35 T
4 9 Q
(T) 207 602.02 T
(ripp, T) 212.17 602.02 T
(.M., Cardelli, J.A., and Savage, B.D. 1994, AJ, 107, 645\320650.) 236.67 602.02 T
3 10 Q
0.44 (\322G191\320B2B: Accurate Abundances for Nitr) 189 582.35 P
0.44 (ogen, Silicon, and Ir) 366.47 582.35 P
0.44 (on fr) 449.35 582.35 P
0.44 (om GHRS Obser-) 468.59 582.35 P
(vations\323) 198 570.35 T
4 9 Q
(V) 207 553.02 T
(idal-Madjar) 212.84 553.02 T
(, A., et al. 1994, A&A, in press.) 256.85 553.02 T
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2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (109) 541.32 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
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72 74.02 558 74.02 2 L
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72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
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72 74.02 558 74.02 2 L
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(GHRS Bibliography) 207 736.18 T
72 671.02 558 674.02 C
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207 672.52 558 672.52 2 L
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72 672.52 198 672.52 2 L
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0 0 612 792 C
2 12 Q
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0 0 0 1 0 0 0 K
(9.4) 181.32 678.02 T
(Acknowledgments) 207 678.02 T
0 10 Q
0.28 (It is easier to write a document like this for an instrument that has already been operat-) 207 650.35 P
0.28 (ing for several years, so we owe a debt to Dennis Ebbets and Doug Duncan, who com-) 207 638.35 P
0.64 (piled earlier versions of this) 207 626.35 P
3 F
0.64 (Handbook) 324.33 626.35 P
0 F
0.64 ( when much less was known. Others who have) 365.99 626.35 P
0.14 (contributed to the success of the GHRS, especially in the technical areas that this docu-) 207 614.35 P
1.48 (ment treats, include D. Lindler) 207 602.35 P
1.48 (, E. Malumuth, S. Shore, G. W) 335.27 602.35 P
1.48 (ahlgren \050and others at) 466.65 602.35 P
1.42 (Goddard Space Flight Center\051, and R. Gilliland and J. Skapik at STScI. The GHRS) 207 590.35 P
0.12 (Investigation De\336nition T) 207 578.35 P
0.12 (eam \050IDT\051 is also thanked for their help and for the quality of) 310.44 578.35 P
(the instrument that they have provided to the astronomical community) 207 566.35 T
(.) 487.72 566.35 T
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0 X
0 0 0 1 0 0 0 K
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2 9 Q
(GHRS Bibliography) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(1) 54 60.29 T
(10) 59.01 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
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0 Z
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54 726.98 540 726.98 2 L
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0 Z
0 X
0 0 0 1 0 0 0 K
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (1) 542.42 60.29 P
-2.78 (1) 547.43 60.29 P
-2.78 (1) 552.44 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
5 24 Q
-0.48 (Glossary of T) 207 677 S
-0.48 (erms and) 327.41 677 S
-0.48 (Abbr) 207 647 S
-0.48 (eviations) 253.54 647 S
0 10 Q
0.12 (Here we provide de\336nitions and explanations of technical terms and abbreviations used) 207 425.33 P
1.59 (in the text. The usual abbreviations found in HST) 207 413.33 P
1.59 (-related documents \050e.g., WFPC2,) 416.85 413.33 P
(FGS\051 are not repeated here.) 207 401.33 T
2 F
(Blaze Function) 189 377.33 T
0 F
-0.13 (The ef) 207 353.33 P
-0.13 (\336ciency of an echelle grating drops sharply as one moves away from blaze center) 232.51 353.33 P
-0.13 (.) 555.5 353.33 P
0.06 (The shape of the response function is virtually the same for the dif) 207 341.33 P
0.06 (ferent orders and this) 473.11 341.33 P
(function is known as the Ripple Function \050see Section) 207 329.33 T
(8.3.3 on page) 425.6 329.33 T
(91\051.) 481.98 329.33 T
2 F
(Corner diodes) 189 305.33 T
0 F
0.36 (The detector area of the Digicons is laid out into speci\336c diodes, each of which acts as) 207 281.33 P
0.18 (an independent detector) 207 269.33 P
0.18 (. There are 500 science diodes, each of which is skinny but tall,) 302.33 269.33 P
0.17 (four focus diodes \050see below\051, and four corner diodes. The corner diodes are lar) 207 257.33 P
0.17 (ge rect-) 527.57 257.33 P
0.47 (angles \0500.1) 207 245.33 P
13 F
0.47 (\264) 254.32 245.33 P
0 F
0.47 ( 1 mm\051 of detector area above and below the science diodes and are used) 259.81 245.33 P
(for measuring background.) 207 233.33 T
2 F
(Cycles) 189 209.33 T
0 F
0.31 (Proposals to use HST are solicited and reviewed on roughly an annual basis. However) 207 185.33 P
0.31 (,) 555.5 185.33 P
1.53 (because HST\325) 207 173.33 P
1.53 (s properties changed fundamentally when COST) 264.35 173.33 P
1.53 (AR and WFPC2 were) 465.91 173.33 P
-0.25 (installed, Cycle 3 was de\336ned to end at the time of the Servicing Mission. Cycle 4 began) 207 161.33 P
(at the end of SMOV) 207 149.33 T
(. Cycle 5 is due to begin in mid 1995.) 286.81 149.33 T
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2 9 Q
(Glossary of T) 189 736.18 T
(erms and Abbreviations) 245.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(1) 54 60.29 T
(12) 59.01 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
(CVZ) 171 679.35 T
0 F
0.55 (Continuous V) 189 655.35 P
0.55 (iewing Zones. The inclined orbit of HST allows for uninterrupted obser-) 244.79 655.35 P
-0.24 (vations of objects in some declination ranges at certain times. See the) 189 643.35 P
3 F
-0.24 (Call for Pr) 466.39 643.35 P
-0.24 (oposals) 509.44 643.35 P
0 F
(for further information.) 189 631.35 T
2 F
(DEFCAL) 171 607.35 T
0 F
0.58 (Short for De\337ection Calibration. All GHRS acquisitions begin with a) 189 583.35 P
9 F
1.4 (DEFCAL) 473.98 583.35 P
0 F
0.58 (, which) 509.98 583.35 P
0.5 (measures the instantaneous location of the images on the onboard spectrum lamps and) 189 571.35 P
0.44 (then compares that location to the nominal coordinates stored in the onboard database.) 189 559.35 P
0.08 (The dif) 189 547.35 P
0.08 (ferences can range over several de\337ection steps in response to thermal and mag-) 218.06 547.35 P
0.35 (netic drifts. The of) 189 535.35 P
0.35 (fsets are applied to the database coordinates of the science apertures) 264.31 535.35 P
0.4 (to provide an updated estimate of their location. In practice, only observations of lamp) 189 523.35 P
0.69 (SC2 are used because of the loss of Side 1 and because using SC2 decreases the time) 189 511.35 P
(interval between the) 189 499.35 T
9 F
(DEFCAL) 272.59 499.35 T
0 F
( and the tar) 308.59 499.35 T
(get locate phase of the acquisition.) 353.12 499.35 T
2 F
(Focus diodes) 171 475.35 T
0 F
-0.16 (See Chapter 7 to see how the diodes in the GHRS Digicons are con\336gured. At both ends) 189 451.35 P
0.74 (of the array of 500 science diodes are two focus diodes. The focus diodes are smaller) 189 439.35 P
0.43 (than the science diodes and are square. The image of the LSA is de\337ected to the focus) 189 427.35 P
(diodes to generate) 189 415.35 T
9 F
(MAP) 264.26 415.35 T
0 F
(s and) 282.26 415.35 T
9 F
(IMAGE) 305.59 415.35 T
0 F
(s. The focus diodes are 25 microns square.) 335.59 415.35 T
2 F
(GIMP) 171 391.35 T
0 F
1.21 (Geomagnetically-induced image motion problem. This problem underlies our recom-) 189 367.35 P
1.16 (mendation to have no single exposure be longer than about 5 minutes in length. See) 189 355.35 P
(Section) 189 343.35 T
(8.6.5 on page) 221.5 343.35 T
(98.) 277.88 343.35 T
2 F
(GSC) 171 319.35 T
0 F
-0.19 (Guide Star Catalog, the list used to \336nd stars upon which the Fine Guidance Sensors can) 189 295.35 P
(lock to control the pointing of HST) 189 283.35 T
(.) 329.37 283.35 T
2 F
(LSA) 171 259.35 T
0 F
0.34 (Lar) 189 235.35 P
0.34 (ge Science Aperture. This is a square opening at the front of the GHRS that is used) 202.7 235.35 P
1.52 (to acquire stars and for some science observations. Its dimensions were 2.00 arcsec) 189 223.35 P
0.57 (square before COST) 189 211.35 P
0.57 (AR is installed and 1.74 arcsec square afterwards. The name used) 271.55 211.35 P
(for the LSA will continue to be \322) 189 199.35 T
9 F
(2.0) 320.93 199.35 T
0 F
(\323.) 338.93 199.35 T
2 F
(OSS) 171 175.35 T
0 F
-0.21 (Observation Support System, which is the facility located at STScI for real-time interac-) 189 151.35 P
(tion between the ground and the) 189 139.35 T
3 F
(HST) 320.09 139.35 T
0 F
( spacecraft.) 337.87 139.35 T
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2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (1) 541.87 60.29 P
-2.78 (13) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
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72 74.02 558 74.02 2 L
2 Z
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72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Glossary of T) 207 736.18 T
(erms and Abbreviations) 263.85 736.18 T
2 10 Q
(Phase I) 189 679.35 T
0 F
0.01 (A Phase I proposal for) 207 655.35 P
3 F
0.01 (HST) 299.51 655.35 P
0 F
0.01 ( includes just the information need by the T) 317.29 655.35 P
0.01 (elescope Alloca-) 491.07 655.35 P
0.65 (tion Committee \050T) 207 643.35 P
0.65 (AC\051 and STScI to judge scienti\336c merit and technical feasibility) 281.94 643.35 P
0.65 (. In) 544.02 643.35 P
0.52 (addition to the scienti\336c justi\336cation, you are asked to provide a list of the tar) 207 631.35 P
0.52 (gets that) 523.86 631.35 P
0.31 (you wish to observe and a brief description of the observations themselves. W) 207 619.35 P
0.31 (e recom-) 522.42 619.35 P
-0.26 (mend adding comments to provide a clearer explanation of what you intend, even if they) 207 607.35 P
(are not required.) 207 595.35 T
2 F
(Phase II) 189 571.35 T
0 F
1.02 (The Phase II proposal is written once the Phase I proposal has been accepted for the) 207 547.35 P
-0.03 (HST science program. The Phase II proposal includes all the detailed speci\336cations that) 207 535.35 P
-0.12 (are needed to turn your science program into the commands that the spacecraft will exe-) 207 523.35 P
0.72 (cute. As with Phase I, we recommend the liberal use of comments to help ensure that) 207 511.35 P
(your goals will be achieved.) 207 499.35 T
2 F
(Ripple Function) 189 475.35 T
0 F
(See Blaze Function) 207 451.35 T
2 F
(SAA) 189 427.35 T
0 F
1.22 (South Atlantic Anomaly) 207 403.35 P
1.22 (. A region lying over southeastern South America where the) 306.56 403.35 P
0.17 (earth\325) 207 391.35 P
0.17 (s radiation belts dip low) 229.77 391.35 P
0.17 (, leading to high particle background rates for satellites in) 325.92 391.35 P
(Low Earth Orbit. GHRS observations are suspended during passage through the SAA.) 207 379.35 T
2 F
(Side 1, Side 2) 189 355.35 T
0 F
0.29 (GHRS is split into two \322sides,\323 one for the short-wavelength detector \050D1\051 and one for) 207 331.35 P
-0.1 (the long-wavelength detector \050D2\051. The sides operate independently but depend on each) 207 319.35 P
0.57 (other for communication with the spacecraft. The installation of the GHRS Repair Kit) 207 307.35 P
0.69 (during the HST Servicing Mission has meant that all GHRS communications are now) 207 295.35 P
1.07 (through Side 2. Moreover) 207 283.35 P
1.07 (, Side 2 now solely controls the grating carrousel and LSA) 313.14 283.35 P
(shutter) 207 271.35 T
(.) 233.67 271.35 T
2 F
(SMOV) 189 247.35 T
0 F
0.19 (Servicing Mission Orbital V) 207 223.35 P
0.19 (eri\336cation, the period of time immediately after the Servic-) 320.09 223.35 P
-0.09 (ing Mission in which the basic capabilities of the telescope and instruments are veri\336ed.) 207 211.35 P
2 F
(SPYBAL) 189 187.35 T
0 F
0 (SPectrum Y BALance. A) 207 163.35 P
9 F
0.01 (SPYBAL) 311.17 163.35 P
0 F
0 ( consists of a quick observation of the spectrum cali-) 347.17 163.35 P
0.43 (bration lamp SC2 at a standard wavelength setting to ensure that the spectrum is prop-) 207 151.35 P
1.83 (erly centered on the diodes in the cross-dispersion direction. The) 207 139.35 P
3 F
1.83 (y) 486.66 139.35 P
0 F
1.83 ( position at this) 491.1 139.35 P
0.61 (standard wavelength is compared to a stored value and the dif) 207 127.35 P
0.61 (ference is applied to the) 460.05 127.35 P
1.22 (observations made with the proposal con\336guration until another) 207 115.35 P
9 F
2.91 (SPYBAL) 475.03 115.35 P
0 F
1.22 ( is done. A) 511.03 115.35 P
9 F
-0.1 (SPYBAL) 207 103.35 P
0 F
-0.04 ( is normally done before each new use of a dif) 243 103.35 P
-0.04 (ferent spectrum element, such as) 427.36 103.35 P
FMENDPAGE
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[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
2 9 Q
(Glossary of T) 189 736.18 T
(erms and Abbreviations) 245.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
2 10 Q
(1) 54 60.29 T
(14) 59.01 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 F
-0.15 (a grating. The resultant spectrum is provided to the observer and can be used to improve) 189 679.35 P
(the default wavelength calibration.) 189 667.35 T
2 F
(SSA) 171 643.35 T
0 F
0.57 (Small Science Aperture. The nominal \050pre-COST) 189 619.35 P
0.57 (AR\051 size was 0.25 arcsec square, but) 389.37 619.35 P
0.66 (after COST) 189 607.35 P
0.66 (AR it is 0.22 arcsec square. The name for this aperture will continue to be) 235.24 607.35 P
(\322) 189 595.35 T
9 F
(0.25) 193.44 595.35 T
0 F
(\323.) 217.44 595.35 T
2 F
(STEIS) 171 571.35 T
0 F
1.28 (Space T) 189 547.35 P
1.28 (elescope Electronic Information Service. This service provides on-line news,) 222.07 547.35 P
0.03 (information, and documents via anonymous ftp. T) 189 535.35 P
0.03 (o use it,) 389 535.35 P
3 F
0.03 (ftp) 422.96 535.35 P
0 F
0.03 ( to) 433.52 535.35 P
3 F
0.03 (stsci.edu) 446.36 535.35 P
0 F
0.03 (\050Internet node) 483.6 535.35 P
0.85 (130.167.1.2\051 and login with username) 189 523.35 P
3 F
0.85 (anonymous) 347.69 523.35 P
0 F
0.85 (, using your last name as password.) 393.24 523.35 P
0.42 (Use) 189 511.35 P
3 F
0.42 (get) 207.47 511.35 P
0 F
0.42 ( to transfer the README \336le in the entry directory; this will provide a general) 219.69 511.35 P
1.34 (explanation of how to access STEIS information. For more details, consult the User) 189 499.35 P
(Support Branch.) 189 487.35 T
2 F
(STEP-P) 171 463.35 T
(A) 206.38 463.35 T
(TT) 212.86 463.35 T
9 F
2.35 (STEP-PATT) 189 439.35 P
0 F
0.98 ( is the pattern of operations undertaken in an) 243 439.35 P
9 F
2.35 (ACCUM) 432.62 439.35 P
0 F
0.98 (. A typical) 462.62 439.35 P
9 F
2.35 (STEP-) 510 439.35 P
0.3 (PATT) 189 427.35 P
0 F
0.12 ( de\336nes the relative proportions of time spent accumulating on the science diodes) 213 427.35 P
(versus time with the background diodes. See Section) 189 415.35 T
(8.4 on page) 402.59 415.35 T
(92.) 451.47 415.35 T
2 F
(STEP-TIME) 171 391.35 T
0 F
-0.24 (STEP-TIME is the exposure time for the smallest unit of an exposure. For example, dur-) 189 367.35 P
0.48 (ing an acquisition,) 189 355.35 P
9 F
1.15 (STEP-TIME) 266.55 355.35 P
0 F
0.48 ( is the amount of time spent at each dwell point while) 320.55 355.35 P
-0.19 (executing a spiral search pattern. During an) 189 343.35 P
9 F
-0.47 (ACCUM) 364.26 343.35 P
0 F
-0.19 (, the detector integrates for a) 394.26 343.35 P
9 F
-0.47 (STEP-) 510 343.35 P
3.18 (TIME) 189 331.35 P
0 F
1.32 ( before reading the diodes and adding their contents to the memory) 213 331.35 P
1.32 (. A unit of) 494.92 331.35 P
9 F
(STEP-TIME) 189 319.35 T
0 F
( is spent executing each portion of a) 243 319.35 T
9 F
(STEP-PATT) 389.64 319.35 T
0 F
(, for example.) 442.9 319.35 T
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (1) 541.87 60.29 P
-2.78 (15) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
2 9 Q
(Glossary of T) 207 736.18 T
(erms and Abbreviations) 263.85 736.18 T
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 756 558 756 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 72 558 72 2 L
0.5 H
2 Z
N
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
-2.78 (1) 541.87 60.29 P
-2.78 (15) 546.88 60.29 P
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 24 Q
-0.41 (Index) 207 668 S
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
54 72 540 72 2 L
0.5 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
(1) 54 60.29 T
(16) 59.01 60.29 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(GHRS Instrument Handbook 5.0) 189 60.29 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 9 Q
(A) 54 681.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(Accumulation Mode) 54 672.33 T
(13, 19, 34, 43\32045) 132.74 672.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(CENSOR) 63 662.33 T
0 9 Q
(44) 103.5 662.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(details) 72 652.33 T
(95\32096) 100 652.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(CENSOR) 63 642.33 T
0 9 Q
(, see also noise rejection) 99 642.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(COMB) 63 632.33 T
0 9 Q
(15, 44) 91.5 632.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(DOPPLER) 63 622.33 T
0 9 Q
(44) 109.5 622.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(FP-SPLIT) 63 612.33 T
0 9 Q
(14, 30, 43, 44) 115.5 612.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(high signal-to-noise methods) 63 602.33 T
(107) 172 602.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(parameter summary) 63 592.33 T
(44) 139.23 592.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(STEP-PATT) 63 582.33 T
0 9 Q
(15, 44, 92, 1) 121.5 582.33 T
(14) 166.17 582.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(STEP-TIME) 63 572.33 T
0 9 Q
(44) 121.5 572.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(substepping) 63 562.33 T
(19) 110.5 562.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(acquisition parameters) 54 552.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(ACQ/PEAKUP) 63 542.33 T
0 9 Q
(, see acquisition parameters,) 122 542.33 T
9 10 Q
(PEAKUP) 225.98 542.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(BRIGHT) 63 532.33 T
0 9 Q
( and) 99 532.33 T
9 10 Q
(FAINT) 116.5 532.33 T
0 9 Q
( limits) 146.5 532.33 T
(17, 26, 37, 41) 173.76 532.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(calculating) 72 522.33 T
(68) 115.99 522.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(BRIGHT=RETURN) 63 512.33 T
0 9 Q
(17, 25, 34, 37, 41, 71) 145.5 512.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(BRIGHT=RETURN) 63 502.33 T
0 9 Q
( compared to specifying limits) 141 502.33 T
(37) 254.99 502.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(DEC-OFF) 63 492.33 T
0 9 Q
(40) 109.5 492.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(ETA-OFF) 63 482.33 T
0 9 Q
(40) 109.5 482.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(EXTENDED) 63 472.33 T
0 9 Q
(39) 115.5 472.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(LOCATE) 63 462.33 T
0 9 Q
(17, 41) 103.5 462.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(LOCATE=EXTENDED) 63 452.33 T
0 9 Q
(8) 157.5 452.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(MAP) 63 442.33 T
0 9 Q
(37, 40, 41, 42) 85.5 442.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(MAP=ALL-POINTS) 63 432.33 T
0 9 Q
(40) 151.5 432.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(PEAKUP) 63 422.33 T
0 9 Q
(15, 34, 38, 40, 41) 103.5 422.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(STEP-TIME) 72 412.33 T
0 9 Q
(71) 130.5 412.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(RA-OFF) 63 402.33 T
0 9 Q
(40) 103.5 402.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(SEARCH-SIZE) 63 392.33 T
0 9 Q
(36, 37, 40) 133.5 392.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Special Requirements) 63 382.33 T
(41) 146.24 382.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(STEP-TIME) 63 372.33 T
0 9 Q
(71) 121.5 372.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(for) 72 362.33 T
9 10 Q
(PEAKUP) 84.74 362.33 T
0 9 Q
(71) 125.24 362.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(maximum permitted) 72 352.33 T
(38) 149.75 352.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(STEP-TIME) 63 342.33 T
0 9 Q
(as) 123 342.33 T
9 10 Q
(COMMENT) 132.75 342.33 T
0 9 Q
(41) 179.25 342.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(summary) 63 332.33 T
(40) 101 332.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(XI-OFF) 63 322.33 T
0 9 Q
(40) 103.5 322.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(acquisitions) 54 312.33 T
(15, 17, 24, 34, 35\32041, 68\32080) 101.5 312.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(early) 63 302.33 T
(16, 18, 25, 35, 36) 85.49 302.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(extended objects) 63 292.33 T
(39, 76) 127.74 292.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(faint objects) 63 282.33 T
(39) 111.74 282.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(DARK TIME) 72 272.33 T
0 9 Q
(39, 80) 130.5 272.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Side 2 acquisition for Side 1 observing) 72 262.33 T
(8, 38) 216.49 262.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(using FOS) 72 252.33 T
(8, 39) 114.76 252.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(\337ux measurement) 63 242.33 T
(17) 131.74 242.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(initial pointing) 63 232.33 T
(35) 120.76 232.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(interactive) 63 222.33 T
(16, 18, 24, 35) 105.49 222.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(of) 63 212.33 T
(fseting) 70.33 212.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(and guide stars) 72 202.33 T
(40) 130.49 202.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(of) 63 192.33 T
(fsetting) 70.33 192.33 T
(36, 39) 101.83 192.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(onboard) 63 182.33 T
(17, 36, 40) 96.99 182.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(parameter summary) 63 172.33 T
(40) 139.23 172.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(real time, see acquisitions, interactive) 63 162.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(reddening) 63 152.33 T
(68) 103.49 152.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(see also tar) 63 142.33 T
(gets) 102.82 142.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(spiral search) 63 132.33 T
(36, 37) 112.73 132.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(tar) 63 122.33 T
(gets, see tar) 72.33 122.33 T
(gets) 114.41 122.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(apertures) 306 681.33 T
(12) 343.48 681.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(angular scale) 315 671.33 T
(9) 366.73 671.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(LSA) 315 661.33 T
(9, 12, 17, 18, 28, 34, 35, 36, 38, 41, 42, 85, 1) 336.5 661.33 T
(12) 498.17 661.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(shutter) 324 651.33 T
(12, 28) 353 651.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(nomenclature) 315 641.33 T
(9) 368.49 641.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(physical locations) 315 631.33 T
(58) 384.25 631.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(physical size) 315 621.33 T
(60) 365.74 621.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(plate scale) 315 611.33 T
(9) 357.24 611.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(SSA) 315 601.33 T
(9, 12, 17, 28, 34, 38, 41, 42, 1) 336.01 601.33 T
(14) 443.67 601.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(B) 306 582.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(background) 306 573.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(echelle interorder) 315 563.33 T
(19) 382.73 563.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(geocoronal L) 315 553.33 T
(yman-) 362.24 553.33 T
13 10 Q
(a) 385.24 553.33 T
0 9 Q
(80) 396.05 553.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(LSA shutter) 315 543.33 T
(12) 363.25 543.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(measurement) 315 533.33 T
(92) 367.49 533.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(scattered light) 315 523.33 T
(87, 88) 370.24 523.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(echelles) 324 513.33 T
(103) 357.49 513.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(bandpass) 306 503.33 T
(87, 88) 343.49 503.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(blaze function) 306 493.33 T
(91, 1) 361.74 493.33 T
(1) 379.4 493.33 T
(1) 383.57 493.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(C) 306 474.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(calibrations) 306 465.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(precision and accuracy) 315 455.33 T
(46) 401.97 455.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(wavelength) 315 445.33 T
(34, 47, 98) 360.99 445.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(aperture of) 324 435.33 T
(fsets) 363.07 435.33 T
(98) 384.07 435.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(contamination from SSA) 324 425.33 T
(98) 418.5 425.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(geomagnetic ef) 324 415.33 T
(fects) 379.07 415.33 T
(99) 400.56 415.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(lamps) 324 405.33 T
(98) 350 405.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(line widths) 324 395.33 T
(98) 368.25 395.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(tables) 324 385.33 T
(102) 349.5 385.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(thermal ef) 324 375.33 T
(fects) 360.58 375.33 T
(99) 382.07 375.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(carrousel) 306 365.33 T
(14) 343.48 365.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(CENSOR) 306 355.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 9 Q
(see noise rejection) 315 345.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Continuous V) 306 335.33 T
(iewing Zone) 355.72 335.33 T
(16, 1) 405.46 335.33 T
(12) 423.13 335.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(conventions) 306 325.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(text) 315 315.33 T
(7) 333 315.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(units) 315 305.33 T
(8) 337.01 305.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(coordinated observations) 306 295.33 T
(47) 400.73 295.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(cosmic rays) 306 285.33 T
(95) 353.24 285.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(CVZ, see Continuous V) 306 275.33 T
(iewing Zone) 391.96 275.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Cycle 5) 306 265.33 T
(1) 338.25 265.33 T
(1) 342.41 265.33 T
(1) 346.58 265.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(D) 306 246.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(DARK TIME) 306 237.33 T
0 9 Q
( Special Requirement) 360 237.33 T
(39, 80) 441.99 237.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(data quality) 306 227.33 T
(43) 352.75 227.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(deadtime correction) 306 217.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(see paired pulse correction) 315 207.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(deconvolution) 306 197.33 T
(103) 362 197.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(DEFCAL) 306 187.33 T
0 9 Q
(1) 346.5 187.33 T
(12) 350.67 187.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(detectors) 306 177.33 T
(60) 342.99 177.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(count rate linearity) 315 167.33 T
(98) 387.49 167.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(D1) 315 157.33 T
(14) 330.5 157.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(D2) 315 147.33 T
(14) 330.5 147.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(dark count) 315 137.33 T
(95) 357.74 137.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Digicon, see Digicon) 315 127.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(granularity) 315 117.33 T
(14) 358.99 117.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(image stability) 315 107.33 T
(98) 372.75 107.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(sampling) 315 97.33 T
(15) 352.5 97.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
72 72 558 72 2 L
0.5 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
-2.78 (1) 541.87 60.29 P
-2.78 (17) 546.88 60.29 P
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 9 Q
(Digicon) 72 681.33 T
(14) 105.5 681.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(paired pulse correction) 81 671.33 T
(71) 167.98 671.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(diodes) 72 661.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(corner) 81 651.33 T
(28, 92) 108.49 651.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(focus) 81 641.33 T
(42, 43, 1) 104.99 641.33 T
(12) 136.16 641.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(science) 81 631.33 T
(92) 111.99 631.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(diodes, corner) 72 621.33 T
(1) 127.49 621.33 T
(1) 131.65 621.33 T
(1) 135.82 621.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Doppler shift) 72 611.33 T
(19, 44, 46) 124.25 611.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(E) 72 592.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(early acquisition, see acquisitions, early) 72 583.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(e-mail addresses) 72 573.33 T
(2) 136.23 573.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(exposure time calculation) 72 563.33 T
(26) 168.98 563.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(extinction, ultraviolet) 72 553.33 T
(93, 102) 154 553.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(F) 72 534.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(\337uxes, variable) 72 525.33 T
(18) 131.49 525.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(FLYLIM) 72 515.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 9 Q
(see noise rejection) 81 505.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(FOC) 72 495.33 T
(18, 24, 35, 36, 43) 94 495.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(G) 72 476.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(geocoronal L) 72 467.33 T
(yman-) 119.24 467.33 T
13 10 Q
(a) 142.24 467.33 T
0 9 Q
(27, 80, 105) 153.05 467.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(geomagnetically-induced image motion) 72 457.33 T
(47, 98, 1) 219.48 457.33 T
(12) 250.65 457.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(GHRS) 72 447.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(as slitless spectrograph) 81 437.33 T
(43) 168.49 437.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(paired pulse correction) 81 427.33 T
(71) 167.98 427.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(photometric precision) 81 417.33 T
(13) 164.24 417.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Point Spread Function) 81 407.33 T
(94) 166.01 407.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(resolving power) 81 397.33 T
(12, 83, 103) 143.74 397.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(scienti\336c papers) 81 387.33 T
(104) 143.74 387.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(STScI contacts) 81 377.33 T
(2) 139.74 377.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(technical papers) 81 367.33 T
(102) 143.73 367.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(time resolution) 81 357.33 T
(13) 139.75 357.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(useful wavelength range) 81 347.33 T
(12) 173.48 347.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(granularity) 72 337.33 T
(14) 115.99 337.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(gratings) 72 327.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(cross-dispersers) 81 317.33 T
(60) 142.98 317.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Ech-A) 81 307.33 T
(87) 108.99 307.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Ech-B) 81 297.33 T
(88) 108.5 297.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(echelle) 81 287.33 T
(12, 14, 60) 110.99 287.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(bandpass and sensitivity) 90 277.33 T
(87) 182 277.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(blaze function) 90 267.33 T
(91, 1) 145.74 267.33 T
(1) 163.4 267.33 T
(1) 167.57 267.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(resolving power) 90 257.33 T
(83) 152.74 257.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(scattered light) 90 247.33 T
(87) 145.24 247.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(wavelength format) 90 237.33 T
(89) 162.23 237.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(\336rst-order) 81 227.33 T
(12, 14, 60, 85) 121.49 227.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(resolving power) 90 217.33 T
(83) 152.74 217.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(useful ranges) 90 207.33 T
(83) 142.24 207.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(holographic) 81 197.33 T
(14) 128.49 197.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(GSC) 72 187.33 T
(35, 1) 94 187.33 T
(12) 111.67 187.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(H) 72 168.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(HST memory capacity) 72 159.33 T
(13, 16, 47) 157.99 159.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(I) 324 681.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(IMAGE Mode) 324 672.33 T
(16, 20, 40, 42\32043) 381.24 672.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(as slitless spectrograph) 333 662.33 T
(43) 420.49 662.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(critically sampling) 333 652.33 T
(42) 404.75 652.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(DELTA-X, DELTA-Y) 333 642.33 T
0 9 Q
(42) 433.5 642.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(maximum) 333 632.33 T
9 10 Q
(STEP-TIME) 371.75 632.33 T
0 9 Q
(43) 430.25 632.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(NX, NY) 333 622.33 T
0 9 Q
(42) 373.5 622.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(parameter summary) 333 612.33 T
(42) 409.23 612.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(PRECISION) 333 602.33 T
0 9 Q
(43) 391.5 602.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(interactive acquisitions, see acquisitions, interactive) 324 592.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(L) 324 573.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(Lar) 324 564.33 T
(ge Science Aperture, see apertures, LSA) 336.33 564.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Line Spread Function \050LSF\051) 324 554.33 T
(103) 430.24 554.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(M) 324 535.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(MAP) 324 526.33 T
(, see acquisition parameters,) 342.5 526.33 T
9 10 Q
(MAP) 446.48 526.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 9 Q
(mirrors) 324 516.33 T
(36, 40, 42, 60) 355 516.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(A1) 333 506.33 T
(14, 25) 348.5 506.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(A2) 333 496.33 T
(14) 348.5 496.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(attenuated) 333 486.33 T
(14) 374.49 486.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Cam-A) 333 476.33 T
(14) 364 476.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Cam-B) 333 466.33 T
(14) 363.5 466.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(ef) 333 456.33 T
(fective areas) 339.83 456.33 T
(78) 389.56 456.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(N1) 333 446.33 T
(14) 348.5 446.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(N2) 333 436.33 T
(14) 348.5 436.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(normal) 333 426.33 T
(14) 363 426.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(moving tar) 324 416.33 T
(ges, see tar) 363.09 416.33 T
(gets, moving) 402.66 416.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(N) 324 397.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(NO GAP) 324 388.33 T
0 9 Q
( Special Requirement) 360 388.33 T
(34) 441.99 388.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(noise rejection) 324 378.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(CENSOR) 333 368.33 T
0 9 Q
(27, 95) 373.5 368.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(FLYLIM) 333 358.33 T
0 9 Q
(9, 27, 45, 97) 373.5 358.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(noise, \336xed-pattern) 324 348.33 T
(30) 397.99 348.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(O) 324 329.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(OSCAN Mode) 324 320.33 T
(20, 45) 382.25 320.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(see also parameters for Accumulation Mode) 333 310.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(OSS) 324 300.33 T
(1) 345.01 300.33 T
(12) 349.17 300.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(P) 324 281.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(paired pulse correction) 324 272.33 T
(71) 410.98 272.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(peakup, see acquisition parameters,) 324 262.33 T
9 10 Q
(PEAKUP) 453.97 262.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 9 Q
(Phase I) 324 252.33 T
(22, 1) 354.74 252.33 T
(13) 372.41 252.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(acquisitions) 333 242.33 T
(24) 380.5 242.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Phase II) 324 232.33 T
(22, 1) 357.74 232.33 T
(13) 375.41 232.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(photometric precision) 324 222.33 T
(13) 407.24 222.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(plate scale) 324 212.33 T
(9) 366.24 212.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Point Spread Function) 324 202.33 T
(94, 103) 409.01 202.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(R) 324 183.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(RAPID Mode) 324 174.33 T
(13, 16, 20, 45, 46) 378.75 174.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(SAMPLE-TIME) 333 164.33 T
0 9 Q
(20, 46) 403.5 164.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Rapid Readout Mode, see RAPID Mode) 324 154.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(reddening) 324 144.33 T
(27, 93, 102) 364.49 144.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(ef) 333 134.33 T
(fect on acquisition count rates) 339.83 134.33 T
(68) 452.31 134.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(resolution, time) 324 124.33 T
(13) 385 124.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(resolving power) 324 114.33 T
(12, 83) 386.74 114.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(ripple function) 324 104.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(see blaze function) 333 94.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
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612 792 0 FMBEGINPAGE
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[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
54 72 540 72 2 L
0.5 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
(1) 54 60.29 T
(18) 59.01 60.29 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(GHRS Instrument Handbook 5.0) 189 60.29 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 9 Q
(S) 54 681.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(SAA, see South Atlantic Anomaly) 54 672.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(sampling) 54 662.33 T
(15) 91.5 662.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(scattered light) 54 652.33 T
(28, 87, 88) 109.24 652.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(SEARCH-SIZE) 54 642.33 T
0 9 Q
(, see acquisition parameters,) 120 642.33 T
9 10 Q
(SEARCH-) 223.98 642.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(SIZE) 72 632.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 9 Q
(sensitivity) 54 622.33 T
(26) 95.51 622.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(sensitivity function) 54 612.33 T
(85) 127.75 612.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Side 1) 54 602.33 T
(8, 12, 1) 81.25 602.33 T
(13) 107.92 602.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Side 2) 54 592.33 T
(12, 1) 81.25 592.33 T
(13) 98.92 592.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(signal-to-noise estimation) 54 582.33 T
(29) 151.75 582.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(slitless spectrograph mode) 54 572.33 T
(43) 153.99 572.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Small Science Aperture, see apertures, SSA) 54 562.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(South Atlantic Anomaly) 54 552.33 T
(16, 19, 27, 95, 1) 146.5 552.33 T
(13) 204.67 552.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(spectrograph temperature) 54 542.33 T
(47) 150.22 542.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Spectrum Y Balance, see) 54 532.33 T
9 10 Q
(SPYBAL) 146.73 532.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 9 Q
(spiral search, see acquisitions, spiral search) 54 522.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(SPYBAL) 54 512.33 T
0 9 Q
(19, 1) 94.5 512.33 T
(13) 112.17 512.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(STEIS) 54 502.33 T
(10, 1) 82.5 502.33 T
(14) 100.17 502.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(STEP-TIME) 54 492.33 T
0 9 Q
(1) 112.5 492.33 T
(14) 116.67 492.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(substepping) 54 482.33 T
(92) 101.5 482.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(T) 54 463.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(tar) 54 454.33 T
(gets) 63.33 454.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(bright problems) 63 444.33 T
(25) 124.75 444.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(complex) 63 434.33 T
(38) 98.5 434.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(coordinates) 63 424.33 T
(18) 108.99 424.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(crowded \336elds) 63 414.33 T
(25, 35) 120.24 414.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(extended) 63 404.33 T
(8, 18, 26) 99.99 404.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(faint) 63 394.33 T
(26, 39) 84 394.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(moving) 63 384.33 T
(18, 25, 35) 95 384.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(nearby neighbors) 63 374.33 T
(18) 129.74 374.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(of) 63 364.33 T
(fsetting) 70.33 364.33 T
(36, 39) 101.83 364.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(point source) 63 354.33 T
(36) 111.74 354.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(variable) 63 344.33 T
(18, 26, 35) 96.49 344.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(T) 54 334.33 T
(ar) 58.87 334.33 T
(gets of Opportunity) 65.7 334.33 T
(47) 140.7 334.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(telephone numbers) 54 324.33 T
(2) 126.74 324.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(time resolution) 54 314.33 T
(13) 112.75 314.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(W) 54 295.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(wavelength tables) 54 286.33 T
(102) 123.24 286.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(WFPC2) 54 276.33 T
(18, 24, 35, 36) 87.51 276.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(WSCAN Mode) 54 266.33 T
(20, 45) 114.25 266.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(see also parameters for Accumulation Mode) 63 256.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
9 10 Q
(WAVE-STEP) 63 246.33 T
0 9 Q
(45) 121.5 246.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
FMENDPAGE
%%EndPage: "118" 119
%%Trailer
%%BoundingBox: 0 0 612 792
%%PageOrder: Ascend
%%Pages: 119
%%DocumentFonts: Times-Roman
%%+ Times-Bold
%%+ Helvetica-Bold
%%+ Times-Italic
%%+ Helvetica
%%+ Palatino-Italic
%%+ Helvetica-BoldOblique
%%+ Palatino-BoldItalic
%%+ Helvetica-Oblique
%%+ Courier
%%+ Courier-Bold
%%+ AvantGarde-Book
%%+ AvantGarde-BookOblique
%%+ Symbol
%%+ ZapfChancery-MediumItalic
%%+ AvantGarde-Demi
%%+ Courier-Oblique
%%EOF
%!PS-Adobe-3.0
%%BoundingBox: (atend)
%%Pages: (atend)
%%PageOrder: (atend)
%%DocumentFonts: (atend)
%%Creator: Frame 4.0
%%DocumentData: Clean7Bit
%%EndComments
%%BeginProlog
%
% Frame ps_prolog 4.0, for use with Frame 4.0 products
% This ps_prolog file is Copyright (c) 1986-1993 Frame Technology
% Corporation. All rights reserved. This ps_prolog file may be
% freely copied and distributed in conjunction with documents created
% using FrameMaker, FrameBuilder and FrameViewer as long as this
% copyright notice is preserved.
%
% Frame products normally print colors as their true color on a color printer
% or as shades of gray, based on luminance, on a black-and white printer. The
% following flag, if set to True, forces all non-white colors to print as pure
% black. This has no effect on bitmap images.
/FMPrintAllColorsAsBlack false def
%
% Frame products can either set their own line screens or use a printer's
% default settings. Three flags below control this separately for no
% separations, spot separations and process separations. If a flag
% is true, then the default printer settings will not be changed. If it is
% false, Frame products will use their own settings from a table based on
% the printer's resolution.
/FMUseDefaultNoSeparationScreen true def
/FMUseDefaultSpotSeparationScreen true def
/FMUseDefaultProcessSeparationScreen false def
%
% For any given PostScript printer resolution, Frame products have two sets of
% screen angles and frequencies for printing process separations, which are
% recomended by Adobe. The following variable chooses the higher frequencies
% when set to true or the lower frequencies when set to false. This is only
% effective if the appropriate FMUseDefault...SeparationScreen flag is false.
/FMUseHighFrequencyScreens true def
%
% PostScript Level 2 printers contain an "Accurate Screens" feature which can
% improve process separation rendering at the expense of compute time. This
% flag is ignored by PostScript Level 1 printers.
/FMUseAcccurateScreens true def
%
% The following PostScript procedure defines the spot function that Frame
% products will use for process separations. You may un-comment-out one of
% the alternative functions below, or use your own.
%
% Dot function
/FMSpotFunction {abs exch abs 2 copy add 1 gt
{1 sub dup mul exch 1 sub dup mul add 1 sub }
{dup mul exch dup mul add 1 exch sub }ifelse } def
%
% Line function
% /FMSpotFunction { pop } def
%
% Elipse function
% /FMSpotFunction { dup 5 mul 8 div mul exch dup mul exch add
% sqrt 1 exch sub } def
%
%
/FMversion (4.0) def
/FMLevel1 /languagelevel where {pop languagelevel} {1} ifelse 2 lt def
/FMPColor
FMLevel1 {
false
/colorimage where {pop pop true} if
} {
true
} ifelse
def
/FrameDict 400 dict def
systemdict /errordict known not {/errordict 10 dict def
errordict /rangecheck {stop} put} if
% The readline in PS 23.0 doesn't recognize cr's as nl's on AppleTalk
FrameDict /tmprangecheck errordict /rangecheck get put
errordict /rangecheck {FrameDict /bug true put} put
FrameDict /bug false put
mark
% Some PS machines read past the CR, so keep the following 3 lines together!
currentfile 5 string readline
00
0000000000
cleartomark
errordict /rangecheck FrameDict /tmprangecheck get put
FrameDict /bug get {
/readline {
/gstring exch def
/gfile exch def
/gindex 0 def
{
gfile read pop
dup 10 eq {exit} if
dup 13 eq {exit} if
gstring exch gindex exch put
/gindex gindex 1 add def
} loop
pop
gstring 0 gindex getinterval true
} bind def
} if
/FMshowpage /showpage load def
/FMquit /quit load def
/FMFAILURE {
dup = flush
FMshowpage
/Helvetica findfont 12 scalefont setfont
72 200 moveto
show FMshowpage
FMquit
} def
/FMVERSION {
FMversion ne {
(Frame product version does not match ps_prolog!) FMFAILURE
} if
} def
/FMBADEPSF {
(PostScript Lang. Ref. Man., 2nd Ed., H.2.4 says EPS must not call X )
dup dup (X) search pop exch pop exch pop length
4 -1 roll
putinterval
FMFAILURE
} def
/FMLOCAL {
FrameDict begin
0 def
end
} def
/concatprocs
{
/proc2 exch cvlit def/proc1 exch cvlit def/newproc proc1 length proc2 length add array def
newproc 0 proc1 putinterval newproc proc1 length proc2 putinterval newproc cvx
}def
FrameDict begin
/FMnone 0 def
/FMcyan 1 def
/FMmagenta 2 def
/FMyellow 3 def
/FMblack 4 def
/FMcustom 5 def
/FrameNegative false def
/FrameSepIs FMnone def
/FrameSepBlack 0 def
/FrameSepYellow 0 def
/FrameSepMagenta 0 def
/FrameSepCyan 0 def
/FrameSepRed 1 def
/FrameSepGreen 1 def
/FrameSepBlue 1 def
/FrameCurGray 1 def
/FrameCurPat null def
/FrameCurColors [ 0 0 0 1 0 0 0 ] def
/FrameColorEpsilon .001 def
/eqepsilon {
sub dup 0 lt {neg} if
FrameColorEpsilon le
} bind def
/FrameCmpColorsCMYK {
2 copy 0 get exch 0 get eqepsilon {
2 copy 1 get exch 1 get eqepsilon {
2 copy 2 get exch 2 get eqepsilon {
3 get exch 3 get eqepsilon
} {pop pop false} ifelse
}{pop pop false} ifelse
} {pop pop false} ifelse
} bind def
/FrameCmpColorsRGB {
2 copy 4 get exch 0 get eqepsilon {
2 copy 5 get exch 1 get eqepsilon {
6 get exch 2 get eqepsilon
}{pop pop false} ifelse
} {pop pop false} ifelse
} bind def
/RGBtoCMYK {
1 exch sub
3 1 roll
1 exch sub
3 1 roll
1 exch sub
3 1 roll
3 copy
2 copy
le { pop } { exch pop } ifelse
2 copy
le { pop } { exch pop } ifelse
dup dup dup
6 1 roll
4 1 roll
7 1 roll
sub
6 1 roll
sub
5 1 roll
sub
4 1 roll
} bind def
/CMYKtoRGB {
dup dup 4 -1 roll add
5 1 roll 3 -1 roll add
4 1 roll add
1 exch sub dup 0 lt {pop 0} if 3 1 roll
1 exch sub dup 0 lt {pop 0} if exch
1 exch sub dup 0 lt {pop 0} if exch
} bind def
/FrameSepInit {
1.0 RealSetgray
} bind def
/FrameSetSepColor {
/FrameSepBlue exch def
/FrameSepGreen exch def
/FrameSepRed exch def
/FrameSepBlack exch def
/FrameSepYellow exch def
/FrameSepMagenta exch def
/FrameSepCyan exch def
/FrameSepIs FMcustom def
setCurrentScreen
} bind def
/FrameSetCyan {
/FrameSepBlue 1.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 1.0 def
/FrameSepIs FMcyan def
setCurrentScreen
} bind def

/FrameSetMagenta {
/FrameSepBlue 1.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 1.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMmagenta def
setCurrentScreen
} bind def

/FrameSetYellow {
/FrameSepBlue 0.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 1.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMyellow def
setCurrentScreen
} bind def

/FrameSetBlack {
/FrameSepBlue 0.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 1.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMblack def
setCurrentScreen
} bind def

/FrameNoSep {
/FrameSepIs FMnone def
setCurrentScreen
} bind def
/FrameSetSepColors {
FrameDict begin
[ exch 1 add 1 roll ]
/FrameSepColors
exch def end
} bind def
/FrameColorInSepListCMYK {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsCMYK
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/FrameColorInSepListRGB {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsRGB
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/RealSetgray /setgray load def
/RealSetrgbcolor /setrgbcolor load def
/RealSethsbcolor /sethsbcolor load def
end
/setgray {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetgray }
{
FrameSepIs FMblack eq
{ RealSetgray }
{ FrameSepIs FMcustom eq
FrameSepRed 0 eq and
FrameSepGreen 0 eq and
FrameSepBlue 0 eq and {
RealSetgray
} {
1 RealSetgray pop
} ifelse
} ifelse
} ifelse
end
} bind def
/setrgbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetrgbcolor }
{
3 copy [ 4 1 roll ]
FrameColorInSepListRGB
{
FrameSepBlue eq exch
FrameSepGreen eq and exch
FrameSepRed eq and
{ 0 } { 1 } ifelse
}
{
FMPColor {
RealSetrgbcolor
currentcmykcolor
} {
RGBtoCMYK
} ifelse
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
RealSetgray
}
ifelse
end
} bind def
/sethsbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSethsbcolor }
{
RealSethsbcolor
currentrgbcolor
setrgbcolor
}
ifelse
end
} bind def
FrameDict begin
/setcmykcolor where {
pop /RealSetcmykcolor /setcmykcolor load def
} {
/RealSetcmykcolor {
4 1 roll
3 { 3 index add 0 max 1 min 1 exch sub 3 1 roll} repeat
setrgbcolor pop
} bind def
} ifelse
userdict /setcmykcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetcmykcolor }
{
4 copy [ 5 1 roll ]
FrameColorInSepListCMYK
{
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
{ 0 } { 1 } ifelse
}
{
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
RealSetgray
}
ifelse
end
} bind put
FMLevel1 not {

/patProcDict 5 dict dup begin
<0f1e3c78f0e1c387> { 3 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<0f87c3e1f0783c1e> { 3 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
<8142241818244281> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-1 -1 moveto 9 9 lineto stroke } bind def
<03060c183060c081> { 1 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<8040201008040201> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
end def
/patDict 15 dict dup begin
/PatternType 1 def
/PaintType 2 def
/TilingType 3 def
/BBox [ 0 0 8 8 ] def
/XStep 8 def
/YStep 8 def
/PaintProc {
begin
patProcDict bstring known {
patProcDict bstring get exec
} {
8 8 true [1 0 0 -1 0 8] bstring imagemask
} ifelse
end
} bind def
end def
} if
/combineColor {
FrameSepIs FMnone eq
{
graymode FMLevel1 or not {

[/Pattern [/DeviceCMYK]] setcolorspace
FrameCurColors 0 4 getinterval aload pop FrameCurPat setcolor
} {
FrameCurColors 3 get 1.0 ge {
FrameCurGray RealSetgray
} {
FMPColor graymode and {
0 1 3 {
FrameCurColors exch get
1 FrameCurGray sub mul
} for
RealSetcmykcolor
} {
4 1 6 {
FrameCurColors exch get
graymode {
1 exch sub 1 FrameCurGray sub mul 1 exch sub
} {
1.0 lt {FrameCurGray} {1} ifelse
} ifelse
} for
RealSetrgbcolor
} ifelse
} ifelse
} ifelse
} {
FrameCurColors 0 4 getinterval aload
FrameColorInSepListCMYK {
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
FrameSepIs FMcustom eq and
{ FrameCurGray } { 1 } ifelse
} {
FrameSepIs FMblack eq
{FrameCurGray 1.0 exch sub mul 1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop FrameCurGray 1.0 exch sub mul 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
graymode FMLevel1 or not {

[/Pattern [/DeviceGray]] setcolorspace
FrameCurPat setcolor
} {
graymode not FMLevel1 and {

dup 1 lt {pop FrameCurGray} if
} if
RealSetgray
} ifelse
} ifelse
} bind def
/savematrix {
orgmatrix currentmatrix pop
} bind def
/restorematrix {
orgmatrix setmatrix
} bind def
/dmatrix matrix def
/dpi 72 0 dmatrix defaultmatrix dtransform
dup mul exch dup mul add sqrt def

/freq dpi dup 72 div round dup 0 eq {pop 1} if 8 mul div def
/sangle 1 0 dmatrix defaultmatrix dtransform exch atan def
/dpiranges [ 2540 2400 1693 1270 1200 635 600 0 ] def
/CMLowFreqs [ 100.402 94.8683 89.2289 100.402 94.8683 66.9349 63.2456 47.4342 ] def
/YLowFreqs [ 95.25 90.0 84.65 95.25 90.0 70.5556 66.6667 50.0 ] def
/KLowFreqs [ 89.8026 84.8528 79.8088 89.8026 84.8528 74.8355 70.7107 53.033 ] def
/CLowAngles [ 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 ] def
/MLowAngles [ 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 ] def
/YLowTDot [ true true false true true false false false ] def
/CMHighFreqs [ 133.87 126.491 133.843 108.503 102.523 100.402 94.8683 63.2456 ] def
/YHighFreqs [ 127.0 120.0 126.975 115.455 109.091 95.25 90.0 60.0 ] def
/KHighFreqs [ 119.737 113.137 119.713 128.289 121.218 89.8026 84.8528 63.6395 ] def
/CHighAngles [ 71.5651 71.5651 71.5651 70.0169 70.0169 71.5651 71.5651 71.5651 ] def
/MHighAngles [ 18.4349 18.4349 18.4349 19.9831 19.9831 18.4349 18.4349 18.4349 ] def
/YHighTDot [ false false true false false true true false ] def
/PatFreq [ 10.5833 10.0 9.4055 10.5833 10.0 10.5833 10.0 9.375 ] def
/screenIndex {
0 1 dpiranges length 1 sub { dup dpiranges exch get 1 sub dpi le {exit} {pop} ifelse } for
} bind def
/getCyanScreen {
FMUseHighFrequencyScreens { CHighAngles CMHighFreqs} {CLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getMagentaScreen {
FMUseHighFrequencyScreens { MHighAngles CMHighFreqs } {MLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getYellowScreen {
FMUseHighFrequencyScreens { YHighTDot YHighFreqs} { YLowTDot YLowFreqs } ifelse
screenIndex dup 3 1 roll get 3 1 roll get { 3 div
{2 { 1 add 2 div 3 mul dup floor sub 2 mul 1 sub exch} repeat
FMSpotFunction } } {/FMSpotFunction load } ifelse
0.0 exch
} bind def
/getBlackScreen {
FMUseHighFrequencyScreens { KHighFreqs } { KLowFreqs } ifelse
screenIndex get 45.0 /FMSpotFunction load
} bind def
/getSpotScreen {
getBlackScreen
} bind def
/getCompositeScreen {
getBlackScreen
} bind def
/FMSetScreen
FMLevel1 { /setscreen load
}{ {
8 dict begin
/HalftoneType 1 def
/SpotFunction exch def
/Angle exch def
/Frequency exch def
/AccurateScreens FMUseAcccurateScreens def
currentdict end sethalftone
} bind } ifelse
def
/setDefaultScreen {
FMPColor {
orgrxfer cvx orggxfer cvx orgbxfer cvx orgxfer cvx setcolortransfer
}
{
orgxfer cvx settransfer
} ifelse
orgfreq organgle orgproc cvx setscreen
} bind def
/setCurrentScreen {
FrameSepIs FMnone eq {
FMUseDefaultNoSeparationScreen {
setDefaultScreen
} {
getCompositeScreen FMSetScreen
} ifelse
} {
FrameSepIs FMcustom eq {
FMUseDefaultSpotSeparationScreen {
setDefaultScreen
} {
getSpotScreen FMSetScreen
} ifelse
} {
FMUseDefaultProcessSeparationScreen {
setDefaultScreen
} {
FrameSepIs FMcyan eq {
getCyanScreen FMSetScreen
} {
FrameSepIs FMmagenta eq {
getMagentaScreen FMSetScreen
} {
FrameSepIs FMyellow eq {
getYellowScreen FMSetScreen
} {
getBlackScreen FMSetScreen
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} bind def
end
/gstring FMLOCAL
/gfile FMLOCAL
/gindex FMLOCAL
/orgrxfer FMLOCAL
/orggxfer FMLOCAL
/orgbxfer FMLOCAL
/orgxfer FMLOCAL
/orgproc FMLOCAL
/orgrproc FMLOCAL
/orggproc FMLOCAL
/orgbproc FMLOCAL
/organgle FMLOCAL
/orgrangle FMLOCAL
/orggangle FMLOCAL
/orgbangle FMLOCAL
/orgfreq FMLOCAL
/orgrfreq FMLOCAL
/orggfreq FMLOCAL
/orgbfreq FMLOCAL
/yscale FMLOCAL
/xscale FMLOCAL
/edown FMLOCAL
/manualfeed FMLOCAL
/paperheight FMLOCAL
/paperwidth FMLOCAL
/FMDOCUMENT {
array /FMfonts exch def
/#copies exch def
FrameDict begin
0 ne /manualfeed exch def
/paperheight exch def
/paperwidth exch def
0 ne /FrameNegative exch def
0 ne /edown exch def
/yscale exch def
/xscale exch def
FMLevel1 {
manualfeed {setmanualfeed} if
/FMdicttop countdictstack 1 add def
/FMoptop count def
% setpapername
% manualfeed {true} {papersize} ifelse
% {manualpapersize} {false} ifelse
% {desperatepapersize} {false} ifelse
% { (Can't select requested paper size for Frame print job!) FMFAILURE } if
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
}
{{1 dict dup /PageSize [paperwidth paperheight]put setpagedevice}stopped
{ (Can't select requested paper size for Frame print job!) FMFAILURE } if
{1 dict dup /ManualFeed manualfeed put setpagedevice } stopped pop }
ifelse

FMPColor {
currentcolorscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def
cvlit /orgbproc exch def
/orgbangle exch def
/orgbfreq exch def
cvlit /orggproc exch def
/orggangle exch def
/orggfreq exch def
cvlit /orgrproc exch def
/orgrangle exch def
/orgrfreq exch def
currentcolortransfer
FrameNegative {
1 1 4 {
pop { 1 exch sub } concatprocs 4 1 roll
} for
4 copy
setcolortransfer
} if
cvlit /orgxfer exch def
cvlit /orgbxfer exch def
cvlit /orggxfer exch def
cvlit /orgrxfer exch def
} {
currentscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def

currenttransfer
FrameNegative {
{ 1 exch sub } concatprocs
dup settransfer
} if
cvlit /orgxfer exch def
} ifelse
end
} def
/pagesave FMLOCAL
/orgmatrix FMLOCAL
/landscape FMLOCAL
/pwid FMLOCAL
/FMBEGINPAGE {
FrameDict begin
/pagesave save def
3.86 setmiterlimit
/landscape exch 0 ne def
landscape {
90 rotate 0 exch dup /pwid exch def neg translate pop
}{
pop /pwid exch def
} ifelse
edown { [-1 0 0 1 pwid 0] concat } if
0 0 moveto paperwidth 0 lineto paperwidth paperheight lineto
0 paperheight lineto 0 0 lineto 1 setgray fill
xscale yscale scale
/orgmatrix matrix def
gsave
} def
/FMENDPAGE {
grestore
pagesave restore
end
showpage
} def
/FMFONTDEFINE {
FrameDict begin
findfont
ReEncode
1 index exch
definefont
FMfonts 3 1 roll
put
end
} def
/FMFILLS {
FrameDict begin dup
array /fillvals exch def
dict /patCache exch def
end
} def
/FMFILL {
FrameDict begin
fillvals 3 1 roll put
end
} def
/FMNORMALIZEGRAPHICS {
newpath
0.0 0.0 moveto
1 setlinewidth
0 setlinecap
0 0 0 sethsbcolor
0 setgray
} bind def
/fx FMLOCAL
/fy FMLOCAL
/fh FMLOCAL
/fw FMLOCAL
/llx FMLOCAL
/lly FMLOCAL
/urx FMLOCAL
/ury FMLOCAL
/FMBEGINEPSF {
end
/FMEPSF save def
/showpage {} def
% See Adobe's "PostScript Language Reference Manual, 2nd Edition", page 714.
% "...the following operators MUST NOT be used in an EPS file:" (emphasis ours)
/banddevice {(banddevice) FMBADEPSF} def
/clear {(clear) FMBADEPSF} def
/cleardictstack {(cleardictstack) FMBADEPSF} def
/copypage {(copypage) FMBADEPSF} def
/erasepage {(erasepage) FMBADEPSF} def
/exitserver {(exitserver) FMBADEPSF} def
/framedevice {(framedevice) FMBADEPSF} def
/grestoreall {(grestoreall) FMBADEPSF} def
/initclip {(initclip) FMBADEPSF} def
/initgraphics {(initgraphics) FMBADEPSF} def
/initmatrix {(initmatrix) FMBADEPSF} def
/quit {(quit) FMBADEPSF} def
/renderbands {(renderbands) FMBADEPSF} def
/setglobal {(setglobal) FMBADEPSF} def
/setpagedevice {(setpagedevice) FMBADEPSF} def
/setshared {(setshared) FMBADEPSF} def
/startjob {(startjob) FMBADEPSF} def
/lettertray {(lettertray) FMBADEPSF} def
/letter {(letter) FMBADEPSF} def
/lettersmall {(lettersmall) FMBADEPSF} def
/11x17tray {(11x17tray) FMBADEPSF} def
/11x17 {(11x17) FMBADEPSF} def
/ledgertray {(ledgertray) FMBADEPSF} def
/ledger {(ledger) FMBADEPSF} def
/legaltray {(legaltray) FMBADEPSF} def
/legal {(legal) FMBADEPSF} def
/statementtray {(statementtray) FMBADEPSF} def
/statement {(statement) FMBADEPSF} def
/executivetray {(executivetray) FMBADEPSF} def
/executive {(executive) FMBADEPSF} def
/a3tray {(a3tray) FMBADEPSF} def
/a3 {(a3) FMBADEPSF} def
/a4tray {(a4tray) FMBADEPSF} def
/a4 {(a4) FMBADEPSF} def
/a4small {(a4small) FMBADEPSF} def
/b4tray {(b4tray) FMBADEPSF} def
/b4 {(b4) FMBADEPSF} def
/b5tray {(b5tray) FMBADEPSF} def
/b5 {(b5) FMBADEPSF} def
FMNORMALIZEGRAPHICS
[/fy /fx /fh /fw /ury /urx /lly /llx] {exch def} forall
fx fw 2 div add fy fh 2 div add translate
rotate
fw 2 div neg fh 2 div neg translate
fw urx llx sub div fh ury lly sub div scale
llx neg lly neg translate
/FMdicttop countdictstack 1 add def
/FMoptop count def
} bind def
/FMENDEPSF {
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
FMEPSF restore
FrameDict begin
} bind def
FrameDict begin
/setmanualfeed {
%%BeginFeature *ManualFeed True
statusdict /manualfeed true put
%%EndFeature
} bind def
/max {2 copy lt {exch} if pop} bind def
/min {2 copy gt {exch} if pop} bind def
/inch {72 mul} def
/pagedimen {
paperheight sub abs 16 lt exch
paperwidth sub abs 16 lt and
{/papername exch def} {pop} ifelse
} bind def
/papersizedict FMLOCAL
/setpapername {
/papersizedict 14 dict def
papersizedict begin
/papername /unknown def
/Letter 8.5 inch 11.0 inch pagedimen
/LetterSmall 7.68 inch 10.16 inch pagedimen
/Tabloid 11.0 inch 17.0 inch pagedimen
/Ledger 17.0 inch 11.0 inch pagedimen
/Legal 8.5 inch 14.0 inch pagedimen
/Statement 5.5 inch 8.5 inch pagedimen
/Executive 7.5 inch 10.0 inch pagedimen
/A3 11.69 inch 16.5 inch pagedimen
/A4 8.26 inch 11.69 inch pagedimen
/A4Small 7.47 inch 10.85 inch pagedimen
/B4 10.125 inch 14.33 inch pagedimen
/B5 7.16 inch 10.125 inch pagedimen
end
} bind def
/papersize {
papersizedict begin
/Letter {lettertray letter} def
/LetterSmall {lettertray lettersmall} def
/Tabloid {11x17tray 11x17} def
/Ledger {ledgertray ledger} def
/Legal {legaltray legal} def
/Statement {statementtray statement} def
/Executive {executivetray executive} def
/A3 {a3tray a3} def
/A4 {a4tray a4} def
/A4Small {a4tray a4small} def
/B4 {b4tray b4} def
/B5 {b5tray b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
statusdict begin stopped end
} bind def
/manualpapersize {
papersizedict begin
/Letter {letter} def
/LetterSmall {lettersmall} def
/Tabloid {11x17} def
/Ledger {ledger} def
/Legal {legal} def
/Statement {statement} def
/Executive {executive} def
/A3 {a3} def
/A4 {a4} def
/A4Small {a4small} def
/B4 {b4} def
/B5 {b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
stopped
} bind def
/desperatepapersize {
statusdict /setpageparams known
{
paperwidth paperheight 0 1
statusdict begin
{setpageparams} stopped
end
} {true} ifelse
} bind def
/DiacriticEncoding [
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /space /exclam /quotedbl
/numbersign /dollar /percent /ampersand /quotesingle /parenleft
/parenright /asterisk /plus /comma /hyphen /period /slash /zero /one
/two /three /four /five /six /seven /eight /nine /colon /semicolon
/less /equal /greater /question /at /A /B /C /D /E /F /G /H /I /J /K
/L /M /N /O /P /Q /R /S /T /U /V /W /X /Y /Z /bracketleft /backslash
/bracketright /asciicircum /underscore /grave /a /b /c /d /e /f /g /h
/i /j /k /l /m /n /o /p /q /r /s /t /u /v /w /x /y /z /braceleft /bar
/braceright /asciitilde /.notdef /Adieresis /Aring /Ccedilla /Eacute
/Ntilde /Odieresis /Udieresis /aacute /agrave /acircumflex /adieresis
/atilde /aring /ccedilla /eacute /egrave /ecircumflex /edieresis
/iacute /igrave /icircumflex /idieresis /ntilde /oacute /ograve
/ocircumflex /odieresis /otilde /uacute /ugrave /ucircumflex
/udieresis /dagger /.notdef /cent /sterling /section /bullet
/paragraph /germandbls /registered /copyright /trademark /acute
/dieresis /.notdef /AE /Oslash /.notdef /.notdef /.notdef /.notdef
/yen /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/ordfeminine /ordmasculine /.notdef /ae /oslash /questiondown
/exclamdown /logicalnot /.notdef /florin /.notdef /.notdef
/guillemotleft /guillemotright /ellipsis /.notdef /Agrave /Atilde
/Otilde /OE /oe /endash /emdash /quotedblleft /quotedblright
/quoteleft /quoteright /.notdef /.notdef /ydieresis /Ydieresis
/fraction /currency /guilsinglleft /guilsinglright /fi /fl /daggerdbl
/periodcentered /quotesinglbase /quotedblbase /perthousand
/Acircumflex /Ecircumflex /Aacute /Edieresis /Egrave /Iacute
/Icircumflex /Idieresis /Igrave /Oacute /Ocircumflex /.notdef /Ograve
/Uacute /Ucircumflex /Ugrave /dotlessi /circumflex /tilde /macron
/breve /dotaccent /ring /cedilla /hungarumlaut /ogonek /caron
] def
/ReEncode {
dup
length
dict begin
{
1 index /FID ne
{def}
{pop pop} ifelse
} forall
0 eq {/Encoding DiacriticEncoding def} if
currentdict
end
} bind def
FMPColor

{
/BEGINBITMAPCOLOR {
BITMAPCOLOR} def
/BEGINBITMAPCOLORc {
BITMAPCOLORc} def
/BEGINBITMAPTRUECOLOR {
BITMAPTRUECOLOR } def
/BEGINBITMAPTRUECOLORc {
BITMAPTRUECOLORc } def
}

{
/BEGINBITMAPCOLOR {
BITMAPGRAY} def
/BEGINBITMAPCOLORc {
BITMAPGRAYc} def
/BEGINBITMAPTRUECOLOR {
BITMAPTRUEGRAY } def
/BEGINBITMAPTRUECOLORc {
BITMAPTRUEGRAYc } def
}
ifelse
/K {
FMPrintAllColorsAsBlack {
dup 1 eq 2 index 1 eq and 3 index 1 eq and not
{7 {pop} repeat 0 0 0 1 0 0 0} if
} if
FrameCurColors astore
pop combineColor
} bind def
/graymode true def
/bwidth FMLOCAL
/bpside FMLOCAL
/bstring FMLOCAL
/onbits FMLOCAL
/offbits FMLOCAL
/xindex FMLOCAL
/yindex FMLOCAL
/x FMLOCAL
/y FMLOCAL
/setPatternMode {
FMLevel1 {
/bwidth exch def
/bpside exch def
/bstring exch def
/onbits 0 def /offbits 0 def
freq sangle landscape {90 add} if
{/y exch def
/x exch def
/xindex x 1 add 2 div bpside mul cvi def
/yindex y 1 add 2 div bpside mul cvi def
bstring yindex bwidth mul xindex 8 idiv add get
1 7 xindex 8 mod sub bitshift and 0 ne FrameNegative {not} if
{/onbits onbits 1 add def 1}
{/offbits offbits 1 add def 0}
ifelse
}
setscreen
offbits offbits onbits add div FrameNegative {1.0 exch sub} if
/FrameCurGray exch def
} {
pop pop
dup patCache exch known {
patCache exch get
} {
dup
patDict /bstring 3 -1 roll put
patDict
9 PatFreq screenIndex get div dup matrix scale
makepattern
dup
patCache 4 -1 roll 3 -1 roll put
} ifelse
/FrameCurGray 0 def
/FrameCurPat exch def
} ifelse
/graymode false def
combineColor
} bind def
/setGrayScaleMode {
graymode not {
/graymode true def
FMLevel1 {
setCurrentScreen
} if
} if
/FrameCurGray exch def
combineColor
} bind def
/normalize {
transform round exch round exch itransform
} bind def
/dnormalize {
dtransform round exch round exch idtransform
} bind def
/lnormalize {
0 dtransform exch cvi 2 idiv 2 mul 1 add exch idtransform pop
} bind def
/H {
lnormalize setlinewidth
} bind def
/Z {
setlinecap
} bind def

/PFill {
graymode FMLevel1 or not {
gsave 1 setgray eofill grestore
} if
} bind def
/PStroke {
graymode FMLevel1 or not {
gsave 1 setgray stroke grestore
} if
stroke
} bind def
/fillvals FMLOCAL
/X {
fillvals exch get
dup type /stringtype eq
{8 1 setPatternMode}
{setGrayScaleMode}
ifelse
} bind def
/V {
PFill gsave eofill grestore
} bind def
/Vclip {
clip
} bind def
/Vstrk {
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/N {
PStroke
} bind def
/Nclip {
strokepath clip newpath
} bind def
/Nstrk {
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/M {newpath moveto} bind def
/E {lineto} bind def
/D {curveto} bind def
/O {closepath} bind def
/n FMLOCAL
/L {
/n exch def
newpath
normalize
moveto
2 1 n {pop normalize lineto} for
} bind def
/Y {
L
closepath
} bind def
/x1 FMLOCAL
/x2 FMLOCAL
/y1 FMLOCAL
/y2 FMLOCAL
/R {
/y2 exch def
/x2 exch def
/y1 exch def
/x1 exch def
x1 y1
x2 y1
x2 y2
x1 y2
4 Y
} bind def
/rad FMLOCAL
/rarc
{rad
arcto
} bind def
/RR {
/rad exch def
normalize
/y2 exch def
/x2 exch def
normalize
/y1 exch def
/x1 exch def
mark
newpath
{
x1 y1 rad add moveto
x1 y2 x2 y2 rarc
x2 y2 x2 y1 rarc
x2 y1 x1 y1 rarc
x1 y1 x1 y2 rarc
closepath
} stopped {x1 y1 x2 y2 R} if
cleartomark
} bind def
/RRR {
/rad exch def
normalize /y4 exch def /x4 exch def
normalize /y3 exch def /x3 exch def
normalize /y2 exch def /x2 exch def
normalize /y1 exch def /x1 exch def
newpath
normalize moveto
mark
{
x2 y2 x3 y3 rarc
x3 y3 x4 y4 rarc
x4 y4 x1 y1 rarc
x1 y1 x2 y2 rarc
closepath
} stopped
{x1 y1 x2 y2 x3 y3 x4 y4 newpath moveto lineto lineto lineto closepath} if
cleartomark
} bind def
/C {
grestore
gsave
R
clip
setCurrentScreen
} bind def
/CP {
grestore
gsave
Y
clip
setCurrentScreen
} bind def
/FMpointsize FMLOCAL
/F {
FMfonts exch get
FMpointsize scalefont
setfont
} bind def
/Q {
/FMpointsize exch def
F
} bind def
/T {
moveto show
} bind def
/RF {
rotate
0 ne {-1 1 scale} if
} bind def
/TF {
gsave
moveto
RF
show
grestore
} bind def
/P {
moveto
0 32 3 2 roll widthshow
} bind def
/PF {
gsave
moveto
RF
0 32 3 2 roll widthshow
grestore
} bind def
/S {
moveto
0 exch ashow
} bind def
/SF {
gsave
moveto
RF
0 exch ashow
grestore
} bind def
/B {
moveto
0 32 4 2 roll 0 exch awidthshow
} bind def
/BF {
gsave
moveto
RF
0 32 4 2 roll 0 exch awidthshow
grestore
} bind def
/G {
gsave
newpath
normalize translate 0.0 0.0 moveto
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
PFill fill
grestore
} bind def
/Gstrk {
savematrix
newpath
2 index 2 div add exch 3 index 2 div sub exch
normalize 2 index 2 div sub exch 3 index 2 div add exch
translate
scale
0.0 0.0 1.0 5 3 roll arc
restorematrix
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/Gclip {
newpath
savematrix
normalize translate 0.0 0.0 moveto
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
clip newpath
restorematrix
} bind def
/GG {
gsave
newpath
normalize translate 0.0 0.0 moveto
rotate
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
PFill
fill
grestore
} bind def
/GGclip {
savematrix
newpath
normalize translate 0.0 0.0 moveto
rotate
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
clip newpath
restorematrix
} bind def
/GGstrk {
savematrix
newpath
normalize translate 0.0 0.0 moveto
rotate
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
restorematrix
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/A {
gsave
savematrix
newpath
2 index 2 div add exch 3 index 2 div sub exch
normalize 2 index 2 div sub exch 3 index 2 div add exch
translate
scale
0.0 0.0 1.0 5 3 roll arc
restorematrix
PStroke
grestore
} bind def
/Aclip {
newpath
savematrix
normalize translate 0.0 0.0 moveto
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
strokepath clip newpath
restorematrix
} bind def
/Astrk {
Gstrk
} bind def
/AA {
gsave
savematrix
newpath

3 index 2 div add exch 4 index 2 div sub exch

normalize 3 index 2 div sub exch 4 index 2 div add exch
translate
rotate
scale
0.0 0.0 1.0 5 3 roll arc
restorematrix
PStroke
grestore
} bind def
/AAclip {
savematrix
newpath
normalize translate 0.0 0.0 moveto
rotate
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
strokepath clip newpath
restorematrix
} bind def
/AAstrk {
GGstrk
} bind def
/x FMLOCAL
/y FMLOCAL
/w FMLOCAL
/h FMLOCAL
/xx FMLOCAL
/yy FMLOCAL
/ww FMLOCAL
/hh FMLOCAL
/FMsaveobject FMLOCAL
/FMoptop FMLOCAL
/FMdicttop FMLOCAL
/BEGINPRINTCODE {
/FMdicttop countdictstack 1 add def
/FMoptop count 7 sub def
/FMsaveobject save def
userdict begin
/showpage {} def
FMNORMALIZEGRAPHICS
3 index neg 3 index neg translate
} bind def
/ENDPRINTCODE {
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
FMsaveobject restore
} bind def
/gn {
0
{ 46 mul
cf read pop
32 sub
dup 46 lt {exit} if
46 sub add
} loop
add
} bind def
/str FMLOCAL
/cfs {
/str sl string def
0 1 sl 1 sub {str exch val put} for
str def
} bind def
/ic [
0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0223
0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0223
0
{0 hx} {1 hx} {2 hx} {3 hx} {4 hx} {5 hx} {6 hx} {7 hx} {8 hx} {9 hx}
{10 hx} {11 hx} {12 hx} {13 hx} {14 hx} {15 hx} {16 hx} {17 hx} {18 hx}
{19 hx} {gn hx} {0} {1} {2} {3} {4} {5} {6} {7} {8} {9} {10} {11} {12}
{13} {14} {15} {16} {17} {18} {19} {gn} {0 wh} {1 wh} {2 wh} {3 wh}
{4 wh} {5 wh} {6 wh} {7 wh} {8 wh} {9 wh} {10 wh} {11 wh} {12 wh}
{13 wh} {14 wh} {gn wh} {0 bl} {1 bl} {2 bl} {3 bl} {4 bl} {5 bl} {6 bl}
{7 bl} {8 bl} {9 bl} {10 bl} {11 bl} {12 bl} {13 bl} {14 bl} {gn bl}
{0 fl} {1 fl} {2 fl} {3 fl} {4 fl} {5 fl} {6 fl} {7 fl} {8 fl} {9 fl}
{10 fl} {11 fl} {12 fl} {13 fl} {14 fl} {gn fl}
] def
/sl FMLOCAL
/val FMLOCAL
/ws FMLOCAL
/im FMLOCAL
/bs FMLOCAL
/cs FMLOCAL
/len FMLOCAL
/pos FMLOCAL
/ms {
/sl exch def
/val 255 def
/ws cfs
/im cfs
/val 0 def
/bs cfs
/cs cfs
} bind def
400 ms
/ip {
is
0
cf cs readline pop
{ ic exch get exec
add
} forall
pop

} bind def
/rip {


bis ris copy pop
is
0
cf cs readline pop
{ ic exch get exec
add
} forall
pop pop
ris gis copy pop
dup is exch

cf cs readline pop
{ ic exch get exec
add
} forall
pop pop
gis bis copy pop
dup add is exch

cf cs readline pop
{ ic exch get exec
add
} forall
pop

} bind def
/wh {
/len exch def
/pos exch def
ws 0 len getinterval im pos len getinterval copy pop
pos len
} bind def
/bl {
/len exch def
/pos exch def
bs 0 len getinterval im pos len getinterval copy pop
pos len
} bind def
/s1 1 string def
/fl {
/len exch def
/pos exch def
/val cf s1 readhexstring pop 0 get def
pos 1 pos len add 1 sub {im exch val put} for
pos len
} bind def
/hx {
3 copy getinterval
cf exch readhexstring pop pop
} bind def
/h FMLOCAL
/w FMLOCAL
/d FMLOCAL
/lb FMLOCAL
/bitmapsave FMLOCAL
/is FMLOCAL
/cf FMLOCAL
/wbytes {
dup dup
24 eq { pop pop 3 mul }
{ 8 eq {pop} {1 eq {7 add 8 idiv} {3 add 4 idiv} ifelse} ifelse } ifelse
} bind def
/BEGINBITMAPBWc {
1 {} COMMONBITMAPc
} bind def
/BEGINBITMAPGRAYc {
8 {} COMMONBITMAPc
} bind def
/BEGINBITMAP2BITc {
2 {} COMMONBITMAPc
} bind def
/COMMONBITMAPc {

/r exch def
/d exch def
gsave

3 index 2 div add exch
4 index 2 div add exch
translate
rotate
1 index 2 div neg
1 index 2 div neg
translate
scale
/h exch def /w exch def
/lb w d wbytes def
sl lb lt {lb ms} if
/bitmapsave save def
r
/is im 0 lb getinterval def
ws 0 lb getinterval is copy pop
/cf currentfile def
w h d [w 0 0 h neg 0 h]
{ip} image
bitmapsave restore
grestore
} bind def
/BEGINBITMAPBW {
1 {} COMMONBITMAP
} bind def
/BEGINBITMAPGRAY {
8 {} COMMONBITMAP
} bind def
/BEGINBITMAP2BIT {
2 {} COMMONBITMAP
} bind def
/COMMONBITMAP {
/r exch def
/d exch def
gsave

3 index 2 div add exch
4 index 2 div add exch
translate
rotate
1 index 2 div neg
1 index 2 div neg
translate
scale
/h exch def /w exch def
/bitmapsave save def
r
/is w d wbytes string def
/cf currentfile def
w h d [w 0 0 h neg 0 h]
{cf is readhexstring pop} image
bitmapsave restore
grestore
} bind def
/ngrayt 256 array def
/nredt 256 array def
/nbluet 256 array def
/ngreent 256 array def
/gryt FMLOCAL
/blut FMLOCAL
/grnt FMLOCAL
/redt FMLOCAL
/indx FMLOCAL
/cynu FMLOCAL
/magu FMLOCAL
/yelu FMLOCAL
/k FMLOCAL
/u FMLOCAL
FMLevel1 {
/colorsetup {
currentcolortransfer
/gryt exch def
/blut exch def
/grnt exch def
/redt exch def
0 1 255 {
/indx exch def
/cynu 1 red indx get 255 div sub def
/magu 1 green indx get 255 div sub def
/yelu 1 blue indx get 255 div sub def
/k cynu magu min yelu min def
/u k currentundercolorremoval exec def
% /u 0 def
nredt indx 1 0 cynu u sub max sub redt exec put
ngreent indx 1 0 magu u sub max sub grnt exec put
nbluet indx 1 0 yelu u sub max sub blut exec put
ngrayt indx 1 k currentblackgeneration exec sub gryt exec put
} for
{255 mul cvi nredt exch get}
{255 mul cvi ngreent exch get}
{255 mul cvi nbluet exch get}
{255 mul cvi ngrayt exch get}
setcolortransfer
{pop 0} setundercolorremoval
{} setblackgeneration
} bind def
}
{
/colorSetup2 {
[ /Indexed /DeviceRGB 255
{dup red exch get 255 div
exch dup green exch get 255 div
exch blue exch get 255 div}
] setcolorspace
} bind def
} ifelse
/tran FMLOCAL
/fakecolorsetup {
/tran 256 string def
0 1 255 {/indx exch def
tran indx
red indx get 77 mul
green indx get 151 mul
blue indx get 28 mul
add add 256 idiv put} for
currenttransfer
{255 mul cvi tran exch get 255.0 div}
exch concatprocs settransfer
} bind def
/BITMAPCOLOR {
/d 8 def
gsave

3 index 2 div add exch
4 index 2 div add exch
translate
rotate
1 index 2 div neg
1 index 2 div neg
translate
scale
/h exch def /w exch def
/bitmapsave save def
FMLevel1 {
colorsetup
/is w d wbytes string def
/cf currentfile def
w h d [w 0 0 h neg 0 h]
{cf is readhexstring pop} {is} {is} true 3 colorimage
} {
colorSetup2
/is w d wbytes string def
/cf currentfile def
7 dict dup begin
/ImageType 1 def
/Width w def
/Height h def
/ImageMatrix [w 0 0 h neg 0 h] def
/DataSource {cf is readhexstring pop} bind def
/BitsPerComponent d def
/Decode [0 255] def
end image
} ifelse
bitmapsave restore
grestore
} bind def
/BITMAPCOLORc {
/d 8 def
gsave

3 index 2 div add exch
4 index 2 div add exch
translate
rotate
1 index 2 div neg
1 index 2 div neg
translate
scale
/h exch def /w exch def
/lb w d wbytes def
sl lb lt {lb ms} if
/bitmapsave save def
FMLevel1 {
colorsetup
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(May) 207 498.67 T
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-0.25 (This is version 5.0 of the Instrument Handbook for the Goddard High Resolution Spectrograph \050GHRS\051 of) 72 712.67 P
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(Editor and principal author is David R. Soderblom.) 72 676.67 T
(Date of issue is May 31, 1994.) 72 652.67 T
(Date of last revision was May 2, 1994) 72 640.67 T
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(Lead GHRS Instrument Scientist) 257.6 371 T
(410-338-4543) 389.62 371 T
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(soderblom@stsci.edu) 454.13 371 T
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(Stephen J. Hulbert) 173.62 356 T
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(410-338-491) 389.62 356 T
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(hulbert@stsci.edu) 454.13 356 T
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(Claus Leitherer) 173.62 341 T
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(410-338-4425) 389.62 341 T
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(leither) 454.13 341 T
(er@stsci.edu) 477.29 341 T
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(Lisa Sherbert) 173.62 326 T
(T) 257.6 326 T
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(410-338-5036) 389.62 326 T
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(lisa@stsci.edu) 454.13 326 T
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(Proposal-speci\336c) 94.85 311 T
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(GHRS Instrument Handbook Revision History) 207 245 T
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(V) 220.78 221.67 T
(ersion) 225.67 221.67 T
(Date of Issue) 274.78 221.67 T
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0 9 Q
(1.0) 220.78 207 T
(1985 October) 274.78 207 T
(D. Ebbets) 357.03 207 T
(2.0) 220.78 192 T
(1989 May) 274.78 192 T
(D. Duncan and D. Ebbets) 357.03 192 T
(2.1) 220.78 177 T
(1990 March) 274.78 177 T
(D. Duncan) 357.03 177 T
(3.0) 220.78 162 T
(1992 January) 274.78 162 T
(D. Duncan) 357.03 162 T
(4.0) 220.78 147 T
(1993 January) 274.78 147 T
(D. Soderblom) 357.03 147 T
(4.1) 220.78 132 T
(1993 March) 274.78 132 T
(D. Soderblom) 357.03 132 T
(5.0) 220.78 117 T
(1994 May) 274.78 117 T
(D. Soderblom) 357.03 117 T
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(GHRS Instrument Handbook 5.0) 207 60.29 T
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(This Handbook) 207 621.35 T
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(8) 388.17 605.35 T
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(...................) 441 552.68 T
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(1) 508.77 552.68 T
(1) 515 552.68 T
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2 10 Q
(2.1) 184.1 535.35 T
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(Fundamental properties of the instrument) 207 535.35 T
(12) 415.36 535.35 T
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(2.2) 184.1 519.35 T
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(A Brief Description of the Instrument and Its Operation) 207 519.35 T
(13) 477.04 519.35 T
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(2.3) 184.1 503.35 T
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(A Little About How) 207 503.35 T
6 F
(HST) 299.22 503.35 T
2 F
( and GHRS W) 319.22 503.35 T
(ork) 383.49 503.35 T
(15) 409.05 503.35 T
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(2.4) 184.1 487.35 T
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(GHRS Modes of Operation) 207 487.35 T
(17) 342.57 487.35 T
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2 14 Q
(Part II: W) 72 450.68 T
(riting GHRS Proposals) 132.42 450.68 T
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5 F
(Chapter 3) 72 412.68 T
0 0 0 1 0 0 0 K
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(Phase I: What the T) 171 412.68 T
(AC Sees) 281.29 412.68 T
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(...................................................) 329 412.68 T
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(21) 508 412.68 T
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0 0 0 1 0 0 0 K
2 10 Q
(3.1) 184.1 395.35 T
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(Essential questions) 207 395.35 T
(22) 310.92 395.35 T
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0 0 0 1 0 0 0 K
(3.2) 184.1 379.35 T
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0 0 0 1 0 0 0 K
(Creating an Observation Scenario) 207 379.35 T
(23) 378.16 379.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(3.3) 184.1 363.35 T
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0 0 0 1 0 0 0 K
(Specifying T) 207 363.35 T
(arget Acquisition) 265.72 363.35 T
(24) 357.4 363.35 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(3.4) 184.1 347.35 T
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(Calculating the Exposure T) 207 347.35 T
(ime) 335.74 347.35 T
(26) 362.97 347.35 T
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5 14 Q
(Chapter 4) 72 310.68 T
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(Y) 171 310.68 T
(our Phase II Pr) 178.78 310.68 T
(oposal) 264.46 310.68 T
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(...........................................................) 301 310.68 T
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(33) 508 310.68 T
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0 0 0 1 0 0 0 K
2 10 Q
(4.1) 184.1 293.35 T
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(Acquisitions) 207 293.35 T
(35) 277.01 293.35 T
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(4.2) 184.1 277.35 T
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(Image Mode) 207 277.35 T
(42) 274.79 277.35 T
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0 0 0 1 0 0 0 K
(4.3) 184.1 261.35 T
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(Accumulation Mode) 207 261.35 T
(43) 312.01 261.35 T
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(4.4) 184.1 245.35 T
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(Rapid Readout Mode) 207 245.35 T
(45) 316.45 245.35 T
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(4.5) 184.1 229.35 T
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(The Precision and Accuracy of Standard Calibrations) 207 229.35 T
(46) 469.85 229.35 T
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(4.6) 184.1 213.35 T
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(Other Considerations) 207 213.35 T
(47) 319.24 213.35 T
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5 14 Q
(Chapter 5) 72 176.68 T
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(Phase II Pr) 171 176.68 T
(oposal Examples) 233.73 176.68 T
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(...................................................) 329 176.68 T
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(49) 508 176.68 T
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(4) 54 60.29 T
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(GHRS Instrument Handbook 5.0) 189 60.29 T
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(Part III: GHRS Reference Information) 54 676.68 T
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(Chapter 6) 54 638.68 T
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(.................................) 374.5 638.68 T
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(55) 490 638.68 T
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(6.1) 166.1 621.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(The HST Focal Plane and the GHRS Apertures) 189 621.35 T
(56) 417.94 621.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(6.2) 166.1 605.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Gratings and Optical Elements) 189 605.35 T
(60) 344.6 605.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(6.3) 166.1 589.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(The Digicon Detectors) 189 589.35 T
(62) 305.13 589.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 14 Q
(Chapter 7) 54 552.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(T) 153 552.68 T
(ar) 160 552.68 T
(get Acquisition Refer) 171.41 552.68 T
(ence Information) 290.69 552.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(.............................) 388.5 552.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(67) 490 552.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
(7.1) 166.1 535.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Predicting T) 189 535.35 T
(arget Acquisition Count Rates for Stars) 246.05 535.35 T
(68) 443.3 535.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(7.2) 166.1 519.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Constraints on the V) 189 519.35 T
(alue of the STEP-TIME Parameter) 286.24 519.35 T
(71) 454.06 519.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(7.3) 166.1 503.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Acquisition Count Rates for Extended Objects) 189 503.35 T
(76) 418.48 503.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(7.4) 166.1 487.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Other Acquisition Information) 189 487.35 T
(78) 340.68 487.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 14 Q
(Chapter 8) 54 450.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Refer) 153 450.68 T
(ence T) 182.32 450.68 T
(ables for Instrument Performance) 217.19 450.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(.......................) 409.5 450.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(81) 490 450.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
(8.1) 166.1 433.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(The Effect of COST) 189 433.35 T
(AR on the GHRS) 279.38 433.35 T
(82) 368.27 433.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(8.2) 166.1 417.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Properties of the First-Order Gratings) 189 417.35 T
(83) 377.37 417.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(8.3) 166.1 401.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Properties of the Echelle Gratings) 189 401.35 T
(87) 360.16 401.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(8.4) 166.1 385.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Standard Patterns for Substepping and Background Measurement) 189 385.35 T
(92) 513.5 385.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(8.5) 166.1 369.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(The Effects of Reddening in the Ultraviolet) 189 369.35 T
(93) 400.7 369.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(8.6) 166.1 353.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Instrumental Properties) 189 353.35 T
(94) 311.25 353.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 14 Q
(Chapter 9) 54 316.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(GHRS Bibliography) 153 316.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(.............................................................) 269.5 316.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(101) 483 316.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 10 Q
(9.1) 166.1 299.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Ultraviolet Extinction) 189 299.35 T
(102) 299.02 299.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(9.2) 166.1 283.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(GHRS-Related T) 189 283.35 T
(echnical Papers) 265.49 283.35 T
(102) 351.64 283.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(9.3) 166.1 267.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(GHRS Scienti\336c Papers) 189 267.35 T
(104) 311.26 267.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(9.4) 166.1 251.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Acknowledgments) 189 251.35 T
(109) 287.35 251.35 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 14 Q
(Part IV) 54 214.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 F
(Glossary of T) 153 176.68 T
(erms and Abbr) 226.88 176.68 T
(eviations) 310.37 176.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(..................................) 364 176.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(1) 484.54 176.68 T
(1) 490.77 176.68 T
(1) 497 176.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Index) 153 138.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(.....................................................................................) 185.5 138.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(1) 483.77 138.68 T
(15) 490 138.68 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
FMENDPAGE
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%%BeginProlog
%
% Frame ps_prolog 4.0, for use with Frame 4.0 products
% This ps_prolog file is Copyright (c) 1986-1993 Frame Technology
% Corporation. All rights reserved. This ps_prolog file may be
% freely copied and distributed in conjunction with documents created
% using FrameMaker, FrameBuilder and FrameViewer as long as this
% copyright notice is preserved.
%
% Frame products normally print colors as their true color on a color printer
% or as shades of gray, based on luminance, on a black-and white printer. The
% following flag, if set to True, forces all non-white colors to print as pure
% black. This has no effect on bitmap images.
/FMPrintAllColorsAsBlack false def
%
% Frame products can either set their own line screens or use a printer's
% default settings. Three flags below control this separately for no
% separations, spot separations and process separations. If a flag
% is true, then the default printer settings will not be changed. If it is
% false, Frame products will use their own settings from a table based on
% the printer's resolution.
/FMUseDefaultNoSeparationScreen true def
/FMUseDefaultSpotSeparationScreen true def
/FMUseDefaultProcessSeparationScreen false def
%
% For any given PostScript printer resolution, Frame products have two sets of
% screen angles and frequencies for printing process separations, which are
% recomended by Adobe. The following variable chooses the higher frequencies
% when set to true or the lower frequencies when set to false. This is only
% effective if the appropriate FMUseDefault...SeparationScreen flag is false.
/FMUseHighFrequencyScreens true def
%
% PostScript Level 2 printers contain an "Accurate Screens" feature which can
% improve process separation rendering at the expense of compute time. This
% flag is ignored by PostScript Level 1 printers.
/FMUseAcccurateScreens true def
%
% The following PostScript procedure defines the spot function that Frame
% products will use for process separations. You may un-comment-out one of
% the alternative functions below, or use your own.
%
% Dot function
/FMSpotFunction {abs exch abs 2 copy add 1 gt
{1 sub dup mul exch 1 sub dup mul add 1 sub }
{dup mul exch dup mul add 1 exch sub }ifelse } def
%
% Line function
% /FMSpotFunction { pop } def
%
% Elipse function
% /FMSpotFunction { dup 5 mul 8 div mul exch dup mul exch add
% sqrt 1 exch sub } def
%
%
/FMversion (4.0) def
/FMLevel1 /languagelevel where {pop languagelevel} {1} ifelse 2 lt def
/FMPColor
FMLevel1 {
false
/colorimage where {pop pop true} if
} {
true
} ifelse
def
/FrameDict 400 dict def
systemdict /errordict known not {/errordict 10 dict def
errordict /rangecheck {stop} put} if
% The readline in PS 23.0 doesn't recognize cr's as nl's on AppleTalk
FrameDict /tmprangecheck errordict /rangecheck get put
errordict /rangecheck {FrameDict /bug true put} put
FrameDict /bug false put
mark
% Some PS machines read past the CR, so keep the following 3 lines together!
currentfile 5 string readline
00
0000000000
cleartomark
errordict /rangecheck FrameDict /tmprangecheck get put
FrameDict /bug get {
/readline {
/gstring exch def
/gfile exch def
/gindex 0 def
{
gfile read pop
dup 10 eq {exit} if
dup 13 eq {exit} if
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/gindex gindex 1 add def
} loop
pop
gstring 0 gindex getinterval true
} bind def
} if
/FMshowpage /showpage load def
/FMquit /quit load def
/FMFAILURE {
dup = flush
FMshowpage
/Helvetica findfont 12 scalefont setfont
72 200 moveto
show FMshowpage
FMquit
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/FMVERSION {
FMversion ne {
(Frame product version does not match ps_prolog!) FMFAILURE
} if
} def
/FMBADEPSF {
(PostScript Lang. Ref. Man., 2nd Ed., H.2.4 says EPS must not call X )
dup dup (X) search pop exch pop exch pop length
4 -1 roll
putinterval
FMFAILURE
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/FMLOCAL {
FrameDict begin
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/concatprocs
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FrameDict begin
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/FMcyan 1 def
/FMmagenta 2 def
/FMyellow 3 def
/FMblack 4 def
/FMcustom 5 def
/FrameNegative false def
/FrameSepIs FMnone def
/FrameSepBlack 0 def
/FrameSepYellow 0 def
/FrameSepMagenta 0 def
/FrameSepCyan 0 def
/FrameSepRed 1 def
/FrameSepGreen 1 def
/FrameSepBlue 1 def
/FrameCurGray 1 def
/FrameCurPat null def
/FrameCurColors [ 0 0 0 1 0 0 0 ] def
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sub dup 0 lt {neg} if
FrameColorEpsilon le
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2 copy 2 get exch 2 get eqepsilon {
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2 copy 5 get exch 1 get eqepsilon {
6 get exch 2 get eqepsilon
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/RGBtoCMYK {
1 exch sub
3 1 roll
1 exch sub
3 1 roll
1 exch sub
3 1 roll
3 copy
2 copy
le { pop } { exch pop } ifelse
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le { pop } { exch pop } ifelse
dup dup dup
6 1 roll
4 1 roll
7 1 roll
sub
6 1 roll
sub
5 1 roll
sub
4 1 roll
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/CMYKtoRGB {
dup dup 4 -1 roll add
5 1 roll 3 -1 roll add
4 1 roll add
1 exch sub dup 0 lt {pop 0} if 3 1 roll
1 exch sub dup 0 lt {pop 0} if exch
1 exch sub dup 0 lt {pop 0} if exch
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/FrameSepInit {
1.0 RealSetgray
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/FrameSetSepColor {
/FrameSepBlue exch def
/FrameSepGreen exch def
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/FrameSepIs FMcustom def
setCurrentScreen
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/FrameSetCyan {
/FrameSepBlue 1.0 def
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/FrameSepBlack 0.0 def
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/FrameSepIs FMcyan def
setCurrentScreen
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/FrameSetMagenta {
/FrameSepBlue 1.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 1.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMmagenta def
setCurrentScreen
} bind def

/FrameSetYellow {
/FrameSepBlue 0.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 1.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMyellow def
setCurrentScreen
} bind def

/FrameSetBlack {
/FrameSepBlue 0.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 1.0 def
/FrameSepYellow 0.0 def
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/FrameSepCyan 0.0 def
/FrameSepIs FMblack def
setCurrentScreen
} bind def

/FrameNoSep {
/FrameSepIs FMnone def
setCurrentScreen
} bind def
/FrameSetSepColors {
FrameDict begin
[ exch 1 add 1 roll ]
/FrameSepColors
exch def end
} bind def
/FrameColorInSepListCMYK {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsCMYK
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/FrameColorInSepListRGB {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsRGB
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/RealSetgray /setgray load def
/RealSetrgbcolor /setrgbcolor load def
/RealSethsbcolor /sethsbcolor load def
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/setgray {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetgray }
{
FrameSepIs FMblack eq
{ RealSetgray }
{ FrameSepIs FMcustom eq
FrameSepRed 0 eq and
FrameSepGreen 0 eq and
FrameSepBlue 0 eq and {
RealSetgray
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1 RealSetgray pop
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/setrgbcolor {
FrameDict begin
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{ RealSetrgbcolor }
{
3 copy [ 4 1 roll ]
FrameColorInSepListRGB
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FrameSepBlue eq exch
FrameSepGreen eq and exch
FrameSepRed eq and
{ 0 } { 1 } ifelse
}
{
FMPColor {
RealSetrgbcolor
currentcmykcolor
} {
RGBtoCMYK
} ifelse
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
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RealSetgray
}
ifelse
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} bind def
/sethsbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSethsbcolor }
{
RealSethsbcolor
currentrgbcolor
setrgbcolor
}
ifelse
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} bind def
FrameDict begin
/setcmykcolor where {
pop /RealSetcmykcolor /setcmykcolor load def
} {
/RealSetcmykcolor {
4 1 roll
3 { 3 index add 0 max 1 min 1 exch sub 3 1 roll} repeat
setrgbcolor pop
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userdict /setcmykcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetcmykcolor }
{
4 copy [ 5 1 roll ]
FrameColorInSepListCMYK
{
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
{ 0 } { 1 } ifelse
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{
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
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FrameSepIs FMcyan eq
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RealSetgray
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} bind put
FMLevel1 not {

/patProcDict 5 dict dup begin
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<8040201008040201> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
end def
/patDict 15 dict dup begin
/PatternType 1 def
/PaintType 2 def
/TilingType 3 def
/BBox [ 0 0 8 8 ] def
/XStep 8 def
/YStep 8 def
/PaintProc {
begin
patProcDict bstring known {
patProcDict bstring get exec
} {
8 8 true [1 0 0 -1 0 8] bstring imagemask
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/combineColor {
FrameSepIs FMnone eq
{
graymode FMLevel1 or not {

[/Pattern [/DeviceCMYK]] setcolorspace
FrameCurColors 0 4 getinterval aload pop FrameCurPat setcolor
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FrameCurColors 3 get 1.0 ge {
FrameCurGray RealSetgray
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FMPColor graymode and {
0 1 3 {
FrameCurColors exch get
1 FrameCurGray sub mul
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RealSetcmykcolor
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4 1 6 {
FrameCurColors exch get
graymode {
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FrameCurColors 0 4 getinterval aload
FrameColorInSepListCMYK {
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FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
FrameSepIs FMcustom eq and
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FrameSepIs FMblack eq
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[/Pattern [/DeviceGray]] setcolorspace
FrameCurPat setcolor
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graymode not FMLevel1 and {

dup 1 lt {pop FrameCurGray} if
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/dmatrix matrix def
/dpi 72 0 dmatrix defaultmatrix dtransform
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/freq dpi dup 72 div round dup 0 eq {pop 1} if 8 mul div def
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/dpiranges [ 2540 2400 1693 1270 1200 635 600 0 ] def
/CMLowFreqs [ 100.402 94.8683 89.2289 100.402 94.8683 66.9349 63.2456 47.4342 ] def
/YLowFreqs [ 95.25 90.0 84.65 95.25 90.0 70.5556 66.6667 50.0 ] def
/KLowFreqs [ 89.8026 84.8528 79.8088 89.8026 84.8528 74.8355 70.7107 53.033 ] def
/CLowAngles [ 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 ] def
/MLowAngles [ 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 ] def
/YLowTDot [ true true false true true false false false ] def
/CMHighFreqs [ 133.87 126.491 133.843 108.503 102.523 100.402 94.8683 63.2456 ] def
/YHighFreqs [ 127.0 120.0 126.975 115.455 109.091 95.25 90.0 60.0 ] def
/KHighFreqs [ 119.737 113.137 119.713 128.289 121.218 89.8026 84.8528 63.6395 ] def
/CHighAngles [ 71.5651 71.5651 71.5651 70.0169 70.0169 71.5651 71.5651 71.5651 ] def
/MHighAngles [ 18.4349 18.4349 18.4349 19.9831 19.9831 18.4349 18.4349 18.4349 ] def
/YHighTDot [ false false true false false true true false ] def
/PatFreq [ 10.5833 10.0 9.4055 10.5833 10.0 10.5833 10.0 9.375 ] def
/screenIndex {
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/getCyanScreen {
FMUseHighFrequencyScreens { CHighAngles CMHighFreqs} {CLowAngles CMLowFreqs} ifelse
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/getMagentaScreen {
FMUseHighFrequencyScreens { MHighAngles CMHighFreqs } {MLowAngles CMLowFreqs} ifelse
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/getYellowScreen {
FMUseHighFrequencyScreens { YHighTDot YHighFreqs} { YLowTDot YLowFreqs } ifelse
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{2 { 1 add 2 div 3 mul dup floor sub 2 mul 1 sub exch} repeat
FMSpotFunction } } {/FMSpotFunction load } ifelse
0.0 exch
} bind def
/getBlackScreen {
FMUseHighFrequencyScreens { KHighFreqs } { KLowFreqs } ifelse
screenIndex get 45.0 /FMSpotFunction load
} bind def
/getSpotScreen {
getBlackScreen
} bind def
/getCompositeScreen {
getBlackScreen
} bind def
/FMSetScreen
FMLevel1 { /setscreen load
}{ {
8 dict begin
/HalftoneType 1 def
/SpotFunction exch def
/Angle exch def
/Frequency exch def
/AccurateScreens FMUseAcccurateScreens def
currentdict end sethalftone
} bind } ifelse
def
/setDefaultScreen {
FMPColor {
orgrxfer cvx orggxfer cvx orgbxfer cvx orgxfer cvx setcolortransfer
}
{
orgxfer cvx settransfer
} ifelse
orgfreq organgle orgproc cvx setscreen
} bind def
/setCurrentScreen {
FrameSepIs FMnone eq {
FMUseDefaultNoSeparationScreen {
setDefaultScreen
} {
getCompositeScreen FMSetScreen
} ifelse
} {
FrameSepIs FMcustom eq {
FMUseDefaultSpotSeparationScreen {
setDefaultScreen
} {
getSpotScreen FMSetScreen
} ifelse
} {
FMUseDefaultProcessSeparationScreen {
setDefaultScreen
} {
FrameSepIs FMcyan eq {
getCyanScreen FMSetScreen
} {
FrameSepIs FMmagenta eq {
getMagentaScreen FMSetScreen
} {
FrameSepIs FMyellow eq {
getYellowScreen FMSetScreen
} {
getBlackScreen FMSetScreen
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} bind def
end
/gstring FMLOCAL
/gfile FMLOCAL
/gindex FMLOCAL
/orgrxfer FMLOCAL
/orggxfer FMLOCAL
/orgbxfer FMLOCAL
/orgxfer FMLOCAL
/orgproc FMLOCAL
/orgrproc FMLOCAL
/orggproc FMLOCAL
/orgbproc FMLOCAL
/organgle FMLOCAL
/orgrangle FMLOCAL
/orggangle FMLOCAL
/orgbangle FMLOCAL
/orgfreq FMLOCAL
/orgrfreq FMLOCAL
/orggfreq FMLOCAL
/orgbfreq FMLOCAL
/yscale FMLOCAL
/xscale FMLOCAL
/edown FMLOCAL
/manualfeed FMLOCAL
/paperheight FMLOCAL
/paperwidth FMLOCAL
/FMDOCUMENT {
array /FMfonts exch def
/#copies exch def
FrameDict begin
0 ne /manualfeed exch def
/paperheight exch def
/paperwidth exch def
0 ne /FrameNegative exch def
0 ne /edown exch def
/yscale exch def
/xscale exch def
FMLevel1 {
manualfeed {setmanualfeed} if
/FMdicttop countdictstack 1 add def
/FMoptop count def
% setpapername
% manualfeed {true} {papersize} ifelse
% {manualpapersize} {false} ifelse
% {desperatepapersize} {false} ifelse
% { (Can't select requested paper size for Frame print job!) FMFAILURE } if
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
}
{{1 dict dup /PageSize [paperwidth paperheight]put setpagedevice}stopped
{ (Can't select requested paper size for Frame print job!) FMFAILURE } if
{1 dict dup /ManualFeed manualfeed put setpagedevice } stopped pop }
ifelse

FMPColor {
currentcolorscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def
cvlit /orgbproc exch def
/orgbangle exch def
/orgbfreq exch def
cvlit /orggproc exch def
/orggangle exch def
/orggfreq exch def
cvlit /orgrproc exch def
/orgrangle exch def
/orgrfreq exch def
currentcolortransfer
FrameNegative {
1 1 4 {
pop { 1 exch sub } concatprocs 4 1 roll
} for
4 copy
setcolortransfer
} if
cvlit /orgxfer exch def
cvlit /orgbxfer exch def
cvlit /orggxfer exch def
cvlit /orgrxfer exch def
} {
currentscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def

currenttransfer
FrameNegative {
{ 1 exch sub } concatprocs
dup settransfer
} if
cvlit /orgxfer exch def
} ifelse
end
} def
/pagesave FMLOCAL
/orgmatrix FMLOCAL
/landscape FMLOCAL
/pwid FMLOCAL
/FMBEGINPAGE {
FrameDict begin
/pagesave save def
3.86 setmiterlimit
/landscape exch 0 ne def
landscape {
90 rotate 0 exch dup /pwid exch def neg translate pop
}{
pop /pwid exch def
} ifelse
edown { [-1 0 0 1 pwid 0] concat } if
0 0 moveto paperwidth 0 lineto paperwidth paperheight lineto
0 paperheight lineto 0 0 lineto 1 setgray fill
xscale yscale scale
/orgmatrix matrix def
gsave
} def
/FMENDPAGE {
grestore
pagesave restore
end
showpage
} def
/FMFONTDEFINE {
FrameDict begin
findfont
ReEncode
1 index exch
definefont
FMfonts 3 1 roll
put
end
} def
/FMFILLS {
FrameDict begin dup
array /fillvals exch def
dict /patCache exch def
end
} def
/FMFILL {
FrameDict begin
fillvals 3 1 roll put
end
} def
/FMNORMALIZEGRAPHICS {
newpath
0.0 0.0 moveto
1 setlinewidth
0 setlinecap
0 0 0 sethsbcolor
0 setgray
} bind def
/fx FMLOCAL
/fy FMLOCAL
/fh FMLOCAL
/fw FMLOCAL
/llx FMLOCAL
/lly FMLOCAL
/urx FMLOCAL
/ury FMLOCAL
/FMBEGINEPSF {
end
/FMEPSF save def
/showpage {} def
% See Adobe's "PostScript Language Reference Manual, 2nd Edition", page 714.
% "...the following operators MUST NOT be used in an EPS file:" (emphasis ours)
/banddevice {(banddevice) FMBADEPSF} def
/clear {(clear) FMBADEPSF} def
/cleardictstack {(cleardictstack) FMBADEPSF} def
/copypage {(copypage) FMBADEPSF} def
/erasepage {(erasepage) FMBADEPSF} def
/exitserver {(exitserver) FMBADEPSF} def
/framedevice {(framedevice) FMBADEPSF} def
/grestoreall {(grestoreall) FMBADEPSF} def
/initclip {(initclip) FMBADEPSF} def
/initgraphics {(initgraphics) FMBADEPSF} def
/initmatrix {(initmatrix) FMBADEPSF} def
/quit {(quit) FMBADEPSF} def
/renderbands {(renderbands) FMBADEPSF} def
/setglobal {(setglobal) FMBADEPSF} def
/setpagedevice {(setpagedevice) FMBADEPSF} def
/setshared {(setshared) FMBADEPSF} def
/startjob {(startjob) FMBADEPSF} def
/lettertray {(lettertray) FMBADEPSF} def
/letter {(letter) FMBADEPSF} def
/lettersmall {(lettersmall) FMBADEPSF} def
/11x17tray {(11x17tray) FMBADEPSF} def
/11x17 {(11x17) FMBADEPSF} def
/ledgertray {(ledgertray) FMBADEPSF} def
/ledger {(ledger) FMBADEPSF} def
/legaltray {(legaltray) FMBADEPSF} def
/legal {(legal) FMBADEPSF} def
/statementtray {(statementtray) FMBADEPSF} def
/statement {(statement) FMBADEPSF} def
/executivetray {(executivetray) FMBADEPSF} def
/executive {(executive) FMBADEPSF} def
/a3tray {(a3tray) FMBADEPSF} def
/a3 {(a3) FMBADEPSF} def
/a4tray {(a4tray) FMBADEPSF} def
/a4 {(a4) FMBADEPSF} def
/a4small {(a4small) FMBADEPSF} def
/b4tray {(b4tray) FMBADEPSF} def
/b4 {(b4) FMBADEPSF} def
/b5tray {(b5tray) FMBADEPSF} def
/b5 {(b5) FMBADEPSF} def
FMNORMALIZEGRAPHICS
[/fy /fx /fh /fw /ury /urx /lly /llx] {exch def} forall
fx fw 2 div add fy fh 2 div add translate
rotate
fw 2 div neg fh 2 div neg translate
fw urx llx sub div fh ury lly sub div scale
llx neg lly neg translate
/FMdicttop countdictstack 1 add def
/FMoptop count def
} bind def
/FMENDEPSF {
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
FMEPSF restore
FrameDict begin
} bind def
FrameDict begin
/setmanualfeed {
%%BeginFeature *ManualFeed True
statusdict /manualfeed true put
%%EndFeature
} bind def
/max {2 copy lt {exch} if pop} bind def
/min {2 copy gt {exch} if pop} bind def
/inch {72 mul} def
/pagedimen {
paperheight sub abs 16 lt exch
paperwidth sub abs 16 lt and
{/papername exch def} {pop} ifelse
} bind def
/papersizedict FMLOCAL
/setpapername {
/papersizedict 14 dict def
papersizedict begin
/papername /unknown def
/Letter 8.5 inch 11.0 inch pagedimen
/LetterSmall 7.68 inch 10.16 inch pagedimen
/Tabloid 11.0 inch 17.0 inch pagedimen
/Ledger 17.0 inch 11.0 inch pagedimen
/Legal 8.5 inch 14.0 inch pagedimen
/Statement 5.5 inch 8.5 inch pagedimen
/Executive 7.5 inch 10.0 inch pagedimen
/A3 11.69 inch 16.5 inch pagedimen
/A4 8.26 inch 11.69 inch pagedimen
/A4Small 7.47 inch 10.85 inch pagedimen
/B4 10.125 inch 14.33 inch pagedimen
/B5 7.16 inch 10.125 inch pagedimen
end
} bind def
/papersize {
papersizedict begin
/Letter {lettertray letter} def
/LetterSmall {lettertray lettersmall} def
/Tabloid {11x17tray 11x17} def
/Ledger {ledgertray ledger} def
/Legal {legaltray legal} def
/Statement {statementtray statement} def
/Executive {executivetray executive} def
/A3 {a3tray a3} def
/A4 {a4tray a4} def
/A4Small {a4tray a4small} def
/B4 {b4tray b4} def
/B5 {b5tray b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
statusdict begin stopped end
} bind def
/manualpapersize {
papersizedict begin
/Letter {letter} def
/LetterSmall {lettersmall} def
/Tabloid {11x17} def
/Ledger {ledger} def
/Legal {legal} def
/Statement {statement} def
/Executive {executive} def
/A3 {a3} def
/A4 {a4} def
/A4Small {a4small} def
/B4 {b4} def
/B5 {b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
stopped
} bind def
/desperatepapersize {
statusdict /setpageparams known
{
paperwidth paperheight 0 1
statusdict begin
{setpageparams} stopped
end
} {true} ifelse
} bind def
/DiacriticEncoding [
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /space /exclam /quotedbl
/numbersign /dollar /percent /ampersand /quotesingle /parenleft
/parenright /asterisk /plus /comma /hyphen /period /slash /zero /one
/two /three /four /five /six /seven /eight /nine /colon /semicolon
/less /equal /greater /question /at /A /B /C /D /E /F /G /H /I /J /K
/L /M /N /O /P /Q /R /S /T /U /V /W /X /Y /Z /bracketleft /backslash
/bracketright /asciicircum /underscore /grave /a /b /c /d /e /f /g /h
/i /j /k /l /m /n /o /p /q /r /s /t /u /v /w /x /y /z /braceleft /bar
/braceright /asciitilde /.notdef /Adieresis /Aring /Ccedilla /Eacute
/Ntilde /Odieresis /Udieresis /aacute /agrave /acircumflex /adieresis
/atilde /aring /ccedilla /eacute /egrave /ecircumflex /edieresis
/iacute /igrave /icircumflex /idieresis /ntilde /oacute /ograve
/ocircumflex /odieresis /otilde /uacute /ugrave /ucircumflex
/udieresis /dagger /.notdef /cent /sterling /section /bullet
/paragraph /germandbls /registered /copyright /trademark /acute
/dieresis /.notdef /AE /Oslash /.notdef /.notdef /.notdef /.notdef
/yen /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/ordfeminine /ordmasculine /.notdef /ae /oslash /questiondown
/exclamdown /logicalnot /.notdef /florin /.notdef /.notdef
/guillemotleft /guillemotright /ellipsis /.notdef /Agrave /Atilde
/Otilde /OE /oe /endash /emdash /quotedblleft /quotedblright
/quoteleft /quoteright /.notdef /.notdef /ydieresis /Ydieresis
/fraction /currency /guilsinglleft /guilsinglright /fi /fl /daggerdbl
/periodcentered /quotesinglbase /quotedblbase /perthousand
/Acircumflex /Ecircumflex /Aacute /Edieresis /Egrave /Iacute
/Icircumflex /Idieresis /Igrave /Oacute /Ocircumflex /.notdef /Ograve
/Uacute /Ucircumflex /Ugrave /dotlessi /circumflex /tilde /macron
/breve /dotaccent /ring /cedilla /hungarumlaut /ogonek /caron
] def
/ReEncode {
dup
length
dict begin
{
1 index /FID ne
{def}
{pop pop} ifelse
} forall
0 eq {/Encoding DiacriticEncoding def} if
currentdict
end
} bind def
FMPColor

{
/BEGINBITMAPCOLOR {
BITMAPCOLOR} def
/BEGINBITMAPCOLORc {
BITMAPCOLORc} def
/BEGINBITMAPTRUECOLOR {
BITMAPTRUECOLOR } def
/BEGINBITMAPTRUECOLORc {
BITMAPTRUECOLORc } def
}

{
/BEGINBITMAPCOLOR {
BITMAPGRAY} def
/BEGINBITMAPCOLORc {
BITMAPGRAYc} def
/BEGINBITMAPTRUECOLOR {
BITMAPTRUEGRAY } def
/BEGINBITMAPTRUECOLORc {
BITMAPTRUEGRAYc } def
}
ifelse
/K {
FMPrintAllColorsAsBlack {
dup 1 eq 2 index 1 eq and 3 index 1 eq and not
{7 {pop} repeat 0 0 0 1 0 0 0} if
} if
FrameCurColors astore
pop combineColor
} bind def
/graymode true def
/bwidth FMLOCAL
/bpside FMLOCAL
/bstring FMLOCAL
/onbits FMLOCAL
/offbits FMLOCAL
/xindex FMLOCAL
/yindex FMLOCAL
/x FMLOCAL
/y FMLOCAL
/setPatternMode {
FMLevel1 {
/bwidth exch def
/bpside exch def
/bstring exch def
/onbits 0 def /offbits 0 def
freq sangle landscape {90 add} if
{/y exch def
/x exch def
/xindex x 1 add 2 div bpside mul cvi def
/yindex y 1 add 2 div bpside mul cvi def
bstring yindex bwidth mul xindex 8 idiv add get
1 7 xindex 8 mod sub bitshift and 0 ne FrameNegative {not} if
{/onbits onbits 1 add def 1}
{/offbits offbits 1 add def 0}
ifelse
}
setscreen
offbits offbits onbits add div FrameNegative {1.0 exch sub} if
/FrameCurGray exch def
} {
pop pop
dup patCache exch known {
patCache exch get
} {
dup
patDict /bstring 3 -1 roll put
patDict
9 PatFreq screenIndex get div dup matrix scale
makepattern
dup
patCache 4 -1 roll 3 -1 roll put
} ifelse
/FrameCurGray 0 def
/FrameCurPat exch def
} ifelse
/graymode false def
combineColor
} bind def
/setGrayScaleMode {
graymode not {
/graymode true def
FMLevel1 {
setCurrentScreen
} if
} if
/FrameCurGray exch def
combineColor
} bind def
/normalize {
transform round exch round exch itransform
} bind def
/dnormalize {
dtransform round exch round exch idtransform
} bind def
/lnormalize {
0 dtransform exch cvi 2 idiv 2 mul 1 add exch idtransform pop
} bind def
/H {
lnormalize setlinewidth
} bind def
/Z {
setlinecap
} bind def

/PFill {
graymode FMLevel1 or not {
gsave 1 setgray eofill grestore
} if
} bind def
/PStroke {
graymode FMLevel1 or not {
gsave 1 setgray stroke grestore
} if
stroke
} bind def
/fillvals FMLOCAL
/X {
fillvals exch get
dup type /stringtype eq
{8 1 setPatternMode}
{setGrayScaleMode}
ifelse
} bind def
/V {
PFill gsave eofill grestore
} bind def
/Vclip {
clip
} bind def
/Vstrk {
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/N {
PStroke
} bind def
/Nclip {
strokepath clip newpath
} bind def
/Nstrk {
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/M {newpath moveto} bind def
/E {lineto} bind def
/D {curveto} bind def
/O {closepath} bind def
/n FMLOCAL
/L {
/n exch def
newpath
normalize
moveto
2 1 n {pop normalize lineto} for
} bind def
/Y {
L
closepath
} bind def
/x1 FMLOCAL
/x2 FMLOCAL
/y1 FMLOCAL
/y2 FMLOCAL
/R {
/y2 exch def
/x2 exch def
/y1 exch def
/x1 exch def
x1 y1
x2 y1
x2 y2
x1 y2
4 Y
} bind def
/rad FMLOCAL
/rarc
{rad
arcto
} bind def
/RR {
/rad exch def
normalize
/y2 exch def
/x2 exch def
normalize
/y1 exch def
/x1 exch def
mark
newpath
{
x1 y1 rad add moveto
x1 y2 x2 y2 rarc
x2 y2 x2 y1 rarc
x2 y1 x1 y1 rarc
x1 y1 x1 y2 rarc
closepath
} stopped {x1 y1 x2 y2 R} if
cleartomark
} bind def
/RRR {
/rad exch def
normalize /y4 exch def /x4 exch def
normalize /y3 exch def /x3 exch def
normalize /y2 exch def /x2 exch def
normalize /y1 exch def /x1 exch def
newpath
normalize moveto
mark
{
x2 y2 x3 y3 rarc
x3 y3 x4 y4 rarc
x4 y4 x1 y1 rarc
x1 y1 x2 y2 rarc
closepath
} stopped
{x1 y1 x2 y2 x3 y3 x4 y4 newpath moveto lineto lineto lineto closepath} if
cleartomark
} bind def
/C {
grestore
gsave
R
clip
setCurrentScreen
} bind def
/CP {
grestore
gsave
Y
clip
setCurrentScreen
} bind def
/FMpointsize FMLOCAL
/F {
FMfonts exch get
FMpointsize scalefont
setfont
} bind def
/Q {
/FMpointsize exch def
F
} bind def
/T {
moveto show
} bind def
/RF {
rotate
0 ne {-1 1 scale} if
} bind def
/TF {
gsave
moveto
RF
show
grestore
} bind def
/P {
moveto
0 32 3 2 roll widthshow
} bind def
/PF {
gsave
moveto
RF
0 32 3 2 roll widthshow
grestore
} bind def
/S {
moveto
0 exch ashow
} bind def
/SF {
gsave
moveto
RF
0 exch ashow
grestore
} bind def
/B {
moveto
0 32 4 2 roll 0 exch awidthshow
} bind def
/BF {
gsave
moveto
RF
0 32 4 2 roll 0 exch awidthshow
grestore
} bind def
/G {
gsave
newpath
normalize translate 0.0 0.0 moveto
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
PFill fill
grestore
} bind def
/Gstrk {
savematrix
newpath
2 index 2 div add exch 3 index 2 div sub exch
normalize 2 index 2 div sub exch 3 index 2 div add exch
translate
scale
0.0 0.0 1.0 5 3 roll arc
restorematrix
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/Gclip {
newpath
savematrix
normalize translate 0.0 0.0 moveto
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
clip newpath
restorematrix
} bind def
/GG {
gsave
newpath
normalize translate 0.0 0.0 moveto
rotate
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
PFill
fill
grestore
} bind def
/GGclip {
savematrix
newpath
normalize translate 0.0 0.0 moveto
rotate
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
clip newpath
restorematrix
} bind def
/GGstrk {
savematrix
newpath
normalize translate 0.0 0.0 moveto
rotate
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
restorematrix
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/A {
gsave
savematrix
newpath
2 index 2 div add exch 3 index 2 div sub exch
normalize 2 index 2 div sub exch 3 index 2 div add exch
translate
scale
0.0 0.0 1.0 5 3 roll arc
restorematrix
PStroke
grestore
} bind def
/Aclip {
newpath
savematrix
normalize translate 0.0 0.0 moveto
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
strokepath clip newpath
restorematrix
} bind def
/Astrk {
Gstrk
} bind def
/AA {
gsave
savematrix
newpath

3 index 2 div add exch 4 index 2 div sub exch

normalize 3 index 2 div sub exch 4 index 2 div add exch
translate
rotate
scale
0.0 0.0 1.0 5 3 roll arc
restorematrix
PStroke
grestore
} bind def
/AAclip {
savematrix
newpath
normalize translate 0.0 0.0 moveto
rotate
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
strokepath clip newpath
restorematrix
} bind def
/AAstrk {
GGstrk
} bind def
/x FMLOCAL
/y FMLOCAL
/w FMLOCAL
/h FMLOCAL
/xx FMLOCAL
/yy FMLOCAL
/ww FMLOCAL
/hh FMLOCAL
/FMsaveobject FMLOCAL
/FMoptop FMLOCAL
/FMdicttop FMLOCAL
/BEGINPRINTCODE {
/FMdicttop countdictstack 1 add def
/FMoptop count 7 sub def
/FMsaveobject save def
userdict begin
/showpage {} def
FMNORMALIZEGRAPHICS
3 index neg 3 index neg translate
} bind def
/ENDPRINTCODE {
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
FMsaveobject restore
} bind def
/gn {
0
{ 46 mul
cf read pop
32 sub
dup 46 lt {exit} if
46 sub add
} loop
add
} bind def
/str FMLOCAL
/cfs {
/str sl string def
0 1 sl 1 sub {str exch val put} for
str def
} bind def
/ic [
0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0223
0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0223
0
{0 hx} {1 hx} {2 hx} {3 hx} {4 hx} {5 hx} {6 hx} {7 hx} {8 hx} {9 hx}
{10 hx} {11 hx} {12 hx} {13 hx} {14 hx} {15 hx} {16 hx} {17 hx} {18 hx}
{19 hx} {gn hx} {0} {1} {2} {3} {4} {5} {6} {7} {8} {9} {10} {11} {12}
{13} {14} {15} {16} {17} {18} {19} {gn} {0 wh} {1 wh} {2 wh} {3 wh}
{4 wh} {5 wh} {6 wh} {7 wh} {8 wh} {9 wh} {10 wh} {11 wh} {12 wh}
{13 wh} {14 wh} {gn wh} {0 bl} {1 bl} {2 bl} {3 bl} {4 bl} {5 bl} {6 bl}
{7 bl} {8 bl} {9 bl} {10 bl} {11 bl} {12 bl} {13 bl} {14 bl} {gn bl}
{0 fl} {1 fl} {2 fl} {3 fl} {4 fl} {5 fl} {6 fl} {7 fl} {8 fl} {9 fl}
{10 fl} {11 fl} {12 fl} {13 fl} {14 fl} {gn fl}
] def
/sl FMLOCAL
/val FMLOCAL
/ws FMLOCAL
/im FMLOCAL
/bs FMLOCAL
/cs FMLOCAL
/len FMLOCAL
/pos FMLOCAL
/ms {
/sl exch def
/val 255 def
/ws cfs
/im cfs
/val 0 def
/bs cfs
/cs cfs
} bind def
400 ms
/ip {
is
0
cf cs readline pop
{ ic exch get exec
add
} forall
pop

} bind def
/rip {


bis ris copy pop
is
0
cf cs readline pop
{ ic exch get exec
add
} forall
pop pop
ris gis copy pop
dup is exch

cf cs readline pop
{ ic exch get exec
add
} forall
pop pop
gis bis copy pop
dup add is exch

cf cs readline pop
{ ic exch get exec
add
} forall
pop

} bind def
/wh {
/len exch def
/pos exch def
ws 0 len getinterval im pos len getinterval copy pop
pos len
} bind def
/bl {
/len exch def
/pos exch def
bs 0 len getinterval im pos len getinterval copy pop
pos len
} bind def
/s1 1 string def
/fl {
/len exch def
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(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (5) 552.44 60.29 P
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1 12 Q
1.2 (Chapter 1) 72 677 S
2 24 Q
-0.48 (Pr) 207 677 S
-0.48 (eliminaries and) 229.61 677 S
-0.48 (Essential Reading) 207 647 S
3 12 Q
(1.1) 144 424 T
( This Handbook) 164.02 424 T
4 F
( 7) 511.99 424 T
3 F
(1.2) 144 406 T
( Changes since the previous version) 164.02 406 T
4 F
( 8) 511.99 406 T
3 10 Q
(1.2.1) 162 389.33 T
( This Handbook) 187.02 389.33 T
4 F
( 8) 513.66 389.33 T
3 F
(1.2.2) 162 373.33 T
( Side 1 A) 187.02 373.33 T
(vailability) 227.42 373.33 T
4 F
( 8) 513.66 373.33 T
3 F
(1.2.3) 162 357.33 T
( Acquiring Extended Objects with the GHRS) 187.02 357.33 T
4 F
( 8) 513.66 357.33 T
3 F
(1.2.4) 162 341.33 T
( Acquiring Faint Objects with the GHRS or FOS) 187.02 341.33 T
4 F
( 8) 513.66 341.33 T
3 F
(1.2.5) 162 325.33 T
( Noise Rejection for V) 187.02 325.33 T
(ery Faint Objects) 283.17 325.33 T
4 F
( 9) 513.66 325.33 T
3 F
(1.2.6) 162 309.33 T
( The Proposal Process for Cycle 5) 187.02 309.33 T
4 F
( 9) 513.66 309.33 T
3 F
(1.2.7) 162 293.33 T
( Updated Instrument Parameters) 187.02 293.33 T
4 F
( 9) 513.66 293.33 T
3 F
(1.2.8) 162 277.33 T
( GHRS Sensitivity) 187.02 277.33 T
4 F
( 9) 513.66 277.33 T
3 F
(1.2.9) 162 261.33 T
( GHRS Aperture Nomenclature) 187.02 261.33 T
4 F
( 9) 513.66 261.33 T
3 12 Q
(1.3) 144 244 T
( Where to \336nd additional information, changes, errata, etc.) 164.02 244 T
4 F
( 10) 505.32 244 T
FMENDPAGE
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(Preliminaries and Essential Reading) 189 736.18 T
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(6) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
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5 F
-0.13 (There are two reasons you may be referring to this) 189 679.35 P
6 F
-0.13 (Handbook) 392.06 679.35 P
5 F
-0.13 (. First, you may be consid-) 433.72 679.35 P
1.12 (ering using the GHRS to observe some celestial object, and you would like to know) 189 667.35 P
0.13 (what the instrument can do and how long it might take. Better yet, your proposal to use) 189 655.35 P
0.58 (the) 189 643.35 P
6 F
0.58 (Hubble Space T) 204.3 643.35 P
0.58 (elescope) 268.41 643.35 P
5 F
0.58 ( with the GHRS has been successful and you now need to) 302.84 643.35 P
0.57 (supply all the details of your observations that are needed in Phase II of proposal pro-) 189 631.35 P
(cessing.) 189 619.35 T
2.31 (Both tasks may seem daunting at \336rst because any versatile instrument has many) 189 599.35 P
0.85 (options. But for what most people want to do most of the time there are defaults that) 189 587.35 P
0.84 (apply) 189 575.35 P
0.84 (, and the GHRS is, in fact, a very easy-to-use device. Once you know that what) 210.57 575.35 P
-0.23 (you want to do falls within the bounds of conventional uses of the spectrograph, you can) 189 563.35 P
0.88 (proceed with some con\336dence that your observations will be successfully obtained in) 189 551.35 P
-0.23 (the form you originally desired. Or you can at least get a sense that what you are propos-) 189 539.35 P
(ing is truly unusual and may push the limits of the instrument.) 189 527.35 T
1.38 (This) 189 507.35 P
6 F
1.38 (Handbook) 210.66 507.35 P
5 F
1.38 ( exists as a basic reference manual for the Goddard High Resolution) 252.32 507.35 P
1.49 (Spectrograph \050GHRS\051, and describes its properties and operation. This) 189 495.35 P
6 F
1.49 (Handbook) 487.68 495.35 P
5 F
1.49 ( is) 529.34 495.35 P
-0.12 (revised and reissued approximately once each year) 189 483.35 P
-0.12 (. This version is written for observers) 391.01 483.35 P
0.77 (wishing to propose to use the GHRS in) 189 471.35 P
6 F
0.77 (HST\325) 354.06 471.35 P
5 F
0.77 (s Cycle 5, and it supersedes all previous) 374.62 471.35 P
1.76 (versions of the) 189 459.35 P
6 F
1.76 ( Instrument Handbook) 251.4 459.35 P
5 F
1.76 (. No) 344.91 459.35 P
6 F
1.76 (HST) 368.15 459.35 P
5 F
1.76 ( document stands alone in providing) 385.93 459.35 P
0.77 (complete information because each \336lls a particular need. The) 189 447.35 P
6 F
0.77 (Call for Pr) 446.95 447.35 P
0.77 (oposals) 492.01 447.35 P
5 F
0.77 (, for) 522.57 447.35 P
1.56 (example, describes the proposal submission process and provides a summary of the) 189 435.35 P
2.61 (observatory and its instruments. The) 189 423.35 P
6 F
2.61 (Phase II Pr) 350.38 423.35 P
2.61 (oposal Instructions) 401.33 423.35 P
5 F
2.61 ( give detailed) 480.9 423.35 P
0.02 (instructions for providing STScI with the speci\336cations that translate your program into) 189 411.35 P
0.73 (commands that) 189 399.35 P
6 F
0.73 (HST) 253.79 399.35 P
5 F
0.73 ( executes. The instrument handbooks supplement both documents) 271.57 399.35 P
0.95 (by providing the technical details of instrument performance and operation. The) 189 387.35 P
6 F
0.95 (HST) 522.22 387.35 P
-0.19 (Data Handbook) 189 375.35 P
5 F
-0.19 (describes how software takes the raw data from the telescope and trans-) 255.27 375.35 P
0.34 (forms it into a reduced and calibrated form for your further analysis and interpretation,) 189 363.35 P
(and how you can duplicate those steps.) 189 351.35 T
6 F
0.35 (HST) 189 331.35 P
5 F
0.35 ( is now a fairly mature spacecraft and so we can predict what many observers will) 206.78 331.35 P
1.46 (need. This) 189 319.35 P
6 F
1.46 (Handbook) 236.09 319.35 P
5 F
1.46 ( is designed around the needs of the majority of users, so that) 277.75 319.35 P
0.4 (essential information is concentrated in a few sections. Full details must also be given,) 189 307.35 P
0.26 (of course, and they are provided in a reference section. W) 189 295.35 P
0.26 (e demonstrate the ease of use) 421.8 295.35 P
1.44 (of the GHRS by providing examples for some of the dif) 189 283.35 P
1.44 (ferent situations that a user) 426.49 283.35 P
-0.17 (might encounter) 189 271.35 P
-0.17 (. W) 253.55 271.35 P
-0.17 (e have also tried to provide the information you need to decide when) 267.03 271.35 P
(your observations deviate from the \322normal\323 and involve special aspects.) 189 259.35 T
0.8 (No handbook of this kind can be complete and error) 189 239.35 P
0.8 (-free until the instrument itself is) 404.6 239.35 P
0.21 (obsolete. W) 189 227.35 P
0.21 (e have, of course, edited it thoroughly) 236.18 227.35 P
0.21 (, but if signi\336cant revisions are called) 388.46 227.35 P
0.09 (for they will be announced via STEIS) 189 215.35 P
5 8 Q
0.07 (1) 340.65 219.35 P
5 10 Q
0.09 (, as with other) 344.65 215.35 P
6 F
0.09 (HST) 404.18 215.35 P
5 F
0.09 ( news items. Do not be afraid) 421.96 215.35 P
-0.04 (to consult with us if you have questions; the means of contact are provided just after the) 189 203.35 P
(title page.) 189 191.35 T
0.51 (As we said, this particular version of the) 189 171.35 P
6 F
0.51 (GHRS Instrument Handbook) 357.2 171.35 P
5 F
0.51 ( is being written) 473.76 171.35 P
0.22 (for Cycle 5 of the) 189 159.35 P
6 F
0.22 (HST) 263.11 159.35 P
5 F
0.22 ( science program. That means that we are providing information) 280.89 159.35 P
1.82 (on how the instrument works after the Servicing Mission installed COST) 189 147.35 P
1.82 (AR and a) 498.59 147.35 P
0.4 (GHRS Repair Kit. COST) 189 135.35 P
0.4 (AR changed the image scale of) 291.07 135.35 P
6 F
0.4 (HST) 420.66 135.35 P
5 F
0.4 ( at the entrance apertures) 438.44 135.35 P
54 96.98 540 126.98 C
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(1. This and other terms are de\336ned and described in a Glossary at the end of this) 189 90.98 T
6 F
(Handbook.) 482.7 90.98 T
FMENDPAGE
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(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (7) 552.44 60.29 P
72 750.02 558 750.02 2 L
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0 9 Q
(Preliminaries and Essential Reading) 207 736.18 T
5 10 Q
-0.25 (of the GHRS; it also produces dif) 207 679.35 P
-0.25 (fraction-limited images, but does not alter GHRS oper-) 339.21 679.35 P
-0.01 (ations in any fundamental manner) 207 667.35 P
-0.01 (. In other words, COST) 342.51 667.35 P
-0.01 (AR alters some of the parame-) 435.56 667.35 P
1.22 (ters used in various calculations for pointing and throughput, but the instrument still) 207 655.35 P
(operates in the same way) 207 643.35 T
(.) 306.88 643.35 T
0.26 (The GHRS Repair Kit enabled the reactivation of Side 1 of the GHRS, once again per-) 207 623.35 P
1.64 (mitting short-wavelength echelle spectra to be obtained, as well as spectra with the) 207 611.35 P
1.12 (G140L and G140M gratings. At the time this is written Side 1 reactivation has been) 207 599.35 P
1.09 (completed and a few observations have been made. They indicate that Side 1 is per-) 207 587.35 P
0.79 (forming with essentially the same science capabilities that it had at the time of) 207 575.35 P
6 F
0.79 (HST\325) 533.55 575.35 P
5 F
0.79 (s) 554.11 575.35 P
(launch.) 207 563.35 T
72 520.02 558 523.02 C
0 0 0 1 0 0 0 K
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207 521.52 558 521.52 2 L
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72 521.52 198 521.52 2 L
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0 0 612 792 C
0 12 Q
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0 0 0 1 0 0 0 K
(1.1) 181.32 527.02 T
(This Handbook) 207 527.02 T
5 10 Q
0.78 (If you have looked through the T) 207 503.35 P
0.78 (able of Contents, you will have seen that this) 343.2 503.35 P
6 F
0.78 (Hand-) 532.45 503.35 P
(book) 207 491.35 T
5 F
( is divided into four parts:) 226.44 491.35 T
0.4 (Part I is a summary in which this) 221.4 473.35 P
6 F
0.4 (Handbook) 359 473.35 P
5 F
0.4 ( is described and suggestions are made) 400.66 473.35 P
0.48 (on how to use this document and how it is related to other) 221.4 461.35 P
6 F
0.48 (HST) 461.79 461.35 P
5 F
0.48 (-related documents.) 478.65 461.35 P
0.42 (Part I also describes how) 221.4 449.35 P
6 F
0.42 (HST) 325.97 449.35 P
5 F
0.42 ( proposals are processed for review by the T) 343.75 449.35 P
0.42 (elescope) 523.57 449.35 P
1.41 (Allocation Committee \050T) 221.4 437.35 P
1.41 (AC\051 and how successful proposals get turned into com-) 324.53 437.35 P
0.06 (mands that the spacecraft can execute; and it describes how the installation of COS-) 221.4 425.35 P
(T) 221.4 413.35 T
(AR af) 226.71 413.35 T
(fects the GHRS and what the basic properties of the instrument are.) 250.69 413.35 T
0.16 (Part II elaborates on the writing of proposals to use the GHRS, both for Phase I and) 221.4 398.35 P
0.63 (Phase II. The Phase I proposal is what the T) 221.4 386.35 P
0.63 (AC sees, and it describes the observa-) 402.33 386.35 P
0.14 (tions to be made in broad terms. The most important technical decisions to be made) 221.4 374.35 P
0.89 (regard the tar) 221.4 362.35 P
0.89 (get acquisition strategy to adopt and the amount of exposure time to) 276.31 362.35 P
1.5 (request. The Phase II proposal encompasses all the details that the planning and) 221.4 350.35 P
(scheduling systems need to turn your program into commands for the spacecraft.) 221.4 338.35 T
1.21 (Part III is a reference section, and it includes the details that a) 221.4 323.35 P
6 F
1.21 (Handbook) 485.96 323.35 P
5 F
1.21 ( should) 527.62 323.35 P
(without cluttering the introductory explanations.) 221.4 311.35 T
(Part IV is a short glossary of GHRS terms and abbreviations and an index.) 221.4 296.35 T
0.49 (Data reduction and analysis are not covered in this) 207 276.35 P
6 F
0.49 (Handbook) 416.09 276.35 P
5 F
0.49 ( because they are treated) 457.75 276.35 P
0.9 (in detail in the) 207 264.35 P
6 F
0.9 (HST Data Handbook,) 270.62 264.35 P
5 F
0.9 (although we anticipate mer) 362.77 264.35 P
0.9 (ging portions of that) 473.9 264.35 P
(document into this in the future.) 207 252.35 T
-0.14 (External references have been included where appropriate in order not to duplicate what) 207 232.35 P
-0.1 (is available elsewhere, but we have tried to include almost everything you need to know) 207 220.35 P
0.37 (about the GHRS when writing a proposal. If you \336nd that you need information that is) 207 208.35 P
(not in here, please consult with us.) 207 196.35 T
0.22 (This document follows the usual STScI convention in which terms, words, and phrases) 207 176.35 P
0.19 (which are to be entered by the user in a literal way on a form are shown in a typewriter) 207 164.35 P
(font \050e.g.,) 207 152.35 T
7 F
(BRIGHT=RETURN,EARLY ACQ) 248.38 152.35 T
5 F
(\051.) 386.38 152.35 T
FMENDPAGE
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(8) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
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54 726.98 540 726.98 2 L
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54 74.02 540 74.02 2 L
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54 750.02 540 750.02 2 L
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54 726.98 540 726.98 2 L
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(1.2) 163.32 678.02 T
(Changes since the previous version) 189 678.02 T
0 10 Q
(1.2.1) 157.76 644.35 T
(This Handbook) 189 644.35 T
5 F
0.94 (This version of the) 189 624.35 P
6 F
0.94 (GHRS) 270.54 624.35 P
0.94 (Instrument) 299.54 624.35 P
0.94 (Handbook) 346.31 624.35 P
5 F
0.94 ( has been only modestly rewritten. It) 387.97 624.35 P
1.85 (incorporates a few updates since version 4.0 that were issued electronically) 189 612.35 P
1.85 (. Please) 507.6 612.35 P
0.14 (bring errors to the attention of a GHRS Instrument Scientist \050see back of title page\051. As) 189 600.35 P
0.06 (before, wavelength units in this) 189 588.35 P
6 F
0.06 (Handbook) 317.62 588.35 P
5 F
0.06 ( are in \201ngstroms \050\201\051, in keeping with astro-) 359.28 588.35 P
(nomical tradition. A transition to SI units may take place in a future edition.) 189 576.35 T
0 F
(1.2.2) 157.76 546.35 T
(Side 1 A) 189 546.35 T
(vailability) 228.09 546.35 T
5 F
1.64 (At the time this is written, the capabilities of Side 1 of the GHRS have been fully) 189 526.35 P
1.86 (restored, permitting one to obtain high-, medium-, or low-resolution spectra with a) 189 514.35 P
0.34 (cesium iodide photocathode. W) 189 502.35 P
0.34 (e encourage you to consider its use. The low-resolution) 315.89 502.35 P
-0.07 (mode on Side 1 using grating G140L particularly makes the GHRS useful for observing) 189 490.35 P
1.36 (faint objects in the far ultraviolet. The next two paragraphs discuss issues related to) 189 478.35 P
(acquiring such tar) 189 466.35 T
(gets.) 260.47 466.35 T
0 F
(1.2.3) 157.76 436.35 T
(Acquiring Extended Objects with the GHRS) 189 436.35 T
5 F
2.07 (An) 189 416.35 P
7 F
4.97 (EXTENDED) 205.79 416.35 P
5 F
2.07 ( option for) 253.79 416.35 P
7 F
4.97 (ACQ/PEAKUP) 304.72 416.35 P
5 F
2.07 ( was described in earlier versions of this) 364.72 416.35 P
6 F
2.07 (Handbook.) 189 404.35 P
5 F
2.07 (It will be tested in Cycle 4 and should be available for routine use in) 237.73 404.35 P
1.12 (Cycle) 189 392.35 P
1.12 (5. It was written with the Gallilean satellites of Jupiter in mind, but should be) 214.83 392.35 P
(applicable to other extended objects. See Section) 189 380.35 T
(4.1.5.4 on page) 387.3 380.35 T
(39 for more details.) 451.18 380.35 T
1.32 (W) 189 360.35 P
1.32 (e have also provided some guidance for users who may wish to observe extended) 197.64 360.35 P
(objects so that acquisition count rates can be estimated; see Section) 189 348.35 T
(7.3 on page) 460.91 348.35 T
(76.) 509.79 348.35 T
0 F
(1.2.4) 157.76 318.35 T
(Acquiring Faint Objects with the GHRS or FOS) 189 318.35 T
5 F
-0.01 (In some cases the G140L grating on Side 1 may provide an ef) 189 298.35 P
-0.01 (\336cient means of obtaining) 435.87 298.35 P
1.89 (a low-resolution spectrum of a source, but acquiring that object can be dif) 189 286.35 P
1.89 (\336cult or) 506.72 286.35 P
-0.06 (impossible with the GHRS\325 Side 1 because of the limited response of mirror N1 and the) 189 274.35 P
-0.04 (maximum permissible) 189 262.35 P
7 F
-0.1 (STEP-TIME) 280.59 262.35 P
5 F
-0.04 ( of 12.75 seconds. There are two ways to overcome) 334.59 262.35 P
(this problem:) 189 250.35 T
8 11 Q
(\245) 189 232.35 T
5 10 Q
0.28 (Acquire the object with Side 2 of the GHRS \050mirror N2\051, then observe with Side 1.) 203.4 232.35 P
-0.15 (Using this technique will add about 40 minutes of overhead time involved in switch-) 203.4 220.35 P
(ing Sides, but often that can occur when the spacecraft is behind the earth anyway) 203.4 208.35 T
(.) 530.73 208.35 T
8 11 Q
(\245) 189 193.35 T
5 10 Q
0.28 (Acquire the object with the Faint Object Spectrograph and then move it to the LSA) 203.4 193.35 P
1.14 (of the GHRS. The positions of the COST) 203.4 181.35 P
1.14 (AR mirrors for the FOS and GHRS are) 375.61 181.35 P
0.36 (quite close, so that the movement of an object from an FOS aperture to the LSA of) 203.4 169.35 P
0.59 (the GHRS is only about 1 arcmin, a small enough motion to ensure that the object) 203.4 157.35 P
1.26 (will fall within the LSA because one set of guide stars will suf) 203.4 145.35 P
1.26 (\336ce. This method) 467.76 145.35 P
(should) 203.4 133.35 T
6 F
(not) 232.57 133.35 T
5 F
( be used for SSA observations.) 245.35 133.35 T
0.14 (At the time this is being written this method of cross-spectrograph acquisitions is being) 189 113.35 P
-0.1 (evaluated and tested. Please consult with us if you wish to consider using it. Also please) 189 101.35 P
FMENDPAGE
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72 726.98 558 726.98 2 L
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72 74.02 558 74.02 2 L
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(GHRS Instrument Handbook 5.0) 207 60.29 T
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72 750.02 558 750.02 2 L
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0 Z
N
72 726.98 558 726.98 2 L
0.25 H
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72 74.02 558 74.02 2 L
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72 750.02 558 750.02 2 L
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72 726.98 558 726.98 2 L
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72 74.02 558 74.02 2 L
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(Preliminaries and Essential Reading) 207 736.18 T
5 10 Q
0.17 (note that the opposite sense will also work, namely acquiring a \322bright\323 object with the) 207 679.35 P
(GHRS in order to observe it with the FOS.) 207 667.35 T
0 F
(1.2.5) 175.76 637.35 T
(Noise Rejection for V) 207 637.35 T
(ery Faint Objects) 307.03 637.35 T
5 F
1.48 (A special commanding option called) 207 617.35 P
7 F
3.55 (FLYLIM) 363.54 617.35 P
5 F
1.48 ( can be invoked to reject noise in the) 399.54 617.35 P
-0.11 (GHRS when the object observed is signi\336cantly fainter than the level of the background) 207 605.35 P
-0.03 (noise. Although only applicable in special situations, it can be very ef) 207 593.35 P
-0.03 (fective. Please see) 485.04 593.35 P
(Section) 207 581.35 T
(8.6.3 on page) 239.5 581.35 T
(97.) 295.88 581.35 T
0 F
(1.2.6) 175.76 551.35 T
(The Proposal Process for Cycle 5) 207 551.35 T
5 F
0.16 (The basic methodology of proposal writing for) 207 531.35 P
6 F
0.16 (HST) 397.8 531.35 P
5 F
0.16 ( has been changed. Y) 415.58 531.35 P
0.16 (ou should rely) 500.46 531.35 P
0.62 (on the proposal instructions being issued with this) 207 519.35 P
6 F
0.62 (Handbook) 414.7 519.35 P
5 F
0.62 ( for guidance if there are) 456.36 519.35 P
0.95 (any con\337icts, but the essential information needed \050sequence of operations and expo-) 207 507.35 P
(sure times\051 has not changed.) 207 495.35 T
0 F
(1.2.7) 175.76 465.35 T
(Updated Instrument Parameters) 207 465.35 T
5 F
2.38 (Because of the Servicing Mission, the GHRS is a brand-new instrument in many) 207 445.35 P
0.95 (respects. W) 207 433.35 P
0.95 (e have undertaken to measure many basic instrumental quantities, such as) 253.8 433.35 P
0.37 (sensitivities,) 207 421.35 P
6 F
0.37 (ab) 259.6 421.35 P
0.37 (initio) 272.47 421.35 P
5 F
0.37 ( so that observations obtained in Cycle 4 and beyond can be cali-) 293.59 421.35 P
0.69 (brated to the best possible level. Many of those observations were not been fully ana-) 207 409.35 P
0.72 (lyzed at the time this) 207 397.35 P
6 F
0.72 (Handbook) 296.45 397.35 P
5 F
0.72 ( was last revised before issuance. The numeric values) 338.11 397.35 P
0.1 (herein, particularly sensitivities, are therefore not \322\336nal\323 values that will be in place for) 207 385.35 P
0.34 (data reduction, but they do re\337ect our knowledge of the post-Servicing Mission GHRS) 207 373.35 P
0.16 (and will therefore lead to reliable exposure estimates. Updated information will be pro-) 207 361.35 P
(vided on STEIS as it becomes available.) 207 349.35 T
0 F
(1.2.8) 175.76 319.35 T
(GHRS Sensitivity) 207 319.35 T
5 F
0.14 (The sensitivity of the GHRS has turned out to be more wavelength-dependent than was) 207 303.35 P
0.46 (anticipated prior to the Servicing Mission; see Section) 207 291.35 P
0.46 (8.1 on page) 429.63 291.35 P
0.46 (82. The reasons for) 479.43 291.35 P
-0.11 (this are not known, but users should use the measured sensitivity values in Section) 207 279.35 P
-0.11 (8.2.3) 538 279.35 P
0.85 (on page) 207 267.35 P
0.85 (85 and Section) 241.73 267.35 P
0.85 (8.3.1 on page) 305.38 267.35 P
0.85 (87 when calculating exposure times and should) 363.46 267.35 P
(de\336nitely) 207 255.35 T
6 F
(not) 247.28 255.35 T
5 F
( scale exposures from older proposals.) 260.06 255.35 T
0 F
(1.2.9) 175.76 225.35 T
(GHRS Aperture Nomenclature) 207 225.35 T
5 F
0.37 (The plate scale at the entrance apertures of the GHRS is altered by COST) 207 205.35 P
0.37 (AR such that) 505.05 205.35 P
0.22 (the angular scale per unit of physical length is reduced by a factor of 0.87. \050COST) 207 193.35 P
0.22 (AR\325) 537.44 193.35 P
0.22 (s) 554.11 193.35 P
0.03 (mirrors also introduce anamorphic magni\336cation, but its ef) 207 181.35 P
0.03 (fect is so small \320 about 0.5%) 442.55 181.35 P
1.14 (\320 that it is ignored here.\051 That means that the aperture sizes change in the following) 207 169.35 P
(way:) 207 157.35 T
0 8 Q
(Aperture) 211.3 135.68 T
(Nomenclature) 341.16 135.68 T
-0.2 (Pre-COST) 425.19 135.68 P
-0.2 (AR Size) 462.38 135.68 P
(New Size) 503.96 135.68 T
5 9 Q
(Lar) 211.3 121.02 T
(ge Science Aperture \050LSA\051) 223.63 121.02 T
7 F
(2.0) 369.07 121.02 T
5 F
(2.00 arcsec) 438.34 121.02 T
(1.74 arcsec) 503.96 121.02 T
(Small Science Aperture \050SSA\051) 211.3 106.02 T
7 F
(0.25) 366.37 106.02 T
5 F
(0.25 arcsec) 438.34 106.02 T
(0.22 arcsec) 503.96 106.02 T
205.3 147.77 205.3 101.27 2 L
V
0.5 H
0 Z
N
335.16 148.27 335.16 100.77 2 L
V
N
419.19 148.27 419.19 100.77 2 L
V
N
497.96 148.27 497.96 100.77 2 L
V
N
553.72 147.77 553.72 101.27 2 L
V
N
205.05 148.02 553.97 148.02 2 L
V
N
205.05 131.02 553.97 131.02 2 L
V
2 H
N
205.05 101.02 553.97 101.02 2 L
V
0.5 H
N
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0 0 0 1 0 0 0 K
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0 9 Q
(Preliminaries and Essential Reading) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
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0 10 Q
(10) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
5 F
-0.17 (Note that the names used to designate the apertures of the GHRS have not changed even) 189 679.35 P
0.58 (though their angular sizes did. T) 189 667.35 P
0.58 (o lessen confusion somewhat, we will use \322LSA\323 and) 320.64 667.35 P
(\322SSA\323 to refer to the lar) 189 655.35 T
(ge and small apertures, respectively) 285.74 655.35 T
(, of the GHRS.) 428.11 655.35 T
54 612.02 540 615.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 613.52 540 613.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
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54 613.52 180 613.52 2 L
0 Z
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0 0 612 792 C
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0 0 0 1 0 0 0 K
(1.3) 163.32 619.02 T
(Where to \336nd additional information, changes, errata, etc.) 189 619.02 T
5 10 Q
0.19 (As we mentioned, the) 189 595.35 P
6 F
0.19 (Call for Pr) 279.48 595.35 P
0.19 (oposals) 323.4 595.35 P
5 F
0.19 ( provides an overview of) 353.96 595.35 P
6 F
0.19 (HST) 456.84 595.35 P
5 F
0.19 ( capabilities and) 474.62 595.35 P
1.92 (describes how a Phase I proposal is to be prepared. It goes hand-in-hand with the) 189 583.35 P
6 F
-0.06 (Phase) 189 571.35 P
-0.06 (I Pr) 215.94 571.35 P
-0.06 (oposal Instructions) 231.34 571.35 P
5 F
-0.06 ( and documents for the Remote Proposal Submission Sys-) 308.24 571.35 P
0.2 (tem \050RPSS\051. If your proposal is successful, you will need to submit a Phase II proposal) 189 559.35 P
2.28 (that provides all the speci\336c details we need to ensure that your observations are) 189 547.35 P
0.25 (obtained in the form you intend. This) 189 535.35 P
6 F
0.25 (Handbook) 342.41 535.35 P
5 F
0.25 ( provides much of the information you) 384.07 535.35 P
0.64 (will need in Phase II, with the proposal procedures themselves in a) 189 523.35 P
6 F
0.64 (Phase II Pr) 466.33 523.35 P
0.64 (oposal) 513.33 523.35 P
0.29 (Instructions) 189 511.35 P
5 F
0.29 (book. There is also a separate document that describes how to process and) 239.57 511.35 P
2.08 (reduce GHRS data. Contact the User Support Branch of STScI for further details.) 189 499.35 P
0.6 (\050Please note, incidentally) 189 487.35 P
0.6 (, that the) 290.37 487.35 P
6 F
0.6 (T) 329.38 487.35 P
0.6 (ar) 334.02 487.35 P
0.6 (get Acquisition Handbook) 342.54 487.35 P
5 F
0.6 (is no longer produced) 451.27 487.35 P
(because it is redundant.\051) 189 475.35 T
0.62 (There is a separate document titled) 189 455.35 P
6 F
0.62 (HST Data Handbook) 334.88 455.35 P
5 F
0.62 (that describes how) 423.67 455.35 P
6 F
0.62 (HST) 502.44 455.35 P
5 F
0.62 ( data) 520.22 455.35 P
0.75 (are reduced by the \322pipeline\323 system and how you can reproduce those steps to tailor) 189 443.35 P
(the reduction to your needs. A copy may be obtained from the User Support Branch.) 189 431.35 T
1.01 (This) 189 411.35 P
6 F
1.01 ( Instrument Handbook) 206.78 411.35 P
5 F
1.01 (is written to apply to the Goddard High Resolution Spec-) 302.3 411.35 P
0.97 (trograph as it will be con\336gured and will operate in Cycle 5 of the) 189 399.35 P
6 F
0.97 (HST) 469.19 399.35 P
5 F
0.97 ( science pro-) 486.97 399.35 P
1.24 (gram. The installation of COST) 189 387.35 P
1.24 (AR has changed the dimensions of the apertures and) 320.11 387.35 P
0.7 (other elements of GHRS as measured in arcsec projected on the sky) 189 375.35 P
0.7 (. The new dimen-) 467.36 375.35 P
-0.06 (sions have been used throughout this document. This) 189 363.35 P
6 F
-0.06 (Handbook) 403.25 363.35 P
5 F
-0.06 ( supersedes all previous) 444.91 363.35 P
0.19 (versions, but if another document con\337icts with this) 189 351.35 P
6 F
0.19 (Handbook) 400.75 351.35 P
5 F
0.19 (, you should use the one) 442.41 351.35 P
(with the most recent date-of-issue.) 189 339.35 T
0.86 (Y) 189 319.35 P
0.86 (ou should also be aware of STEIS, the) 195.22 319.35 P
6 F
0.86 (Space T) 357.89 319.35 P
0.86 (elescope Electr) 389.77 319.35 P
0.86 (onic Information Ser-) 451.62 319.35 P
-0.04 (vice) 189 307.35 P
5 F
-0.04 (. STEIS provides an easy way to check for updates to existing documents and to get) 205.1 307.35 P
6 F
0.55 (HST) 189 295.35 P
5 F
0.55 (-related information and news. T) 205.86 295.35 P
0.55 (o use STEIS,) 338.7 295.35 P
6 F
0.55 (ftp) 395.34 295.35 P
5 F
0.55 (to) 408.95 295.35 P
6 F
0.55 (stsci.edu) 419.77 295.35 P
5 F
0.55 (, enter) 454.49 295.35 P
6 F
0.55 (anonymous) 483.07 295.35 P
5 F
0.55 (as) 531.67 295.35 P
0.17 (the user and your last name as the password. T) 189 283.35 P
0.17 (ransfer the README \336le in the highest-) 376.79 283.35 P
-0.17 (level directory with a) 189 271.35 P
6 F
-0.17 ( get) 273.76 271.35 P
5 F
-0.17 (command to get basic information. V) 290.65 271.35 P
-0.17 (arious subdirectories pro-) 438.13 271.35 P
0.01 (vide details on speci\336c subjects. For more information on STEIS, contact the User Sup-) 189 259.35 P
0.55 (port Branch. The xterm interface to) 189 247.35 P
6 F
0.55 (ftp) 336.41 247.35 P
5 F
0.55 ( called) 346.97 247.35 P
6 F
0.55 (Mosaic) 376.94 247.35 P
5 F
0.55 ( is an especially ef) 406.38 247.35 P
0.55 (fective way to) 482.26 247.35 P
(access STEIS.) 189 235.35 T
-0.14 (Y) 189 215.35 P
-0.14 (ou are always welcome to call us, the STScI GHRS team, to get information when you) 195.22 215.35 P
0.01 (\336nd yourself confused or at a loss. W) 189 203.35 P
0.01 (e prefer e-mail \050to the addresses on the back of the) 337.71 203.35 P
(title page\051, but you may contact us by telephone if you wish.) 189 191.35 T
(Finally) 189 171.35 T
(, you will \336nd some additional sources of information in Chapter 9.) 216.69 171.35 T
54 265.71 180.29 403.3 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 265.71 180.29 403.3 R
6 X
0 0 0 1 0 0 0 K
V
63 274.59 171.29 395.02 R
7 X
V
9 11 Q
0 X
0.3 (Do not use out-of-) 68.76 383.68 P
7.07 (date documents) 68.76 370.68 P
7.34 (as a sour) 68.76 357.68 P
7.34 (ce of) 130.22 357.68 P
1.86 (infor) 68.76 344.68 P
1.86 (mation! If this) 91.95 344.68 P
10 F
10.86 (Handbook) 68.76 331.68 P
9 F
10.86 ( does) 125.46 331.68 P
7.13 (not contain the) 68.76 318.68 P
13.07 (infor) 68.76 305.68 P
13.07 (mation you) 91.95 305.68 P
26.34 (need, please) 68.76 292.68 P
(consult us.) 68.76 279.68 T
63 274.59 171.29 395.02 R
1 H
2 Z
N
54.5 266.21 179.79 402.8 R
0 Z
N
0 0 612 792 C
FMENDPAGE
%%EndPage: "10" 6
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%%Pages: 6
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%%+ Times-Roman
%%+ Times-Italic
%%+ Courier
%%+ Courier-Bold
%%+ AvantGarde-Book
%%+ AvantGarde-BookOblique
%%EOF
%!PS-Adobe-3.0
%%BoundingBox: (atend)
%%Pages: (atend)
%%PageOrder: (atend)
%%DocumentFonts: (atend)
%%Creator: Frame 4.0
%%DocumentData: Clean7Bit
%%EndComments
%%BeginProlog
%
% Frame ps_prolog 4.0, for use with Frame 4.0 products
% This ps_prolog file is Copyright (c) 1986-1993 Frame Technology
% Corporation. All rights reserved. This ps_prolog file may be
% freely copied and distributed in conjunction with documents created
% using FrameMaker, FrameBuilder and FrameViewer as long as this
% copyright notice is preserved.
%
% Frame products normally print colors as their true color on a color printer
% or as shades of gray, based on luminance, on a black-and white printer. The
% following flag, if set to True, forces all non-white colors to print as pure
% black. This has no effect on bitmap images.
/FMPrintAllColorsAsBlack false def
%
% Frame products can either set their own line screens or use a printer's
% default settings. Three flags below control this separately for no
% separations, spot separations and process separations. If a flag
% is true, then the default printer settings will not be changed. If it is
% false, Frame products will use their own settings from a table based on
% the printer's resolution.
/FMUseDefaultNoSeparationScreen true def
/FMUseDefaultSpotSeparationScreen true def
/FMUseDefaultProcessSeparationScreen false def
%
% For any given PostScript printer resolution, Frame products have two sets of
% screen angles and frequencies for printing process separations, which are
% recomended by Adobe. The following variable chooses the higher frequencies
% when set to true or the lower frequencies when set to false. This is only
% effective if the appropriate FMUseDefault...SeparationScreen flag is false.
/FMUseHighFrequencyScreens true def
%
% PostScript Level 2 printers contain an "Accurate Screens" feature which can
% improve process separation rendering at the expense of compute time. This
% flag is ignored by PostScript Level 1 printers.
/FMUseAcccurateScreens true def
%
% The following PostScript procedure defines the spot function that Frame
% products will use for process separations. You may un-comment-out one of
% the alternative functions below, or use your own.
%
% Dot function
/FMSpotFunction {abs exch abs 2 copy add 1 gt
{1 sub dup mul exch 1 sub dup mul add 1 sub }
{dup mul exch dup mul add 1 exch sub }ifelse } def
%
% Line function
% /FMSpotFunction { pop } def
%
% Elipse function
% /FMSpotFunction { dup 5 mul 8 div mul exch dup mul exch add
% sqrt 1 exch sub } def
%
%
/FMversion (4.0) def
/FMLevel1 /languagelevel where {pop languagelevel} {1} ifelse 2 lt def
/FMPColor
FMLevel1 {
false
/colorimage where {pop pop true} if
} {
true
} ifelse
def
/FrameDict 400 dict def
systemdict /errordict known not {/errordict 10 dict def
errordict /rangecheck {stop} put} if
% The readline in PS 23.0 doesn't recognize cr's as nl's on AppleTalk
FrameDict /tmprangecheck errordict /rangecheck get put
errordict /rangecheck {FrameDict /bug true put} put
FrameDict /bug false put
mark
% Some PS machines read past the CR, so keep the following 3 lines together!
currentfile 5 string readline
00
0000000000
cleartomark
errordict /rangecheck FrameDict /tmprangecheck get put
FrameDict /bug get {
/readline {
/gstring exch def
/gfile exch def
/gindex 0 def
{
gfile read pop
dup 10 eq {exit} if
dup 13 eq {exit} if
gstring exch gindex exch put
/gindex gindex 1 add def
} loop
pop
gstring 0 gindex getinterval true
} bind def
} if
/FMshowpage /showpage load def
/FMquit /quit load def
/FMFAILURE {
dup = flush
FMshowpage
/Helvetica findfont 12 scalefont setfont
72 200 moveto
show FMshowpage
FMquit
} def
/FMVERSION {
FMversion ne {
(Frame product version does not match ps_prolog!) FMFAILURE
} if
} def
/FMBADEPSF {
(PostScript Lang. Ref. Man., 2nd Ed., H.2.4 says EPS must not call X )
dup dup (X) search pop exch pop exch pop length
4 -1 roll
putinterval
FMFAILURE
} def
/FMLOCAL {
FrameDict begin
0 def
end
} def
/concatprocs
{
/proc2 exch cvlit def/proc1 exch cvlit def/newproc proc1 length proc2 length add array def
newproc 0 proc1 putinterval newproc proc1 length proc2 putinterval newproc cvx
}def
FrameDict begin
/FMnone 0 def
/FMcyan 1 def
/FMmagenta 2 def
/FMyellow 3 def
/FMblack 4 def
/FMcustom 5 def
/FrameNegative false def
/FrameSepIs FMnone def
/FrameSepBlack 0 def
/FrameSepYellow 0 def
/FrameSepMagenta 0 def
/FrameSepCyan 0 def
/FrameSepRed 1 def
/FrameSepGreen 1 def
/FrameSepBlue 1 def
/FrameCurGray 1 def
/FrameCurPat null def
/FrameCurColors [ 0 0 0 1 0 0 0 ] def
/FrameColorEpsilon .001 def
/eqepsilon {
sub dup 0 lt {neg} if
FrameColorEpsilon le
} bind def
/FrameCmpColorsCMYK {
2 copy 0 get exch 0 get eqepsilon {
2 copy 1 get exch 1 get eqepsilon {
2 copy 2 get exch 2 get eqepsilon {
3 get exch 3 get eqepsilon
} {pop pop false} ifelse
}{pop pop false} ifelse
} {pop pop false} ifelse
} bind def
/FrameCmpColorsRGB {
2 copy 4 get exch 0 get eqepsilon {
2 copy 5 get exch 1 get eqepsilon {
6 get exch 2 get eqepsilon
}{pop pop false} ifelse
} {pop pop false} ifelse
} bind def
/RGBtoCMYK {
1 exch sub
3 1 roll
1 exch sub
3 1 roll
1 exch sub
3 1 roll
3 copy
2 copy
le { pop } { exch pop } ifelse
2 copy
le { pop } { exch pop } ifelse
dup dup dup
6 1 roll
4 1 roll
7 1 roll
sub
6 1 roll
sub
5 1 roll
sub
4 1 roll
} bind def
/CMYKtoRGB {
dup dup 4 -1 roll add
5 1 roll 3 -1 roll add
4 1 roll add
1 exch sub dup 0 lt {pop 0} if 3 1 roll
1 exch sub dup 0 lt {pop 0} if exch
1 exch sub dup 0 lt {pop 0} if exch
} bind def
/FrameSepInit {
1.0 RealSetgray
} bind def
/FrameSetSepColor {
/FrameSepBlue exch def
/FrameSepGreen exch def
/FrameSepRed exch def
/FrameSepBlack exch def
/FrameSepYellow exch def
/FrameSepMagenta exch def
/FrameSepCyan exch def
/FrameSepIs FMcustom def
setCurrentScreen
} bind def
/FrameSetCyan {
/FrameSepBlue 1.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 1.0 def
/FrameSepIs FMcyan def
setCurrentScreen
} bind def

/FrameSetMagenta {
/FrameSepBlue 1.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 1.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMmagenta def
setCurrentScreen
} bind def

/FrameSetYellow {
/FrameSepBlue 0.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 1.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMyellow def
setCurrentScreen
} bind def

/FrameSetBlack {
/FrameSepBlue 0.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 1.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMblack def
setCurrentScreen
} bind def

/FrameNoSep {
/FrameSepIs FMnone def
setCurrentScreen
} bind def
/FrameSetSepColors {
FrameDict begin
[ exch 1 add 1 roll ]
/FrameSepColors
exch def end
} bind def
/FrameColorInSepListCMYK {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsCMYK
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/FrameColorInSepListRGB {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsRGB
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/RealSetgray /setgray load def
/RealSetrgbcolor /setrgbcolor load def
/RealSethsbcolor /sethsbcolor load def
end
/setgray {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetgray }
{
FrameSepIs FMblack eq
{ RealSetgray }
{ FrameSepIs FMcustom eq
FrameSepRed 0 eq and
FrameSepGreen 0 eq and
FrameSepBlue 0 eq and {
RealSetgray
} {
1 RealSetgray pop
} ifelse
} ifelse
} ifelse
end
} bind def
/setrgbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetrgbcolor }
{
3 copy [ 4 1 roll ]
FrameColorInSepListRGB
{
FrameSepBlue eq exch
FrameSepGreen eq and exch
FrameSepRed eq and
{ 0 } { 1 } ifelse
}
{
FMPColor {
RealSetrgbcolor
currentcmykcolor
} {
RGBtoCMYK
} ifelse
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
RealSetgray
}
ifelse
end
} bind def
/sethsbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSethsbcolor }
{
RealSethsbcolor
currentrgbcolor
setrgbcolor
}
ifelse
end
} bind def
FrameDict begin
/setcmykcolor where {
pop /RealSetcmykcolor /setcmykcolor load def
} {
/RealSetcmykcolor {
4 1 roll
3 { 3 index add 0 max 1 min 1 exch sub 3 1 roll} repeat
setrgbcolor pop
} bind def
} ifelse
userdict /setcmykcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetcmykcolor }
{
4 copy [ 5 1 roll ]
FrameColorInSepListCMYK
{
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
{ 0 } { 1 } ifelse
}
{
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
RealSetgray
}
ifelse
end
} bind put
FMLevel1 not {

/patProcDict 5 dict dup begin
<0f1e3c78f0e1c387> { 3 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<0f87c3e1f0783c1e> { 3 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
<8142241818244281> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-1 -1 moveto 9 9 lineto stroke } bind def
<03060c183060c081> { 1 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<8040201008040201> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
end def
/patDict 15 dict dup begin
/PatternType 1 def
/PaintType 2 def
/TilingType 3 def
/BBox [ 0 0 8 8 ] def
/XStep 8 def
/YStep 8 def
/PaintProc {
begin
patProcDict bstring known {
patProcDict bstring get exec
} {
8 8 true [1 0 0 -1 0 8] bstring imagemask
} ifelse
end
} bind def
end def
} if
/combineColor {
FrameSepIs FMnone eq
{
graymode FMLevel1 or not {

[/Pattern [/DeviceCMYK]] setcolorspace
FrameCurColors 0 4 getinterval aload pop FrameCurPat setcolor
} {
FrameCurColors 3 get 1.0 ge {
FrameCurGray RealSetgray
} {
FMPColor graymode and {
0 1 3 {
FrameCurColors exch get
1 FrameCurGray sub mul
} for
RealSetcmykcolor
} {
4 1 6 {
FrameCurColors exch get
graymode {
1 exch sub 1 FrameCurGray sub mul 1 exch sub
} {
1.0 lt {FrameCurGray} {1} ifelse
} ifelse
} for
RealSetrgbcolor
} ifelse
} ifelse
} ifelse
} {
FrameCurColors 0 4 getinterval aload
FrameColorInSepListCMYK {
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
FrameSepIs FMcustom eq and
{ FrameCurGray } { 1 } ifelse
} {
FrameSepIs FMblack eq
{FrameCurGray 1.0 exch sub mul 1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop FrameCurGray 1.0 exch sub mul 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
graymode FMLevel1 or not {

[/Pattern [/DeviceGray]] setcolorspace
FrameCurPat setcolor
} {
graymode not FMLevel1 and {

dup 1 lt {pop FrameCurGray} if
} if
RealSetgray
} ifelse
} ifelse
} bind def
/savematrix {
orgmatrix currentmatrix pop
} bind def
/restorematrix {
orgmatrix setmatrix
} bind def
/dmatrix matrix def
/dpi 72 0 dmatrix defaultmatrix dtransform
dup mul exch dup mul add sqrt def

/freq dpi dup 72 div round dup 0 eq {pop 1} if 8 mul div def
/sangle 1 0 dmatrix defaultmatrix dtransform exch atan def
/dpiranges [ 2540 2400 1693 1270 1200 635 600 0 ] def
/CMLowFreqs [ 100.402 94.8683 89.2289 100.402 94.8683 66.9349 63.2456 47.4342 ] def
/YLowFreqs [ 95.25 90.0 84.65 95.25 90.0 70.5556 66.6667 50.0 ] def
/KLowFreqs [ 89.8026 84.8528 79.8088 89.8026 84.8528 74.8355 70.7107 53.033 ] def
/CLowAngles [ 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 ] def
/MLowAngles [ 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 ] def
/YLowTDot [ true true false true true false false false ] def
/CMHighFreqs [ 133.87 126.491 133.843 108.503 102.523 100.402 94.8683 63.2456 ] def
/YHighFreqs [ 127.0 120.0 126.975 115.455 109.091 95.25 90.0 60.0 ] def
/KHighFreqs [ 119.737 113.137 119.713 128.289 121.218 89.8026 84.8528 63.6395 ] def
/CHighAngles [ 71.5651 71.5651 71.5651 70.0169 70.0169 71.5651 71.5651 71.5651 ] def
/MHighAngles [ 18.4349 18.4349 18.4349 19.9831 19.9831 18.4349 18.4349 18.4349 ] def
/YHighTDot [ false false true false false true true false ] def
/PatFreq [ 10.5833 10.0 9.4055 10.5833 10.0 10.5833 10.0 9.375 ] def
/screenIndex {
0 1 dpiranges length 1 sub { dup dpiranges exch get 1 sub dpi le {exit} {pop} ifelse } for
} bind def
/getCyanScreen {
FMUseHighFrequencyScreens { CHighAngles CMHighFreqs} {CLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getMagentaScreen {
FMUseHighFrequencyScreens { MHighAngles CMHighFreqs } {MLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getYellowScreen {
FMUseHighFrequencyScreens { YHighTDot YHighFreqs} { YLowTDot YLowFreqs } ifelse
screenIndex dup 3 1 roll get 3 1 roll get { 3 div
{2 { 1 add 2 div 3 mul dup floor sub 2 mul 1 sub exch} repeat
FMSpotFunction } } {/FMSpotFunction load } ifelse
0.0 exch
} bind def
/getBlackScreen {
FMUseHighFrequencyScreens { KHighFreqs } { KLowFreqs } ifelse
screenIndex get 45.0 /FMSpotFunction load
} bind def
/getSpotScreen {
getBlackScreen
} bind def
/getCompositeScreen {
getBlackScreen
} bind def
/FMSetScreen
FMLevel1 { /setscreen load
}{ {
8 dict begin
/HalftoneType 1 def
/SpotFunction exch def
/Angle exch def
/Frequency exch def
/AccurateScreens FMUseAcccurateScreens def
currentdict end sethalftone
} bind } ifelse
def
/setDefaultScreen {
FMPColor {
orgrxfer cvx orggxfer cvx orgbxfer cvx orgxfer cvx setcolortransfer
}
{
orgxfer cvx settransfer
} ifelse
orgfreq organgle orgproc cvx setscreen
} bind def
/setCurrentScreen {
FrameSepIs FMnone eq {
FMUseDefaultNoSeparationScreen {
setDefaultScreen
} {
getCompositeScreen FMSetScreen
} ifelse
} {
FrameSepIs FMcustom eq {
FMUseDefaultSpotSeparationScreen {
setDefaultScreen
} {
getSpotScreen FMSetScreen
} ifelse
} {
FMUseDefaultProcessSeparationScreen {
setDefaultScreen
} {
FrameSepIs FMcyan eq {
getCyanScreen FMSetScreen
} {
FrameSepIs FMmagenta eq {
getMagentaScreen FMSetScreen
} {
FrameSepIs FMyellow eq {
getYellowScreen FMSetScreen
} {
getBlackScreen FMSetScreen
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} bind def
end
/gstring FMLOCAL
/gfile FMLOCAL
/gindex FMLOCAL
/orgrxfer FMLOCAL
/orggxfer FMLOCAL
/orgbxfer FMLOCAL
/orgxfer FMLOCAL
/orgproc FMLOCAL
/orgrproc FMLOCAL
/orggproc FMLOCAL
/orgbproc FMLOCAL
/organgle FMLOCAL
/orgrangle FMLOCAL
/orggangle FMLOCAL
/orgbangle FMLOCAL
/orgfreq FMLOCAL
/orgrfreq FMLOCAL
/orggfreq FMLOCAL
/orgbfreq FMLOCAL
/yscale FMLOCAL
/xscale FMLOCAL
/edown FMLOCAL
/manualfeed FMLOCAL
/paperheight FMLOCAL
/paperwidth FMLOCAL
/FMDOCUMENT {
array /FMfonts exch def
/#copies exch def
FrameDict begin
0 ne /manualfeed exch def
/paperheight exch def
/paperwidth exch def
0 ne /FrameNegative exch def
0 ne /edown exch def
/yscale exch def
/xscale exch def
FMLevel1 {
manualfeed {setmanualfeed} if
/FMdicttop countdictstack 1 add def
/FMoptop count def
% setpapername
% manualfeed {true} {papersize} ifelse
% {manualpapersize} {false} ifelse
% {desperatepapersize} {false} ifelse
% { (Can't select requested paper size for Frame print job!) FMFAILURE } if
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
}
{{1 dict dup /PageSize [paperwidth paperheight]put setpagedevice}stopped
{ (Can't select requested paper size for Frame print job!) FMFAILURE } if
{1 dict dup /ManualFeed manualfeed put setpagedevice } stopped pop }
ifelse

FMPColor {
currentcolorscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def
cvlit /orgbproc exch def
/orgbangle exch def
/orgbfreq exch def
cvlit /orggproc exch def
/orggangle exch def
/orggfreq exch def
cvlit /orgrproc exch def
/orgrangle exch def
/orgrfreq exch def
currentcolortransfer
FrameNegative {
1 1 4 {
pop { 1 exch sub } concatprocs 4 1 roll
} for
4 copy
setcolortransfer
} if
cvlit /orgxfer exch def
cvlit /orgbxfer exch def
cvlit /orggxfer exch def
cvlit /orgrxfer exch def
} {
currentscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def

currenttransfer
FrameNegative {
{ 1 exch sub } concatprocs
dup settransfer
} if
cvlit /orgxfer exch def
} ifelse
end
} def
/pagesave FMLOCAL
/orgmatrix FMLOCAL
/landscape FMLOCAL
/pwid FMLOCAL
/FMBEGINPAGE {
FrameDict begin
/pagesave save def
3.86 setmiterlimit
/landscape exch 0 ne def
landscape {
90 rotate 0 exch dup /pwid exch def neg translate pop
}{
pop /pwid exch def
} ifelse
edown { [-1 0 0 1 pwid 0] concat } if
0 0 moveto paperwidth 0 lineto paperwidth paperheight lineto
0 paperheight lineto 0 0 lineto 1 setgray fill
xscale yscale scale
/orgmatrix matrix def
gsave
} def
/FMENDPAGE {
grestore
pagesave restore
end
showpage
} def
/FMFONTDEFINE {
FrameDict begin
findfont
ReEncode
1 index exch
definefont
FMfonts 3 1 roll
put
end
} def
/FMFILLS {
FrameDict begin dup
array /fillvals exch def
dict /patCache exch def
end
} def
/FMFILL {
FrameDict begin
fillvals 3 1 roll put
end
} def
/FMNORMALIZEGRAPHICS {
newpath
0.0 0.0 moveto
1 setlinewidth
0 setlinecap
0 0 0 sethsbcolor
0 setgray
} bind def
/fx FMLOCAL
/fy FMLOCAL
/fh FMLOCAL
/fw FMLOCAL
/llx FMLOCAL
/lly FMLOCAL
/urx FMLOCAL
/ury FMLOCAL
/FMBEGINEPSF {
end
/FMEPSF save def
/showpage {} def
% See Adobe's "PostScript Language Reference Manual, 2nd Edition", page 714.
% "...the following operators MUST NOT be used in an EPS file:" (emphasis ours)
/banddevice {(banddevice) FMBADEPSF} def
/clear {(clear) FMBADEPSF} def
/cleardictstack {(cleardictstack) FMBADEPSF} def
/copypage {(copypage) FMBADEPSF} def
/erasepage {(erasepage) FMBADEPSF} def
/exitserver {(exitserver) FMBADEPSF} def
/framedevice {(framedevice) FMBADEPSF} def
/grestoreall {(grestoreall) FMBADEPSF} def
/initclip {(initclip) FMBADEPSF} def
/initgraphics {(initgraphics) FMBADEPSF} def
/initmatrix {(initmatrix) FMBADEPSF} def
/quit {(quit) FMBADEPSF} def
/renderbands {(renderbands) FMBADEPSF} def
/setglobal {(setglobal) FMBADEPSF} def
/setpagedevice {(setpagedevice) FMBADEPSF} def
/setshared {(setshared) FMBADEPSF} def
/startjob {(startjob) FMBADEPSF} def
/lettertray {(lettertray) FMBADEPSF} def
/letter {(letter) FMBADEPSF} def
/lettersmall {(lettersmall) FMBADEPSF} def
/11x17tray {(11x17tray) FMBADEPSF} def
/11x17 {(11x17) FMBADEPSF} def
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FMPColor

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savematrix
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GGstrk
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bs 0 len getinterval im pos len getinterval copy pop
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cf exch readhexstring pop pop
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} bind def
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} bind def
/BEGINBITMAP2BITc {
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} bind def
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3 index 2 div add exch
4 index 2 div add exch
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1 index 2 div neg
1 index 2 div neg
translate
scale
/h exch def /w exch def
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sl lb lt {lb ms} if
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r
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ws 0 lb getinterval is copy pop
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w h d [w 0 0 h neg 0 h]
{ip} image
bitmapsave restore
grestore
} bind def
/BEGINBITMAPBW {
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} bind def
/BEGINBITMAPGRAY {
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} bind def
/BEGINBITMAP2BIT {
2 {} COMMONBITMAP
} bind def
/COMMONBITMAP {
/r exch def
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gsave

3 index 2 div add exch
4 index 2 div add exch
translate
rotate
1 index 2 div neg
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translate
scale
/h exch def /w exch def
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r
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w h d [w 0 0 h neg 0 h]
{cf is readhexstring pop} image
bitmapsave restore
grestore
} bind def
/ngrayt 256 array def
/nredt 256 array def
/nbluet 256 array def
/ngreent 256 array def
/gryt FMLOCAL
/blut FMLOCAL
/grnt FMLOCAL
/redt FMLOCAL
/indx FMLOCAL
/cynu FMLOCAL
/magu FMLOCAL
/yelu FMLOCAL
/k FMLOCAL
/u FMLOCAL
FMLevel1 {
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currentcolortransfer
/gryt exch def
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0 1 255 {
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/cynu 1 red indx get 255 div sub def
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/k cynu magu min yelu min def
/u k currentundercolorremoval exec def
% /u 0 def
nredt indx 1 0 cynu u sub max sub redt exec put
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nbluet indx 1 0 yelu u sub max sub blut exec put
ngrayt indx 1 k currentblackgeneration exec sub gryt exec put
} for
{255 mul cvi nredt exch get}
{255 mul cvi ngreent exch get}
{255 mul cvi nbluet exch get}
{255 mul cvi ngrayt exch get}
setcolortransfer
{pop 0} setundercolorremoval
{} setblackgeneration
} bind def
}
{
/colorSetup2 {
[ /Indexed /DeviceRGB 255
{dup red exch get 255 div
exch dup green exch get 255 div
exch blue exch get 255 div}
] setcolorspace
} bind def
} ifelse
/tran FMLOCAL
/fakecolorsetup {
/tran 256 string def
0 1 255 {/indx exch def
tran indx
red indx get 77 mul
green indx get 151 mul
blue indx get 28 mul
add add 256 idiv put} for
currenttransfer
{255 mul cvi tran exch get 255.0 div}
exch concatprocs settransfer
} bind def
/BITMAPCOLOR {
/d 8 def
gsave

3 index 2 div add exch
4 index 2 div add exch
translate
rotate
1 index 2 div neg
1 index 2 div neg
translate
scale
/h exch def /w exch def
/bitmapsave save def
FMLevel1 {
colorsetup
/is w d wbytes string def
/cf currentfile def
w h d [w 0 0 h neg 0 h]
{cf is readhexstring pop} {is} {is} true 3 colorimage
} {
colorSetup2
/is w d wbytes string def
/cf currentfile def
7 dict dup begin
/ImageType 1 def
/Width w def
/Height h def
/ImageMatrix [w 0 0 h neg 0 h] def
/DataSource {cf is readhexstring pop} bind def
/BitsPerComponent d def
/Decode [0 255] def
end image
} ifelse
bitmapsave restore
grestore
} bind def
/BITMAPCOLORc {
/d 8 def
gsave

3 index 2 div add exch
4 index 2 div add exch
translate
rotate
1 index 2 div neg
1 index 2 div neg
translate
scale
/h exch def /w exch def
/lb w d wbytes def
sl lb lt {lb ms} if
/bitmapsave save def
FMLevel1 {
colorsetup
/is im 0 lb getinterval def
ws 0 lb getinterval is copy pop
/cf currentfile def
w h d [w 0 0 h neg 0 h]
{ip} {is} {is} true 3 colorimage
} {
colorSetup2
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ws 0 lb getinterval is copy pop
/cf currentfile def
7 dict dup begin
/ImageType 1 def
/Width w def
/Height h def
/ImageMatrix [w 0 0 h neg 0 h] def
/DataSource {ip} bind def
/BitsPerComponent d def
/Decode [0 255] def
end image
} ifelse
bitmapsave restore
grestore
} bind def
/BITMAPTRUECOLORc {
/d 24 def
gsave

3 index 2 div add exch
4 index 2 div add exch
translate
rotate
1 index 2 div neg
1 index 2 div neg
translate
scale
/h exch def /w exch def
/lb w d wbytes def
sl lb lt {lb ms} if
/bitmapsave save def

/is im 0 lb getinterval def
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ws 0 lb getinterval is copy pop
/cf currentfile def
w h 8 [w 0 0 h neg 0 h]
{w rip pop ris} {gis} {bis} true 3 colorimage
bitmapsave restore
grestore
} bind def
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(GHRS Instrument Handbook 5.0) 207 60.29 T
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-2.78 (1) 552.44 60.29 P
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1.2 (Chapter 2) 72 677 S
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-0.48 (Instrument Summary \321) 207 677 S
-0.48 (Why Use the GHRS?) 207 647 S
3 12 Q
(2.1) 144 424 T
( Fundamental properties of the instrument) 164.02 424 T
4 F
( 12) 505.32 424 T
3 10 Q
(2.1.1) 162 407.33 T
( Entrance Apertures) 187.02 407.33 T
4 F
( 12) 508.1 407.33 T
3 F
(2.1.2) 162 391.33 T
( Useful W) 187.02 391.33 T
(avelength Range) 229.99 391.33 T
4 F
( 12) 508.1 391.33 T
3 F
(2.1.3) 162 375.33 T
( A) 187.02 375.33 T
(vailable Resolving Powers) 196.29 375.33 T
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( 12) 508.1 375.33 T
3 F
(2.1.4) 162 359.33 T
( Photometric Precision and Accuracy) 187.02 359.33 T
4 F
( 13) 508.1 359.33 T
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(2.1.5) 162 343.33 T
( T) 187.02 343.33 T
(ime Resolution) 195.54 343.33 T
4 F
( 13) 508.1 343.33 T
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(2.1.6) 162 327.33 T
( Operational Complexity) 187.02 327.33 T
4 F
( 13) 508.1 327.33 T
3 12 Q
(2.2) 144 310 T
( A Brief Description of the Instrument and Its Operation) 164.02 310 T
4 F
( 13) 505.32 310 T
3 F
(2.3) 144 292 T
( A Little About How HST and GHRS W) 164.02 292 T
(ork) 369.2 292 T
4 F
( 15) 505.32 292 T
3 F
(2.4) 144 274 T
( GHRS Modes of Operation) 164.02 274 T
4 F
( 17) 505.32 274 T
3 10 Q
(2.4.1) 162 257.33 T
( T) 187.02 257.33 T
(arget Acquisition Mode) 194.8 257.33 T
4 F
( 17) 508.1 257.33 T
3 F
(2.4.2) 162 241.33 T
( Science Data Acquisition Modes) 187.02 241.33 T
4 F
( 19) 508.1 241.33 T
FMENDPAGE
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(Instrument Summary \321 Why Use the GHRS?) 189 736.18 T
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(12) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
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0.37 (The Goddard High Resolution Spectrograph was built to obtain high-quality spectra of) 189 679.35 P
1.38 (astronomical sources ef) 189 667.35 P
1.38 (\336ciently) 286.01 667.35 P
1.38 (. The GHRS can also record images of the objects it) 318.14 667.35 P
1.66 (observes, but that is mostly as an adjunct to its spectroscopic properties to con\336rm) 189 655.35 P
(pointing.) 189 643.35 T
54 600.02 540 603.02 C
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54 601.52 180 601.52 2 L
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(2.1) 163.32 607.02 T
(Fundamental properties of the instrument) 189 607.02 T
5 10 Q
0.78 (Here we provide a brief overview of the basic properties of the GHRS. Each of these) 189 583.35 P
-0.12 (aspects is described in more detail in the next two chapters. Chapters 6, 7, and 8 provide) 189 571.35 P
(illustrations of the GHRS and tables of instrument parameters.) 189 559.35 T
0 F
(2.1.1) 157.76 529.35 T
(Entrance Apertures) 189 529.35 T
5 F
1.18 (The source to be observed may be centered in a) 189 509.35 P
1.18 (Lar) 393.51 509.35 P
1.18 (ge Science Aperture \050LSA\051 or a) 407.21 509.35 P
1.16 (Small Science Aperture \050SSA\051) 189 497.35 P
5 8 Q
0.93 (1) 314.96 501.35 P
5 10 Q
1.16 (. Because of the installation of COST) 318.96 497.35 P
1.16 (AR, the LSA is) 474.85 497.35 P
1.09 (1.74 arcsec square and the SSA is 0.22 arcsec square, although they retain their pre-) 189 485.35 P
-0.1 (COST) 189 473.35 P
-0.1 (AR names \050) 213.76 473.35 P
6 F
-0.25 (2.0) 261.32 473.35 P
5 F
-0.1 ( and) 279.32 473.35 P
6 F
-0.25 (0.25) 298.55 473.35 P
5 F
-0.1 (, respectively\051. The high-quality images that COST) 322.55 473.35 P
-0.1 (AR) 526.11 473.35 P
0.5 (produces mean that spectra with good spectroscopic resolution result when the LSA is) 189 461.35 P
0.42 (used. The SSA has about 50 to 70% of the throughput of the LSA; using the LSA will) 189 449.35 P
1.46 (degrade resolution by 10 to 20% compared to the SSA because of the wings to the) 189 437.35 P
(instrumental pro\336le.) 189 425.35 T
0.03 (The LSA has a shutter which automatically closes when an observation with the SSA is) 189 405.35 P
(being performed, in order to reduce stray light.) 189 393.35 T
0 F
(2.1.2) 157.76 363.35 T
(Useful W) 189 363.35 T
(avelength Range) 231.41 363.35 T
5 F
0.66 (The GHRS can obtain spectra from about 1) 189 343.35 P
0.66 (150 to 3200 \201. These limits are set by the) 366.84 343.35 P
1.02 (magnesium \337uoride coatings on) 189 331.35 P
7 F
1.02 (HST) 323.63 331.35 P
5 F
1.02 (\325) 341.41 331.35 P
1.02 (s optics and by the nature of the detectors. The) 344.19 331.35 P
3.84 (additional two re\337ections introduced by COST) 189 319.35 P
3.84 (AR\325) 394.88 319.35 P
3.84 (s mirrors signi\336cantly reduce) 411.55 319.35 P
1.25 (throughput at the very shortest wavelengths \050i.e., below L) 189 307.35 P
1.25 (yman-) 429.26 307.35 P
8 F
1.25 (a) 454.81 307.35 P
5 F
1.25 (\051 so that even very) 461.12 307.35 P
-0.22 (bright stars \050e.g.,) 189 295.35 P
8 F
-0.22 (m) 258.34 295.35 P
5 F
-0.22 (Col\051 have failed to produce detectable \337ux below 1) 266.6 295.35 P
-0.22 (150 \201. It is possi-) 469.47 295.35 P
(ble to observe bright stars out to 3400 \201.) 189 283.35 T
0 F
(2.1.3) 157.76 253.35 T
(A) 189 253.35 T
(vailable Resolving Powers) 195.85 253.35 T
5 F
0.14 (W) 189 233.35 P
0.14 (ith Side 1, observations may be made) 198.04 233.35 P
0.14 (from 1) 351.23 233.35 P
0.14 (150 to 1800 \201 at) 377.94 233.35 P
9 F
0.12 (R) 448.36 233.35 P
5 F
0.14 ( = 2,000, 25,000, and) 454.36 233.35 P
-0.2 (80,000 \050gratings G140L, G140M, and Ech-A, respectively\051. W) 189 221.35 P
-0.2 (ith Side 2, the options are) 438.8 221.35 P
9 F
0.29 (R) 189 209.35 P
5 F
0.33 ( = 25,000 from 1) 195 209.35 P
0.33 (150 to 3200 \201 \050G160M, G200M, and G270M\051 and) 263.55 209.35 P
9 F
0.29 (R) 472.92 209.35 P
5 F
0.33 ( = 80,000 from) 478.92 209.35 P
0.29 (1680 to 3400 \201 \050Ech-B\051. For certain applications it can be advantageous to use grating) 189 197.35 P
(G270M to wavelengths as low as 2100 \201 because of its high ef) 189 185.35 T
(\336ciency) 441.56 185.35 T
(.) 472.57 185.35 T
54 130.98 540 160.98 C
0 0 0 1 0 0 0 K
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189 138.98 333 138.98 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
0 0 612 792 C
5 9 Q
0 X
0 0 0 1 0 0 0 K
(1. W) 189 124.98 T
(e will use \322LSA\323 and \322SSA\323 to denote the two science apertures of the GHRS in this docu-) 208.03 124.98 T
-0.13 (ment in order to lessen ambiguity about their apparent size. Note that the of) 189 114.98 P
-0.13 (\336cial nomenclature of) 459.15 114.98 P
(\322) 189 104.98 T
6 F
(2.0) 193 104.98 T
5 F
(\323 and \322) 209.2 104.98 T
6 F
(0.25) 234.68 104.98 T
5 F
(\323 does not change despite the fact that these two apertures are now 1.74 and) 256.28 104.98 T
(0.22 arcsec square respectively) 189 94.98 T
(.) 300.38 94.98 T
FMENDPAGE
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(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (13) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
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72 726.98 558 726.98 2 L
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72 726.98 558 726.98 2 L
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0 9 Q
(Instrument Summary \321 Why Use the GHRS?) 207 736.18 T
0 10 Q
(2.1.4) 175.76 679.35 T
(Photometric Precision and Accuracy) 207 679.35 T
5 F
-0.23 (Routine calibrations on standard stars provide \337ux-calibrated spectra that are accurate to) 207 659.35 P
0.76 (10%) 207 647.35 P
5 8 Q
0.61 (1) 225.33 651.35 P
5 10 Q
0.76 (. Relative \337uxes obtained at dif) 229.33 647.35 P
0.76 (ferent wavelengths should be good to better than) 357.96 647.35 P
0.07 (5%. The repeatability of \337uxes is even better) 207 635.35 P
0.07 (, being better than 1%; i.e., it is possible to) 386.52 635.35 P
0.41 (compare measures of the same wavelength in the same star at dif) 207 623.35 P
0.41 (ferent times to within) 470.95 623.35 P
(1% for observations with the LSA.) 207 611.35 T
1.47 (W) 207 591.35 P
1.47 (ithin a single bandpass \050i.e., one grating setting\051, relative photometric precision is) 216.04 591.35 P
0.75 (limited by photon statistics for S/N < 30 and by detector non-uniformities above that,) 207 579.35 P
1.02 (provided that the detectors are being used within the linear portion of their response.) 207 567.35 P
0.52 (W) 207 555.35 P
0.52 (ith suitable observing strategies, it is possible to achieve relative S/N as high as 900) 216.04 555.35 P
(\050Lambert et al. 1994\051) 207 543.35 T
5 8 Q
(2) 291.98 547.35 T
5 10 Q
(.) 295.98 543.35 T
0.13 (W) 207 523.35 P
0.13 (e have found that the photometric sensitivity of the GHRS has not changed with time) 215.64 523.35 P
(to within 1% or less.) 207 511.35 T
0 F
(2.1.5) 175.76 481.35 T
(T) 207 481.35 T
(ime Resolution) 212.93 481.35 T
5 F
0.59 (Most observers use the GHRS to accumulate photons for the time needed to reach the) 207 461.35 P
0.59 (signal-to-noise they desire. In) 207 449.35 P
6 F
1.42 (ACCUM) 330.74 449.35 P
5 F
0.59 ( mode the exposures may be as short as 0.2 sec-) 360.74 449.35 P
0.65 (onds, although use of standard procedures for improving S/N usually limits exposures) 207 437.35 P
-0 (to no shorter than about 15 seconds. The GHRS has a rapid readout mode \050) 207 425.35 P
6 F
-0.01 (RAPID) 507.17 425.35 P
5 F
-0 (\051 that) 537.17 425.35 P
0.05 (can obtain spectra as often as every 50 milliseconds, but that can only be done by sacri-) 207 413.35 P
(\336cing many features that are important for producing high-quality spectra.) 207 401.35 T
0 F
(2.1.6) 175.76 371.35 T
(Operational Complexity) 207 371.35 T
5 F
-0.24 (The limited availability of memory on the) 207 351.35 P
7 F
-0.24 (HST) 375.58 351.35 P
5 F
-0.24 ( spacecraft means that there exists a max-) 393.36 351.35 P
0.61 (imum number of operating commands that can be in place for a single set of observa-) 207 339.35 P
2.64 (tions. That can be a limit for use of the GHRS in certain cases, described later) 207 327.35 P
(\050Section) 207 315.35 T
(4.6 on page) 242.83 315.35 T
(47\051.) 291.71 315.35 T
72 272.02 558 275.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 273.52 558 273.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 273.52 198 273.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(2.2) 181.32 279.02 T
(A Brief Description of the Instrument and Its Operation) 207 279.02 T
5 10 Q
0.73 (The GHRS has the usual components of an astronomical spectrograph: entrance aper-) 207 255.35 P
1.21 (tures, a collimator) 207 243.35 P
1.21 (, dispersers, camera mirrors, and detectors. There are also a wave-) 281.52 243.35 P
0.04 (length calibration lamp, \337at \336eld lamps, and mirrors to acquire and center objects in the) 207 231.35 P
0.69 (observing apertures. The apertures were described above in basic terms, and are illus-) 207 219.35 P
0.58 (trated in Section) 207 207.35 P
0.58 (6.1 on page) 276.2 207.35 P
0.58 (56. The collimator and camera mirrors are unexceptional) 326.24 207.35 P
-0.19 (and need no further description here \050see Section) 207 195.35 P
-0.19 (6.2 on page) 403.92 195.35 P
-0.19 (60 for details\051. The impor-) 452.41 195.35 P
(tant elements are the dispersers and the detectors.) 207 183.35 T
72 133.98 558 163.98 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 141.98 351 141.98 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
0 0 612 792 C
5 9 Q
0 X
0 0 0 1 0 0 0 K
(1. Starting in Cycle 4, the routine \337uxes delivered by the pipeline data reduction system are no) 207 127.98 T
-0.19 (longer on the) 207 117.98 P
7 F
-0.19 (IUE) 256.17 117.98 P
5 F
-0.19 ( system but instead have been adjusted to conform to models of the white dwarf) 271.16 117.98 P
(G191B2B. This can produce systematic dif) 207 107.98 T
(ferences when comparing observations.) 362.32 107.98 T
(2. References are listed in Chapter 9.) 207 94.98 T
FMENDPAGE
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54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Instrument Summary \321 Why Use the GHRS?) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(14) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
5 F
0.3 (The dispersers are mounted on a rotating carrousel, together with several plane mirrors) 189 679.35 P
-0.18 (used for acquisition. The \336rst-order gratings are designated as G140L, G140M, G160M,) 189 667.35 P
1.36 (G200M, and G270M, where \322G\323 indicates a grating, the number indicates the blaze) 189 655.35 P
0.07 (wavelength \050in nm\051, and the \322L\323 or \322M\323 suf) 189 643.35 P
0.07 (\336x denotes a \322low\323 or \322medium\323 resolution) 365.16 643.35 P
0.03 (grating, respectively) 189 631.35 P
0.03 (. The GHRS medium resolution \336rst-order gratings are holographic) 270.03 631.35 P
0.15 (in order to achieve very high ef) 189 619.35 P
0.15 (\336ciency within a limited wavelength region. G140L is a) 315.23 619.35 P
0.57 (ruled grating. The \336rst two \336rst-order gratings, G140L and G140M, have their spectra) 189 607.35 P
0.68 (imaged by mirror Cam-A onto detector D1, which is optimized for the shortest wave-) 189 595.35 P
0.02 (lengths. The other three gratings have their spectra imaged by Cam-B onto detector D2,) 189 583.35 P
0.51 (which works best at wavelengths from about 1700 to 3200 \201, but which is also useful) 189 571.35 P
(down to 1200 \201.) 189 559.35 T
1.28 (The carrousel also has an echelle grating. The higher orders are designated as mode) 189 539.35 P
0.36 (Ech-A, and they are imaged onto D1 by the cross-disperser CD1. The lower orders are) 189 527.35 P
-0.11 (designated as mode Ech-B, and they are directed to D2 by CD2. Finally) 189 515.35 P
-0.11 (, mirrors N1 and) 474.23 515.35 P
0.53 (A1 image the apertures onto detector D1, and mirrors N2 and A2 image onto D2. The) 189 503.35 P
2.36 (\322N\323 mirrors are \322normal,\323 i.e., unattenuated, while the \322A\323 mirrors \050\322attenuated\323\051) 189 491.35 P
0.5 (re\337ect a smaller fraction of the light to the detectors, so as to enable the acquisition of) 189 479.35 P
1.48 (bright stars. \050T) 189 467.35 P
1.48 (o be precise, the mode designated as N1 actually uses the zero-order) 250.43 467.35 P
(image produced by grating G140L.\051) 189 455.35 T
0.31 (Use of the various gratings or mirrors in concert with the camera mirrors produces one) 189 435.35 P
-0.05 (of three kinds of image at the camera focus: 1\051 an image of the entrance aperture, which) 189 423.35 P
-0.25 (may be mapped to \336nd and center the object of interest; 2\051 a single-order spectrum; or 3\051) 189 411.35 P
(a cross-dispersed, two-dimensional echelle spectrum.) 189 399.35 T
-0.04 (The \337ux in these images is measured by Digicon detectors, and the portion of the image) 189 379.35 P
0.51 (plane that is mapped onto the Digicon is determined by magnetic de\337ection coils. The) 189 367.35 P
0.04 (detectors are the heart of the GHRS and they involve subtleties that must be understood) 189 355.35 P
(if the instrument is to be used competently) 189 343.35 T
(.) 358.62 343.35 T
0.9 (First, there are two Digicons: D1 and D2. D1 has a cesium iodide photocathode on a) 189 323.35 P
1.48 (lithium \337uoride window; that makes D1 ef) 189 311.35 P
1.48 (fectively) 368.22 311.35 P
1.48 (\322solar) 407.18 311.35 P
1.48 (-blind,\323 i.e., the enormous) 430.86 311.35 P
0.74 (\337ux of visible-light photons that dominate the spectrum of most stars will produce no) 189 299.35 P
1.49 (signal with this detector) 189 287.35 P
1.49 (, and only far) 288.89 287.35 P
1.49 (-ultraviolet photons \0501) 346.47 287.35 P
1.49 (100 to 1800 \201\051 produce) 438.51 287.35 P
0.15 (electrons that are accelerated by the 23 kV \336eld onto the diodes. D2 has a cesium tellu-) 189 275.35 P
0.35 (ride photocathode on a magnesium \337uoride window) 189 263.35 P
0.35 (. Each Digicon has 512 diodes that) 398.76 263.35 P
0.78 (accumulate counts from accelerated electrons. 500 of those are \322science diodes,\323 plus) 189 251.35 P
(there are \322corner diodes\323 and \322focus diodes\323 \050see Chapter 6\051.) 189 239.35 T
1.71 (Second, both photocathodes have granularity \320 irregularities in response \320 of about) 189 219.35 P
0.39 (0.5% \050rms\051 that can limit the S/N achieved, and there are localized blemishes that pro-) 189 207.35 P
0.02 (duce irregularities of several percent. The Side 1 photocathode also exhibits \322sleeking,\323) 189 195.35 P
-0 (which is slanted, scratch-like features that have an amplitude of 1 to 2% over regions as) 189 183.35 P
2.08 (lar) 189 171.35 P
2.08 (ge as half the faceplate. The ef) 199.37 171.35 P
2.08 (fects of these irregularities could in principle be) 334.11 171.35 P
0.8 (removed by obtaining a \337at \336eld measurement at every position on the photocathode,) 189 159.35 P
0.44 (but that is impractical. Instead, the observing strategy is to rotate the carrousel slightly) 189 147.35 P
-0.01 (between separate exposures and so use dif) 189 135.35 P
-0.01 (ferent portions of the photocathode. This pro-) 357.6 135.35 P
0.85 (cedure is called an) 189 123.35 P
6 F
2.03 (FP-SPLIT) 269.02 123.35 P
5 F
0.85 (, and with it each exposure is divided into two or four) 316.28 123.35 P
-0.18 (separate-but-equal parts, with the carrousel moving the spectrum about 5.2 diode widths) 189 111.35 P
FMENDPAGE
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72 750.02 558 750.02 2 L
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0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (15) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Instrument Summary \321 Why Use the GHRS?) 207 736.18 T
5 10 Q
1.82 (each time in the direction of dispersion. These individual spectra can be combined) 207 679.35 P
(together during the reduction phase.) 207 667.35 T
0.96 (Third, the diodes in the Digicons also have response irregularities, but these are very) 207 647.35 P
-0.05 (slight. The biggest ef) 207 635.35 P
-0.05 (fect is a systematic of) 291.1 635.35 P
-0.05 (fset of about 1% in response of the odd-num-) 377.35 635.35 P
1.56 (bered diodes relative to the even-numbered ones. This ef) 207 623.35 P
1.56 (fect can be almost entirely) 446.22 623.35 P
1.39 (defeated by use of the default) 207 611.35 P
6 F
3.33 (COMB) 335.86 611.35 P
5 F
1.39 ( addition procedure.) 359.86 611.35 P
6 F
3.33 (COMB) 446.78 611.35 P
5 F
1.39 ( addition de\337ects the) 470.78 611.35 P
0.18 (spectrum by an integral number of diodes between subexposures and has the additional) 207 599.35 P
1.38 (bene\336t of working around dead diodes in the instrument that would otherwise leave) 207 587.35 P
(image defects.) 207 575.35 T
0.73 (Fourth, the Digicons\325 diodes are only slightly smaller than the image of the SSA pro-) 207 555.35 P
0.48 (duced by the optics, and are lar) 207 543.35 P
0.48 (ger than the point spread function \050PSF\051 for) 334.41 543.35 P
7 F
0.48 (HST) 515.48 543.35 P
5 F
0.48 (. Thus) 532.52 543.35 P
0.72 (the true resolution of the spectrum cannot be realized unless it is adequately sampled.) 207 531.35 P
0.2 (That is done by making the magnetic \336eld move the spectrum by fractions of the width) 207 519.35 P
1 (of a diode, by either half- or quarter) 207 507.35 P
1 (-diode widths, and then storing those as separate) 357.11 507.35 P
1.19 (spectra in the onboard memory) 207 495.35 P
1.19 (. These are mer) 335.52 495.35 P
1.19 (ged into a single spectrum in the data) 400.54 495.35 P
1.44 (reduction phase. The manner in which this is done is speci\336ed by the) 207 483.35 P
6 F
3.45 (STEP-PATT) 504 483.35 P
5 F
0.81 (parameter) 207 471.35 P
0.81 (, described in more detail later) 246.58 471.35 P
0.81 (. The choice of) 371.7 471.35 P
6 F
1.93 (STEP-PATT) 437.4 471.35 P
5 F
0.81 ( also determines) 491.4 471.35 P
(how the background around the spectrum is measured.) 207 459.35 T
0.79 (Defaults exist for these parameters and they have been set to yield the best quality of) 207 439.35 P
1.68 (spectrum for the con\336guration to which they apply \050except for) 207 427.35 P
6 F
4.02 (FP-SPLIT,) 475.38 427.35 P
5 F
1.68 ( which) 529.38 427.35 P
0.85 (must be invoked explicitly\051. Details on the defaults are provided later \050Section) 207 415.35 P
0.85 (4.3 on) 532.15 415.35 P
0.06 (page) 207 403.35 P
0.06 (43\051, but we strongly encourage you to use the defaults unless there are compelling) 228.38 403.35 P
(reasons not to.) 207 391.35 T
72 348.02 558 351.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 349.52 558 349.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 349.52 198 349.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(2.3) 181.32 355.02 T
(A Little About How) 207 355.02 T
10 F
(HST) 317.66 355.02 T
0 F
( and GHRS W) 341.66 355.02 T
(ork) 418.79 355.02 T
5 10 Q
0.5 (Because of the dif) 207 331.35 P
0.5 (\336culties of working with and communicating with a satellite in low-) 280.8 331.35 P
0.66 (earth orbit, and in order to make) 207 319.35 P
7 F
0.66 (HST) 343.23 319.35 P
5 F
0.66 ( more ef) 361.01 319.35 P
0.66 (\336cient, virtually all actions taken by the) 395.46 319.35 P
0.89 (spacecraft are planned weeks in advance. Only a small fraction of) 207 307.35 P
7 F
0.89 (HST) 482.28 307.35 P
5 F
0.89 (\325) 500.06 307.35 P
0.89 (s time can be) 502.84 307.35 P
0.88 (used for real-time actions that are at the discretion of the observer) 207 295.35 P
0.88 (, and even then the) 479.23 295.35 P
-0.14 (realm of possible actions is very limited, being restricted to deciding which object in the) 207 283.35 P
(\336eld should be centered in the aperture before a subsequent observation is begun.) 207 271.35 T
1.15 (This need for detailed planning of) 207 251.35 P
7 F
1.15 (HST) 352.19 251.35 P
5 F
1.15 ( observations lies at the heart of the apparent) 369.97 251.35 P
0.5 (complexity of the use of the spacecraft and its instruments. At the same time, by care-) 207 239.35 P
0.1 (fully laying out every aspect of what you want done you will \336nd yourself with a better) 207 227.35 P
1.28 (understanding of what actually happens and more con\336dence that the desired results) 207 215.35 P
(will be achieved.) 207 203.35 T
1.45 (All) 207 183.35 P
7 F
1.45 (HST) 223.73 183.35 P
5 F
1.45 ( observations begin with an acquisition. An acquisition can be as simple as) 241.51 183.35 P
3.24 (blindly pointing to particular celestial coordinates, although such a procedure is) 207 171.35 P
1.19 (unlikely to succeed with the GHRS because its entrance apertures are small. For the) 207 159.35 P
-0.08 (GHRS, an acquisition usually means a pointing to precisely speci\336ed coordinates, small) 207 147.35 P
0.08 (motions of the telescope in a spiral pattern to sample the region of sky in the vicinity of) 207 135.35 P
0.07 (the coordinates, and then a peakup motion to center a star in the aperture after on-board) 207 123.35 P
-0.19 (software has determined its location. V) 207 111.35 P
-0.19 (ariations include of) 361.58 111.35 P
-0.19 (fsetting from the acquired star) 438.23 111.35 P
-0.04 (to another nearby object or moving the star to the small aperture. In rare cases it may be) 207 99.35 P
FMENDPAGE
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54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Instrument Summary \321 Why Use the GHRS?) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(16) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
5 F
1.91 (necessary to perform an interactive acquisition, in which the observer speci\336es the) 189 679.35 P
0.81 (object in real time. An intermediate possibility is to take an image with one of) 189 667.35 P
7 F
0.81 (HST) 515.55 667.35 P
5 F
0.81 (\325) 533.33 667.35 P
0.81 (s) 536.11 667.35 P
0.32 (cameras \050or with the GHRS itself\051 in advance of the spectroscopic observation \050by one) 189 655.35 P
-0.12 (to two months\051 and to then derive precise coordinates from that image \050an early acquisi-) 189 643.35 P
-0.09 (tion\051. For very faint objects, especially those to be observed with Side 1 of the GHRS, it) 189 631.35 P
0.19 (is possible to acquire the object with the Faint Object Spectrograph before moving it to) 189 619.35 P
(the LSA.) 189 607.35 T
-0.14 (Once the star has been properly positioned in the appropriate aperture of the GHRS, sci-) 189 587.35 P
0.23 (ence observations may begin. In some cases you may wish to use) 189 575.35 P
6 F
0.56 (IMAGE) 455.37 575.35 P
5 F
0.23 ( mode, which) 485.37 575.35 P
0.68 (can map the LSA at ultraviolet wavelengths, but in general this part means dispersing) 189 563.35 P
1.71 (the light with one of the gratings and adding up the counts to form a spectrum. A) 189 551.35 P
6 F
2.13 (RAPID) 189 539.35 P
5 F
0.89 ( mode also exists to record spectra that change on very short time scales. The) 219 539.35 P
-0.03 (GHRS has no independent microprocessor and so depends on the spacecraft\325) 189 527.35 P
-0.03 (s computer) 495.87 527.35 P
1.11 (and memory for control of its operations. One implication of that dependence is that) 189 515.35 P
1.22 (there is a maximum number of commands that can be stored at any one time. Since) 189 503.35 P
0.3 (those commands are generally loaded into the spacecraft only a few times per day) 189 491.35 P
0.3 (, that) 519.7 491.35 P
0.23 (limitation restricts the total number of GHRS exposures that may be made in a 24 hour) 189 479.35 P
1.14 (period. At the same time, image motion within the instrument that is induced by the) 189 467.35 P
0.4 (earth\325) 189 455.35 P
0.4 (s magnetic \336eld \050see Section) 211.77 455.35 P
0.4 (8.6.5 on page) 330.3 455.35 P
0.4 (98\051 is best dealt with by making indi-) 387.48 455.35 P
-0.05 (vidual exposures no longer than about 5 minutes, thereby increasing the total number of) 189 443.35 P
0.49 (exposures you need to make to get a science observation. In some cases these require-) 189 431.35 P
1.94 (ments come into con\337ict and compromises must be made to accommodate science) 189 419.35 P
(goals.) 189 407.35 T
(Some other relevant aspects of scheduling) 189 387.35 T
7 F
(HST) 360.08 387.35 T
5 F
( observations are:) 377.86 387.35 T
11 11 Q
(\245) 189 369.35 T
5 10 Q
0.2 (Objects in most regions of the sky \322rise\323 and \322set\323 and will be available for science) 203.4 369.35 P
0.6 (observations for about half of an orbit \050about 45 to 50 minutes\051. Longer exposures) 203.4 357.35 P
-0.16 (get spread over several orbits, with a reacquisition at the beginning of each orbit, but) 203.4 345.35 P
0.32 (this occurs at no practical cost in science terms since the GHRS\325 detectors are pho-) 203.4 333.35 P
0.08 (ton counters. Some objects sometimes fall within) 203.4 321.35 P
7 F
0.08 (HST\325) 403.41 321.35 P
5 F
0.08 (s Continuous V) 423.97 321.35 P
0.08 (iewing Zones) 485.76 321.35 P
-0.17 (\050CVZs\051, which enables them to be observed for long times at high ef) 203.4 309.35 P
-0.17 (\336ciency; see the) 475.9 309.35 P
7 F
(Call for Pr) 203.4 297.35 T
(oposals) 246.93 297.35 T
5 F
( for details on taking advantage of the CVZs.) 277.49 297.35 T
11 11 Q
(\245) 189 282.35 T
5 10 Q
1.32 (The orbit of) 203.4 282.35 P
7 F
1.32 (HST) 257.63 282.35 P
5 F
1.32 ( passes through the South Atlantic Anomaly \050SAA\051, which is a) 275.41 282.35 P
0.81 (region in which the background count rate is very high. At present the scheduling) 203.4 270.35 P
0.69 (software simply stops the counting of photons during times when the spacecraft is) 203.4 258.35 P
(within the SAA.) 203.4 246.35 T
FMENDPAGE
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72 726.98 558 726.98 2 L
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72 74.02 558 74.02 2 L
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0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (17) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Instrument Summary \321 Why Use the GHRS?) 207 736.18 T
72 671.02 558 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 672.52 558 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 672.52 198 672.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(2.4) 181.32 678.02 T
(GHRS Modes of Operation) 207 678.02 T
5 10 Q
0.47 (GHRS has several operational modes for tar) 207 654.35 P
0.47 (get acquisition and obtaining science data.) 386.25 654.35 P
(See also Section) 207 642.35 T
(4.1 on page) 275.05 642.35 T
(35 for more discussion of acquisitions.) 323.93 642.35 T
0 F
(2.4.1) 175.76 612.35 T
(T) 207 612.35 T
(arget Acquisition Mode) 212.37 612.35 T
0 9 Q
(2.4.1.1) 170.48 589.02 T
(Onboard Acquisitions) 207 589.02 T
5 10 Q
0.75 (Most tar) 207 568.35 P
0.75 (gets observed with the GHRS can be automatically acquired with an onboard) 241.18 568.35 P
-0.02 (acquisition \050) 207 556.35 P
6 F
-0.04 (ONBOARD) 256.7 556.35 P
-0.04 (ACQ) 301.18 556.35 P
5 F
-0.02 (\051. An onboard tar) 319.18 556.35 P
-0.02 (get acquisition observation consists of dis-) 387.82 556.35 P
0.36 (tinct phases, which are executed in ascending numerical order) 207 544.35 P
0.36 (. Phases 1 and 2 perform) 457.33 544.35 P
0.32 (initialization and internal calibration functions, and need not concern the observer) 207 532.35 P
0.32 (. The) 537.13 532.35 P
0.46 (third phase is called T) 207 520.35 P
0.46 (ar) 296.45 520.35 P
0.46 (get Search. A series of small angle maneuvers, called a \322spiral) 304.04 520.35 P
1.86 (search,\323 scans an area of the sky centered on the initial position. The \337ux coming) 207 508.35 P
2.04 (through the Lar) 207 496.35 P
2.04 (ge Science Aperture \050LSA\051 is measured at each dwell point in the) 273.11 496.35 P
0.49 (search. If the) 207 484.35 P
6 F
1.17 (BRIGHT=RETURN) 262.88 484.35 P
5 F
0.49 ( option has been chosen \050and it is recommended\051, the) 340.88 484.35 P
2.43 (telescope returns to that dwell point which had the greatest number of counts. If) 207 472.35 P
6 F
1.65 (BRIGHT) 207 460.35 P
5 F
0.69 ( and) 243 460.35 P
6 F
1.65 (FAINT) 263.81 460.35 P
5 F
0.69 ( limits have instead been speci\336ed, the \337ux is compared to these) 293.81 460.35 P
-0.09 (upper and lower limits at each step in the spiral, and if the measured value falls between) 207 448.35 P
0.48 (these limits the tar) 207 436.35 P
0.48 (get is assumed to be within the aperture and the search immediately) 281.88 436.35 P
-0.21 (stops. Y) 207 424.35 P
-0.21 (ou may request that a \336eld map be generated at the \336nal dwell point by means of) 238.57 424.35 P
0.04 (the) 207 412.35 P
6 F
0.09 (MAP) 221.76 412.35 P
5 F
0.04 ( optional parameter) 239.76 412.35 P
0.04 (. Y) 317.04 412.35 P
0.04 (ou should be aware, though, that approximately two min-) 328.29 412.35 P
0.28 (utes is required for each map, and that many pointings may be made during the search.) 207 400.35 P
1.01 (\050If you intend to analyze the maps in real time, the search phase must be done as an) 207 388.35 P
-0.18 (interactive acquisition.\051 If you wish to con\336rm the spacecraft\325) 207 376.35 P
-0.18 (s pointing, we recommend) 452.45 376.35 P
2.65 (obtaining an) 207 364.35 P
6 F
6.35 (IMAGE) 264.51 364.35 P
7 F
2.65 (after) 299.66 364.35 P
5 F
2.65 ( the acquisition instead of using the) 318.55 364.35 P
6 F
6.35 (MAP) 481.23 364.35 P
5 F
2.65 ( option \320 see) 499.23 364.35 P
(Chapter) 207 352.35 T
(4.) 241.16 352.35 T
1.17 (The fourth phase is tar) 207 332.35 P
1.17 (get locate \050) 301.5 332.35 P
6 F
2.82 (ACQ/PEAKUP) 348.28 332.35 P
5 F
1.17 (\051. This process measures the precise) 408.28 332.35 P
0.23 (location of the tar) 207 320.35 P
0.23 (get within the aperture, and requests a small angle maneuver to move) 278.32 320.35 P
-0.14 (it to the center) 207 308.35 P
-0.14 (. The \336eld map of the LSA may be made) 263.51 308.35 P
7 F
-0.14 (befor) 427.87 308.35 P
-0.14 (e) 448.61 308.35 P
5 F
-0.14 ( the centering maneuver is) 453.05 308.35 P
1.74 (performed by specifying) 207 296.35 P
6 F
4.18 (MAP=END-POINT) 313.03 296.35 P
5 F
1.74 (. If done) 390.29 296.35 P
7 F
1.74 (after) 431.61 296.35 P
5 F
1.74 ( the centering \050in) 450.5 296.35 P
6 F
4.18 (IMAGE) 528 296.35 P
5 F
-0.04 (mode\051, the map can be helpful for con\336rming that the object was placed precisely in the) 207 284.35 P
-0.05 (center of the aperture) 207 272.35 P
5 8 Q
-0.04 (1) 292.1 276.35 P
5 10 Q
-0.05 (. The \336nal phase of an acquisition is a \337ux measurement in which) 296.1 272.35 P
0.88 (the \337ux entering the GHRS through the \336nal tar) 207 260.35 P
0.88 (get aperture is measured and inserted) 405 260.35 P
0.09 (into the data. After centering, a second maneuver will automatically translate the object) 207 248.35 P
0.45 (to the SSA if that is the aperture speci\336ed for the observation. An) 207 236.35 P
6 F
1.08 (ACQ/PEAKUP) 477.27 236.35 P
5 F
0.45 ( with) 537.27 236.35 P
(\322) 207 224.35 T
6 F
(0.25) 211.44 224.35 T
5 F
(\323 as the speci\336ed aperture will also center the object in the SSA.) 235.44 224.35 T
72 120.98 558 150.98 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 128.98 351 128.98 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
0 0 612 792 C
5 9 Q
0 X
0 0 0 1 0 0 0 K
-0.07 (1. Please don\325) 207 114.98 P
-0.07 (t get the wrong impression. Getting an image of the aperture to con\336rm pointing is) 259.61 114.98 P
(rarely necessary or useful and we mention it here mostly for completeness. If you are working in) 207 104.98 T
(a crowded \336eld, it might help to know exactly what was in the aperture after the fact.) 207 94.98 T
FMENDPAGE
%%EndPage: "17" 7
%%Page: "18" 8
612 792 0 FMBEGINPAGE
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0 9 Q
(Instrument Summary \321 Why Use the GHRS?) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
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(18) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
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5 F
-0.23 (For some kinds of dif) 189 679.35 P
-0.23 (\336cult tar) 273.99 679.35 P
-0.23 (gets an onboard acquisition may not work. Possible causes) 307.18 679.35 P
(might be:) 189 667.35 T
11 11 Q
(\245) 189 649.35 T
5 10 Q
-0.02 (The error in the coordinates is greater than a few arcsec in either declination or right) 203.4 649.35 P
-0.01 (ascension, so that the tar) 203.4 637.35 P
-0.01 (get lies outside the lar) 301.21 637.35 P
-0.01 (gest area that the GHRS can search in) 388.74 637.35 P
(its onboard procedure.) 203.4 625.35 T
11 11 Q
(\245) 189 610.35 T
5 10 Q
-0.05 (The object is a moving tar) 203.4 610.35 P
-0.05 (get whose coordinates could not be predicted with) 307.67 610.35 P
8 F
-0.05 (\261) 511.52 610.35 P
5 F
-0.05 (5 arc-) 517.01 610.35 P
0.11 (sec accuracy when the proposal was written. Features in the atmosphere of a planet,) 203.4 598.35 P
(and comets are possible examples.) 203.4 586.35 T
11 11 Q
(\245) 189 571.35 T
5 10 Q
(The object has a poorly known or unpredictably variable ultraviolet \337ux.) 203.4 571.35 T
11 11 Q
(\245) 189 556.35 T
5 10 Q
0.48 (The tar) 203.4 556.35 P
0.48 (get has nearby neighbors of similar brightness \320 the onboard search process) 232.3 556.35 P
(could center up on the wrong object.) 203.4 544.35 T
11 11 Q
(\245) 189 529.35 T
5 10 Q
1.55 (The object has a spatial extent greater than two arcsec. The automatic centering) 203.4 529.35 P
1.74 (algorithms may not produce acceptable results on objects comparable in size or) 203.4 517.35 P
(lar) 203.4 505.35 T
(ger than the Lar) 213.77 505.35 T
(ge Science Aperture.) 277.18 505.35 T
11 11 Q
(\245) 189 490.35 T
5 10 Q
-0.24 (The object is too faint to get adequate counts with the maximum permissible integra-) 203.4 490.35 P
(tion time of 12.75 seconds.) 203.4 478.35 T
-0.16 (In many cases these problems can be worked around by using an onboard acquisition on) 189 458.35 P
0.26 (a nearby star and then of) 189 446.35 P
0.26 (fsetting to the object of interest, or) 288.69 446.35 P
0.26 (, perhaps, by using the FOS) 427.88 446.35 P
(to acquire before slewing the tar) 189 434.35 T
(get to the GHRS.) 317.95 434.35 T
0 9 Q
(2.4.1.2) 152.48 411.02 T
(Early and Interactive Acquisitions) 189 411.02 T
5 10 Q
-0.18 (Y) 189 390.35 P
-0.18 (ou may choose to obtain an early acquisition \050) 195.22 390.35 P
6 F
-0.44 (EARLY) 378.18 390.35 P
-0.44 (ACQ) 410.5 390.35 P
5 F
-0.18 (\051 image with WFPC2, FOC,) 428.5 390.35 P
0.75 (or GHRS itself. In some cases an acquisition image would be helpful, but the \336eld of) 189 378.35 P
-0.13 (view of the WFPC2 is not needed. Stationary point sources in crowded but recognizable) 189 366.35 P
-0.18 (\336elds would be examples. The GHRS has its own \322\336eld map\323 capability which will pro-) 189 354.35 P
0.35 (duce an image of the sky as seen through the LSA. Each map is a square array of 16) 189 342.35 P
8 F
0.35 ( \264) 531.66 342.35 P
5 F
-0.02 (16 pixels, covering) 189 330.35 P
-0.02 ( arcsec with 0.1) 315.29 330.35 P
-0.02 (1 arcsec spatial resolution. A single \336eld) 377.63 330.35 P
0.22 (map requires a minimum of two minutes to take the data and send it to the ground, and) 189 318.35 P
0.27 (much longer if each point in a spiral search is mapped or if a) 189 306.35 P
6 F
0.64 (STEP-TIME) 437.7 306.35 P
5 F
0.27 ( longer than) 491.7 306.35 P
-0.04 (the default \0500.2 sec\051 is used. One WFPC2 image requires from three to \336ve minutes, but) 189 294.35 P
0.51 (covers a much lar) 189 282.35 P
0.51 (ger area of the sky) 261.17 282.35 P
0.51 (. As a practical matter) 336.43 282.35 P
0.51 (, if more than one \336eld map) 426.11 282.35 P
0.06 (would be needed, a WFPC2 image may be a more ef) 189 270.35 P
0.06 (\336cient choice. The FOC could also) 400.25 270.35 P
(be an appropriate choice for ultraviolet-bright objects.) 189 258.35 T
1.5 (If an interactive acquisition \050) 189 238.35 P
6 F
3.6 (INT) 310.53 238.35 P
3.6 (ACQ) 332.53 238.35 P
5 F
1.5 (\051 is required, the observer must be present at) 350.53 238.35 P
0.64 (STScI, prepared to inspect the image and identify the tar) 189 226.35 P
0.64 (get in a timely fashion. Real-) 420.68 226.35 P
0.2 (time observations are subject to many constraints and are dif) 189 214.35 P
0.2 (\336cult to schedule \050they are) 433.1 214.35 P
0.36 (occasionally impossible\051. Early acquisition should therefore be chosen in preference to) 189 202.35 P
1.02 (interactive acquisition whenever possible. The) 189 190.35 P
7 F
1.02 (HST) 382.41 190.35 P
5 F
1.02 ( \050Phase I\051 Proposal Forms require) 400.19 190.35 P
(justi\336cation of requests for real-time observation.) 189 178.35 T
267.83 327.18 315.29 338.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 268.32 330.35 T
(.) 273.32 330.35 T
(7) 275.82 330.35 T
(4) 280.82 330.35 T
(1) 296.3 330.35 T
(.) 301.3 330.35 T
(7) 303.8 330.35 T
(4) 308.8 330.35 T
8 F
(\264) 288.31 330.35 T
0 0 612 792 C
FMENDPAGE
%%EndPage: "18" 8
%%Page: "19" 9
612 792 0 FMBEGINPAGE
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72 726.98 558 726.98 2 L
0.25 H
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72 74.02 558 74.02 2 L
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0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (19) 546.88 60.29 P
72 750.02 558 750.02 2 L
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72 726.98 558 726.98 2 L
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72 750.02 558 750.02 2 L
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0 Z
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72 726.98 558 726.98 2 L
0.25 H
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72 74.02 558 74.02 2 L
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0 9 Q
(Instrument Summary \321 Why Use the GHRS?) 207 736.18 T
0 10 Q
(2.4.2) 175.76 679.35 T
(Science Data Acquisition Modes) 207 679.35 T
5 F
1.5 (There are several modes of science data acquisition, including Accumulation Mode,) 207 659.35 P
0.35 (Rapid Readout Mode, and Image Mode. Each of these modes may be used in conjunc-) 207 647.35 P
(tion with any of the optical con\336gurations described earlier) 207 635.35 T
(.) 443.08 635.35 T
12 F
(Accumulation Mode) 207 615.35 T
5 F
1.94 (Accumulation Mode \050) 207 595.35 P
6 F
4.65 (ACCUM) 299.2 595.35 P
5 F
1.94 (\051 is the normal way of obtaining a spectrum with the) 329.2 595.35 P
0.7 (GHRS. The name refers to the fact that data can be accumulated in the onboard com-) 207 583.35 P
0.59 (puter during a long exposure. All of the features of the \337ight software are available in) 207 571.35 P
0.39 (this mode, making it the most powerful, \337exible, and automatic way to use the GHRS.) 207 559.35 P
1.09 (There are two types of bene\336ts which one can expect by using the \337ight software in) 207 547.35 P
(Accumulation Mode.) 207 535.35 T
0.41 (The \336rst is the ability to make long duration observations with ef) 207 515.35 P
0.41 (fective and automatic) 471.08 515.35 P
0.29 (control of the process. The time varying Doppler shift caused by the orbital velocity of) 207 503.35 P
0.16 (the spacecraft is compensated for automatically) 207 491.35 P
0.16 (. The software constantly monitors a set) 397.36 491.35 P
0.28 (of data quality criteria and can \337ag, reject, or reobserve individual integrations that fail) 207 479.35 P
0.79 (the tests. Finally) 207 467.35 P
0.79 (, the software can suspend the observation during scheduled or unex-) 273.77 467.35 P
0.78 (pected interruptions, such as occultation of the tar) 207 455.35 P
0.78 (get by the Earth or passage through) 411.68 455.35 P
0.07 (the South Atlantic Anomaly) 207 443.35 P
0.07 (, and then resume when the interruption ends. The very low) 319.05 443.35 P
0.19 (background count rate and absence of readout noise in the Digicons make exposures of) 207 431.35 P
0.08 (hours duration feasible, though it is strongly suggested that these be broken into shorter) 207 419.35 P
0.47 (segments to aid in scheduling and protect against catastrophic data loss in the event of) 207 407.35 P
(an unexpected problem.) 207 395.35 T
0.35 (The second category of bene\336ts results from the ability of the software to perform pat-) 207 375.35 P
0.04 (terns of integrations at closely spaced positions on the photocathode, a process which is) 207 363.35 P
1.54 (referred to as substepping. There are four purposes for this. At the beginning of an) 207 351.35 P
0.7 (observation, the software executes a procedure called Spectrum Y Balance \050) 207 339.35 P
6 F
1.69 (SPYBAL) 518.67 339.35 P
5 F
0.7 (\051) 554.67 339.35 P
1.05 (to \336nd the optimum centering of the image on the diode array) 207 327.35 P
1.05 (. This compensates for) 464.3 327.35 P
0.37 (minor changes in the image location due to thermal or electrical drifts. The second use) 207 315.35 P
0.79 (is to make multiple \0502 or 4\051 samples per resolution element \0501 diode width\051 to ensure) 207 303.35 P
0.29 (that the digital data satisfy the Nyquist sampling criterion. This is) 207 291.35 P
7 F
0.29 (very) 474.65 291.35 P
5 F
0.29 ( important when) 491.86 291.35 P
1.13 (the ultimate spectral resolution of narrow features is required. Third, the background) 207 279.35 P
0.97 (adjacent to the spectrum or in the echelle interorder region can be measured. Finally) 207 267.35 P
0.97 (,) 555.5 267.35 P
-0.04 (comb addition allows the ef) 207 255.35 P
-0.04 (fect of small diode-to-diode sensitivity variations to be min-) 317.77 255.35 P
1.09 (imized and eliminates the holes in the data due to a few inoperative channels. When) 207 243.35 P
-0.05 (substepping is used to de\336ne the detailed sampling of the spectrum and background, the) 207 231.35 P
0.1 (data obtained at each step are accumulated into one of up to seven distinct \322bins\323 in the) 207 219.35 P
(memory of the onboard computer) 207 207.35 T
(.) 340.87 207.35 T
0.99 (This overview of the \337ight software features is not exhaustive, but summarizes those) 207 187.35 P
0.83 (capabilities which are immediately relevant to the acquisition of spectra in accumula-) 207 175.35 P
3.24 (tion mode. Several items, namely substepping and exposure control, require the) 207 163.35 P
0.81 (observer to specify certain parameters. These will be described in more detail later in) 207 151.35 P
(this) 207 139.35 T
7 F
(Handbook) 223.95 139.35 T
5 F
(.) 265.61 139.35 T
FMENDPAGE
%%EndPage: "19" 9
%%Page: "20" 10
612 792 0 FMBEGINPAGE
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0 9 Q
(Instrument Summary \321 Why Use the GHRS?) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
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0 10 Q
(20) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
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54 726.98 540 726.98 2 L
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54 750.02 540 750.02 2 L
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54 726.98 540 726.98 2 L
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12 F
(Rapid Readout Mode) 189 679.35 T
(\050sometimes called Dir) 283.17 679.35 T
(ect Downlink\051) 375.19 679.35 T
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0.32 (Rapid Readout Mode \050) 189 659.35 P
6 F
0.76 (RAPID) 281.33 659.35 P
5 F
0.32 (\051 is intended to provide very fast time resolution without) 311.33 659.35 P
2.42 (the overhead times associated with Accumulation Mode. The sample time can be) 189 647.35 P
-0.04 (between 50 ms and 12.75 seconds, in increments of 50 milliseconds \050i.e., 1 to 255 times) 189 635.35 P
-0.22 (50 ms\051. At the end of each integration the data are read out, either directly to the TDRSS) 189 623.35 P
0.43 (satellite or to the spacecraft science data tape recorder) 189 611.35 P
0.43 (. The \337ight software cannot exe-) 407.89 611.35 P
0.44 (cute all of its functions and still allow readouts every 50 ms. When the Rapid Readout) 189 599.35 P
1.54 (Mode is entered, substepping, data quality checks and exposure control features are) 189 587.35 P
0.66 (deactivated. The primary factor governing the choice between) 189 575.35 P
6 F
1.57 (ACCUM) 445.01 575.35 P
5 F
0.66 ( and) 475.01 575.35 P
6 F
1.57 ( RAPID) 492.6 575.35 P
5 F
0.66 ( is) 530.17 575.35 P
0.62 (time resolution. In accumulation mode, the time between exposures can be as short as) 189 563.35 P
0.12 (about one minute. If higher time resolution is required, if the source is bright enough to) 189 551.35 P
1.03 (give useful counts in a shorter integration, and if one is willing to sacri\336ce the \337ight) 189 539.35 P
0.29 (software control, then direct downlink is a useful alternative. In) 189 527.35 P
6 F
0.69 (RAPID) 448.48 527.35 P
5 F
0.29 ( mode, a) 478.48 527.35 P
6 F
0.69 (SAM-) 516 527.35 P
5.38 (PLE-TIME) 189 515.35 P
5 F
2.24 ( of less than 0.33 sec requires the use of the 1 Mb data channel \050see) 237 515.35 P
0.17 (Section) 189 503.35 P
0.17 (4.4 on page) 221.5 503.35 P
0.17 (45\051. Such a high data rate stresses) 270.72 503.35 P
7 F
0.17 (HST\325) 409.67 503.35 P
5 F
0.17 (s data-handling capabilities) 430.23 503.35 P
(and means that only about 20 minutes of observations can be stored.) 189 491.35 T
12 F
(Image Mode) 189 471.35 T
5 F
0.23 (Images may be obtained in this mode by de\337ecting the image of the photocathode over) 189 451.35 P
0.41 (the 0.1) 189 439.35 P
0.41 (1) 216.26 439.35 P
8 F
0.41 (\264) 224.17 439.35 P
5 F
0.41 ( 0.1) 229.66 439.35 P
0.41 (1 arcsec focus diodes. The result is a map similar to that obtained during) 244.7 439.35 P
-0.11 (tar) 189 427.35 P
-0.11 (get acquisition, but without an acquisition being performed. Also, a) 199.37 427.35 P
6 F
-0.26 (MAP) 470.78 427.35 P
5 F
-0.11 ( as part of an) 488.78 427.35 P
-0.25 (acquisition can cover more of the sky than the LSA subtends at one time by small move-) 189 415.35 P
0.29 (ments of the telescope, whereas an) 189 403.35 P
6 F
0.7 (IMAGE) 332.11 403.35 P
5 F
0.29 ( is limited to the 1.74 by 1.74 arcsec area of) 362.11 403.35 P
(the LSA; see Section) 189 391.35 T
(4.2 on page) 275.66 391.35 T
(42.) 324.54 391.35 T
12 F
(WSCAN and OSCAN Modes) 189 371.35 T
5 F
-0.22 (These are really modi\336cations of the) 189 351.35 P
6 F
-0.52 (ACCUM) 336.57 351.35 P
5 F
-0.22 (ulation mode designed for higher ef) 366.57 351.35 P
-0.22 (\336ciency) 508.34 351.35 P
-0.18 (in multiple observations, and they may be requested during Phase II of the proposal pro-) 189 339.35 P
0.54 (cess.) 189 327.35 P
6 F
1.3 (WSCAN) 211.2 327.35 P
5 F
0.54 ( obtains a series of spectra within a given order) 241.2 327.35 P
0.54 (, incrementing by a speci-) 434.24 327.35 P
0.76 (\336ed wavelength increment between each. The result is a spectrum spanning a broader) 189 315.35 P
2.24 (wavelength range than is possible with a single exposure.) 189 303.35 P
6 F
5.37 (OSCAN) 441.34 303.35 P
5 F
2.24 ( works with the) 471.34 303.35 P
0.49 (echelle, and uses the magnetic de\337ection of the Digicon to obtain spectra over a range) 189 291.35 P
0.24 (of echelle orders. The grating carrousel is not rotated, and spectra are obtained at equal) 189 279.35 P
0.95 (values of) 189 267.35 P
7 F
0.95 (m) 229.77 267.35 P
8 F
0.95 (l) 236.99 267.35 P
5 F
0.95 (, where) 242.48 267.35 P
7 F
0.95 (m) 276.3 267.35 P
5 F
0.95 ( is the echelle order) 283.52 267.35 P
0.95 (.) 365.07 267.35 P
6 F
2.27 (OSCAN) 371.01 267.35 P
5 F
0.95 ( is not ordinarily used for science) 401.01 267.35 P
(observations.) 189 255.35 T
FMENDPAGE
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/FrameCurGray 1 def
/FrameCurPat null def
/FrameCurColors [ 0 0 0 1 0 0 0 ] def
/FrameColorEpsilon .001 def
/eqepsilon {
sub dup 0 lt {neg} if
FrameColorEpsilon le
} bind def
/FrameCmpColorsCMYK {
2 copy 0 get exch 0 get eqepsilon {
2 copy 1 get exch 1 get eqepsilon {
2 copy 2 get exch 2 get eqepsilon {
3 get exch 3 get eqepsilon
} {pop pop false} ifelse
}{pop pop false} ifelse
} {pop pop false} ifelse
} bind def
/FrameCmpColorsRGB {
2 copy 4 get exch 0 get eqepsilon {
2 copy 5 get exch 1 get eqepsilon {
6 get exch 2 get eqepsilon
}{pop pop false} ifelse
} {pop pop false} ifelse
} bind def
/RGBtoCMYK {
1 exch sub
3 1 roll
1 exch sub
3 1 roll
1 exch sub
3 1 roll
3 copy
2 copy
le { pop } { exch pop } ifelse
2 copy
le { pop } { exch pop } ifelse
dup dup dup
6 1 roll
4 1 roll
7 1 roll
sub
6 1 roll
sub
5 1 roll
sub
4 1 roll
} bind def
/CMYKtoRGB {
dup dup 4 -1 roll add
5 1 roll 3 -1 roll add
4 1 roll add
1 exch sub dup 0 lt {pop 0} if 3 1 roll
1 exch sub dup 0 lt {pop 0} if exch
1 exch sub dup 0 lt {pop 0} if exch
} bind def
/FrameSepInit {
1.0 RealSetgray
} bind def
/FrameSetSepColor {
/FrameSepBlue exch def
/FrameSepGreen exch def
/FrameSepRed exch def
/FrameSepBlack exch def
/FrameSepYellow exch def
/FrameSepMagenta exch def
/FrameSepCyan exch def
/FrameSepIs FMcustom def
setCurrentScreen
} bind def
/FrameSetCyan {
/FrameSepBlue 1.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 1.0 def
/FrameSepIs FMcyan def
setCurrentScreen
} bind def

/FrameSetMagenta {
/FrameSepBlue 1.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 1.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMmagenta def
setCurrentScreen
} bind def

/FrameSetYellow {
/FrameSepBlue 0.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 1.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMyellow def
setCurrentScreen
} bind def

/FrameSetBlack {
/FrameSepBlue 0.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 1.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMblack def
setCurrentScreen
} bind def

/FrameNoSep {
/FrameSepIs FMnone def
setCurrentScreen
} bind def
/FrameSetSepColors {
FrameDict begin
[ exch 1 add 1 roll ]
/FrameSepColors
exch def end
} bind def
/FrameColorInSepListCMYK {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsCMYK
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/FrameColorInSepListRGB {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsRGB
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/RealSetgray /setgray load def
/RealSetrgbcolor /setrgbcolor load def
/RealSethsbcolor /sethsbcolor load def
end
/setgray {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetgray }
{
FrameSepIs FMblack eq
{ RealSetgray }
{ FrameSepIs FMcustom eq
FrameSepRed 0 eq and
FrameSepGreen 0 eq and
FrameSepBlue 0 eq and {
RealSetgray
} {
1 RealSetgray pop
} ifelse
} ifelse
} ifelse
end
} bind def
/setrgbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetrgbcolor }
{
3 copy [ 4 1 roll ]
FrameColorInSepListRGB
{
FrameSepBlue eq exch
FrameSepGreen eq and exch
FrameSepRed eq and
{ 0 } { 1 } ifelse
}
{
FMPColor {
RealSetrgbcolor
currentcmykcolor
} {
RGBtoCMYK
} ifelse
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
RealSetgray
}
ifelse
end
} bind def
/sethsbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSethsbcolor }
{
RealSethsbcolor
currentrgbcolor
setrgbcolor
}
ifelse
end
} bind def
FrameDict begin
/setcmykcolor where {
pop /RealSetcmykcolor /setcmykcolor load def
} {
/RealSetcmykcolor {
4 1 roll
3 { 3 index add 0 max 1 min 1 exch sub 3 1 roll} repeat
setrgbcolor pop
} bind def
} ifelse
userdict /setcmykcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetcmykcolor }
{
4 copy [ 5 1 roll ]
FrameColorInSepListCMYK
{
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
{ 0 } { 1 } ifelse
}
{
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
RealSetgray
}
ifelse
end
} bind put
FMLevel1 not {

/patProcDict 5 dict dup begin
<0f1e3c78f0e1c387> { 3 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<0f87c3e1f0783c1e> { 3 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
<8142241818244281> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-1 -1 moveto 9 9 lineto stroke } bind def
<03060c183060c081> { 1 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<8040201008040201> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
end def
/patDict 15 dict dup begin
/PatternType 1 def
/PaintType 2 def
/TilingType 3 def
/BBox [ 0 0 8 8 ] def
/XStep 8 def
/YStep 8 def
/PaintProc {
begin
patProcDict bstring known {
patProcDict bstring get exec
} {
8 8 true [1 0 0 -1 0 8] bstring imagemask
} ifelse
end
} bind def
end def
} if
/combineColor {
FrameSepIs FMnone eq
{
graymode FMLevel1 or not {

[/Pattern [/DeviceCMYK]] setcolorspace
FrameCurColors 0 4 getinterval aload pop FrameCurPat setcolor
} {
FrameCurColors 3 get 1.0 ge {
FrameCurGray RealSetgray
} {
FMPColor graymode and {
0 1 3 {
FrameCurColors exch get
1 FrameCurGray sub mul
} for
RealSetcmykcolor
} {
4 1 6 {
FrameCurColors exch get
graymode {
1 exch sub 1 FrameCurGray sub mul 1 exch sub
} {
1.0 lt {FrameCurGray} {1} ifelse
} ifelse
} for
RealSetrgbcolor
} ifelse
} ifelse
} ifelse
} {
FrameCurColors 0 4 getinterval aload
FrameColorInSepListCMYK {
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
FrameSepIs FMcustom eq and
{ FrameCurGray } { 1 } ifelse
} {
FrameSepIs FMblack eq
{FrameCurGray 1.0 exch sub mul 1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop FrameCurGray 1.0 exch sub mul 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
graymode FMLevel1 or not {

[/Pattern [/DeviceGray]] setcolorspace
FrameCurPat setcolor
} {
graymode not FMLevel1 and {

dup 1 lt {pop FrameCurGray} if
} if
RealSetgray
} ifelse
} ifelse
} bind def
/savematrix {
orgmatrix currentmatrix pop
} bind def
/restorematrix {
orgmatrix setmatrix
} bind def
/dmatrix matrix def
/dpi 72 0 dmatrix defaultmatrix dtransform
dup mul exch dup mul add sqrt def

/freq dpi dup 72 div round dup 0 eq {pop 1} if 8 mul div def
/sangle 1 0 dmatrix defaultmatrix dtransform exch atan def
/dpiranges [ 2540 2400 1693 1270 1200 635 600 0 ] def
/CMLowFreqs [ 100.402 94.8683 89.2289 100.402 94.8683 66.9349 63.2456 47.4342 ] def
/YLowFreqs [ 95.25 90.0 84.65 95.25 90.0 70.5556 66.6667 50.0 ] def
/KLowFreqs [ 89.8026 84.8528 79.8088 89.8026 84.8528 74.8355 70.7107 53.033 ] def
/CLowAngles [ 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 ] def
/MLowAngles [ 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 ] def
/YLowTDot [ true true false true true false false false ] def
/CMHighFreqs [ 133.87 126.491 133.843 108.503 102.523 100.402 94.8683 63.2456 ] def
/YHighFreqs [ 127.0 120.0 126.975 115.455 109.091 95.25 90.0 60.0 ] def
/KHighFreqs [ 119.737 113.137 119.713 128.289 121.218 89.8026 84.8528 63.6395 ] def
/CHighAngles [ 71.5651 71.5651 71.5651 70.0169 70.0169 71.5651 71.5651 71.5651 ] def
/MHighAngles [ 18.4349 18.4349 18.4349 19.9831 19.9831 18.4349 18.4349 18.4349 ] def
/YHighTDot [ false false true false false true true false ] def
/PatFreq [ 10.5833 10.0 9.4055 10.5833 10.0 10.5833 10.0 9.375 ] def
/screenIndex {
0 1 dpiranges length 1 sub { dup dpiranges exch get 1 sub dpi le {exit} {pop} ifelse } for
} bind def
/getCyanScreen {
FMUseHighFrequencyScreens { CHighAngles CMHighFreqs} {CLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getMagentaScreen {
FMUseHighFrequencyScreens { MHighAngles CMHighFreqs } {MLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getYellowScreen {
FMUseHighFrequencyScreens { YHighTDot YHighFreqs} { YLowTDot YLowFreqs } ifelse
screenIndex dup 3 1 roll get 3 1 roll get { 3 div
{2 { 1 add 2 div 3 mul dup floor sub 2 mul 1 sub exch} repeat
FMSpotFunction } } {/FMSpotFunction load } ifelse
0.0 exch
} bind def
/getBlackScreen {
FMUseHighFrequencyScreens { KHighFreqs } { KLowFreqs } ifelse
screenIndex get 45.0 /FMSpotFunction load
} bind def
/getSpotScreen {
getBlackScreen
} bind def
/getCompositeScreen {
getBlackScreen
} bind def
/FMSetScreen
FMLevel1 { /setscreen load
}{ {
8 dict begin
/HalftoneType 1 def
/SpotFunction exch def
/Angle exch def
/Frequency exch def
/AccurateScreens FMUseAcccurateScreens def
currentdict end sethalftone
} bind } ifelse
def
/setDefaultScreen {
FMPColor {
orgrxfer cvx orggxfer cvx orgbxfer cvx orgxfer cvx setcolortransfer
}
{
orgxfer cvx settransfer
} ifelse
orgfreq organgle orgproc cvx setscreen
} bind def
/setCurrentScreen {
FrameSepIs FMnone eq {
FMUseDefaultNoSeparationScreen {
setDefaultScreen
} {
getCompositeScreen FMSetScreen
} ifelse
} {
FrameSepIs FMcustom eq {
FMUseDefaultSpotSeparationScreen {
setDefaultScreen
} {
getSpotScreen FMSetScreen
} ifelse
} {
FMUseDefaultProcessSeparationScreen {
setDefaultScreen
} {
FrameSepIs FMcyan eq {
getCyanScreen FMSetScreen
} {
FrameSepIs FMmagenta eq {
getMagentaScreen FMSetScreen
} {
FrameSepIs FMyellow eq {
getYellowScreen FMSetScreen
} {
getBlackScreen FMSetScreen
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} bind def
end
/gstring FMLOCAL
/gfile FMLOCAL
/gindex FMLOCAL
/orgrxfer FMLOCAL
/orggxfer FMLOCAL
/orgbxfer FMLOCAL
/orgxfer FMLOCAL
/orgproc FMLOCAL
/orgrproc FMLOCAL
/orggproc FMLOCAL
/orgbproc FMLOCAL
/organgle FMLOCAL
/orgrangle FMLOCAL
/orggangle FMLOCAL
/orgbangle FMLOCAL
/orgfreq FMLOCAL
/orgrfreq FMLOCAL
/orggfreq FMLOCAL
/orgbfreq FMLOCAL
/yscale FMLOCAL
/xscale FMLOCAL
/edown FMLOCAL
/manualfeed FMLOCAL
/paperheight FMLOCAL
/paperwidth FMLOCAL
/FMDOCUMENT {
array /FMfonts exch def
/#copies exch def
FrameDict begin
0 ne /manualfeed exch def
/paperheight exch def
/paperwidth exch def
0 ne /FrameNegative exch def
0 ne /edown exch def
/yscale exch def
/xscale exch def
FMLevel1 {
manualfeed {setmanualfeed} if
/FMdicttop countdictstack 1 add def
/FMoptop count def
% setpapername
% manualfeed {true} {papersize} ifelse
% {manualpapersize} {false} ifelse
% {desperatepapersize} {false} ifelse
% { (Can't select requested paper size for Frame print job!) FMFAILURE } if
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
}
{{1 dict dup /PageSize [paperwidth paperheight]put setpagedevice}stopped
{ (Can't select requested paper size for Frame print job!) FMFAILURE } if
{1 dict dup /ManualFeed manualfeed put setpagedevice } stopped pop }
ifelse

FMPColor {
currentcolorscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def
cvlit /orgbproc exch def
/orgbangle exch def
/orgbfreq exch def
cvlit /orggproc exch def
/orggangle exch def
/orggfreq exch def
cvlit /orgrproc exch def
/orgrangle exch def
/orgrfreq exch def
currentcolortransfer
FrameNegative {
1 1 4 {
pop { 1 exch sub } concatprocs 4 1 roll
} for
4 copy
setcolortransfer
} if
cvlit /orgxfer exch def
cvlit /orgbxfer exch def
cvlit /orggxfer exch def
cvlit /orgrxfer exch def
} {
currentscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def

currenttransfer
FrameNegative {
{ 1 exch sub } concatprocs
dup settransfer
} if
cvlit /orgxfer exch def
} ifelse
end
} def
/pagesave FMLOCAL
/orgmatrix FMLOCAL
/landscape FMLOCAL
/pwid FMLOCAL
/FMBEGINPAGE {
FrameDict begin
/pagesave save def
3.86 setmiterlimit
/landscape exch 0 ne def
landscape {
90 rotate 0 exch dup /pwid exch def neg translate pop
}{
pop /pwid exch def
} ifelse
edown { [-1 0 0 1 pwid 0] concat } if
0 0 moveto paperwidth 0 lineto paperwidth paperheight lineto
0 paperheight lineto 0 0 lineto 1 setgray fill
xscale yscale scale
/orgmatrix matrix def
gsave
} def
/FMENDPAGE {
grestore
pagesave restore
end
showpage
} def
/FMFONTDEFINE {
FrameDict begin
findfont
ReEncode
1 index exch
definefont
FMfonts 3 1 roll
put
end
} def
/FMFILLS {
FrameDict begin dup
array /fillvals exch def
dict /patCache exch def
end
} def
/FMFILL {
FrameDict begin
fillvals 3 1 roll put
end
} def
/FMNORMALIZEGRAPHICS {
newpath
0.0 0.0 moveto
1 setlinewidth
0 setlinecap
0 0 0 sethsbcolor
0 setgray
} bind def
/fx FMLOCAL
/fy FMLOCAL
/fh FMLOCAL
/fw FMLOCAL
/llx FMLOCAL
/lly FMLOCAL
/urx FMLOCAL
/ury FMLOCAL
/FMBEGINEPSF {
end
/FMEPSF save def
/showpage {} def
% See Adobe's "PostScript Language Reference Manual, 2nd Edition", page 714.
% "...the following operators MUST NOT be used in an EPS file:" (emphasis ours)
/banddevice {(banddevice) FMBADEPSF} def
/clear {(clear) FMBADEPSF} def
/cleardictstack {(cleardictstack) FMBADEPSF} def
/copypage {(copypage) FMBADEPSF} def
/erasepage {(erasepage) FMBADEPSF} def
/exitserver {(exitserver) FMBADEPSF} def
/framedevice {(framedevice) FMBADEPSF} def
/grestoreall {(grestoreall) FMBADEPSF} def
/initclip {(initclip) FMBADEPSF} def
/initgraphics {(initgraphics) FMBADEPSF} def
/initmatrix {(initmatrix) FMBADEPSF} def
/quit {(quit) FMBADEPSF} def
/renderbands {(renderbands) FMBADEPSF} def
/setglobal {(setglobal) FMBADEPSF} def
/setpagedevice {(setpagedevice) FMBADEPSF} def
/setshared {(setshared) FMBADEPSF} def
/startjob {(startjob) FMBADEPSF} def
/lettertray {(lettertray) FMBADEPSF} def
/letter {(letter) FMBADEPSF} def
/lettersmall {(lettersmall) FMBADEPSF} def
/11x17tray {(11x17tray) FMBADEPSF} def
/11x17 {(11x17) FMBADEPSF} def
/ledgertray {(ledgertray) FMBADEPSF} def
/ledger {(ledger) FMBADEPSF} def
/legaltray {(legaltray) FMBADEPSF} def
/legal {(legal) FMBADEPSF} def
/statementtray {(statementtray) FMBADEPSF} def
/statement {(statement) FMBADEPSF} def
/executivetray {(executivetray) FMBADEPSF} def
/executive {(executive) FMBADEPSF} def
/a3tray {(a3tray) FMBADEPSF} def
/a3 {(a3) FMBADEPSF} def
/a4tray {(a4tray) FMBADEPSF} def
/a4 {(a4) FMBADEPSF} def
/a4small {(a4small) FMBADEPSF} def
/b4tray {(b4tray) FMBADEPSF} def
/b4 {(b4) FMBADEPSF} def
/b5tray {(b5tray) FMBADEPSF} def
/b5 {(b5) FMBADEPSF} def
FMNORMALIZEGRAPHICS
[/fy /fx /fh /fw /ury /urx /lly /llx] {exch def} forall
fx fw 2 div add fy fh 2 div add translate
rotate
fw 2 div neg fh 2 div neg translate
fw urx llx sub div fh ury lly sub div scale
llx neg lly neg translate
/FMdicttop countdictstack 1 add def
/FMoptop count def
} bind def
/FMENDEPSF {
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
FMEPSF restore
FrameDict begin
} bind def
FrameDict begin
/setmanualfeed {
%%BeginFeature *ManualFeed True
statusdict /manualfeed true put
%%EndFeature
} bind def
/max {2 copy lt {exch} if pop} bind def
/min {2 copy gt {exch} if pop} bind def
/inch {72 mul} def
/pagedimen {
paperheight sub abs 16 lt exch
paperwidth sub abs 16 lt and
{/papername exch def} {pop} ifelse
} bind def
/papersizedict FMLOCAL
/setpapername {
/papersizedict 14 dict def
papersizedict begin
/papername /unknown def
/Letter 8.5 inch 11.0 inch pagedimen
/LetterSmall 7.68 inch 10.16 inch pagedimen
/Tabloid 11.0 inch 17.0 inch pagedimen
/Ledger 17.0 inch 11.0 inch pagedimen
/Legal 8.5 inch 14.0 inch pagedimen
/Statement 5.5 inch 8.5 inch pagedimen
/Executive 7.5 inch 10.0 inch pagedimen
/A3 11.69 inch 16.5 inch pagedimen
/A4 8.26 inch 11.69 inch pagedimen
/A4Small 7.47 inch 10.85 inch pagedimen
/B4 10.125 inch 14.33 inch pagedimen
/B5 7.16 inch 10.125 inch pagedimen
end
} bind def
/papersize {
papersizedict begin
/Letter {lettertray letter} def
/LetterSmall {lettertray lettersmall} def
/Tabloid {11x17tray 11x17} def
/Ledger {ledgertray ledger} def
/Legal {legaltray legal} def
/Statement {statementtray statement} def
/Executive {executivetray executive} def
/A3 {a3tray a3} def
/A4 {a4tray a4} def
/A4Small {a4tray a4small} def
/B4 {b4tray b4} def
/B5 {b5tray b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
statusdict begin stopped end
} bind def
/manualpapersize {
papersizedict begin
/Letter {letter} def
/LetterSmall {lettersmall} def
/Tabloid {11x17} def
/Ledger {ledger} def
/Legal {legal} def
/Statement {statement} def
/Executive {executive} def
/A3 {a3} def
/A4 {a4} def
/A4Small {a4small} def
/B4 {b4} def
/B5 {b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
stopped
} bind def
/desperatepapersize {
statusdict /setpageparams known
{
paperwidth paperheight 0 1
statusdict begin
{setpageparams} stopped
end
} {true} ifelse
} bind def
/DiacriticEncoding [
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /space /exclam /quotedbl
/numbersign /dollar /percent /ampersand /quotesingle /parenleft
/parenright /asterisk /plus /comma /hyphen /period /slash /zero /one
/two /three /four /five /six /seven /eight /nine /colon /semicolon
/less /equal /greater /question /at /A /B /C /D /E /F /G /H /I /J /K
/L /M /N /O /P /Q /R /S /T /U /V /W /X /Y /Z /bracketleft /backslash
/bracketright /asciicircum /underscore /grave /a /b /c /d /e /f /g /h
/i /j /k /l /m /n /o /p /q /r /s /t /u /v /w /x /y /z /braceleft /bar
/braceright /asciitilde /.notdef /Adieresis /Aring /Ccedilla /Eacute
/Ntilde /Odieresis /Udieresis /aacute /agrave /acircumflex /adieresis
/atilde /aring /ccedilla /eacute /egrave /ecircumflex /edieresis
/iacute /igrave /icircumflex /idieresis /ntilde /oacute /ograve
/ocircumflex /odieresis /otilde /uacute /ugrave /ucircumflex
/udieresis /dagger /.notdef /cent /sterling /section /bullet
/paragraph /germandbls /registered /copyright /trademark /acute
/dieresis /.notdef /AE /Oslash /.notdef /.notdef /.notdef /.notdef
/yen /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/ordfeminine /ordmasculine /.notdef /ae /oslash /questiondown
/exclamdown /logicalnot /.notdef /florin /.notdef /.notdef
/guillemotleft /guillemotright /ellipsis /.notdef /Agrave /Atilde
/Otilde /OE /oe /endash /emdash /quotedblleft /quotedblright
/quoteleft /quoteright /.notdef /.notdef /ydieresis /Ydieresis
/fraction /currency /guilsinglleft /guilsinglright /fi /fl /daggerdbl
/periodcentered /quotesinglbase /quotedblbase /perthousand
/Acircumflex /Ecircumflex /Aacute /Edieresis /Egrave /Iacute
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%%EndProlog
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0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (21) 546.88 60.29 P
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1 12 Q
1.2 (Chapter 3) 72 677 S
2 24 Q
-0.48 (Phase I:) 207 677 S
-0.48 (What the T) 207 647 S
-0.48 (AC Sees) 309.29 647 S
3 12 Q
(3.1) 144 424 T
( Essential questions) 164.02 424 T
4 F
( 22) 505.32 424 T
3 F
(3.2) 144 406 T
( Creating an Observation Scenario) 164.02 406 T
4 F
( 23) 505.32 406 T
3 10 Q
(3.2.1) 162 389.33 T
( The Simplest Case: One Spectrum for One Star) 187.02 389.33 T
4 F
( 23) 508.1 389.33 T
3 F
(3.2.2) 162 373.33 T
( Several Spectra for One Star) 187.02 373.33 T
4 F
( 23) 508.1 373.33 T
3 F
(3.2.3) 162 357.33 T
( Spectra of Several Stars) 187.02 357.33 T
4 F
( 24) 508.1 357.33 T
3 F
(3.2.4) 162 341.33 T
( RAPID Mode Observations) 187.02 341.33 T
4 F
( 24) 508.1 341.33 T
3 F
(3.2.5) 162 325.33 T
( Adding Calibrations) 187.02 325.33 T
4 F
( 24) 508.1 325.33 T
3 12 Q
(3.3) 144 308 T
( Specifying T) 164.02 308 T
(arget Acquisition) 232.04 308 T
4 F
( 24) 505.32 308 T
3 10 Q
(3.3.1) 162 291.33 T
( V) 187.02 291.33 T
(ery Bright Stars) 195.92 291.33 T
4 F
( 25) 508.1 291.33 T
3 F
(3.3.2) 162 275.33 T
( Moving T) 187.02 275.33 T
(argets) 229.81 275.33 T
4 F
( 25) 508.1 275.33 T
3 F
(3.3.3) 162 259.33 T
( Crowded Fields) 187.02 259.33 T
4 F
( 25) 508.1 259.33 T
3 F
(3.3.4) 162 243.33 T
( Extended and V) 187.02 243.33 T
(ery Faint Objects) 260.41 243.33 T
4 F
( 26) 508.1 243.33 T
3 F
(3.3.5) 162 227.33 T
( V) 187.02 227.33 T
(ariable Objects) 195.73 227.33 T
4 F
( 26) 508.1 227.33 T
3 12 Q
(3.4) 144 210 T
( Calculating the Exposure T) 164.02 210 T
(ime) 310.97 210 T
4 F
( 26) 505.32 210 T
3 10 Q
(3.4.1) 162 193.33 T
( Sensitivity) 187.02 193.33 T
4 F
( 26) 508.1 193.33 T
3 F
(3.4.2) 162 177.33 T
( Reddening) 187.02 177.33 T
4 F
( 27) 508.1 177.33 T
3 F
(3.4.3) 162 161.33 T
( Background) 187.02 161.33 T
4 F
( 27) 508.1 161.33 T
3 F
(3.4.4) 162 145.33 T
( Scattered light) 187.02 145.33 T
4 F
( 28) 508.1 145.33 T
3 F
(3.4.5) 162 129.33 T
( Signal-to-noise) 187.02 129.33 T
4 F
( 29) 508.1 129.33 T
3 F
(3.4.6) 162 113.33 T
( A Simple Example) 187.02 113.33 T
4 F
( 31) 508.1 113.33 T
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
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2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Phase I: What the T) 189 736.18 T
(AC Sees) 271.35 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(22) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
5 F
0.09 (A proposal for the) 189 679.35 P
6 F
0.09 (Hubble Space T) 264.9 679.35 P
0.09 (elescope) 328.04 679.35 P
5 F
0.09 ( is written in two phases. In Phase I, you are) 362.47 679.35 P
0.64 (asked to provide the minimum information needed for the T) 189 667.35 P
0.64 (elescope Allocation Com-) 434.29 667.35 P
-0.01 (mittee and STScI to judge the scienti\336c merit and technical feasibility of what you wish) 189 655.35 P
-0.18 (to do. If your proposal is successful, you will be asked in Phase II to provide the speci\336c) 189 643.35 P
0.35 (details and parameters that are needed to turn your proposal into a series of commands) 189 631.35 P
0.73 (that the spacecraft can execute. At the time this) 189 619.35 P
6 F
0.73 (Handbook) 387.2 619.35 P
5 F
0.73 ( is being written the proce-) 428.86 619.35 P
0.04 (dures for submission of) 189 607.35 P
6 F
0.04 (HST) 285.83 607.35 P
5 F
0.04 ( proposals are under review; consult the) 303.61 607.35 P
6 F
0.04 (Call for Pr) 465.82 607.35 P
0.04 (oposals) 509.44 607.35 P
5 F
0.07 (for the procedures in ef) 189 595.35 P
0.07 (fect. In particular) 282.39 595.35 P
0.07 (, Cycle 5 proposals will ask for time in units of) 351.27 595.35 P
1.13 (orbits instead of total spacecraft time and an orbit calculator has been constructed to) 189 583.35 P
(allow for planning.) 189 571.35 T
-0.17 (These instructions for completing a Phase I proposal are meant to work with the Cycle 5) 189 551.35 P
6 F
(Call for Pr) 189 539.35 T
(oposals) 232.53 539.35 T
5 F
(and) 265.59 539.35 T
6 F
(Phase I Pr) 282.53 539.35 T
(oposal Instructions) 324.93 539.35 T
5 F
(.) 401.88 539.35 T
54 496.02 540 499.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 497.52 540 497.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 497.52 180 497.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(3.1) 163.32 503.02 T
(Essential questions) 189 503.02 T
5 10 Q
(The essential questions you must answer in \336lling out an) 189 479.35 T
6 F
(HST) 418.44 479.35 T
5 F
( proposal form are:) 436.22 479.35 T
7 11 Q
(\245) 189 461.35 T
5 10 Q
(Do I need real-time acquisition for my tar) 203.4 461.35 T
(gets?) 370.13 461.35 T
7 11 Q
(\245) 189 446.35 T
5 10 Q
(How long will my exposures take?) 203.4 446.35 T
7 11 Q
(\245) 189 431.35 T
5 10 Q
(Are standard calibrations adequate for my needs?) 203.4 431.35 T
7 11 Q
(\245) 189 416.35 T
5 10 Q
(Does my science call for any special requirements?) 203.4 416.35 T
(All of these lead up to:) 189 396.35 T
7 11 Q
(\245) 189 378.35 T
5 10 Q
(What is the total number of orbits my program asks for?) 203.4 378.35 T
0.87 (The information you provide on the execution of observations is divided into Phase I) 189 358.35 P
0.27 (and Phase II. Phase I proposal processing takes place before the T) 189 346.35 P
0.27 (AC meets and at that) 455.03 346.35 P
0.03 (time you are asked to provide only the information that they need to arrive at a decision) 189 334.35 P
1.49 (on the scienti\336c merit and feasibility of your proposal. The T) 189 322.35 P
1.49 (AC needs to know) 447.21 322.35 P
1.49 (, of) 525.18 322.35 P
0.75 (course, how much telescope time your program is likely to need. Phase II takes place) 189 310.35 P
0.03 (only after your proposal is successful and at that time you are required to specify all the) 189 298.35 P
1.36 (details needed to transform your observational needs into spacecraft commands, and) 189 286.35 P
(you must do so within the total spacecraft time that you have been allotted.) 189 274.35 T
0.55 (The distinction between Phase I and Phase II is somewhat arbitrary and in some cases) 189 254.35 P
-0.2 (the Phase I forms actually prevent you from supplying information \050such as the entrance) 189 242.35 P
1.33 (aperture to be used\051 that could be helpful in assessing the proposal. The intent is to) 189 230.35 P
0.73 (make writing the Phase I proposal easier) 189 218.35 P
0.73 (, but you may \336nd that your proposal will be) 355.14 218.35 P
-0.25 (better if you understand fully the operation and use of the GHRS right from the start. W) 189 206.35 P
-0.25 (e) 535.56 206.35 P
1.23 (encourage you to think in terms of the Phase II requirements even when writing the) 189 194.35 P
0.53 (Phase I proposal because in most cases that will not require much more work and you) 189 182.35 P
0.26 (may be able to save some time later on. Thus there is information in this section that is) 189 170.35 P
-0.21 (only entered on the Phase II forms but which has been included here to provide a picture) 189 158.35 P
(of how the instrument works.) 189 146.35 T
FMENDPAGE
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612 792 0 FMBEGINPAGE
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[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (23) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Phase I: What the T) 207 736.18 T
(AC Sees) 289.35 736.18 T
72 671.02 558 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 672.52 558 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 672.52 198 672.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(3.2) 181.32 678.02 T
(Creating an Observation Scenario) 207 678.02 T
0 10 Q
(3.2.1) 175.76 644.35 T
(The Simplest Case: One Spectrum for One Star) 207 644.35 T
5 F
0.31 (Let us assume that in answering the above questions you have decided that an onboard) 207 624.35 P
0.61 (acquisition will suf) 207 612.35 P
0.61 (\336ce \050more on that in a moment\051, that standard calibrations are ade-) 284.7 612.35 P
0.45 (quate, and that you wish to obtain a single spectrum of a single star) 207 600.35 P
0.45 (. By specifying the) 481.11 600.35 P
0.74 (resolving power you desire for a particular wavelength, you have, in ef) 207 588.35 P
0.74 (fect, chosen to) 498.48 588.35 P
0.36 (observe with either Side 1 or Side 2 and with a particular grating \050see Chapter 7\051. This) 207 576.35 P
2.55 (simplest of observation scenarios then involves one acquisition sequence and one) 207 564.35 P
8 F
3.15 (ACCUM) 207 552.35 P
5 F
1.31 ( observation. \050An) 237 552.35 P
8 F
3.15 (IMAGE) 313.15 552.35 P
5 F
1.31 ( mode observation may be speci\336ed in place of the) 343.15 552.35 P
8 F
1.12 (ACCUM) 207 540.35 P
5 F
0.47 ( with no loss of generality) 237 540.35 P
0.47 (. A) 342.85 540.35 P
8 F
1.12 (WSCAN) 358.51 540.35 P
5 F
0.47 ( or) 388.51 540.35 P
8 F
1.12 (OSCAN) 402.78 540.35 P
5 F
0.47 ( is just a minor variation on an) 432.78 540.35 P
8 F
(ACCUM) 207 528.35 T
5 F
(. See below for) 237 528.35 T
8 F
(RAPID) 300.04 528.35 T
5 F
(s.\051) 330.04 528.35 T
-0.18 (The choice of Side 1 or Side 2 for obtaining the spectrum need not necessarily force you) 207 508.35 P
0.12 (to that Side for the acquisition; for example, you might wish to observe a cool star with) 207 496.35 P
0.92 (grating G140L on Side 1, but the far ultraviolet \337ux would be too low to acquire the) 207 484.35 P
-0.04 (object with mirror N1. In that case you can use mirror N2; it is permissible to mix Sides) 207 472.35 P
-0.09 (in a scenario, but there may be a cost in observing time for doing so \050see Section) 207 460.35 P
-0.09 (4.1.5.1) 530.5 460.35 P
0.54 (on page) 207 448.35 P
0.54 (38\051. Some dif) 241.42 448.35 P
0.54 (\336cult tar) 297.03 448.35 P
0.54 (gets may be best acquired with the FOS before they are) 331 448.35 P
(observed with the GHRS.) 207 436.35 T
0.63 (For this simple case this sequence of events can be compared to the) 207 416.35 P
6 F
0.63 (Phase I Pr) 487.67 416.35 P
0.63 (oposal) 531.33 416.35 P
(Instructions) 207 404.35 T
5 F
(:) 254.78 404.35 T
7 11 Q
(\245) 207 386.35 T
5 10 Q
(A guide star acquisition.) 221.4 386.35 T
7 11 Q
(\245) 207 371.35 T
5 10 Q
(The tar) 221.4 371.35 T
(get acquisition with the GHRS.) 249.82 371.35 T
7 11 Q
(\245) 207 356.35 T
5 10 Q
(The) 221.4 356.35 T
8 F
(ACCUM) 239.45 356.35 T
5 F
( \050or) 269.45 356.35 T
8 F
(IMAGE) 286.11 356.35 T
5 F
(\051.) 316.11 356.35 T
7 11 Q
(\245) 207 341.35 T
5 10 Q
(Some overhead time to read the observation.) 221.4 341.35 T
0 F
(3.2.2) 175.76 311.35 T
(Several Spectra for One Star) 207 311.35 T
5 F
0.24 (If more than one spectrum is desired for the star) 207 291.35 P
0.24 (, the) 400.68 291.35 P
8 F
0.58 (ACCUM) 420.88 291.35 P
5 F
0.24 (s + overheads are repeated) 450.88 291.35 P
-0.11 (as necessary) 207 279.35 P
-0.11 (, bearing in mind the need to reacquire the star at the start of each orbit. The) 255.94 279.35 P
1.47 (multiple spectra could be either an assortment of wavelengths or repeats at a single) 207 267.35 P
0.33 (wavelength to follow an object in time or to improve signal-to-noise. In all cases over-) 207 255.35 P
(head time must be added for each separate exposure:) 207 243.35 T
7 11 Q
(\245) 207 225.35 T
5 10 Q
(A guide star acquisition.) 221.4 225.35 T
7 11 Q
(\245) 207 210.35 T
5 10 Q
(The tar) 221.4 210.35 T
(get acquisition with the GHRS.) 249.82 210.35 T
7 11 Q
(\245) 207 195.35 T
5 10 Q
(The \336rst) 221.4 195.35 T
8 F
(ACCUM) 257.51 195.35 T
5 F
( or) 287.51 195.35 T
8 F
(IMAGE) 300.84 195.35 T
5 F
(.) 330.84 195.35 T
7 11 Q
(\245) 207 180.35 T
5 10 Q
(Some overhead time to read the observation.) 221.4 180.35 T
7 11 Q
(\245) 207 165.35 T
5 10 Q
(The second) 221.4 165.35 T
8 F
(ACCUM) 269.72 165.35 T
5 F
( or) 299.72 165.35 T
8 F
(IMAGE) 313.05 165.35 T
5 F
(, followed by an overhead allowance.) 343.05 165.35 T
7 11 Q
(\245) 207 150.35 T
5 10 Q
(The third) 221.4 150.35 T
8 F
(ACCUM) 260.84 150.35 T
5 F
(\311) 290.84 150.35 T
FMENDPAGE
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0 9 Q
(Phase I: What the T) 189 736.18 T
(AC Sees) 271.35 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(24) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
(3.2.3) 157.76 679.35 T
(Spectra of Several Stars) 189 679.35 T
5 F
0.02 (This instance is just multiple versions of the previous case since changing stars requires) 189 659.35 P
1.62 (a new visit, meaning a full guide star acquisition, acquisition of the object into the) 189 647.35 P
(GHRS LSA, etc.) 189 635.35 T
0 F
(3.2.4) 157.76 605.35 T
7 F
(RAPID) 189 605.35 T
0 F
( Mode Observations) 219 605.35 T
8 F
2.45 (RAPID) 189 585.35 P
5 F
1.02 ( mode observations can be planned just as for) 219 585.35 P
8 F
2.45 (ACCUM) 412.88 585.35 P
5 F
1.02 (s. The overhead time is) 442.88 585.35 P
(added only once at the very end of the whole) 189 573.35 T
8 F
(RAPID) 371.18 573.35 T
5 F
( sequence.) 401.18 573.35 T
0 F
(3.2.5) 157.76 543.35 T
(Adding Calibrations) 189 543.35 T
5 F
0.05 (The only kind of calibration exposure that an observer will ordinarily need is one of the) 189 523.35 P
-0.14 (wavelength calibration lamp. An exposure of 30 to 60 seconds is adequate for almost all) 189 511.35 P
1.56 (settings with the \336rst-order gratings; otherwise the exposure is just another) 189 499.35 P
8 F
3.74 (ACCUM) 507.5 499.35 P
5 F
1.56 (.) 537.5 499.35 P
-0.09 (Note that for most applications the information contained in the) 189 487.35 P
8 F
-0.21 (SPYBAL) 445.31 487.35 P
5 F
-0.09 ( that accompa-) 481.31 487.35 P
0.32 (nies each \336rst use of a grating is likely to suf) 189 475.35 P
0.32 (\336ce and a separate wavelength calibration) 370.93 475.35 P
(is super\337uous; see Section) 189 463.35 T
(4.5 on page) 297.33 463.35 T
(46.) 346.21 463.35 T
54 420.02 540 423.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 421.52 540 421.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 421.52 180 421.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(3.3) 163.32 427.02 T
(Specifying T) 189 427.02 T
(arget Acquisition) 259.46 427.02 T
5 10 Q
2.69 (For most situations, a standard onboard acquisition that automatically centers the) 189 403.35 P
0.33 (brightest object in the \336eld into the desired aperture is all that is needed. Such a proce-) 189 391.35 P
-0.15 (dure is especially appropriate for isolated point sources that are beyond our solar system) 189 379.35 P
0.35 (and which have fairly predictable ultraviolet \337uxes, i.e., most stars. In other cases, it is) 189 367.35 P
1.58 (possible to use a variation on the automatic procedure to acquire other objects. For) 189 355.35 P
-0.09 (example, an extended object or some moving objects may be acquired by \336rst automati-) 189 343.35 P
0.11 (cally centering on a nearby pointlike source and then of) 189 331.35 P
0.11 (fsetting to the object of interest.) 412.25 331.35 P
(Some potential problem cases are:) 189 319.35 T
7 11 Q
(\245) 189 301.35 T
5 10 Q
(very bright stars, which can saturate the detectors;) 203.4 301.35 T
7 11 Q
(\245) 189 286.35 T
5 10 Q
(moving tar) 203.4 286.35 T
(gets, such as planets and their satellites;) 246.83 286.35 T
7 11 Q
(\245) 189 271.35 T
5 10 Q
(crowded \336elds, in which the automatic centering procedure might) 203.4 271.35 T
(get confused;) 468.91 271.35 T
7 11 Q
(\245) 189 256.35 T
5 10 Q
(extended objects that do not have a sharply peaked source to center on;) 203.4 256.35 T
7 11 Q
(\245) 189 241.35 T
5 10 Q
0.06 (very faint objects for which few counts would be accumulated in the maximum per-) 203.4 241.35 P
(missible integration time \05012.75 sec\051.) 203.4 229.35 T
7 11 Q
(\245) 189 214.35 T
5 10 Q
1 (objects that are so variable that their brightness relative to nearby objects may be) 203.4 214.35 P
(unpredictable.) 203.4 202.35 T
0.8 (These situations may require an interactive \050or real-time\051 acquisition, although an on-) 189 182.35 P
0.1 (board acquisition may still work in many cases. In an interactive acquisition, the space-) 189 170.35 P
0.22 (craft obtains a picture of the tar) 189 158.35 P
0.22 (get\325) 315.64 158.35 P
0.22 (s \336eld with one of the cameras \050WFPC2 or FOC\051 or) 330.64 158.35 P
0.85 (with the \336eld mapping capability of the GHRS itself. This picture is relayed immedi-) 189 146.35 P
0.28 (ately to STScI where the observer is available to study the image and decide where the) 189 134.35 P
1.04 (telescope should be pointed. Interactive acquisitions are obviously helpful in dif) 189 122.35 P
1.04 (\336cult) 519.44 122.35 P
2.26 (situations, but the requirement for real-time contact between the ground and) 189 110.35 P
6 F
2.26 (HST) 520.46 110.35 P
5 F
2.26 (,) 537.5 110.35 P
0.1 (together with the need to set aside a block of telescope time for the pointing decision to) 189 98.35 P
FMENDPAGE
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (25) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Phase I: What the T) 207 736.18 T
(AC Sees) 289.35 736.18 T
5 10 Q
1.26 (be made, makes interactive acquisitions consume much more spacecraft time than is) 207 679.35 P
2.71 (needed for a standard onboard acquisition. Interactive acquisitions require special) 207 667.35 P
1.87 (scheduling and so require greater) 207 655.35 P
1.87 (-than-average work on the part of the planners of) 347.01 655.35 P
6 F
0.29 (HST\325) 207 643.35 P
5 F
0.29 (s time. Real-time contact with) 227.56 643.35 P
6 F
0.29 (HST) 351.79 643.35 P
5 F
0.29 ( is a limited resource \050it cannot exceed 20% of) 369.57 643.35 P
(the total time\051 which must be reserved for genuine need.) 207 631.35 T
0.57 (A variation on this procedure is to get the \336eld image two months or so in advance of) 207 611.35 P
-0.08 (the time the spectrum will be obtained. This is called an early acquisition \050) 207 599.35 P
8 F
-0.19 (EARLY) 504.25 599.35 P
-0.19 (ACQ) 536.67 599.35 P
5 F
-0.08 (\051) 554.67 599.35 P
0.83 (and it takes more time than an on-board acquisition but much less than an interactive) 207 587.35 P
0.2 (acquisition and imposes no burden of real-time contact. The observer must be prepared) 207 575.35 P
0.83 (to analyze the early acquisition image quickly \050within a week or two\051 if the positions) 207 563.35 P
(from it are to be incorporated into the telescope schedule.) 207 551.35 T
0.09 (If you wish to use either WFPC2 or FOC for early- or interactive acquisitions you must) 207 531.35 P
-0.03 (refer to documents speci\336c to those instruments. Details on the use of the GHRS\325 imag-) 207 519.35 P
(ing capability are provided in the next chapter) 207 507.35 T
(.) 390.58 507.35 T
0 F
(3.3.1) 175.76 477.35 T
(V) 207 477.35 T
(ery Bright Stars) 213.12 477.35 T
5 F
0.14 (When is a star too bright for an onboard acquisition? In practice we are unaware of any) 207 457.35 P
0.06 (real need to use interactive acquisition just because a star is very bright. GHRS acquisi-) 207 445.35 P
0.53 (tions are done with ultraviolet light, so it is the UV \337ux of the star that matters. There) 207 433.35 P
0.09 (are no stars too bright to acquire with the attenuated mirror A1, for example. Even with) 207 421.35 P
-0.05 (Side 2 it is not necessary to specify an interactive acquisition for a very bright star if the) 207 409.35 P
8 F
2.33 (BRIGHT=RETURN) 207 397.35 P
5 F
0.97 ( option is used. Since the few very bright stars which could cause) 285 397.35 P
1.49 (problems are always the brightest point sources in their immediate area, there is no) 207 385.35 P
(apparent reason not to use) 207 373.35 T
8 F
(BRIGHT=RETURN) 313.92 373.35 T
5 F
( with an onboard acquisition.) 391.92 373.35 T
0 F
(3.3.2) 175.76 343.35 T
(Moving T) 207 343.35 T
(argets) 250.15 343.35 T
5 F
1.36 (Sophisticated pointing at moving objects \050i.e., objects within the solar system\051 often) 207 323.35 P
0.7 (requires interactive acquisition to be sure the desired portion of the object\325) 207 311.35 P
0.7 (s surface is) 512.17 311.35 P
0.53 (centered in the observing aperture. There are cases where an on-board acquisition will) 207 299.35 P
1.42 (suf) 207 287.35 P
1.42 (\336ce, especially if the object is small \050essentially point-like\051 and has a well-deter-) 219.04 287.35 P
1.72 (mined orbit. An on-board acquisition can often work well even for a lar) 207 275.35 P
1.72 (ge moving) 513.78 275.35 P
0.31 (object like Jupiter by \336rst centering on a small object nearby whose relative position is) 207 263.35 P
0.02 (well known \050one of Jupiter) 207 251.35 P
0.02 (\325) 315.21 251.35 P
0.02 (s moons, for example\051, and then of) 317.99 251.35 P
0.02 (fsetting to the position of) 457.36 251.35 P
1.36 (interest on the planetary disk. Solar system astronomers may wish to consult with a) 207 239.35 P
(moving-tar) 207 227.35 T
(get specialist at STScI before specifying the acquisition mode.) 251.26 227.35 T
0 F
(3.3.3) 175.76 197.35 T
(Crowded Fields) 207 197.35 T
5 F
0.79 (W) 207 177.35 P
0.79 (ork in crowded \336elds can usually be done by obtaining an early acquisition, so that) 215.64 177.35 P
0.09 (you have an image to work from to specify the object to be observed, an image that has) 207 165.35 P
0.02 (been obtained with) 207 153.35 P
6 F
0.02 (HST) 285.65 153.35 P
5 F
0.02 (\325) 303.43 153.35 P
0.02 (s full spatial resolution. The camera observation is usually best) 306.21 153.35 P
(done at about the same wavelength that the spectroscopic observations will be made.) 207 141.35 T
0.21 (The Point Spread Function \050PSF\051 of the GHRS has been restored by the COST) 207 121.35 P
0.21 (AR mir-) 524.18 121.35 P
1.55 (rors, making it possible to separately observe stars that are very close together) 207 109.35 P
1.55 (. For) 537.55 109.35 P
0.34 (example, in an Early Release Observation in April, 1994, two stars in R136a separated) 207 97.35 P
FMENDPAGE
%%EndPage: "25" 5
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Phase I: What the T) 189 736.18 T
(AC Sees) 271.35 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(26) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
5 F
-0.21 (by only 0.25 arcsec were observed independently) 189 679.35 P
-0.21 (. One of these stars was only 0.1 arcsec) 384.52 679.35 P
0.19 (from a brighter neighbor) 189 667.35 P
0.19 (. This was done by centering on a bright object in the \336eld and) 287.6 667.35 P
0.01 (then of) 189 655.35 P
0.01 (fsetting to the tar) 216.88 655.35 P
0.01 (gets of interest. W) 284.8 655.35 P
0.01 (e suggest that you consult with us if you wish) 357.36 655.35 P
(to work in crowded \336elds. Also, see Section) 189 643.35 T
(8.6.1 on page) 367.87 643.35 T
(94.) 424.25 643.35 T
0 F
(3.3.4) 157.76 613.35 T
(Extended and V) 189 613.35 T
(ery Faint Objects) 263.47 613.35 T
5 F
0.13 (For most extended objects, it may be possible to of) 189 593.35 P
0.13 (fset from a nearby point source or at) 393.86 593.35 P
1.96 (the least the pointing can be speci\336ed from an early acquisition image. Interactive) 189 581.35 P
1 (acquisitions should be necessary only rarely) 189 569.35 P
1 (. Another method is to acquire the object) 369.7 569.35 P
(with the FOS and then of) 189 557.35 T
(fset to the GHRS\325 LSA.) 289.65 557.35 T
-0.22 (In Cycle 5 observers can use a centering option designed expressly for extended objects,) 189 537.35 P
0.29 (especially uniform ones like the Gallilean satellites of Jupiter) 189 525.35 P
0.29 (. Chapter 4 contains more) 435.78 525.35 P
(information on this option, known as) 189 513.35 T
8 F
(LOCATE) 339.28 513.35 T
(=) 377.78 513.35 T
(EXTENDED) 386.28 513.35 T
5 F
(.) 434.28 513.35 T
0 F
(3.3.5) 157.76 483.35 T
(V) 189 483.35 T
(ariable Objects) 195.12 483.35 T
5 F
-0.14 (Objects whose ultraviolet brightness varied often caused acquisitions to fail when it was) 189 463.35 P
-0.21 (necessary to specify both) 189 451.35 P
8 F
-0.5 (BRIGHT) 291.47 451.35 P
5 F
-0.21 ( and) 327.47 451.35 P
8 F
-0.5 (FAINT) 346.49 451.35 P
5 F
-0.21 ( count limits. The advent of software that) 376.49 451.35 P
0.7 (automatically \336nds the brightest object in the \336eld) 189 439.35 P
8 F
1.68 (\050BRIGHT=RETURN) 397.94 439.35 P
5 F
0.7 (\051 obviates that) 481.94 439.35 P
0.11 (problem in most cases. A variable object in a crowded \336eld might bene\336t from an early) 189 427.35 P
0.47 (acquisition to determine precise coordinates, but an interactive acquisition should gen-) 189 415.35 P
(erally be unnecessary) 189 403.35 T
(.) 274.43 403.35 T
54 360.02 540 363.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 361.52 540 361.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 361.52 180 361.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(3.4) 163.32 367.02 T
(Calculating the Exposure T) 189 367.02 T
(ime) 343.49 367.02 T
0 10 Q
(3.4.1) 157.76 333.35 T
(Sensitivity) 189 333.35 T
5 F
1.07 (The sensitivity of the GHRS and) 189 313.35 P
6 F
1.07 (HST) 328.73 313.35 P
5 F
1.07 ( Optical T) 346.52 313.35 P
1.07 (elescope Assembly \050OT) 388.5 313.35 P
1.07 (A\051, using the) 485.92 313.35 P
-0.19 (LSA, has been determined from observations of stars with known ultraviolet \337uxes. The) 189 301.35 P
0.32 (sensitivity is designated as) 189 289.35 P
0.32 (, and has units of \050counts diode) 310.41 289.35 P
5 8 Q
0.26 (-1) 437.07 293.35 P
5 10 Q
0.32 ( sec) 443.73 289.35 P
5 8 Q
0.26 (-1) 459.33 293.35 P
5 10 Q
0.32 (\051 for each incident) 465.99 289.35 P
0.07 (\050er) 189 277.35 P
0.07 (g cm) 199.92 277.35 P
5 8 Q
0.06 (-2) 219.71 281.35 P
5 10 Q
0.07 ( sec) 226.38 277.35 P
5 8 Q
0.06 (-1) 241.72 281.35 P
5 10 Q
0.07 ( \201\051. It varies as a function of wavelength for each grating. Y) 248.38 277.35 P
0.07 (ou must \336rst) 489.85 277.35 P
0.21 (estimate the intrinsic \337ux of your tar) 189 265.35 P
0.21 (get and then multiply that by the appropriate value) 336.15 265.35 P
-0.19 (of) 189 253.35 P
-0.19 ( to yield an estimate of the count rate to be expected for a particular grating con\336g-) 210.86 253.35 P
0.25 (uration at the chosen wavelength. Sensitivity curves for the \336rst-order gratings are pro-) 189 241.35 P
(vided in Section) 189 229.35 T
(8.2.3 on page) 256.5 229.35 T
(85 and for the echelles in Section) 312.88 229.35 T
(8.3.1 on page) 448.69 229.35 T
(87.) 505.07 229.35 T
0.68 (In the echelle con\336gurations, the sensitivity varies with wavelength across each order) 189 209.35 P
0.68 (.) 537.5 209.35 P
-0.17 (This behavior is characteristic of all echelle spectrographs, and is called the Blaze Func-) 189 197.35 P
0.16 (tion. The basic nature of the variation with wavelength is similar for all orders, and can) 189 185.35 P
0.15 (be parameterized in terms of the product) 189 173.35 P
0.15 (, where) 370.01 173.35 P
6 F
0.15 (m) 402.23 173.35 P
5 F
0.15 ( is the order number and) 409.45 173.35 P
9 F
0.15 (l) 510.32 173.35 P
5 F
0.15 ( is the) 515.81 173.35 P
0.66 (wavelength \050\201\051. The shape of the blaze function, normalized to a peak value of unity) 189 161.35 P
0.66 (,) 537.5 161.35 P
0.05 (and plotted as a function of) 189 149.35 P
0.05 ( is shown in Section) 316.23 149.35 P
0.05 (8.3.3 on page) 399.49 149.35 P
0.05 (91. The sensitivity at) 455.96 149.35 P
0.31 (any wavelength in any order can be estimated by multiplying the peak response of that) 189 137.35 P
1.03 (order by the relative response shown. The blaze function, relative to the center of an) 189 125.35 P
-0.25 (order) 189 113.35 P
-0.25 (, falls as low as 0.25 at the end of the free spectral range and its ef) 209.7 113.35 P
-0.25 (fect should not be) 469.36 113.35 P
(omitted in exposure calculations.) 189 101.35 T
299.19 283.26 310.41 297.19 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(S) 299.69 289.35 T
9 7 Q
(l) 305.07 286.25 T
0 0 612 792 C
199.64 247.26 210.86 261.19 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(S) 200.14 253.35 T
9 7 Q
(l) 205.52 250.25 T
0 0 612 792 C
354.72 169.02 370.01 181.19 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(m) 355.21 173.35 T
9 F
(l) 363.02 173.35 T
0 0 612 792 C
300.94 145.02 316.23 157.19 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(m) 301.44 149.35 T
9 F
(l) 309.25 149.35 T
0 0 612 792 C
FMENDPAGE
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612 792 0 FMBEGINPAGE
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[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
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[ 0 0 1 0 1 1 0]
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0 0 0 1 0 0 0 K
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (27) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Phase I: What the T) 207 736.18 T
(AC Sees) 289.35 736.18 T
0 10 Q
(3.4.2) 175.76 672.36 T
(Reddening) 207 672.36 T
5 F
3.66 (Corrections for ultraviolet extinction in the interstellar medium are included in) 207 652.36 P
0.02 (Section) 207 640.36 P
0.02 (8.5 on page) 239.5 640.36 P
0.02 (93. These are standard values, and their applicability in speci\336c sit-) 288.42 640.36 P
(uations is left to the judgment of the observer) 207 628.36 T
(.) 388.1 628.36 T
0 F
(3.4.3) 175.76 598.36 T
(Background) 207 598.36 T
5 F
-0.18 (There are several potential sources of background counts, including detector dark count,) 207 578.36 P
0.7 (electrical interference or cross talk with devices either within the GHRS or the space-) 207 566.36 P
0 (craft, and ef) 207 554.36 P
0 (fects caused by the char) 254.86 554.36 P
0 (ged particle radiation environment of the) 350.22 554.36 P
6 F
0 (HST) 516.33 554.36 P
5 F
0 ( orbit.) 534.1 554.36 P
1.18 (The intrinsic sources of dark count are very small. During \322thermal vacuum\323 testing) 207 542.36 P
0.25 (prior to launch the detector dark count rates were observed to be approximately 0.0004) 207 530.36 P
0.04 (counts per diode per second. On-orbit, the background is caused primarily by Cerenkov) 207 518.36 P
0.17 (radiation bursts induced in the faceplate of the Digicon by cosmic rays. This causes the) 207 506.37 P
1.01 (actual background to range from) 207 494.37 P
1.01 ( to about four times that, depending on the) 380.17 494.37 P
0.42 (orbital position of) 207 482.37 P
6 F
0.42 (HST) 282.44 482.37 P
5 F
0.42 (. For planning purposes these mean values suf) 299.48 482.37 P
0.42 (\336ce: 0.01) 486.69 482.37 P
0.42 (1 counts) 523.97 482.37 P
0.14 (s) 207 470.37 P
5 8 Q
0.11 (-1) 210.89 474.36 P
5 10 Q
0.14 ( for D2 and 0.008 counts s) 217.55 470.37 P
5 8 Q
0.11 (-1) 324.18 474.36 P
5 10 Q
0.14 ( for D1. The counts appear to be randomly distributed in) 330.85 470.37 P
0.13 (time, so that the \322noise\323 in the dark count is the square root of the total counts accumu-) 207 458.37 P
0.25 (lated during the observation. If one is observing very faint objects with low count rates) 207 446.37 P
0.21 (the background can in\337uence the signal to noise ratio of the data. Formulae for making) 207 434.37 P
1.29 (quantitative estimates of S/N are given in Section) 207 422.37 P
1.29 (3.4.5.1 on page) 416.57 422.37 P
1.29 (29. At the present) 483.03 422.37 P
0.53 (time there are no known sources of interference or cross talk which af) 207 410.37 P
0.53 (fect the detector) 492.52 410.37 P
(count rates.) 207 398.37 T
-0.1 (The GHRS is equipped with both hardware \050automatic\051 and software capabilities to rec-) 207 378.37 P
0.05 (ognize and respond to cosmic ray and trapped particle events. Y) 207 366.37 P
0.05 (ou may invoke the soft-) 462.82 366.37 P
2.82 (ware capability by specifying) 207 354.37 P
8 F
6.76 (CENSOR) 338.8 354.37 P
6.76 (=) 380.12 354.37 P
6.76 (YES) 391.44 354.37 P
5 F
2.82 ( on an Exposure Logsheet line in) 409.44 354.37 P
1.93 (Phase) 207 342.37 P
1.93 (II. This causes rejection of individual) 232.83 342.37 P
8 F
4.63 (STEP-TIME) 396.32 342.37 P
5 F
1.93 ( segments of data if they) 450.32 342.37 P
0.64 (included a speci\336ed number of photons arriving within a short \050) 207 330.37 P
9 F
0.64 (8 m) 468.33 330.37 P
5 F
0.64 (s\051 interval, as hap-) 482.22 330.37 P
0.5 (pens with cosmic rays. Any rejected integration is repeated, so there is no loss of total) 207 318.37 P
0.05 (exposure time. Y) 207 306.37 P
0.05 (ou should only use this anticoincidence rejection on faint tar) 274.69 306.37 P
0.05 (gets, since) 516.29 306.37 P
0.01 (on bright tar) 207 294.37 P
0.01 (gets the interval between actual photon events will be small and real counts) 256.28 294.37 P
0.19 (would be rejected. W) 207 282.37 P
0.19 (e recommend using) 292.31 282.37 P
8 F
0.46 (CENSOR) 373.7 282.37 P
0.46 (=) 412.39 282.37 P
0.46 (YES) 421.09 282.37 P
5 F
0.19 ( only for count rates less than) 439.09 282.37 P
0.24 (about 0.1 counts per diode per second. The expected dark count reduction is a few tens) 207 270.37 P
(of per cent \050For more details on) 207 258.37 T
8 F
(CENSOR) 336.14 258.37 T
5 F
(, see Section) 372.14 258.37 T
(8.6.2 on page) 424.91 258.37 T
(95\051.) 481.29 258.37 T
-0.24 (For extremely faint sources for which the expected count rate is well below the expected) 207 238.37 P
1.73 (dark level, it is possible to use a special commanding option called) 207 226.37 P
8 F
4.16 (FLYLIM) 497.49 226.37 P
5 F
1.73 (. This) 533.49 226.37 P
-0.22 (option, if pertinent to your needs, should be explored with a GHRS Instrument Scientist.) 207 214.37 P
(See also Section) 207 202.37 T
(8.6.3 on page) 275.05 202.37 T
(97.) 331.43 202.37 T
0.06 (An external source of background which can potentially be a problem during the acqui-) 207 182.37 P
1.51 (sition \050and sometimes the observation\051 of faint tar) 207 170.37 P
1.51 (gets is geocoronal L) 417.06 170.37 P
1.51 (yman-) 501.85 170.37 P
9 F
1.51 (a) 527.4 170.37 P
5 F
1.51 (. This) 533.71 170.37 P
(problem and what to do about it are discussed in Section) 207 158.37 T
(7.4.2 on page) 435.59 158.37 T
(80.) 491.97 158.37 T
-0.25 (The \336nal cause of background counts is passage through the dip in the Earth\325) 207 138.37 P
-0.25 (s V) 511.83 138.37 P
-0.25 (an Allen) 524.08 138.37 P
-0.22 (radiation belt called the South Atlantic Anomaly \050SAA\051. SAA passage occurs on 7 of 16) 207 126.37 P
0.01 (daily orbits of) 207 114.37 P
6 F
0.01 (HST) 265.64 114.37 P
5 F
0.01 (. During the most central of these passages, dark count rates increase) 282.68 114.37 P
-0.17 (about two orders of magnitude, to about 1 count per diode per second. A contour around) 207 102.37 P
-0.05 (the SSA which corresponds to 0.02 cts/s/diode is known and no GHRS observations are) 207 90.37 P
345.09 491.2 380.17 505.32 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(4) 345.51 494.37 T
(1) 360.99 494.37 T
(0) 365.99 494.37 T
5 7 Q
(3) 375.26 497.24 T
(\320) 371.49 497.24 T
9 10 Q
(\264) 353.01 494.37 T
0 0 612 792 C
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
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[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
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FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Phase I: What the T) 189 736.18 T
(AC Sees) 271.35 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(28) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
5 F
0.6 (scheduled when the) 189 679.35 P
6 F
0.6 (HST) 272.18 679.35 P
5 F
0.6 ( is within this zone. At the time of this writing the SAA con-) 289.96 679.35 P
(tours for the GHRS are being reviewed to allow for more ef) 189 667.35 T
(\336cient usage.) 427.93 667.35 T
0 F
(3.4.4) 157.76 637.35 T
(Scattered light) 189 637.35 T
5 F
0.29 (The presence of stray and scattered light in a spectrograph is an ef) 189 617.35 P
0.29 (fect which can in\337u-) 456.65 617.35 P
-0.18 (ence the planning and execution of an observation, as well as the reduction and interpre-) 189 605.35 P
0.51 (tation of the data. None of the optical con\336gurations which include \336rst order gratings) 189 593.35 P
-0.03 (has any serious problem with scattered light. The high quality of the imaging optics and) 189 581.35 P
1.05 (holographic dif) 189 569.35 P
1.05 (fraction gratings and the ef) 251.25 569.35 P
1.05 (fectiveness of the baf) 363.02 569.35 P
1.05 (\337es have successfully) 451.25 569.35 P
0.66 (minimized the stray light. On-orbit measurements indicate that it amounts to less than) 189 557.35 P
-0.21 (10) 189 545.35 P
5 8 Q
-0.17 (-3) 199 549.35 P
5 10 Q
-0.21 ( when using the SSA, and at most a few times 10) 205.66 545.35 P
5 8 Q
-0.17 (-3) 399.45 549.35 P
5 10 Q
-0.21 (when using the LSA \050these are in) 407.95 545.35 P
(units of the peak intensity\051.) 189 533.35 T
-0 (In the echelle con\336guration, both the echelle and the cross-dispersers are ruled gratings.) 189 513.35 P
0.85 (This fact, plus the presence of light from sixteen orders simultaneously on the photo-) 189 501.35 P
-0.24 (cathode, results in a detectable level of background radiation. The irradiance on the pho-) 189 489.35 P
0.13 (tocathode due to scattered light \050measured as count rate per unit area\051 amounts to a few) 189 477.35 P
0.37 (percent of the signal in the order) 189 465.35 P
0.37 (. T) 320.61 465.35 P
0.37 (wo factors complicate this ef) 331.39 465.35 P
0.37 (fect. The \336rst is a geo-) 448.2 465.35 P
1.37 (metrical ef) 189 453.35 P
1.37 (fect caused by the fact that the science diodes are 400) 233.23 453.35 P
9 F
1.37 (m) 465.14 453.35 P
5 F
1.37 (m tall, while the) 470.9 453.35 P
0.28 (image of the spectrum is only about 55) 189 441.35 P
9 F
0.28 (m) 349.53 441.35 P
5 F
0.28 (m high. Thus about 1/8 of the diode is illumi-) 355.29 441.35 P
0.88 (nated by the spectrum+background, while the rest is measuring background, meaning) 189 429.35 P
0.79 (that a weak background irradiance is multiplied to the point that a signi\336cant fraction) 189 417.35 P
-0.1 (\050anywhere from 2 to 50%\051 of the gross count rate on a diode may be due to background.) 189 405.35 P
3.27 (The measured scattered light background can be calculated from information in) 189 393.35 P
(Section) 189 381.35 T
(8.3.1 on page) 221.5 381.35 T
(87. It varies signi\336cantly with order number) 277.88 381.35 T
(.) 453.7 381.35 T
1.73 (The second complication arises at the short wavelength ends of the echelle format.) 189 361.35 P
0.64 (Below a wavelength of about 1800 \201 with Echelle B \050or 1250 \201 with Echelle A\051, the) 189 349.35 P
0.75 (spacing between orders is comparable to the length of the diodes, and it is dif) 189 337.35 P
0.75 (\336cult to) 508.41 337.35 P
1.26 (make a clean measurement of a single order) 189 325.35 P
1.26 (. The diode array has four lar) 373.07 325.35 P
1.26 (ge \322corner) 496.82 325.35 P
0.57 (diodes\323 which are long \0501 mm\051 in the direction of the echelle\325) 189 313.35 P
0.57 (s dispersion, but narrow) 442.19 313.35 P
1.3 (\050100) 189 301.35 P
9 F
1.3 (m) 211.13 301.35 P
5 F
1.3 (m\051 in the cross-dispersion direction. These diodes may be used to sample the) 216.89 301.35 P
0.25 (interorder background without the problem of contamination by in order light, but they) 189 289.35 P
0.17 (do not provide any spatial resolution. The) 189 277.35 P
6 F
0.17 (HST) 359.64 277.35 P
5 F
0.17 ( scheduling system will default to use of) 377.42 277.35 P
-0 (the corner diodes when that is appropriate. At a minimum, the time spent measuring the) 189 265.35 P
0.99 (background should be about 10% of the time spent on the spectrum. If the goal is to) 189 253.35 P
1.19 (achieve a very high signal to noise ratio in the net spectrum, it may be necessary to) 189 241.35 P
0.39 (devote a greater fraction of time to the background measurement. Suggestions for esti-) 189 229.35 P
(mating signal to noise ratios are made in the next section.) 189 217.35 T
-0.08 (In order to reduce stray light, there is a shutter over the LSA which automatically closes) 189 197.35 P
1.09 (whenever the SSA is being used for an observation. There is no shutter on the SSA.) 189 185.35 P
1.55 (Thus a wavelength calibration exposure obtained with a bright star in the SSA will) 189 173.35 P
0.4 (result in a combined spectrum of the two because the aperture for the wavelength cali-) 189 161.35 P
0.17 (bration lamp \050SC2\051 is displaced from the SSA in the same sense as the direction of dis-) 189 149.35 P
2.77 (persion. Usually you can subtract the stellar spectrum to recover the wavelength) 189 137.35 P
(calibration.) 189 125.35 T
0.32 (More detailed quantitative information on background and scattered light in the GHRS) 189 105.35 P
(is provided in Section) 189 93.35 T
(8.6.1 on page) 279 93.35 T
(94.) 335.38 93.35 T
FMENDPAGE
%%EndPage: "28" 8
%%Page: "29" 9
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (29) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Phase I: What the T) 207 736.18 T
(AC Sees) 289.35 736.18 T
0 10 Q
(3.4.5) 175.76 679.35 T
( Signal-to-noise) 207 679.35 T
5 F
0.16 (There are several factors which in\337uence the signal to noise, including statistical \050Pois-) 207 659.35 P
0.58 (son\051 noise in the detected spectrum, dark count noise in the detector) 207 647.35 P
0.58 (, scattered light in) 484.6 647.35 P
1.23 (the spectrograph, diode to diode gain variations, and granularity in the photocathode) 207 635.35 P
0.74 (sensitivity) 207 623.35 P
0.74 (. For signal to noise ratios up to approximately 50, statistical \337uctuations in) 247.47 623.35 P
-0.19 (the signal and background will dominate. Diode to diode variations are extremely small,) 207 611.35 P
1.31 (and are accounted for in the routine calibration procedures. Cathode granularity will) 207 599.35 P
-0 (become important if signal to noise greater than 50 is required, and must be treated sep-) 207 587.35 P
0.12 (arately) 207 575.35 P
0.12 (. For sources observed through the small aperture the sky background should not) 233.56 575.35 P
(contribute signi\336cantly to the noise, except, perhaps, when observing at L) 207 563.35 T
(yman-) 501.69 563.35 T
9 F
(a) 527.24 563.35 T
5 F
(.) 533.55 563.35 T
0 9 Q
(3.4.5.1) 170.48 540.02 T
(Photon Noise) 207 540.02 T
5 10 Q
-0.03 (The following equations may be used to estimate signal to noise ratio, depending on the) 207 519.35 P
(relative importance of scattered light and dark count.) 207 507.35 T
0 F
(Case 1) 207 487.35 T
3 F
(. Neither scattered light nor dark count are important.) 239.24 487.35 T
5 F
( Let:) 207 467.35 T
6 F
-0.12 (s) 221.4 449.35 P
5 F
-0.12 (= signal strength \050counts per diode per second\051 estimated by multiplying the stellar) 227.67 449.35 P
(\337ux by the sensitivity at the desired wavelength.) 235.8 437.35 T
6 F
0.03 (t) 221.4 422.35 P
5 F
0.03 ( = duration of the observation in seconds. This total time will be divided among the) 224.18 422.35 P
(separate substep bins.) 235.8 410.35 T
0.2 (= the number of adjacent diodes that will be binned together to produce an ef) 231.5 395.35 P
0.2 (fec-) 542.46 395.35 P
0.4 (tive resolution element. Usually) 235.8 383.35 P
6 F
0.4 (n) 367.66 383.35 P
5 8 Q
0.32 (s) 372.66 380.85 P
5 10 Q
0.4 ( = 1. This is not the mer) 375.78 383.35 P
0.4 (ging of substep bins,) 474.02 383.35 P
0.37 (but the deliberate averaging to increase signal to noise at the expense of resolu-) 235.8 371.35 P
(tion.) 235.8 359.35 T
(Then) 207 339.35 T
0.5 (This formula would be appropriate for relatively bright objects observed with any \336rst) 207 282.34 P
(order grating, when substep pattern 1, 2, or 3 is used \050see Section) 207 270.34 T
(8.4 on page) 470.29 270.34 T
(92\051.) 519.17 270.34 T
0 F
(Case 2) 207 250.34 T
3 F
(. Dark count is important, scattered light is not.) 239.24 250.34 T
5 F
( Let:) 207 230.34 T
6 F
(d) 221.4 212.34 T
5 F
( = dark count rate in counts per diode per second.) 226.4 212.34 T
(Then) 207 192.34 T
0.85 (If the signal is less than about ten times the dark count rate, the factor in parentheses) 207 152.34 P
0.14 (should be included in the estimate. This formula would be useful if) 207 140.34 P
8 F
0.35 (STEP-PATT) 479.55 140.34 P
5 F
0.14 ( 5, for) 533.55 140.34 P
0.26 (example, were used with a \336rst order grating to measure a faint source \050see Section) 207 128.34 P
0.26 (8.4) 545.5 128.34 P
(on page) 207 116.34 T
(92\051.) 240.88 116.34 T
221.4 390.02 231.5 403.19 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(n) 221.9 395.35 T
6 7 Q
(s) 227.28 392.25 T
0 0 612 792 C
72 87.98 558 686.02 C
275.83 299.01 354.17 336.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(S) 281.96 311.39 T
(N) 293.62 311.39 T
9 F
(\244) 289.46 311.39 T
(\050) 277.67 311.39 T
(\051) 300.76 311.39 T
5 7 Q
(2) 306.25 314.27 T
6 10 Q
(s) 325.39 311.39 T
(n) 329.87 311.39 T
6 7 Q
(s) 335.25 308.29 T
6 10 Q
(t) 338.56 311.39 T
5 F
(=) 314.75 311.39 T
72 87.98 558 686.02 C
0 0 612 792 C
207 162.5 450 186.4 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(S) 303.68 172.34 T
(N) 315.35 172.34 T
9 F
(\244) 311.18 172.34 T
(\050) 299.39 172.34 T
(\051) 322.48 172.34 T
5 7 Q
(2) 327.98 175.22 T
6 10 Q
(s) 361.09 178.13 T
(d) 371.65 178.13 T
9 F
(\244) 367.48 178.13 T
5 F
(1) 353.27 165.88 T
6 F
(s) 368.91 165.88 T
(d) 379.46 165.88 T
9 F
(\244) 375.3 165.88 T
5 F
(+) 360.77 165.88 T
(-) 353.27 172.57 T
(-) 354.93 172.57 T
(-) 356.6 172.57 T
(-) 358.27 172.57 T
(-) 359.93 172.57 T
(-) 361.6 172.57 T
(-) 363.26 172.57 T
(-) 364.92 172.57 T
(-) 366.59 172.57 T
(-) 368.26 172.57 T
(-) 369.92 172.57 T
(-) 371.58 172.57 T
(-) 373.25 172.57 T
(-) 374.92 172.57 T
(-) 376.58 172.57 T
(-) 378.24 172.57 T
(-) 379.91 172.57 T
(-) 381.13 172.57 T
9 F
(\350) 347.11 168.43 T
(\370) 385.12 168.43 T
(\346) 347.11 177 T
(\366) 385.12 177 T
6 F
(s) 390.71 172.34 T
(n) 395.19 172.34 T
6 7 Q
(s) 400.57 169.24 T
6 10 Q
(t) 403.89 172.34 T
5 F
(=) 336.47 172.34 T
0 0 612 792 C
FMENDPAGE
%%EndPage: "29" 9
%%Page: "30" 10
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Phase I: What the T) 189 736.18 T
(AC Sees) 271.35 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(30) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
(Case 3) 189 679.35 T
3 F
(. Scattered light is important, dark count is not.) 221.24 679.35 T
5 F
(Let:) 189 659.35 T
6 F
(f) 203.4 641.35 T
5 F
(= fraction of time spent measuring the spectrum. \050See Section) 208.68 641.35 T
(8.4 on page) 458.45 641.35 T
(92\051) 507.33 641.35 T
6 F
(b) 203.4 626.35 T
5 F
( = scattered light as a fraction of the signal in the adjacent orders.) 208.4 626.35 T
(Then) 189 606.35 T
0.75 (This formula gives a good estimate of the performance for observations with the ech-) 189 562.45 P
0.43 (elles when stepping patterns 6, 7, 8 or 9 are used. This formula assumes that the back-) 189 550.45 P
0.98 (ground bins are heavily smoothed. Most of the high frequency statistical noise in the) 189 538.45 P
(background bins is thus suppressed.) 189 526.45 T
0 F
(Case 4) 189 506.45 T
3 F
(. Both scattered light and dark count are important.) 221.24 506.45 T
5 F
(Let:) 189 486.45 T
0.01 (= number of adjacent diodes to smooth the background bins over before subtract-) 214.28 468.45 P
1.5 (ing. Experiments with ground-based data indicate that) 217.8 456.45 P
1.5 ( gives the best) 478.55 456.45 P
(results.) 217.8 444.45 T
(Then) 189 424.45 T
0.19 (There are two ways to use these formulae. If you need a certain S/N to do the scienti\336c) 189 358.37 P
0.7 (analysis, use the appropriate equation to solve for the required exposure time) 189 346.37 P
6 F
0.7 (t) 507.64 346.37 P
5 F
0.7 (. Alter-) 510.42 346.37 P
0.66 (nately) 189 334.37 P
0.66 (, you can decide to devote a \336xed length of time to the observation, and use the) 212.79 334.37 P
(equations to estimate what S/N will be achieved.) 189 322.37 T
0 9 Q
(3.4.5.2) 152.48 299.03 T
(Fixed Pattern Noise) 189 299.03 T
5 10 Q
-0.07 (The formulae just presented suggest that the signal to noise ratio increases in proportion) 189 278.37 P
0.13 (to the square root of the exposure time. These relations only hold true until S/N) 189 266.37 P
9 F
0.13 (\273) 510.92 266.37 P
5 F
0.13 ( 50 or) 516.41 266.37 P
3.23 (so is reached. At higher signal levels the photocathode granularity described in) 189 254.37 P
0.04 (Section) 189 242.37 P
0.04 (4.3 on page) 221.5 242.37 P
0.04 (43 will become the limiting factor) 270.46 242.37 P
0.04 (. Observing standard stars to pro-) 406.49 242.37 P
0.39 (vide a precise \322\337at \336eld\323 observation is too inef) 189 230.37 P
0.39 (\336cient, and there is no onboard contin-) 382.98 230.37 P
-0.1 (uum lamp that illuminates the optics and detectors in exactly the same way as the stellar) 189 218.37 P
0.16 (spectrum. The best practice is to use the) 189 206.37 P
8 F
0.39 (FP-SPLIT) 352.76 206.37 P
5 F
0.16 ( option \050Section) 400.76 206.37 P
0.16 (4.3.1 on page) 467.47 206.37 P
0.16 (43\051.) 524.17 206.37 P
-0.17 (Rather than merely averaging the four) 189 194.37 P
8 F
-0.42 (FP-SPLIT) 342.91 194.37 P
5 F
-0.17 ( sub-exposures, the data analysis pro-) 390.91 194.37 P
0.83 (cedure solves for the two vectors representing photocathode granularity and the spec-) 189 182.37 P
(trum. S/N well in excess of 100 has been obtained this way on bright tar) 189 170.37 T
(gets.) 477.4 170.37 T
-0.1 (Achieving extremely high signal-to-noise \050200 or more\051 is possible by obtaining a num-) 189 150.37 P
1.61 (ber of spectra, each with) 189 138.37 P
8 F
3.87 (FP-SPLIT) 297.57 138.37 P
5 F
1.61 ( but at slightly dif) 345.57 138.37 P
1.61 (ferent grating positions. See) 422.96 138.37 P
(Lambert et al. \0501994\051 for a discussion.) 189 126.37 T
54 87.98 540 686.02 C
254.81 579.11 339.19 603.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(S) 261.56 588.96 T
(N) 273.23 588.96 T
9 F
(\244) 269.06 588.96 T
(\050) 257.27 588.96 T
(\051) 280.36 588.96 T
5 7 Q
(2) 285.86 591.84 T
6 10 Q
(f) 308.98 594.75 T
5 F
(1) 300.05 582.5 T
6 F
(b) 315.68 582.5 T
5 F
(+) 307.54 582.5 T
(-) 300.05 589.2 T
(-) 301.71 589.2 T
(-) 303.38 589.2 T
(-) 305.04 589.2 T
(-) 306.7 589.2 T
(-) 308.37 589.2 T
(-) 310.04 589.2 T
(-) 311.7 589.2 T
(-) 313.36 589.2 T
(-) 315.03 589.2 T
(-) 316.7 589.2 T
(-) 317.35 589.2 T
6 F
(s) 321.47 588.96 T
(n) 325.95 588.96 T
6 7 Q
(s) 331.33 585.86 T
6 10 Q
(t) 334.64 588.96 T
9 F
(\273) 291.86 588.96 T
54 87.98 540 686.02 C
0 0 612 792 C
203.4 463.12 214.28 476.28 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(n) 203.9 468.45 T
6 7 Q
(b) 209.28 465.35 T
0 0 612 792 C
447.19 451.12 478.55 464.28 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(n) 447.68 456.45 T
6 7 Q
(b) 453.07 453.35 T
5 10 Q
(1) 467.05 456.45 T
(0) 472.05 456.45 T
9 F
(\273) 459.06 456.45 T
0 0 612 792 C
54 87.98 540 686.02 C
103.51 375.03 490.49 421.11 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(S) 248.12 403.92 T
(N) 259.79 403.92 T
9 F
(\244) 255.62 403.92 T
(\050) 243.83 403.92 T
(\051) 266.92 403.92 T
5 7 Q
(2) 272.41 406.79 T
6 10 Q
(s) 374.05 409.47 T
5 7 Q
(2) 378.44 412.34 T
6 10 Q
(t) 382.53 409.47 T
(s) 291.75 391.67 T
5 F
(1) 302.39 397.22 T
6 F
(b) 318.02 397.22 T
5 F
(+) 309.89 397.22 T
6 F
(n) 306.97 384.97 T
6 7 Q
(s) 312.35 381.87 T
6 10 Q
(f) 315.66 384.97 T
5 F
(-) 302.39 391.67 T
(-) 304.05 391.67 T
(-) 305.72 391.67 T
(-) 307.38 391.67 T
(-) 309.05 391.67 T
(-) 310.71 391.67 T
(-) 312.38 391.67 T
(-) 314.04 391.67 T
(-) 315.71 391.67 T
(-) 317.37 391.67 T
(-) 319.04 391.67 T
(-) 319.69 391.67 T
6 F
(b) 350.89 397.22 T
(n) 334.06 384.97 T
6 7 Q
(b) 339.44 381.87 T
5 10 Q
(1) 349.49 384.97 T
6 F
(f) 364.49 384.97 T
5 F
(\320) 356.99 384.97 T
9 F
(\050) 345.2 384.97 T
(\051) 367.73 384.97 T
5 F
(-) 334.06 391.67 T
(-) 335.73 391.67 T
(-) 337.39 391.67 T
(-) 339.06 391.67 T
(-) 340.72 391.67 T
(-) 342.39 391.67 T
(-) 344.05 391.67 T
(-) 345.72 391.67 T
(-) 347.38 391.67 T
(-) 349.05 391.67 T
(-) 350.71 391.67 T
(-) 352.38 391.67 T
(-) 354.04 391.67 T
(-) 355.71 391.67 T
(-) 357.37 391.67 T
(-) 359.04 391.67 T
(-) 360.7 391.67 T
(-) 362.37 391.67 T
(-) 364.03 391.67 T
(-) 365.7 391.67 T
(-) 367.36 391.67 T
(-) 369.03 391.67 T
(-) 369.4 391.67 T
(+) 325.72 391.67 T
6 F
(d) 389.02 391.67 T
5 F
(1) 404.01 397.22 T
6 F
(n) 400.77 384.97 T
6 7 Q
(s) 406.15 381.87 T
6 10 Q
(f) 409.47 384.97 T
5 F
(-) 400.77 391.67 T
(-) 402.44 391.67 T
(-) 404.1 391.67 T
(-) 405.77 391.67 T
(-) 407.43 391.67 T
(-) 408.92 391.67 T
(1) 440.12 397.22 T
6 F
(n) 423.28 384.97 T
6 7 Q
(b) 428.66 381.87 T
5 10 Q
(1) 438.71 384.97 T
6 F
(f) 453.71 384.97 T
5 F
(\320) 446.21 384.97 T
9 F
(\050) 434.42 384.97 T
(\051) 456.95 384.97 T
5 F
(-) 423.28 391.67 T
(-) 424.95 391.67 T
(-) 426.61 391.67 T
(-) 428.28 391.67 T
(-) 429.94 391.67 T
(-) 431.61 391.67 T
(-) 433.27 391.67 T
(-) 434.94 391.67 T
(-) 436.6 391.67 T
(-) 438.27 391.67 T
(-) 439.93 391.67 T
(-) 441.6 391.67 T
(-) 443.26 391.67 T
(-) 444.93 391.67 T
(-) 446.59 391.67 T
(-) 448.26 391.67 T
(-) 449.92 391.67 T
(-) 451.59 391.67 T
(-) 453.25 391.67 T
(-) 454.92 391.67 T
(-) 456.58 391.67 T
(-) 458.25 391.67 T
(-) 458.62 391.67 T
(+) 414.95 391.67 T
(+) 380.89 391.67 T
(-) 291.75 403.92 T
(-) 293.41 403.92 T
(-) 295.08 403.92 T
(-) 296.74 403.92 T
(-) 298.41 403.92 T
(-) 300.07 403.92 T
(-) 301.74 403.92 T
(-) 303.4 403.92 T
(-) 305.07 403.92 T
(-) 306.73 403.92 T
(-) 308.4 403.92 T
(-) 310.06 403.92 T
(-) 311.73 403.92 T
(-) 313.39 403.92 T
(-) 315.06 403.92 T
(-) 316.72 403.92 T
(-) 318.39 403.92 T
(-) 320.05 403.92 T
(-) 321.72 403.92 T
(-) 323.38 403.92 T
(-) 325.05 403.92 T
(-) 326.71 403.92 T
(-) 328.38 403.92 T
(-) 330.04 403.92 T
(-) 331.71 403.92 T
(-) 333.37 403.92 T
(-) 335.04 403.92 T
(-) 336.7 403.92 T
(-) 338.37 403.92 T
(-) 340.03 403.92 T
(-) 341.7 403.92 T
(-) 343.36 403.92 T
(-) 345.03 403.92 T
(-) 346.69 403.92 T
(-) 348.36 403.92 T
(-) 350.02 403.92 T
(-) 351.69 403.92 T
(-) 353.35 403.92 T
(-) 355.02 403.92 T
(-) 356.68 403.92 T
(-) 358.35 403.92 T
(-) 360.01 403.92 T
(-) 361.68 403.92 T
(-) 363.34 403.92 T
(-) 365.01 403.92 T
(-) 366.67 403.92 T
(-) 368.34 403.92 T
(-) 370 403.92 T
(-) 371.67 403.92 T
(-) 373.33 403.92 T
(-) 375 403.92 T
(-) 376.66 403.92 T
(-) 378.33 403.92 T
(-) 379.99 403.92 T
(-) 381.66 403.92 T
(-) 383.32 403.92 T
(-) 384.99 403.92 T
(-) 386.65 403.92 T
(-) 388.32 403.92 T
(-) 389.98 403.92 T
(-) 391.65 403.92 T
(-) 393.31 403.92 T
(-) 394.98 403.92 T
(-) 396.64 403.92 T
(-) 398.31 403.92 T
(-) 399.97 403.92 T
(-) 401.64 403.92 T
(-) 403.3 403.92 T
(-) 404.97 403.92 T
(-) 406.63 403.92 T
(-) 408.3 403.92 T
(-) 409.96 403.92 T
(-) 411.63 403.92 T
(-) 413.29 403.92 T
(-) 414.96 403.92 T
(-) 416.62 403.92 T
(-) 418.29 403.92 T
(-) 419.95 403.92 T
(-) 421.62 403.92 T
(-) 423.28 403.92 T
(-) 424.95 403.92 T
(-) 426.61 403.92 T
(-) 428.28 403.92 T
(-) 429.94 403.92 T
(-) 431.61 403.92 T
(-) 433.27 403.92 T
(-) 434.94 403.92 T
(-) 436.6 403.92 T
(-) 438.27 403.92 T
(-) 439.93 403.92 T
(-) 441.6 403.92 T
(-) 443.26 403.92 T
(-) 444.93 403.92 T
(-) 446.59 403.92 T
(-) 448.26 403.92 T
(-) 449.92 403.92 T
(-) 451.59 403.92 T
(-) 453.25 403.92 T
(-) 454.92 403.92 T
(-) 456.58 403.92 T
(-) 458.25 403.92 T
(-) 459.91 403.92 T
(-) 461.58 403.92 T
(-) 463.24 403.92 T
(-) 464.28 403.92 T
(=) 280.91 403.92 T
301.23 382.12 298.23 382.12 298.23 402.72 3 L
0.45 H
2 Z
N
298.23 402.72 301.23 402.72 2 L
N
373.39 382.12 376.39 382.12 376.39 402.72 3 L
N
376.39 402.72 373.39 402.72 2 L
N
399.61 382.12 396.61 382.12 396.61 402.72 3 L
N
396.61 402.72 399.61 402.72 2 L
N
462.61 382.12 465.61 382.12 465.61 402.72 3 L
N
465.61 402.72 462.61 402.72 2 L
N
54 87.98 540 686.02 C
0 0 612 792 C
FMENDPAGE
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612 792 0 FMBEGINPAGE
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N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
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0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (31) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
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72 726.98 558 726.98 2 L
0.25 H
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72 74.02 558 74.02 2 L
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72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
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72 74.02 558 74.02 2 L
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0 9 Q
(Phase I: What the T) 207 736.18 T
(AC Sees) 289.35 736.18 T
0 10 Q
(3.4.6) 175.76 679.35 T
(A Simple Example) 207 679.35 T
5 F
0.57 (Here is a very simple example to illustrate how an integration time may be computed.) 207 663.35 P
0.81 (Suppose that the goal is to obtain a spectrum of a 13th magnitude B0 star at 1900 \201,) 207 651.35 P
0.07 (with the G160M grating and with a signal-to-noise of 25 per diode in the continuum. In) 207 639.35 P
-0.21 (this case we will assume that this star has not been previously observed in the ultraviolet) 207 627.35 P
(so that there is no) 207 615.35 T
6 F
(a priori) 280.05 615.35 T
5 F
( knowledge of the UV \337ux.) 310.89 615.35 T
3.6 (T) 207 595.35 P
3.6 (o be speci\336c, take the star to have a spectral type of B0I,) 212.41 595.35 P
3.6 (, and) 534.96 595.35 P
-0.05 (. The unreddened color for this spectral type is) 276.77 583.35 P
-0.05 (, so) 544.16 583.35 P
0.54 (that) 207 571.35 P
0.54 (. The total visual extinction is then) 301.51 571.35 P
0.54 (, leading) 523.02 571.35 P
1.58 (to a dereddened magnitude of) 207 559.35 P
1.58 (. The dereddened \337ux at 5500 \201 is then) 387.36 559.35 P
(.) 353.56 547.35 T
-0.2 (What \337ux can we anticipate at 1900 \201? The model atmospheres of Kurucz \0501979, ApJS,) 207 527.35 P
-0.03 (40, 1\051 predict) 207 513.35 P
-0.03 ( for a star with) 339.28 513.35 P
-0.03 (K. This leads to a \337ux of) 459.04 513.35 P
0.19 ( at 1900 \201 for the unreddened star) 353.56 499.35 P
0.19 (. Reddening will) 491.23 499.35 P
0.51 (diminish this by a factor of) 207 485.35 P
0.51 (, where the absorption at 1900 \201 can be deter-) 368.42 485.35 P
0.43 (mined from the data in Section) 207 471.35 P
0.43 (8.5 on page) 335.27 471.35 P
0.43 (93; the result in this case is) 385.01 471.35 P
0.43 (.) 555.5 471.35 P
(W) 207 457.35 T
(e therefore predict this star to have a \337ux at 1900 \201 of) 215.64 457.35 T
(.) 545.2 457.35 T
0.31 (The next step is to determine the detected count rate. For G160M at 1900 \201, the sensi-) 207 435.35 P
0.87 (tivity is) 207 423.35 P
0.87 (, in units of counts per second per diode per incident er) 309.75 423.35 P
0.87 (g s) 539.08 423.35 P
5 8 Q
0.69 (-1) 551.34 427.35 P
5 10 Q
0.1 (cm) 207 411.35 P
5 8 Q
0.08 (-2) 219.22 415.35 P
5 10 Q
0.1 ( \201) 225.88 411.35 P
5 8 Q
0.08 (-1) 235.71 415.35 P
5 10 Q
0.1 (. This leads to an expected count rate of) 242.37 411.35 P
0.1 (. An inte-) 519.74 411.35 P
0.59 (gration time of about 2.25 hours would lead to approximately 625 detected counts per) 207 399.35 P
1.34 (diode, or the required signal-to-noise of 25. This neglects the ef) 207 387.35 P
1.34 (fects of dark, which) 474.57 387.35 P
(should be an order) 207 375.35 T
(-of-magnitude below this count rate.) 280.95 375.35 T
487.72 590.85 534.96 603.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(V) 488.72 595.35 T
5 F
(1) 510.46 595.35 T
(2) 515.46 595.35 T
(.) 520.46 595.35 T
(8) 522.96 595.35 T
(9) 527.96 595.35 T
(=) 499.83 595.35 T
0 0 612 792 C
207 578.85 276.77 591.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(B) 213.96 583.35 T
(V) 230.07 583.35 T
5 F
(\320) 222.57 583.35 T
9 F
(\050) 209.67 583.35 T
(\051) 236.64 583.35 T
5 F
(0) 257.27 583.35 T
(.) 262.27 583.35 T
(0) 264.77 583.35 T
(3) 269.77 583.35 T
(=) 246.63 583.35 T
0 0 612 792 C
465.14 576.5 544.16 591.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(B) 472.09 583.35 T
(V) 488.2 583.35 T
5 F
(\320) 480.7 583.35 T
9 F
(\050) 467.8 583.35 T
(\051) 494.77 583.35 T
5 7 Q
(0) 500.15 580.25 T
5 10 Q
(0) 524.66 583.35 T
(.) 529.66 583.35 T
(2) 532.16 583.35 T
(4) 537.16 583.35 T
(\320) 519.28 583.35 T
(=) 508.65 583.35 T
0 0 612 792 C
225.04 566.85 301.51 579.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(E) 226.04 571.35 T
(B) 238.7 571.35 T
(V) 254.81 571.35 T
5 F
(\320) 247.31 571.35 T
9 F
(\050) 234.41 571.35 T
(\051) 261.38 571.35 T
5 F
(0) 282.01 571.35 T
(.) 287.01 571.35 T
(2) 289.51 571.35 T
(7) 294.51 571.35 T
(=) 271.37 571.35 T
0 0 612 792 C
446.4 566.85 523.02 579.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(3) 447.4 571.35 T
(.) 452.4 571.35 T
(1) 454.9 571.35 T
(0) 470.39 571.35 T
(.) 475.39 571.35 T
(2) 477.89 571.35 T
(7) 482.89 571.35 T
9 F
(\264) 462.4 571.35 T
5 F
(0) 503.52 571.35 T
(.) 508.52 571.35 T
(8) 511.02 571.35 T
(4) 516.02 571.35 T
(=) 492.88 571.35 T
0 0 612 792 C
336.24 552.5 387.36 567.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(V) 337.24 559.35 T
5 7 Q
(0) 343.73 556.25 T
5 10 Q
(1) 362.86 559.35 T
(2) 367.86 559.35 T
(.) 372.86 559.35 T
(0) 375.36 559.35 T
(5) 380.36 559.35 T
(=) 352.23 559.35 T
0 0 612 792 C
207 540.5 353.56 559.45 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(F) 208 547.35 T
5 7 Q
(5) 214.49 544.25 T
(5) 217.99 544.25 T
(0) 221.49 544.25 T
(0) 224.99 544.25 T
5 10 Q
(5) 244.12 547.35 T
(.) 249.12 547.35 T
(4) 251.62 547.35 T
(1) 267.11 547.35 T
(0) 272.11 547.35 T
5 7 Q
(1) 281.26 553.2 T
(4) 284.76 553.2 T
(\320) 277.49 553.2 T
5 10 Q
(e) 288.85 547.35 T
(r) 293.29 547.35 T
(g) 296.62 547.35 T
(s) 304.12 547.35 T
5 7 Q
(1) 312.15 553.2 T
(\320) 308.39 553.2 T
5 10 Q
(c) 316.24 547.35 T
(m) 320.68 547.35 T
5 7 Q
(2) 332.61 553.2 T
(\320) 328.84 553.2 T
5 10 Q
(\201) 336.7 547.35 T
5 7 Q
(1) 348.06 553.2 T
(\320) 344.3 553.2 T
9 10 Q
(\264) 259.12 547.35 T
5 F
(=) 233.49 547.35 T
0 0 612 792 C
263 506.5 339.28 521.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(F) 264 513.35 T
5 7 Q
(1) 270.49 510.25 T
(9) 273.99 510.25 T
(0) 277.49 510.25 T
(0) 280.99 510.25 T
6 10 Q
(F) 291.16 513.35 T
5 7 Q
(5) 297.65 510.25 T
(5) 301.15 510.25 T
(0) 304.65 510.25 T
(0) 308.15 510.25 T
9 10 Q
(\244) 286.99 513.35 T
5 F
(2) 327.28 513.35 T
(3) 332.28 513.35 T
(=) 316.65 513.35 T
0 0 612 792 C
399.94 506.5 459.04 521.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(T) 400.94 513.35 T
5 7 Q
(e) 406.88 510.25 T
(f) 409.99 510.25 T
(f) 412.32 510.25 T
5 10 Q
(2) 432.04 513.35 T
(5) 437.04 513.35 T
(0) 442.04 513.35 T
(0) 447.04 513.35 T
(0) 452.04 513.35 T
(=) 421.4 513.35 T
0 0 612 792 C
207 492.5 353.56 511.45 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(F) 208 499.35 T
5 7 Q
(1) 214.49 496.25 T
(9) 217.99 496.25 T
(0) 221.49 496.25 T
(0) 224.99 496.25 T
5 10 Q
(1) 244.12 499.35 T
(.) 249.12 499.35 T
(2) 251.62 499.35 T
(1) 267.11 499.35 T
(0) 272.11 499.35 T
5 7 Q
(1) 281.26 505.2 T
(2) 284.76 505.2 T
(\320) 277.49 505.2 T
5 10 Q
(e) 288.85 499.35 T
(r) 293.29 499.35 T
(g) 296.62 499.35 T
(s) 304.12 499.35 T
5 7 Q
(1) 312.15 505.2 T
(\320) 308.39 505.2 T
5 10 Q
(c) 316.24 499.35 T
(m) 320.68 499.35 T
5 7 Q
(2) 332.61 505.2 T
(\320) 328.84 505.2 T
5 10 Q
(\201) 336.7 499.35 T
5 7 Q
(1) 348.06 505.2 T
(\320) 344.3 505.2 T
9 10 Q
(\264) 259.12 499.35 T
5 F
(=) 233.49 499.35 T
0 0 612 792 C
320.64 480.85 368.42 499.2 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 321.64 485.35 T
(0) 326.64 485.35 T
5 7 Q
(0) 335.79 492.95 T
(.) 339.29 492.95 T
(4) 341.04 492.95 T
6 F
(A) 351.87 492.95 T
5 5 Q
(1) 356.42 490.7 T
(9) 358.92 490.7 T
(0) 361.42 490.7 T
(0) 363.92 490.7 T
9 7 Q
(\264) 346.28 492.95 T
5 F
(\320) 332.02 492.95 T
0 0 612 792 C
498.88 464.5 555.5 479.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(A) 499.88 471.35 T
5 7 Q
(1) 506.36 468.25 T
(9) 509.86 468.25 T
(0) 513.36 468.25 T
(0) 516.86 468.25 T
5 10 Q
(2) 536 471.35 T
(.) 541 471.35 T
(2) 543.5 471.35 T
(6) 548.5 471.35 T
(=) 525.36 471.35 T
0 0 612 792 C
434.76 452.85 545.2 469.45 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 435.76 457.35 T
(.) 440.76 457.35 T
(5) 443.26 457.35 T
(1) 458.75 457.35 T
(0) 463.75 457.35 T
5 7 Q
(1) 472.89 463.2 T
(3) 476.39 463.2 T
(\320) 469.13 463.2 T
5 10 Q
(e) 480.48 457.35 T
(r) 484.92 457.35 T
(g) 488.25 457.35 T
(s) 495.75 457.35 T
5 7 Q
(1) 503.79 463.2 T
(\320) 500.02 463.2 T
5 10 Q
(c) 507.88 457.35 T
(m) 512.32 457.35 T
5 7 Q
(2) 524.24 463.2 T
(\320) 520.48 463.2 T
5 10 Q
(\201) 528.33 457.35 T
5 7 Q
(1) 539.7 463.2 T
(\320) 535.93 463.2 T
9 10 Q
(\264) 450.76 457.35 T
0 0 612 792 C
241.53 416.5 309.75 435.45 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(S) 242.53 423.35 T
9 7 Q
(l) 247.91 420.25 T
5 10 Q
(5) 267.38 423.35 T
(.) 272.38 423.35 T
(2) 274.88 423.35 T
(1) 290.37 423.35 T
(0) 295.37 423.35 T
5 7 Q
(1) 300.75 429.2 T
(1) 304.25 429.2 T
9 10 Q
(\264) 282.38 423.35 T
5 F
(=) 256.75 423.35 T
0 0 612 792 C
404.92 406.85 519.74 423.45 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(7) 405.92 411.35 T
(.) 410.92 411.35 T
(8) 413.42 411.35 T
(1) 428.91 411.35 T
(0) 433.91 411.35 T
5 7 Q
(2) 443.05 417.2 T
(\320) 439.29 417.2 T
5 10 Q
(c) 447.14 411.35 T
(o) 451.58 411.35 T
(u) 456.58 411.35 T
(n) 461.58 411.35 T
(t) 466.58 411.35 T
(s) 469.36 411.35 T
(s) 475.75 411.35 T
5 7 Q
(1) 483.79 417.2 T
(\320) 480.02 417.2 T
5 10 Q
(d) 487.88 411.35 T
(i) 492.88 411.35 T
(o) 495.66 411.35 T
(d) 500.66 411.35 T
(e) 505.66 411.35 T
5 7 Q
(1) 514.24 417.2 T
(\320) 510.48 417.2 T
9 10 Q
(\264) 420.92 411.35 T
0 0 612 792 C
FMENDPAGE
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(Phase I: What the T) 189 736.18 T
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54 726.98 540 726.98 2 L
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54 74.02 540 74.02 2 L
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(32) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
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54 726.98 540 726.98 2 L
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% Frame ps_prolog 4.0, for use with Frame 4.0 products
% This ps_prolog file is Copyright (c) 1986-1993 Frame Technology
% Corporation. All rights reserved. This ps_prolog file may be
% freely copied and distributed in conjunction with documents created
% using FrameMaker, FrameBuilder and FrameViewer as long as this
% copyright notice is preserved.
%
% Frame products normally print colors as their true color on a color printer
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2 copy 0 get exch 0 get eqepsilon {
2 copy 1 get exch 1 get eqepsilon {
2 copy 2 get exch 2 get eqepsilon {
3 get exch 3 get eqepsilon
} {pop pop false} ifelse
}{pop pop false} ifelse
} {pop pop false} ifelse
} bind def
/FrameCmpColorsRGB {
2 copy 4 get exch 0 get eqepsilon {
2 copy 5 get exch 1 get eqepsilon {
6 get exch 2 get eqepsilon
}{pop pop false} ifelse
} {pop pop false} ifelse
} bind def
/RGBtoCMYK {
1 exch sub
3 1 roll
1 exch sub
3 1 roll
1 exch sub
3 1 roll
3 copy
2 copy
le { pop } { exch pop } ifelse
2 copy
le { pop } { exch pop } ifelse
dup dup dup
6 1 roll
4 1 roll
7 1 roll
sub
6 1 roll
sub
5 1 roll
sub
4 1 roll
} bind def
/CMYKtoRGB {
dup dup 4 -1 roll add
5 1 roll 3 -1 roll add
4 1 roll add
1 exch sub dup 0 lt {pop 0} if 3 1 roll
1 exch sub dup 0 lt {pop 0} if exch
1 exch sub dup 0 lt {pop 0} if exch
} bind def
/FrameSepInit {
1.0 RealSetgray
} bind def
/FrameSetSepColor {
/FrameSepBlue exch def
/FrameSepGreen exch def
/FrameSepRed exch def
/FrameSepBlack exch def
/FrameSepYellow exch def
/FrameSepMagenta exch def
/FrameSepCyan exch def
/FrameSepIs FMcustom def
setCurrentScreen
} bind def
/FrameSetCyan {
/FrameSepBlue 1.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 1.0 def
/FrameSepIs FMcyan def
setCurrentScreen
} bind def

/FrameSetMagenta {
/FrameSepBlue 1.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 1.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMmagenta def
setCurrentScreen
} bind def

/FrameSetYellow {
/FrameSepBlue 0.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 1.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMyellow def
setCurrentScreen
} bind def

/FrameSetBlack {
/FrameSepBlue 0.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 1.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMblack def
setCurrentScreen
} bind def

/FrameNoSep {
/FrameSepIs FMnone def
setCurrentScreen
} bind def
/FrameSetSepColors {
FrameDict begin
[ exch 1 add 1 roll ]
/FrameSepColors
exch def end
} bind def
/FrameColorInSepListCMYK {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsCMYK
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/FrameColorInSepListRGB {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsRGB
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/RealSetgray /setgray load def
/RealSetrgbcolor /setrgbcolor load def
/RealSethsbcolor /sethsbcolor load def
end
/setgray {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetgray }
{
FrameSepIs FMblack eq
{ RealSetgray }
{ FrameSepIs FMcustom eq
FrameSepRed 0 eq and
FrameSepGreen 0 eq and
FrameSepBlue 0 eq and {
RealSetgray
} {
1 RealSetgray pop
} ifelse
} ifelse
} ifelse
end
} bind def
/setrgbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetrgbcolor }
{
3 copy [ 4 1 roll ]
FrameColorInSepListRGB
{
FrameSepBlue eq exch
FrameSepGreen eq and exch
FrameSepRed eq and
{ 0 } { 1 } ifelse
}
{
FMPColor {
RealSetrgbcolor
currentcmykcolor
} {
RGBtoCMYK
} ifelse
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
RealSetgray
}
ifelse
end
} bind def
/sethsbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSethsbcolor }
{
RealSethsbcolor
currentrgbcolor
setrgbcolor
}
ifelse
end
} bind def
FrameDict begin
/setcmykcolor where {
pop /RealSetcmykcolor /setcmykcolor load def
} {
/RealSetcmykcolor {
4 1 roll
3 { 3 index add 0 max 1 min 1 exch sub 3 1 roll} repeat
setrgbcolor pop
} bind def
} ifelse
userdict /setcmykcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetcmykcolor }
{
4 copy [ 5 1 roll ]
FrameColorInSepListCMYK
{
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
{ 0 } { 1 } ifelse
}
{
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
RealSetgray
}
ifelse
end
} bind put
FMLevel1 not {

/patProcDict 5 dict dup begin
<0f1e3c78f0e1c387> { 3 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<0f87c3e1f0783c1e> { 3 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
<8142241818244281> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-1 -1 moveto 9 9 lineto stroke } bind def
<03060c183060c081> { 1 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<8040201008040201> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
end def
/patDict 15 dict dup begin
/PatternType 1 def
/PaintType 2 def
/TilingType 3 def
/BBox [ 0 0 8 8 ] def
/XStep 8 def
/YStep 8 def
/PaintProc {
begin
patProcDict bstring known {
patProcDict bstring get exec
} {
8 8 true [1 0 0 -1 0 8] bstring imagemask
} ifelse
end
} bind def
end def
} if
/combineColor {
FrameSepIs FMnone eq
{
graymode FMLevel1 or not {

[/Pattern [/DeviceCMYK]] setcolorspace
FrameCurColors 0 4 getinterval aload pop FrameCurPat setcolor
} {
FrameCurColors 3 get 1.0 ge {
FrameCurGray RealSetgray
} {
FMPColor graymode and {
0 1 3 {
FrameCurColors exch get
1 FrameCurGray sub mul
} for
RealSetcmykcolor
} {
4 1 6 {
FrameCurColors exch get
graymode {
1 exch sub 1 FrameCurGray sub mul 1 exch sub
} {
1.0 lt {FrameCurGray} {1} ifelse
} ifelse
} for
RealSetrgbcolor
} ifelse
} ifelse
} ifelse
} {
FrameCurColors 0 4 getinterval aload
FrameColorInSepListCMYK {
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
FrameSepIs FMcustom eq and
{ FrameCurGray } { 1 } ifelse
} {
FrameSepIs FMblack eq
{FrameCurGray 1.0 exch sub mul 1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop FrameCurGray 1.0 exch sub mul 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
graymode FMLevel1 or not {

[/Pattern [/DeviceGray]] setcolorspace
FrameCurPat setcolor
} {
graymode not FMLevel1 and {

dup 1 lt {pop FrameCurGray} if
} if
RealSetgray
} ifelse
} ifelse
} bind def
/savematrix {
orgmatrix currentmatrix pop
} bind def
/restorematrix {
orgmatrix setmatrix
} bind def
/dmatrix matrix def
/dpi 72 0 dmatrix defaultmatrix dtransform
dup mul exch dup mul add sqrt def

/freq dpi dup 72 div round dup 0 eq {pop 1} if 8 mul div def
/sangle 1 0 dmatrix defaultmatrix dtransform exch atan def
/dpiranges [ 2540 2400 1693 1270 1200 635 600 0 ] def
/CMLowFreqs [ 100.402 94.8683 89.2289 100.402 94.8683 66.9349 63.2456 47.4342 ] def
/YLowFreqs [ 95.25 90.0 84.65 95.25 90.0 70.5556 66.6667 50.0 ] def
/KLowFreqs [ 89.8026 84.8528 79.8088 89.8026 84.8528 74.8355 70.7107 53.033 ] def
/CLowAngles [ 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 ] def
/MLowAngles [ 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 ] def
/YLowTDot [ true true false true true false false false ] def
/CMHighFreqs [ 133.87 126.491 133.843 108.503 102.523 100.402 94.8683 63.2456 ] def
/YHighFreqs [ 127.0 120.0 126.975 115.455 109.091 95.25 90.0 60.0 ] def
/KHighFreqs [ 119.737 113.137 119.713 128.289 121.218 89.8026 84.8528 63.6395 ] def
/CHighAngles [ 71.5651 71.5651 71.5651 70.0169 70.0169 71.5651 71.5651 71.5651 ] def
/MHighAngles [ 18.4349 18.4349 18.4349 19.9831 19.9831 18.4349 18.4349 18.4349 ] def
/YHighTDot [ false false true false false true true false ] def
/PatFreq [ 10.5833 10.0 9.4055 10.5833 10.0 10.5833 10.0 9.375 ] def
/screenIndex {
0 1 dpiranges length 1 sub { dup dpiranges exch get 1 sub dpi le {exit} {pop} ifelse } for
} bind def
/getCyanScreen {
FMUseHighFrequencyScreens { CHighAngles CMHighFreqs} {CLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getMagentaScreen {
FMUseHighFrequencyScreens { MHighAngles CMHighFreqs } {MLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getYellowScreen {
FMUseHighFrequencyScreens { YHighTDot YHighFreqs} { YLowTDot YLowFreqs } ifelse
screenIndex dup 3 1 roll get 3 1 roll get { 3 div
{2 { 1 add 2 div 3 mul dup floor sub 2 mul 1 sub exch} repeat
FMSpotFunction } } {/FMSpotFunction load } ifelse
0.0 exch
} bind def
/getBlackScreen {
FMUseHighFrequencyScreens { KHighFreqs } { KLowFreqs } ifelse
screenIndex get 45.0 /FMSpotFunction load
} bind def
/getSpotScreen {
getBlackScreen
} bind def
/getCompositeScreen {
getBlackScreen
} bind def
/FMSetScreen
FMLevel1 { /setscreen load
}{ {
8 dict begin
/HalftoneType 1 def
/SpotFunction exch def
/Angle exch def
/Frequency exch def
/AccurateScreens FMUseAcccurateScreens def
currentdict end sethalftone
} bind } ifelse
def
/setDefaultScreen {
FMPColor {
orgrxfer cvx orggxfer cvx orgbxfer cvx orgxfer cvx setcolortransfer
}
{
orgxfer cvx settransfer
} ifelse
orgfreq organgle orgproc cvx setscreen
} bind def
/setCurrentScreen {
FrameSepIs FMnone eq {
FMUseDefaultNoSeparationScreen {
setDefaultScreen
} {
getCompositeScreen FMSetScreen
} ifelse
} {
FrameSepIs FMcustom eq {
FMUseDefaultSpotSeparationScreen {
setDefaultScreen
} {
getSpotScreen FMSetScreen
} ifelse
} {
FMUseDefaultProcessSeparationScreen {
setDefaultScreen
} {
FrameSepIs FMcyan eq {
getCyanScreen FMSetScreen
} {
FrameSepIs FMmagenta eq {
getMagentaScreen FMSetScreen
} {
FrameSepIs FMyellow eq {
getYellowScreen FMSetScreen
} {
getBlackScreen FMSetScreen
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} bind def
end
/gstring FMLOCAL
/gfile FMLOCAL
/gindex FMLOCAL
/orgrxfer FMLOCAL
/orggxfer FMLOCAL
/orgbxfer FMLOCAL
/orgxfer FMLOCAL
/orgproc FMLOCAL
/orgrproc FMLOCAL
/orggproc FMLOCAL
/orgbproc FMLOCAL
/organgle FMLOCAL
/orgrangle FMLOCAL
/orggangle FMLOCAL
/orgbangle FMLOCAL
/orgfreq FMLOCAL
/orgrfreq FMLOCAL
/orggfreq FMLOCAL
/orgbfreq FMLOCAL
/yscale FMLOCAL
/xscale FMLOCAL
/edown FMLOCAL
/manualfeed FMLOCAL
/paperheight FMLOCAL
/paperwidth FMLOCAL
/FMDOCUMENT {
array /FMfonts exch def
/#copies exch def
FrameDict begin
0 ne /manualfeed exch def
/paperheight exch def
/paperwidth exch def
0 ne /FrameNegative exch def
0 ne /edown exch def
/yscale exch def
/xscale exch def
FMLevel1 {
manualfeed {setmanualfeed} if
/FMdicttop countdictstack 1 add def
/FMoptop count def
% setpapername
% manualfeed {true} {papersize} ifelse
% {manualpapersize} {false} ifelse
% {desperatepapersize} {false} ifelse
% { (Can't select requested paper size for Frame print job!) FMFAILURE } if
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
}
{{1 dict dup /PageSize [paperwidth paperheight]put setpagedevice}stopped
{ (Can't select requested paper size for Frame print job!) FMFAILURE } if
{1 dict dup /ManualFeed manualfeed put setpagedevice } stopped pop }
ifelse

FMPColor {
currentcolorscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def
cvlit /orgbproc exch def
/orgbangle exch def
/orgbfreq exch def
cvlit /orggproc exch def
/orggangle exch def
/orggfreq exch def
cvlit /orgrproc exch def
/orgrangle exch def
/orgrfreq exch def
currentcolortransfer
FrameNegative {
1 1 4 {
pop { 1 exch sub } concatprocs 4 1 roll
} for
4 copy
setcolortransfer
} if
cvlit /orgxfer exch def
cvlit /orgbxfer exch def
cvlit /orggxfer exch def
cvlit /orgrxfer exch def
} {
currentscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def

currenttransfer
FrameNegative {
{ 1 exch sub } concatprocs
dup settransfer
} if
cvlit /orgxfer exch def
} ifelse
end
} def
/pagesave FMLOCAL
/orgmatrix FMLOCAL
/landscape FMLOCAL
/pwid FMLOCAL
/FMBEGINPAGE {
FrameDict begin
/pagesave save def
3.86 setmiterlimit
/landscape exch 0 ne def
landscape {
90 rotate 0 exch dup /pwid exch def neg translate pop
}{
pop /pwid exch def
} ifelse
edown { [-1 0 0 1 pwid 0] concat } if
0 0 moveto paperwidth 0 lineto paperwidth paperheight lineto
0 paperheight lineto 0 0 lineto 1 setgray fill
xscale yscale scale
/orgmatrix matrix def
gsave
} def
/FMENDPAGE {
grestore
pagesave restore
end
showpage
} def
/FMFONTDEFINE {
FrameDict begin
findfont
ReEncode
1 index exch
definefont
FMfonts 3 1 roll
put
end
} def
/FMFILLS {
FrameDict begin dup
array /fillvals exch def
dict /patCache exch def
end
} def
/FMFILL {
FrameDict begin
fillvals 3 1 roll put
end
} def
/FMNORMALIZEGRAPHICS {
newpath
0.0 0.0 moveto
1 setlinewidth
0 setlinecap
0 0 0 sethsbcolor
0 setgray
} bind def
/fx FMLOCAL
/fy FMLOCAL
/fh FMLOCAL
/fw FMLOCAL
/llx FMLOCAL
/lly FMLOCAL
/urx FMLOCAL
/ury FMLOCAL
/FMBEGINEPSF {
end
/FMEPSF save def
/showpage {} def
% See Adobe's "PostScript Language Reference Manual, 2nd Edition", page 714.
% "...the following operators MUST NOT be used in an EPS file:" (emphasis ours)
/banddevice {(banddevice) FMBADEPSF} def
/clear {(clear) FMBADEPSF} def
/cleardictstack {(cleardictstack) FMBADEPSF} def
/copypage {(copypage) FMBADEPSF} def
/erasepage {(erasepage) FMBADEPSF} def
/exitserver {(exitserver) FMBADEPSF} def
/framedevice {(framedevice) FMBADEPSF} def
/grestoreall {(grestoreall) FMBADEPSF} def
/initclip {(initclip) FMBADEPSF} def
/initgraphics {(initgraphics) FMBADEPSF} def
/initmatrix {(initmatrix) FMBADEPSF} def
/quit {(quit) FMBADEPSF} def
/renderbands {(renderbands) FMBADEPSF} def
/setglobal {(setglobal) FMBADEPSF} def
/setpagedevice {(setpagedevice) FMBADEPSF} def
/setshared {(setshared) FMBADEPSF} def
/startjob {(startjob) FMBADEPSF} def
/lettertray {(lettertray) FMBADEPSF} def
/letter {(letter) FMBADEPSF} def
/lettersmall {(lettersmall) FMBADEPSF} def
/11x17tray {(11x17tray) FMBADEPSF} def
/11x17 {(11x17) FMBADEPSF} def
/ledgertray {(ledgertray) FMBADEPSF} def
/ledger {(ledger) FMBADEPSF} def
/legaltray {(legaltray) FMBADEPSF} def
/legal {(legal) FMBADEPSF} def
/statementtray {(statementtray) FMBADEPSF} def
/statement {(statement) FMBADEPSF} def
/executivetray {(executivetray) FMBADEPSF} def
/executive {(executive) FMBADEPSF} def
/a3tray {(a3tray) FMBADEPSF} def
/a3 {(a3) FMBADEPSF} def
/a4tray {(a4tray) FMBADEPSF} def
/a4 {(a4) FMBADEPSF} def
/a4small {(a4small) FMBADEPSF} def
/b4tray {(b4tray) FMBADEPSF} def
/b4 {(b4) FMBADEPSF} def
/b5tray {(b5tray) FMBADEPSF} def
/b5 {(b5) FMBADEPSF} def
FMNORMALIZEGRAPHICS
[/fy /fx /fh /fw /ury /urx /lly /llx] {exch def} forall
fx fw 2 div add fy fh 2 div add translate
rotate
fw 2 div neg fh 2 div neg translate
fw urx llx sub div fh ury lly sub div scale
llx neg lly neg translate
/FMdicttop countdictstack 1 add def
/FMoptop count def
} bind def
/FMENDEPSF {
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
FMEPSF restore
FrameDict begin
} bind def
FrameDict begin
/setmanualfeed {
%%BeginFeature *ManualFeed True
statusdict /manualfeed true put
%%EndFeature
} bind def
/max {2 copy lt {exch} if pop} bind def
/min {2 copy gt {exch} if pop} bind def
/inch {72 mul} def
/pagedimen {
paperheight sub abs 16 lt exch
paperwidth sub abs 16 lt and
{/papername exch def} {pop} ifelse
} bind def
/papersizedict FMLOCAL
/setpapername {
/papersizedict 14 dict def
papersizedict begin
/papername /unknown def
/Letter 8.5 inch 11.0 inch pagedimen
/LetterSmall 7.68 inch 10.16 inch pagedimen
/Tabloid 11.0 inch 17.0 inch pagedimen
/Ledger 17.0 inch 11.0 inch pagedimen
/Legal 8.5 inch 14.0 inch pagedimen
/Statement 5.5 inch 8.5 inch pagedimen
/Executive 7.5 inch 10.0 inch pagedimen
/A3 11.69 inch 16.5 inch pagedimen
/A4 8.26 inch 11.69 inch pagedimen
/A4Small 7.47 inch 10.85 inch pagedimen
/B4 10.125 inch 14.33 inch pagedimen
/B5 7.16 inch 10.125 inch pagedimen
end
} bind def
/papersize {
papersizedict begin
/Letter {lettertray letter} def
/LetterSmall {lettertray lettersmall} def
/Tabloid {11x17tray 11x17} def
/Ledger {ledgertray ledger} def
/Legal {legaltray legal} def
/Statement {statementtray statement} def
/Executive {executivetray executive} def
/A3 {a3tray a3} def
/A4 {a4tray a4} def
/A4Small {a4tray a4small} def
/B4 {b4tray b4} def
/B5 {b5tray b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
statusdict begin stopped end
} bind def
/manualpapersize {
papersizedict begin
/Letter {letter} def
/LetterSmall {lettersmall} def
/Tabloid {11x17} def
/Ledger {ledger} def
/Legal {legal} def
/Statement {statement} def
/Executive {executive} def
/A3 {a3} def
/A4 {a4} def
/A4Small {a4small} def
/B4 {b4} def
/B5 {b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
stopped
} bind def
/desperatepapersize {
statusdict /setpageparams known
{
paperwidth paperheight 0 1
statusdict begin
{setpageparams} stopped
end
} {true} ifelse
} bind def
/DiacriticEncoding [
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /space /exclam /quotedbl
/numbersign /dollar /percent /ampersand /quotesingle /parenleft
/parenright /asterisk /plus /comma /hyphen /period /slash /zero /one
/two /three /four /five /six /seven /eight /nine /colon /semicolon
/less /equal /greater /question /at /A /B /C /D /E /F /G /H /I /J /K
/L /M /N /O /P /Q /R /S /T /U /V /W /X /Y /Z /bracketleft /backslash
/bracketright /asciicircum /underscore /grave /a /b /c /d /e /f /g /h
/i /j /k /l /m /n /o /p /q /r /s /t /u /v /w /x /y /z /braceleft /bar
/braceright /asciitilde /.notdef /Adieresis /Aring /Ccedilla /Eacute
/Ntilde /Odieresis /Udieresis /aacute /agrave /acircumflex /adieresis
/atilde /aring /ccedilla /eacute /egrave /ecircumflex /edieresis
/iacute /igrave /icircumflex /idieresis /ntilde /oacute /ograve
/ocircumflex /odieresis /otilde /uacute /ugrave /ucircumflex
/udieresis /dagger /.notdef /cent /sterling /section /bullet
/paragraph /germandbls /registered /copyright /trademark /acute
/dieresis /.notdef /AE /Oslash /.notdef /.notdef /.notdef /.notdef
/yen /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/ordfeminine /ordmasculine /.notdef /ae /oslash /questiondown
/exclamdown /logicalnot /.notdef /florin /.notdef /.notdef
/guillemotleft /guillemotright /ellipsis /.notdef /Agrave /Atilde
/Otilde /OE /oe /endash /emdash /quotedblleft /quotedblright
/quoteleft /quoteright /.notdef /.notdef /ydieresis /Ydieresis
/fraction /currency /guilsinglleft /guilsinglright /fi /fl /daggerdbl
/periodcentered /quotesinglbase /quotedblbase /perthousand
/Acircumflex /Ecircumflex /Aacute /Edieresis /Egrave /Iacute
/Icircumflex /Idieresis /Igrave /Oacute /Ocircumflex /.notdef /Ograve
/Uacute /Ucircumflex /Ugrave /dotlessi /circumflex /tilde /macron
/breve /dotaccent /ring /cedilla /hungarumlaut /ogonek /caron
] def
/ReEncode {
dup
length
dict begin
{
1 index /FID ne
{def}
{pop pop} ifelse
} forall
0 eq {/Encoding DiacriticEncoding def} if
currentdict
end
} bind def
FMPColor

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setscreen
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F
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RF
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RF
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RF
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grestore
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400 ms
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/BITMAPCOLOR {
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3 index 2 div add exch
4 index 2 div add exch
translate
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/h exch def /w exch def
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FMLevel1 {
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/is w d wbytes string def
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{cf is readhexstring pop} {is} {is} true 3 colorimage
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7 dict dup begin
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/BITMAPCOLORc {
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3 index 2 div add exch
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translate
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translate
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sl lb lt {lb ms} if
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FMLevel1 {
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{ip} {is} {is} true 3 colorimage
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3 index 2 div add exch
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%%EndProlog
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72 750.02 558 750.02 2 L
2 H
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72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
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0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (33) 546.88 60.29 P
72 750.02 558 750.02 2 L
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1 12 Q
1.2 (Chapter 4) 72 677 S
2 24 Q
-0.48 (Y) 207 677 S
-0.48 (our Phase II Pr) 219.86 677 S
-0.48 (oposal) 359.55 677 S
3 12 Q
(4.1) 144 419 T
( Acquisitions) 164.02 419 T
4 F
( 35) 505.32 419 T
3 10 Q
(4.1.1) 162 402.33 T
( Initial Pointing) 187.02 402.33 T
4 F
( 35) 508.1 402.33 T
3 F
(4.1.2) 162 386.33 T
( Interactive Acquisitions) 187.02 386.33 T
4 F
( 35) 508.1 386.33 T
3 F
(4.1.3) 162 370.33 T
( Early Acquisitions) 187.02 370.33 T
4 F
( 36) 508.1 370.33 T
3 F
(4.1.4) 162 354.33 T
( Onboard Acquisitions) 187.02 354.33 T
4 F
( 36) 508.1 354.33 T
3 F
(4.1.5) 162 338.33 T
( Special Onboard Strategies for Special Situations) 187.02 338.33 T
4 F
( 38) 508.1 338.33 T
3 F
(4.1.6) 162 322.33 T
( MAPs) 187.02 322.33 T
4 F
( 40) 508.1 322.33 T
3 F
(4.1.7) 162 306.33 T
( Acquisition Parameters \321 A Summary) 187.02 306.33 T
4 F
( 40) 508.1 306.33 T
3 12 Q
(4.2) 144 289 T
( Image Mode) 164.02 289 T
4 F
( 42) 505.32 289 T
3 10 Q
(4.2.1) 162 272.33 T
( Image Mode Parameters) 187.02 272.33 T
4 F
( 42) 508.1 272.33 T
3 F
(4.2.2) 162 256.33 T
( The GHRS as a Slitless Spectrograph) 187.02 256.33 T
4 F
( 43) 508.1 256.33 T
3 12 Q
(4.3) 144 239 T
( Accumulation Mode) 164.02 239 T
4 F
( 43) 505.32 239 T
3 10 Q
(4.3.1) 162 222.33 T
( Optimizing Data Quality) 187.02 222.33 T
4 F
( 43) 508.1 222.33 T
3 F
(4.3.2) 162 206.33 T
( Summary of Accumulation Mode Parameters) 187.02 206.33 T
4 F
( 44) 508.1 206.33 T
3 F
(4.3.3) 162 190.33 T
( WSCAN mode) 187.02 190.33 T
4 F
( 45) 508.1 190.33 T
3 F
(4.3.4) 162 174.33 T
( OSCAN mode) 187.02 174.33 T
4 F
( 45) 508.1 174.33 T
3 12 Q
(4.4) 144 157 T
( Rapid Readout Mode) 164.02 157 T
4 F
( 45) 505.32 157 T
3 F
(4.5) 144 139 T
( The Precision and Accuracy of Standard Calibrations) 164.02 139 T
4 F
( 46) 505.32 139 T
3 F
(4.6) 144 121 T
( Other Considerations) 164.02 121 T
4 F
( 47) 505.32 121 T
FMENDPAGE
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0 0 0 1 0 0 0 K
N
0 9 Q
(Y) 189 736.18 T
(our Phase II Proposal) 194.34 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(34) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
5 F
1.64 (This chapter supplements the) 189 560.33 P
6 F
1.64 ( Phase II Pr) 310.86 560.33 P
1.64 (oposal Instructions) 364.02 560.33 P
5 F
1.64 ( that will be issued for) 442.62 560.33 P
-0 (Cycle 5. Y) 189 548.33 P
-0 (ou may also wish to consult) 231.05 548.33 P
6 F
-0 ( Phase II Instructions for the Solar System T) 342.43 548.33 P
-0 (ar) 519.26 548.33 P
-0 (get) 527.78 548.33 P
(List) 189 536.33 T
5 F
(if your program is to observe solar system objects.) 206.51 536.33 T
0.27 (Most users of the GHRS will \336nd that a simple sequence of commands will work most) 189 516.33 P
(of the time to obtain the data they desire:) 189 504.33 T
7 11 Q
(\245) 189 486.33 T
8 10 Q
(ACQ) 203.4 486.33 T
5 F
( in LSA with) 221.4 486.33 T
8 F
(BRIGHT=RETURN) 275.85 486.33 T
5 F
(.) 353.85 486.33 T
7 11 Q
(\245) 189 471.33 T
8 10 Q
-0.31 (ACQ/PEAKUP) 203.4 471.33 P
5 F
-0.13 ( to center star in LSA or SSA, whichever is appropriate to the science) 263.4 471.33 P
(observations that follow) 203.4 459.33 T
(.) 299.41 459.33 T
7 11 Q
(\245) 189 444.33 T
8 10 Q
(IMAGE) 203.4 444.33 T
5 F
(, if you wish to verify tar) 233.4 444.33 T
(get centering or to obtain an image of the object.) 332.93 444.33 T
7 11 Q
(\245) 189 429.33 T
5 10 Q
(W) 203.4 429.33 T
(avelength calibration exposure, if desired.) 212.04 429.33 T
7 11 Q
(\245) 189 414.33 T
8 10 Q
0.94 (ACCUM) 203.4 414.33 P
5 F
0.39 (s at wavelengths of interest.) 233.4 414.33 P
8 F
0.94 (NO) 349.23 414.33 P
0.94 (GAP) 364.12 414.33 P
5 F
0.39 ( is recommended as a Special Require-) 382.12 414.33 P
1.01 (ment in order to ensure the) 203.4 402.33 P
8 F
2.43 (PEAKUP) 319.45 402.33 P
5 F
1.01 ( operation is properly applied to the spectro-) 355.45 402.33 P
(scopic exposures.) 203.4 390.33 T
7 11 Q
(\245) 189 375.33 T
8 10 Q
(ACQ/PEAKUP) 203.4 375.33 T
5 F
( in the SSA if the previous observation was in the LSA.) 263.4 375.33 T
7 11 Q
(\245) 189 360.33 T
8 10 Q
(ACCUM) 203.4 360.33 T
5 F
(s for that dif) 233.4 360.33 T
(ferent aperture, again with) 282.38 360.33 T
8 F
(NO) 390.4 360.33 T
(GAP) 404.9 360.33 T
5 F
(.) 421.79 360.33 T
7 11 Q
(\245) 189 345.33 T
5 10 Q
(Repeat the above as needed for more stars.) 203.4 345.33 T
1.25 (T) 189 325.33 P
1.25 (ar) 194.41 325.33 P
1.25 (get acquisitions always take place with the LSA because the SSA is too small to) 202 325.33 P
0.57 (enable a \336eld to be mapped ef) 189 313.33 P
0.57 (fectively) 312.23 313.33 P
0.57 (. Additional) 346.57 313.33 P
8 F
1.38 (ACCUM) 397.99 313.33 P
5 F
0.57 (s may be speci\336ed after the) 427.99 313.33 P
(\336rst so as to obtain spectra at several wavelengths.) 189 301.33 T
0.67 (One task of the Instrument Scientists at STScI is to check the feasibility of successful) 189 281.33 P
1.18 (proposals after the Phase II proposals have been submitted.) 189 269.33 P
9 F
1.18 ( It is in your inter) 435.33 269.33 P
1.18 (est to) 516.33 269.33 P
-0.19 (help us with that by using standard and consistent formats for the Phase II pr) 189 257.33 P
-0.19 (opos-) 517.22 257.33 P
2.31 (als) 189 245.33 P
5 F
2.31 ( because that can greatly reduce ambiguity about the intentions of the General) 200.67 245.33 P
(Observer) 189 233.33 T
(. W) 225.1 233.33 T
(e suggest the following:) 238.74 233.33 T
7 11 Q
(\245) 189 215.33 T
5 10 Q
2.2 (Follow the examples in the next chapter) 203.4 215.33 P
2.2 (. The examples usually specify all the) 376.01 215.33 P
-0.03 (defaults for clarity) 203.4 203.33 P
-0.03 (, which is not strictly necessary) 276.56 203.33 P
-0.03 (, but, like comments in a computer) 401.3 203.33 P
2.56 (program, can help to con\336rm that a procedure conforms to the intents of the) 203.4 191.33 P
(observer) 203.4 179.33 T
(.) 237.28 179.33 T
7 11 Q
(\245) 189 164.33 T
5 10 Q
0.55 (Although the submission software does not strictly require it, we ask that you give) 203.4 164.33 P
0.53 (the commands in the order just listed: First the acquisition, then embellishments to) 203.4 152.33 P
-0.18 (the acquisition \050) 203.4 140.33 P
8 F
-0.44 (PEAKUP) 267.47 140.33 P
5 F
-0.18 (,) 302.36 140.33 P
8 F
-0.44 (OFFSET) 307.18 140.33 P
5 F
-0.18 (, etc.\051, then an) 342.44 140.33 P
8 F
-0.44 (IMAGE) 400.86 140.33 P
5 F
-0.18 ( and/or wavelength calibra-) 430.86 140.33 P
2.53 (tion exposure \050if desired\051, and then the actual science observation \050usually an) 203.4 128.33 P
8 F
(ACCUM) 203.4 116.33 T
5 F
(\051.) 233.4 116.33 T
54 87.98 540 686.02 C
108 576 540 679.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
108 576 540 679.02 R
5 X
0 0 0 1 0 0 0 K
V
117.83 586.52 530.17 669.18 R
7 X
V
10 14 Q
0 X
(CAUTION) 292.92 651.85 T
11 11 Q
1.54 (The pr) 123.59 632.85 P
1.54 (ocedur) 157.49 632.85 P
1.54 (es for cr) 196.45 632.85 P
1.54 (eating a Phase II pr) 241.39 632.85 P
1.54 (oposal ar) 349.84 632.85 P
1.54 (e being r) 401.1 632.85 P
1.54 (eviewed and) 451.64 632.85 P
2.93 (r) 123.59 619.85 P
2.93 (evised as this is written. W) 126.86 619.85 P
2.93 (e str) 275.37 619.85 P
2.93 (ongly r) 299.76 619.85 P
2.93 (ecommend that users check the) 338.42 619.85 P
1.36 (Phase) 123.59 606.85 P
1.36 (II documentation car) 158.79 606.85 P
1.36 (efully. W) 274.29 606.85 P
1.36 (e also r) 319.38 606.85 P
1.36 (ecommend checking on STEIS) 359.8 606.85 P
(at that time for a r) 123.59 593.85 T
(evised version of this Instrument Handbook.) 219.9 593.85 T
117.83 586.52 530.17 669.18 R
1 H
2 Z
N
108.5 576.5 539.5 678.52 R
0 Z
N
54 87.98 540 686.02 C
0 0 612 792 C
FMENDPAGE
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[ 0 0 1 0 1 1 0]
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FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (35) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Y) 207 736.18 T
(our Phase II Proposal) 212.34 736.18 T
7 11 Q
(\245) 207 679.35 T
5 10 Q
0.71 (Add plenty of comment lines \050RPSS imposes a limit\051 to explain what you want to) 221.4 679.35 P
0.19 (have happen so that we can see whether or not your proposal actually accomplishes) 221.4 667.35 P
(that. In particular) 221.4 655.35 T
(, please explain brie\337y how the exposure time was determined.) 290.15 655.35 T
72 612.02 558 615.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 613.52 558 613.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 613.52 198 613.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(4.1) 181.32 619.02 T
(Acquisitions) 207 619.02 T
5 10 Q
0.21 (Most objects observed with the GHRS are point sources \050stars\051, and the majority of the) 207 595.35 P
0.53 (remainder can be observed by \336rst centering on a nearby point source and then of) 207 583.35 P
0.53 (fset-) 540.23 583.35 P
0 (ting to the object of interest. Point sources with accurate coordinates are very) 207 571.35 P
0 (, very easy) 514.95 571.35 P
-0.02 (to acquire with the GHRS: just specify) 207 559.35 P
8 F
-0.05 (ACQ) 364.35 559.35 P
5 F
-0.02 ( with) 382.35 559.35 P
8 F
-0.05 (BRIGHT=RETURN) 405.09 559.35 P
5 F
-0.02 ( to have the instru-) 483.09 559.35 P
(ment automatically center on the brightest object found within the LSA.) 207 547.35 T
0 F
(4.1.1) 175.76 517.35 T
(Initial Pointing) 207 517.35 T
5 F
0.17 (A blind pointing with) 207 497.35 P
6 F
0.17 (HST) 296.6 497.35 P
5 F
0.17 ( is likely to place the object of interest within 2 arcsec of the) 314.38 497.35 P
-0 (center of the aperture. That accuracy is limited in part by the quality of coordinates pro-) 207 485.35 P
0.72 (vided by users and partly by errors in the positions of the FGSs relative to the GHRS) 207 473.35 P
0.02 (apertures \050see the) 207 461.35 P
6 F
0.02 ( FOS Instrument Handbook) 277.01 461.35 P
5 F
0.02 ( for a discussion of pointing errors\051. Using) 387.89 461.35 P
0.23 (J2000 coordinates tied to the GSC reference frame can help to reduce the possibility of) 207 449.35 P
1.05 (a failed acquisition. And don\325) 207 437.35 P
1.05 (t for) 330.16 437.35 P
1.05 (get to include proper motions if appropriate and to) 347.97 437.35 P
(check the equinox and epoch of astrometric quantities.) 207 425.35 T
0 F
(4.1.2) 175.76 395.35 T
(Interactive Acquisitions) 207 395.35 T
5 F
0.26 (W) 207 375.35 P
0.26 (e discuss interactive acquisitions \050) 215.64 375.35 P
8 F
0.62 (INT) 353.31 375.35 P
0.62 (ACQ) 374.07 375.35 P
5 F
0.26 (\051 \336rst in the hope of dissuading you from) 392.07 375.35 P
0.78 (using that capability) 207 363.35 P
0.78 (. An) 289.01 363.35 P
8 F
1.86 (INT) 310.29 363.35 P
1.86 (ACQ) 331.56 363.35 P
5 F
0.78 ( requires real-time contact between the ground and) 349.56 363.35 P
6 F
-0.14 (HST) 207 351.35 P
5 F
-0.14 (. Real-time contact is a limited and expensive resource that should only be used as a) 224.04 351.35 P
0.29 (last resort. In almost all cases where an onboard acquisition will not work \050because the) 207 339.35 P
0.52 (object is in a crowded \336eld, or is variable, or is a moving tar) 207 327.35 P
0.52 (get\051, it is suf) 454.45 327.35 P
0.52 (\336cient to use) 505.84 327.35 P
8 F
3.29 (EARLY) 207 315.35 P
3.29 (ACQ) 240.87 315.35 P
5 F
1.37 ( to get a WFPC2 or FOC image a few weeks in advance of the GHRS) 258.87 315.35 P
-0.22 (observation. The image can then be analyzed to pinpoint the source to be observed with-) 207 303.35 P
0.54 (out requiring real-time contact.) 207 291.35 P
8 F
1.3 (INT) 336.08 291.35 P
1.3 (ACQ) 357.13 291.35 P
5 F
0.54 ( may be needed in a few instances where the) 375.13 291.35 P
0.78 (object changes in its ultraviolet brightness unpredictably) 207 279.35 P
0.78 (. W) 437.12 279.35 P
0.78 (e suggest that you consult) 451.55 279.35 P
(with us before requesting) 207 267.35 T
8 F
(INT) 310.87 267.35 T
(ACQ) 331.37 267.35 T
5 F
(.) 349.37 267.35 T
0.69 (If an interactive acquisition with the GHRS has been speci\336ed, a spiral search will be) 207 247.35 P
0.26 (run after) 207 235.35 P
6 F
0.26 (HST) 244.16 235.35 P
5 F
0.26 ( makes its initial pointing. A map of the LSA is made at each dwell point) 261.94 235.35 P
1.5 (and each map is then downlinked to STScI in real time and may be viewed almost) 207 223.35 P
-0.12 (immediately in OSS. After the spiral is complete, the telescope remains at its \336nal dwell) 207 211.35 P
0.59 (point, awaiting instructions. The \336nal 9 \050or 25\051 maps are assembled into a mosaic and) 207 199.35 P
0.82 (displayed for the observer to identify the tar) 207 187.35 P
0.82 (get, either from a cursor position or from) 388.38 187.35 P
0.05 (calculation of a centroid. The motion needed to center the speci\336ed position in the LSA) 207 175.35 P
-0.24 (is computed and uplinked to) 207 163.35 P
6 F
-0.24 (HST) 321.65 163.35 P
5 F
-0.24 (. The recentering of the tar) 338.69 163.35 P
-0.24 (get usually takes place about) 443.96 163.35 P
-0.02 (an orbit after the spiral search, and must be scheduled for a speci\336c time. If you have so) 207 151.35 P
0.52 (requested in your proposal, an image of the LSA will be made after the recentering so) 207 139.35 P
0.14 (that you may con\336rm the position of the tar) 207 127.35 P
0.14 (get \050but additional interaction at that time is) 381.78 127.35 P
(not normally possible\051.) 207 115.35 T
FMENDPAGE
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[0 0 0 1 0 0 0]
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[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Y) 189 736.18 T
(our Phase II Proposal) 194.34 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(36) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
(4.1.3) 157.76 679.35 T
(Early Acquisitions) 189 679.35 T
5 F
0.46 (In an early acquisition \050) 189 659.35 P
8 F
1.11 (EARLY) 285.83 659.35 P
1.11 (ACQ) 318.79 659.35 P
5 F
0.46 (\051, an image of the \336eld of interest is obtained sev-) 336.79 659.35 P
0.16 (eral weeks \0508 or more\051 in advance of the spectroscopic observation that the GHRS is to) 189 647.35 P
0.03 (make. The image may be obtained with WFPC2, with the FOC \050especially if an ultravi-) 189 635.35 P
0.23 (olet image is desired\051, or with the imaging capability of the GHRS itself. The GHRS is) 189 623.35 P
0.23 (relatively slow at getting images, so if you wish to map an area much lar) 189 611.35 P
0.23 (ger than about) 482.32 611.35 P
-0.23 (2) 189 599.35 P
12 F
-0.23 (\264) 196.5 599.35 P
5 F
-0.23 (2 arcsec we recommend that you consider WFPC2 or FOC. However) 204.26 599.35 P
-0.23 (, the GHRS has) 478.46 599.35 P
1.84 (the capability of obtaining a monochromatic map \050see Section) 189 587.35 P
1.84 (4.2.2 on page) 454.5 587.35 P
1.84 (43\051 in) 514.55 587.35 P
8 F
0.09 (IMAGE) 189 575.35 P
5 F
0.04 (mode, which can be useful in some situations. For any) 225.09 575.35 P
8 F
0.09 (EARLY) 445.46 575.35 P
0.09 (ACQ) 478 575.35 P
5 F
0.04 (, be sure to) 496 575.35 P
2.68 (note the relationship of the image to the spectroscopic observations as a Special) 189 563.35 P
0.12 (Requirement \050see the \336rst example in the next chapter\051. Also, you should plan ahead so) 189 551.35 P
-0.24 (that the early acquisition image can be analyzed quickly and the positions measured sent) 189 539.35 P
(back to STScI for incorporation into the telescope observing schedule.) 189 527.35 T
0 F
(4.1.4) 157.76 497.35 T
(Onboard Acquisitions) 189 497.35 T
5 F
-0.04 (After the initial pointing, a GHRS onboard tar) 189 477.35 P
-0.04 (get acquisition begins with a spiral search) 373.01 477.35 P
0.21 (centered on the \336eld of view) 189 465.35 P
0.21 (. The motions are made by the telescope, and at each point) 303.55 465.35 P
0.59 (of the search either a single \337ux measurement \050with 8 science diodes\051 or a map of the) 189 453.35 P
0.66 (LSA is made. The default is a) 189 441.35 P
0.66 ( pattern \050) 337.72 441.35 P
8 F
1.57 (SEARCH-SIZE=3) 375.13 441.35 P
5 F
0.66 (\051 of maps in a square) 453.13 441.35 P
0.67 (4.6 arcsec on a side. Other options available are a) 189 429.35 P
0.67 ( pattern \050) 418.72 429.35 P
8 F
1.62 (SEARCH-SIZE=5) 456.17 429.35 P
5 F
0.67 (\051,) 534.17 429.35 P
1.48 (7.7 arcsec on a side, or a single integration \050) 189 417.35 P
8 F
3.54 (SEARCH-SIZE=1) 378.62 417.35 P
5 F
1.48 (\051 that is 1.74 arcsec) 456.62 417.35 P
0.35 (square \050this latter option can be useful for obtaining a) 189 405.35 P
8 F
0.85 (MAP) 409.16 405.35 P
5 F
0.35 ( after an object is centered\051.) 427.16 405.35 P
0.59 (The telescope motions are made in the) 189 393.35 P
6 F
0.59 (x) 349.47 393.35 P
5 F
0.59 ( and) 353.91 393.35 P
6 F
0.59 (y) 374.52 393.35 P
5 F
0.59 ( coordinate system of the GHRS with a) 378.96 393.35 P
(step-size of 1.53 arcsec, not the U2, U3 system of the telescope.) 189 381.35 T
0.41 (For stars with good coordinates, the default \050) 189 361.35 P
0.41 (\051 acquisition strategy should suf) 393.81 361.35 P
0.41 (\336ce,) 523.06 361.35 P
1.16 (but the) 189 349.35 P
1.16 ( pattern usually costs little more in total time and guards against minor) 243.81 349.35 P
-0.01 (coordinate uncertainties \050the time needed increases in proportion to [) 189 337.35 P
8 F
-0.01 (SEARCH-SIZE) 464.17 337.35 P
5 F
-0.01 (]) 530.17 337.35 P
5 8 Q
-0 (2) 533.5 341.35 P
5 10 Q
-0.01 (,) 537.5 337.35 P
0.37 (but the) 189 325.35 P
8 F
0.9 (STEP-TIME) 219.75 325.35 P
5 F
0.37 ( for an acquisition is usually so low that the total time involved is) 273.75 325.35 P
(small\051.) 189 313.35 T
(Y) 189 293.35 T
(ou should use) 195.22 293.35 T
8 F
(ONBOARD) 252.72 293.35 T
(ACQ) 297.22 293.35 T
5 F
( whenever:) 315.22 293.35 T
7 11 Q
(\245) 189 275.35 T
5 10 Q
(The object is a point source, or) 203.4 275.35 T
7 11 Q
(\245) 189 260.35 T
5 10 Q
0.65 (The object can be reached by of) 203.4 260.35 P
0.65 (fsetting from a nearby object that meets the above) 334.85 260.35 P
(description, or) 203.4 248.35 T
7 11 Q
(\245) 189 233.35 T
5 10 Q
2.38 (An extended object is small enough that) 203.4 233.35 P
8 F
5.72 (LOCATE=EXTENDED) 383.14 233.35 P
5 F
2.38 ( will work \050see) 473.14 233.35 P
(Section) 203.4 221.35 T
(4.1.5.4 on page) 235.9 221.35 T
(39\051.) 299.78 221.35 T
0.69 (Also, the object to be centered should be the brightest object within the area searched) 189 201.35 P
0.13 (\050about) 189 189.35 P
0.13 ( arcsec for a 3) 254.65 189.35 P
12 F
0.13 ( \264) 311.24 189.35 P
5 F
0.13 ( 3 search\051 but with allowance for about 3 arcsec uncer-) 319.36 189.35 P
0.64 (tainty in positioning as well. In other words, you should ensure that your object is the) 189 177.35 P
-0.14 (brightest one that) 189 165.35 P
6 F
-0.14 (HST) 260.52 165.35 P
5 F
-0.14 ( will \336nd within a box whose total size is about 8) 278.3 165.35 P
12 F
-0.14 (\264) 475.51 165.35 P
5 F
-0.14 ( 8 arcsec. Note) 481 165.35 P
(that the \337ux is measured in the ultraviolet \050see Section) 189 153.35 T
(7.4.1 on page) 408.98 153.35 T
(78\051.) 465.36 153.35 T
(The items you must specify for the) 189 133.35 T
8 F
(ONBOARD) 330.93 133.35 T
(ACQ) 375.43 133.35 T
5 F
( are:) 393.43 133.35 T
7 11 Q
(\245) 189 115.35 T
5 10 Q
0.21 (The mirror to use. N2 and A2 should suf) 203.4 115.35 P
0.21 (\336ce for virtually all tar) 367.35 115.35 P
0.21 (gets you might wish) 458.54 115.35 P
0.36 (to observe. Mirrors N1 or A1 may also be used, especially for spectroscopic obser-) 203.4 103.35 P
0.79 (vations that utilize Side 1 \050i.e., detector D1\051. Mirror N2 provides a \337at re\337ectivity) 203.4 91.35 P
315.24 438.18 337.72 449.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(3) 315.74 441.35 T
(3) 331.22 441.35 T
12 F
(\264) 323.23 441.35 T
0 0 612 792 C
396.24 426.18 418.72 437.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(5) 396.74 429.35 T
(5) 412.23 429.35 T
12 F
(\264) 404.24 429.35 T
0 0 612 792 C
371.33 358.18 393.81 369.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(3) 371.82 361.35 T
(3) 387.31 361.35 T
12 F
(\264) 379.32 361.35 T
0 0 612 792 C
221.33 346.18 243.81 357.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(5) 221.83 349.35 T
(5) 237.31 349.35 T
12 F
(\264) 229.33 349.35 T
0 0 612 792 C
217.18 186.18 254.65 197.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(4) 217.67 189.35 T
(.) 222.67 189.35 T
(8) 225.17 189.35 T
(4) 240.66 189.35 T
(.) 245.66 189.35 T
(8) 248.16 189.35 T
12 F
(\264) 232.67 189.35 T
0 0 612 792 C
FMENDPAGE
%%EndPage: "36" 4
%%Page: "37" 5
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (37) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Y) 207 736.18 T
(our Phase II Proposal) 212.34 736.18 T
5 10 Q
0 (over a broad range of ultraviolet wavelengths \050see Section) 221.4 679.35 P
0 (7.4.1 on page) 456.63 679.35 P
0 (78\051. Mirror) 513.01 679.35 P
0.26 (A2 has a similar spectrum response but re\337ects much less light than N2, in order to) 221.4 667.35 P
-0.2 (acquire bright objects. Both detectors may be active at the same time, so it is permis-) 221.4 655.35 P
1.16 (sible to specify mirror N2 for an acquisition to observe with Side 1; this may be) 221.4 643.35 P
1.27 (desirable, for example, when observing cool stars. However) 221.4 631.35 P
1.27 (, doing this may cost) 469.85 631.35 P
(you observing time; see below) 221.4 619.35 T
(.) 342.96 619.35 T
7 11 Q
(\245) 207 604.35 T
8 10 Q
0.88 (BRIGHT) 221.4 604.35 P
5 F
0.37 ( and) 257.4 604.35 P
8 F
0.88 (FAINT) 277.58 604.35 P
5 F
0.37 ( \337ux limits so the instrument knows when the object has been) 307.58 604.35 P
-0.05 (found. However) 221.4 592.35 P
-0.05 (, in almost all cases it is better to use) 285.93 592.35 P
8 F
-0.12 (BRIGHT=RETURN) 434.6 592.35 P
5 F
-0.05 (, which is a) 512.6 592.35 P
0.71 (feature that automatically centers the brightest object found. If) 221.4 580.35 P
8 F
1.72 (BRIGHT=RETURN) 480 580.35 P
5 F
(is speci\336ed, any) 221.4 568.35 T
8 F
(FAINT) 288.06 568.35 T
5 F
( limit given is ignored.) 318.06 568.35 T
7 11 Q
(\245) 207 553.35 T
5 10 Q
0.69 (The size of the spiral search pattern to execute \050) 221.4 553.35 P
8 F
1.66 (SEARCH-SIZE) 418.97 553.35 P
5 F
0.69 (\051. The default is a) 484.97 553.35 P
0.27 (3) 221.4 541.35 P
12 F
0.27 (\264) 228.9 541.35 P
5 F
0.27 ( 3 grid \050which covers about 4.6 arcsec square\051, but you may also request a 5) 234.39 541.35 P
12 F
0.27 (\264) 544.74 541.35 P
5 F
0.27 ( 5) 550.23 541.35 P
(search over a square 7.7 arcsec on a side.) 221.4 529.35 T
7 11 Q
(\245) 207 514.35 T
5 10 Q
0.15 (Whether or not to record a map of the \336eld at the search points so that you can con-) 221.4 514.35 P
1.31 (\336rm the telescope\325) 221.4 502.35 P
1.31 (s pointing after the fact. A) 297.89 502.35 P
8 F
3.13 (MAP) 413.21 502.35 P
5 F
1.31 ( is usually unnecessary and so) 431.21 502.35 P
-0.11 (wastes spacecraft time. At most, a) 221.4 490.35 P
8 F
-0.26 (MAP=END-POINT) 359.62 490.35 P
5 F
-0.11 ( should suf) 437.62 490.35 P
-0.11 (\336ce. Note that such) 481.11 490.35 P
-0.23 (a) 221.4 478.35 P
8 F
-0.54 (MAP) 228.11 478.35 P
5 F
-0.23 ( occurs after the return to the brightest point in the \336eld but before the object is) 246.11 478.35 P
0.23 (centered in the LSA by an) 221.4 466.35 P
8 F
0.54 (ACQ/PEAKUP) 329.96 466.35 P
5 F
0.23 (. T) 388.85 466.35 P
0.23 (o determine the position of an object in) 399.48 466.35 P
0.47 (the LSA before spectroscopic observations are begun, we recommend obtaining an) 221.4 454.35 P
8 F
0.03 (IMAGE) 221.4 442.35 P
5 F
0.01 ( on a separate Exposure Logsheet line. The) 251.4 442.35 P
8 F
0.03 (MAP=ALL-POINTS) 426.19 442.35 P
5 F
0.01 ( option may) 510.19 442.35 P
6 F
(not) 221.4 430.35 T
5 F
( be used with an) 234.18 430.35 T
8 F
(ONBOARD) 301.67 430.35 T
(ACQ) 346.17 430.35 T
5 F
(.) 364.17 430.35 T
7 11 Q
(\245) 207 415.35 T
5 10 Q
(The of) 221.4 415.35 T
(fset to apply once the object is centered \050if appropriate\051.) 247.6 415.35 T
0 9 Q
(4.1.4.1) 170.48 392.02 T
(Explicitly Specifying) 207 392.02 T
7 10 Q
(BRIGHT) 297.04 392.02 T
0 9 Q
(,) 332.04 392.02 T
7 10 Q
( FAINT) 334.54 392.02 T
0 9 Q
(, and) 369.54 392.02 T
7 10 Q
(STEP-TIME) 393.05 392.02 T
5 F
0.02 (Explicit) 207 371.35 P
8 F
0.05 (BRIGHT) 241.19 371.35 P
5 F
0.02 ( and) 277.19 371.35 P
8 F
0.05 (FAINT) 296.67 371.35 P
5 F
0.02 ( limits may be speci\336ed if you desire, although there is an) 326.67 371.35 P
1.49 (increased risk of a failed acquisition unless you are fairly con\336dent of those \337uxes.) 207 359.35 P
1.34 (Also, a few very bright stars cannot be acquired with Side 2 if an explicit) 207 347.35 P
8 F
3.21 (BRIGHT) 522 347.35 P
5 F
(value is given but they can be acquired automatically with) 207 335.35 T
8 F
(BRIGHT=RETURN) 442.52 335.35 T
5 F
(.) 520.52 335.35 T
0.15 (Details on computing) 207 315.35 P
8 F
0.37 (BRIGHT) 296.07 315.35 P
5 F
0.15 (and) 338.44 315.35 P
8 F
0.37 (FAINT) 355.54 315.35 P
5 F
0.15 ( limits are given in Section) 385.54 315.35 P
0.15 (7.1 on page) 496.31 315.35 P
0.15 (68.) 545.5 315.35 P
0.07 (Please note that although we discourage the use of explicit) 207 303.35 P
8 F
0.16 (BRIGHT) 444.31 303.35 P
5 F
0.07 ( and) 480.31 303.35 P
8 F
0.16 (FAINT) 499.88 303.35 P
5 F
0.07 ( values) 529.88 303.35 P
-0.25 (unless they are unavoidable, you still need to estimate the tar) 207 291.35 P
-0.25 (get acquisition count rate in) 447.9 291.35 P
1.3 (order to ensure that you choose the acquisition mirror correctly and that the) 207 279.35 P
8 F
3.12 (STEP-) 528 279.35 P
(TIME) 207 267.35 T
5 F
( is determined properly) 231 267.35 T
(.) 323.39 267.35 T
7 11 Q
(\245) 207 249.35 T
5 10 Q
0.63 (Note that using) 221.4 249.35 P
8 F
1.51 (BRIGHT=RETURN) 286.9 249.35 P
5 F
0.63 ( and explicitly specifying) 364.9 249.35 P
8 F
1.51 (BRIGHT) 471.3 249.35 P
5 F
0.63 ( and) 507.3 249.35 P
8 F
1.51 (FAINT) 528 249.35 P
5 F
2.44 (limits result in fundamentally dif) 221.4 237.35 P
2.44 (ferent acquisition procedures. If) 362.64 237.35 P
8 F
5.85 (BRIGHT) 502.62 237.35 P
5 F
2.44 ( and) 538.62 237.35 P
8 F
1.33 (FAINT) 221.4 225.35 P
5 F
0.55 ( are speci\336ed, the acquisition stops as soon as those conditions are met and) 251.4 225.35 P
3.14 (the point at which that happened is moved to the center of the LSA. W) 221.4 213.35 P
3.14 (ith) 547.44 213.35 P
8 F
5.07 (BRIGHT=RETURN) 221.4 201.35 P
5 F
2.11 (, the entire spiral search region is sampled and the brightest) 299.4 201.35 P
0.67 (object in it determined before any movement is made to center on the tar) 221.4 189.35 P
0.67 (get. Both) 520.66 189.35 P
1.14 (procedures require the same amount of telescope time because the schedule must) 221.4 177.35 P
(allow for the entire region to be sampled.) 221.4 165.35 T
0 9 Q
(4.1.4.2) 170.48 142.02 T
(Peakups) 207 142.02 T
5 10 Q
-0.12 (After the initial acquisition, a peakup helps to precisely center the object in the aperture.) 207 121.35 P
1.08 (Specifying a) 207 109.35 P
8 F
2.59 (ACQ/PEAKUP) 261.93 109.35 P
5 F
1.08 ( before starting LSA observations will help to ensure the) 321.93 109.35 P
FMENDPAGE
%%EndPage: "37" 5
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Y) 189 736.18 T
(our Phase II Proposal) 194.34 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(38) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
5 F
1.58 (reliability of measured \337uxes. A) 189 679.35 P
8 F
3.78 (ACQ/PEAKUP) 328.52 679.35 P
5 F
1.58 ( before starting SSA observations is) 388.52 679.35 P
(vital for achieving the best throughput with the small aperture.) 189 667.35 T
1.19 (In the past we recommended using a) 189 647.35 P
8 F
2.86 (STEP-TIME) 345.92 647.35 P
5 F
1.19 ( value of 1.6 seconds for a) 399.92 647.35 P
8 F
2.86 (ACQ/) 516 647.35 P
-0.46 (PEAKUP) 189 635.35 P
5 F
-0.19 (, but that is unnecessary for the post-Servicing Mission observatory) 223.89 635.35 P
-0.19 (. W) 491.48 635.35 P
-0.19 (e recom-) 504.93 635.35 P
0.35 (mend aiming to achieve 1,000 to 10,000 counts in the peak step, as for the acquisition,) 189 623.35 P
(but levels as low as 100 will suf) 189 611.35 T
(\336ce for faint tar) 316.87 611.35 T
(gets.) 379.17 611.35 T
0 F
(4.1.5) 157.76 581.35 T
(Special Onboard Strategies for Special Situations) 189 581.35 T
0 9 Q
(4.1.5.1) 152.48 558.02 T
(Side 2 Acquisitions for Side 1 Science Observations) 189 558.02 T
5 10 Q
-0.17 (There are situations in which an object can be observed satisfactorily with Side 1 but for) 189 545.35 P
0.02 (which the count rates for acquisition mirrors N1 or A1 are extremely low) 189 533.35 P
0.02 (. One possibil-) 481.34 533.35 P
1.58 (ity is to increase the exposure time for the acquisition, but the maximum permitted) 189 521.35 P
8 F
0.3 (STEP-TIME) 189 509.35 P
5 F
0.12 ( is 12.75 seconds. A better option may be to acquire with mirror N2. Both) 243 509.35 P
-0.08 (detectors, D1 and D2, may be active in the GHRS at the same time, but there is an over-) 189 497.35 P
-0.18 (head involved in making one primary and the other secondary; to go from Side 2 to Side) 189 485.35 P
0.34 (1, that time is approximately 40 minutes. Whether or not that is a \322cost\323 or not to your) 189 473.35 P
0.53 (program depends on speci\336c details. It is often the case that an acquisition takes place) 189 461.35 P
-0.04 (over the \336rst orbit, followed by science observations in later orbits. In that case, most or) 189 449.35 P
0.32 (all of the 40 minutes can take place during the part of the orbit when the tar) 189 437.35 P
0.32 (get is inac-) 495.49 437.35 P
(cessible. But for CVZ viewing the cost can be real.) 189 425.35 T
0 9 Q
(4.1.5.2) 152.48 402.02 T
(Complex T) 189 402.02 T
(argets) 234.34 402.02 T
5 10 Q
-0.04 (Given the centering algorithm for the GHRS, which we will now describe, you can usu-) 189 381.35 P
0.92 (ally predict the results of an onboard tar) 189 369.35 P
0.92 (get acquisition. Stepping, in both the) 354.91 369.35 P
6 F
0.92 (x) 509.85 369.35 P
5 F
0.92 ( and) 514.29 369.35 P
6 F
0.92 (y) 535.56 369.35 P
5 F
0.03 (directions, is done in 0.027 arcsec steps, and on a point source the centering is expected) 189 357.35 P
0.92 (to be good to within two steps. If the tar) 189 345.35 P
0.92 (get is extended enough that the \337uxes in the) 357.1 345.35 P
0.41 (areas which are compared do not change signi\336cantly when a step is made, the center-) 189 333.35 P
0.33 (ing accuracy will be degraded. An example is the case in which there is more than one) 189 321.35 P
(source of light within the LSA.) 189 309.35 T
0.92 (Consider) 189 289.35 P
0.92 (, for instance, two stars which are separated by 1.0 arcsec and for which the) 224.71 289.35 P
-0.12 (second star is 1 magnitude fainter than the primary star) 189 277.35 P
-0.12 (. Exact results will depend on the) 407.65 277.35 P
0.59 (position angle between the two stars. The) 189 265.35 P
6 F
0.59 (x) 361.46 265.35 P
5 F
0.59 (balancing algorithm begins by placing the) 368.99 265.35 P
-0.1 (brightest source on the fourth of the eight diodes that are used during an acquisition \050the) 189 253.35 P
0.58 (LSA is imaged onto eight diodes\051, and moving until the \337ux on diodes 4 and 5 is bal-) 189 241.35 P
0.2 (anced. The second star would not af) 189 229.35 P
0.2 (fect this balance at all unless its light fell on one of) 334.17 229.35 P
-0.22 (the same diodes as the primary star) 189 217.35 P
-0.22 (. In that case it would af) 327.66 217.35 P
-0.22 (fect centering by a fraction of) 422.53 217.35 P
(a diode.) 189 205.35 T
0.55 (In the) 189 185.35 P
6 F
0.55 (y) 215.65 185.35 P
5 F
0.55 ( direction the results are dif) 220.09 185.35 P
0.55 (ferent. If the second star is \322above\323 or \322below\323 the) 332.35 185.35 P
1.33 (primary) 189 173.35 P
1.33 (, it will \322pull\323 the centering in that direction. In the case described, an extra) 220.01 173.35 P
0.01 (source of light 40% as bright as the primary would be present in the upper or lower half) 189 161.35 P
-0.05 (of the LSA. The \337ux-balancing algorithm would divide the primary image 70-30, rather) 189 149.35 P
-0 (than 50-50, with the image displaced towards the half of the LSA which did not contain) 189 137.35 P
-0.17 (the second star) 189 125.35 P
-0.17 (. In this case the centering error should be less than 0.1 arcsec. If the LSA) 247.55 125.35 P
0.08 (acquisition were to be followed by a slew to the SSA,) 189 113.35 P
8 F
0.18 (PEAKUP) 407.04 113.35 P
5 F
0.08 (, and an observation, the) 441.93 113.35 P
3.33 (primary object should be successfully centered and observed. More complicated) 189 101.35 P
FMENDPAGE
%%EndPage: "38" 6
%%Page: "39" 7
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (39) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Y) 207 736.18 T
(our Phase II Proposal) 212.34 736.18 T
5 10 Q
0.42 (images, or sources more similar in brightness may not be suitable for onboard acquisi-) 207 679.35 P
(tion. \050Note that balancing in the) 207 667.35 T
6 F
(y) 336.71 667.35 T
5 F
( direction is done before the) 341.15 667.35 T
6 F
(x) 455.57 667.35 T
5 F
( direction is balanced.\051) 460.01 667.35 T
0 9 Q
(4.1.5.3) 170.48 644.02 T
(Acquiring Faint T) 207 644.02 T
(argets with the GHRS or FOS) 280.34 644.02 T
5 10 Q
0.34 (Sometimes a star may be just plain faint to the point where geocoronal L) 207 623.35 P
0.34 (yman-) 501.64 623.35 P
12 F
0.34 (a) 527.19 623.35 P
5 F
0.34 ( inter-) 533.5 623.35 P
0.75 (feres. Some guidance for when this may be a problem is provided in Section) 207 611.35 P
0.75 (7.4.2 on) 524.75 611.35 P
0.44 (page) 207 599.35 P
0.44 (80. If it is, we recommend that you specify) 228.38 599.35 P
8 F
1.05 (DARK) 406.45 599.35 P
1.05 (TIME) 433.39 599.35 P
5 F
0.44 ( as a special requirement) 457.39 599.35 P
1.16 (on the acquisition line on your Phase II form. Doing so constrains the scheduling of) 207 587.35 P
0.33 (your proposal and is likely to result in greater resource char) 207 575.35 P
0.33 (ges to you, so) 448.37 575.35 P
8 F
0.78 (DARK) 507.17 575.35 P
0.78 (TIME) 534 575.35 P
5 F
(should only be requested when it is necessary) 207 563.35 T
(.) 388.82 563.35 T
1.87 (Another way to acquire very faint tar) 207 543.35 P
1.87 (gets reliably is to use the Faint Object Spec-) 366.36 543.35 P
1.26 (trograph. This can be especially useful for acquiring extragalactic objects to observe) 207 531.35 P
-0 (with grating G140L because the acquisition mirrors for Side 1 of the GHRS re\337ect only) 207 519.35 P
1.12 (far) 207 507.35 P
1.12 (-ultraviolet light and because the maximum permissible integration time per dwell) 217.9 507.35 P
0.74 (point is only 12.75 seconds. FOS-assisted acquisitions for the GHRS will be tested in) 207 495.35 P
(Cycle 4, so we suggest that you consult us if you wish to explore this option.) 207 483.35 T
0 9 Q
(4.1.5.4) 170.48 460.02 T
(Acquiring Extended Sources with the GHRS) 207 460.02 T
5 10 Q
(There are three classes of extended sources we can consider:) 207 439.35 T
7 11 Q
(\245) 207 421.35 T
5 10 Q
(Objects lar) 221.4 421.35 T
(ger than the LSA that have roughly uniform surface brightness.) 264.82 421.35 T
7 11 Q
(\245) 207 406.35 T
5 10 Q
(Objects smaller than the LSA with roughly uniform surface brightness.) 221.4 406.35 T
7 11 Q
(\245) 207 391.35 T
5 10 Q
(Objects with signi\336cant structure, some of which is on scales smaller than the LSA.) 221.4 391.35 T
0.64 (The \336rst class might be typi\336ed by Jupiter) 207 371.35 P
0.64 (, and such objects are impossible to acquire) 379.67 371.35 P
0.77 (directly with the GHRS because there is no clear photometric \322center\323 to align on. In) 207 359.35 P
(such cases it is necessary to of) 207 347.35 T
(fset from a smaller object which can be centered.) 328.46 347.35 T
0.02 (The second class of objects includes the Gallilean satellites of Jupiter) 207 327.35 P
0.02 (, and it is these for) 484.01 327.35 P
0.39 (which the) 207 315.35 P
8 F
0.94 (LOCATE=EXTENDED) 249.44 315.35 P
5 F
0.39 ( acquisition option was written. In a normal) 339.44 315.35 P
8 F
0.94 (LOCATE) 519.5 315.35 P
5 F
0.39 (,) 555.5 315.35 P
0.34 (the object to be observed is moved in the) 207 303.35 P
6 F
0.34 (x) 376.42 303.35 P
5 F
0.34 ( direction until the signal seen by the center) 380.86 303.35 P
6.54 (two diodes \050of the eight onto which the LSA is imaged\051 is balanced.) 207 291.35 P
8 F
3.05 (LOCATE=EXTENDED) 207 279.35 P
5 F
1.27 ( in) 297 279.35 P
8 F
3.05 (ACQUISITION) 312.32 279.35 P
5 F
1.27 ( mode balances the four left diodes against) 378.32 279.35 P
2.26 (the four right-hand ones to roughly center an object. In) 207 267.35 P
8 F
5.43 (ACQ/PEAKUP) 451.53 267.35 P
5 F
2.26 ( mode, the) 511.53 267.35 P
8 F
2.77 (EXTENDED) 207 255.35 P
5 F
1.15 ( option allows you to specify that the balancing be done over the central) 255 255.35 P
(four) 207 243.35 T
(, six, or eight diodes \050speci\336ed as) 223.26 243.35 T
8 F
(EXTENDED=2) 359.08 243.35 T
5 F
(,) 419.08 243.35 T
8 F
(3) 424.08 243.35 T
5 F
(, or) 430.08 243.35 T
8 F
(4) 445.91 243.35 T
5 F
(\051.) 451.91 243.35 T
1.38 (The third class of objects can be the most problematic, especially if the tar) 207 223.35 P
1.38 (get is an) 521.91 223.35 P
0.04 (extragalactic one at high latitude. In such cases there may be no nearby star from which) 207 211.35 P
0.31 (you could of) 207 199.35 P
0.31 (fset, but the source itself often contains point-like sources that can be cen-) 257.98 199.35 P
0.65 (tered on; in these cases an early acquisition or a pre-existing image is invaluable. The) 207 187.35 P
0.66 (problem is then one of predicting acquisition count rates; that is treated in Section) 207 175.35 P
0.66 (7.1) 545.5 175.35 P
0.06 (on page) 207 163.35 P
0.06 (68. Y) 240.94 163.35 P
0.06 (ou may also wish to consider an acquisition with the FOS, as described in) 262.22 163.35 P
(the previous section.) 207 151.35 T
0 9 Q
(4.1.5.5) 170.48 128.02 T
(Offsetting) 207 128.02 T
5 10 Q
0.23 (Even if an) 207 107.35 P
8 F
0.55 (ONBOARD) 251.28 107.35 P
0.55 (ACQ) 296.01 107.35 P
5 F
0.23 (uisition will not work for your tar) 314.01 107.35 P
0.23 (get, it may still be possible) 449.63 107.35 P
0.61 (to acquire a nearby reference star and to then of) 207 95.35 P
0.61 (fset to your tar) 403.03 95.35 P
0.61 (get. Such an of) 463.27 95.35 P
0.61 (fset will) 524.89 95.35 P
FMENDPAGE
%%EndPage: "39" 7
%%Page: "40" 8
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Y) 189 736.18 T
(our Phase II Proposal) 194.34 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(40) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
5 F
0.54 (happen automatically if the coordinates given for an acquisition exposure are dif) 189 679.35 P
0.54 (ferent) 516.68 679.35 P
0.6 (from those given for the science exposure. Y) 189 667.35 P
0.6 (ou would normally use two or three lines) 371.62 667.35 P
-0.12 (on the Phase II Exposure Logsheet to achieve this: acquisition of a reference star) 189 655.35 P
-0.12 (, of) 510.03 655.35 P
-0.12 (fset,) 523.06 655.35 P
0.05 (peakup on the tar) 189 643.35 P
0.05 (get \050if desired\051, and a science observation. The \336rst line would request) 258.12 643.35 P
1.76 (an onboard acquisition of the reference star) 189 631.35 P
1.76 (. It should specify) 372.29 631.35 P
8 F
4.22 (ONBOARD) 453.48 631.35 P
4.22 (ACQ) 499.74 631.35 P
4.22 (FOR) 522 631.35 P
5 F
1.64 ( 1.64 (2>. Line 2 should then be an) 212.14 619.35 P
8 F
3.94 (ACQ/PEAKUP) 340.36 619.35 P
5 F
1.64 (, and it should specify) 399.25 619.35 P
8 F
3.94 (ONBOARD) 498 619.35 P
1.79 (ACQ) 189 607.35 P
1.79 (FOR) 210.25 607.35 P
5 F
0.75 ( . The next line would specify an of) 228.25 607.35 P
0.75 (fset to move from the reference) 410.48 607.35 P
(star to the tar) 189 595.35 T
(get, and the \336nal line should be your intended science observation.) 241.31 595.35 T
1.33 (Y) 189 575.35 P
1.33 (ou must, of course, include the reference star as one of the objects on your T) 195.22 575.35 P
1.33 (ar) 520.19 575.35 P
1.33 (get) 527.78 575.35 P
0.5 (Logsheet. It should be designated) 189 563.35 P
13 F
1.19 (xxx) 328.14 563.35 P
8 F
1.19 (-OFFSET) 346.14 563.35 P
5 F
0.5 (, where) 387.4 563.35 P
13 F
1.19 (xxx) 420.32 563.35 P
5 F
0.5 ( is the name of the tar) 438.32 563.35 P
0.5 (get) 527.78 563.35 P
1.04 (object. If desired, you may give the position of your tar) 189 551.35 P
1.04 (get by using) 420.26 551.35 P
8 F
2.49 (RA-OFF) 474.76 551.35 P
5 F
1.04 (,) 509.96 551.35 P
8 F
2.49 (DEC-) 516 551.35 P
4.01 (OFF) 189 539.35 P
5 F
1.67 (, or) 206.2 539.35 P
8 F
4.01 (XI-OFF) 225.37 539.35 P
5 F
1.67 (,) 260.57 539.35 P
8 F
4.01 (ETA-OFF) 267.24 539.35 P
5 F
1.67 ( and) 309.24 539.35 P
8 F
4.01 (FROM) 332.02 539.35 P
5 F
1.67 ( relative to the of) 356.02 539.35 P
1.67 (fset star) 430.83 539.35 P
1.67 (. See the Proposal) 463.33 539.35 P
0.09 (Instructions for details and notes on proper units. On the Exposure Logsheet, the T) 189 527.35 P
0.09 (ar) 520.19 527.35 P
0.09 (get) 527.78 527.35 P
0.31 (Name for lines 1 and 2 are) 189 515.35 P
13 F
0.74 (xxx) 299.74 515.35 P
8 F
0.74 (-OFFSET) 317.74 515.35 P
5 F
0.31 (, and in the example above, the T) 359.01 515.35 P
0.31 (ar) 493.5 515.35 P
0.31 (get Name) 501.09 515.35 P
(for line 3 is) 189 503.35 T
13 F
(xxx) 237.33 503.35 T
8 F
(.) 255.33 503.35 T
5 F
0.6 (T) 189 483.35 P
0.6 (o make a successful of) 194.41 483.35 P
0.6 (fset, the relative positions of the of) 287.15 483.35 P
0.6 (fset star and tar) 429.71 483.35 P
0.6 (get must be) 492.69 483.35 P
0.11 (very well known \320 about as well as 1/4 the size of the aperture. \050e.g., rms errors of 0.05) 189 471.35 P
0.81 (arcsec for the SSA.\051 One way of obtaining such positions is by requesting an) 189 459.35 P
8 F
1.94 (EARLY) 510 459.35 P
0.66 (ACQ) 189 447.35 P
5 F
0.27 (uisition WFPC2 image, and measuring relative positions from it \050at least 2 months) 207 447.35 P
-0.16 (prior to the science observation\051. The of) 189 435.35 P
-0.16 (fset positioning accuracy of the) 348.1 435.35 P
6 F
-0.16 (HST) 475.33 435.35 P
5 F
-0.16 ( is expected) 493.11 435.35 P
-0.02 (to be very good \050of the order of 0.03 to 0.05 arcsec for a 30 arcsec of) 189 423.35 P
-0.02 (fset\051, and the accu-) 463.98 423.35 P
0.72 (racy of the placement will be primarily determined by the accuracy of your positions.) 189 411.35 P
0.38 (An of) 189 399.35 P
0.38 (fset of more than 30 arcsec may require the telescope to acquire new guide stars,) 212.25 399.35 P
(which would worsen the accuracy of the positioning.) 189 387.35 T
0 F
(4.1.6) 157.76 357.35 T
(MAPs) 189 357.35 T
5 F
0.26 (The GHRS has the ability to make a) 189 337.35 P
8 F
0.63 (MAP) 338.3 337.35 P
5 F
0.26 ( of the LSA by raster scanning one or both of) 356.3 337.35 P
0.4 (its small focus diodes over the aperture. Y) 189 325.35 P
0.4 (ou may) 359.68 325.35 P
0.4 (, for example, want a map to con\336rm) 389.15 325.35 P
0.63 (the pointing at the time your spectrum was taken. The default for) 189 313.35 P
8 F
1.52 (ONBOARD) 459.08 313.35 P
1.52 (ACQ) 504.22 313.35 P
5 F
0.63 (uisi-) 522.22 313.35 P
0.11 (tions is to make no map. If you ask for) 189 301.35 P
8 F
0.26 (MAP=END-POINT) 347.01 301.35 P
5 F
0.11 (, you will get a map after the) 424.27 301.35 P
0.71 (spiral search has found your tar) 189 289.35 P
0.71 (get, but before it has been centered \050with) 318.18 289.35 P
8 F
1.71 (LOCATE) 489.68 289.35 P
5 F
0.71 (\051 in) 525.68 289.35 P
1.07 (the LSA. If you want a map after the \336nal centering, you can add a single Exposure) 189 277.35 P
0.01 (Logsheet line in) 189 265.35 P
8 F
0.03 (IMAGE) 255.98 265.35 P
5 F
0.01 ( mode. An) 285.98 265.35 P
8 F
0.03 (IMAGE) 330.46 265.35 P
5 F
0.01 ( may also be obtained of the SSA, which can) 360.46 265.35 P
0.93 (be a useful) 189 253.35 P
6 F
0.93 (a posteriori) 237.61 253.35 P
5 F
0.93 ( means of determining what was observed in a crowded \336eld.) 285.48 253.35 P
(The) 189 241.35 T
8 F
(MAP=ALL-POINTS) 207.05 241.35 T
5 F
( option may) 291.05 241.35 T
6 F
(not) 341.33 241.35 T
5 F
( be used with an onboard acquisition.) 354.11 241.35 T
0 F
(4.1.7) 157.76 211.35 T
(Acquisition Parameters \321 A Summary) 189 211.35 T
9 F
(Step 1:) 189 191.35 T
5 F
( Mode=) 218.72 191.35 T
8 F
(ACQ) 250.19 191.35 T
7 11 Q
(\245) 189 173.35 T
5 10 Q
(Aperture is always LSA \050\322) 203.4 173.35 T
8 F
(2.0) 310.04 173.35 T
5 F
(\323\051.) 328.04 173.35 T
7 11 Q
(\245) 189 158.35 T
8 10 Q
2.73 (MIRROR) 203.4 158.35 P
5 F
1.14 ( is usually) 239.4 158.35 P
8 F
2.73 (N2) 285.87 158.35 P
5 F
1.14 ( or) 297.87 158.35 P
8 F
2.73 (N1) 313.47 158.35 P
5 F
1.14 ( unless object is too bright \050then use) 325.47 158.35 P
8 F
2.73 (A2) 481.21 158.35 P
5 F
1.14 ( or) 493.21 158.35 P
8 F
2.73 (A1) 508.81 158.35 P
5 F
1.14 (; see) 520.81 158.35 P
0.43 (Section) 203.4 146.35 P
0.43 (7.1 on page) 235.9 146.35 P
0.43 (68\051. Mirrors A1 and N1 may also be used and it is permissible) 285.65 146.35 P
-0.18 (to acquire with one side \050mirror) 203.4 134.35 P
8 F
-0.44 (N2) 331.72 134.35 P
5 F
-0.18 (, say\051 and observe with the other \050grating G140L,) 343.72 134.35 P
(perhaps\051, but with a possible cost in time.) 203.4 122.35 T
7 11 Q
(\245) 189 107.35 T
8 10 Q
0.77 (SEARCH-SIZE=3) 203.4 107.35 P
5 F
0.32 ( is the default and adequate almost all the time. V) 281.4 107.35 P
0.32 (alues of 1 or 5) 481.51 107.35 P
(may also be used.) 203.4 95.35 T
FMENDPAGE
%%EndPage: "40" 8
%%Page: "41" 9
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (41) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Y) 207 736.18 T
(our Phase II Proposal) 212.34 736.18 T
7 11 Q
(\245) 207 679.35 T
8 10 Q
2.65 (BRIGHT=RETURN) 221.4 679.35 P
5 F
1.1 ( is the default for \336nding the tar) 299.4 679.35 P
1.1 (get and should be used unless) 433.88 679.35 P
1.01 (you are forced not to. Do not specify) 221.4 667.35 P
8 F
2.42 (FAINT) 379.17 667.35 P
5 F
1.01 ( unless you must specify an explicit) 409.17 667.35 P
8 F
(BRIGHT) 221.4 655.35 T
5 F
( limit. \050) 257.4 655.35 T
8 F
(FAINT) 287.13 655.35 T
5 F
( is ignored if) 317.13 655.35 T
8 F
(BRIGHT=RETURN) 370.46 655.35 T
5 F
( is used.\051) 448.46 655.35 T
7 11 Q
(\245) 207 640.35 T
8 10 Q
2.51 (LOCATE) 221.4 640.35 P
5 F
1.04 (: Default is) 257.4 640.35 P
8 F
2.51 (YES) 307.48 640.35 P
5 F
1.04 ( for an) 325.48 640.35 P
8 F
2.51 (ONBOARD) 357.21 640.35 P
2.51 (ACQ) 402.76 640.35 P
5 F
1.04 ( and) 420.76 640.35 P
8 F
2.51 (NO) 442.29 640.35 P
5 F
1.04 ( for) 454.29 640.35 P
8 F
2.51 (EARLY) 473.04 640.35 P
2.51 (ACQ) 506.58 640.35 P
5 F
1.04 ( or) 524.58 640.35 P
8 F
2.51 (INT) 540 640.35 P
0.32 (ACQ) 221.4 628.35 P
5 F
0.13 (. W) 239.4 628.35 P
0.13 (e recommend these defaults. Note that) 253.17 628.35 P
8 F
0.32 ( LOCATE=EXTENDED) 407.13 628.35 P
5 F
0.13 ( is now avail-) 503.45 628.35 P
-0.22 (able. W) 221.4 616.35 P
-0.22 (ith an) 251.88 616.35 P
8 F
-0.54 (ONBOARD) 276.42 616.35 P
-0.54 (ACQ) 320.7 616.35 P
5 F
-0.22 (,) 338.7 616.35 P
8 F
-0.54 (LOCATE=NO) 343.47 616.35 P
5 F
-0.22 ( may be used only if) 397.47 616.35 P
8 F
-0.54 (MAP=END-POINT) 480 616.35 P
5 F
(is speci\336ed.) 221.4 604.35 T
7 11 Q
(\245) 207 589.35 T
8 10 Q
0.38 (MAP) 221.4 589.35 P
5 F
0.16 (: The defaults provide for an image to be transmitted to the ground if) 239.4 589.35 P
8 F
0.38 (INT) 519.34 589.35 P
0.38 (ACQ) 540 589.35 P
5 F
-0.24 (or) 221.4 577.35 P
8 F
-0.57 (EARLY) 231.99 577.35 P
-0.57 (ACQ) 264.26 577.35 P
5 F
-0.24 ( is speci\336ed. No image is generated by default for an) 282.26 577.35 P
8 F
-0.57 (ONBOARD) 492.95 577.35 P
-0.57 (ACQ) 537.22 577.35 P
5 F
-0.24 (;) 555.22 577.35 P
8 F
1.47 (MAP=END-POINT) 221.4 565.35 P
5 F
0.61 (will provide one with the tar) 306.87 565.35 P
0.61 (get in the LSA, but it will not be) 423.36 565.35 P
-0.06 (centered. As we have pointed out, if you wish to determine the actual position of the) 221.4 553.35 P
-0.21 (object in the LSA before spectroscopic observations are begun, you should obtain an) 221.4 541.35 P
8 F
1.58 (IMAGE) 221.4 529.35 P
5 F
0.66 ( as a separate Exposure Logsheet line and you should not specify a) 251.4 529.35 P
8 F
1.58 (MAP) 529.62 529.35 P
5 F
0.66 ( at) 547.62 529.35 P
(all.) 221.4 517.35 T
8 F
(MAP=ALL-POINTS) 236.4 517.35 T
5 F
( may not be used with an) 320.4 517.35 T
8 F
(ONBOARD) 422.89 517.35 T
(ACQ) 467.39 517.35 T
5 F
(.) 485.39 517.35 T
7 11 Q
(\245) 207 502.35 T
5 10 Q
(The time per exposure can be calculated from) 221.4 502.35 T
0.36 (where) 221.4 440.14 P
0.36 ( \050i.e., 1, 9, or 25\051, and) 383.81 440.14 P
0.36 ( is the number) 499.98 440.14 P
2.36 (of dwell points mapped \050=1 if) 221.4 428.14 P
8 F
5.67 (MAP=END-POINT) 357.31 428.14 P
5 F
2.36 ( is chosen and =) 435.31 428.14 P
2.36 ( if) 547.03 428.14 P
8 F
2.87 (MAP=ALL-POINTS) 221.4 416.14 P
5 F
1.2 (.) 305.4 416.14 P
8 F
2.87 ( MAP=ALL-POINTS) 307.9 416.14 P
5 F
1.2 ( can only be used with) 400.77 416.14 P
8 F
2.87 (INT) 500.17 416.14 P
2.87 (ACQ) 521.86 416.14 P
5 F
1.2 ( and) 539.86 416.14 P
8 F
0.22 (EARLY) 221.4 404.14 P
0.22 (ACQ) 253.99 404.14 P
5 F
0.09 (.\051.) 271.99 404.14 P
9 F
0.09 (Please note the value of) 282.92 404.14 P
7 F
0.22 (STEP-TIME) 385.32 404.14 P
9 F
0.09 ( you want as a) 439.32 404.14 P
7 F
0.22 (COMMENT) 502.85 404.14 P
9 F
0.09 ( on) 544.85 404.14 P
(the Exposur) 221.4 392.14 T
(e Logsheet.) 273.17 392.14 T
7 11 Q
(\245) 207 377.14 T
5 10 Q
(Special Requirements are) 221.4 377.14 T
8 F
(INT) 326.1 377.14 T
(ACQ) 346.6 377.14 T
5 F
(,) 364.6 377.14 T
8 F
(EARLY) 369.6 377.14 T
(ACQ) 402.1 377.14 T
5 F
(, or) 420.1 377.14 T
8 F
(ONBOARD) 435.93 377.14 T
(ACQ) 480.43 377.14 T
5 F
(.) 498.43 377.14 T
9 F
(Step 2:) 207 357.14 T
5 F
( Mode=) 236.72 357.14 T
8 F
(ACQ/PEAKUP) 268.19 357.14 T
7 11 Q
(\245) 207 339.14 T
5 10 Q
-0.11 (The aperture can be either the LSA \050\322) 221.4 339.14 P
8 F
-0.27 (2.0) 371.39 339.14 P
5 F
-0.11 (\323\051 or SSA \050\322) 389.39 339.14 P
8 F
-0.27 (0.25) 438.76 339.14 P
5 F
-0.11 (\323\051; specify the one to be) 462.76 339.14 P
(used for the science observations that immediately follow) 221.4 327.14 T
(.) 451.55 327.14 T
7 11 Q
(\245) 207 312.14 T
5 10 Q
0.02 (Specify the) 221.4 312.14 P
8 F
0.05 (MIRROR) 269.21 312.14 P
5 F
0.02 ( as for Mode=) 305.21 312.14 P
8 F
0.05 (ACQ) 361.73 312.14 P
5 F
0.02 (; i.e.,) 379.73 312.14 P
8 F
0.05 (N1) 402.27 312.14 P
5 F
0.02 (,) 414.27 312.14 P
8 F
0.05 (A1) 419.3 312.14 P
5 F
0.02 (,) 431.3 312.14 P
8 F
0.05 (N2) 436.32 312.14 P
5 F
0.02 (, or) 448.32 312.14 P
8 F
0.05 (A2) 464.19 312.14 P
5 F
0.02 ( depending on tar) 476.19 312.14 P
0.02 (get) 545.78 312.14 P
(brightness.) 221.4 300.14 T
7 11 Q
(\245) 207 285.14 T
5 10 Q
(The time per exposure can be calculated from) 221.4 285.14 T
1.14 (where) 221.4 225.14 P
6 F
1.14 (f) 249.47 225.14 P
6 8 Q
0.92 (Apertur) 255.9 222.64 P
0.92 (e) 280.49 222.64 P
5 10 Q
1.14 ( = 102 if the LSA is used and = \050) 284.04 225.14 P
8 F
2.75 (SEARCH-SIZE) 426.75 225.14 P
5 F
1.14 (\051) 492.75 225.14 P
5 8 Q
0.92 (2) 496.08 229.14 P
5 10 Q
1.14 ( if the SSA is) 500.08 225.14 P
0.69 (used. Note that the throughput of the SSA is half to 2/3 that of the LSA so that in) 221.4 213.14 P
0.17 (general you should specify a) 221.4 201.14 P
8 F
0.41 (STEP-TIME) 339.17 201.14 P
5 F
0.17 ( that is lar) 393.17 201.14 P
0.17 (ger than the one you used for a) 433.23 201.14 P
8 F
(PEAKUP) 221.4 189.14 T
5 F
( in the LSA.) 257.4 189.14 T
7 11 Q
(\245) 207 174.14 T
5 10 Q
0.02 (W) 221.4 174.14 P
0.02 (e ur) 230.04 174.14 P
0.02 (ge you to be precise and explicit about the way in which you specify an) 245.15 174.14 P
8 F
0.05 (ACQ/) 534 174.14 P
-0.51 (PEAKUP) 221.4 162.14 P
5 F
-0.21 ( and the order in which observations are to be made. The defaults that apply) 257.4 162.14 P
0.79 (to) 221.4 150.14 P
8 F
1.89 (ACQ) 232.47 150.14 P
5 F
0.79 ( and) 250.47 150.14 P
8 F
1.89 (ACQ/PEAKUP) 271.48 150.14 P
5 F
0.79 ( modes will usually accomplish what you wish, but the) 331.48 150.14 P
0.07 (way to be sure is to specify the details. Confusion can arise particularly when a pro-) 221.4 138.14 P
0.17 (gram mixes LSA and SSA observations. W) 221.4 126.14 P
0.17 (e would recommend that you do an) 395.22 126.14 P
8 F
0.41 (ACQ) 540 126.14 P
5 F
0.22 (in the \336rst line of the Exposure Logsheet, then on line 2 specify) 221.4 114.14 P
8 F
0.52 (ACQ/PEAKUP) 480.84 114.14 P
5 F
0.22 ( and) 540.84 114.14 P
1.09 (indicate the lines to which it applies \050all of which should use the same aperture\051.) 221.4 102.14 P
72 87.98 558 686.02 C
140.85 466.81 489.15 484.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(t) 276.32 475.6 T
6 7 Q
(e) 279.48 472.5 T
(x) 283.12 472.5 T
(p) 286.77 472.5 T
5 10 Q
(1) 311.86 475.6 T
(2) 316.86 475.6 T
(8) 321.86 475.6 T
6 F
(N) 337.35 475.6 T
6 7 Q
(M) 344.4 472.5 T
(A) 350.77 472.5 T
(P) 355.58 472.5 T
12 10 Q
(\264) 329.36 475.6 T
6 F
(N) 370.5 475.6 T
6 7 Q
(S) 377.55 472.5 T
(E) 381.59 472.5 T
(A) 386.4 472.5 T
(R) 391.22 472.5 T
(C) 396.03 472.5 T
(H) 401.24 472.5 T
5 10 Q
(+) 362.36 475.6 T
12 F
(\050) 307.57 475.6 T
(\051) 406.75 475.6 T
8 F
(S) 422.24 475.6 T
(T) 428.24 475.6 T
(E) 434.24 475.6 T
(P) 440.24 475.6 T
(-) 446.24 475.6 T
(T) 452.24 475.6 T
(I) 458.24 475.6 T
(M) 464.24 475.6 T
(E) 470.24 475.6 T
12 F
(\264) 414.25 475.6 T
5 F
(=) 295.27 475.6 T
72 87.98 558 686.02 C
0 0 612 792 C
248.69 434.81 383.81 450.94 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(N) 249.33 440.14 T
6 7 Q
(S) 256.38 437.04 T
(E) 260.42 437.04 T
(A) 265.23 437.04 T
(R) 270.05 437.04 T
(C) 274.86 437.04 T
(H) 280.07 437.04 T
8 10 Q
(S) 306.71 440.14 T
(E) 312.71 440.14 T
(A) 318.71 440.14 T
(R) 324.71 440.14 T
(C) 330.71 440.14 T
(H) 336.71 440.14 T
(-) 342.71 440.14 T
(S) 348.71 440.14 T
(I) 354.71 440.14 T
(Z) 360.71 440.14 T
(E) 366.71 440.14 T
12 F
(\050) 302.42 440.14 T
(\051) 373.17 440.14 T
5 7 Q
(2) 378.67 443.02 T
5 10 Q
(=) 290.12 440.14 T
0 0 612 792 C
475.49 434.81 499.98 447.98 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(N) 475.98 440.14 T
6 7 Q
(M) 483.03 437.04 T
(A) 489.39 437.04 T
(P) 494.21 437.04 T
0 0 612 792 C
509.27 422.81 547.03 435.98 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(N) 509.75 428.14 T
6 7 Q
(S) 516.8 425.04 T
(E) 520.84 425.04 T
(A) 525.66 425.04 T
(R) 530.47 425.04 T
(C) 535.29 425.04 T
(H) 540.49 425.04 T
0 0 612 792 C
221.4 244 495 271 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(t) 305.09 255.14 T
6 7 Q
(e) 308.25 252.04 T
(x) 311.89 252.04 T
(p) 315.54 252.04 T
6 10 Q
(f) 334.67 255.14 T
6 7 Q
(A) 337.84 252.04 T
(p) 342.65 252.04 T
(e) 346.69 252.04 T
(r) 350.33 252.04 T
(t) 353.6 252.04 T
(u) 356.08 252.04 T
(r) 360.12 252.04 T
(e) 363.38 252.04 T
8 10 Q
(S) 376.98 255.14 T
(T) 382.98 255.14 T
(E) 388.98 255.14 T
(P) 394.98 255.14 T
(-) 400.98 255.14 T
(T) 406.98 255.14 T
(I) 412.98 255.14 T
(M) 418.98 255.14 T
(E) 424.98 255.14 T
12 F
(\264) 368.99 255.14 T
5 F
(=) 324.04 255.14 T
0 0 612 792 C
FMENDPAGE
%%EndPage: "41" 9
%%Page: "42" 10
612 792 0 FMBEGINPAGE
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[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
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[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Y) 189 736.18 T
(our Phase II Proposal) 194.34 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(42) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
5 F
0.68 (Also indicate a) 203.4 679.35 P
8 F
1.64 (NO) 267.94 679.35 P
1.64 (GAP) 283.12 679.35 P
5 F
0.68 ( Special Requirement for that group of lines. Then specify) 301.12 679.35 P
0.36 (another) 203.4 667.35 P
8 F
0.87 (ACQ/PEAKUP) 236.25 667.35 P
5 F
0.36 ( before starting observations in the other aperture, and again) 296.25 667.35 P
(specify) 203.4 655.35 T
8 F
(NO) 234.78 655.35 T
(GAP) 249.28 655.35 T
5 F
( to ensure that they are treated as a group.) 267.28 655.35 T
54 612.02 540 615.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 613.52 540 613.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 613.52 180 613.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(4.2) 163.32 619.02 T
(Image Mode) 189 619.02 T
5 10 Q
0.29 (The GHRS is, of course, primarily a spectrograph, but it includes useful imaging capa-) 189 595.35 P
0.65 (bilities, especially because the detectors of the GHRS are blind to much of the visible) 189 583.35 P
0.25 (light that dominates the \337ux of most stars. Y) 189 571.35 P
0.25 (ou may wish to request an) 368.07 571.35 P
8 F
0.6 (IMAGE) 476.78 571.35 P
5 F
0.25 ( or) 506.78 571.35 P
8 F
0.6 (MAP) 520.61 571.35 P
5 F
0.25 (,) 537.5 571.35 P
-0.02 (for example, to con\336rm that the telescope had your object properly centered in the data-) 189 559.35 P
(taking aperture before the exposure was taken.) 189 547.35 T
(Note the following in using the imaging capability:) 189 527.35 T
7 11 Q
(\245) 189 509.35 T
5 10 Q
1.18 (GHRS) 203.4 509.35 P
8 F
2.84 (IMAGE) 233.75 509.35 P
5 F
1.18 (s and) 263.75 509.35 P
8 F
2.84 (MAP) 289.45 509.35 P
5 F
1.18 (s are obtained with the focus diodes \050see Section) 307.45 509.35 P
1.18 (6.3 on) 513.82 509.35 P
1.87 (page) 203.4 497.35 P
1.87 (62\051 at the ends of the array of main science diodes. The focus diodes are) 224.78 497.35 P
1.47 (smaller and square, making them more useful for focusing, but at the price of a) 203.4 485.35 P
-0.24 (lower count rate. The total count rate over the LSA is, of course, unchanged, and it is) 203.4 473.35 P
0.18 (that which is predicted with the information in Section) 203.4 461.35 P
0.18 (7.1 on page) 425.67 461.35 P
0.18 (68. Multiply the) 474.91 461.35 P
1.24 (count rate estimated for the regular diodes by approximately 0.3 to get the value) 203.4 449.35 P
(appropriate to the focus diodes when they are centered on the star) 203.4 437.35 T
(.) 465.28 437.35 T
7 11 Q
(\245) 189 422.35 T
5 10 Q
0.02 (A) 203.4 422.35 P
8 F
0.05 (MAP) 213.14 422.35 P
5 F
0.02 ( is obtained as an integral part of an acquisition whereas an) 231.14 422.35 P
8 F
0.05 (IMAGE) 470.23 422.35 P
5 F
0.02 ( is a sepa-) 500.23 422.35 P
-0.24 (rate observation that may or may not have anything to do with an acquisition. A) 203.4 410.35 P
8 F
-0.57 (MAP) 522 410.35 P
5 F
0.64 (with) 203.4 398.35 P
8 F
1.53 (SEARCH-SIZE=3) 224.32 398.35 P
5 F
0.64 ( or) 302.32 398.35 P
8 F
1.53 (5) 316.92 398.35 P
5 F
0.64 ( is made as the acquisition procedure causes the tele-) 322.92 398.35 P
0.1 (scope to make small motions in a square spiral pattern, thereby enabling it to record) 203.4 386.35 P
0.2 (a lar) 203.4 374.35 P
0.2 (ger portion of the sky than the LSA itself subtends. An) 220.91 374.35 P
8 F
0.47 (IMAGE) 444.71 374.35 P
5 F
0.2 ( can only record) 474.71 374.35 P
1.47 (the light in the) 203.4 362.35 P
1.47 ( arcsec region of the LSA. A single) 317.32 362.35 P
8 F
3.54 (MAP) 472.7 362.35 P
5 F
1.47 ( \050) 490.7 362.35 P
8 F
3.54 (SEARCH-) 498 362.35 P
3.02 (SIZE=1) 203.4 350.35 P
5 F
1.26 (\051 is equivalent to an) 239.4 350.35 P
8 F
3.02 (IMAGE) 327.07 350.35 P
5 F
1.26 (. Note that) 357.07 350.35 P
8 F
3.02 (MAP=ALL-POINTS) 405.29 350.35 P
5 F
1.26 ( may not be) 489.29 350.35 P
(used with an) 203.4 338.35 T
8 F
(ONBOARD) 256.45 338.35 T
(ACQ) 300.95 338.35 T
5 F
(.) 318.95 338.35 T
7 11 Q
(\245) 189 323.35 T
5 10 Q
1.49 (A standard) 203.4 323.35 P
8 F
3.57 (IMAGE) 252.48 323.35 P
5 F
1.49 ( will have a pixel spacing of 0.109 arcsec and will cover the) 282.48 323.35 P
1.13 (entire LSA aperture of 1.74) 203.4 311.35 P
12 F
1.13 ( \264) 318.16 311.35 P
5 F
1.13 (1.74 arcsec. Y) 330.91 311.35 P
1.13 (ou may also select pixel spacings of) 389.36 311.35 P
1.13 (0.055 or 0.027 arcsec, with proportionately smaller regions of the sky covered in) 203.4 299.35 P
(a) 203.4 287.35 T
( \050the default\051) 240.32 287.35 T
8 F
(IMAGE) 294.47 287.35 T
5 F
(. Y) 324.47 287.35 T
(ou may also use) 335.69 287.35 T
8 F
(IMAGE) 402.35 287.35 T
5 F
( with the SSA.) 432.35 287.35 T
0 F
(4.2.1) 157.76 257.35 T
(Image Mode Parameters) 189 257.35 T
7 11 Q
(\245) 189 241.35 T
5 10 Q
-0.16 (Either the LSA \050\322) 203.4 241.35 P
8 F
-0.39 (2.0) 273.73 241.35 P
5 F
-0.16 (\323\051 or SSA \050\322) 291.73 241.35 P
8 F
-0.39 (0.25) 340.96 241.35 P
5 F
-0.16 (\323\051 may be selected as the aperture. The SSA) 364.96 241.35 P
0.81 (is so small that it is generally pointless to image it, although there may be special) 203.4 229.35 P
2.57 (cases where) 203.4 217.35 P
8 F
6.16 (IMAGE) 259.07 217.35 P
5 F
2.57 ( mode is of use, particularly for con\336rming pointing in a) 289.07 217.35 P
(crowded \336eld.) 203.4 205.35 T
7 11 Q
(\245) 189 190.35 T
5 10 Q
-0.23 (A mirror is the usual choice as optical element. A grating may also be speci\336ed \320 see) 203.4 190.35 P
(below) 203.4 178.35 T
(.) 227.19 178.35 T
7 11 Q
(\245) 189 163.35 T
5 10 Q
1.21 (The number of pixels in the) 203.4 163.35 P
6 F
1.21 (x) 323.95 163.35 P
5 F
1.21 ( and) 328.39 163.35 P
6 F
1.21 (y) 350.24 163.35 P
5 F
1.21 ( directions can be chosen separately and can) 354.68 163.35 P
0 (range from 1 to 512 pixels. However) 203.4 151.35 P
0 (, a lar) 350.48 151.35 P
0 (ge number of pixels only oversamples the) 372.79 151.35 P
0.22 (region of sky subtended by the LSA and does not make the) 203.4 139.35 P
8 F
0.51 (IMAGE) 444.84 139.35 P
5 F
0.22 ( include a lar) 474.84 139.35 P
0.22 (ger) 527.23 139.35 P
-0.12 (area. The parameters to specify are) 203.4 127.35 P
8 F
-0.28 (NX) 345.14 127.35 P
5 F
-0.12 (,) 357.14 127.35 P
8 F
-0.28 (NY) 362.02 127.35 P
5 F
-0.12 (,) 372.73 127.35 P
8 F
-0.28 (DELTA-X) 377.61 127.35 P
5 F
-0.12 (, and) 419.61 127.35 P
8 F
-0.28 (DELTA-Y) 441.32 127.35 P
5 F
-0.12 (, for which the) 482.03 127.35 P
-0.16 (defaults are 16, 16, 4, and 4, respectively) 203.4 115.35 P
-0.16 (. The product of) 365.78 115.35 P
8 F
-0.38 (NX) 432.08 115.35 P
5 F
-0.16 ( and) 444.08 115.35 P
8 F
-0.38 (NY) 463.21 115.35 P
5 F
-0.16 ( may not exceed) 475.21 115.35 P
-0.04 (512. An image that is critically sampled in the) 203.4 103.35 P
6 F
-0.04 (x) 390.26 103.35 P
5 F
-0.04 ( direction may be obtained by speci-) 394.7 103.35 P
(fying) 203.4 91.35 T
8 F
(NX=32) 227.01 91.35 T
5 F
(,) 257.01 91.35 T
8 F
(NY=16) 262.01 91.35 T
5 F
(,) 292.01 91.35 T
8 F
(DELTA-X=2) 297.01 91.35 T
5 F
(, and) 351.01 91.35 T
8 F
(DELTA-Y=4) 372.95 91.35 T
5 F
(.) 426.95 91.35 T
269.86 359.18 317.32 370.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 270.35 362.35 T
(.) 275.35 362.35 T
(7) 277.85 362.35 T
(4) 282.85 362.35 T
(1) 298.33 362.35 T
(.) 303.33 362.35 T
(7) 305.83 362.35 T
(4) 310.83 362.35 T
12 F
(\264) 290.35 362.35 T
0 0 612 792 C
207.84 284.18 240.32 295.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 208.33 287.35 T
(6) 213.33 287.35 T
(1) 228.82 287.35 T
(6) 233.82 287.35 T
12 F
(\264) 220.83 287.35 T
0 0 612 792 C
FMENDPAGE
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612 792 0 FMBEGINPAGE
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7 FrameSetSepColors
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (43) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Y) 207 736.18 T
(our Phase II Proposal) 212.34 736.18 T
5 10 Q
0.93 (Only the N1 mirror intercepts the full beam diameter) 221.4 679.35 P
0.93 (, meaning that images of the) 440.05 679.35 P
-0.15 (LSA with the other acquisition mirrors will not yield an accurate Point Spread Func-) 221.4 667.35 P
(tion \050PSF\051.) 221.4 655.35 T
7 11 Q
(\245) 207 640.35 T
5 10 Q
1.05 (The) 221.4 640.35 P
8 F
2.52 (PRECISION) 240.5 640.35 P
5 F
1.05 ( parameter may be speci\336ed as) 294.5 640.35 P
8 F
2.52 (NORMAL) 426.32 640.35 P
5 F
1.05 ( \050the default\051 or) 462.32 640.35 P
8 F
2.52 (HIGH) 531.5 640.35 P
5 F
1.05 (.) 555.5 640.35 P
8 F
3.63 (PRECISION) 221.4 628.35 P
5 F
1.51 ( may only be speci\336ed if) 275.4 628.35 P
8 F
3.63 (DELTA-Y=4) 385.58 628.35 P
5 F
1.51 (. Using) 439.58 628.35 P
8 F
3.63 (PRECISION=HIGH) 474 628.35 P
5 F
0.59 (causes the image to be obtained with only one focus diode instead of two \050thereby) 221.4 616.35 P
-0.09 (eliminating uncertainty over the relative response of the two\051, but the time per expo-) 221.4 604.35 P
-0.06 (sure you must list is the same in either case \050but using) 221.4 592.35 P
8 F
-0.14 (PRECISION=NORMAL) 439.01 592.35 P
5 F
-0.06 ( takes) 535.01 592.35 P
-0.23 (less actual time to execute and the dif) 221.4 580.35 P
-0.23 (ferences in response of the diodes are known to) 369.87 580.35 P
(be small\051.) 221.4 568.35 T
7 11 Q
(\245) 207 553.35 T
5 10 Q
1.29 (There are two focus diodes available to raster over the LSA. Thus the total time) 221.4 553.35 P
0.59 (needed is the dwell time per pixel \0500.2 seconds is the default\051 times the number of) 221.4 541.35 P
0.35 (pixels in the) 221.4 529.35 P
6 F
0.35 (x) 273.84 529.35 P
5 F
0.35 ( direction \050default is) 278.28 529.35 P
8 F
0.84 (NX=16) 363 529.35 P
5 F
0.35 (\051 times the number of) 393 529.35 P
6 F
0.35 (y) 483.35 529.35 P
5 F
0.35 ( pixels \050default is) 487.79 529.35 P
8 F
1.22 (NY=16) 221.4 517.35 P
5 F
0.51 (\051, all divided by 2. The maximum permissible dwell time per pixel is 12.75) 251.4 517.35 P
0.67 (seconds. \050Note that the) 221.4 505.35 P
6 F
0.67 (Phase II Pr) 318.22 505.35 P
0.67 (oposal Instructions) 365.29 505.35 P
5 F
0.67 ( for Cycle 4 required you to) 442.9 505.35 P
1.84 (calculate the total time without dividing by the factor of two. The situation for) 221.4 493.35 P
(Cycle) 221.4 481.35 T
(5 should be con\336rmed before a value is entered.\051) 247.23 481.35 T
0 F
(4.2.2) 175.76 451.35 T
(The GHRS as a Slitless Spectrograph) 207 451.35 T
5 F
0.24 (In) 207 431.35 P
8 F
0.57 (IMAGE) 218.07 431.35 P
5 F
0.24 ( mode you may specify a grating instead of a mirror as the spectrum element) 248.07 431.35 P
0.58 (\050note that this may) 207 419.35 P
6 F
0.58 (not) 286.54 419.35 P
5 F
0.58 ( be done in Acquisition Mode\051. Doing so for a tar) 299.32 419.35 P
0.58 (get that emits) 502.95 419.35 P
0.79 (primarily in lines can yield the equivalent of using a slitless spectrograph over a very) 207 407.35 P
1.31 (small portion of the sky \050the 1.74 arcsec square region of the LSA\051. Thus the focus) 207 395.35 P
0.59 (diodes would be swept over the image of the line to produce a picture that is resolved) 207 383.35 P
1.01 (spatially in the) 207 371.35 P
6 F
1.01 (y) 271.41 371.35 P
5 F
1.01 ( direction and spectroscopically in the) 275.85 371.35 P
6 F
1.01 (x) 436.31 371.35 P
5 F
1.01 ( direction. This mode of use) 440.75 371.35 P
1.04 (would be very slow if all you wanted was the spatial structure of a small object \050the) 207 359.35 P
0.38 (FOC would probably be better\051, but there might be interesting uses for obtaining spec-) 207 347.35 P
-0.03 (trophotometrically pure, spatially resolved images in the ultraviolet. Please consult us if) 207 335.35 P
(you wish to explore this option.) 207 323.35 T
72 280.02 558 283.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 281.52 558 281.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 281.52 198 281.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(4.3) 181.32 287.02 T
(Accumulation Mode) 207 287.02 T
0 10 Q
(4.3.1) 175.76 253.35 T
(Optimizing Data Quality) 207 253.35 T
5 F
0.5 (The previous chapter provided the information needed to estimate an exposure time to) 207 233.35 P
0.57 (achieve a given level of signal-to-noise. W) 207 221.35 P
0.57 (e reiterate several factors having to do with) 380.98 221.35 P
-0.15 (the detectors that must be taken into account to achieve the best data quality) 207 209.35 P
-0.15 (. Note that it) 508.46 209.35 P
0.2 (is not necessary to explicitly specify these parameters \050except for) 207 197.35 P
8 F
0.49 (FP-SPLIT) 472.32 197.35 P
5 F
0.2 (\051 because) 520.32 197.35 P
-0.13 (the defaults that apply to each mode of operation will automatically invoke them. More-) 207 185.35 P
(over) 207 173.35 T
(, you should not deviate from the defaults without good reason.) 224.37 173.35 T
1.19 (The Digicon detectors have faceplates with some granularity \050uneven response\051. The) 207 153.35 P
0.06 (diodes onto which the faceplate is imaged also have response irregularities and some of) 207 141.35 P
0.58 (them have been turned of) 207 129.35 P
0.58 (f because of misbehavior) 310.79 129.35 P
0.58 (. Both of these ef) 412.23 129.35 P
0.58 (fects are relatively) 482.98 129.35 P
0.05 (small but enough to prevent you from obtaining a spectrum with S/N much in excess of) 207 117.35 P
2.25 (50. They can also produce \322glitches\323 that can mimic spectrum features. The) 207 105.35 P
8 F
5.39 (FP-) 540 105.35 P
-0.19 (SPLIT) 207 93.35 P
5 F
-0.08 ( parameter causes the carrousel to move slightly between each of the two or four) 237 93.35 P
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
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[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
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0 0 0 1 0 0 0 K
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0 9 Q
(Y) 189 736.18 T
(our Phase II Proposal) 194.34 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(44) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
5 F
0.5 (separate subexposures. The) 189 679.35 P
8 F
1.21 (COMB) 302.7 679.35 P
5 F
0.5 ( parameter suppresses diode-to-diode gain variations) 326.7 679.35 P
-0.2 (and allows one to work around the dead diodes. Both features should be used, especially) 189 667.35 P
(since they cost little or nothing in exposure time and improve data quality) 189 655.35 T
(.) 483.33 655.35 T
2.09 (The Digicon diodes also undersample the spectrum by about a factor of two. The) 189 635.35 P
0.54 (parameter) 189 623.35 P
8 F
1.3 (STEP-PATT) 232.02 623.35 P
5 F
0.54 ( causes electronic motions of the spectrum so as to sample the) 286.02 623.35 P
0.87 (spectrum fully) 189 611.35 P
0.87 (. It is possible to) 247.26 611.35 P
8 F
2.08 (STEP-PATT) 319.93 611.35 P
5 F
0.87 ( at two samples per diode width, but we) 373.93 611.35 P
0.37 (recommend using four samples per diode to yield optimum results, and again at no net) 189 599.35 P
0.91 (cost. Y) 189 587.35 P
0.91 (ou can always rebin a quarter) 217.24 587.35 P
0.91 (-stepped spectrum into a half-stepped one during) 339.04 587.35 P
1.29 (your data analysis, but the process cannot make a quarter) 189 575.35 P
1.29 (-stepped spectrum out of a) 428.73 575.35 P
2.18 (half-stepped one. Deconvolution has worked best with quarter) 189 563.35 P
2.18 (-stepped spectra \050the) 452.89 563.35 P
0.22 (default\051; see Gilliland et al. \0501992\051.) 189 551.35 P
8 F
0.53 (STEP-PATT) 333.64 551.35 P
5 F
0.22 ( also determines the way in which the) 387.64 551.35 P
(background is measured \050see Section) 189 539.35 T
(8.4 on page) 339.8 539.35 T
(92\051.) 388.68 539.35 T
0.97 (W) 189 519.35 P
0.97 (e also remind you to break up long exposures into subexposures that are no longer) 197.64 519.35 P
-0.03 (than about 5 minutes each, so as to defeat the ef) 189 507.35 P
-0.03 (fects of geomagnetically-induced image) 379.86 507.35 P
1.94 (motion. Bear in mind that a 20 minute exposure, for example, speci\336ed with) 189 495.35 P
8 F
4.66 (FP-) 522 495.35 P
(SPLIT=4) 189 483.35 T
5 F
( will result in four 5-minute exposures.) 231 483.35 T
0 F
(4.3.2) 157.76 453.35 T
(Summary of Accumulation Mode Parameters) 189 453.35 T
7 11 Q
(\245) 189 437.35 T
5 10 Q
0.64 (Specify the aperture as \322) 203.4 437.35 P
8 F
1.54 (2.0) 304.27 437.35 P
5 F
0.64 (\323 \050LSA\051 or \322) 322.27 437.35 P
8 F
1.54 (0.25) 374.46 437.35 P
5 F
0.64 (\323 \050SSA\051. The object will automati-) 398.46 437.35 P
0.12 (cally be moved to the correct aperture even if the acquisition was into the other) 203.4 425.35 P
0.12 (. If a) 521.16 425.35 P
0.62 (SSA spectroscopic observation follows an LSA spectroscopic observation, we rec-) 203.4 413.35 P
-0.19 (ommend an) 203.4 401.35 P
8 F
-0.47 (ACQ/PEAKUP) 252.45 401.35 P
5 F
-0.19 ( in the SSA with) 312.45 401.35 P
8 F
-0.47 (SEARCH-SIZE=5) 380.1 401.35 P
5 F
-0.19 ( before beginning an) 458.1 401.35 P
8 F
(ACCUM) 203.4 389.35 T
5 F
(.) 233.4 389.35 T
7 11 Q
(\245) 189 374.35 T
5 10 Q
2.55 (If wavelength accuracy is needed that exceeds the default \050see Section) 203.4 374.35 P
2.55 (4.5 on) 512.45 374.35 P
1.39 (page) 203.4 362.35 P
1.39 (46\051, then specify) 224.78 362.35 P
8 F
3.34 (WAVE) 298.38 362.35 P
5 F
1.39 ( as the tar) 322.38 362.35 P
1.39 (get with an aperture of) 364.97 362.35 P
8 F
3.34 (SC2) 464.95 362.35 P
5 F
1.39 (. Get a) 482.95 362.35 P
8 F
3.34 (WAVE) 516 362.35 P
6 F
(befor) 203.4 350.35 T
(e) 224.14 350.35 T
5 F
( the) 228.58 350.35 T
8 F
(ACCUM) 245.8 350.35 T
5 F
( to which it is to apply) 275.8 350.35 T
(.) 364.6 350.35 T
7 11 Q
(\245) 189 335.35 T
5 10 Q
0.65 (Specify the grating to be used, either \336rst-order or echelle. If you wish to force an) 203.4 335.35 P
0.33 (echelle observation to be done in an order other than the default, you may do so by) 203.4 323.35 P
(specifying the grating as, for example,) 203.4 311.35 T
8 F
(ECH-B24) 359.48 311.35 T
5 F
(, where 24 was the order chosen.) 401.48 311.35 T
7 11 Q
(\245) 189 296.35 T
8 10 Q
-0.35 (STEP-PATT) 203.4 296.35 P
5 F
-0.15 ( may be chosen as a number from 1 to 15, and speci\336c pattern numbers) 257.4 296.35 P
0.5 (go with speci\336c spectrograph con\336gurations. W) 203.4 284.35 P
0.5 (e recommend using the default that) 396.71 284.35 P
1.05 (pertains to the setup you have chosen. The details of how the substepping is per-) 203.4 272.35 P
(formed and the background measured are given in Section) 203.4 260.35 T
(8.4 on page) 439.18 260.35 T
(92.) 488.06 260.35 T
7 11 Q
(\245) 189 245.35 T
8 10 Q
2.31 (FP-SPLIT=STD) 203.4 245.35 P
5 F
0.96 ( is recommended. The default for) 275.4 245.35 P
8 F
2.31 (FP-SPLIT) 416.98 245.35 P
5 F
0.96 ( is) 464.98 245.35 P
8 F
2.31 (NO) 478.57 245.35 P
5 F
0.96 (, which will) 490.57 245.35 P
6 F
(not) 203.4 233.35 T
5 F
( yield a spectrum with the best signal-to-noise.) 216.18 233.35 T
7 11 Q
(\245) 189 218.35 T
8 10 Q
(COMB=FOUR) 203.4 218.35 T
5 F
( is the default value and is recommended for the best results.) 257.4 218.35 T
7 11 Q
(\245) 189 203.35 T
8 10 Q
6.11 (DOPPLER=DEF) 203.4 203.35 P
5 F
2.55 ( is recommended. This activates compensation for the velocity) 269.4 203.35 P
0.29 (shifts of astronomical spectra over the course of an orbit but turns it of) 203.4 191.35 P
0.29 (f for internal) 488.88 191.35 P
(exposures.) 203.4 179.35 T
7 11 Q
(\245) 189 164.35 T
8 10 Q
3.15 (STEP-TIME) 203.4 164.35 P
5 F
1.32 ( may be speci\336ed as a number from 0.2 to 12.75 seconds, in incre-) 257.4 164.35 P
0.31 (ments of 0.05 seconds.) 203.4 152.35 P
8 F
0.75 (STEP-TIME) 298.54 152.35 P
5 F
0.31 ( speci\336es the length of the individual subspec-) 352.54 152.35 P
0.63 (tra that are accumulated to form the \336nal spectrum, and there is no good reason to) 203.4 140.35 P
(not use the default of 0.2 sec.) 203.4 128.35 T
7 11 Q
(\245) 189 113.35 T
5 10 Q
-0.08 (The) 203.4 113.35 P
8 F
-0.2 (CENSOR) 221.37 113.35 P
5 F
-0.08 ( parameter may also be speci\336ed. The default is) 257.37 113.35 P
8 F
-0.2 (NO) 449.92 113.35 P
5 F
-0.08 (, which is appropri-) 461.92 113.35 P
0.41 (ate in almost all cases. If) 203.4 101.35 P
8 F
0.99 (CENSOR=YES) 307.26 101.35 P
5 F
0.41 ( is used, individual subspectra \050of duration) 367.26 101.35 P
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (45) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Y) 207 736.18 T
(our Phase II Proposal) 212.34 736.18 T
8 10 Q
4.64 (STEP-TIME) 221.4 679.35 P
5 F
1.93 (, which should be used at the default value of 0.2s\051 are examined) 275.4 679.35 P
0.56 (onboard the spacecraft and are discarded if multiple counts have occurred within a) 221.4 667.35 P
0.65 (8) 221.4 655.35 P
12 F
0.65 (m) 228.9 655.35 P
5 F
0.65 (s interval. This allows for the lowering of background noise in cases where the) 234.66 655.35 P
0.89 (object being observed is very faint, i.e., less than about 0.1 counts per second per) 221.4 643.35 P
2.04 (diode. Rejected exposures are repeated by the GHRS, leading to a longer total) 221.4 631.35 P
0.32 (elapsed time for the observation, but only by about 2%. Since the observation must) 221.4 619.35 P
0.5 (end at a speci\336c time that is predetermined in the spacecraft schedule, using) 221.4 607.35 P
8 F
1.21 (CEN-) 534 607.35 P
-0.48 (SOR) 221.4 595.35 P
5 F
-0.2 ( involves a risk of losing all the data if too many subexposures are rejected. This) 239.4 595.35 P
-0.05 (is guarded against by adding some padding time in the observation planning process) 221.4 583.35 P
1.58 (\050that is done at STScI and does not af) 221.4 571.35 P
1.58 (fect the exposure time you estimate\051. See) 383.83 571.35 P
(Section) 221.4 559.35 T
(8.6.2 on page) 253.9 559.35 T
(95 for more information on) 310.28 559.35 T
8 F
(CENSOR) 422.21 559.35 T
5 F
(.) 458.21 559.35 T
7 11 Q
(\245) 207 544.35 T
5 10 Q
1.14 (A special commanding option called) 221.4 544.35 P
8 F
2.73 (FLYLIM) 376.25 544.35 P
5 F
1.14 ( can also be used to reject noise in) 412.25 544.35 P
0.91 (cases where the object is substantially fainter than the background. Please consult) 221.4 532.35 P
(with us if you wish to explore this possibility) 221.4 520.35 T
(.) 401.32 520.35 T
7 11 Q
(\245) 207 505.35 T
5 10 Q
0.75 (If you have any doubts about the manner in which your program will be executed) 221.4 505.35 P
2.13 (\050which spectra \336rst, whether a peakup is done, etc.\051, remove the ambiguity by) 221.4 493.35 P
3.46 (explicitly indicating the nature and order of the exposures on the Exposure) 221.4 481.35 P
(Logsheet.) 221.4 469.35 T
0 F
(4.3.3) 175.76 439.35 T
7 F
(WSCAN) 207 439.35 T
0 F
( mode) 237 439.35 T
5 F
0.16 (Use of) 207 419.35 P
8 F
0.39 (WSCAN) 236.21 419.35 P
5 F
0.16 ( can result in a spectrum covering a broader total bandpass than is possi-) 266.21 419.35 P
0.37 (ble with a single exposure. All the parameters listed above for an) 207 407.35 P
8 F
0.9 (ACCUM) 473.94 407.35 P
5 F
0.37 ( exposure are) 503.94 407.35 P
0.7 (available in) 207 395.35 P
8 F
1.68 (WSCAN) 257.28 395.35 P
5 F
0.7 ( mode. The most important parameter to specify is) 287.28 395.35 P
8 F
1.68 (WAVE-STEP,) 498 395.35 P
5 F
0.5 (which is the spacing \050in \201ngstroms\051 between each subexposure. If) 207 383.35 P
8 F
1.2 (WAVE-STEP=DEF) 480 383.35 P
5 F
0.04 (is speci\336ed, the central wavelengths of the separate exposures will be equally spaced so) 207 371.35 P
0.71 (as to cover the range of wavelengths that you specify) 207 359.35 P
0.71 (, with at least 20% overlap from) 425.17 359.35 P
(one subspectrum to the next.) 207 347.35 T
0.16 (Y) 207 327.35 P
0.16 (ou may also explicitly give a) 213.22 327.35 P
8 F
0.38 (WAVE-STEP) 331.95 327.35 P
5 F
0.16 ( value. If) 385.95 327.35 P
0.16 ( is the central wavelength of) 444.17 327.35 P
1.1 (the shortest-wavelength exposure, and) 207 315.35 P
1.1 ( is the central wavelength of the longest-) 387.8 315.35 P
0.94 (wavelength exposure, then choose these values in concert with) 207 303.35 P
8 F
2.24 (WAVE-STEP) 468.7 303.35 P
5 F
0.94 ( so as to) 522.7 303.35 P
(yield an integral number of) 207 291.35 T
8 F
(WAVE-STEP) 318.37 291.35 T
5 F
(s between) 372.37 291.35 T
( and) 434.01 291.35 T
(.) 474.04 291.35 T
0 F
(4.3.4) 175.76 261.35 T
7 F
(OSCAN) 207 261.35 T
0 F
( mode) 237 261.35 T
5 F
0.12 (This mode makes it possible to scan across echelle orders at a \336xed value of) 207 241.35 P
6 F
0.12 (m) 515.74 241.35 P
12 F
0.12 (l) 522.96 241.35 P
5 F
0.12 (, where) 528.45 241.35 P
6 F
0.3 (m) 207 229.35 P
5 F
0.3 ( is the order number and) 214.22 229.35 P
12 F
0.3 (l) 315.98 229.35 P
5 F
0.3 ( is the wavelength. It is rare that adjacent orders both have) 321.46 229.35 P
0.1 (features of astrophysical interest and so this mode is primarily used for calibrations and) 207 217.35 P
0.57 (not for science observations. If you do use this mode, all the parameters of an) 207 205.35 P
8 F
1.37 (ACCUM) 528 205.35 P
5 F
(observation are available.) 207 193.35 T
72 150.02 558 153.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 151.52 558 151.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 151.52 198 151.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(4.4) 181.32 157.02 T
(Rapid Readout Mode) 207 157.02 T
5 10 Q
0.42 (This mode is sometimes referred to as Direct Downlink. A normal) 207 133.35 P
8 F
1.01 (ACCUM) 479.39 133.35 P
5 F
0.42 ( exposure is) 509.39 133.35 P
1.16 (the best way to get a good spectrum because all the features of the spectrograph are) 207 121.35 P
1.38 (available to you: automatic compensation for the motion of the spacecraft along the) 207 109.35 P
2.35 (line-of-sight, rejection of high-noise subspectra with) 207 97.35 P
8 F
5.63 (CENSOR) 433.54 97.35 P
5 F
2.35 (, use of) 469.54 97.35 P
8 F
5.63 (FP-SPLIT) 508.24 97.35 P
5 F
2.35 (,) 555.5 97.35 P
424.74 321.29 444.17 335.01 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
12 10 Q
0 X
0 0 0 1 0 0 0 K
(l) 425.23 327.35 T
6 7 Q
(m) 431.11 324.25 T
(i) 436.7 324.25 T
(n) 439.18 324.25 T
0 0 612 792 C
367.21 309.29 387.8 323.01 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
12 10 Q
0 X
0 0 0 1 0 0 0 K
(l) 367.71 315.35 T
6 7 Q
(m) 373.58 312.25 T
(a) 379.17 312.25 T
(x) 383.21 312.25 T
0 0 612 792 C
414.58 285.29 434.01 299.01 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
12 10 Q
0 X
0 0 0 1 0 0 0 K
(l) 415.07 291.35 T
6 7 Q
(m) 420.94 288.25 T
(i) 426.53 288.25 T
(n) 429.02 288.25 T
0 0 612 792 C
453.45 285.29 474.04 299.01 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
12 10 Q
0 X
0 0 0 1 0 0 0 K
(l) 453.94 291.35 T
6 7 Q
(m) 459.81 288.25 T
(a) 465.4 288.25 T
(x) 469.44 288.25 T
0 0 612 792 C
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612 792 0 FMBEGINPAGE
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[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Y) 189 736.18 T
(our Phase II Proposal) 194.34 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(46) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
8 F
1.12 (COMB) 189 679.35 P
5 F
0.47 (, and) 213 679.35 P
8 F
1.12 (STEP-PATT) 235.87 679.35 P
5 F
0.47 ( to optimize data quality) 289.87 679.35 P
0.47 (, and so on. However) 388.3 679.35 P
0.47 (, there are times) 474.74 679.35 P
-0.04 (when) 189 667.35 P
8 F
-0.1 (ACCUM) 213.12 667.35 P
5 F
-0.04 ( cannot obtain successive spectra as quickly as is needed to probe a partic-) 243.12 667.35 P
(ular phenomenon.) 189 655.35 T
0.1 (In those cases you can use) 189 635.35 P
8 F
0.23 (RAPID) 297.33 635.35 P
5 F
0.1 ( mode. The data are read from the detector at the end) 327.33 635.35 P
0.22 (of each short integration, either to the science tape recorder on) 189 623.35 P
6 F
0.22 (HST) 443.52 623.35 P
5 F
0.22 ( or through TDRSS) 461.3 623.35 P
0.51 (to the ground. Data obtained in) 189 611.35 P
8 F
1.22 (RAPID) 318.98 611.35 P
5 F
0.51 ( mode require special handling by the observer) 348.98 611.35 P
0.16 (to correct for some of the ef) 189 599.35 P
0.16 (fects \050especially doppler shifts\051 that are automatically com-) 301.42 599.35 P
(pensated for in) 189 587.35 T
8 F
(ACCUM) 250.93 587.35 T
5 F
( mode.) 280.93 587.35 T
-0.13 (As for an) 189 567.35 P
8 F
-0.31 (ACCUM) 228.32 567.35 P
5 F
-0.13 (, you should specify the science aperture and the spectral element. Y) 258.32 567.35 P
-0.13 (ou) 530 567.35 P
0.85 (may also choose to observe) 189 555.35 P
8 F
2.05 (WAVE) 305.75 555.35 P
5 F
0.85 ( as tar) 329.75 555.35 P
0.85 (get to get a wavelength calibration. The only) 355.16 555.35 P
0.43 (other parameter you may specify is) 189 543.35 P
8 F
1.04 (SAMPLE-TIME) 334.89 543.35 P
5 F
0.43 (, which is the length of each sepa-) 400.89 543.35 P
0.66 (rate exposure that is read to the ground. The default) 189 531.35 P
8 F
1.58 (SAMPLE-TIME) 404.7 531.35 P
5 F
0.66 ( is also the mini-) 470.7 531.35 P
0.07 (mum, 0.05 seconds.) 189 519.35 P
8 F
0.16 (SAMPLE-TIME) 271.42 519.35 P
5 F
0.07 ( may be incremented in 0.05 second values up to a) 337.42 519.35 P
0.28 (maximum of 12.75 seconds. Use of a very short) 189 507.35 P
8 F
0.67 (SAMPLE-TIME) 385.67 507.35 P
5 F
0.28 ( and/or use of) 451.67 507.35 P
8 F
0.67 (RAPID) 510 507.35 P
5 F
-0.15 (mode for extended periods can cause scheduling problems because of the very high data) 189 495.35 P
2.38 (volumes that are generated. In particular) 189 483.35 P
2.38 (, a) 362.1 483.35 P
8 F
5.7 (SAMPLE-TIME) 378.8 483.35 P
5 F
2.38 ( of less than 0.33 sec) 444.8 483.35 P
1 (records data at the 1 Mb rate and so can proceed for no more than about 20 minutes) 189 471.35 P
-0.21 (before \336lling the onboard tape recorder) 189 459.35 P
-0.21 (. A) 344.3 459.35 P
8 F
-0.5 (SAMPLE-TIME) 358.61 459.35 P
5 F
-0.21 ( of 0.33 seconds or more, but) 424.61 459.35 P
0.49 (less than 2.57 seconds, results in a 32k data rate, while a) 189 447.35 P
8 F
1.16 (SAMPLE-TIME) 422.84 447.35 P
5 F
0.49 ( in excess of) 488.84 447.35 P
-0 (2.57 seconds results in a 4k data rate. This latter low rate can be sustained almost indef-) 189 435.35 P
(initely) 189 423.35 T
(.) 213.91 423.35 T
54 380.02 540 383.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 381.52 540 381.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 381.52 180 381.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(4.5) 163.32 387.02 T
(The Precision and Accuracy of Standard Calibrations) 189 387.02 T
5 10 Q
1.14 (Our job of calibrating the GHRS on a routine basis ensures that you can rely on the) 189 363.35 P
-0.02 (wavelength scale and \337ux calibration that you are provided. The quality of the \337ux cali-) 189 351.35 P
0.37 (bration is limited primarily by innate factors that are present in tying together dif) 189 339.35 P
0.37 (ferent) 516.68 339.35 P
0.02 (photometric systems. The GHRS has proved to be a reliable instrument whose response) 189 327.35 P
1.02 (has not been seen to vary with time. Routine calibrations will deliver absolute \337uxes) 189 315.35 P
0.37 (accurate to 10% and photometrically precise to better than 1% with the LSA) 189 303.35 P
5 8 Q
0.29 (1) 498.89 307.35 P
5 10 Q
0.37 (. In other) 502.89 303.35 P
0.12 (words, we monitor the sensitivity of the GHRS on a regular basis \050approximately every) 189 291.35 P
1.05 (four months\051 and have not seen changes in the count rates for the standard stars that) 189 279.35 P
0.64 (exceed 1%, once the ef) 189 267.35 P
0.64 (fects of telescope focus are taken into account. However) 283.86 267.35 P
0.64 (, there) 514.37 267.35 P
-0.12 (are undoubtedly systematic ef) 189 255.35 P
-0.12 (fects present that preclude knowing absolute \337uxes to bet-) 308.18 255.35 P
0.81 (ter than 5 to 10%. The solid performance of the GHRS means that it is impossible to) 189 243.35 P
1.18 (improve substantially on the \337ux-calibration by obtaining observations on your own.) 189 231.35 P
0.18 (The GHRS dark count is so low for most objects as to be irrelevant \050but see the discus-) 189 219.35 P
0.33 (sion on) 189 207.35 P
8 F
0.78 (CENSOR) 221.32 207.35 P
5 F
0.33 ( in Section) 257.32 207.35 P
0.33 (8.6.2 on page) 303.26 207.35 P
0.33 (95\051 and high signal-to-noise can be obtained) 360.29 207.35 P
(without the need for \337at-\336eld exposures.) 189 195.35 T
0.21 (The one area in which you might wish to consider a special calibration is for the wave-) 189 175.35 P
0.22 (length scale. However) 189 163.35 P
0.22 (, even here the default wavelength scale provided by the pipeline) 278.17 163.35 P
54 120.98 540 150.98 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 128.98 333 128.98 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
0 0 612 792 C
5 9 Q
0 X
0 0 0 1 0 0 0 K
-0.02 (1. Starting in Cycle 4, the \337uxes from the data reduction pipeline in the ultraviolet can dif) 189 114.98 P
-0.02 (fer sys-) 513.28 114.98 P
(tematically from earlier values by up to 1% because of the use of models of the white dwarf) 189 104.98 T
(G191B2B as the fundamental standard.) 189 94.98 T
FMENDPAGE
%%EndPage: "46" 14
%%Page: "47" 15
612 792 0 FMBEGINPAGE
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
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0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (47) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
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72 726.98 558 726.98 2 L
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72 74.02 558 74.02 2 L
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72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
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0 9 Q
(Y) 207 736.18 T
(our Phase II Proposal) 212.34 736.18 T
5 10 Q
0.41 (data reduction system has been improved to take account of several systematic ef) 207 679.35 P
0.41 (fects.) 536.62 679.35 P
0.69 (As a result those wavelengths are good to better than 1 km s) 207 667.35 P
5 8 Q
0.55 (-1) 455.82 671.35 P
5 10 Q
0.69 ( for the \336rst-order grat-) 462.48 667.35 P
0.41 (ings, except at the shortest wavelengths \050L) 207 655.35 P
0.41 (y-) 379.14 655.35 P
12 F
0.41 (a) 387.47 655.35 P
5 F
0.41 (\051. For Echelle-B, the rms scatter in \336tted) 393.78 655.35 P
0.1 (wavelengths is about 0.6 km s) 207 643.35 P
5 8 Q
0.08 (-1) 328.07 647.35 P
5 10 Q
0.1 (. These values are uncertainties for the wavelength zero) 334.73 643.35 P
(point of a spectrum; the dispersion of spectra dif) 207 631.35 T
(fer negligibly from the routine values.) 400.68 631.35 T
1.48 (Our) 207 611.35 P
6 F
1.48 (speci\336cations) 226.53 611.35 P
5 F
1.48 ( for routine wavelength calibration are to have them good to only) 280.97 611.35 P
(about one diode rms, estimated as follows:) 207 599.35 T
7 11 Q
(\245) 207 581.35 T
5 10 Q
(First, errors in carrousel positioning can amount to 0.2 diode.) 221.4 581.35 T
7 11 Q
(\245) 207 566.35 T
5 10 Q
-0.12 (Second, if a wavelength calibration is not available for the precise carrousel position) 221.4 566.35 P
0.06 (you select then it is necessary to interpolate in the dispersion constants, and that can) 221.4 554.35 P
(lead to an error of 0.5 diode.) 221.4 542.35 T
7 11 Q
(\245) 207 527.35 T
5 10 Q
0.31 (Third, changing temperatures within the spectrograph can lead to wavelength shifts) 221.4 527.35 P
(of about 0.5 diode over the course of an orbit.) 221.4 515.35 T
7 11 Q
(\245) 207 500.35 T
5 10 Q
0.91 (Finally) 221.4 500.35 P
0.91 (, geomagnetically-induced image motion can lead to oscillations of up to 1) 249.09 500.35 P
(diode peak-to-peak amplitude over half an orbit.) 221.4 488.35 T
7 11 Q
(\245) 207 473.35 T
5 10 Q
(The net result is that about 1 1/4 diode accuracy is what is routinely expected.) 221.4 473.35 T
-0.01 (Precision of about 0.2 diode can be achieved by requesting that an) 207 453.35 P
8 F
-0.03 (ACCUM) 474.31 453.35 P
5 F
-0.01 ( with a) 504.31 453.35 P
8 F
-0.03 (TAR-) 534 453.35 P
-0.1 (GET) 207 441.35 P
5 F
-0.04 ( of) 225 441.35 P
8 F
-0.1 (WAVE) 238.24 441.35 P
5 F
-0.04 ( be made immediately) 262.24 441.35 P
6 F
-0.04 (befor) 353.18 441.35 P
-0.04 (e) 373.92 441.35 P
5 F
-0.04 ( your science exposure. Nearly the same pre-) 378.36 441.35 P
3.34 (cision can be realized by using information in the) 207 429.35 P
8 F
8.01 (SPYBAL) 437.29 429.35 P
5 F
3.34 ( exposures that are) 473.29 429.35 P
0.27 (automatically taken at the start of a sequence of observations with a new grating. Also,) 207 417.35 P
1.4 (you should specify) 207 405.35 P
8 F
3.35 (NO) 289.24 405.35 P
3.35 (GAP) 305.13 405.35 P
5 F
1.4 ( for the exposure lines to which the) 323.13 405.35 P
8 F
3.35 (WAVE) 477.61 405.35 P
5 F
1.4 ( pertains. See) 501.61 405.35 P
-0.04 (Chapter 5 for an example. Bear in mind that the several separate exposures you list may) 207 393.35 P
0.22 (not necessarily be obtained one right after the other \050unless you so specify in Phase II\051,) 207 381.35 P
(so that separate) 207 369.35 T
8 F
(WAVE) 271.15 369.35 T
5 F
( calibrations may be needed.) 295.15 369.35 T
0.2 (W) 207 349.35 P
0.2 (e also recommend breaking long exposures into subexposures that are no longer than) 215.64 349.35 P
2.32 (about 5 minutes each. This is done to ensure that geomagnetically-induced image) 207 337.35 P
0.64 (motion will not degrade the quality of your data. Any shifts in the dif) 207 325.35 P
0.64 (ferent spectra of) 491.76 325.35 P
-0 (the same object can generally be determined by cross-correlating them during your data) 207 313.35 P
(analysis.) 207 301.35 T
72 258.02 558 261.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 259.52 558 259.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 259.52 198 259.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(4.6) 181.32 265.02 T
(Other Considerations) 207 265.02 T
5 10 Q
0.59 (There are many factors that may in\337uence how you specify the manner in which your) 207 241.35 P
1.22 (observations should be obtained. Here we mention two that have arisen in particular) 207 229.35 P
0.99 (instances. The \336rst has to do with T) 207 217.35 P
0.99 (ar) 355.97 217.35 P
0.99 (gets of Opportunity \050T) 363.56 217.35 P
0.99 (OOs\051 and/or coordinated) 456.61 217.35 P
-0.03 (observations. The) 207 205.35 P
6 F
-0.03 (Call for Pr) 280.55 205.35 P
-0.03 (oposals) 324.03 205.35 P
5 F
-0.03 (should be consulted for information about propos-) 357.06 205.35 P
1.54 (ing to observe T) 207 193.35 P
1.54 (ar) 276.19 193.35 P
1.54 (gets of Opportunity with) 283.78 193.35 P
6 F
1.54 (HST) 391.05 193.35 P
5 F
1.54 ( and GHRS. Observations of T) 408.83 193.35 P
1.54 (OOs) 539.67 193.35 P
1.11 (often need to be coordinated with other satellites or ground-based observatories. The) 207 181.35 P
0.8 (long lead times for planning) 207 169.35 P
6 F
0.8 (HST) 326.27 169.35 P
5 F
0.8 ( observations, even for T) 344.05 169.35 P
0.8 (OOs, are an impediment to) 446.76 169.35 P
2.06 (that coordination. W) 207 157.35 P
2.06 (e encourage you to explain in detail exactly what is or is not) 292.8 157.35 P
(required for the successful completion of your program.) 207 145.35 T
-0.01 (Another problem that can occur arises when a science program speci\336es a lar) 207 125.35 P
-0.01 (ge number) 515.52 125.35 P
0.42 (of separate GHRS exposures. The problem is caused by the relatively small amount of) 207 113.35 P
0.33 (memory available on) 207 101.35 P
6 F
0.33 (HST) 294.92 101.35 P
5 F
0.33 ( in which to store GHRS commands. It is usually possible to) 312.7 101.35 P
FMENDPAGE
%%EndPage: "47" 15
%%Page: "48" 16
612 792 0 FMBEGINPAGE
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54 750.02 540 750.02 2 L
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(Y) 189 736.18 T
(our Phase II Proposal) 194.34 736.18 T
54 726.98 540 726.98 2 L
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54 74.02 540 74.02 2 L
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0 10 Q
(48) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
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54 726.98 540 726.98 2 L
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0.77 (break up such a program so that the separate exposures are not all together) 189 679.35 P
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0.41 (Roughly speaking, about 40 total spectra can be scheduled in a single block \050a) 189 655.35 P
8 F
0.99 (WSCAN) 510 655.35 P
5 F
0.21 (with) 189 643.35 P
6 F
0.21 (n) 209.49 643.35 P
5 F
0.21 ( set-points counts as) 214.49 643.35 P
6 F
0.21 (n) 298.65 643.35 P
5 F
0.21 ( exposures and an) 303.65 643.35 P
8 F
0.5 (FP-SPLIT) 378.35 643.35 P
5 F
0.21 ( counts as 2 or 4\051. Once that) 426.35 643.35 P
0.96 (number is exceeded the remaining observations must be scheduled in a new block of) 189 631.35 P
-0.23 (time, and that means a new tar) 189 619.35 P
-0.23 (get acquisition will be needed, with the concomitant over-) 309.36 619.35 P
(head time.) 189 607.35 T
FMENDPAGE
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<03060c183060c081> { 1 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<8040201008040201> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
end def
/patDict 15 dict dup begin
/PatternType 1 def
/PaintType 2 def
/TilingType 3 def
/BBox [ 0 0 8 8 ] def
/XStep 8 def
/YStep 8 def
/PaintProc {
begin
patProcDict bstring known {
patProcDict bstring get exec
} {
8 8 true [1 0 0 -1 0 8] bstring imagemask
} ifelse
end
} bind def
end def
} if
/combineColor {
FrameSepIs FMnone eq
{
graymode FMLevel1 or not {

[/Pattern [/DeviceCMYK]] setcolorspace
FrameCurColors 0 4 getinterval aload pop FrameCurPat setcolor
} {
FrameCurColors 3 get 1.0 ge {
FrameCurGray RealSetgray
} {
FMPColor graymode and {
0 1 3 {
FrameCurColors exch get
1 FrameCurGray sub mul
} for
RealSetcmykcolor
} {
4 1 6 {
FrameCurColors exch get
graymode {
1 exch sub 1 FrameCurGray sub mul 1 exch sub
} {
1.0 lt {FrameCurGray} {1} ifelse
} ifelse
} for
RealSetrgbcolor
} ifelse
} ifelse
} ifelse
} {
FrameCurColors 0 4 getinterval aload
FrameColorInSepListCMYK {
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
FrameSepIs FMcustom eq and
{ FrameCurGray } { 1 } ifelse
} {
FrameSepIs FMblack eq
{FrameCurGray 1.0 exch sub mul 1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop FrameCurGray 1.0 exch sub mul 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
graymode FMLevel1 or not {

[/Pattern [/DeviceGray]] setcolorspace
FrameCurPat setcolor
} {
graymode not FMLevel1 and {

dup 1 lt {pop FrameCurGray} if
} if
RealSetgray
} ifelse
} ifelse
} bind def
/savematrix {
orgmatrix currentmatrix pop
} bind def
/restorematrix {
orgmatrix setmatrix
} bind def
/dmatrix matrix def
/dpi 72 0 dmatrix defaultmatrix dtransform
dup mul exch dup mul add sqrt def

/freq dpi dup 72 div round dup 0 eq {pop 1} if 8 mul div def
/sangle 1 0 dmatrix defaultmatrix dtransform exch atan def
/dpiranges [ 2540 2400 1693 1270 1200 635 600 0 ] def
/CMLowFreqs [ 100.402 94.8683 89.2289 100.402 94.8683 66.9349 63.2456 47.4342 ] def
/YLowFreqs [ 95.25 90.0 84.65 95.25 90.0 70.5556 66.6667 50.0 ] def
/KLowFreqs [ 89.8026 84.8528 79.8088 89.8026 84.8528 74.8355 70.7107 53.033 ] def
/CLowAngles [ 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 ] def
/MLowAngles [ 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 ] def
/YLowTDot [ true true false true true false false false ] def
/CMHighFreqs [ 133.87 126.491 133.843 108.503 102.523 100.402 94.8683 63.2456 ] def
/YHighFreqs [ 127.0 120.0 126.975 115.455 109.091 95.25 90.0 60.0 ] def
/KHighFreqs [ 119.737 113.137 119.713 128.289 121.218 89.8026 84.8528 63.6395 ] def
/CHighAngles [ 71.5651 71.5651 71.5651 70.0169 70.0169 71.5651 71.5651 71.5651 ] def
/MHighAngles [ 18.4349 18.4349 18.4349 19.9831 19.9831 18.4349 18.4349 18.4349 ] def
/YHighTDot [ false false true false false true true false ] def
/PatFreq [ 10.5833 10.0 9.4055 10.5833 10.0 10.5833 10.0 9.375 ] def
/screenIndex {
0 1 dpiranges length 1 sub { dup dpiranges exch get 1 sub dpi le {exit} {pop} ifelse } for
} bind def
/getCyanScreen {
FMUseHighFrequencyScreens { CHighAngles CMHighFreqs} {CLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getMagentaScreen {
FMUseHighFrequencyScreens { MHighAngles CMHighFreqs } {MLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getYellowScreen {
FMUseHighFrequencyScreens { YHighTDot YHighFreqs} { YLowTDot YLowFreqs } ifelse
screenIndex dup 3 1 roll get 3 1 roll get { 3 div
{2 { 1 add 2 div 3 mul dup floor sub 2 mul 1 sub exch} repeat
FMSpotFunction } } {/FMSpotFunction load } ifelse
0.0 exch
} bind def
/getBlackScreen {
FMUseHighFrequencyScreens { KHighFreqs } { KLowFreqs } ifelse
screenIndex get 45.0 /FMSpotFunction load
} bind def
/getSpotScreen {
getBlackScreen
} bind def
/getCompositeScreen {
getBlackScreen
} bind def
/FMSetScreen
FMLevel1 { /setscreen load
}{ {
8 dict begin
/HalftoneType 1 def
/SpotFunction exch def
/Angle exch def
/Frequency exch def
/AccurateScreens FMUseAcccurateScreens def
currentdict end sethalftone
} bind } ifelse
def
/setDefaultScreen {
FMPColor {
orgrxfer cvx orggxfer cvx orgbxfer cvx orgxfer cvx setcolortransfer
}
{
orgxfer cvx settransfer
} ifelse
orgfreq organgle orgproc cvx setscreen
} bind def
/setCurrentScreen {
FrameSepIs FMnone eq {
FMUseDefaultNoSeparationScreen {
setDefaultScreen
} {
getCompositeScreen FMSetScreen
} ifelse
} {
FrameSepIs FMcustom eq {
FMUseDefaultSpotSeparationScreen {
setDefaultScreen
} {
getSpotScreen FMSetScreen
} ifelse
} {
FMUseDefaultProcessSeparationScreen {
setDefaultScreen
} {
FrameSepIs FMcyan eq {
getCyanScreen FMSetScreen
} {
FrameSepIs FMmagenta eq {
getMagentaScreen FMSetScreen
} {
FrameSepIs FMyellow eq {
getYellowScreen FMSetScreen
} {
getBlackScreen FMSetScreen
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} bind def
end
/gstring FMLOCAL
/gfile FMLOCAL
/gindex FMLOCAL
/orgrxfer FMLOCAL
/orggxfer FMLOCAL
/orgbxfer FMLOCAL
/orgxfer FMLOCAL
/orgproc FMLOCAL
/orgrproc FMLOCAL
/orggproc FMLOCAL
/orgbproc FMLOCAL
/organgle FMLOCAL
/orgrangle FMLOCAL
/orggangle FMLOCAL
/orgbangle FMLOCAL
/orgfreq FMLOCAL
/orgrfreq FMLOCAL
/orggfreq FMLOCAL
/orgbfreq FMLOCAL
/yscale FMLOCAL
/xscale FMLOCAL
/edown FMLOCAL
/manualfeed FMLOCAL
/paperheight FMLOCAL
/paperwidth FMLOCAL
/FMDOCUMENT {
array /FMfonts exch def
/#copies exch def
FrameDict begin
0 ne /manualfeed exch def
/paperheight exch def
/paperwidth exch def
0 ne /FrameNegative exch def
0 ne /edown exch def
/yscale exch def
/xscale exch def
FMLevel1 {
manualfeed {setmanualfeed} if
/FMdicttop countdictstack 1 add def
/FMoptop count def
% setpapername
% manualfeed {true} {papersize} ifelse
% {manualpapersize} {false} ifelse
% {desperatepapersize} {false} ifelse
% { (Can't select requested paper size for Frame print job!) FMFAILURE } if
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
}
{{1 dict dup /PageSize [paperwidth paperheight]put setpagedevice}stopped
{ (Can't select requested paper size for Frame print job!) FMFAILURE } if
{1 dict dup /ManualFeed manualfeed put setpagedevice } stopped pop }
ifelse

FMPColor {
currentcolorscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def
cvlit /orgbproc exch def
/orgbangle exch def
/orgbfreq exch def
cvlit /orggproc exch def
/orggangle exch def
/orggfreq exch def
cvlit /orgrproc exch def
/orgrangle exch def
/orgrfreq exch def
currentcolortransfer
FrameNegative {
1 1 4 {
pop { 1 exch sub } concatprocs 4 1 roll
} for
4 copy
setcolortransfer
} if
cvlit /orgxfer exch def
cvlit /orgbxfer exch def
cvlit /orggxfer exch def
cvlit /orgrxfer exch def
} {
currentscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def

currenttransfer
FrameNegative {
{ 1 exch sub } concatprocs
dup settransfer
} if
cvlit /orgxfer exch def
} ifelse
end
} def
/pagesave FMLOCAL
/orgmatrix FMLOCAL
/landscape FMLOCAL
/pwid FMLOCAL
/FMBEGINPAGE {
FrameDict begin
/pagesave save def
3.86 setmiterlimit
/landscape exch 0 ne def
landscape {
90 rotate 0 exch dup /pwid exch def neg translate pop
}{
pop /pwid exch def
} ifelse
edown { [-1 0 0 1 pwid 0] concat } if
0 0 moveto paperwidth 0 lineto paperwidth paperheight lineto
0 paperheight lineto 0 0 lineto 1 setgray fill
xscale yscale scale
/orgmatrix matrix def
gsave
} def
/FMENDPAGE {
grestore
pagesave restore
end
showpage
} def
/FMFONTDEFINE {
FrameDict begin
findfont
ReEncode
1 index exch
definefont
FMfonts 3 1 roll
put
end
} def
/FMFILLS {
FrameDict begin dup
array /fillvals exch def
dict /patCache exch def
end
} def
/FMFILL {
FrameDict begin
fillvals 3 1 roll put
end
} def
/FMNORMALIZEGRAPHICS {
newpath
0.0 0.0 moveto
1 setlinewidth
0 setlinecap
0 0 0 sethsbcolor
0 setgray
} bind def
/fx FMLOCAL
/fy FMLOCAL
/fh FMLOCAL
/fw FMLOCAL
/llx FMLOCAL
/lly FMLOCAL
/urx FMLOCAL
/ury FMLOCAL
/FMBEGINEPSF {
end
/FMEPSF save def
/showpage {} def
% See Adobe's "PostScript Language Reference Manual, 2nd Edition", page 714.
% "...the following operators MUST NOT be used in an EPS file:" (emphasis ours)
/banddevice {(banddevice) FMBADEPSF} def
/clear {(clear) FMBADEPSF} def
/cleardictstack {(cleardictstack) FMBADEPSF} def
/copypage {(copypage) FMBADEPSF} def
/erasepage {(erasepage) FMBADEPSF} def
/exitserver {(exitserver) FMBADEPSF} def
/framedevice {(framedevice) FMBADEPSF} def
/grestoreall {(grestoreall) FMBADEPSF} def
/initclip {(initclip) FMBADEPSF} def
/initgraphics {(initgraphics) FMBADEPSF} def
/initmatrix {(initmatrix) FMBADEPSF} def
/quit {(quit) FMBADEPSF} def
/renderbands {(renderbands) FMBADEPSF} def
/setglobal {(setglobal) FMBADEPSF} def
/setpagedevice {(setpagedevice) FMBADEPSF} def
/setshared {(setshared) FMBADEPSF} def
/startjob {(startjob) FMBADEPSF} def
/lettertray {(lettertray) FMBADEPSF} def
/letter {(letter) FMBADEPSF} def
/lettersmall {(lettersmall) FMBADEPSF} def
/11x17tray {(11x17tray) FMBADEPSF} def
/11x17 {(11x17) FMBADEPSF} def
/ledgertray {(ledgertray) FMBADEPSF} def
/ledger {(ledger) FMBADEPSF} def
/legaltray {(legaltray) FMBADEPSF} def
/legal {(legal) FMBADEPSF} def
/statementtray {(statementtray) FMBADEPSF} def
/statement {(statement) FMBADEPSF} def
/executivetray {(executivetray) FMBADEPSF} def
/executive {(executive) FMBADEPSF} def
/a3tray {(a3tray) FMBADEPSF} def
/a3 {(a3) FMBADEPSF} def
/a4tray {(a4tray) FMBADEPSF} def
/a4 {(a4) FMBADEPSF} def
/a4small {(a4small) FMBADEPSF} def
/b4tray {(b4tray) FMBADEPSF} def
/b4 {(b4) FMBADEPSF} def
/b5tray {(b5tray) FMBADEPSF} def
/b5 {(b5) FMBADEPSF} def
FMNORMALIZEGRAPHICS
[/fy /fx /fh /fw /ury /urx /lly /llx] {exch def} forall
fx fw 2 div add fy fh 2 div add translate
rotate
fw 2 div neg fh 2 div neg translate
fw urx llx sub div fh ury lly sub div scale
llx neg lly neg translate
/FMdicttop countdictstack 1 add def
/FMoptop count def
} bind def
/FMENDEPSF {
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
FMEPSF restore
FrameDict begin
} bind def
FrameDict begin
/setmanualfeed {
%%BeginFeature *ManualFeed True
statusdict /manualfeed true put
%%EndFeature
} bind def
/max {2 copy lt {exch} if pop} bind def
/min {2 copy gt {exch} if pop} bind def
/inch {72 mul} def
/pagedimen {
paperheight sub abs 16 lt exch
paperwidth sub abs 16 lt and
{/papername exch def} {pop} ifelse
} bind def
/papersizedict FMLOCAL
/setpapername {
/papersizedict 14 dict def
papersizedict begin
/papername /unknown def
/Letter 8.5 inch 11.0 inch pagedimen
/LetterSmall 7.68 inch 10.16 inch pagedimen
/Tabloid 11.0 inch 17.0 inch pagedimen
/Ledger 17.0 inch 11.0 inch pagedimen
/Legal 8.5 inch 14.0 inch pagedimen
/Statement 5.5 inch 8.5 inch pagedimen
/Executive 7.5 inch 10.0 inch pagedimen
/A3 11.69 inch 16.5 inch pagedimen
/A4 8.26 inch 11.69 inch pagedimen
/A4Small 7.47 inch 10.85 inch pagedimen
/B4 10.125 inch 14.33 inch pagedimen
/B5 7.16 inch 10.125 inch pagedimen
end
} bind def
/papersize {
papersizedict begin
/Letter {lettertray letter} def
/LetterSmall {lettertray lettersmall} def
/Tabloid {11x17tray 11x17} def
/Ledger {ledgertray ledger} def
/Legal {legaltray legal} def
/Statement {statementtray statement} def
/Executive {executivetray executive} def
/A3 {a3tray a3} def
/A4 {a4tray a4} def
/A4Small {a4tray a4small} def
/B4 {b4tray b4} def
/B5 {b5tray b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
statusdict begin stopped end
} bind def
/manualpapersize {
papersizedict begin
/Letter {letter} def
/LetterSmall {lettersmall} def
/Tabloid {11x17} def
/Ledger {ledger} def
/Legal {legal} def
/Statement {statement} def
/Executive {executive} def
/A3 {a3} def
/A4 {a4} def
/A4Small {a4small} def
/B4 {b4} def
/B5 {b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
stopped
} bind def
/desperatepapersize {
statusdict /setpageparams known
{
paperwidth paperheight 0 1
statusdict begin
{setpageparams} stopped
end
} {true} ifelse
} bind def
/DiacriticEncoding [
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /space /exclam /quotedbl
/numbersign /dollar /percent /ampersand /quotesingle /parenleft
/parenright /asterisk /plus /comma /hyphen /period /slash /zero /one
/two /three /four /five /six /seven /eight /nine /colon /semicolon
/less /equal /greater /question /at /A /B /C /D /E /F /G /H /I /J /K
/L /M /N /O /P /Q /R /S /T /U /V /W /X /Y /Z /bracketleft /backslash
/bracketright /asciicircum /underscore /grave /a /b /c /d /e /f /g /h
/i /j /k /l /m /n /o /p /q /r /s /t /u /v /w /x /y /z /braceleft /bar
/braceright /asciitilde /.notdef /Adieresis /Aring /Ccedilla /Eacute
/Ntilde /Odieresis /Udieresis /aacute /agrave /acircumflex /adieresis
/atilde /aring /ccedilla /eacute /egrave /ecircumflex /edieresis
/iacute /igrave /icircumflex /idieresis /ntilde /oacute /ograve
/ocircumflex /odieresis /otilde /uacute /ugrave /ucircumflex
/udieresis /dagger /.notdef /cent /sterling /section /bullet
/paragraph /germandbls /registered /copyright /trademark /acute
/dieresis /.notdef /AE /Oslash /.notdef /.notdef /.notdef /.notdef
/yen /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/ordfeminine /ordmasculine /.notdef /ae /oslash /questiondown
/exclamdown /logicalnot /.notdef /florin /.notdef /.notdef
/guillemotleft /guillemotright /ellipsis /.notdef /Agrave /Atilde
/Otilde /OE /oe /endash /emdash /quotedblleft /quotedblright
/quoteleft /quoteright /.notdef /.notdef /ydieresis /Ydieresis
/fraction /currency /guilsinglleft /guilsinglright /fi /fl /daggerdbl
/periodcentered /quotesinglbase /quotedblbase /perthousand
/Acircumflex /Ecircumflex /Aacute /Edieresis /Egrave /Iacute
/Icircumflex /Idieresis /Igrave /Oacute /Ocircumflex /.notdef /Ograve
/Uacute /Ucircumflex /Ugrave /dotlessi /circumflex /tilde /macron
/breve /dotaccent /ring /cedilla /hungarumlaut /ogonek /caron
] def
/ReEncode {
dup
length
dict begin
{
1 index /FID ne
{def}
{pop pop} ifelse
} forall
0 eq {/Encoding DiacriticEncoding def} if
currentdict
end
} bind def
FMPColor

{
/BEGINBITMAPCOLOR {
BITMAPCOLOR} def
/BEGINBITMAPCOLORc {
BITMAPCOLORc} def
/BEGINBITMAPTRUECOLOR {
BITMAPTRUECOLOR } def
/BEGINBITMAPTRUECOLORc {
BITMAPTRUECOLORc } def
}

{
/BEGINBITMAPCOLOR {
BITMAPGRAY} def
/BEGINBITMAPCOLORc {
BITMAPGRAYc} def
/BEGINBITMAPTRUECOLOR {
BITMAPTRUEGRAY } def
/BEGINBITMAPTRUECOLORc {
BITMAPTRUEGRAYc } def
}
ifelse
/K {
FMPrintAllColorsAsBlack {
dup 1 eq 2 index 1 eq and 3 index 1 eq and not
{7 {pop} repeat 0 0 0 1 0 0 0} if
} if
FrameCurColors astore
pop combineColor
} bind def
/graymode true def
/bwidth FMLOCAL
/bpside FMLOCAL
/bstring FMLOCAL
/onbits FMLOCAL
/offbits FMLOCAL
/xindex FMLOCAL
/yindex FMLOCAL
/x FMLOCAL
/y FMLOCAL
/setPatternMode {
FMLevel1 {
/bwidth exch def
/bpside exch def
/bstring exch def
/onbits 0 def /offbits 0 def
freq sangle landscape {90 add} if
{/y exch def
/x exch def
/xindex x 1 add 2 div bpside mul cvi def
/yindex y 1 add 2 div bpside mul cvi def
bstring yindex bwidth mul xindex 8 idiv add get
1 7 xindex 8 mod sub bitshift and 0 ne FrameNegative {not} if
{/onbits onbits 1 add def 1}
{/offbits offbits 1 add def 0}
ifelse
}
setscreen
offbits offbits onbits add div FrameNegative {1.0 exch sub} if
/FrameCurGray exch def
} {
pop pop
dup patCache exch known {
patCache exch get
} {
dup
patDict /bstring 3 -1 roll put
patDict
9 PatFreq screenIndex get div dup matrix scale
makepattern
dup
patCache 4 -1 roll 3 -1 roll put
} ifelse
/FrameCurGray 0 def
/FrameCurPat exch def
} ifelse
/graymode false def
combineColor
} bind def
/setGrayScaleMode {
graymode not {
/graymode true def
FMLevel1 {
setCurrentScreen
} if
} if
/FrameCurGray exch def
combineColor
} bind def
/normalize {
transform round exch round exch itransform
} bind def
/dnormalize {
dtransform round exch round exch idtransform
} bind def
/lnormalize {
0 dtransform exch cvi 2 idiv 2 mul 1 add exch idtransform pop
} bind def
/H {
lnormalize setlinewidth
} bind def
/Z {
setlinecap
} bind def

/PFill {
graymode FMLevel1 or not {
gsave 1 setgray eofill grestore
} if
} bind def
/PStroke {
graymode FMLevel1 or not {
gsave 1 setgray stroke grestore
} if
stroke
} bind def
/fillvals FMLOCAL
/X {
fillvals exch get
dup type /stringtype eq
{8 1 setPatternMode}
{setGrayScaleMode}
ifelse
} bind def
/V {
PFill gsave eofill grestore
} bind def
/Vclip {
clip
} bind def
/Vstrk {
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/N {
PStroke
} bind def
/Nclip {
strokepath clip newpath
} bind def
/Nstrk {
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/M {newpath moveto} bind def
/E {lineto} bind def
/D {curveto} bind def
/O {closepath} bind def
/n FMLOCAL
/L {
/n exch def
newpath
normalize
moveto
2 1 n {pop normalize lineto} for
} bind def
/Y {
L
closepath
} bind def
/x1 FMLOCAL
/x2 FMLOCAL
/y1 FMLOCAL
/y2 FMLOCAL
/R {
/y2 exch def
/x2 exch def
/y1 exch def
/x1 exch def
x1 y1
x2 y1
x2 y2
x1 y2
4 Y
} bind def
/rad FMLOCAL
/rarc
{rad
arcto
} bind def
/RR {
/rad exch def
normalize
/y2 exch def
/x2 exch def
normalize
/y1 exch def
/x1 exch def
mark
newpath
{
x1 y1 rad add moveto
x1 y2 x2 y2 rarc
x2 y2 x2 y1 rarc
x2 y1 x1 y1 rarc
x1 y1 x1 y2 rarc
closepath
} stopped {x1 y1 x2 y2 R} if
cleartomark
} bind def
/RRR {
/rad exch def
normalize /y4 exch def /x4 exch def
normalize /y3 exch def /x3 exch def
normalize /y2 exch def /x2 exch def
normalize /y1 exch def /x1 exch def
newpath
normalize moveto
mark
{
x2 y2 x3 y3 rarc
x3 y3 x4 y4 rarc
x4 y4 x1 y1 rarc
x1 y1 x2 y2 rarc
closepath
} stopped
{x1 y1 x2 y2 x3 y3 x4 y4 newpath moveto lineto lineto lineto closepath} if
cleartomark
} bind def
/C {
grestore
gsave
R
clip
setCurrentScreen
} bind def
/CP {
grestore
gsave
Y
clip
setCurrentScreen
} bind def
/FMpointsize FMLOCAL
/F {
FMfonts exch get
FMpointsize scalefont
setfont
} bind def
/Q {
/FMpointsize exch def
F
} bind def
/T {
moveto show
} bind def
/RF {
rotate
0 ne {-1 1 scale} if
} bind def
/TF {
gsave
moveto
RF
show
grestore
} bind def
/P {
moveto
0 32 3 2 roll widthshow
} bind def
/PF {
gsave
moveto
RF
0 32 3 2 roll widthshow
grestore
} bind def
/S {
moveto
0 exch ashow
} bind def
/SF {
gsave
moveto
RF
0 exch ashow
grestore
} bind def
/B {
moveto
0 32 4 2 roll 0 exch awidthshow
} bind def
/BF {
gsave
moveto
RF
0 32 4 2 roll 0 exch awidthshow
grestore
} bind def
/G {
gsave
newpath
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(GHRS Instrument Handbook 5.0) 207 60.29 T
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1.2 (Chapter 5) 72 677 S
2 24 Q
-0.48 (Phase II Pr) 207 677 S
-0.48 (oposal) 309.27 677 S
-0.48 (Examples) 207 647 S
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(Phase II Proposal Examples) 189 736.18 T
54 726.98 540 726.98 2 L
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(50) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
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1.32 (W) 189 679.35 P
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0.24 (, partly for formatting reasons, since they require a side-) 313.19 655.35 P
0.7 (ways orientation of the page, and partly to assemble them in one place for easy refer-) 189 643.35 P
(ence.) 189 631.35 T
0.01 (W) 189 607.35 P
0.01 (e begin by showing how the \336rst entry on the next page would look as input to RPSS.) 197.64 607.35 P
-0.09 (The remainder of this chapter shows how Phase II proposals look to us. In most of these) 189 595.35 P
1.34 (examples, the various parameters have been explicitly listed for clarity) 189 583.35 P
1.34 (, even though) 483.15 583.35 P
(they often correspond to the defaults that would apply anyway) 189 571.35 T
(.) 438.03 571.35 T
-0.21 (W) 189 547.35 P
-0.21 (e remind you that any if dif) 197.64 547.35 P
-0.21 (ferences exist between this document and, say) 305.64 547.35 P
-0.21 (, the Phase II) 488.42 547.35 P
0.41 (Proposal Instructions, the one with the most recent date of issue should be followed or) 189 535.35 P
(you should consult us to resolve the discrepancy) 189 523.35 T
(.) 381.94 523.35 T
4 8 Q
(exposure_logsheet:) 203.42 482.68 T
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(1.0) 294.02 459.68 T
(targname:) 203.42 448.68 T
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(conf) 203.42 437.68 T
(ig:) 222.62 437.68 T
(HRS) 294.02 437.68 T
(opmode:) 203.42 426.68 T
(ACQ) 294.02 426.68 T
(aperture) 203.42 415.68 T
(2.0) 294.02 415.68 T
(sp_element:) 203.42 404.68 T
(MIRROR-A2) 294.02 404.68 T
(num_exp:) 203.42 393.68 T
(1) 294.02 393.68 T
(time_per_exp:) 203.42 382.68 T
(10.75M) 294.02 382.68 T
(f) 203.42 371.68 T
(luxnum_1:) 208.22 371.68 T
(1) 294.02 371.68 T
(priority:) 203.42 360.68 T
(1) 294.02 360.68 T
(param_1:) 203.42 349.68 T
(SEARCH-SIZE=5,) 294.02 349.68 T
(param_2:) 203.42 338.68 T
(MAP=ALL-POINTS) 294.02 338.68 T
(req_1:) 203.42 327.68 T
(CYCLE 5/ 1-2;) 294.02 327.68 T
(req_2:) 203.42 316.68 T
(EARLY ACQ FOR 2.0) 294.02 316.68 T
(comment_1:) 203.42 305.68 T
(STEP-TIME=0.2S;) 294.02 305.68 T
(comment_2:) 203.42 294.68 T
(EXPECT 21000 COUNTS IN STEP-TIME) 294.02 294.68 T
(!) 203.42 283.68 T
(linenum:) 203.42 272.68 T
(2.0) 294.02 272.68 T
(targname:) 203.42 261.68 T
(MU-COL) 294.02 261.68 T
(conf) 203.42 250.68 T
(ig:) 222.62 250.68 T
(HRS) 294.02 250.68 T
(opmode:) 203.42 239.68 T
(ACCUM) 294.02 239.68 T
(aperture:) 203.42 228.68 T
(2.0) 294.02 228.68 T
(sp_element:) 203.42 217.68 T
(ECH-B) 294.02 217.68 T
(num_exp:) 203.42 206.68 T
(1) 294.02 206.68 T
(time_per_exp:) 203.42 195.68 T
(4.8S) 294.02 195.68 T
(f) 203.42 184.68 T
(luxnum_1:) 208.22 184.68 T
(1) 294.02 184.68 T
(priority:) 203.42 173.68 T
(1) 294.02 173.68 T
(param_1:) 203.42 162.68 T
(STEP-PATT=13) 294.02 162.68 T
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(GHRS Instrument Handbook 5.0) 207 60.29 T
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0 X
-0.13 (1. Example of an observation that speci\336es an early acquisition. Note that the TIME in column \0501) 0 -270 102.67 90 PF
-0.13 (1\051 is 0.2 sec \050the STEP-TIME\051 times) 0 -270 102.67 546.19 PF
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(mentioned.) 0 -270 126.67 90 TF
4 8 Q
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 167.33 90 TF
-0.13 ( 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15) 0 -270 177.33 90 PF
-0.26 ( LN | SEQ | TARGET |INSTR | OPER. | APER |SPECTRAL|CENTRAL| OPTIONAL |NUM| TIME | S/N |FLX|PR| SPECIAL) 0 -270 187.33 90 PF
-0.24 ( NM | NAME | NAME |CONFIG| MODE |OR FOV |ELEMENT |WAVELN | PARAMETERS |EXP| | |REF| | REQUIREMENTS) 0 -270 197.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 207.33 90 TF
-0.17 (1.0 MU-COL HRS ACQ 2.0 MIRROR- SEARCH-SIZE=5, 1 10.75M 1 1 CYCLE 5/ 1-2;) 0 -270 217.33 90 PF
-0.12 ( A2 MAP=ALL-POINTS EARLY ACQ FOR 2.0) 0 -270 227.33 90 PF
-0.16 ( COMMENTS: STEP-TIME=0.2S; EXPECT 21000 COUNTS IN STEP-TIME) 0 -270 237.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 247.33 90 TF
-0.15 (2.0 MU-COL HRS ACCUM 2.0 ECH-B 1600 STEP-PATT=13 1 4.8S 1 1) 0 -270 257.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 287.33 90 TF
0 10 Q
(2. The same observation as above speci\336ed as an interactive acquisition.) 0 -270 322.67 90 TF
4 8 Q
(--------------------------------------------------------------------------------------------------------------------------------) 0 -270 349.33 90 TF
-0.13 ( 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15) 0 -270 359.33 90 PF
-0.26 ( LN | SEQ | TARGET |INSTR | OPER. | APER |SPECTRAL|CENTRAL| OPTIONAL |NUM| TIME | S/N |FLX|PR| SPECIAL) 0 -270 369.33 90 PF
-0.24 ( NM | NAME | NAME |CONFIG| MODE |OR FOV |ELEMENT |WAVELN | PARAMETERS |EXP| | |REF| | REQUIREMENTS) 0 -270 379.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 389.33 90 TF
(10.0 MU-COL HRS ACQ 2.0 MIRROR- SEARCH-SIZE=5, 1 10.75M 1 1 CYCLE 5/ 10-20;) 0 -270 399.33 90 TF
(00 A2 MAP=ALL-POINT INT ACQ FOR 20;) 0 -270 409.33 90 TF
( S) 0 -270 419.33 90 TF
( COMMENTS: STEP-TIME=0.2S; EXPECT 21000 COUNTS IN STEP-TIME) 0 -270 429.33 90 TF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 439.33 90 TF
-0.15 (20.0 MU-COL HRS ACCUM 2.0 ECH-B 1600 STEP-PATT=13 1 4.8S 1 1) 0 -270 449.33 90 PF
-0.1 (00) 0 -270 459.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 479.33 90 TF
72 90 558 711 R
FMENDPAGE
%%EndPage: "51" 3
%%Page: "52" 4
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
54 726.98 540 726.98 2 L
0.25 H
N
0 9 Q
(Phase II Proposal Examples) 189 736.18 T
0 10 Q
(52) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 74.02 540 74.02 2 L
2 Z
N
54 90 540 711 R
7 X
V
0 X
(3. A GHRS acquisition speci\336ed with explicit BRIGHT and F) 0 -270 60.67 90 TF
(AINT limits.) 0 -270 60.67 371.74 TF
4 8 Q
(--------------------------------------------------------------------------------------------------------------------------------) 0 -270 87.33 90 TF
-0.13 ( 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15) 0 -270 97.33 90 PF
-0.26 ( LN | SEQ | TARGET |INSTR | OPER. | APER |SPECTRAL|CENTRAL| OPTIONAL |NUM| TIME | S/N |FLX|PR| SPECIAL) 0 -270 107.33 90 PF
-0.24 ( NM | NAME | NAME |CONFIG| MODE |OR FOV |ELEMENT |WAVELN | PARAMETERS |EXP| | |REF| | REQUIREMENTS) 0 -270 117.33 90 PF
(--------------------------------------------------------------------------------------------------------------------------------) 0 -270 127.33 90 TF
-0.18 (100. BD28D4211 HRS ACQ 2.0 MIRROR- BRIGHT=65535, 1 9S 1 1 ONBOARD ACQ FOR 2) 0 -270 137.33 90 PF
-0.11 (000 A2 FAINT=700 00;) 0 -270 147.33 90 PF
-0.29 ( COMMENTS: STEP_TIME=1.0S; EXPECT 1800 COUNTS IN STEP-TIME; FAINT SET TO APPROX. 40% OF EXPECTED COUNTS.) 0 -270 167.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 177.33 90 TF
0 10 Q
(4. Example of an acquisition with an offset.) 0 -270 210.67 90 TF
4 8 Q
(--------------------------------------------------------------------------------------------------------------------------------) 0 -270 237.33 90 TF
-0.13 ( 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15) 0 -270 247.33 90 PF
-0.26 ( LN | SEQ | TARGET |INSTR | OPER. | APER |SPECTRAL|CENTRAL| OPTIONAL |NUM| TIME | S/N |FLX|PR| SPECIAL) 0 -270 257.33 90 PF
-0.24 ( NM | NAME | NAME |CONFIG| MODE |OR FOV |ELEMENT |WAVELN | PARAMETERS |EXP| | |REF| | REQUIREMENTS) 0 -270 267.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 277.33 90 TF
-0.18 (900. HII-POS1 HRS ACQ 2.0 MIRROR- BRIGHT=RETURN 1 1.8S 1 1 ONBOARD ACQ FOR 9) 0 -270 287.33 90 PF
-0.1 (000 N2 10) 0 -270 297.33 90 PF
-0.12 ( COMMENTS: STEP-TIME=0.2S) 0 -270 307.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 317.33 90 TF
-0.14 (910. HII-POS2 HRS ACCUM 2.0 G160M 1500 1 272S 50 1 1) 0 -270 327.33 90 PF
-0.1 (000) 0 -270 337.33 90 PF
-0.19 ( COMMENTS: RA-OFF = +0.227S +/- 0.001S, DEC-OFF = +6.0\323 +/- 0.01\323, FROM HII-POS1) 0 -270 347.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 357.33 90 TF
54 90 540 711 R
FMENDPAGE
%%EndPage: "52" 4
%%Page: "53" 5
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Phase II Proposal Examples) 207 736.18 T
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (53) 546.88 60.29 P
72 90 558 711 R
7 X
V
0 X
0 (5. A fairly typical GHRS observation, starting with an acquisition using BRIGHT=RETURN and proceeding to several spectroscopic) 0 -270 78.67 90 PF
0.25 (exposures that use alternative variants of ACCUM speci\336cations. Not all of these would be used in one program. Note the IMAGE) 0 -270 90.67 90 PF
(\050line 300\051 that is obtained to later con\336rm centering of the target in the LSA.) 0 -270 102.67 90 TF
4 8 Q
(--------------------------------------------------------------------------------------------------------------------------------) 0 -270 129.33 90 TF
-0.13 ( 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15) 0 -270 139.33 90 PF
-0.26 ( LN | SEQ | TARGET |INSTR | OPER. | APER |SPECTRAL|CENTRAL| OPTIONAL |NUM| TIME | S/N |FLX|PR| SPECIAL) 0 -270 149.33 90 PF
-0.24 ( NM | NAME | NAME |CONFIG| MODE |OR FOV |ELEMENT |WAVELN | PARAMETERS |EXP| | |REF| | REQUIREMENTS) 0 -270 159.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 169.33 90 TF
-0.18 (100. BD28D4211 HRS ACQ 2.0 MIRROR- BRIGHT=RETURN, 1 9S 1 1 ONBOARD ACQ FOR 2) 0 -270 179.33 90 PF
-0.1 (000 A2 00;) 0 -270 189.33 90 PF
-0.16 ( COMMENTS: STEP_TIME=1.0S; EXPECT 1800 COUNTS IN STEP-TIME.) 0 -270 199.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 209.33 90 TF
-0.16 (200. BD28D4211 HRS ACQ/PE 2.0 MIRROR- 1 102S 1 1 ONBOARD ACQ FOR 3) 0 -270 219.33 90 PF
-0.11 (000 AKUP A2 00-800;) 0 -270 229.33 90 PF
-0.12 ( COMMENTS: STEP_TIME=1.0S) 0 -270 239.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 249.33 90 TF
-0.16 (300. BD28D4211 HRS IMAGE 2.0 MIRROR- NX=16, NY=16 1 256.0S 1 1) 0 -270 259.33 90 PF
-0.1 (000 A2) 0 -270 269.33 90 PF
( COMMENTS: STEP-TIME=1.0S) 0 -270 279.33 90 TF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 289.33 90 TF
(400. BD28D4211 HRS ACCUM 2.0 G160M 1500 STEP-PATT=5, S 1 217.6S 50 1 1) 0 -270 299.33 90 TF
-0.11 (000 TEP-TIME=0.2,) 0 -270 309.33 90 PF
-0.11 ( FP-SPLIT=NO, C) 0 -270 319.33 90 PF
-0.18 ( OOMB=FOUR) 0 -270 329.33 90 PF
-0.45 ( COMMENTS: EXPOSURE TIME IS A INTEGRAL NUMBER OF MINIMUM EXPOSURE TIME \05027.2S IN THIS CASE\051; S/N IS PER DIODE; STEP-PATT WILL) 0 -270 339.33 90 PF
( RESULT IN 4 PIXELS/DIODE.) 0 -270 349.33 90 TF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 359.33 90 TF
-0.17 (450. BD28D4211 HRS ACCUM 2.0 G160M 1500 STEP-PATT=5, S 1 217.6S 50 1 1) 0 -270 369.33 90 PF
-0.11 (000 TEP-TIME=0.2,) 0 -270 379.33 90 PF
-0.11 ( FP-SPLIT=FOUR,) 0 -270 389.33 90 PF
-0.1 ( COMB=FOUR) 0 -270 399.33 90 PF
( COMMENTS: FP-SPLIT WILL PRODUCE 4 SPECTRA EACH WITH 54.4S EXPOSURE TIME.) 0 -270 409.33 90 TF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 419.33 90 TF
-0.14 (475. BD28D4211 HRS ACCUM 2.0 G160M 1500 10 217.6S 50 1 1) 0 -270 429.33 90 PF
-0.1 (000) 0 -270 439.33 90 PF
-0.28 ( COMMENTS: TOTAL EXPOSURE = 2176S--BREAK UP LONG EXPOSURE TO AVOID DRIFT DUE TO GIMP.) 0 -270 459.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 469.33 90 TF
72 90 558 711 R
FMENDPAGE
%%EndPage: "53" 5
%%Page: "54" 6
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
54 726.98 540 726.98 2 L
0.25 H
N
0 9 Q
(Phase II Proposal Examples) 189 736.18 T
0 10 Q
(54) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 74.02 540 74.02 2 L
2 Z
N
54 90 540 711 R
7 X
V
0 X
(6. A sequence of exposures that could be added to Example 5 if additional SSA observations were desired. The ACCUM, RAPID,) 0 -270 60.67 90 TF
(and WSCAN lines illustrate a range of options. Note the ACQ/PEAKUP with the SSA \050line 550\051 to move the star to that aperture.) 0 -270 72.67 90 TF
(If line 550 were absent the star would still be moved to the SSA, but it would not be as well centered.) 0 -270 84.67 90 TF
4 8 Q
(--------------------------------------------------------------------------------------------------------------------------------) 0 -270 111.33 90 TF
-0.13 ( 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |10 | 11 | 12 |13 |14| 15) 0 -270 121.33 90 PF
-0.26 ( LN | SEQ | TARGET |INSTR | OPER. | APER |SPECTRAL|CENTRAL| OPTIONAL |NUM| TIME | S/N |FLX|PR| SPECIAL) 0 -270 131.33 90 PF
-0.24 ( NM | NAME | NAME |CONFIG| MODE |OR FOV |ELEMENT |WAVELN | PARAMETERS |EXP| | |REF| | REQUIREMENTS) 0 -270 141.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 151.33 90 TF
(550. BD28D4211 HRS ACQ/PE 0.25 MIRROR- SEARCH-SIZE=5 1 25S 1 1 ONBOARD ACQ FOR) 0 -270 161.33 90 TF
( AKUP A2 600.00;) 0 -270 171.33 90 TF
-0.12 ( COMMENTS: STEP_TIME=1.0S) 0 -270 181.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 191.33 90 TF
-0.15 (575. WAVE HRS ACCUM SC2 G160M 1500 1 60S 1 1 CALIB FOR 525;) 0 -270 201.33 90 PF
-0.11 (000 SEQ 500-600 NO GAP) 0 -270 211.33 90 PF
-0.14 ( COMMENTS: STANDARD SPECTRAL CAL LAMP SPECTRUM.) 0 -270 221.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 231.33 90 TF
-0.17 (600. BD28D4211 HRS ACCUM 0.25 G160M 1500 STEP-PATT=5, S 1 326.4S 50 1 1) 0 -270 241.33 90 PF
-0.11 (000 TEP-TIME=0.2,) 0 -270 251.33 90 PF
-0.11 ( FP-SPLIT=NO, C) 0 -270 261.33 90 PF
-0.1 ( OMB=FOUR) 0 -270 271.33 90 PF
-0.15 ( COMMENTS: THROUGHPUT OF SSA APPROX. 0.67 OF LSA AT 1500A.) 0 -270 281.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 291.33 90 TF
-0.17 (700. BD28D4211 HRS RAPID 0.25 G160M 1500 SAMPLE-TIME=1. 1 20M 25 1 1) 0 -270 301.33 90 PF
-0.1 (000 0) 0 -270 311.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 321.33 90 TF
-0.18 (800. BD28D4211 HRS WSCAN 0.25 G160M 1400-1 WAVE-STEP=30.0 1 217.6S 50 1 1) 0 -270 331.33 90 PF
-0.1 (000 610) 0 -270 341.33 90 PF
-0.57 ( COMMENTS: WSCAN TO PRODUCE 7 SPECTRA W/ CENTRAL WAVELENGTHS: W1=1415.0,W2=1445,W3=1475,W4=1505, W5=1535,W6=1565,W7=1595.) 0 -270 351.33 90 PF
(---------------------------------------------------------------------------------------------------------------------------------) 0 -270 361.33 90 TF
54 90 540 711 R
FMENDPAGE
%%EndPage: "54" 6
%%Trailer
%%BoundingBox: 0 0 612 792
%%PageOrder: Ascend
%%Pages: 6
%%DocumentFonts: Helvetica-Bold
%%+ Palatino-BoldItalic
%%+ Palatino-Italic
%%+ Times-Roman
%%+ Courier
%%EOF
%!PS-Adobe-3.0
%%BoundingBox: (atend)
%%Pages: (atend)
%%PageOrder: (atend)
%%DocumentFonts: (atend)
%%Creator: Frame 4.0
%%DocumentData: Clean7Bit
%%EndComments
%%BeginProlog
%
% Frame ps_prolog 4.0, for use with Frame 4.0 products
% This ps_prolog file is Copyright (c) 1986-1993 Frame Technology
% Corporation. All rights reserved. This ps_prolog file may be
% freely copied and distributed in conjunction with documents created
% using FrameMaker, FrameBuilder and FrameViewer as long as this
% copyright notice is preserved.
%
% Frame products normally print colors as their true color on a color printer
% or as shades of gray, based on luminance, on a black-and white printer. The
% following flag, if set to True, forces all non-white colors to print as pure
% black. This has no effect on bitmap images.
/FMPrintAllColorsAsBlack false def
%
% Frame products can either set their own line screens or use a printer's
% default settings. Three flags below control this separately for no
% separations, spot separations and process separations. If a flag
% is true, then the default printer settings will not be changed. If it is
% false, Frame products will use their own settings from a table based on
% the printer's resolution.
/FMUseDefaultNoSeparationScreen true def
/FMUseDefaultSpotSeparationScreen true def
/FMUseDefaultProcessSeparationScreen false def
%
% For any given PostScript printer resolution, Frame products have two sets of
% screen angles and frequencies for printing process separations, which are
% recomended by Adobe. The following variable chooses the higher frequencies
% when set to true or the lower frequencies when set to false. This is only
% effective if the appropriate FMUseDefault...SeparationScreen flag is false.
/FMUseHighFrequencyScreens true def
%
% PostScript Level 2 printers contain an "Accurate Screens" feature which can
% improve process separation rendering at the expense of compute time. This
% flag is ignored by PostScript Level 1 printers.
/FMUseAcccurateScreens true def
%
% The following PostScript procedure defines the spot function that Frame
% products will use for process separations. You may un-comment-out one of
% the alternative functions below, or use your own.
%
% Dot function
/FMSpotFunction {abs exch abs 2 copy add 1 gt
{1 sub dup mul exch 1 sub dup mul add 1 sub }
{dup mul exch dup mul add 1 exch sub }ifelse } def
%
% Line function
% /FMSpotFunction { pop } def
%
% Elipse function
% /FMSpotFunction { dup 5 mul 8 div mul exch dup mul exch add
% sqrt 1 exch sub } def
%
%
/FMversion (4.0) def
/FMLevel1 /languagelevel where {pop languagelevel} {1} ifelse 2 lt def
/FMPColor
FMLevel1 {
false
/colorimage where {pop pop true} if
} {
true
} ifelse
def
/FrameDict 400 dict def
systemdict /errordict known not {/errordict 10 dict def
errordict /rangecheck {stop} put} if
% The readline in PS 23.0 doesn't recognize cr's as nl's on AppleTalk
FrameDict /tmprangecheck errordict /rangecheck get put
errordict /rangecheck {FrameDict /bug true put} put
FrameDict /bug false put
mark
% Some PS machines read past the CR, so keep the following 3 lines together!
currentfile 5 string readline
00
0000000000
cleartomark
errordict /rangecheck FrameDict /tmprangecheck get put
FrameDict /bug get {
/readline {
/gstring exch def
/gfile exch def
/gindex 0 def
{
gfile read pop
dup 10 eq {exit} if
dup 13 eq {exit} if
gstring exch gindex exch put
/gindex gindex 1 add def
} loop
pop
gstring 0 gindex getinterval true
} bind def
} if
/FMshowpage /showpage load def
/FMquit /quit load def
/FMFAILURE {
dup = flush
FMshowpage
/Helvetica findfont 12 scalefont setfont
72 200 moveto
show FMshowpage
FMquit
} def
/FMVERSION {
FMversion ne {
(Frame product version does not match ps_prolog!) FMFAILURE
} if
} def
/FMBADEPSF {
(PostScript Lang. Ref. Man., 2nd Ed., H.2.4 says EPS must not call X )
dup dup (X) search pop exch pop exch pop length
4 -1 roll
putinterval
FMFAILURE
} def
/FMLOCAL {
FrameDict begin
0 def
end
} def
/concatprocs
{
/proc2 exch cvlit def/proc1 exch cvlit def/newproc proc1 length proc2 length add array def
newproc 0 proc1 putinterval newproc proc1 length proc2 putinterval newproc cvx
}def
FrameDict begin
/FMnone 0 def
/FMcyan 1 def
/FMmagenta 2 def
/FMyellow 3 def
/FMblack 4 def
/FMcustom 5 def
/FrameNegative false def
/FrameSepIs FMnone def
/FrameSepBlack 0 def
/FrameSepYellow 0 def
/FrameSepMagenta 0 def
/FrameSepCyan 0 def
/FrameSepRed 1 def
/FrameSepGreen 1 def
/FrameSepBlue 1 def
/FrameCurGray 1 def
/FrameCurPat null def
/FrameCurColors [ 0 0 0 1 0 0 0 ] def
/FrameColorEpsilon .001 def
/eqepsilon {
sub dup 0 lt {neg} if
FrameColorEpsilon le
} bind def
/FrameCmpColorsCMYK {
2 copy 0 get exch 0 get eqepsilon {
2 copy 1 get exch 1 get eqepsilon {
2 copy 2 get exch 2 get eqepsilon {
3 get exch 3 get eqepsilon
} {pop pop false} ifelse
}{pop pop false} ifelse
} {pop pop false} ifelse
} bind def
/FrameCmpColorsRGB {
2 copy 4 get exch 0 get eqepsilon {
2 copy 5 get exch 1 get eqepsilon {
6 get exch 2 get eqepsilon
}{pop pop false} ifelse
} {pop pop false} ifelse
} bind def
/RGBtoCMYK {
1 exch sub
3 1 roll
1 exch sub
3 1 roll
1 exch sub
3 1 roll
3 copy
2 copy
le { pop } { exch pop } ifelse
2 copy
le { pop } { exch pop } ifelse
dup dup dup
6 1 roll
4 1 roll
7 1 roll
sub
6 1 roll
sub
5 1 roll
sub
4 1 roll
} bind def
/CMYKtoRGB {
dup dup 4 -1 roll add
5 1 roll 3 -1 roll add
4 1 roll add
1 exch sub dup 0 lt {pop 0} if 3 1 roll
1 exch sub dup 0 lt {pop 0} if exch
1 exch sub dup 0 lt {pop 0} if exch
} bind def
/FrameSepInit {
1.0 RealSetgray
} bind def
/FrameSetSepColor {
/FrameSepBlue exch def
/FrameSepGreen exch def
/FrameSepRed exch def
/FrameSepBlack exch def
/FrameSepYellow exch def
/FrameSepMagenta exch def
/FrameSepCyan exch def
/FrameSepIs FMcustom def
setCurrentScreen
} bind def
/FrameSetCyan {
/FrameSepBlue 1.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 1.0 def
/FrameSepIs FMcyan def
setCurrentScreen
} bind def

/FrameSetMagenta {
/FrameSepBlue 1.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 1.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMmagenta def
setCurrentScreen
} bind def

/FrameSetYellow {
/FrameSepBlue 0.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 1.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMyellow def
setCurrentScreen
} bind def

/FrameSetBlack {
/FrameSepBlue 0.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 1.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMblack def
setCurrentScreen
} bind def

/FrameNoSep {
/FrameSepIs FMnone def
setCurrentScreen
} bind def
/FrameSetSepColors {
FrameDict begin
[ exch 1 add 1 roll ]
/FrameSepColors
exch def end
} bind def
/FrameColorInSepListCMYK {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsCMYK
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/FrameColorInSepListRGB {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsRGB
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/RealSetgray /setgray load def
/RealSetrgbcolor /setrgbcolor load def
/RealSethsbcolor /sethsbcolor load def
end
/setgray {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetgray }
{
FrameSepIs FMblack eq
{ RealSetgray }
{ FrameSepIs FMcustom eq
FrameSepRed 0 eq and
FrameSepGreen 0 eq and
FrameSepBlue 0 eq and {
RealSetgray
} {
1 RealSetgray pop
} ifelse
} ifelse
} ifelse
end
} bind def
/setrgbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetrgbcolor }
{
3 copy [ 4 1 roll ]
FrameColorInSepListRGB
{
FrameSepBlue eq exch
FrameSepGreen eq and exch
FrameSepRed eq and
{ 0 } { 1 } ifelse
}
{
FMPColor {
RealSetrgbcolor
currentcmykcolor
} {
RGBtoCMYK
} ifelse
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
RealSetgray
}
ifelse
end
} bind def
/sethsbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSethsbcolor }
{
RealSethsbcolor
currentrgbcolor
setrgbcolor
}
ifelse
end
} bind def
FrameDict begin
/setcmykcolor where {
pop /RealSetcmykcolor /setcmykcolor load def
} {
/RealSetcmykcolor {
4 1 roll
3 { 3 index add 0 max 1 min 1 exch sub 3 1 roll} repeat
setrgbcolor pop
} bind def
} ifelse
userdict /setcmykcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetcmykcolor }
{
4 copy [ 5 1 roll ]
FrameColorInSepListCMYK
{
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
{ 0 } { 1 } ifelse
}
{
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
RealSetgray
}
ifelse
end
} bind put
FMLevel1 not {

/patProcDict 5 dict dup begin
<0f1e3c78f0e1c387> { 3 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<0f87c3e1f0783c1e> { 3 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
<8142241818244281> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-1 -1 moveto 9 9 lineto stroke } bind def
<03060c183060c081> { 1 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<8040201008040201> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
end def
/patDict 15 dict dup begin
/PatternType 1 def
/PaintType 2 def
/TilingType 3 def
/BBox [ 0 0 8 8 ] def
/XStep 8 def
/YStep 8 def
/PaintProc {
begin
patProcDict bstring known {
patProcDict bstring get exec
} {
8 8 true [1 0 0 -1 0 8] bstring imagemask
} ifelse
end
} bind def
end def
} if
/combineColor {
FrameSepIs FMnone eq
{
graymode FMLevel1 or not {

[/Pattern [/DeviceCMYK]] setcolorspace
FrameCurColors 0 4 getinterval aload pop FrameCurPat setcolor
} {
FrameCurColors 3 get 1.0 ge {
FrameCurGray RealSetgray
} {
FMPColor graymode and {
0 1 3 {
FrameCurColors exch get
1 FrameCurGray sub mul
} for
RealSetcmykcolor
} {
4 1 6 {
FrameCurColors exch get
graymode {
1 exch sub 1 FrameCurGray sub mul 1 exch sub
} {
1.0 lt {FrameCurGray} {1} ifelse
} ifelse
} for
RealSetrgbcolor
} ifelse
} ifelse
} ifelse
} {
FrameCurColors 0 4 getinterval aload
FrameColorInSepListCMYK {
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
FrameSepIs FMcustom eq and
{ FrameCurGray } { 1 } ifelse
} {
FrameSepIs FMblack eq
{FrameCurGray 1.0 exch sub mul 1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop FrameCurGray 1.0 exch sub mul 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
graymode FMLevel1 or not {

[/Pattern [/DeviceGray]] setcolorspace
FrameCurPat setcolor
} {
graymode not FMLevel1 and {

dup 1 lt {pop FrameCurGray} if
} if
RealSetgray
} ifelse
} ifelse
} bind def
/savematrix {
orgmatrix currentmatrix pop
} bind def
/restorematrix {
orgmatrix setmatrix
} bind def
/dmatrix matrix def
/dpi 72 0 dmatrix defaultmatrix dtransform
dup mul exch dup mul add sqrt def

/freq dpi dup 72 div round dup 0 eq {pop 1} if 8 mul div def
/sangle 1 0 dmatrix defaultmatrix dtransform exch atan def
/dpiranges [ 2540 2400 1693 1270 1200 635 600 0 ] def
/CMLowFreqs [ 100.402 94.8683 89.2289 100.402 94.8683 66.9349 63.2456 47.4342 ] def
/YLowFreqs [ 95.25 90.0 84.65 95.25 90.0 70.5556 66.6667 50.0 ] def
/KLowFreqs [ 89.8026 84.8528 79.8088 89.8026 84.8528 74.8355 70.7107 53.033 ] def
/CLowAngles [ 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 ] def
/MLowAngles [ 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 ] def
/YLowTDot [ true true false true true false false false ] def
/CMHighFreqs [ 133.87 126.491 133.843 108.503 102.523 100.402 94.8683 63.2456 ] def
/YHighFreqs [ 127.0 120.0 126.975 115.455 109.091 95.25 90.0 60.0 ] def
/KHighFreqs [ 119.737 113.137 119.713 128.289 121.218 89.8026 84.8528 63.6395 ] def
/CHighAngles [ 71.5651 71.5651 71.5651 70.0169 70.0169 71.5651 71.5651 71.5651 ] def
/MHighAngles [ 18.4349 18.4349 18.4349 19.9831 19.9831 18.4349 18.4349 18.4349 ] def
/YHighTDot [ false false true false false true true false ] def
/PatFreq [ 10.5833 10.0 9.4055 10.5833 10.0 10.5833 10.0 9.375 ] def
/screenIndex {
0 1 dpiranges length 1 sub { dup dpiranges exch get 1 sub dpi le {exit} {pop} ifelse } for
} bind def
/getCyanScreen {
FMUseHighFrequencyScreens { CHighAngles CMHighFreqs} {CLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getMagentaScreen {
FMUseHighFrequencyScreens { MHighAngles CMHighFreqs } {MLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getYellowScreen {
FMUseHighFrequencyScreens { YHighTDot YHighFreqs} { YLowTDot YLowFreqs } ifelse
screenIndex dup 3 1 roll get 3 1 roll get { 3 div
{2 { 1 add 2 div 3 mul dup floor sub 2 mul 1 sub exch} repeat
FMSpotFunction } } {/FMSpotFunction load } ifelse
0.0 exch
} bind def
/getBlackScreen {
FMUseHighFrequencyScreens { KHighFreqs } { KLowFreqs } ifelse
screenIndex get 45.0 /FMSpotFunction load
} bind def
/getSpotScreen {
getBlackScreen
} bind def
/getCompositeScreen {
getBlackScreen
} bind def
/FMSetScreen
FMLevel1 { /setscreen load
}{ {
8 dict begin
/HalftoneType 1 def
/SpotFunction exch def
/Angle exch def
/Frequency exch def
/AccurateScreens FMUseAcccurateScreens def
currentdict end sethalftone
} bind } ifelse
def
/setDefaultScreen {
FMPColor {
orgrxfer cvx orggxfer cvx orgbxfer cvx orgxfer cvx setcolortransfer
}
{
orgxfer cvx settransfer
} ifelse
orgfreq organgle orgproc cvx setscreen
} bind def
/setCurrentScreen {
FrameSepIs FMnone eq {
FMUseDefaultNoSeparationScreen {
setDefaultScreen
} {
getCompositeScreen FMSetScreen
} ifelse
} {
FrameSepIs FMcustom eq {
FMUseDefaultSpotSeparationScreen {
setDefaultScreen
} {
getSpotScreen FMSetScreen
} ifelse
} {
FMUseDefaultProcessSeparationScreen {
setDefaultScreen
} {
FrameSepIs FMcyan eq {
getCyanScreen FMSetScreen
} {
FrameSepIs FMmagenta eq {
getMagentaScreen FMSetScreen
} {
FrameSepIs FMyellow eq {
getYellowScreen FMSetScreen
} {
getBlackScreen FMSetScreen
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} bind def
end
/gstring FMLOCAL
/gfile FMLOCAL
/gindex FMLOCAL
/orgrxfer FMLOCAL
/orggxfer FMLOCAL
/orgbxfer FMLOCAL
/orgxfer FMLOCAL
/orgproc FMLOCAL
/orgrproc FMLOCAL
/orggproc FMLOCAL
/orgbproc FMLOCAL
/organgle FMLOCAL
/orgrangle FMLOCAL
/orggangle FMLOCAL
/orgbangle FMLOCAL
/orgfreq FMLOCAL
/orgrfreq FMLOCAL
/orggfreq FMLOCAL
/orgbfreq FMLOCAL
/yscale FMLOCAL
/xscale FMLOCAL
/edown FMLOCAL
/manualfeed FMLOCAL
/paperheight FMLOCAL
/paperwidth FMLOCAL
/FMDOCUMENT {
array /FMfonts exch def
/#copies exch def
FrameDict begin
0 ne /manualfeed exch def
/paperheight exch def
/paperwidth exch def
0 ne /FrameNegative exch def
0 ne /edown exch def
/yscale exch def
/xscale exch def
FMLevel1 {
manualfeed {setmanualfeed} if
/FMdicttop countdictstack 1 add def
/FMoptop count def
% setpapername
% manualfeed {true} {papersize} ifelse
% {manualpapersize} {false} ifelse
% {desperatepapersize} {false} ifelse
% { (Can't select requested paper size for Frame print job!) FMFAILURE } if
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
}
{{1 dict dup /PageSize [paperwidth paperheight]put setpagedevice}stopped
{ (Can't select requested paper size for Frame print job!) FMFAILURE } if
{1 dict dup /ManualFeed manualfeed put setpagedevice } stopped pop }
ifelse

FMPColor {
currentcolorscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def
cvlit /orgbproc exch def
/orgbangle exch def
/orgbfreq exch def
cvlit /orggproc exch def
/orggangle exch def
/orggfreq exch def
cvlit /orgrproc exch def
/orgrangle exch def
/orgrfreq exch def
currentcolortransfer
FrameNegative {
1 1 4 {
pop { 1 exch sub } concatprocs 4 1 roll
} for
4 copy
setcolortransfer
} if
cvlit /orgxfer exch def
cvlit /orgbxfer exch def
cvlit /orggxfer exch def
cvlit /orgrxfer exch def
} {
currentscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def

currenttransfer
FrameNegative {
{ 1 exch sub } concatprocs
dup settransfer
} if
cvlit /orgxfer exch def
} ifelse
end
} def
/pagesave FMLOCAL
/orgmatrix FMLOCAL
/landscape FMLOCAL
/pwid FMLOCAL
/FMBEGINPAGE {
FrameDict begin
/pagesave save def
3.86 setmiterlimit
/landscape exch 0 ne def
landscape {
90 rotate 0 exch dup /pwid exch def neg translate pop
}{
pop /pwid exch def
} ifelse
edown { [-1 0 0 1 pwid 0] concat } if
0 0 moveto paperwidth 0 lineto paperwidth paperheight lineto
0 paperheight lineto 0 0 lineto 1 setgray fill
xscale yscale scale
/orgmatrix matrix def
gsave
} def
/FMENDPAGE {
grestore
pagesave restore
end
showpage
} def
/FMFONTDEFINE {
FrameDict begin
findfont
ReEncode
1 index exch
definefont
FMfonts 3 1 roll
put
end
} def
/FMFILLS {
FrameDict begin dup
array /fillvals exch def
dict /patCache exch def
end
} def
/FMFILL {
FrameDict begin
fillvals 3 1 roll put
end
} def
/FMNORMALIZEGRAPHICS {
newpath
0.0 0.0 moveto
1 setlinewidth
0 setlinecap
0 0 0 sethsbcolor
0 setgray
} bind def
/fx FMLOCAL
/fy FMLOCAL
/fh FMLOCAL
/fw FMLOCAL
/llx FMLOCAL
/lly FMLOCAL
/urx FMLOCAL
/ury FMLOCAL
/FMBEGINEPSF {
end
/FMEPSF save def
/showpage {} def
% See Adobe's "PostScript Language Reference Manual, 2nd Edition", page 714.
% "...the following operators MUST NOT be used in an EPS file:" (emphasis ours)
/banddevice {(banddevice) FMBADEPSF} def
/clear {(clear) FMBADEPSF} def
/cleardictstack {(cleardictstack) FMBADEPSF} def
/copypage {(copypage) FMBADEPSF} def
/erasepage {(erasepage) FMBADEPSF} def
/exitserver {(exitserver) FMBADEPSF} def
/framedevice {(framedevice) FMBADEPSF} def
/grestoreall {(grestoreall) FMBADEPSF} def
/initclip {(initclip) FMBADEPSF} def
/initgraphics {(initgraphics) FMBADEPSF} def
/initmatrix {(initmatrix) FMBADEPSF} def
/quit {(quit) FMBADEPSF} def
/renderbands {(renderbands) FMBADEPSF} def
/setglobal {(setglobal) FMBADEPSF} def
/setpagedevice {(setpagedevice) FMBADEPSF} def
/setshared {(setshared) FMBADEPSF} def
/startjob {(startjob) FMBADEPSF} def
/lettertray {(lettertray) FMBADEPSF} def
/letter {(letter) FMBADEPSF} def
/lettersmall {(lettersmall) FMBADEPSF} def
/11x17tray {(11x17tray) FMBADEPSF} def
/11x17 {(11x17) FMBADEPSF} def
/ledgertray {(ledgertray) FMBADEPSF} def
/ledger {(ledger) FMBADEPSF} def
/legaltray {(legaltray) FMBADEPSF} def
/legal {(legal) FMBADEPSF} def
/statementtray {(statementtray) FMBADEPSF} def
/statement {(statement) FMBADEPSF} def
/executivetray {(executivetray) FMBADEPSF} def
/executive {(executive) FMBADEPSF} def
/a3tray {(a3tray) FMBADEPSF} def
/a3 {(a3) FMBADEPSF} def
/a4tray {(a4tray) FMBADEPSF} def
/a4 {(a4) FMBADEPSF} def
/a4small {(a4small) FMBADEPSF} def
/b4tray {(b4tray) FMBADEPSF} def
/b4 {(b4) FMBADEPSF} def
/b5tray {(b5tray) FMBADEPSF} def
/b5 {(b5) FMBADEPSF} def
FMNORMALIZEGRAPHICS
[/fy /fx /fh /fw /ury /urx /lly /llx] {exch def} forall
fx fw 2 div add fy fh 2 div add translate
rotate
fw 2 div neg fh 2 div neg translate
fw urx llx sub div fh ury lly sub div scale
llx neg lly neg translate
/FMdicttop countdictstack 1 add def
/FMoptop count def
} bind def
/FMENDEPSF {
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
FMEPSF restore
FrameDict begin
} bind def
FrameDict begin
/setmanualfeed {
%%BeginFeature *ManualFeed True
statusdict /manualfeed true put
%%EndFeature
} bind def
/max {2 copy lt {exch} if pop} bind def
/min {2 copy gt {exch} if pop} bind def
/inch {72 mul} def
/pagedimen {
paperheight sub abs 16 lt exch
paperwidth sub abs 16 lt and
{/papername exch def} {pop} ifelse
} bind def
/papersizedict FMLOCAL
/setpapername {
/papersizedict 14 dict def
papersizedict begin
/papername /unknown def
/Letter 8.5 inch 11.0 inch pagedimen
/LetterSmall 7.68 inch 10.16 inch pagedimen
/Tabloid 11.0 inch 17.0 inch pagedimen
/Ledger 17.0 inch 11.0 inch pagedimen
/Legal 8.5 inch 14.0 inch pagedimen
/Statement 5.5 inch 8.5 inch pagedimen
/Executive 7.5 inch 10.0 inch pagedimen
/A3 11.69 inch 16.5 inch pagedimen
/A4 8.26 inch 11.69 inch pagedimen
/A4Small 7.47 inch 10.85 inch pagedimen
/B4 10.125 inch 14.33 inch pagedimen
/B5 7.16 inch 10.125 inch pagedimen
end
} bind def
/papersize {
papersizedict begin
/Letter {lettertray letter} def
/LetterSmall {lettertray lettersmall} def
/Tabloid {11x17tray 11x17} def
/Ledger {ledgertray ledger} def
/Legal {legaltray legal} def
/Statement {statementtray statement} def
/Executive {executivetray executive} def
/A3 {a3tray a3} def
/A4 {a4tray a4} def
/A4Small {a4tray a4small} def
/B4 {b4tray b4} def
/B5 {b5tray b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
statusdict begin stopped end
} bind def
/manualpapersize {
papersizedict begin
/Letter {letter} def
/LetterSmall {lettersmall} def
/Tabloid {11x17} def
/Ledger {ledger} def
/Legal {legal} def
/Statement {statement} def
/Executive {executive} def
/A3 {a3} def
/A4 {a4} def
/A4Small {a4small} def
/B4 {b4} def
/B5 {b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
stopped
} bind def
/desperatepapersize {
statusdict /setpageparams known
{
paperwidth paperheight 0 1
statusdict begin
{setpageparams} stopped
end
} {true} ifelse
} bind def
/DiacriticEncoding [
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /space /exclam /quotedbl
/numbersign /dollar /percent /ampersand /quotesingle /parenleft
/parenright /asterisk /plus /comma /hyphen /period /slash /zero /one
/two /three /four /five /six /seven /eight /nine /colon /semicolon
/less /equal /greater /question /at /A /B /C /D /E /F /G /H /I /J /K
/L /M /N /O /P /Q /R /S /T /U /V /W /X /Y /Z /bracketleft /backslash
/bracketright /asciicircum /underscore /grave /a /b /c /d /e /f /g /h
/i /j /k /l /m /n /o /p /q /r /s /t /u /v /w /x /y /z /braceleft /bar
/braceright /asciitilde /.notdef /Adieresis /Aring /Ccedilla /Eacute
/Ntilde /Odieresis /Udieresis /aacute /agrave /acircumflex /adieresis
/atilde /aring /ccedilla /eacute /egrave /ecircumflex /edieresis
/iacute /igrave /icircumflex /idieresis /ntilde /oacute /ograve
/ocircumflex /odieresis /otilde /uacute /ugrave /ucircumflex
/udieresis /dagger /.notdef /cent /sterling /section /bullet
/paragraph /germandbls /registered /copyright /trademark /acute
/dieresis /.notdef /AE /Oslash /.notdef /.notdef /.notdef /.notdef
/yen /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/ordfeminine /ordmasculine /.notdef /ae /oslash /questiondown
/exclamdown /logicalnot /.notdef /florin /.notdef /.notdef
/guillemotleft /guillemotright /ellipsis /.notdef /Agrave /Atilde
/Otilde /OE /oe /endash /emdash /quotedblleft /quotedblright
/quoteleft /quoteright /.notdef /.notdef /ydieresis /Ydieresis
/fraction /currency /guilsinglleft /guilsinglright /fi /fl /daggerdbl
/periodcentered /quotesinglbase /quotedblbase /perthousand
/Acircumflex /Ecircumflex /Aacute /Edieresis /Egrave /Iacute
/Icircumflex /Idieresis /Igrave /Oacute /Ocircumflex /.notdef /Ograve
/Uacute /Ucircumflex /Ugrave /dotlessi /circumflex /tilde /macron
/breve /dotaccent /ring /cedilla /hungarumlaut /ogonek /caron
] def
/ReEncode {
dup
length
dict begin
{
1 index /FID ne
{def}
{pop pop} ifelse
} forall
0 eq {/Encoding DiacriticEncoding def} if
currentdict
end
} bind def
FMPColor

{
/BEGINBITMAPCOLOR {
BITMAPCOLOR} def
/BEGINBITMAPCOLORc {
BITMAPCOLORc} def
/BEGINBITMAPTRUECOLOR {
BITMAPTRUECOLOR } def
/BEGINBITMAPTRUECOLORc {
BITMAPTRUECOLORc } def
}

{
/BEGINBITMAPCOLOR {
BITMAPGRAY} def
/BEGINBITMAPCOLORc {
BITMAPGRAYc} def
/BEGINBITMAPTRUECOLOR {
BITMAPTRUEGRAY } def
/BEGINBITMAPTRUECOLORc {
BITMAPTRUEGRAYc } def
}
ifelse
/K {
FMPrintAllColorsAsBlack {
dup 1 eq 2 index 1 eq and 3 index 1 eq and not
{7 {pop} repeat 0 0 0 1 0 0 0} if
} if
FrameCurColors astore
pop combineColor
} bind def
/graymode true def
/bwidth FMLOCAL
/bpside FMLOCAL
/bstring FMLOCAL
/onbits FMLOCAL
/offbits FMLOCAL
/xindex FMLOCAL
/yindex FMLOCAL
/x FMLOCAL
/y FMLOCAL
/setPatternMode {
FMLevel1 {
/bwidth exch def
/bpside exch def
/bstring exch def
/onbits 0 def /offbits 0 def
freq sangle landscape {90 add} if
{/y exch def
/x exch def
/xindex x 1 add 2 div bpside mul cvi def
/yindex y 1 add 2 div bpside mul cvi def
bstring yindex bwidth mul xindex 8 idiv add get
1 7 xindex 8 mod sub bitshift and 0 ne FrameNegative {not} if
{/onbits onbits 1 add def 1}
{/offbits offbits 1 add def 0}
ifelse
}
setscreen
offbits offbits onbits add div FrameNegative {1.0 exch sub} if
/FrameCurGray exch def
} {
pop pop
dup patCache exch known {
patCache exch get
} {
dup
patDict /bstring 3 -1 roll put
patDict
9 PatFreq screenIndex get div dup matrix scale
makepattern
dup
patCache 4 -1 roll 3 -1 roll put
} ifelse
/FrameCurGray 0 def
/FrameCurPat exch def
} ifelse
/graymode false def
combineColor
} bind def
/setGrayScaleMode {
graymode not {
/graymode true def
FMLevel1 {
setCurrentScreen
} if
} if
/FrameCurGray exch def
combineColor
} bind def
/normalize {
transform round exch round exch itransform
} bind def
/dnormalize {
dtransform round exch round exch idtransform
} bind def
/lnormalize {
0 dtransform exch cvi 2 idiv 2 mul 1 add exch idtransform pop
} bind def
/H {
lnormalize setlinewidth
} bind def
/Z {
setlinecap
} bind def

/PFill {
graymode FMLevel1 or not {
gsave 1 setgray eofill grestore
} if
} bind def
/PStroke {
graymode FMLevel1 or not {
gsave 1 setgray stroke grestore
} if
stroke
} bind def
/fillvals FMLOCAL
/X {
fillvals exch get
dup type /stringtype eq
{8 1 setPatternMode}
{setGrayScaleMode}
ifelse
} bind def
/V {
PFill gsave eofill grestore
} bind def
/Vclip {
clip
} bind def
/Vstrk {
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/N {
PStroke
} bind def
/Nclip {
strokepath clip newpath
} bind def
/Nstrk {
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/M {newpath moveto} bind def
/E {lineto} bind def
/D {curveto} bind def
/O {closepath} bind def
/n FMLOCAL
/L {
/n exch def
newpath
normalize
moveto
2 1 n {pop normalize lineto} for
} bind def
/Y {
L
closepath
} bind def
/x1 FMLOCAL
/x2 FMLOCAL
/y1 FMLOCAL
/y2 FMLOCAL
/R {
/y2 exch def
/x2 exch def
/y1 exch def
/x1 exch def
x1 y1
x2 y1
x2 y2
x1 y2
4 Y
} bind def
/rad FMLOCAL
/rarc
{rad
arcto
} bind def
/RR {
/rad exch def
normalize
/y2 exch def
/x2 exch def
normalize
/y1 exch def
/x1 exch def
mark
newpath
{
x1 y1 rad add moveto
x1 y2 x2 y2 rarc
x2 y2 x2 y1 rarc
x2 y1 x1 y1 rarc
x1 y1 x1 y2 rarc
closepath
} stopped {x1 y1 x2 y2 R} if
cleartomark
} bind def
/RRR {
/rad exch def
normalize /y4 exch def /x4 exch def
normalize /y3 exch def /x3 exch def
normalize /y2 exch def /x2 exch def
normalize /y1 exch def /x1 exch def
newpath
normalize moveto
mark
{
x2 y2 x3 y3 rarc
x3 y3 x4 y4 rarc
x4 y4 x1 y1 rarc
x1 y1 x2 y2 rarc
closepath
} stopped
{x1 y1 x2 y2 x3 y3 x4 y4 newpath moveto lineto lineto lineto closepath} if
cleartomark
} bind def
/C {
grestore
gsave
R
clip
setCurrentScreen
} bind def
/CP {
grestore
gsave
Y
clip
setCurrentScreen
} bind def
/FMpointsize FMLOCAL
/F {
FMfonts exch get
FMpointsize scalefont
setfont
} bind def
/Q {
/FMpointsize exch def
F
} bind def
/T {
moveto show
} bind def
/RF {
rotate
0 ne {-1 1 scale} if
} bind def
/TF {
gsave
moveto
RF
show
grestore
} bind def
/P {
moveto
0 32 3 2 roll widthshow
} bind def
/PF {
gsave
moveto
RF
0 32 3 2 roll widthshow
grestore
} bind def
/S {
moveto
0 exch ashow
} bind def
/SF {
gsave
moveto
RF
0 exch ashow
grestore
} bind def
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%%EndProlog
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(GHRS Instrument Handbook 5.0) 207 60.29 T
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1.2 (Chapter 6) 72 677 S
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-0.48 (Design and Construction) 207 677 S
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(6.1) 144 424 T
( The HST Focal Plane and the GHRS Apertures) 164.02 424 T
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( 56) 505.32 424 T
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(6.2) 144 406 T
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( 60) 505.32 406 T
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(6.3) 144 388 T
( The Digicon Detectors) 164.02 388 T
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( 62) 505.32 388 T
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(Design and Construction of the GHRS) 189 736.18 T
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(56) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
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(6.1) 163.32 678.02 T
(The HST Focal Plane and the GHRS Apertures) 189 678.02 T
5 10 Q
-0.06 (W) 189 654.35 P
-0.06 (e provide here a description of the instrument in lar) 197.64 654.35 P
-0.06 (gely pictorial terms. More illustra-) 402.19 654.35 P
0.67 (tions and full technical descriptions of the GHRS may be found in the references \050see) 189 642.35 P
(Section) 189 630.35 T
(9.2 on page) 221.5 630.35 T
(102\051.) 270.38 630.35 T
54 87.98 540 686.02 C
54 132.98 540 492.98 C
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54 87.98 540 686.02 C
54 87.98 540 132.98 C
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0 X
0 0 0 1 0 0 0 K
(Figure 6-1) 207 109.15 T
3 F
(. The Hubble Space T) 254.79 109.15 T
(elescope and its components, with the) 350.95 109.15 T
(locations of important operational elements shown.) 207 99.15 T
54 87.98 540 686.02 C
0 0 612 792 C
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0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (57) 546.88 60.29 P
72 750.02 558 750.02 2 L
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72 726.98 558 726.98 2 L
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72 726.98 558 726.98 2 L
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(Design and Construction of the GHRS) 207 736.18 T
72 87.98 558 686.02 C
72 118.15 558 478.15 C
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(Figure 6-2.) 207 109.15 T
3 F
(The focal plane of HST and the de\336nitions of the V2, V3 and U2,) 260.35 109.15 T
(U3 coordinate systems of the spacecraft.) 207 99.15 T
72 87.98 558 686.02 C
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(Design and Construction of the GHRS) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
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54 74.02 540 74.02 2 L
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0 10 Q
(58) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
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0 Z
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54 726.98 540 726.98 2 L
0.25 H
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54 74.02 540 74.02 2 L
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54 750.02 540 750.02 2 L
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0 Z
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54 726.98 540 726.98 2 L
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54 74.02 540 74.02 2 L
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54 87.98 540 686.02 C
0 0 612 792 C
54 87.98 540 686.02 C
54 87.98 540 168.12 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(Figure 6-3.) 189 159.12 T
3 F
( Locations of GHRS apertures relative to spacecraft axes. Note) 239.57 159.12 T
(that the sense of the) 189 149.12 T
4 F
(x) 282.4 149.12 T
3 F
( and) 287.4 149.12 T
4 F
(y) 309.64 149.12 T
3 F
( motions are shown by the arrows, but that the) 314.64 149.12 T
(zero point for each aperture \050SSA and LSA\051 is located at its center) 189 139.12 T
(. COST) 481.37 139.12 T
(AR) 513.97 139.12 T
(does not, of course, change the layout of the entrance apertures, but it does) 189 129.12 T
(alter the way that the sky is imaged onto the focal plane. The sense is easy) 189 119.12 T
(to remember: the COST) 189 109.12 T
(AR mirrors invert the sense of the original image,) 294.96 109.12 T
(which means that the signs of motions in both coordinates, V2 and V3, \050or U2) 189 99.12 T
(and U3\051 are reversed.) 189 89.12 T
54 87.98 540 686.02 C
0 0 612 792 C
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[0 0 0 1 0 0 0]
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[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (59) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Design and Construction of the GHRS) 207 736.18 T
72 90 558 688.03 C
72 116.14 558 428.47 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 90 558 688.03 C
0 0 612 792 C
72 90 558 688.03 C
72 90 558 116.14 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(Figure 6-4.) 207 107.14 T
3 F
( Optical schematic of the GHRS.) 257.57 107.14 T
72 90 558 688.03 C
0 0 612 792 C
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Design and Construction of the GHRS) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(60) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 671.02 540 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 672.52 540 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 672.52 180 672.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(6.2) 163.32 678.02 T
(Gratings and Optical Elements) 189 678.02 T
5 10 Q
1.54 (Note that the \322CD\323 gratings are cross-dispersers for the echelles. CD-A has a focal) 189 433.35 P
0.68 (length of 1460 mm and CD-B has a focal length of 1340 mm. Note also that the \322M\323) 189 421.35 P
-0.11 (gratings are holographic and that the blaze angle quoted formally is that which correctly) 189 409.35 P
1.09 (predicts the center of the wavelength region the grating is optimized for) 189 397.35 P
1.09 (. G140L is a) 487.3 397.35 P
0.41 (ruled grating. \322Ech-A\323 and \322Ech-B\323 refer to two modes of operation that use the same) 189 385.35 P
(echelle grating but dif) 189 373.35 T
(ferent cross-dispersers and detectors.) 276.86 373.35 T
197.42 112.02 486.58 119.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 612 792 C
5 9 Q
0 X
0 0 0 1 0 0 0 K
-0.35 (a. Mirror N2 is actually \322D\323 shaped, being a circle with a small slice of) 197.42 106.02 P
-0.35 (f one) 448.79 106.02 P
(side. It is about 60) 204.62 96.02 T
6 F
(\264) 273.12 96.02 T
5 F
( 80 mm.) 278.06 96.02 T
54 632.02 540 645.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 639.02 540 639.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 639.02 180 639.02 2 L
0 Z
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 626.02 T
(ABLE 6-1) 58.83 626.02 T
3 F
(Properties of GHRS Gratings) 189 626.02 T
0 8 Q
(Name) 117.6 593.68 T
(Grooves) 176.37 602.68 T
(per mm) 178.15 593.68 T
(Blaze) 236.15 602.68 T
(Angle) 235.49 593.68 T
(Order of) 284.82 602.68 T
(use) 293.71 593.68 T
(Angle of) 338.6 602.68 T
(Incidence) 336.15 593.68 T
-0.92 (Diffraction) 388.9 602.68 P
(Angle) 397.79 593.68 T
(Deviation) 444.9 602.68 T
(Angle) 451.79 593.68 T
(Detector) 500.38 593.68 T
5 9 Q
(G140L) 117.6 579.02 T
(600) 185.85 579.02 T
(2.6) 240.98 579.02 T
(1) 298.35 579.02 T
(9.0 \320 10.3) 336.6 579.02 T
(-5.3 \320 -4.0) 390.15 579.02 T
(14.25) 452.77 579.02 T
(D1) 511.1 579.02 T
(G140M) 117.6 564.02 T
(6000) 183.6 564.02 T
(23) 242.1 564.02 T
(1) 298.35 564.02 T
(26 \320 38) 341.1 564.02 T
(1) 395.57 564.02 T
(1 \320 24) 399.73 564.02 T
(14.25) 452.77 564.02 T
(D1) 511.1 564.02 T
(G160M) 117.6 549.02 T
(4960) 183.6 549.02 T
(19) 242.1 549.02 T
(1) 298.35 549.02 T
(21 \320 33) 341.1 549.02 T
(14 \320 27) 395.4 549.02 T
(6.25) 455.02 549.02 T
(D2) 511.1 549.02 T
(G200M) 117.6 534.02 T
(4320) 183.6 534.02 T
(26) 242.1 534.02 T
(1) 298.35 534.02 T
(23 \320 34) 341.1 534.02 T
(17 \320 28) 395.4 534.02 T
(6.25) 455.02 534.02 T
(D2) 511.1 534.02 T
(G270M) 117.6 519.02 T
(3600) 183.6 519.02 T
(28) 242.1 519.02 T
(1) 298.35 519.02 T
(27 \320 38) 341.1 519.02 T
(20 \320 32) 395.4 519.02 T
(6.25) 455.02 519.02 T
(D2) 511.1 519.02 T
(Ech-A) 117.6 504.02 T
(316) 185.85 504.02 T
(63.4) 238.73 504.02 T
(33 \320 53) 287.1 504.02 T
(68 \320 74) 341.1 504.02 T
(54 \320 61) 395.4 504.02 T
(13.25) 452.77 504.02 T
(D1) 511.1 504.02 T
(Ech-B) 117.6 489.02 T
(316) 185.85 489.02 T
(63.4) 238.73 489.02 T
(17 \320 33) 287.1 489.02 T
(63 \320 72) 341.1 489.02 T
(58 \320 66) 395.4 489.02 T
(5.75) 455.02 489.02 T
(D2) 511.1 489.02 T
(CD-A) 117.6 474.02 T
(194.6) 182.48 474.02 T
(0.75) 238.73 474.02 T
(1) 298.35 474.02 T
(D1) 511.1 474.02 T
(CD-B) 117.6 459.02 T
(85.7) 184.73 459.02 T
(0.54) 238.73 459.02 T
(1) 298.35 459.02 T
(D2) 511.1 459.02 T
54 327.02 540 340.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 334.02 540 334.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 334.02 180 334.02 2 L
0 Z
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 321.02 T
(ABLE 6-2) 58.83 321.02 T
3 F
(Properties of Other GHRS Optical Components) 189 321.02 T
0 8 Q
(Name) 203.42 288.68 T
(Clear Aperture) 283 297.68 T
(\050mm\051) 301.01 288.68 T
(Focal Length) 367.18 297.68 T
(\050mm\051) 382.3 288.68 T
(Detector) 443.35 288.68 T
5 9 Q
(LSA = \322) 203.42 274.02 T
7 F
(2.0) 234 274.02 T
5 F
(\323) 250.2 274.02 T
(0.559) 300.66 274.02 T
(D1, D2) 446.33 274.02 T
(SSA = \322) 203.42 259.02 T
7 F
(0.25) 233.5 259.02 T
5 F
(\323) 255.1 259.02 T
(0.067) 300.66 259.02 T
(D1, D2) 446.33 259.02 T
(Collimator) 203.42 244.02 T
(80) 306.29 244.02 T
(1850) 383.08 244.02 T
(D1, D2) 446.33 244.02 T
(Mirror N2) 203.42 229.02 T
5 7.2 Q
(a) 240.67 232.61 T
5 9 Q
(80) 306.29 229.02 T
(D2) 454.08 229.02 T
(Mirror A2) 203.42 214.02 T
(20) 306.29 214.02 T
(D2) 454.08 214.02 T
(Mirror N1) 203.42 199.02 T
(80) 306.29 199.02 T
(D1) 454.08 199.02 T
(Mirror A1) 203.42 184.02 T
(20) 306.29 184.02 T
(D1) 454.08 184.02 T
(Cam-A) 203.42 169.02 T
(84) 306.29 169.02 T
(1425) 383.08 169.02 T
(D1) 454.08 169.02 T
(Cam-B) 203.42 154.02 T
(86) 306.29 154.02 T
(1350) 383.08 154.02 T
(D2) 454.08 154.02 T
(D1) 203.42 139.02 T
(22) 297.07 139.02 T
6 F
( \264) 306.07 139.02 T
5 F
( 28) 313.26 139.02 T
(D2) 203.42 124.02 T
(22) 297.07 124.02 T
6 F
( \264) 306.07 124.02 T
5 F
( 28) 313.26 124.02 T
111.6 614.89 111.6 454.14 2 L
V
0.25 H
0 Z
N
165.6 615.14 165.6 453.89 2 L
V
0.5 H
N
219.6 615.14 219.6 453.89 2 L
V
0.25 H
N
273.6 615.14 273.6 453.89 2 L
V
N
327.6 615.14 327.6 453.89 2 L
V
N
381.6 615.14 381.6 453.89 2 L
V
N
436.2 615.14 436.2 453.89 2 L
V
N
489.6 615.14 489.6 453.89 2 L
V
N
543.6 614.89 543.6 454.14 2 L
V
N
111.47 615.02 543.72 615.02 2 L
V
N
111.47 589.02 543.72 589.02 2 L
V
0.5 H
N
111.47 574.02 543.72 574.02 2 L
V
0.25 H
N
111.47 559.02 543.72 559.02 2 L
V
N
111.47 544.02 543.72 544.02 2 L
V
N
111.47 529.02 543.72 529.02 2 L
V
N
111.47 514.02 543.72 514.02 2 L
V
N
111.47 499.02 543.72 499.02 2 L
V
N
111.47 484.02 543.72 484.02 2 L
V
N
111.47 469.02 543.72 469.02 2 L
V
N
111.47 454.02 543.72 454.02 2 L
V
N
197.42 309.89 197.42 119.14 2 L
V
N
270 310.14 270 118.89 2 L
V
0.5 H
N
351.58 310.14 351.58 118.89 2 L
V
0.25 H
N
432.58 310.14 432.58 118.89 2 L
V
N
486.58 309.89 486.58 119.14 2 L
V
N
197.3 310.02 486.7 310.02 2 L
V
N
197.3 284.02 486.7 284.02 2 L
V
0.5 H
N
197.3 269.02 486.7 269.02 2 L
V
0.25 H
N
197.3 254.02 486.7 254.02 2 L
V
N
197.3 239.02 486.7 239.02 2 L
V
N
197.3 224.02 486.7 224.02 2 L
V
N
197.3 209.02 486.7 209.02 2 L
V
N
197.3 194.02 486.7 194.02 2 L
V
N
197.3 179.02 486.7 179.02 2 L
V
N
197.3 164.02 486.7 164.02 2 L
V
N
197.3 149.02 486.7 149.02 2 L
V
N
197.3 134.02 486.7 134.02 2 L
V
N
197.3 119.02 486.7 119.02 2 L
V
N
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[0 0 0 1 0 0 0]
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[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (61) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Design and Construction of the GHRS) 207 736.18 T
72 87.98 558 686.02 C
72 118.15 558 427.75 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 87.98 558 686.02 C
0 0 612 792 C
72 87.98 558 686.02 C
72 87.98 558 118.15 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(Figure 6-5.) 207 109.15 T
3 F
( Schematic diagram of GHRS\325 acquisition optics. The \322main) 257.57 109.15 T
(acquisition mirror\323 is N2.) 207 99.15 T
72 87.98 558 686.02 C
0 0 612 792 C
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[0 0 0 1 0 0 0]
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[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Design and Construction of the GHRS) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(62) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
72 636.02 558 639.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 637.52 558 637.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 637.52 198 637.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(6.3) 181.32 643.02 T
(The Digicon Detectors) 207 643.02 T
72 87.98 558 686.02 C
72 102.17 558 411.77 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 87.98 558 686.02 C
0 0 612 792 C
72 87.98 558 686.02 C
72 87.98 558 102.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(Figure 6-6.) 207 93.17 T
3 F
( Cutaway view of a Digicon.) 257.57 93.17 T
72 87.98 558 686.02 C
0 0 612 792 C
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[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (63) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Design and Construction of the GHRS) 207 736.18 T
72 87.98 558 686.02 C
72 120.17 558 501.77 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 87.98 558 686.02 C
0 0 612 792 C
72 87.98 558 686.02 C
72 87.98 558 120.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(Figure 6-7.) 207 102.17 T
3 F
( Cross-sectional view of a Digicon and views of its faceplate and) 257.57 102.17 T
(diode arrays.) 207 92.17 T
72 87.98 558 686.02 C
0 0 612 792 C
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[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Design and Construction of the GHRS) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(64) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
72 87.98 558 686.02 C
72 120.17 558 501.77 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 87.98 558 686.02 C
0 0 612 792 C
72 87.98 558 686.02 C
72 87.98 558 120.17 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(Figure 6-8.) 207 102.17 T
3 F
( A view from the cross-dispersers toward the Digicon detectors to) 257.57 102.17 T
(illustrate the senses of) 207 92.17 T
4 F
(x) 309.27 92.17 T
3 F
( and) 314.27 92.17 T
4 F
(y) 336.51 92.17 T
3 F
( motions and of increasing wavelength.) 341.51 92.17 T
72 87.98 558 686.02 C
0 0 612 792 C
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[0 0 0 1 0 0 0]
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[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (65) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Design and Construction of the GHRS) 207 736.18 T
54 87.98 540 686.02 C
54 134.14 540 515.74 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 87.98 540 686.02 C
0 0 612 792 C
54 87.98 540 686.02 C
54 87.98 540 134.14 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
0 X
0 0 0 1 0 0 0 K
(Figure 6-9.) 189 116.14 T
3 F
( A detailed layout of the diodes in the Digicon detectors. Note) 239.57 116.14 T
(the 6 large \322corner diodes\323 and the 6 \322focus diodes\323 \050numbers 4, 5, and 6, for) 189 106.14 T
(example\051.) 189 96.14 T
54 87.98 540 686.02 C
0 0 612 792 C
FMENDPAGE
%%EndPage: "65" 11
%%Page: "66" 12
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Design and Construction of the GHRS) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(66) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
FMENDPAGE
%%EndPage: "66" 12
%%Trailer
%%BoundingBox: 0 0 612 792
%%PageOrder: Ascend
%%Pages: 12
%%DocumentFonts: Helvetica-Bold
%%+ Palatino-BoldItalic
%%+ Palatino-Italic
%%+ Helvetica
%%+ Helvetica-Oblique
%%+ Times-Roman
%%+ Symbol
%%+ Courier
%%EOF
%!PS-Adobe-3.0
%%BoundingBox: (atend)
%%Pages: (atend)
%%PageOrder: (atend)
%%DocumentFonts: (atend)
%%Creator: Frame 4.0
%%DocumentData: Clean7Bit
%%EndComments
%%BeginProlog
%
% Frame ps_prolog 4.0, for use with Frame 4.0 products
% This ps_prolog file is Copyright (c) 1986-1993 Frame Technology
% Corporation. All rights reserved. This ps_prolog file may be
% freely copied and distributed in conjunction with documents created
% using FrameMaker, FrameBuilder and FrameViewer as long as this
% copyright notice is preserved.
%
% Frame products normally print colors as their true color on a color printer
% or as shades of gray, based on luminance, on a black-and white printer. The
% following flag, if set to True, forces all non-white colors to print as pure
% black. This has no effect on bitmap images.
/FMPrintAllColorsAsBlack false def
%
% Frame products can either set their own line screens or use a printer's
% default settings. Three flags below control this separately for no
% separations, spot separations and process separations. If a flag
% is true, then the default printer settings will not be changed. If it is
% false, Frame products will use their own settings from a table based on
% the printer's resolution.
/FMUseDefaultNoSeparationScreen true def
/FMUseDefaultSpotSeparationScreen true def
/FMUseDefaultProcessSeparationScreen false def
%
% For any given PostScript printer resolution, Frame products have two sets of
% screen angles and frequencies for printing process separations, which are
% recomended by Adobe. The following variable chooses the higher frequencies
% when set to true or the lower frequencies when set to false. This is only
% effective if the appropriate FMUseDefault...SeparationScreen flag is false.
/FMUseHighFrequencyScreens true def
%
% PostScript Level 2 printers contain an "Accurate Screens" feature which can
% improve process separation rendering at the expense of compute time. This
% flag is ignored by PostScript Level 1 printers.
/FMUseAcccurateScreens true def
%
% The following PostScript procedure defines the spot function that Frame
% products will use for process separations. You may un-comment-out one of
% the alternative functions below, or use your own.
%
% Dot function
/FMSpotFunction {abs exch abs 2 copy add 1 gt
{1 sub dup mul exch 1 sub dup mul add 1 sub }
{dup mul exch dup mul add 1 exch sub }ifelse } def
%
% Line function
% /FMSpotFunction { pop } def
%
% Elipse function
% /FMSpotFunction { dup 5 mul 8 div mul exch dup mul exch add
% sqrt 1 exch sub } def
%
%
/FMversion (4.0) def
/FMLevel1 /languagelevel where {pop languagelevel} {1} ifelse 2 lt def
/FMPColor
FMLevel1 {
false
/colorimage where {pop pop true} if
} {
true
} ifelse
def
/FrameDict 400 dict def
systemdict /errordict known not {/errordict 10 dict def
errordict /rangecheck {stop} put} if
% The readline in PS 23.0 doesn't recognize cr's as nl's on AppleTalk
FrameDict /tmprangecheck errordict /rangecheck get put
errordict /rangecheck {FrameDict /bug true put} put
FrameDict /bug false put
mark
% Some PS machines read past the CR, so keep the following 3 lines together!
currentfile 5 string readline
00
0000000000
cleartomark
errordict /rangecheck FrameDict /tmprangecheck get put
FrameDict /bug get {
/readline {
/gstring exch def
/gfile exch def
/gindex 0 def
{
gfile read pop
dup 10 eq {exit} if
dup 13 eq {exit} if
gstring exch gindex exch put
/gindex gindex 1 add def
} loop
pop
gstring 0 gindex getinterval true
} bind def
} if
/FMshowpage /showpage load def
/FMquit /quit load def
/FMFAILURE {
dup = flush
FMshowpage
/Helvetica findfont 12 scalefont setfont
72 200 moveto
show FMshowpage
FMquit
} def
/FMVERSION {
FMversion ne {
(Frame product version does not match ps_prolog!) FMFAILURE
} if
} def
/FMBADEPSF {
(PostScript Lang. Ref. Man., 2nd Ed., H.2.4 says EPS must not call X )
dup dup (X) search pop exch pop exch pop length
4 -1 roll
putinterval
FMFAILURE
} def
/FMLOCAL {
FrameDict begin
0 def
end
} def
/concatprocs
{
/proc2 exch cvlit def/proc1 exch cvlit def/newproc proc1 length proc2 length add array def
newproc 0 proc1 putinterval newproc proc1 length proc2 putinterval newproc cvx
}def
FrameDict begin
/FMnone 0 def
/FMcyan 1 def
/FMmagenta 2 def
/FMyellow 3 def
/FMblack 4 def
/FMcustom 5 def
/FrameNegative false def
/FrameSepIs FMnone def
/FrameSepBlack 0 def
/FrameSepYellow 0 def
/FrameSepMagenta 0 def
/FrameSepCyan 0 def
/FrameSepRed 1 def
/FrameSepGreen 1 def
/FrameSepBlue 1 def
/FrameCurGray 1 def
/FrameCurPat null def
/FrameCurColors [ 0 0 0 1 0 0 0 ] def
/FrameColorEpsilon .001 def
/eqepsilon {
sub dup 0 lt {neg} if
FrameColorEpsilon le
} bind def
/FrameCmpColorsCMYK {
2 copy 0 get exch 0 get eqepsilon {
2 copy 1 get exch 1 get eqepsilon {
2 copy 2 get exch 2 get eqepsilon {
3 get exch 3 get eqepsilon
} {pop pop false} ifelse
}{pop pop false} ifelse
} {pop pop false} ifelse
} bind def
/FrameCmpColorsRGB {
2 copy 4 get exch 0 get eqepsilon {
2 copy 5 get exch 1 get eqepsilon {
6 get exch 2 get eqepsilon
}{pop pop false} ifelse
} {pop pop false} ifelse
} bind def
/RGBtoCMYK {
1 exch sub
3 1 roll
1 exch sub
3 1 roll
1 exch sub
3 1 roll
3 copy
2 copy
le { pop } { exch pop } ifelse
2 copy
le { pop } { exch pop } ifelse
dup dup dup
6 1 roll
4 1 roll
7 1 roll
sub
6 1 roll
sub
5 1 roll
sub
4 1 roll
} bind def
/CMYKtoRGB {
dup dup 4 -1 roll add
5 1 roll 3 -1 roll add
4 1 roll add
1 exch sub dup 0 lt {pop 0} if 3 1 roll
1 exch sub dup 0 lt {pop 0} if exch
1 exch sub dup 0 lt {pop 0} if exch
} bind def
/FrameSepInit {
1.0 RealSetgray
} bind def
/FrameSetSepColor {
/FrameSepBlue exch def
/FrameSepGreen exch def
/FrameSepRed exch def
/FrameSepBlack exch def
/FrameSepYellow exch def
/FrameSepMagenta exch def
/FrameSepCyan exch def
/FrameSepIs FMcustom def
setCurrentScreen
} bind def
/FrameSetCyan {
/FrameSepBlue 1.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 1.0 def
/FrameSepIs FMcyan def
setCurrentScreen
} bind def

/FrameSetMagenta {
/FrameSepBlue 1.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 1.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMmagenta def
setCurrentScreen
} bind def

/FrameSetYellow {
/FrameSepBlue 0.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 1.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMyellow def
setCurrentScreen
} bind def

/FrameSetBlack {
/FrameSepBlue 0.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 1.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMblack def
setCurrentScreen
} bind def

/FrameNoSep {
/FrameSepIs FMnone def
setCurrentScreen
} bind def
/FrameSetSepColors {
FrameDict begin
[ exch 1 add 1 roll ]
/FrameSepColors
exch def end
} bind def
/FrameColorInSepListCMYK {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsCMYK
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/FrameColorInSepListRGB {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsRGB
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/RealSetgray /setgray load def
/RealSetrgbcolor /setrgbcolor load def
/RealSethsbcolor /sethsbcolor load def
end
/setgray {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetgray }
{
FrameSepIs FMblack eq
{ RealSetgray }
{ FrameSepIs FMcustom eq
FrameSepRed 0 eq and
FrameSepGreen 0 eq and
FrameSepBlue 0 eq and {
RealSetgray
} {
1 RealSetgray pop
} ifelse
} ifelse
} ifelse
end
} bind def
/setrgbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetrgbcolor }
{
3 copy [ 4 1 roll ]
FrameColorInSepListRGB
{
FrameSepBlue eq exch
FrameSepGreen eq and exch
FrameSepRed eq and
{ 0 } { 1 } ifelse
}
{
FMPColor {
RealSetrgbcolor
currentcmykcolor
} {
RGBtoCMYK
} ifelse
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
RealSetgray
}
ifelse
end
} bind def
/sethsbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSethsbcolor }
{
RealSethsbcolor
currentrgbcolor
setrgbcolor
}
ifelse
end
} bind def
FrameDict begin
/setcmykcolor where {
pop /RealSetcmykcolor /setcmykcolor load def
} {
/RealSetcmykcolor {
4 1 roll
3 { 3 index add 0 max 1 min 1 exch sub 3 1 roll} repeat
setrgbcolor pop
} bind def
} ifelse
userdict /setcmykcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetcmykcolor }
{
4 copy [ 5 1 roll ]
FrameColorInSepListCMYK
{
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
{ 0 } { 1 } ifelse
}
{
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
RealSetgray
}
ifelse
end
} bind put
FMLevel1 not {

/patProcDict 5 dict dup begin
<0f1e3c78f0e1c387> { 3 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<0f87c3e1f0783c1e> { 3 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
<8142241818244281> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-1 -1 moveto 9 9 lineto stroke } bind def
<03060c183060c081> { 1 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<8040201008040201> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
end def
/patDict 15 dict dup begin
/PatternType 1 def
/PaintType 2 def
/TilingType 3 def
/BBox [ 0 0 8 8 ] def
/XStep 8 def
/YStep 8 def
/PaintProc {
begin
patProcDict bstring known {
patProcDict bstring get exec
} {
8 8 true [1 0 0 -1 0 8] bstring imagemask
} ifelse
end
} bind def
end def
} if
/combineColor {
FrameSepIs FMnone eq
{
graymode FMLevel1 or not {

[/Pattern [/DeviceCMYK]] setcolorspace
FrameCurColors 0 4 getinterval aload pop FrameCurPat setcolor
} {
FrameCurColors 3 get 1.0 ge {
FrameCurGray RealSetgray
} {
FMPColor graymode and {
0 1 3 {
FrameCurColors exch get
1 FrameCurGray sub mul
} for
RealSetcmykcolor
} {
4 1 6 {
FrameCurColors exch get
graymode {
1 exch sub 1 FrameCurGray sub mul 1 exch sub
} {
1.0 lt {FrameCurGray} {1} ifelse
} ifelse
} for
RealSetrgbcolor
} ifelse
} ifelse
} ifelse
} {
FrameCurColors 0 4 getinterval aload
FrameColorInSepListCMYK {
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
FrameSepIs FMcustom eq and
{ FrameCurGray } { 1 } ifelse
} {
FrameSepIs FMblack eq
{FrameCurGray 1.0 exch sub mul 1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop FrameCurGray 1.0 exch sub mul 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
graymode FMLevel1 or not {

[/Pattern [/DeviceGray]] setcolorspace
FrameCurPat setcolor
} {
graymode not FMLevel1 and {

dup 1 lt {pop FrameCurGray} if
} if
RealSetgray
} ifelse
} ifelse
} bind def
/savematrix {
orgmatrix currentmatrix pop
} bind def
/restorematrix {
orgmatrix setmatrix
} bind def
/dmatrix matrix def
/dpi 72 0 dmatrix defaultmatrix dtransform
dup mul exch dup mul add sqrt def

/freq dpi dup 72 div round dup 0 eq {pop 1} if 8 mul div def
/sangle 1 0 dmatrix defaultmatrix dtransform exch atan def
/dpiranges [ 2540 2400 1693 1270 1200 635 600 0 ] def
/CMLowFreqs [ 100.402 94.8683 89.2289 100.402 94.8683 66.9349 63.2456 47.4342 ] def
/YLowFreqs [ 95.25 90.0 84.65 95.25 90.0 70.5556 66.6667 50.0 ] def
/KLowFreqs [ 89.8026 84.8528 79.8088 89.8026 84.8528 74.8355 70.7107 53.033 ] def
/CLowAngles [ 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 ] def
/MLowAngles [ 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 ] def
/YLowTDot [ true true false true true false false false ] def
/CMHighFreqs [ 133.87 126.491 133.843 108.503 102.523 100.402 94.8683 63.2456 ] def
/YHighFreqs [ 127.0 120.0 126.975 115.455 109.091 95.25 90.0 60.0 ] def
/KHighFreqs [ 119.737 113.137 119.713 128.289 121.218 89.8026 84.8528 63.6395 ] def
/CHighAngles [ 71.5651 71.5651 71.5651 70.0169 70.0169 71.5651 71.5651 71.5651 ] def
/MHighAngles [ 18.4349 18.4349 18.4349 19.9831 19.9831 18.4349 18.4349 18.4349 ] def
/YHighTDot [ false false true false false true true false ] def
/PatFreq [ 10.5833 10.0 9.4055 10.5833 10.0 10.5833 10.0 9.375 ] def
/screenIndex {
0 1 dpiranges length 1 sub { dup dpiranges exch get 1 sub dpi le {exit} {pop} ifelse } for
} bind def
/getCyanScreen {
FMUseHighFrequencyScreens { CHighAngles CMHighFreqs} {CLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getMagentaScreen {
FMUseHighFrequencyScreens { MHighAngles CMHighFreqs } {MLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getYellowScreen {
FMUseHighFrequencyScreens { YHighTDot YHighFreqs} { YLowTDot YLowFreqs } ifelse
screenIndex dup 3 1 roll get 3 1 roll get { 3 div
{2 { 1 add 2 div 3 mul dup floor sub 2 mul 1 sub exch} repeat
FMSpotFunction } } {/FMSpotFunction load } ifelse
0.0 exch
} bind def
/getBlackScreen {
FMUseHighFrequencyScreens { KHighFreqs } { KLowFreqs } ifelse
screenIndex get 45.0 /FMSpotFunction load
} bind def
/getSpotScreen {
getBlackScreen
} bind def
/getCompositeScreen {
getBlackScreen
} bind def
/FMSetScreen
FMLevel1 { /setscreen load
}{ {
8 dict begin
/HalftoneType 1 def
/SpotFunction exch def
/Angle exch def
/Frequency exch def
/AccurateScreens FMUseAcccurateScreens def
currentdict end sethalftone
} bind } ifelse
def
/setDefaultScreen {
FMPColor {
orgrxfer cvx orggxfer cvx orgbxfer cvx orgxfer cvx setcolortransfer
}
{
orgxfer cvx settransfer
} ifelse
orgfreq organgle orgproc cvx setscreen
} bind def
/setCurrentScreen {
FrameSepIs FMnone eq {
FMUseDefaultNoSeparationScreen {
setDefaultScreen
} {
getCompositeScreen FMSetScreen
} ifelse
} {
FrameSepIs FMcustom eq {
FMUseDefaultSpotSeparationScreen {
setDefaultScreen
} {
getSpotScreen FMSetScreen
} ifelse
} {
FMUseDefaultProcessSeparationScreen {
setDefaultScreen
} {
FrameSepIs FMcyan eq {
getCyanScreen FMSetScreen
} {
FrameSepIs FMmagenta eq {
getMagentaScreen FMSetScreen
} {
FrameSepIs FMyellow eq {
getYellowScreen FMSetScreen
} {
getBlackScreen FMSetScreen
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} bind def
end
/gstring FMLOCAL
/gfile FMLOCAL
/gindex FMLOCAL
/orgrxfer FMLOCAL
/orggxfer FMLOCAL
/orgbxfer FMLOCAL
/orgxfer FMLOCAL
/orgproc FMLOCAL
/orgrproc FMLOCAL
/orggproc FMLOCAL
/orgbproc FMLOCAL
/organgle FMLOCAL
/orgrangle FMLOCAL
/orggangle FMLOCAL
/orgbangle FMLOCAL
/orgfreq FMLOCAL
/orgrfreq FMLOCAL
/orggfreq FMLOCAL
/orgbfreq FMLOCAL
/yscale FMLOCAL
/xscale FMLOCAL
/edown FMLOCAL
/manualfeed FMLOCAL
/paperheight FMLOCAL
/paperwidth FMLOCAL
/FMDOCUMENT {
array /FMfonts exch def
/#copies exch def
FrameDict begin
0 ne /manualfeed exch def
/paperheight exch def
/paperwidth exch def
0 ne /FrameNegative exch def
0 ne /edown exch def
/yscale exch def
/xscale exch def
FMLevel1 {
manualfeed {setmanualfeed} if
/FMdicttop countdictstack 1 add def
/FMoptop count def
% setpapername
% manualfeed {true} {papersize} ifelse
% {manualpapersize} {false} ifelse
% {desperatepapersize} {false} ifelse
% { (Can't select requested paper size for Frame print job!) FMFAILURE } if
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
}
{{1 dict dup /PageSize [paperwidth paperheight]put setpagedevice}stopped
{ (Can't select requested paper size for Frame print job!) FMFAILURE } if
{1 dict dup /ManualFeed manualfeed put setpagedevice } stopped pop }
ifelse

FMPColor {
currentcolorscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def
cvlit /orgbproc exch def
/orgbangle exch def
/orgbfreq exch def
cvlit /orggproc exch def
/orggangle exch def
/orggfreq exch def
cvlit /orgrproc exch def
/orgrangle exch def
/orgrfreq exch def
currentcolortransfer
FrameNegative {
1 1 4 {
pop { 1 exch sub } concatprocs 4 1 roll
} for
4 copy
setcolortransfer
} if
cvlit /orgxfer exch def
cvlit /orgbxfer exch def
cvlit /orggxfer exch def
cvlit /orgrxfer exch def
} {
currentscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def

currenttransfer
FrameNegative {
{ 1 exch sub } concatprocs
dup settransfer
} if
cvlit /orgxfer exch def
} ifelse
end
} def
/pagesave FMLOCAL
/orgmatrix FMLOCAL
/landscape FMLOCAL
/pwid FMLOCAL
/FMBEGINPAGE {
FrameDict begin
/pagesave save def
3.86 setmiterlimit
/landscape exch 0 ne def
landscape {
90 rotate 0 exch dup /pwid exch def neg translate pop
}{
pop /pwid exch def
} ifelse
edown { [-1 0 0 1 pwid 0] concat } if
0 0 moveto paperwidth 0 lineto paperwidth paperheight lineto
0 paperheight lineto 0 0 lineto 1 setgray fill
xscale yscale scale
/orgmatrix matrix def
gsave
} def
/FMENDPAGE {
grestore
pagesave restore
end
showpage
} def
/FMFONTDEFINE {
FrameDict begin
findfont
ReEncode
1 index exch
definefont
FMfonts 3 1 roll
put
end
} def
/FMFILLS {
FrameDict begin dup
array /fillvals exch def
dict /patCache exch def
end
} def
/FMFILL {
FrameDict begin
fillvals 3 1 roll put
end
} def
/FMNORMALIZEGRAPHICS {
newpath
0.0 0.0 moveto
1 setlinewidth
0 setlinecap
0 0 0 sethsbcolor
0 setgray
} bind def
/fx FMLOCAL
/fy FMLOCAL
/fh FMLOCAL
/fw FMLOCAL
/llx FMLOCAL
/lly FMLOCAL
/urx FMLOCAL
/ury FMLOCAL
/FMBEGINEPSF {
end
/FMEPSF save def
/showpage {} def
% See Adobe's "PostScript Language Reference Manual, 2nd Edition", page 714.
% "...the following operators MUST NOT be used in an EPS file:" (emphasis ours)
/banddevice {(banddevice) FMBADEPSF} def
/clear {(clear) FMBADEPSF} def
/cleardictstack {(cleardictstack) FMBADEPSF} def
/copypage {(copypage) FMBADEPSF} def
/erasepage {(erasepage) FMBADEPSF} def
/exitserver {(exitserver) FMBADEPSF} def
/framedevice {(framedevice) FMBADEPSF} def
/grestoreall {(grestoreall) FMBADEPSF} def
/initclip {(initclip) FMBADEPSF} def
/initgraphics {(initgraphics) FMBADEPSF} def
/initmatrix {(initmatrix) FMBADEPSF} def
/quit {(quit) FMBADEPSF} def
/renderbands {(renderbands) FMBADEPSF} def
/setglobal {(setglobal) FMBADEPSF} def
/setpagedevice {(setpagedevice) FMBADEPSF} def
/setshared {(setshared) FMBADEPSF} def
/startjob {(startjob) FMBADEPSF} def
/lettertray {(lettertray) FMBADEPSF} def
/letter {(letter) FMBADEPSF} def
/lettersmall {(lettersmall) FMBADEPSF} def
/11x17tray {(11x17tray) FMBADEPSF} def
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} bind def
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scale
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sl lb lt {lb ms} if
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r
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ws 0 lb getinterval is copy pop
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w h d [w 0 0 h neg 0 h]
{ip} image
bitmapsave restore
grestore
} bind def
/BEGINBITMAPBW {
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} bind def
/BEGINBITMAPGRAY {
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/BEGINBITMAP2BIT {
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} bind def
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gsave

3 index 2 div add exch
4 index 2 div add exch
translate
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1 index 2 div neg
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translate
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r
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w h d [w 0 0 h neg 0 h]
{cf is readhexstring pop} image
bitmapsave restore
grestore
} bind def
/ngrayt 256 array def
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/nbluet 256 array def
/ngreent 256 array def
/gryt FMLOCAL
/blut FMLOCAL
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/redt FMLOCAL
/indx FMLOCAL
/cynu FMLOCAL
/magu FMLOCAL
/yelu FMLOCAL
/k FMLOCAL
/u FMLOCAL
FMLevel1 {
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currentcolortransfer
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0 1 255 {
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/k cynu magu min yelu min def
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% /u 0 def
nredt indx 1 0 cynu u sub max sub redt exec put
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nbluet indx 1 0 yelu u sub max sub blut exec put
ngrayt indx 1 k currentblackgeneration exec sub gryt exec put
} for
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{255 mul cvi ngreent exch get}
{255 mul cvi nbluet exch get}
{255 mul cvi ngrayt exch get}
setcolortransfer
{pop 0} setundercolorremoval
{} setblackgeneration
} bind def
}
{
/colorSetup2 {
[ /Indexed /DeviceRGB 255
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exch dup green exch get 255 div
exch blue exch get 255 div}
] setcolorspace
} bind def
} ifelse
/tran FMLOCAL
/fakecolorsetup {
/tran 256 string def
0 1 255 {/indx exch def
tran indx
red indx get 77 mul
green indx get 151 mul
blue indx get 28 mul
add add 256 idiv put} for
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{255 mul cvi tran exch get 255.0 div}
exch concatprocs settransfer
} bind def
/BITMAPCOLOR {
/d 8 def
gsave

3 index 2 div add exch
4 index 2 div add exch
translate
rotate
1 index 2 div neg
1 index 2 div neg
translate
scale
/h exch def /w exch def
/bitmapsave save def
FMLevel1 {
colorsetup
/is w d wbytes string def
/cf currentfile def
w h d [w 0 0 h neg 0 h]
{cf is readhexstring pop} {is} {is} true 3 colorimage
} {
colorSetup2
/is w d wbytes string def
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7 dict dup begin
/ImageType 1 def
/Width w def
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/ImageMatrix [w 0 0 h neg 0 h] def
/DataSource {cf is readhexstring pop} bind def
/BitsPerComponent d def
/Decode [0 255] def
end image
} ifelse
bitmapsave restore
grestore
} bind def
/BITMAPCOLORc {
/d 8 def
gsave

3 index 2 div add exch
4 index 2 div add exch
translate
rotate
1 index 2 div neg
1 index 2 div neg
translate
scale
/h exch def /w exch def
/lb w d wbytes def
sl lb lt {lb ms} if
/bitmapsave save def
FMLevel1 {
colorsetup
/is im 0 lb getinterval def
ws 0 lb getinterval is copy pop
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w h d [w 0 0 h neg 0 h]
{ip} {is} {is} true 3 colorimage
} {
colorSetup2
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ws 0 lb getinterval is copy pop
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7 dict dup begin
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/Width w def
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/DataSource {ip} bind def
/BitsPerComponent d def
/Decode [0 255] def
end image
} ifelse
bitmapsave restore
grestore
} bind def
/BITMAPTRUECOLORc {
/d 24 def
gsave

3 index 2 div add exch
4 index 2 div add exch
translate
rotate
1 index 2 div neg
1 index 2 div neg
translate
scale
/h exch def /w exch def
/lb w d wbytes def
sl lb lt {lb ms} if
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/is im 0 lb getinterval def
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ws 0 lb getinterval is copy pop
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w h 8 [w 0 0 h neg 0 h]
{w rip pop ris} {gis} {bis} true 3 colorimage
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%%EndProlog
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0 Z
0 X
0 0 0 1 0 0 0 K
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72 445.03 558 445.03 2 L
2 Z
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72 74.02 558 74.02 2 L
0.25 H
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0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (67) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
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72 74.02 558 74.02 2 L
0.25 H
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 445.03 558 445.03 2 L
2 Z
N
72 74.02 558 74.02 2 L
0.25 H
N
1 12 Q
1.2 (Chapter 7) 72 677 S
2 24 Q
-0.48 (T) 207 677 S
-0.48 (ar) 218.52 677 S
-0.48 (get Acquisition) 237.12 677 S
-0.48 (Refer) 207 647 S
-0.48 (ence Information) 254.86 647 S
3 12 Q
(7.1) 144 415 T
( Predicting T) 164.02 415 T
(arget Acquisition Count Rates for Stars) 230.04 415 T
4 F
( 68) 505.32 415 T
3 10 Q
(7.1.1) 162 398.33 T
( Alternate Method for Predicting T) 187.02 398.33 T
(arget Acquisition Count Rates) 335.42 398.33 T
4 F
( 69) 508.1 398.33 T
3 F
(7.1.2) 162 382.33 T
( T) 187.02 382.33 T
(wo Examples) 195.36 382.33 T
4 F
( 69) 508.1 382.33 T
3 12 Q
(7.2) 144 365 T
( Constraints on the V) 164.02 365 T
(alue of the STEP-TIME Parameter) 275.18 365 T
4 F
( 71) 505.32 365 T
3 F
(7.3) 144 347 T
( Acquisition Count Rates for Extended Objects) 164.02 347 T
4 F
( 76) 505.32 347 T
3 F
(7.4) 144 329 T
( Other Acquisition Information) 164.02 329 T
4 F
( 78) 505.32 329 T
3 10 Q
(7.4.1) 162 312.33 T
( Ef) 187.02 312.33 T
(fective Areas of the Acquisition Mirrors) 199.07 312.33 T
4 F
( 78) 508.1 312.33 T
3 F
(7.4.2) 162 296.33 T
( Geocoronal L) 187.02 296.33 T
(yman-a Background) 249.46 296.33 T
4 F
( 80) 508.1 296.33 T
FMENDPAGE
%%EndPage: "67" 1
%%Page: "68" 2
612 792 0 FMBEGINPAGE
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7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(T) 189 736.18 T
(arget Acquisition Reference Information) 193.83 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(68) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
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54 671.02 540 674.02 C
0 0 0 1 0 0 0 K
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189 672.52 540 672.52 2 L
0.25 H
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0 X
0 0 0 1 0 0 0 K
N
54 672.52 180 672.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(7.1) 163.32 678.02 T
(Predicting T) 189 678.02 T
(arget Acquisition Count Rates for Stars) 257.46 678.02 T
5 10 Q
0.78 (W) 189 650.35 P
0.78 (e have calculated GHRS tar) 197.64 650.35 P
0.78 (get acquisition count rates for the spectra of a subset of) 311.67 650.35 P
0.1 (the 175 stars contained in the Bruzual-Persson-Gunn-Stryker \050BPGS\051 Library of Stellar) 189 638.35 P
1.56 (Spectra by using) 189 626.35 P
3 F
1.74 (calcphot) 262.85 626.35 P
5 F
1.56 (, a task in the) 300.09 626.35 P
3 F
1.74 (synphot) 363.46 626.35 P
5 F
1.56 ( package in) 398.48 626.35 P
3 F
1.74 (stsdas) 451.21 626.35 P
5 F
1.56 (. GHRS tar) 480.11 626.35 P
1.56 (get) 527.78 626.35 P
-0 (acquisition count rates for objects similar to those in the BPGS catalog can be predicted) 189 614.35 P
0.79 (by following the procedures described here. Constraints on the value of) 189 602.35 P
6 F
1.9 (STEP-TIME) 486 602.35 P
5 F
-0.05 (are discussed. Please note that the values tabulated are the total count rate for a star) 189 590.35 P
-0.05 (, and) 520.61 590.35 P
0.14 (that the count rate for a particular diode will depend on that portion of the Point Spread) 189 578.35 P
0.02 (Function that strikes it. That can in\337uence the degree, for example, to which the paired-) 189 566.35 P
0.66 (pulse correction applies. However) 189 554.35 P
0.66 (, the acquisition procedure sums the counts over the) 327.22 554.35 P
0.85 (eight science diodes upon which the LSA is imaged, so for most objects these values) 189 542.35 P
(may be used straightforwardly) 189 530.35 T
(.) 310.27 530.35 T
-0.04 (Do not for) 189 506.35 P
-0.04 (get to reduce these values by a factor of 0.3 if the focus diodes are being used) 230.4 506.35 P
-0.11 (for an) 189 494.35 P
6 F
-0.25 (IMAGE) 214.89 494.35 P
5 F
-0.11 (; this is because of the reduced area of the focus diodes compared to using) 244.89 494.35 P
0.03 (eight normal diodes for an acquisition. This factor applies to when a focus diode is cen-) 189 482.35 P
(tered on a point source.) 189 470.35 T
0.64 (The \337ux distributions in the BPGS catalog include ultraviolet wavelengths and can be) 189 446.35 P
0.82 (used for planning GHRS tar) 189 434.35 P
0.82 (get acquisitions. Each spectrum in the catalog was dered-) 304.31 434.35 P
-0.02 (dened and scaled to) 189 422.35 P
7 F
-0.02 (V) 270.02 422.35 P
5 8 Q
-0.01 (0) 276.12 419.85 P
5 10 Q
-0.02 ( = 0.0. The) 280.12 422.35 P
3 F
-0.02 (calcphot) 326.24 422.35 P
5 F
-0.02 ( task in the) 363.48 422.35 P
3 F
-0.02 (synphot) 409.52 422.35 P
5 F
-0.02 ( package of) 444.54 422.35 P
3 F
-0.02 (stsdas) 493.07 422.35 P
5 F
-0.02 ( was) 521.97 422.35 P
-0.05 (used to convolve the catalog \337ux distributions with the ef) 189 410.35 P
-0.05 (fective areas of the acquisition) 418.03 410.35 P
0.44 (mirrors. T) 189 398.35 P
0.44 (able) 229.29 398.35 P
0.44 (7-1 on page) 248.45 398.35 P
0.44 (74 contains columns giving the BPGS catalog object name,) 299.03 398.35 P
0.16 (spectral type,) 189 386.35 P
7 F
0.16 (\050B\320V\051) 245.14 386.35 P
5 8 Q
0.13 (0) 269.02 383.85 P
5 10 Q
0.16 (, count rate for the acquisition mirror with no reddening, and scale) 273.02 386.35 P
-0.19 (factors \050per unit magnitude\051 indicating the relative count rate observed at given amounts) 189 374.35 P
(of reddening compared to the count rate with no reddening.) 189 362.35 T
(T) 189 338.35 T
(o use T) 194.41 338.35 T
(able) 223.15 338.35 T
(7-1 to predict tar) 242.31 338.35 T
(get acquisition count rates:) 309.06 338.35 T
8 11 Q
(\245) 189 320.35 T
5 10 Q
0.1 (Determine the) 203.4 320.35 P
7 F
0.1 (intrinsic) 263.04 320.35 P
5 F
0.1 ( color) 296.38 320.35 P
0.1 (,) 319.13 320.35 P
7 F
0.1 (\050B \320 V\051) 324.23 320.35 P
5 8 Q
0.08 (0) 353.32 317.85 P
5 10 Q
0.1 (, and magnitude,) 357.32 320.35 P
7 F
0.1 (V) 426.79 320.35 P
5 8 Q
0.08 (0) 432.9 317.85 P
5 10 Q
0.1 (, of your object as well as) 436.9 320.35 P
(its color excess,) 203.4 308.35 T
7 F
( E\050B \320 V\051) 267 308.35 T
5 F
(.) 304.49 308.35 T
8 11 Q
(\245) 189 293.35 T
5 10 Q
0.14 (Find an entry in T) 203.4 293.35 P
0.14 (able) 275.47 293.35 P
0.14 (7-1 that has similar spectral characteristics to your object \050by) 294.63 293.35 P
0.53 (spectral type or) 203.4 281.35 P
7 F
0.53 (\050B \320 V\051) 269.13 281.35 P
5 8 Q
0.42 (0) 299.07 278.85 P
5 10 Q
0.53 ( and note that luminosity class is important for the coolest) 303.07 281.35 P
0.38 (stars\051. The table is sorted by increasing) 203.4 269.35 P
7 F
0.38 (\050B \320 V\051) 364.89 269.35 P
5 8 Q
0.3 (0) 394.52 266.85 P
5 10 Q
0.38 (. Make sure you pick from the col-) 398.52 269.35 P
(umn corresponding to the acquisition mirror that you plan to use.) 203.4 257.35 T
8 11 Q
(\245) 189 241.68 T
5 10 Q
1.15 (Scale the predicted count rate found in the previous step by the ratio of apparent) 203.4 241.68 P
(brightness of your object to an object with) 203.4 222.17 T
7 F
(V) 375.05 222.17 T
5 8 Q
(0) 381.16 219.67 T
5 10 Q
( = 0.0, i.e., multiply by) 385.16 222.17 T
(.) 512.9 222.17 T
8 11 Q
(\245) 189 205.33 T
5 10 Q
-0.01 (T) 203.4 205.33 P
-0.01 (o obtain the scale factor by which the unreddened count rate will be reduced for an) 208.81 205.33 P
1.23 (amount of reddening appropriate to your object, multiply the count rate from the) 203.4 193.33 P
(previous step by this factor:) 203.4 181.33 T
8 11 Q
(\245) 189 166.33 T
5 10 Q
0.42 (The GHRS detectors are nonlinear at high count rates: this phenomenon is referred) 203.4 166.33 P
1.42 (to as the \322dead-time\323 or \322paired-pulse\323 ef) 203.4 154.33 P
1.42 (fect. Consequently) 378.34 154.33 P
1.42 (, the predicted count) 454.1 154.33 P
-0.09 (rate from the previous step must be reduced to yield the actual count rate that GHRS) 203.4 142.33 P
0.07 (will measure. Multiply the count rate you just determined by the \322fraction detected\323) 203.4 130.33 P
(value determined from Figure) 203.4 118.33 T
(2 on page) 325.6 118.33 T
(71 to obtain the \336nal predicted count rate.) 366.98 118.33 T
8 11 Q
(\245) 189 103.33 T
5 10 Q
0.29 (This \336nal value is probably reliable to within a factor of two, which is adequate for) 203.4 103.33 P
(acquisition purposes in almost all instances.) 203.4 91.33 T
479.42 217.67 512.9 236.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 480.42 222.17 T
(0) 485.42 222.17 T
5 7 Q
(0) 494.57 229.77 T
(.) 498.07 229.77 T
(4) 499.82 229.77 T
7 F
(V) 503.85 229.77 T
5 5 Q
(0) 508.4 227.52 T
5 7 Q
(\320) 490.8 229.77 T
0 0 612 792 C
317 176.84 398.14 193.43 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 318 181.33 T
(0) 323 181.33 T
5 7 Q
(s) 328.38 187.18 T
(c) 331.1 187.18 T
(a) 334.21 187.18 T
(l) 337.32 187.18 T
(e) 339.27 187.18 T
(f) 344.12 187.18 T
(a) 346.45 187.18 T
(c) 349.56 187.18 T
(t) 352.67 187.18 T
(o) 354.62 187.18 T
(r) 358.12 187.18 T
7 F
(E) 367.78 187.18 T
(B) 376.77 187.18 T
(V) 388.04 187.18 T
5 F
(\320) 382.79 187.18 T
9 F
(\050) 373.77 187.18 T
(\051) 392.64 187.18 T
(\264) 362.19 187.18 T
0 0 612 792 C
FMENDPAGE
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7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (69) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(T) 207 736.18 T
(arget Acquisition Reference Information) 211.83 736.18 T
0 10 Q
(7.1.1) 175.76 679.35 T
(Alternate Method for Predicting T) 207 679.35 T
(arget Acquisition Count Rates) 364.61 679.35 T
5 F
1.47 (Figure) 207 655.35 P
1.47 (7-1 on page) 235.61 655.35 P
1.47 (70 shows mean predicted count rates as a function of) 288.25 655.35 P
-0.23 (color for the four acquisition mirrors. Also shown are the \336ts to the predicted count rates) 207 643.35 P
0.28 (for various amounts of reddening. The label for each curve represents the color excess,) 207 631.35 P
7 F
(E\050B \320 V\051) 207 619.35 T
5 F
(, applied to the spectra.) 241.99 619.35 T
(Y) 207 595.35 T
(ou can estimate tar) 213.22 595.35 T
(get acquisition count rates using the plots instead of T) 288.3 595.35 T
(able) 503.42 595.35 T
(7-1:) 522.58 595.35 T
8 11 Q
(\245) 207 577.35 T
5 10 Q
1.9 (Determine the intrinsic color and magnitude of your object as well as its color) 221.4 577.35 P
(excess.) 221.4 565.35 T
8 11 Q
(\245) 207 550.35 T
5 10 Q
(Read from the Figures \050depending on the mirror used\051 the predicted count rate.) 221.4 550.35 T
8 11 Q
(\245) 207 535.35 T
5 10 Q
-0.13 (Scale the predicted count rate by the ratio of apparent brightness of your object to an) 221.4 535.35 P
(object with zero magnitude.) 221.4 523.35 T
8 11 Q
(\245) 207 508.35 T
5 10 Q
(Use Figure) 221.4 508.35 T
(2 on page) 268.06 508.35 T
(71 to correct for the \322paired-pulse\323 ef) 309.44 508.35 T
(fect.) 459.76 508.35 T
0 F
(7.1.2) 175.76 478.35 T
(T) 207 478.35 T
(wo Examples) 212.37 478.35 T
5 F
(First, suppose you want to observe) 207 454.35 T
9 F
(m) 348.38 454.35 T
5 F
( Col, which has the following properties:) 354.14 454.35 T
-0.12 (Using the table, you would see that HR 8023, an O6 star with) 207 388.35 P
-0.12 ( is the) 534.35 388.35 P
0.09 (closest match, giving a predicted count rate for the A2 mirror of 1.3) 207 376.35 P
0.09 (x) 481.66 376.35 P
0.09 (10) 489.16 376.35 P
5 8 Q
0.07 (7) 499.16 380.35 P
5 10 Q
0.09 (counts s) 503.16 376.35 P
5 8 Q
0.07 (\3201) 535.75 380.35 P
5 10 Q
0.09 ( for) 543.75 376.35 P
0.29 (a) 207 364.35 P
7 F
0.29 (V) 214.24 364.35 P
5 8 Q
0.24 (0) 220.35 361.85 P
5 10 Q
0.29 (= 0 star) 227.14 364.35 P
0.29 (. Multiplying this count rate by 10) 257.26 364.35 P
5 8 Q
0.24 (-0.4) 395.98 368.35 P
9 F
0.24 (\264) 408.64 368.35 P
5 F
0.24 (5.13) 413.04 368.35 P
5 10 Q
0.29 (gives 1.2) 429.27 364.35 P
0.29 (x) 468.17 364.35 P
0.29 (10) 475.67 364.35 P
5 8 Q
0.24 (5) 485.67 368.35 P
5 10 Q
0.29 ( counts s) 489.67 364.35 P
5 8 Q
0.24 (\3201) 525.27 368.35 P
5 10 Q
0.29 (. Red-) 533.27 364.35 P
-0.24 (dening will decrease the counts slightly; calculation of the scale factor indicates that you) 207 352.35 P
0.14 (should multiply by 0.93, giving a new count rate of 1.1) 207 340.35 P
0.14 (x) 431.22 340.35 P
0.14 (10) 438.72 340.35 P
5 8 Q
0.12 (5) 448.72 344.35 P
5 10 Q
0.14 ( counts s) 452.72 340.35 P
5 8 Q
0.12 (-1) 488.01 344.35 P
5 10 Q
0.14 (. The dead-time) 494.67 340.35 P
-0.06 (correction factor estimates that only 83% of those counts will be detected, so one would) 207 328.35 P
0.22 (expect approximately 94000 counts s) 207 316.35 P
5 8 Q
0.17 (-1) 356.74 320.35 P
5 10 Q
0.22 (with this star) 365.58 316.35 P
0.22 (. In fact, when) 417.14 316.35 P
9 F
0.22 (m) 477.99 316.35 P
5 F
0.22 ( Col was observed) 483.75 316.35 P
0.09 (early in Cycle) 207 304.35 P
0.09 (4, 19,600 counts were obtained in 0.2) 265.78 304.35 P
0.09 (seconds with the A2 mirror) 419.08 304.35 P
0.09 (, which) 528.47 304.35 P
(works out to 98,000) 207 292.35 T
(counts s) 289.5 292.35 T
5 8 Q
(-1) 322 296.35 T
5 10 Q
(, which is within 5% of the calculated value.) 328.66 292.35 T
(Second, consider a very red star such as Aldebaran:) 207 268.35 T
0.39 (Using the table, you would see that BD\3201) 207 202.35 P
5 8 Q
0.31 (o) 376.95 206.35 P
5 10 Q
0.39 (31) 380.95 202.35 P
0.39 (13 has a similar spectral type \050K5III\051 and) 390.58 202.35 P
0.52 (color \0501.61\051. The calculated count rate for mirror A2 is then) 207 190.35 P
0.52 ( counts per sec-) 493.95 190.35 P
0.02 (ond. The adjustment for apparent magnitude is) 207 178.35 P
0.02 (, which yields a count rate of) 442.06 178.35 P
0.14 (530 per second, or 210 in 0.2 seconds. Early in Cycle 4 a T) 207 166.35 P
0.14 (au was acquired with mirror) 444.7 166.35 P
(A2 and the count rate seen was 246 in 0.2 seconds, within 15% of the predicted value.) 207 154.35 T
0 8 Q
(Name) 214.11 432.68 T
(Sp. T) 279.51 432.68 T
(ype.) 298.48 432.68 T
10 F
(V) 366.33 432.68 T
(B \320 V) 431 432.68 T
(E\050B \320 V\051) 497.66 432.68 T
9 10 Q
(m) 202.5 416.02 T
5 9 Q
( Columbae) 208.26 416.02 T
(O9V) 288.25 416.02 T
(5.16) 361.12 416.02 T
(\3200.29) 430.88 416.02 T
(0.01) 505.12 416.02 T
0 8 Q
(Name) 214.11 246.68 T
(Sp. T) 279.51 246.68 T
(ype.) 298.48 246.68 T
10 F
(V) 366.33 246.68 T
(B \320 V) 431 246.68 T
(E\050B \320 V\051) 497.66 246.68 T
9 10 Q
(a) 211.16 230.02 T
5 9 Q
(T) 219.97 230.02 T
(auri) 224.84 230.02 T
(K5III) 287.01 230.02 T
(0.84) 361.12 230.02 T
(1.54) 433.12 230.02 T
(0.00) 505.12 230.02 T
189 444.89 189 409.14 2 L
V
0 Z
N
261 445.14 261 408.89 2 L
V
N
333 445.14 333 408.89 2 L
V
N
405 445.14 405 408.89 2 L
V
N
477 445.14 477 408.89 2 L
V
N
549 444.89 549 409.14 2 L
V
N
188.88 445.02 549.12 445.02 2 L
V
N
188.88 426.02 549.12 426.02 2 L
V
0.5 H
N
188.88 409.02 549.12 409.02 2 L
V
0.25 H
N
189 258.89 189 223.14 2 L
V
N
261 259.14 261 222.89 2 L
V
N
333 259.14 333 222.89 2 L
V
N
405 259.14 405 222.89 2 L
V
N
477 259.14 477 222.89 2 L
V
N
549 258.89 549 223.14 2 L
V
N
188.88 259.02 549.12 259.02 2 L
V
N
188.88 240.02 549.12 240.02 2 L
V
0.5 H
N
188.88 223.02 549.12 223.02 2 L
V
0.25 H
N
517.3 648.5 558 663.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
7 10 Q
0 X
0 0 0 1 0 0 0 K
(B) 524.35 655.35 T
(V) 540.46 655.35 T
5 F
(\320) 532.96 655.35 T
9 F
(\050) 520.06 655.35 T
(\051) 547.03 655.35 T
5 7 Q
(0) 552.41 652.25 T
0 0 612 792 C
454.02 383.85 534.35 396.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
7 10 Q
0 X
0 0 0 1 0 0 0 K
(B) 461.07 388.35 T
(V) 477.18 388.35 T
5 F
(\320) 469.68 388.35 T
9 F
(\050) 456.78 388.35 T
(\051) 483.75 388.35 T
5 F
(0) 509.76 388.35 T
(.) 514.76 388.35 T
(3) 517.26 388.35 T
(1) 522.26 388.35 T
(3) 527.26 388.35 T
(\320) 504.38 388.35 T
(=) 493.74 388.35 T
0 0 612 792 C
454.08 185.85 493.95 202.45 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 455.08 190.35 T
(.) 460.08 190.35 T
(6) 462.58 190.35 T
(1) 478.07 190.35 T
(0) 483.07 190.35 T
5 7 Q
(3) 488.45 196.2 T
9 10 Q
(\264) 470.08 190.35 T
0 0 612 792 C
396.58 173.85 442.06 190.45 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 397.58 178.35 T
(0) 402.58 178.35 T
5 7 Q
(0) 411.72 184.2 T
(.) 415.22 184.2 T
(4) 416.97 184.2 T
(0) 427.81 184.2 T
(.) 431.31 184.2 T
(8) 433.06 184.2 T
(4) 436.56 184.2 T
9 F
(\264) 422.22 184.2 T
5 F
(\320) 407.95 184.2 T
0 0 612 792 C
FMENDPAGE
%%EndPage: "69" 3
%%Page: "70" 4
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(T) 189 736.18 T
(arget Acquisition Reference Information) 193.83 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(70) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
63 90 540 711 R
0.01 (Figure 7-1.) 0 -270 517.67 162 PF
3 F
0.01 (Mean target acquisition count rates for stars with the four mirrors of the GHRS. The numbers at) 0 -270 517.67 218.15 PF
(the right indicate the appropriate) 0 -270 529.67 162 TF
4 F
( E\050B \320 V\051) 0 -270 529.67 305.41 TF
3 F
( for each curve.) 0 -270 529.67 345.98 TF
63 90 540 711 R
63 90 540 711 C
70 90 502 711 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 43 29 576 727 213.2 279.2 283.7 425.3 FMBEGINEPSF
%%BeginDocument: /pongo/data2/drs/ghrs/handbook/ih5/figs/mirror_a2.epsi
%!PS-Adobe-2.0 EPSF-1.2
%%BoundingBox: 43 29 576 727
%!PS-Adobe-1.0
%%Creator: PSIKern - An IRAF GKI Translator
%%CreationDate: Thu 15:21:12 28-Apr-94
%%DocumentFonts: (atend)
%%Pages: (atend)
%%BoundingBox: 28 28 583 763
%%EndComments
/MAXNDC 4095 def /PageSizeXMeter 0.2594 def /PageSizeYMeter 0.1959 def
/PageOffXMeter 0.01 def /PageOffYMeter 0.01 def
/PortraitMode false def /PortraitRotation 0. def
/LandScapeRotation 90. def /GT_LEFT 2 def /GT_RIGHT 3 def
/GT_TOP 6 def /GT_BOTTOM 7 def /GT_UP 4 def /GT_DOWN 5 def
/GT_CENTER 1 def /RF /Times-Roman def /GF /Symbol def
/IF /Times-Italic def /BF /Times-Bold def /DASH 49 def /DOT 4 def
/SPACE 24 def

% How to define things.
/BD { bind def } bind def
/LD { load def } bind def

% Constants
/yes true def
/no false def

% Define some shorthand instructions.
/GRS /grestore LD
/GS /gsave LD
/MK /mark LD
/R /restore LD
/S /save LD
/SH /showpage LD
/SW /setlinewidth LD

% Measurement conversions.
/PointperMeter 2834.64 def
/MonoScale .7 def

% SR: Set current path to page: - -> -
/SR { currentpoint stroke moveto } BD

% CL: CLear the page: - -> -
/CL { restore showpage grestore gsave save } BD

% RC: Read Coordinates: string -> x y
/RC {
currentfile read pop 8#77 and 6 bitshift
currentfile read pop 8#77 and or
currentfile read pop 8#77 and 6 bitshift
currentfile read pop 8#77 and or
} BD

% DO - Determine Offset: length -> offset
/DO { DS dup 0 eq { pop pop 0 } { mod } ifelse } BD

% M: Move: M string -> -
% Move to a point and clear length of path.
/M { RC moveto CT OF setdash } BD

% D: Draw: D string -> -
% This also calculates the length of the current path.
/OF 0 def
/D { RC DS 0 ne { 2 copy currentpoint exch 4 1 roll sub dup mul 3 1 roll
sub dup mul add sqrt round OF add cvi DO /OF exch store } if lineto
} BD

% Character/Font definitions.

% FS -- Define the current font size: xsize ysize FS -
/FontXSize 0 def /FontYSize 0 def /NewFont true def
/FS { /FontYSize exch MonoScale mul store /FontXSize exch MonoScale mul store
/NewFont true store } BD

% PH -- Set the current path: path PH -
/Path 0 def
/PH { /Path exch store } BD

% PA -- Set the path angle of the text: angle PA -
/Angle 0 def
/PA { 360 mod dup 0 lt { 360 add } if /Angle exch store /NewFont true store } BD

% HJ, VJ -- Set Horizontal/Verticle Justification: just HJ/VJ -
/HorzJust 0 def /VertJust 0 def
/HJ { /HorzJust exch store } BD /VJ { /VertJust exch store } BD

% VT -- Use mono- or variable-spaced fonts: flag VT -
/VT true def
/VT { /Variable exch store } BD

% SetFont -- Make the required font the default: font SetFont -
% Note scale factor- This is to fill out monospaced better and match other
% IRAF output.
/Font () def
/FontMatrix matrix def
/SetFont {
dup Font ne NewFont or
{ dup /Font exch store findfont
Angle matrix rotate FontXSize MonoScale div FontYSize MonoScale div
matrix scale matrix concatmatrix makefont setfont Angle matrix rotate
FontXSize FontYSize matrix scale matrix concatmatrix /FontMatrix exch
store
}
{ pop } ifelse /NewFont false store
} BD

% StringWidth -- Determine path length of string: string StringWidth - xs ys
/StringWidth { Path GT_RIGHT eq Variable and { stringwidth }
{ Path GT_RIGHT eq { length } { pop 1 } ifelse 0 FontMatrix transform }
ifelse
} BD

% MonoShow -- Write the string out in mono-spaced: string MonoShow -
/MonoShow {
/t 1 string def 1 0 FontMatrix transform
/dy exch def /dx exch def Path GT_RIGHT eq { /mx dx def /my dy def }
{ 0 1 FontMatrix transform /my exch def /mx exch def } ifelse
{ t 0 3 -1 roll put t dup stringwidth dy exch sub 2 div exch dx exch
sub 2 div exch gsave rmoveto show grestore mx my rmoveto
} forall
} BD

% WS -- Draw the string: string font string ... DS -
/*WSDict 13 dict def
/WS { *WSDict begin
counttomark 2 idiv dup dup array /FontArray exch def
array /StringArray exch def 1 sub /NStrings exch def

NStrings -1 0 {
dup 4 1 roll exch StringArray 3 1 roll put FontArray 3 1 roll put
} for
pop

/XSize 0 def /YSize 0 def /NChars 0 def
0 1 NStrings {
dup FontArray exch get SetFont StringArray exch get dup
length NChars add /NChars exch def StringWidth
YSize add /YSize exch def XSize add /XSize exch def
} for

/TAngle HorzJust GT_RIGHT eq
{ Angle 180 add dup 360 ge { 360 sub } if } { Angle } ifelse def
0 TAngle 180 le HorzJust GT_CENTER eq or
{ Angle sin FontYSize mul Path GT_UP eq { NChars mul } if add } if
TAngle 90 ge TAngle 270 le and HorzJust GT_CENTER eq or
{ Path GT_RIGHT eq { XSize } { Angle cos FontXSize mul } ifelse sub } if
HorzJust GT_CENTER eq { .5 mul } if

/TAngle
VertJust GT_TOP eq { Angle 180 sub dup 0 lt { 360 add } if } { Angle } ifelse
def
0 TAngle 90 ge TAngle 270 le and VertJust GT_CENTER eq or
{ Angle cos FontYSize mul Path GT_UP eq { NChars mul } if sub } if
TAngle 180 ge TAngle 360 le and VertJust GT_CENTER eq or
{ Path GT_RIGHT eq { YSize } { Angle sin FontXSize mul } ifelse sub } if
VertJust GT_CENTER eq { .5 mul } if
rmoveto

0 1 NStrings {
dup FontArray exch get SetFont StringArray exch get
Path GT_RIGHT eq Variable and { show } { MonoShow } ifelse
} for

end
} BD

% Define the DASHED, DOTTED, DOTDASH patterns.
/DS 0 def
/LPS {
/OF 0 store /DS 0 store 0 array
} BD
/LPD {
/OF 0 store DASH SPACE 2 copy add /DS exch store 2 array astore
} BD
/LPP {
/OF 0 store DOT SPACE 2 copy add /DS exch store 2 array astore
} BD
/LDD {
/OF 0 store DOT SPACE DASH SPACE 4 copy add add add /DS exch store
4 array astore
} BD

% LT - Set Line Type - array -> -
/CT { currentdash pop } BD
/LT { /CT exch store /OF 0 store } BD

% SC - Set Color: color -> -
/*SCDict 1 dict def
/SC { *SCDict begin
1 sub /color exch def
GR color get 255 div GG color get 255 div GB color get 255 div setrgbcolor
end
} BD

% MI - Make Image LUT: table-name size MI hexstring -> -
/MI { currentfile exch string readhexstring pop def } BD

% Define the graphics color lookup table.
/GR 16 MI 00FFFF0000FF00FFFFB0FFF0D940F0F5
/GG 16 MI 00FF00FF00FFFF0080D0A6E670E082DE
/GB 16 MI 00FF0000FF00FFFF4F61008CD6D1EFB3

% Render an image when no image LUT has been define.
/DefaultGrey {
{ currentfile inarr readhexstring pop } image
} BD

% ColorImage - Produce an image by indexing into the Image Lookup Table.
% There are two versions of this code- one for PostScript that has
% the colorimage operator and one that doesn't. If the PostScript doesn't
% have colorimage, it is assumed that it can only produce black & white,
% in which the Image LUT is combined to produce a single grey which is
% then used as the image for the image operator.
/colorimage where
{ pop
/ColorImage {
{ currentfile inarr readhexstring pop dup /inarr exch def
length 3 mul string /oarr exch def
0 1 inarr length 1 sub
{ /iindex exch def
/oindex iindex 3 mul def
oarr oindex IR inarr iindex get get put
oarr oindex 1 add IG inarr iindex get get put
oarr oindex 2 add IB inarr iindex get get put
} for
oarr
}
false 3 colorimage
} BD
}
{ /ColorImage {
{ currentfile inarr readhexstring pop dup /inarr exch def
length string /oarr exch def
0 1 inarr length 1 sub
{ /iindex exch def
oarr iindex
IR inarr iindex get get 0.3 mul
IG inarr iindex get get 0.59 mul
IB inarr iindex get get 0.11 mul
add add round cvi dup 255 gt { pop 255 } if
put
} for
oarr
}
image
} BD
}
ifelse

% PC: Put Cellarray: width height bitspersample matrix -> -
/*PCdict 10 dict def
/PC {
*PCdict begin
4 -1 roll dup /inarr exch string def 4 1 roll
/IR where {pop ColorImage} {DefaultGrey} ifelse
end
} BD

% Define the Hatch (fill area) styles. H1 and H2 are handled internally
% by PSIKern. Feel free to define more; there is no limit.
/H3 <8888888888888888> def
/H4 def
/H5 <8844221188442211> def
/H6 <1122448811224488> def

% Setup for fill patterns. This whole section of code is taken almost
% directly from _PostScript Language: Tutorial and Cookbook_, Adobe Systems,
% 1986 (the blue book).
/setuserscreendict 22 dict def
setuserscreendict begin
/tempctm matrix def
/temprot matrix def
/tempscale matrix def

/concatprocs
{ /proc2 exch cvlit def
/proc1 exch cvlit def
/newproc proc1 length proc2 length add
array def
newproc 0 proc1 putinterval
newproc proc1 length proc2 putinterval
newproc cvx
} def

/resmatrix matrix def
/findresolution
{ 72 0 resmatrix defaultmatrix dtransform
/yres exch def /xres exch def
xres dup mul yres dup mul add sqrt
} def
end

/setuserscreen
{ setuserscreendict begin
/spotfunction exch def
/screenangle exch def
/cellsize exch def

/m tempctm currentmatrix def
/rm screenangle temprot rotate def
/sm cellsize dup tempscale scale def

sm rm m m concatmatrix m concatmatrix pop
1 0 m dtransform /y1 exch def /x1 exch def

/veclength x1 dup mul y1 dup mul add sqrt def
/frequency findresolution veclength div def

/newscreenangle y1 x1 atan def

m 2 get m 1 get mul m 0 get m 3 get mul sub
0 gt
{ {neg} /spotfunction load concatprocs
/spotfunction exch def
} if

frequency newscreenangle /spotfunction load
setscreen
end
} def

/setpatterndict 18 dict def
setpatterndict begin
/bitison
{ /ybit exch def /xbit exch def
/bytevalue bstring ybit bwidth mul xbit 8 idiv
add get def

/mask 1 7 xbit 8 mod sub bitshift def
bytevalue mask and 0 ne
} def
end

/bitpatternspotfunction
{ setpatterndict begin
/y exch def /x exch def

/xindex x 1 add 2 div bpside mul cvi def
/yindex y 1 add 2 div bpside mul cvi def

xindex yindex bitison
{ /onbits onbits 1 add def 1 }
{ /offbits offbits 1 add def 0 }
ifelse
end
} def

/setpattern
{ setpatterndict begin
/cellsz exch def
/angle exch def
/bwidth exch def
/bpside exch def
/bstring exch def

/onbits 0 def /offbits 0 def
cellsz angle /bitpatternspotfunction load
setuserscreen
{ } settransfer
offbits offbits onbits add div setgray
end
} def

% SP: Set Pattern: pattern -> -
/SP { 8 1 0 MAXNDC 100 div setpattern } BD

% FI: Fill with Pattern: - -> -
/FI { fill grestore } BD

% Set the transformation matrix.
PointperMeter dup scale
PageOffXMeter
PortraitMode not
{ PageSizeYMeter add }
if
PageOffYMeter translate
PortraitMode
{ PortraitRotation rotate }
{ LandScapeRotation rotate}
ifelse
PageSizeXMeter MAXNDC div PageSizeYMeter MAXNDC div scale
1 setlinejoin 1 setlinecap

% Save the current graphics state (to restore after showpage) and the
% VM state to recover after a showpage.
GS S

%%EndProlog
%PSKOpenWorkStation
%%Page: 1 1
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M FYiq D Fyiq SR M FYjO D FyjO SR M FYji D Fyji SR M FYji D GYji SR
M FYmX D FymX SR M FYn~ D Fyn~ SR M FYpG D FypG SR M FYp? D Fyp? SR
M FYqm D Fyqm SR M FYrT D FyrT SR M FYru D Fyru SR M FYsS D FysS SR
M FYsm D Fysm SR M FYsm D GYsm SR M FYv\ D Fyv\ SR M FYxB D FyxB SR
M FYyK D FyyK SR M FYzC D FyzC SR M FYzq D Fyzq SR M FY{X D Fy{X SR
M FY{y D Fy{y SR M FY|W D Fy|W SR M FY|r D Fy|r SR M FY|r D GY|r SR
M ByFy D B?F} SR M B?F} D CHGI SR M CHGI D CHEu SR M CEGE D CEEu SR
M ByEu D CTEu SR M C?GI D CvGE SR M CvGE D CpFy SR M CpFy D ClFe SR
M ClFe D ClFY SR M ClFY D CpFE SR M CpFE D CvEy SR M CvEy D C?Eu SR
M C?Eu D DEEu SR M DEEu D DNEy SR M DNEy D DTFE SR M DTFE D DWFY SR
M DWFY D DWFe SR M DWFe D DTFy SR M DTFy D DNGE SR M DNGE D DEGI SR
M DEGI D C?GI SR M C?GI D CyGE SR M CyGE D CvGA SR M CvGA D CsFy SR
M CsFy D CpFe SR M CpFe D CpFY SR M CpFY D CsFE SR M CsFE D CvE} SR
M CvE} D CyEy SR M CyEy D C?Eu SR M DEEu D DKEy SR M DKEy D DNE} SR
M DNE} D DQFE SR M DQFE D DTFY SR M DTFY D DTFe SR M DTFe D DQFy SR
M DQFy D DNGA SR M DNGA D DKGE SR M DKGE D DEGI SR M EIGm D EJGj SR
M EJGj D EIGh SR M EIGh D EGGj SR M EGGj D EGGm SR M EGGm D EIGr SR
M EIGr D EJGt SR M EJGt D EPGw SR M EPGw D EWGw SR M EWGw D E]Gt SR
M E]Gt D E^Gr SR M E^Gr D E`Gm SR M E`Gm D E`Gh SR M E`Gh D E^Gc SR
M E^Gc D EYG^ SR M EYG^ D EPGZ SR M EPGZ D ELGW SR M ELGW D EIGR SR
M EIGR D EGGK SR M EGGK D EGGD SR M EWGw D E[Gt SR M E[Gt D E]Gr SR
M E]Gr D E^Gm SR M E^Gm D E^Gh SR M E^Gh D E]Gc SR M E]Gc D EWG^ SR
M EWG^ D EPGZ SR M EGGI D EIGK SR M EIGK D ELGK SR M ELGK D EUGF SR
M EUGF D E[GF SR M E[GF D E^GI SR M E^GI D E`GK SR M ELGK D EUGD SR
M EUGD D E]GD SR M E]GD D E^GF SR M E^GF D E`GK SR M E`GK D E`GP SR
M ByO} D B?PA SR M B?PA D CHPN SR M CHPN D CHNy SR M CEPI D CENy SR
M ByNy D CTNy SR M C?PN D CvPI SR M CvPI D CpO} SR M CpO} D ClOi SR
M ClOi D ClO] SR M ClO] D CpOI SR M CpOI D CvN} SR M CvN} D C?Ny SR
M C?Ny D DENy SR M DENy D DNN} SR M DNN} D DTOI SR M DTOI D DWO] SR
M DWO] D DWOi SR M DWOi D DTO} SR M DTO} D DNPI SR M DNPI D DEPN SR
M DEPN D C?PN SR M C?PN D CyPI SR M CyPI D CvPE SR M CvPE D CsO} SR
M CsO} D CpOi SR M CpOi D CpO] SR M CpO] D CsOI SR M CsOI D CvOA SR
M CvOA D CyN} SR M CyN} D C?Ny SR M DENy D DKN} SR M DKN} D DNOA SR
M DNOA D DQOI SR M DQOI D DTO] SR M DTO] D DTOi SR M DTOi D DQO} SR
M DQO} D DNPE SR M DNPE D DKPI SR M DKPI D DEPN SR M EIPs D EJPq SR
M EJPq D EIPo SR M EIPo D EGPq SR M EGPq D EGPs SR M EGPs D EJPx SR
M EJPx D EPP{ SR M EPP{ D EWP{ SR M EWP{ D E]Px SR M E]Px D E^Ps SR
M E^Ps D E^Pl SR M E^Pl D E]Pg SR M E]Pg D EWPe SR M EWPe D ERPe SR
M EWP{ D E[Px SR M E[Px D E]Ps SR M E]Ps D E]Pl SR M E]Pl D E[Pg SR
M E[Pg D EWPe SR M EWPe D E[Pb SR M E[Pb D E^P^ SR M E^P^ D E`PY SR
M E`PY D E`PR SR M E`PR D E^PM SR M E^PM D E]PJ SR M E]PJ D EWPH SR
M EWPH D EPPH SR M EPPH D EJPJ SR M EJPJ D EIPM SR M EIPM D EGPR SR
M EGPR D EGPT SR M EGPT D EIPV SR M EIPV D EJPT SR M EJPT D EIPR SR
M E]P` D E^PY SR M E^PY D E^PR SR M E^PR D E]PM SR M E]PM D E[PJ SR
M E[PJ D EWPH SR M ByYA D B?YF SR M B?YF D CHYR SR M CHYR D CHW} SR
M CEYN D CEW} SR M ByW} D CTW} SR M C?YR D CvYN SR M CvYN D CpYA SR
M CpYA D ClXm SR M ClXm D ClXa SR M ClXa D CpXM SR M CpXM D CvXA SR
M CvXA D C?W} SR M C?W} D DEW} SR M DEW} D DNXA SR M DNXA D DTXM SR
M DTXM D DWXa SR M DWXa D DWXm SR M DWXm D DTYA SR M DTYA D DNYN SR
M DNYN D DEYR SR M DEYR D C?YR SR M C?YR D CyYN SR M CyYN D CvYJ SR
M CvYJ D CsYA SR M CsYA D CpXm SR M CpXm D CpXa SR M CpXa D CsXM SR
M CsXM D CvXE SR M CvXE D CyXA SR M CyXA D C?W} SR M DEW} D DKXA SR
M DKXA D DNXE SR M DNXE D DQXM SR M DQXM D DTXa SR M DTXa D DTXm SR
M DTXm D DQYA SR M DQYA D DNYJ SR M DNYJ D DKYN SR M DKYN D DEYR SR
M EWYz D EWYL SR M EYY? D EYYL SR M EYY? D EEY[ SR M EEY[ D EbY[ SR
M ERYL D E^YL SR M BybF D B?bJ SR M B?bJ D CHbV SR M CHbV D CHaA SR
M CEbR D CEaA SR M ByaA D CTaA SR M C?bV D CvbR SR M CvbR D CpbF SR
M CpbF D Claq SR M Claq D Clae SR M Clae D CpaQ SR M CpaQ D CvaE SR
M CvaE D C?aA SR M C?aA D DEaA SR M DEaA D DNaE SR M DNaE D DTaQ SR
M DTaQ D DWae SR M DWae D DWaq SR M DWaq D DTbF SR M DTbF D DNbR SR
M DNbR D DEbV SR M DEbV D C?bV SR M C?bV D CybR SR M CybR D CvbN SR
M CvbN D CsbF SR M CsbF D Cpaq SR M Cpaq D Cpae SR M Cpae D CsaQ SR
M CsaQ D CvaI SR M CvaI D CyaE SR M CyaE D C?aA SR M DEaA D DKaE SR
M DKaE D DNaI SR M DNaI D DQaQ SR M DQaQ D DTae SR M DTae D DTaq SR
M DTaq D DQbF SR M DQbF D DNbN SR M DNbN D DKbR SR M DKbR D DEbV SR
M EJcC D EGbk SR M EGbk D EJbm SR M EJbm D EPbp SR M EPbp D EUbp SR
M EUbp D E[bm SR M E[bm D E^bh SR M E^bh D E`ba SR M E`ba D E`b_ SR
M E`b_ D E^bW SR M E^bW D E[bS SR M E[bS D EUbP SR M EUbP D EPbP SR
M EPbP D EJbS SR M EJbS D EIbU SR M EIbU D EGbZ SR M EGbZ D EGb\ SR
M EGb\ D EIb_ SR M EIb_ D EJb\ SR M EJb\ D EIbZ SR M EUbp D EYbm SR
M EYbm D E]bh SR M E]bh D E^ba SR M E^ba D E^b_ SR M E^b_ D E]bW SR
M E]bW D EYbS SR M EYbS D EUbP SR M EJcC D E]cC SR M EJcA D EScA SR
M EScA D E]cC SR M BykJ D B?kN SR M B?kN D CHkZ SR M CHkZ D CHjE SR
M CEkV D CEjE SR M ByjE D CTjE SR M C?kZ D CvkV SR M CvkV D CpkJ SR
M CpkJ D Cljv SR M Cljv D Clji SR M Clji D CpjU SR M CpjU D CvjI SR
M CvjI D C?jE SR M C?jE D DEjE SR M DEjE D DNjI SR M DNjI D DTjU SR
M DTjU D DWji SR M DWji D DWjv SR M DWjv D DTkJ SR M DTkJ D DNkV SR
M DNkV D DEkZ SR M DEkZ D C?kZ SR M C?kZ D CykV SR M CykV D CvkR SR
M CvkR D CskJ SR M CskJ D Cpjv SR M Cpjv D Cpji SR M Cpji D CsjU SR
M CsjU D CvjM SR M CvjM D CyjI SR M CyjI D C?jE SR M DEjE D DKjI SR
M DKjI D DNjM SR M DNjM D DQjU SR M DQjU D DTji SR M DTji D DTjv SR
M DTjv D DQkJ SR M DQkJ D DNkR SR M DNkR D DKkV SR M DKkV D DEkZ SR
M E]l@ D E[k} SR M E[k} D E]k{ SR M E]k{ D E^k} SR M E^k} D E^l@ SR
M E^l@ D E]lE SR M E]lE D EYlG SR M EYlG D ESlG SR M ESlG D ENlE SR
M ENlE D EJl@ SR M EJl@ D EIk{ SR M EIk{ D EGkq SR M EGkq D EGkc SR
M EGkc D EIk[ SR M EIk[ D ELkW SR M ELkW D ERkT SR M ERkT D EUkT SR
M EUkT D E[kW SR M E[kW D E^k[ SR M E^k[ D E`kc SR M E`kc D E`ke SR
M E`ke D E^kl SR M E^kl D E[kq SR M E[kq D EUkt SR M EUkt D ESkt SR
M ESkt D ENkq SR M ENkq D EJkl SR M EJkl D EIke SR M ESlG D EPlE SR
M EPlE D ELl@ SR M ELl@ D EJk{ SR M EJk{ D EIkq SR M EIkq D EIkc SR
M EIkc D EJk[ SR M EJk[ D ENkW SR M ENkW D ERkT SR M EUkT D EYkW SR
M EYkW D E]k[ SR M E]k[ D E^kc SR M E^kc D E^ke SR M E^ke D E]kl SR
M E]kl D EYkq SR M EYkq D EUkt SR M BytN D B?tR SR M B?tR D CHt^ SR
M CHt^ D CHsI SR M CEtZ D CEsI SR M BysI D CTsI SR M C?t^ D CvtZ SR
M CvtZ D CptN SR M CptN D Clsz SR M Clsz D Clsn SR M Clsn D CpsY SR
M CpsY D CvsM SR M CvsM D C?sI SR M C?sI D DEsI SR M DEsI D DNsM SR
M DNsM D DTsY SR M DTsY D DWsn SR M DWsn D DWsz SR M DWsz D DTtN SR
M DTtN D DNtZ SR M DNtZ D DEt^ SR M DEt^ D C?t^ SR M C?t^ D CytZ SR
M CytZ D CvtV SR M CvtV D CstN SR M CstN D Cpsz SR M Cpsz D Cpsn SR
M Cpsn D CssY SR M CssY D CvsQ SR M CvsQ D CysM SR M CysM D C?sI SR
M DEsI D DKsM SR M DKsM D DNsQ SR M DNsQ D DQsY SR M DQsY D DTsn SR
M DTsn D DTsz SR M DTsz D DQtN SR M DQtN D DNtV SR M DNtV D DKtZ SR
M DKtZ D DEt^ SR M EGuK D EGt} SR M EGuB D EIuF SR M EIuF D ELuK SR
M ELuK D EPuK SR M EPuK D EYuD SR M EYuD D E]uD SR M E]uD D E^uF SR
M E^uF D E`uK SR M EIuF D ELuI SR M ELuI D EPuI SR M EPuI D EYuD SR
M E`uK D E`uD SR M E`uD D E^t} SR M E^t} D EWtq SR M EWtq D EUtl SR
M EUtl D EStd SR M EStd D EStX SR M E^t} D EUtq SR M EUtq D EStl SR
M EStl D ERtd SR M ERtd D ERtX SR M By}R D B?}V SR M B?}V D CH}b SR
M CH}b D CH|M SR M CE}^ D CE|M SR M By|M D CT|M SR M C?}b D Cv}^ SR
M Cv}^ D Cp}R SR M Cp}R D Cl|~ SR M Cl|~ D Cl|r SR M Cl|r D Cp|^ SR
M Cp|^ D Cv|Q SR M Cv|Q D C?|M SR M C?|M D DE|M SR M DE|M D DN|Q SR
M DN|Q D DT|^ SR M DT|^ D DW|r SR M DW|r D DW|~ SR M DW|~ D DT}R SR
M DT}R D DN}^ SR M DN}^ D DE}b SR M DE}b D C?}b SR M C?}b D Cy}^ SR
M Cy}^ D Cv}Z SR M Cv}Z D Cs}R SR M Cs}R D Cp|~ SR M Cp|~ D Cp|r SR
M Cp|r D Cs|^ SR M Cs|^ D Cv|U SR M Cv|U D Cy|Q SR M Cy|Q D C?|M SR
M DE|M D DK|Q SR M DK|Q D DN|U SR M DN|U D DQ|^ SR M DQ|^ D DT|r SR
M DT|r D DT|~ SR M DT|~ D DQ}R SR M DQ}R D DN}Z SR M DN}Z D DK}^ SR
M DK}^ D DE}b SR M EP~O D EJ~M SR M EJ~M D EI~H SR M EI~H D EI~A SR
M EI~A D EJ}| SR M EJ}| D EP}z SR M EP}z D EW}z SR M EW}z D E]}| SR
M E]}| D E^~A SR M E^~A D E^~H SR M E^~H D E]~M SR M E]~M D EW~O SR
M EW~O D EP~O SR M EP~O D EL~M SR M EL~M D EJ~H SR M EJ~H D EJ~A SR
M EJ~A D EL}| SR M EL}| D EP}z SR M EW}z D E[}| SR M E[}| D E]~A SR
M E]~A D E]~H SR M E]~H D E[~M SR M E[~M D EW~O SR M EP}z D EJ}w SR
M EJ}w D EI}u SR M EI}u D EG}p SR M EG}p D EG}f SR M EG}f D EI}a SR
M EI}a D EJ}_ SR M EJ}_ D EP}\ SR M EP}\ D EW}\ SR M EW}\ D E]}_ SR
M E]}_ D E^}a SR M E^}a D E`}f SR M E`}f D E`}p SR M E`}p D E^}u SR
M E^}u D E]}w SR M E]}w D EW}z SR M EP}z D EL}w SR M EL}w D EJ}u SR
M EJ}u D EI}p SR M EI}p D EI}f SR M EI}f D EJ}a SR M EJ}a D EL}_ SR
M EL}_ D EP}\ SR M EW}\ D E[}_ SR M E[}_ D E]}a SR M E]}a D E^}f SR
M E^}f D E^}p SR M E^}p D E]}u SR M E]}u D E[}w SR M E[}w D EW}z SR
M |rFY D |r|r SR M |rFY D |RFY SR M |rFY D {rFY SR M |rIH D |RIH SR
M |rJn D |RJn SR M |rKv D |RKv SR M |rLn D |RLn SR M |rM\ D |RM\ SR
M |rNC D |RNC SR M |rNe D |RNe SR M |rOB D |ROB SR M |rO] D |RO] SR
M |rO] D {rO] SR M |rRL D |RRL SR M |rSr D |RSr SR M |rTz D |RTz SR
M |rUr D |RUr SR M |rV` D |RV` SR M |rWG D |RWG SR M |rWi D |RWi SR
M |rXG D |RXG SR M |rXa D |RXa SR M |rXa D {rXa SR M |r[P D |R[P SR
M |r\v D |R\v SR M |r]~ D |R]~ SR M |r^w D |R^w SR M |r_e D |R_e SR
M |r`K D |R`K SR M |r`m D |R`m SR M |raK D |RaK SR M |rae D |Rae SR
M |rae D {rae SR M |rdT D |RdT SR M |rez D |Rez SR M |rgB D |RgB SR
M |rg{ D |Rg{ SR M |rhi D |Rhi SR M |riO D |RiO SR M |riq D |Riq SR
M |rjO D |RjO SR M |rji D |Rji SR M |rji D {rji SR M |rmX D |RmX SR
M |rn~ D |Rn~ SR M |rpG D |RpG SR M |rp? D |Rp? SR M |rqm D |Rqm SR
M |rrT D |RrT SR M |rru D |Rru SR M |rsS D |RsS SR M |rsm D |Rsm SR
M |rsm D {rsm SR M |rv\ D |Rv\ SR M |rxB D |RxB SR M |ryK D |RyK SR
M |rzC D |RzC SR M |rzq D |Rzq SR M |r{X D |R{X SR M |r{y D |R{y SR
M |r|W D |R|W SR M |r|r D |R|r SR M |r|r D {r|r SR
M @^Ub D @dUf SR M @dUf D @TUf SR M @TUf D @^Ub SR M @^Ub D @WUZ SR
M @WUZ D @TUN SR M @TUN D @TUF SR M @TUF D @WTz SR M @WTz D @^Tq SR
M @^Tq D @dTm SR M @dTm D @mTi SR M @mTi D @|Ti SR M @|Ti D AETm SR
M AETm D AKTq SR M AKTq D AQTz SR M AQTz D ATUF SR M ATUF D ATUN SR
M ATUN D AQUZ SR M AQUZ D AKUb SR M AKUb D AEUf SR M @TUF D @WT~ SR
M @WT~ D @^Tv SR M @^Tv D @dTq SR M @dTq D @mTm SR M @mTm D @|Tm SR
M @|Tm D AETq SR M AETq D AKTv SR M AKTv D AQT~ SR M AQT~ D ATUF SR
M @jVV D @mVJ SR M @mVJ D @sVB SR M @sVB D @|U~ SR M @|U~ D ABU~ SR
M ABU~ D AKVB SR M AKVB D AQVJ SR M AQVJ D ATVV SR M ATVV D ATV^ SR
M ATV^ D AQVk SR M AQVk D AKVs SR M AKVs D ABVw SR M ABVw D @|Vw SR
M @|Vw D @sVs SR M @sVs D @mVk SR M @mVk D @jV^ SR M @jV^ D @jVV SR
M @jVV D @mVN SR M @mVN D @sVF SR M @sVF D @|VB SR M @|VB D ABVB SR
M ABVB D AKVF SR M AKVF D AQVN SR M AQVN D ATVV SR M ATV^ D AQVf SR
M AQVf D AKVo SR M AKVo D ABVs SR M ABVs D @|Vs SR M @|Vs D @sVo SR
M @sVo D @mVf SR M @mVf D @jV^ SR M @jWW D AKWW SR M AKWW D AQW[ SR
M AQW[ D ATWg SR M ATWg D ATWo SR M ATWo D AQW{ SR M AQW{ D AKXC SR
M @jW[ D AKW[ SR M AKW[ D AQW_ SR M AQW_ D ATWg SR M @jXC D ATXC SR
M @jXG D ATXG SR M @jWK D @jW[ SR M @jWw D @jXG SR M ATXC D ATXS SR
M @jXp D ATXp SR M @jXt D ATXt SR M @sXt D @mX| SR M @mX| D @jYH SR
M @jYH D @jYP SR M @jYP D @mY\ SR M @mY\ D @sY` SR M @sY` D ATY` SR
M @jYP D @mYX SR M @mYX D @sY\ SR M @sY\ D ATY\ SR M @jXd D @jXt SR
M ATXd D ATY@ SR M ATYP D ATYl SR M @TZH D AHZH SR M AHZH D AQZM SR
M AQZM D ATZU SR M ATZU D ATZ] SR M ATZ] D AQZe SR M AQZe D AKZi SR
M @TZM D AHZM SR M AHZM D AQZQ SR M AQZQ D ATZU SR M @jY| D @jZ] SR
M @T\N D AT\N SR M @T\R D AT\R SR M @T\A D @T\r SR M @T\r D @W\~ SR
M @W\~ D @Z]B SR M @Z]B D @a]F SR M @a]F D @g]F SR M @g]F D @m]B SR
M @m]B D @p\~ SR M @p\~ D @s\r SR M @s\r D @s\R SR M @T\r D @W\z SR
M @W\z D @Z\~ SR M @Z\~ D @a]B SR M @a]B D @g]B SR M @g]B D @m\~ SR
M @m\~ D @p\z SR M @p\z D @s\r SR M AT\A D AT\^ SR M @s\j D AN\z SR
M AN\z D AT]B SR M AT]B D AT]J SR M AT]J D AN]N SR M @s\j D @y\r SR
M @y\r D AT]B SR M @p]f D @s]f SR M @s]f D @s]b SR M @s]b D @p]b SR
M @p]b D @m]f SR M @m]f D @j]n SR M @j]n D @j]? SR M @j]? D @m^G SR
M @m^G D @p^K SR M @p^K D @v^O SR M @v^O D AK^O SR M AK^O D AQ^S SR
M AQ^S D AT^W SR M @p^K D AK^K SR M AK^K D AQ^O SR M AQ^O D AT^W SR
M AT^W D AT^[ SR M @v^K D @y^G SR M @y^G D @|]n SR M @|]n D @?]b SR
M @?]b D AE]^ SR M AE]^ D AK]^ SR M AK]^ D AQ]b SR M AQ]b D AT]n SR
M AT]n D AT]z SR M AT]z D AQ^C SR M AQ^C D AK^K SR M @|]n D @?]f SR
M @?]f D AE]b SR M AE]b D AK]b SR M AK]b D AQ]f SR M AQ]f D AT]n SR
M @T^w D AH^w SR M AH^w D AQ^{ SR M AQ^{ D AT_C SR M AT_C D AT_K SR
M AT_K D AQ_S SR M AQ_S D AK_W SR M @T^{ D AH^{ SR M AH^{ D AQ^? SR
M AQ^? D AT_C SR M @j^k D @j_K SR M @|_p D @|`` SR M @|`` D @v`` SR
M @v`` D @p`\ SR M @p`\ D @m`X SR M @m`X D @j`P SR M @j`P D @j`D SR
M @j`D D @m_x SR M @m_x D @s_p SR M @s_p D @|_k SR M @|_k D AB_k SR
M AB_k D AK_p SR M AK_p D AQ_x SR M AQ_x D AT`D SR M AT`D D AT`L SR
M AT`L D AQ`X SR M AQ`X D AK`` SR M @|`\ D @s`\ SR M @s`\ D @m`X SR
M @j`D D @m_| SR M @m_| D @s_t SR M @s_t D @|_p SR M @|_p D AB_p SR
M AB_p D AK_t SR M AK_t D AQ_| SR M AQ_| D AT`D SR M @Hba D @NbY SR
M @NbY D @WbQ SR M @WbQ D @dbI SR M @dbI D @sbE SR M @sbE D @?bE SR
M @?bE D ANbI SR M ANbI D AZbQ SR M AZbQ D AdbY SR M AdbY D Ajba SR
M @NbY D @ZbQ SR M @ZbQ D @dbM SR M @dbM D @sbI SR M @sbI D @?bI SR
M @?bI D ANbM SR M ANbM D AWbQ SR M AWbQ D AdbY SR M @scj D @vcf SR
M @vcf D @ycj SR M @ycj D @vcn SR M @vcn D @scn SR M @scn D @mcf SR
M @mcf D @jc^ SR M @jc^ D @jcQ SR M @jcQ D @mcE SR M @mcE D @sb} SR
M @sb} D @|by SR M @|by D ABby SR M ABby D AKb} SR M AKb} D AQcE SR
M AQcE D ATcQ SR M ATcQ D ATcZ SR M ATcZ D AQcf SR M AQcf D AKcn SR
M @jcQ D @mcI SR M @mcI D @scA SR M @scA D @|b} SR M @|b} D ABb} SR
M ABb} D AKcA SR M AKcA D AQcI SR M AQcI D ATcQ SR M @jd^ D @mdR SR
M @mdR D @sdJ SR M @sdJ D @|dF SR M @|dF D ABdF SR M ABdF D AKdJ SR
M AKdJ D AQdR SR M AQdR D ATd^ SR M ATd^ D ATdf SR M ATdf D AQdr SR
M AQdr D AKdz SR M AKdz D ABd~ SR M ABd~ D @|d~ SR M @|d~ D @sdz SR
M @sdz D @mdr SR M @mdr D @jdf SR M @jdf D @jd^ SR M @jd^ D @mdV SR
M @mdV D @sdN SR M @sdN D @|dJ SR M @|dJ D ABdJ SR M ABdJ D AKdN SR
M AKdN D AQdV SR M AQdV D ATd^ SR M ATdf D AQdn SR M AQdn D AKdv SR
M AKdv D ABdz SR M ABdz D @|dz SR M @|dz D @sdv SR M @sdv D @mdn SR
M @mdn D @jdf SR M @je_ D AKe_ SR M AKe_ D AQec SR M AQec D ATeo SR
M ATeo D ATew SR M ATew D AQfC SR M AQfC D AKfK SR M @jec D AKec SR
M AKec D AQeg SR M AQeg D ATeo SR M @jfK D ATfK SR M @jfO D ATfO SR
M @jeR D @jec SR M @je? D @jfO SR M ATfK D ATf[ SR M @jfw D ATfw SR
M @jf{ D ATf{ SR M @sf{ D @mgC SR M @mgC D @jgP SR M @jgP D @jgX SR
M @jgX D @mgd SR M @mgd D @sgh SR M @sgh D ATgh SR M @jgX D @mg` SR
M @mg` D @sgd SR M @sgd D ATgd SR M @jfk D @jf{ SR M ATfk D ATgH SR
M ATgX D ATgt SR M @ThP D AHhP SR M AHhP D AQhT SR M AQhT D ATh\ SR
M ATh\ D AThd SR M AThd D AQhl SR M AQhl D AKhp SR M @ThT D AHhT SR
M AHhT D AQhX SR M AQhX D ATh\ SR M @jhD D @jhd SR M @mim D @jiq SR
M @jiq D @siq SR M @siq D @mim SR M @mim D @jia SR M @jia D @jiU SR
M @jiU D @miI SR M @miI D @piE SR M @piE D @siE SR M @siE D @yiI SR
M @yiI D @|iQ SR M @|iQ D ABie SR M ABie D AEim SR M AEim D AHiq SR
M @siE D @viI SR M @viI D @yiQ SR M @yiQ D @?ie SR M @?ie D ABim SR
M ABim D AHiq SR M AHiq D ANiq SR M ANiq D AQim SR M AQim D ATia SR
M ATia D ATiU SR M ATiU D AQiI SR M AQiI D AKiE SR M AKiE D ATiE SR
M ATiE D AQiI SR M @mkz D @jk~ SR M @jk~ D @sk~ SR M @sk~ D @mkz SR
M @mkz D @jkn SR M @jkn D @jkb SR M @jkb D @mkV SR M @mkV D @pkR SR
M @pkR D @skR SR M @skR D @ykV SR M @ykV D @|k^ SR M @|k^ D ABkr SR
M ABkr D AEkz SR M AEkz D AHk~ SR M @skR D @vkV SR M @vkV D @yk^ SR
M @yk^ D @?kr SR M @?kr D ABkz SR M ABkz D AHk~ SR M AHk~ D ANk~ SR
M ANk~ D AQkz SR M AQkz D ATkn SR M ATkn D ATkb SR M ATkb D AQkV SR
M AQkV D AKkR SR M AKkR D ATkR SR M ATkR D AQkV SR M @HlR D @Hl} SR
M @@mS D @@mX SR M @@mX D @@m_ SR M @@m_ D @Ym_ SR M @@m] D @Ym] SR
M @YmS D @Ymi SR M @HnA D @NnI SR M @NnI D @WnQ SR M @WnQ D @dnY SR
M @dnY D @sn] SR M @sn] D @?n] SR M @?n] D ANnY SR M ANnY D AZnQ SR
M AZnQ D AdnI SR M AdnI D AjnA SR M @NnI D @ZnQ SR M @ZnQ D @dnU SR
M @dnU D @snY SR M @snY D @?nY SR M @?nY D ANnU SR M ANnU D AWnQ SR
M AWnQ D AdnI SR
M _bBo D _\Bg SR M _\Bg D _VB[ SR M _VB[ D _PBK SR M _PBK D _MAw SR
M _MAw D _MAg SR M _MAg D _PAR SR M _PAR D _VAB SR M _VAB D _\@v SR
M _\@v D _b@n SR M _\Bg D _VBW SR M _VBW D _SBK SR M _SBK D _PAw SR
M _PAw D _PAg SR M _PAg D _SAR SR M _SAR D _VAF SR M _VAF D _\@v SR
M _{B_ D _{AJ SR M _~B_ D _~AJ SR M _rB_ D `VB_ SR M `VB_ D `_B[ SR
M `_B[ D `bBW SR M `bBW D `eBO SR M `eBO D `eBG SR M `eBG D `bA? SR
M `bA? D `_A{ SR M `_A{ D `VAw SR M `VB_ D `\B[ SR M `\B[ D `_BW SR
M `_BW D `bBO SR M `bBO D `bBG SR M `bBG D `_A? SR M `_A? D `\A{ SR
M `\A{ D `VAw SR M _~Aw D `VAw SR M `VAw D `_As SR M `_As D `bAo SR
M `bAo D `eAg SR M `eAg D `eAZ SR M `eAZ D `bAR SR M `bAR D `_AN SR
M `_AN D `VAJ SR M `VAJ D _rAJ SR M `VAw D `\As SR M `\As D `_Ao SR
M `_Ao D `bAg SR M `bAg D `bAZ SR M `bAZ D `_AR SR M `_AR D `\AN SR
M `\AN D `VAJ SR M `xAo D anAo SR M bDB_ D bYAJ SR M bGB_ D bYAV SR
M bnB_ D bYAJ SR M a{B_ D bPB_ SR M beB_ D bxB_ SR M cDBo D cJBg SR
M cJBg D cPB[ SR M cPB[ D cVBK SR M cVBK D cYAw SR M cYAw D cYAg SR
M cYAg D cVAR SR M cVAR D cPAB SR M cPAB D cJ@v SR M cJ@v D cD@n SR
M cJBg D cPBW SR M cPBW D cSBK SR M cSBK D cVAw SR M cVAw D cVAg SR
M cVAg D cSAR SR M cSAR D cPAF SR M cPAF D cJ@v SR M cvAe D cpAb SR
M cpAb D cmA[ SR M cmA[ D ckAO SR M ckAO D ckAH SR M ckAH D cm@| SR
M cm@| D cp@t SR M cp@t D cv@r SR M cv@r D cy@r SR M cy@r D c?@t SR
M c?@t D dC@| SR M dC@| D dDAH SR M dDAH D dDAO SR M dDAO D dCA[ SR
M dCA[ D c?Ab SR M c?Ab D cyAe SR M cyAe D cvAe SR M cvAe D crAb SR
M crAb D cpA` SR M cpA` D cnA[ SR M cnA[ D cmAO SR M cmAO D cmAH SR
M cmAH D cn@| SR M cn@| D cp@w SR M cp@w D cr@t SR M cr@t D cv@r SR
M cy@r D c}@t SR M c}@t D c?@w SR M c?@w D dA@| SR M dA@| D dCAH SR
M dCAH D dCAO SR M dCAO D dAA[ SR M dAA[ D c?A` SR M c?A` D c}Ab SR
M c}Ab D cyAe SR
M kppF D kVn` SR M kppF D lIn` SR M kpow D lFn` SR M k]nx D lBnx SR
M kKn` D kan` SR M k{n` D lTn` SR M lcor D lgom SR M lgom D lcoi SR
M lcoi D l_om SR M l_om D l_or SR M l_or D lco| SR M lco| D lgpA SR
M lgpA D lqpF SR M lqpF D m@pF SR M m@pF D mKpA SR M mKpA D mOo| SR
M mOo| D mRor SR M mRor D mRoi SR M mRoi D mOo_ SR M mOo_ D mDoU SR
M mDoU D lqoK SR M lqoK D ljoG SR M ljoG D lcn} SR M lcn} D l_nn SR
M l_nn D l_n` SR M m@pF D mGpA SR M mGpA D mKo| SR M mKo| D mOor SR
M mOor D mOoi SR M mOoi D mKo_ SR M mKo_ D m@oU SR M m@oU D lqoK SR
M l_nj D lcnn SR M lcnn D ljnn SR M ljnn D l|ne SR M l|ne D mGne SR
M mGne D mOnj SR M mOnj D mRnn SR M ljnn D l|n` SR M l|n` D mKn` SR
M mKn` D mOne SR M mOne D mRnn SR M mRnn D mRnx SR
M Gmza D IAwT D JUtb D KirH D L}pC D NQnP D Oeln D PzkZ D RNjR D SbiS
D Tvh\ D VJgl D W^g@ D XrfX D ZFeq D [ZeK D \nde D ^Bc~ D _VcU D `jbj
D a~a| D cSaJ D dg`U D e{_] D gO^a D hc]b D iw\a D kK[] D l_ZX D msYR
D oGXL D p[WH D qoVF D sCUH D tXTO D ulS^ D w@Ru D xTRW SR
M y~R} D ywRz SR M ywRz D yrRp SR M yrRp D yoR` SR M yoR` D yoRW SR
M yoRW D yrRG SR M yrRG D ywQ} SR M ywQ} D y~Qz SR M y~Qz D zCQz SR
M zCQz D zJQ} SR M zJQ} D zORG SR M zORG D zQRW SR M zQRW D zQR` SR
M zQR` D zORp SR M zORp D zJRz SR M zJRz D zCR} SR M zCR} D y~R} SR
M y~R} D yyRz SR M yyRz D ywRw SR M ywRw D ytRp SR M ytRp D yrR` SR
M yrR` D yrRW SR M yrRW D ytRG SR M ytRG D ywR@ SR M ywR@ D yyQ} SR
M yyQ} D y~Qz SR M zCQz D zHQ} SR M zHQ} D zJR@ SR M zJR@ D zLRG SR
M zLRG D zORW SR M zORW D zOR` SR M zOR` D zLRp SR M zLRp D zJRw SR
M zJRw D zHRz SR M zHRz D zCR} SR M zbR@ D z`Q} SR M z`Q} D zbQz SR
M zbQz D zeQ} SR M zeQ} D zbR@ SR M {BR} D z{Rz SR M z{Rz D zvRp SR
M zvRp D zsR` SR M zsR` D zsRW SR M zsRW D zvRG SR M zvRG D z{Q} SR
M z{Q} D {BQz SR M {BQz D {GQz SR M {GQz D {NQ} SR M {NQ} D {SRG SR
M {SRG D {VRW SR M {VRW D {VR` SR M {VR` D {SRp SR M {SRp D {NRz SR
M {NRz D {GR} SR M {GR} D {BR} SR M {BR} D z}Rz SR M z}Rz D z{Rw SR
M z{Rw D zxRp SR M zxRp D zvR` SR M zvR` D zvRW SR M zvRW D zxRG SR
M zxRG D z{R@ SR M z{R@ D z}Q} SR M z}Q} D {BQz SR M {GQz D {LQ} SR
M {LQ} D {NR@ SR M {NR@ D {QRG SR M {QRG D {SRW SR M {SRW D {SR` SR
M {SR` D {QRp SR M {QRp D {NRw SR M {NRw D {LRz SR M {LRz D {GR} SR
M Gmwl D IAt` D JUqo D KioU D L}mR D NQka D OejA D Pzho D RNgi D Sbfm
D Tvex D VJeJ D W^da D Xrc{ D ZFcW D [Zbt D \nbP D ^Bak D _VaE D `j`[
D a~_o D cS^? D dg^K D e{]T D gO\Z D hc[\ D iwZ\ D kKYY D l_XT D msWO
D oGVI D p[UE D qoTD D sCSF D tXRN D ulQ\ D w@Pt D xTPV SR
M y~P~ D ywP{ SR M ywP{ D yrPq SR M yrPq D yoPa SR M yoPa D yoPW SR
M yoPW D yrPG SR M yrPG D ywO} SR M ywO} D y~Oz SR M y~Oz D zCOz SR
M zCOz D zJO} SR M zJO} D zOPG SR M zOPG D zQPW SR M zQPW D zQPa SR
M zQPa D zOPq SR M zOPq D zJP{ SR M zJP{ D zCP~ SR M zCP~ D y~P~ SR
M y~P~ D yyP{ SR M yyP{ D ywPw SR M ywPw D ytPq SR M ytPq D yrPa SR
M yrPa D yrPW SR M yrPW D ytPG SR M ytPG D ywPA SR M ywPA D yyO} SR
M yyO} D y~Oz SR M zCOz D zHO} SR M zHO} D zJPA SR M zJPA D zLPG SR
M zLPG D zOPW SR M zOPW D zOPa SR M zOPa D zLPq SR M zLPq D zJPw SR
M zJPw D zHP{ SR M zHP{ D zCP~ SR M zbPA D z`O} SR M z`O} D zbOz SR
M zbOz D zeO} SR M zeO} D zbPA SR M z{Pq D {@Pt SR M {@Pt D {GP~ SR
M {GP~ D {GOz SR M {EP{ D {EOz SR M z{Oz D {QOz SR
M Gmt{ D IAqo D JUn? D Kilg D L}je D NQhv D OegX D PzfH D RNeD D SbdJ
D TvcX D VJbm D W^bF D Xrac D ZFaA D [Z`` D \n_~ D ^B_[ D _V^v D `j^O
D a~]d D cS\u D dg\C D e{[N D gOZT D hcYW D iwXW D kKWU D l_VQ D msUL
D oGTG D p[SC D qoRB D sCQE D tXPM D ulO\ D w@Nt D xTNW SR
M y~N~ D ywN{ SR M ywN{ D yrNq SR M yrNq D yoNa SR M yoNa D yoNW SR
M yoNW D yrNG SR M yrNG D ywM~ SR M ywM~ D y~Mz SR M y~Mz D zCMz SR
M zCMz D zJM~ SR M zJM~ D zONG SR M zONG D zQNW SR M zQNW D zQNa SR
M zQNa D zONq SR M zONq D zJN{ SR M zJN{ D zCN~ SR M zCN~ D y~N~ SR
M y~N~ D yyN{ SR M yyN{ D ywNx SR M ywNx D ytNq SR M ytNq D yrNa SR
M yrNa D yrNW SR M yrNW D ytNG SR M ytNG D ywNA SR M ywNA D yyM~ SR
M yyM~ D y~Mz SR M zCMz D zHM~ SR M zHM~ D zJNA SR M zJNA D zLNG SR
M zLNG D zONW SR M zONW D zONa SR M zONa D zLNq SR M zLNq D zJNx SR
M zJNx D zHN{ SR M zHN{ D zCN~ SR M zbNA D z`M~ SR M z`M~ D zbMz SR
M zbMz D zeM~ SR M zeM~ D zbNA SR M zvNq D zxNn SR M zxNn D zvNk SR
M zvNk D zsNn SR M zsNn D zsNq SR M zsNq D zvNx SR M zvNx D zxN{ SR
M zxN{ D {@N~ SR M {@N~ D {IN~ SR M {IN~ D {QN{ SR M {QN{ D {SNx SR
M {SNx D {VNq SR M {VNq D {VNk SR M {VNk D {SNd SR M {SNd D {LN^ SR
M {LN^ D {@NW SR M {@NW D z{NT SR M z{NT D zvNN SR M zvNN D zsND SR
M zsND D zsMz SR M {IN~ D {NN{ SR M {NN{ D {QNx SR M {QNx D {SNq SR
M {SNq D {SNk SR M {SNk D {QNd SR M {QNd D {IN^ SR M {IN^ D {@NW SR
M zsNA D zvND SR M zvND D z{ND SR M z{ND D {GM~ SR M {GM~ D {NM~ SR
M {NM~ D {SNA SR M {SNA D {VND SR M z{ND D {GMz SR M {GMz D {QMz SR
M {QMz D {SM~ SR M {SM~ D {VND SR M {VND D {VNK SR
M GmrM D IAoA D JUlR D Kii| D L}g| D NQfO D Oedr D Pzce D RNbc D Sbak
D Tv`| D VJ`S D W^_n D Xr_M D ZF^m D [Z^N D \n]n D ^B]M D _V\j D `j\D
D a~[[ D cSZm D dgY| D e{YH D gOXO D hcWS D iwVT D kKUR D l_TO D msSJ
D oGRF D p[QB D qoPA D sCOD D tXNL D ulM\ D w@Lt D xTLX SR
M y~L? D ywL{ SR M ywL{ D yrLr SR M yrLr D yoLa SR M yoLa D yoLX SR
M yoLX D yrLH SR M yrLH D ywK~ SR M ywK~ D y~K{ SR M y~K{ D zCK{ SR
M zCK{ D zJK~ SR M zJK~ D zOLH SR M zOLH D zQLX SR M zQLX D zQLa SR
M zQLa D zOLr SR M zOLr D zJL{ SR M zJL{ D zCL? SR M zCL? D y~L? SR
M y~L? D yyL{ SR M yyL{ D ywLx SR M ywLx D ytLr SR M ytLr D yrLa SR
M yrLa D yrLX SR M yrLX D ytLH SR M ytLH D ywLA SR M ywLA D yyK~ SR
M yyK~ D y~K{ SR M zCK{ D zHK~ SR M zHK~ D zJLA SR M zJLA D zLLH SR
M zLLH D zOLX SR M zOLX D zOLa SR M zOLa D zLLr SR M zLLr D zJLx SR
M zJLx D zHL{ SR M zHL{ D zCL? SR M zbLA D z`K~ SR M z`K~ D zbK{ SR
M zbK{ D zeK~ SR M zeK~ D zbLA SR M zvLu D zxLr SR M zxLr D zvLn SR
M zvLn D zsLr SR M zsLr D zsLu SR M zsLu D zxL{ SR M zxL{ D {@L? SR
M {@L? D {IL? SR M {IL? D {QL{ SR M {QL{ D {SLu SR M {SLu D {SLk SR
M {SLk D {QLe SR M {QLe D {ILa SR M {ILa D {BLa SR M {IL? D {NL{ SR
M {NL{ D {QLu SR M {QLu D {QLk SR M {QLk D {NLe SR M {NLe D {ILa SR
M {ILa D {NL^ SR M {NL^ D {SLX SR M {SLX D {VLQ SR M {VLQ D {VLH SR
M {VLH D {SLA SR M {SLA D {QK~ SR M {QK~ D {IK{ SR M {IK{ D {@K{ SR
M {@K{ D zxK~ SR M zxK~ D zvLA SR M zvLA D zsLH SR M zsLH D zsLK SR
M zsLK D zvLN SR M zvLN D zxLK SR M zxLK D zvLH SR M {QL[ D {SLQ SR
M {SLQ D {SLH SR M {SLH D {QLA SR M {QLA D {NK~ SR M {NK~ D {IK{ SR
M Gmoa D IAlW D JUij D KigU D L}eV D NQck D OebQ D PzaE D RN`F D Sb_P
D Tv^c D VJ]| D W^]Y D Xr\z D ZF\\ D [Z[? D \n[a D ^B[A D _VZ` D `jY{
D a~YS D cSXg D dgWw D e{WC D gOVK D hcUP D iwTQ D kKSP D l_RM D msQI
D oGPD D p[OA D qoN@ D sCMD D tXLL D ulK\ D w@Ju D xTJY SR
M y~J? D ywJ| SR M ywJ| D yrJr SR M yrJr D yoJb SR M yoJb D yoJX SR
M yoJX D yrJH SR M yrJH D ywI~ SR M ywI~ D y~I{ SR M y~I{ D zCI{ SR
M zCI{ D zJI~ SR M zJI~ D zOJH SR M zOJH D zQJX SR M zQJX D zQJb SR
M zQJb D zOJr SR M zOJr D zJJ| SR M zJJ| D zCJ? SR M zCJ? D y~J? SR
M y~J? D yyJ| SR M yyJ| D ywJx SR M ywJx D ytJr SR M ytJr D yrJb SR
M yrJb D yrJX SR M yrJX D ytJH SR M ytJH D ywJB SR M ywJB D yyI~ SR
M yyI~ D y~I{ SR M zCI{ D zHI~ SR M zHI~ D zJJB SR M zJJB D zLJH SR
M zLJH D zOJX SR M zOJX D zOJb SR M zOJb D zLJr SR M zLJr D zJJx SR
M zJJx D zHJ| SR M zHJ| D zCJ? SR M zbJB D z`I~ SR M z`I~ D zbI{ SR
M zbI{ D zeI~ SR M zeI~ D zbJB SR M {IJx D {II{ SR M {LJ? D {LI{ SR
M {LJ? D zqJN SR M zqJN D {XJN SR M {BI{ D {SI{ SR
M Gmly D IAiq D JUgE D Kidq D L}bu D NQaL D Oe_s D Pz^i D RN]l D Sb\x
D Tv\M D VJ[h D W^[G D XrZi D ZFZM D [ZYq D \nYU D ^BXw D _VXW D `jWs
D a~WL D cSVa D dgUr D e{T? D gOTH D hcSM D iwRO D kKQN D l_PK D msOH
D oGND D p[MA D qoL@ D sCKD D tXJM D ulI] D w@Hw D xTH[ SR
M y~H? D ywH| SR M ywH| D yrHr SR M yrHr D yoHb SR M yoHb D yoHY SR
M yoHY D yrHH SR M yrHH D ywG? SR M ywG? D y~G| SR M y~G| D zCG| SR
M zCG| D zJG? SR M zJG? D zOHH SR M zOHH D zQHY SR M zQHY D zQHb SR
M zQHb D zOHr SR M zOHr D zJH| SR M zJH| D zCH? SR M zCH? D y~H? SR
M y~H? D yyH| SR M yyH| D ywHy SR M ywHy D ytHr SR M ytHr D yrHb SR
M yrHb D yrHY SR M yrHY D ytHH SR M ytHH D ywHB SR M ywHB D yyG? SR
M yyG? D y~G| SR M zCG| D zHG? SR M zHG? D zJHB SR M zJHB D zLHH SR
M zLHH D zOHY SR M zOHY D zOHb SR M zOHb D zLHr SR M zLHr D zJHy SR
M zJHy D zHH| SR M zHH| D zCH? SR M zbHB D z`G? SR M z`G? D zbG| SR
M zbG| D zeG? SR M zeG? D zbHB SR M zxH? D zsH_ SR M zsH_ D zxHb SR
M zxHb D {@Hf SR M {@Hf D {GHf SR M {GHf D {NHb SR M {NHb D {SH\ SR
M {SH\ D {VHR SR M {VHR D {VHO SR M {VHO D {SHE SR M {SHE D {NG? SR
M {NG? D {GG| SR M {GG| D {@G| SR M {@G| D zxG? SR M zxG? D zvHB SR
M zvHB D zsHH SR M zsHH D zsHL SR M zsHL D zvHO SR M zvHO D zxHL SR
M zxHL D zvHH SR M {GHf D {LHb SR M {LHb D {QH\ SR M {QH\ D {SHR SR
M {SHR D {SHO SR M {SHO D {QHE SR M {QHE D {LG? SR M {LG? D {GG| SR
M zxH? D {QH? SR M zxH| D {EH| SR M {EH| D {QH? SR
%PSKCloseWorkStation
%PSKOpenWorkStation
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FMENDEPSF
63 90 540 711 C
0 0 612 792 C
0 43 29 576 730 213.2 280.4 283.4 117.8 FMBEGINEPSF
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/MAXNDC 4095 def /PageSizeXMeter 0.2594 def /PageSizeYMeter 0.1959 def
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/LandScapeRotation 90. def /GT_LEFT 2 def /GT_RIGHT 3 def
/GT_TOP 6 def /GT_BOTTOM 7 def /GT_UP 4 def /GT_DOWN 5 def
/GT_CENTER 1 def /RF /Times-Roman def /GF /Symbol def
/IF /Times-Italic def /BF /Times-Bold def /DASH 49 def /DOT 4 def
/SPACE 24 def

% How to define things.
/BD { bind def } bind def
/LD { load def } bind def

% Constants
/yes true def
/no false def

% Define some shorthand instructions.
/GRS /grestore LD
/GS /gsave LD
/MK /mark LD
/R /restore LD
/S /save LD
/SH /showpage LD
/SW /setlinewidth LD

% Measurement conversions.
/PointperMeter 2834.64 def
/MonoScale .7 def

% SR: Set current path to page: - -> -
/SR { currentpoint stroke moveto } BD

% CL: CLear the page: - -> -
/CL { restore showpage grestore gsave save } BD

% RC: Read Coordinates: string -> x y
/RC {
currentfile read pop 8#77 and 6 bitshift
currentfile read pop 8#77 and or
currentfile read pop 8#77 and 6 bitshift
currentfile read pop 8#77 and or
} BD

% DO - Determine Offset: length -> offset
/DO { DS dup 0 eq { pop pop 0 } { mod } ifelse } BD

% M: Move: M string -> -
% Move to a point and clear length of path.
/M { RC moveto CT OF setdash } BD

% D: Draw: D string -> -
% This also calculates the length of the current path.
/OF 0 def
/D { RC DS 0 ne { 2 copy currentpoint exch 4 1 roll sub dup mul 3 1 roll
sub dup mul add sqrt round OF add cvi DO /OF exch store } if lineto
} BD

% Character/Font definitions.

% FS -- Define the current font size: xsize ysize FS -
/FontXSize 0 def /FontYSize 0 def /NewFont true def
/FS { /FontYSize exch MonoScale mul store /FontXSize exch MonoScale mul store
/NewFont true store } BD

% PH -- Set the current path: path PH -
/Path 0 def
/PH { /Path exch store } BD

% PA -- Set the path angle of the text: angle PA -
/Angle 0 def
/PA { 360 mod dup 0 lt { 360 add } if /Angle exch store /NewFont true store } BD

% HJ, VJ -- Set Horizontal/Verticle Justification: just HJ/VJ -
/HorzJust 0 def /VertJust 0 def
/HJ { /HorzJust exch store } BD /VJ { /VertJust exch store } BD

% VT -- Use mono- or variable-spaced fonts: flag VT -
/VT true def
/VT { /Variable exch store } BD

% SetFont -- Make the required font the default: font SetFont -
% Note scale factor- This is to fill out monospaced better and match other
% IRAF output.
/Font () def
/FontMatrix matrix def
/SetFont {
dup Font ne NewFont or
{ dup /Font exch store findfont
Angle matrix rotate FontXSize MonoScale div FontYSize MonoScale div
matrix scale matrix concatmatrix makefont setfont Angle matrix rotate
FontXSize FontYSize matrix scale matrix concatmatrix /FontMatrix exch
store
}
{ pop } ifelse /NewFont false store
} BD

% StringWidth -- Determine path length of string: string StringWidth - xs ys
/StringWidth { Path GT_RIGHT eq Variable and { stringwidth }
{ Path GT_RIGHT eq { length } { pop 1 } ifelse 0 FontMatrix transform }
ifelse
} BD

% MonoShow -- Write the string out in mono-spaced: string MonoShow -
/MonoShow {
/t 1 string def 1 0 FontMatrix transform
/dy exch def /dx exch def Path GT_RIGHT eq { /mx dx def /my dy def }
{ 0 1 FontMatrix transform /my exch def /mx exch def } ifelse
{ t 0 3 -1 roll put t dup stringwidth dy exch sub 2 div exch dx exch
sub 2 div exch gsave rmoveto show grestore mx my rmoveto
} forall
} BD

% WS -- Draw the string: string font string ... DS -
/*WSDict 13 dict def
/WS { *WSDict begin
counttomark 2 idiv dup dup array /FontArray exch def
array /StringArray exch def 1 sub /NStrings exch def

NStrings -1 0 {
dup 4 1 roll exch StringArray 3 1 roll put FontArray 3 1 roll put
} for
pop

/XSize 0 def /YSize 0 def /NChars 0 def
0 1 NStrings {
dup FontArray exch get SetFont StringArray exch get dup
length NChars add /NChars exch def StringWidth
YSize add /YSize exch def XSize add /XSize exch def
} for

/TAngle HorzJust GT_RIGHT eq
{ Angle 180 add dup 360 ge { 360 sub } if } { Angle } ifelse def
0 TAngle 180 le HorzJust GT_CENTER eq or
{ Angle sin FontYSize mul Path GT_UP eq { NChars mul } if add } if
TAngle 90 ge TAngle 270 le and HorzJust GT_CENTER eq or
{ Path GT_RIGHT eq { XSize } { Angle cos FontXSize mul } ifelse sub } if
HorzJust GT_CENTER eq { .5 mul } if

/TAngle
VertJust GT_TOP eq { Angle 180 sub dup 0 lt { 360 add } if } { Angle } ifelse
def
0 TAngle 90 ge TAngle 270 le and VertJust GT_CENTER eq or
{ Angle cos FontYSize mul Path GT_UP eq { NChars mul } if sub } if
TAngle 180 ge TAngle 360 le and VertJust GT_CENTER eq or
{ Path GT_RIGHT eq { YSize } { Angle sin FontXSize mul } ifelse sub } if
VertJust GT_CENTER eq { .5 mul } if
rmoveto

0 1 NStrings {
dup FontArray exch get SetFont StringArray exch get
Path GT_RIGHT eq Variable and { show } { MonoShow } ifelse
} for

end
} BD

% Define the DASHED, DOTTED, DOTDASH patterns.
/DS 0 def
/LPS {
/OF 0 store /DS 0 store 0 array
} BD
/LPD {
/OF 0 store DASH SPACE 2 copy add /DS exch store 2 array astore
} BD
/LPP {
/OF 0 store DOT SPACE 2 copy add /DS exch store 2 array astore
} BD
/LDD {
/OF 0 store DOT SPACE DASH SPACE 4 copy add add add /DS exch store
4 array astore
} BD

% LT - Set Line Type - array -> -
/CT { currentdash pop } BD
/LT { /CT exch store /OF 0 store } BD

% SC - Set Color: color -> -
/*SCDict 1 dict def
/SC { *SCDict begin
1 sub /color exch def
GR color get 255 div GG color get 255 div GB color get 255 div setrgbcolor
end
} BD

% MI - Make Image LUT: table-name size MI hexstring -> -
/MI { currentfile exch string readhexstring pop def } BD

% Define the graphics color lookup table.
/GR 16 MI 00FFFF0000FF00FFFFB0FFF0D940F0F5
/GG 16 MI 00FF00FF00FFFF0080D0A6E670E082DE
/GB 16 MI 00FF0000FF00FFFF4F61008CD6D1EFB3

% Render an image when no image LUT has been define.
/DefaultGrey {
{ currentfile inarr readhexstring pop } image
} BD

% ColorImage - Produce an image by indexing into the Image Lookup Table.
% There are two versions of this code- one for PostScript that has
% the colorimage operator and one that doesn't. If the PostScript doesn't
% have colorimage, it is assumed that it can only produce black & white,
% in which the Image LUT is combined to produce a single grey which is
% then used as the image for the image operator.
/colorimage where
{ pop
/ColorImage {
{ currentfile inarr readhexstring pop dup /inarr exch def
length 3 mul string /oarr exch def
0 1 inarr length 1 sub
{ /iindex exch def
/oindex iindex 3 mul def
oarr oindex IR inarr iindex get get put
oarr oindex 1 add IG inarr iindex get get put
oarr oindex 2 add IB inarr iindex get get put
} for
oarr
}
false 3 colorimage
} BD
}
{ /ColorImage {
{ currentfile inarr readhexstring pop dup /inarr exch def
length string /oarr exch def
0 1 inarr length 1 sub
{ /iindex exch def
oarr iindex
IR inarr iindex get get 0.3 mul
IG inarr iindex get get 0.59 mul
IB inarr iindex get get 0.11 mul
add add round cvi dup 255 gt { pop 255 } if
put
} for
oarr
}
image
} BD
}
ifelse

% PC: Put Cellarray: width height bitspersample matrix -> -
/*PCdict 10 dict def
/PC {
*PCdict begin
4 -1 roll dup /inarr exch string def 4 1 roll
/IR where {pop ColorImage} {DefaultGrey} ifelse
end
} BD

% Define the Hatch (fill area) styles. H1 and H2 are handled internally
% by PSIKern. Feel free to define more; there is no limit.
/H3 <8888888888888888> def
/H4 def
/H5 <8844221188442211> def
/H6 <1122448811224488> def

% Setup for fill patterns. This whole section of code is taken almost
% directly from _PostScript Language: Tutorial and Cookbook_, Adobe Systems,
% 1986 (the blue book).
/setuserscreendict 22 dict def
setuserscreendict begin
/tempctm matrix def
/temprot matrix def
/tempscale matrix def

/concatprocs
{ /proc2 exch cvlit def
/proc1 exch cvlit def
/newproc proc1 length proc2 length add
array def
newproc 0 proc1 putinterval
newproc proc1 length proc2 putinterval
newproc cvx
} def

/resmatrix matrix def
/findresolution
{ 72 0 resmatrix defaultmatrix dtransform
/yres exch def /xres exch def
xres dup mul yres dup mul add sqrt
} def
end

/setuserscreen
{ setuserscreendict begin
/spotfunction exch def
/screenangle exch def
/cellsize exch def

/m tempctm currentmatrix def
/rm screenangle temprot rotate def
/sm cellsize dup tempscale scale def

sm rm m m concatmatrix m concatmatrix pop
1 0 m dtransform /y1 exch def /x1 exch def

/veclength x1 dup mul y1 dup mul add sqrt def
/frequency findresolution veclength div def

/newscreenangle y1 x1 atan def

m 2 get m 1 get mul m 0 get m 3 get mul sub
0 gt
{ {neg} /spotfunction load concatprocs
/spotfunction exch def
} if

frequency newscreenangle /spotfunction load
setscreen
end
} def

/setpatterndict 18 dict def
setpatterndict begin
/bitison
{ /ybit exch def /xbit exch def
/bytevalue bstring ybit bwidth mul xbit 8 idiv
add get def

/mask 1 7 xbit 8 mod sub bitshift def
bytevalue mask and 0 ne
} def
end

/bitpatternspotfunction
{ setpatterndict begin
/y exch def /x exch def

/xindex x 1 add 2 div bpside mul cvi def
/yindex y 1 add 2 div bpside mul cvi def

xindex yindex bitison
{ /onbits onbits 1 add def 1 }
{ /offbits offbits 1 add def 0 }
ifelse
end
} def

/setpattern
{ setpatterndict begin
/cellsz exch def
/angle exch def
/bwidth exch def
/bpside exch def
/bstring exch def

/onbits 0 def /offbits 0 def
cellsz angle /bitpatternspotfunction load
setuserscreen
{ } settransfer
offbits offbits onbits add div setgray
end
} def

% SP: Set Pattern: pattern -> -
/SP { 8 1 0 MAXNDC 100 div setpattern } BD

% FI: Fill with Pattern: - -> -
/FI { fill grestore } BD

% Set the transformation matrix.
PointperMeter dup scale
PageOffXMeter
PortraitMode not
{ PageSizeYMeter add }
if
PageOffYMeter translate
PortraitMode
{ PortraitRotation rotate }
{ LandScapeRotation rotate}
ifelse
PageSizeXMeter MAXNDC div PageSizeYMeter MAXNDC div scale
1 setlinejoin 1 setlinecap

% Save the current graphics state (to restore after showpage) and the
% VM state to recover after a showpage.
GS S

%%EndProlog
%PSKOpenWorkStation
%%Page: 1 1
LPS LT 3 SW 1 SC M FYFY D |rFY SR M FYFY D FYGY SR M HUFY D HUFy SR
M JQFY D JQFy SR M LNFY D LNFy SR M NJFY D NJGY SR M PFFY D PFFy SR
M RCFY D RCFy SR M S?FY D S?Fy SR M U{FY D U{GY SR M WxFY D WxFy SR
M YtFY D YtFy SR M [pFY D [pFy SR M ]mFY D ]mGY SR M _iFY D _iFy SR
M aeFY D aeFy SR M cbFY D cbFy SR M e^FY D e^GY SR M gZFY D gZFy SR
M iVFY D iVFy SR M kSFY D kSFy SR M mOFY D mOGY SR M oKFY D oKFy SR
M qHFY D qHFy SR M sDFY D sDFy SR M u@FY D u@GY SR M v}FY D v}Fy SR
M xyFY D xyFy SR M zuFY D zuFy SR M |rFY D |rGY SR M DtD{ D EkD{ SR
M FPEl D FGEh SR M FGEh D FAE\ SR M FAE\ D E~EG SR M E~EG D E~D{ SR
M E~D{ D FADg SR M FADg D FGD[ SR M FGD[ D FPDW SR M FPDW D FVDW SR
M FVDW D F_D[ SR M F_D[ D FeDg SR M FeDg D FhD{ SR M FhD{ D FhEG SR
M FhEG D FeE\ SR M FeE\ D F_Eh SR M F_Eh D FVEl SR M FVEl D FPEl SR
M FPEl D FJEh SR M FJEh D FGEd SR M FGEd D FDE\ SR M FDE\ D FAEG SR
M FAEG D FAD{ SR M FAD{ D FDDg SR M FDDg D FGD_ SR M FGD_ D FJD[ SR
M FJD[ D FPDW SR M FVDW D F\D[ SR M F\D[ D F_D_ SR M F_D_ D FbDg SR
M FbDg D FeD{ SR M FeD{ D FeEG SR M FeEG D FbE\ SR M FbE\ D F_Ed SR
M F_Ed D F\Eh SR M F\Eh D FVEl SR M F~D_ D FzD[ SR M FzD[ D F~DW SR
M F~DW D GAD[ SR M GAD[ D F~D_ SR M GnEd D GnDW SR M GqEl D GqDW SR
M GqEl D GPDo SR M GPDo D HADo SR M GeDW D GzDW SR M LfD{ D M\D{ SR
M NAEl D MxEh SR M MxEh D MrE\ SR M MrE\ D MoEG SR M MoEG D MoD{ SR
M MoD{ D MrDg SR M MrDg D MxD[ SR M MxD[ D NADW SR M NADW D NGDW SR
M NGDW D NPD[ SR M NPD[ D NVDg SR M NVDg D NYD{ SR M NYD{ D NYEG SR
M NYEG D NVE\ SR M NVE\ D NPEh SR M NPEh D NGEl SR M NGEl D NAEl SR
M NAEl D M{Eh SR M M{Eh D MxEd SR M MxEd D MuE\ SR M MuE\ D MrEG SR
M MrEG D MrD{ SR M MrD{ D MuDg SR M MuDg D MxD_ SR M MxD_ D M{D[ SR
M M{D[ D NADW SR M NGDW D NMD[ SR M NMD[ D NPD_ SR M NPD_ D NSDg SR
M NSDg D NVD{ SR M NVD{ D NVEG SR M NVEG D NSE\ SR M NSE\ D NPEd SR
M NPEd D NMEh SR M NMEh D NGEl SR M NoD_ D NlD[ SR M NlD[ D NoDW SR
M NoDW D NrD[ SR M NrD[ D NoD_ SR M OGE\ D OJEX SR M OJEX D OGET SR
M OGET D ODEX SR M ODEX D ODE\ SR M ODE\ D OGEd SR M OGEd D OJEh SR
M OJEh D OSEl SR M OSEl D O`El SR M O`El D OiEh SR M OiEh D OlEd SR
M OlEd D OoE\ SR M OoE\ D OoET SR M OoET D OlEL SR M OlEL D OcEC SR
M OcEC D OSD{ SR M OSD{ D OMDw SR M OMDw D OGDo SR M OGDo D ODDc SR
M ODDc D ODDW SR M O`El D OfEh SR M OfEh D OiEd SR M OiEd D OlE\ SR
M OlE\ D OlET SR M OlET D OiEL SR M OiEL D O`EC SR M O`EC D OSD{ SR
M ODD_ D OGDc SR M OGDc D OMDc SR M OMDc D O\D[ SR M O\D[ D OfD[ SR
M OfD[ D OlD_ SR M OlD_ D OoDc SR M OMDc D O\DW SR M O\DW D OiDW SR
M OiDW D OlD[ SR M OlD[ D OoDc SR M OoDc D OoDk SR M UxEl D UoEh SR
M UoEh D UiE\ SR M UiE\ D UfEG SR M UfEG D UfD{ SR M UfD{ D UiDg SR
M UiDg D UoD[ SR M UoD[ D UxDW SR M UxDW D U~DW SR M U~DW D VHD[ SR
M VHD[ D VNDg SR M VNDg D VQD{ SR M VQD{ D VQEG SR M VQEG D VNE\ SR
M VNE\ D VHEh SR M VHEh D U~El SR M U~El D UxEl SR M UxEl D UrEh SR
M UrEh D UoEd SR M UoEd D UlE\ SR M UlE\ D UiEG SR M UiEG D UiD{ SR
M UiD{ D UlDg SR M UlDg D UoD_ SR M UoD_ D UrD[ SR M UrD[ D UxDW SR
M U~DW D VED[ SR M VED[ D VHD_ SR M VHD_ D VKDg SR M VKDg D VND{ SR
M VND{ D VNEG SR M VNEG D VKE\ SR M VKE\ D VHEd SR M VHEd D VEEh SR
M VEEh D U~El SR M \?El D \vEh SR M \vEh D \pE\ SR M \pE\ D \mEG SR
M \mEG D \mD{ SR M \mD{ D \pDg SR M \pDg D \vD[ SR M \vD[ D \?DW SR
M \?DW D ]EDW SR M ]EDW D ]ND[ SR M ]ND[ D ]TDg SR M ]TDg D ]WD{ SR
M ]WD{ D ]WEG SR M ]WEG D ]TE\ SR M ]TE\ D ]NEh SR M ]NEh D ]EEl SR
M ]EEl D \?El SR M \?El D \yEh SR M \yEh D \vEd SR M \vEd D \sE\ SR
M \sE\ D \pEG SR M \pEG D \pD{ SR M \pD{ D \sDg SR M \sDg D \vD_ SR
M \vD_ D \yD[ SR M \yD[ D \?DW SR M ]EDW D ]KD[ SR M ]KD[ D ]ND_ SR
M ]ND_ D ]QDg SR M ]QDg D ]TD{ SR M ]TD{ D ]TEG SR M ]TEG D ]QE\ SR
M ]QE\ D ]NEd SR M ]NEd D ]KEh SR M ]KEh D ]EEl SR M ]mD_ D ]jD[ SR
M ]jD[ D ]mDW SR M ]mDW D ]pD[ SR M ]pD[ D ]mD_ SR M ^EE\ D ^HEX SR
M ^HEX D ^EET SR M ^EET D ^BEX SR M ^BEX D ^BE\ SR M ^BE\ D ^EEd SR
M ^EEd D ^HEh SR M ^HEh D ^QEl SR M ^QEl D ^]El SR M ^]El D ^gEh SR
M ^gEh D ^jEd SR M ^jEd D ^mE\ SR M ^mE\ D ^mET SR M ^mET D ^jEL SR
M ^jEL D ^`EC SR M ^`EC D ^QD{ SR M ^QD{ D ^KDw SR M ^KDw D ^EDo SR
M ^EDo D ^BDc SR M ^BDc D ^BDW SR M ^]El D ^dEh SR M ^dEh D ^gEd SR
M ^gEd D ^jE\ SR M ^jE\ D ^jET SR M ^jET D ^gEL SR M ^gEL D ^]EC SR
M ^]EC D ^QD{ SR M ^BD_ D ^EDc SR M ^EDc D ^KDc SR M ^KDc D ^ZD[ SR
M ^ZD[ D ^dD[ SR M ^dD[ D ^jD_ SR M ^jD_ D ^mDc SR M ^KDc D ^ZDW SR
M ^ZDW D ^gDW SR M ^gDW D ^jD[ SR M ^jD[ D ^mDc SR M ^mDc D ^mDk SR
M dpEl D dgEh SR M dgEh D daE\ SR M daE\ D d^EG SR M d^EG D d^D{ SR
M d^D{ D daDg SR M daDg D dgD[ SR M dgD[ D dpDW SR M dpDW D dvDW SR
M dvDW D d?D[ SR M d?D[ D eFDg SR M eFDg D eID{ SR M eID{ D eIEG SR
M eIEG D eFE\ SR M eFE\ D d?Eh SR M d?Eh D dvEl SR M dvEl D dpEl SR
M dpEl D djEh SR M djEh D dgEd SR M dgEd D ddE\ SR M ddE\ D daEG SR
M daEG D daD{ SR M daD{ D ddDg SR M ddDg D dgD_ SR M dgD_ D djD[ SR
M djD[ D dpDW SR M dvDW D d|D[ SR M d|D[ D d?D_ SR M d?D_ D eBDg SR
M eBDg D eFD{ SR M eFD{ D eFEG SR M eFEG D eBE\ SR M eBE\ D d?Ed SR
M d?Ed D d|Eh SR M d|Eh D dvEl SR M e^D_ D e[D[ SR M e[D[ D e^DW SR
M e^DW D eaD[ SR M eaD[ D e^D_ SR M fOEd D fODW SR M fREl D fRDW SR
M fREl D epDo SR M epDo D faDo SR M fFDW D f[DW SR M lbEl D lXEh SR
M lXEh D lRE\ SR M lRE\ D lOEG SR M lOEG D lOD{ SR M lOD{ D lRDg SR
M lRDg D lXD[ SR M lXD[ D lbDW SR M lbDW D lhDW SR M lhDW D lqD[ SR
M lqD[ D lwDg SR M lwDg D lzD{ SR M lzD{ D lzEG SR M lzEG D lwE\ SR
M lwE\ D lqEh SR M lqEh D lhEl SR M lhEl D lbEl SR M lbEl D l[Eh SR
M l[Eh D lXEd SR M lXEd D lUE\ SR M lUE\ D lREG SR M lREG D lRD{ SR
M lRD{ D lUDg SR M lUDg D lXD_ SR M lXD_ D l[D[ SR M l[D[ D lbDW SR
M lhDW D lnD[ SR M lnD[ D lqD_ SR M lqD_ D ltDg SR M ltDg D lwD{ SR
M lwD{ D lwEG SR M lwEG D ltE\ SR M ltE\ D lqEd SR M lqEd D lnEh SR
M lnEh D lhEl SR M mOD_ D mLD[ SR M mLD[ D mODW SR M mODW D mRD[ SR
M mRD[ D mOD_ SR M nIE` D nFE\ SR M nFE\ D nIEX SR M nIEX D nLE\ SR
M nLE\ D nLE` SR M nLE` D nIEh SR M nIEh D nCEl SR M nCEl D mzEl SR
M mzEl D mqEh SR M mqEh D mkE` SR M mkE` D mhEX SR M mhEX D meEG SR
M meEG D meDo SR M meDo D mhDc SR M mhDc D mnD[ SR M mnD[ D mwDW SR
M mwDW D m}DW SR M m}DW D nFD[ SR M nFD[ D nLDc SR M nLDc D nODo SR
M nODo D nODs SR M nODs D nLD? SR M nLD? D nFEG SR M nFEG D m}EL SR
M m}EL D mzEL SR M mzEL D mqEG SR M mqEG D mkD? SR M mkD? D mhDs SR
M mzEl D mtEh SR M mtEh D mnE` SR M mnE` D mkEX SR M mkEX D mhEG SR
M mhEG D mhDo SR M mhDo D mkDc SR M mkDc D mqD[ SR M mqD[ D mwDW SR
M m}DW D nCD[ SR M nCD[ D nIDc SR M nIDc D nLDo SR M nLDo D nLDs SR
M nLDs D nID? SR M nID? D nCEG SR M nCEG D m}EL SR M tSEl D tJEh SR
M tJEh D tDE\ SR M tDE\ D t@EG SR M t@EG D t@D{ SR M t@D{ D tDDg SR
M tDDg D tJD[ SR M tJD[ D tSDW SR M tSDW D tYDW SR M tYDW D tbD[ SR
M tbD[ D thDg SR M thDg D tkD{ SR M tkD{ D tkEG SR M tkEG D thE\ SR
M thE\ D tbEh SR M tbEh D tYEl SR M tYEl D tSEl SR M tSEl D tMEh SR
M tMEh D tJEd SR M tJEd D tGE\ SR M tGE\ D tDEG SR M tDEG D tDD{ SR
M tDD{ D tGDg SR M tGDg D tJD_ SR M tJD_ D tMD[ SR M tMD[ D tSDW SR
M tYDW D t_D[ SR M t_D[ D tbD_ SR M tbD_ D teDg SR M teDg D thD{ SR
M thD{ D thEG SR M thEG D teE\ SR M teE\ D tbEd SR M tbEd D t_Eh SR
M t_Eh D tYEl SR M u@D_ D t}D[ SR M t}D[ D u@DW SR M u@DW D uDD[ SR
M uDD[ D u@D_ SR M ueEl D u\Eh SR M u\Eh D uYE` SR M uYE` D uYET SR
M uYET D u\EL SR M u\EL D ueEG SR M ueEG D uqEG SR M uqEG D uzEL SR
M uzEL D u}ET SR M u}ET D u}E` SR M u}E` D uzEh SR M uzEh D uqEl SR
M uqEl D ueEl SR M ueEl D u_Eh SR M u_Eh D u\E` SR M u\E` D u\ET SR
M u\ET D u_EL SR M u_EL D ueEG SR M uqEG D uwEL SR M uwEL D uzET SR
M uzET D uzE` SR M uzE` D uwEh SR M uwEh D uqEl SR M ueEG D u\EC SR
M u\EC D uYD? SR M uYD? D uVDw SR M uVDw D uVDg SR M uVDg D uYD_ SR
M uYD_ D u\D[ SR M u\D[ D ueDW SR M ueDW D uqDW SR M uqDW D uzD[ SR
M uzD[ D u}D_ SR M u}D_ D v@Dg SR M v@Dg D v@Dw SR M v@Dw D u}D? SR
M u}D? D uzEC SR M uzEC D uqEG SR M ueEG D u_EC SR M u_EC D u\D? SR
M u\D? D uYDw SR M uYDw D uYDg SR M uYDg D u\D_ SR M u\D_ D u_D[ SR
M u_D[ D ueDW SR M uqDW D uwD[ SR M uwD[ D uzD_ SR M uzD_ D u}Dg SR
M u}Dg D u}Dw SR M u}Dw D uzD? SR M uzD? D uwEC SR M uwEC D uqEG SR
M |fE\ D |lE` SR M |lE` D |uEl SR M |uEl D |uDW SR M |rEh D |rDW SR
M |fDW D }ADW SR M FY|r D |r|r SR M FY|r D FY{r SR M HU|r D HU|R SR
M JQ|r D JQ|R SR M LN|r D LN|R SR M NJ|r D NJ{r SR M PF|r D PF|R SR
M RC|r D RC|R SR M S?|r D S?|R SR M U{|r D U{{r SR M Wx|r D Wx|R SR
M Yt|r D Yt|R SR M [p|r D [p|R SR M ]m|r D ]m{r SR M _i|r D _i|R SR
M ae|r D ae|R SR M cb|r D cb|R SR M e^|r D e^{r SR M gZ|r D gZ|R SR
M iV|r D iV|R SR M kS|r D kS|R SR M mO|r D mO{r SR M oK|r D oK|R SR
M qH|r D qH|R SR M sD|r D sD|R SR M u@|r D u@{r SR M v}|r D v}|R SR
M xy|r D xy|R SR M zu|r D zu|R SR M |r|r D |r{r SR M FYFY D FY|r SR
M FYFY D FyFY SR M FYFY D GYFY SR M FYH\ D FyH\ SR M FYIh D FyIh SR
M FYJ_ D FyJ_ SR M FYKI D FyKI SR M FYKk D FyKk SR M FYLI D FyLI SR
M FYLb D FyLb SR M FYLx D FyLx SR M FYML D FyML SR M FYML D GYML SR
M FYOO D FyOO SR M FYP\ D FyP\ SR M FYQR D FyQR SR M FYQ| D FyQ| SR
M FYR^ D FyR^ SR M FYR| D FyR| SR M FYSU D FySU SR M FYSk D FySk SR
M FYS? D FyS? SR M FYS? D GYS? SR M FYVB D FyVB SR M FYWO D FyWO SR
M FYXE D FyXE SR M FYXo D FyXo SR M FYYR D FyYR SR M FYYo D FyYo SR
M FYZH D FyZH SR M FYZ^ D FyZ^ SR M FYZr D FyZr SR M FYZr D GYZr SR
M FY\u D Fy\u SR M FY^B D Fy^B SR M FY^x D Fy^x SR M FY_b D Fy_b SR
M FY`E D Fy`E SR M FY`b D Fy`b SR M FY`{ D Fy`{ SR M FYaQ D FyaQ SR
M FYae D Fyae SR M FYae D GYae SR M FYch D Fych SR M FYdu D Fydu SR
M FYek D Fyek SR M FYfU D FyfU SR M FYfx D Fyfx SR M FYgU D FygU SR
M FYgn D Fygn SR M FYhD D FyhD SR M FYhX D FyhX SR M FYhX D GYhX SR
M FYj[ D Fyj[ SR M FYkh D Fykh SR M FYl^ D Fyl^ SR M FYmH D FymH SR
M FYmk D Fymk SR M FYnH D FynH SR M FYna D Fyna SR M FYnw D Fynw SR
M FYoK D FyoK SR M FYoK D GYoK SR M FYqN D FyqN SR M FYr[ D Fyr[ SR
M FYsQ D FysQ SR M FYs| D Fys| SR M FYt^ D Fyt^ SR M FYt{ D Fyt{ SR
M FYuT D FyuT SR M FYuk D Fyuk SR M FYu? D Fyu? SR M FYu? D GYu? SR
M FYxA D FyxA SR M FYyN D FyyN SR M FYzD D FyzD SR M FYzo D Fyzo SR
M FY{Q D Fy{Q SR M FY{n D Fy{n SR M FY|G D Fy|G SR M FY|^ D Fy|^ SR
M FY|r D Fy|r SR M FY|r D GY|r SR M BnFy D BtF} SR M BtF} D B}GI SR
M B}GI D B}Eu SR M BzGE D BzEu SR M BnEu D CIEu SR M CtGI D CkGE SR
M CkGE D CeFy SR M CeFy D CbFe SR M CbFe D CbFY SR M CbFY D CeFE SR
M CeFE D CkEy SR M CkEy D CtEu SR M CtEu D CzEu SR M CzEu D DCEy SR
M DCEy D DIFE SR M DIFE D DLFY SR M DLFY D DLFe SR M DLFe D DIFy SR
M DIFy D DCGE SR M DCGE D CzGI SR M CzGI D CtGI SR M CtGI D CnGE SR
M CnGE D CkGA SR M CkGA D ChFy SR M ChFy D CeFe SR M CeFe D CeFY SR
M CeFY D ChFE SR M ChFE D CkE} SR M CkE} D CnEy SR M CnEy D CtEu SR
M CzEu D D@Ey SR M D@Ey D DCE} SR M DCE} D DFFE SR M DFFE D DIFY SR
M DIFY D DIFe SR M DIFe D DFFy SR M DFFy D DCGA SR M DCGA D D@GE SR
M D@GE D CzGI SR M D[GZ D D|GZ SR M EIGm D EJGj SR M EJGj D EIGh SR
M EIGh D EGGj SR M EGGj D EGGm SR M EGGm D EIGr SR M EIGr D EJGt SR
M EJGt D EPGw SR M EPGw D EWGw SR M EWGw D E]Gt SR M E]Gt D E^Gr SR
M E^Gr D E`Gm SR M E`Gm D E`Gh SR M E`Gh D E^Gc SR M E^Gc D EYG^ SR
M EYG^ D EPGZ SR M EPGZ D ELGW SR M ELGW D EIGR SR M EIGR D EGGK SR
M EGGK D EGGD SR M EWGw D E[Gt SR M E[Gt D E]Gr SR M E]Gr D E^Gm SR
M E^Gm D E^Gh SR M E^Gh D E]Gc SR M E]Gc D EWG^ SR M EWG^ D EPGZ SR
M EGGI D EIGK SR M EIGK D ELGK SR M ELGK D EUGF SR M EUGF D E[GF SR
M E[GF D E^GI SR M E^GI D E`GK SR M ELGK D EUGD SR M EUGD D E]GD SR
M E]GD D E^GF SR M E^GF D E`GK SR M E`GK D E`GP SR M BnMl D BtMp SR
M BtMp D B}M| SR M B}M| D B}Lh SR M BzMx D BzLh SR M BnLh D CILh SR
M CtM| D CkMx SR M CkMx D CeMl SR M CeMl D CbMX SR M CbMX D CbML SR
M CbML D CeLx SR M CeLx D CkLl SR M CkLl D CtLh SR M CtLh D CzLh SR
M CzLh D DCLl SR M DCLl D DILx SR M DILx D DLML SR M DLML D DLMX SR
M DLMX D DIMl SR M DIMl D DCMx SR M DCMx D CzM| SR M CzM| D CtM| SR
M CtM| D CnMx SR M CnMx D CkMt SR M CkMt D ChMl SR M ChMl D CeMX SR
M CeMX D CeML SR M CeML D ChLx SR M ChLx D CkLp SR M CkLp D CnLl SR
M CnLl D CtLh SR M CzLh D D@Ll SR M D@Ll D DCLp SR M DCLp D DFLx SR
M DFLx D DIML SR M DIML D DIMX SR M DIMX D DFMl SR M DFMl D DCMt SR
M DCMt D D@Mx SR M D@Mx D CzM| SR M D[NM D D|NM SR M ELN` D EPNb SR
M EPNb D EUNj SR M EUNj D EUMw SR M ESNg D ESMw SR M ELMw D E]Mw SR
M ByT_ D B?Tc SR M B?Tc D CHTp SR M CHTp D CHS[ SR M CETk D CES[ SR
M ByS[ D CTS[ SR M C?Tp D CvTk SR M CvTk D CpT_ SR M CpT_ D ClTK SR
M ClTK D ClS? SR M ClS? D CpSk SR M CpSk D CvS_ SR M CvS_ D C?S[ SR
M C?S[ D DES[ SR M DES[ D DNS_ SR M DNS_ D DTSk SR M DTSk D DWS? SR
M DWS? D DWTK SR M DWTK D DTT_ SR M DTT_ D DNTk SR M DNTk D DETp SR
M DETp D C?Tp SR M C?Tp D CyTk SR M CyTk D CvTg SR M CvTg D CsT_ SR
M CsT_ D CpTK SR M CpTK D CpS? SR M CpS? D CsSk SR M CsSk D CvSc SR
M CvSc D CyS_ SR M CyS_ D C?S[ SR M DES[ D DKS_ SR M DKS_ D DNSc SR
M DNSc D DQSk SR M DQSk D DTS? SR M DTS? D DTTK SR M DTTK D DQT_ SR
M DQT_ D DNTg SR M DNTg D DKTk SR M DKTk D DETp SR M ERU] D ELUZ SR
M ELUZ D EIUS SR M EIUS D EGUG SR M EGUG D EGU@ SR M EGU@ D EITt SR
M EITt D ELTl SR M ELTl D ERTj SR M ERTj D EUTj SR M EUTj D E[Tl SR
M E[Tl D E^Tt SR M E^Tt D E`U@ SR M E`U@ D E`UG SR M E`UG D E^US SR
M E^US D E[UZ SR M E[UZ D EUU] SR M EUU] D ERU] SR M ERU] D ENUZ SR
M ENUZ D ELUX SR M ELUX D EJUS SR M EJUS D EIUG SR M EIUG D EIU@ SR
M EIU@ D EJTt SR M EJTt D ELTo SR M ELTo D ENTl SR M ENTl D ERTj SR
M EUTj D EYTl SR M EYTl D E[To SR M E[To D E]Tt SR M E]Tt D E^U@ SR
M E^U@ D E^UG SR M E^UG D E]US SR M E]US D E[UX SR M E[UX D EYUZ SR
M EYUZ D EUU] SR M By[S D B?[W SR M B?[W D CH[c SR M CH[c D CHZN SR
M CE[_ D CEZN SR M ByZN D CTZN SR M C?[c D Cv[_ SR M Cv[_ D Cp[S SR
M Cp[S D ClZ~ SR M ClZ~ D ClZr SR M ClZr D CpZ^ SR M CpZ^ D CvZR SR
M CvZR D C?ZN SR M C?ZN D DEZN SR M DEZN D DNZR SR M DNZR D DTZ^ SR
M DTZ^ D DWZr SR M DWZr D DWZ~ SR M DWZ~ D DT[S SR M DT[S D DN[_ SR
M DN[_ D DE[c SR M DE[c D C?[c SR M C?[c D Cy[_ SR M Cy[_ D Cv[[ SR
M Cv[[ D Cs[S SR M Cs[S D CpZ~ SR M CpZ~ D CpZr SR M CpZr D CsZ^ SR
M CsZ^ D CvZV SR M CvZV D CyZR SR M CyZR D C?ZN SR M DEZN D DKZR SR
M DKZR D DNZV SR M DNZV D DQZ^ SR M DQZ^ D DTZr SR M DTZr D DTZ~ SR
M DTZ~ D DQ[S SR M DQ[S D DN[[ SR M DN[[ D DK[_ SR M DK[_ D DE[c SR
M EL\F D EP\I SR M EP\I D EU\P SR M EU\P D EU[] SR M ES\M D ES[] SR
M EL[] D E][] SR M BybF D B?bJ SR M B?bJ D CHbV SR M CHbV D CHaA SR
M CEbR D CEaA SR M ByaA D CTaA SR M C?bV D CvbR SR M CvbR D CpbF SR
M CpbF D Claq SR M Claq D Clae SR M Clae D CpaQ SR M CpaQ D CvaE SR
M CvaE D C?aA SR M C?aA D DEaA SR M DEaA D DNaE SR M DNaE D DTaQ SR
M DTaQ D DWae SR M DWae D DWaq SR M DWaq D DTbF SR M DTbF D DNbR SR
M DNbR D DEbV SR M DEbV D C?bV SR M C?bV D CybR SR M CybR D CvbN SR
M CvbN D CsbF SR M CsbF D Cpaq SR M Cpaq D Cpae SR M Cpae D CsaQ SR
M CsaQ D CvaI SR M CvaI D CyaE SR M CyaE D C?aA SR M DEaA D DKaE SR
M DKaE D DNaI SR M DNaI D DQaQ SR M DQaQ D DTae SR M DTae D DTaq SR
M DTaq D DQbF SR M DQbF D DNbN SR M DNbN D DKbR SR M DKbR D DEbV SR
M EIby D EJbw SR M EJbw D EIbt SR M EIbt D EGbw SR M EGbw D EGby SR
M EGby D EIb~ SR M EIb~ D EJcA SR M EJcA D EPcC SR M EPcC D EWcC SR
M EWcC D E]cA SR M E]cA D E^b~ SR M E^b~ D E`by SR M E`by D E`bt SR
M E`bt D E^bp SR M E^bp D EYbk SR M EYbk D EPbf SR M EPbf D ELbc SR
M ELbc D EIb_ SR M EIb_ D EGbW SR M EGbW D EGbP SR M EWcC D E[cA SR
M E[cA D E]b~ SR M E]b~ D E^by SR M E^by D E^bt SR M E^bt D E]bp SR
M E]bp D EWbk SR M EWbk D EPbf SR M EGbU D EIbW SR M EIbW D ELbW SR
M ELbW D EUbS SR M EUbS D E[bS SR M E[bS D E^bU SR M E^bU D E`bW SR
M ELbW D EUbP SR M EUbP D E]bP SR M E]bP D E^bS SR M E^bS D E`bW SR
M E`bW D E`b\ SR M Byhy D B?h} SR M B?h} D CHiI SR M CHiI D CHgt SR
M CEiE D CEgt SR M Bygt D CTgt SR M C?iI D CviE SR M CviE D Cphy SR
M Cphy D Clhe SR M Clhe D ClhX SR M ClhX D CphD SR M CphD D Cvgx SR
M Cvgx D C?gt SR M C?gt D DEgt SR M DEgt D DNgx SR M DNgx D DThD SR
M DThD D DWhX SR M DWhX D DWhe SR M DWhe D DThy SR M DThy D DNiE SR
M DNiE D DEiI SR M DEiI D C?iI SR M C?iI D CyiE SR M CyiE D CviA SR
M CviA D Cshy SR M Cshy D Cphe SR M Cphe D CphX SR M CphX D CshD SR
M CshD D Cvg| SR M Cvg| D Cygx SR M Cygx D C?gt SR M DEgt D DKgx SR
M DKgx D DNg| SR M DNg| D DQhD SR M DQhD D DThX SR M DThX D DThe SR
M DThe D DQhy SR M DQhy D DNiA SR M DNiA D DKiE SR M DKiE D DEiI SR
M EIio D EJil SR M EJil D EIij SR M EIij D EGil SR M EGil D EGio SR
M EGio D EJit SR M EJit D EPiv SR M EPiv D EWiv SR M EWiv D E]it SR
M E]it D E^io SR M E^io D E^ig SR M E^ig D E]ic SR M E]ic D EWi` SR
M EWi` D ERi` SR M EWiv D E[it SR M E[it D E]io SR M E]io D E]ig SR
M E]ig D E[ic SR M E[ic D EWi` SR M EWi` D E[i^ SR M E[i^ D E^iY SR
M E^iY D E`iT SR M E`iT D E`iM SR M E`iM D E^iH SR M E^iH D E]iF SR
M E]iF D EWiC SR M EWiC D EPiC SR M EPiC D EJiF SR M EJiF D EIiH SR
M EIiH D EGiM SR M EGiM D EGiO SR M EGiO D EIiR SR M EIiR D EJiO SR
M EJiO D EIiM SR M E]i[ D E^iT SR M E^iT D E^iM SR M E^iM D E]iH SR
M E]iH D E[iF SR M E[iF D EWiC SR M Byol D B?op SR M B?op D CHo| SR
M CHo| D CHng SR M CEox D CEng SR M Byng D CTng SR M C?o| D Cvox SR
M Cvox D Cpol SR M Cpol D CloX SR M CloX D CloK SR M CloK D Cpnw SR
M Cpnw D Cvnk SR M Cvnk D C?ng SR M C?ng D DEng SR M DEng D DNnk SR
M DNnk D DTnw SR M DTnw D DWoK SR M DWoK D DWoX SR M DWoX D DTol SR
M DTol D DNox SR M DNox D DEo| SR M DEo| D C?o| SR M C?o| D Cyox SR
M Cyox D Cvot SR M Cvot D Csol SR M Csol D CpoX SR M CpoX D CpoK SR
M CpoK D Csnw SR M Csnw D Cvno SR M Cvno D Cynk SR M Cynk D C?ng SR
M DEng D DKnk SR M DKnk D DNno SR M DNno D DQnw SR M DQnw D DToK SR
M DToK D DToX SR M DToX D DQol SR M DQol D DNot SR M DNot D DKox SR
M DKox D DEo| SR M EWpd D EWov SR M EYpi D EYov SR M EYpi D EEpE SR
M EEpE D EbpE SR M ERov D E^ov SR M Byv_ D B?vc SR M B?vc D CHvo SR
M CHvo D CHuZ SR M CEvk D CEuZ SR M ByuZ D CTuZ SR M C?vo D Cvvk SR
M Cvvk D Cpv_ SR M Cpv_ D ClvK SR M ClvK D Clu? SR M Clu? D Cpuj SR
M Cpuj D Cvu^ SR M Cvu^ D C?uZ SR M C?uZ D DEuZ SR M DEuZ D DNu^ SR
M DNu^ D DTuj SR M DTuj D DWu? SR M DWu? D DWvK SR M DWvK D DTv_ SR
M DTv_ D DNvk SR M DNvk D DEvo SR M DEvo D C?vo SR M C?vo D Cyvk SR
M Cyvk D Cvvg SR M Cvvg D Csv_ SR M Csv_ D CpvK SR M CpvK D Cpu? SR
M Cpu? D Csuj SR M Csuj D Cvub SR M Cvub D Cyu^ SR M Cyu^ D C?uZ SR
M DEuZ D DKu^ SR M DKu^ D DNub SR M DNub D DQuj SR M DQuj D DTu? SR
M DTu? D DTvK SR M DTvK D DQv_ SR M DQv_ D DNvg SR M DNvg D DKvk SR
M DKvk D DEvo SR M EJw\ D EGwD SR M EGwD D EJwF SR M EJwF D EPwI SR
M EPwI D EUwI SR M EUwI D E[wF SR M E[wF D E^wB SR M E^wB D E`vz SR
M E`vz D E`vx SR M E`vx D E^vq SR M E^vq D E[vl SR M E[vl D EUvi SR
M EUvi D EPvi SR M EPvi D EJvl SR M EJvl D EIvn SR M EIvn D EGvs SR
M EGvs D EGvv SR M EGvv D EIvx SR M EIvx D EJvv SR M EJvv D EIvs SR
M EUwI D EYwF SR M EYwF D E]wB SR M E]wB D E^vz SR M E^vz D E^vx SR
M E^vx D E]vq SR M E]vq D EYvl SR M EYvl D EUvi SR M EJw\ D E]w\ SR
M EJwZ D ESwZ SR M ESwZ D E]w\ SR M By}R D B?}V SR M B?}V D CH}b SR
M CH}b D CH|M SR M CE}^ D CE|M SR M By|M D CT|M SR M C?}b D Cv}^ SR
M Cv}^ D Cp}R SR M Cp}R D Cl|~ SR M Cl|~ D Cl|r SR M Cl|r D Cp|^ SR
M Cp|^ D Cv|Q SR M Cv|Q D C?|M SR M C?|M D DE|M SR M DE|M D DN|Q SR
M DN|Q D DT|^ SR M DT|^ D DW|r SR M DW|r D DW|~ SR M DW|~ D DT}R SR
M DT}R D DN}^ SR M DN}^ D DE}b SR M DE}b D C?}b SR M C?}b D Cy}^ SR
M Cy}^ D Cv}Z SR M Cv}Z D Cs}R SR M Cs}R D Cp|~ SR M Cp|~ D Cp|r SR
M Cp|r D Cs|^ SR M Cs|^ D Cv|U SR M Cv|U D Cy|Q SR M Cy|Q D C?|M SR
M DE|M D DK|Q SR M DK|Q D DN|U SR M DN|U D DQ|^ SR M DQ|^ D DT|r SR
M DT|r D DT|~ SR M DT|~ D DQ}R SR M DQ}R D DN}Z SR M DN}Z D DK}^ SR
M DK}^ D DE}b SR M E]~H D E[~F SR M E[~F D E]~C SR M E]~C D E^~F SR
M E^~F D E^~H SR M E^~H D E]~M SR M E]~M D EY~O SR M EY~O D ES~O SR
M ES~O D EN~M SR M EN~M D EJ~H SR M EJ~H D EI~C SR M EI~C D EG}z SR
M EG}z D EG}k SR M EG}k D EI}d SR M EI}d D EL}_ SR M EL}_ D ER}\ SR
M ER}\ D EU}\ SR M EU}\ D E[}_ SR M E[}_ D E^}d SR M E^}d D E`}k SR
M E`}k D E`}m SR M E`}m D E^}u SR M E^}u D E[}z SR M E[}z D EU}| SR
M EU}| D ES}| SR M ES}| D EN}z SR M EN}z D EJ}u SR M EJ}u D EI}m SR
M ES~O D EP~M SR M EP~M D EL~H SR M EL~H D EJ~C SR M EJ~C D EI}z SR
M EI}z D EI}k SR M EI}k D EJ}d SR M EJ}d D EN}_ SR M EN}_ D ER}\ SR
M EU}\ D EY}_ SR M EY}_ D E]}d SR M E]}d D E^}k SR M E^}k D E^}m SR
M E^}m D E]}u SR M E]}u D EY}z SR M EY}z D EU}| SR M |rFY D |r|r SR
M |rFY D |RFY SR M |rFY D {rFY SR M |rH\ D |RH\ SR M |rIh D |RIh SR
M |rJ_ D |RJ_ SR M |rKI D |RKI SR M |rKk D |RKk SR M |rLI D |RLI SR
M |rLb D |RLb SR M |rLx D |RLx SR M |rML D |RML SR M |rML D {rML SR
M |rOO D |ROO SR M |rP\ D |RP\ SR M |rQR D |RQR SR M |rQ| D |RQ| SR
M |rR^ D |RR^ SR M |rR| D |RR| SR M |rSU D |RSU SR M |rSk D |RSk SR
M |rS? D |RS? SR M |rS? D {rS? SR M |rVB D |RVB SR M |rWO D |RWO SR
M |rXE D |RXE SR M |rXo D |RXo SR M |rYR D |RYR SR M |rYo D |RYo SR
M |rZH D |RZH SR M |rZ^ D |RZ^ SR M |rZr D |RZr SR M |rZr D {rZr SR
M |r\u D |R\u SR M |r^B D |R^B SR M |r^x D |R^x SR M |r_b D |R_b SR
M |r`E D |R`E SR M |r`b D |R`b SR M |r`{ D |R`{ SR M |raQ D |RaQ SR
M |rae D |Rae SR M |rae D {rae SR M |rch D |Rch SR M |rdu D |Rdu SR
M |rek D |Rek SR M |rfU D |RfU SR M |rfx D |Rfx SR M |rgU D |RgU SR
M |rgn D |Rgn SR M |rhD D |RhD SR M |rhX D |RhX SR M |rhX D {rhX SR
M |rj[ D |Rj[ SR M |rkh D |Rkh SR M |rl^ D |Rl^ SR M |rmH D |RmH SR
M |rmk D |Rmk SR M |rnH D |RnH SR M |rna D |Rna SR M |rnw D |Rnw SR
M |roK D |RoK SR M |roK D {roK SR M |rqN D |RqN SR M |rr[ D |Rr[ SR
M |rsQ D |RsQ SR M |rs| D |Rs| SR M |rt^ D |Rt^ SR M |rt{ D |Rt{ SR
M |ruT D |RuT SR M |ruk D |Ruk SR M |ru? D |Ru? SR M |ru? D {ru? SR
M |rxA D |RxA SR M |ryN D |RyN SR M |rzD D |RzD SR M |rzo D |Rzo SR
M |r{Q D |R{Q SR M |r{n D |R{n SR M |r|G D |R|G SR M |r|^ D |R|^ SR
M |r|r D |R|r SR M |r|r D {r|r SR
M @^Ub D @dUf SR M @dUf D @TUf SR M @TUf D @^Ub SR M @^Ub D @WUZ SR
M @WUZ D @TUN SR M @TUN D @TUF SR M @TUF D @WTz SR M @WTz D @^Tq SR
M @^Tq D @dTm SR M @dTm D @mTi SR M @mTi D @|Ti SR M @|Ti D AETm SR
M AETm D AKTq SR M AKTq D AQTz SR M AQTz D ATUF SR M ATUF D ATUN SR
M ATUN D AQUZ SR M AQUZ D AKUb SR M AKUb D AEUf SR M @TUF D @WT~ SR
M @WT~ D @^Tv SR M @^Tv D @dTq SR M @dTq D @mTm SR M @mTm D @|Tm SR
M @|Tm D AETq SR M AETq D AKTv SR M AKTv D AQT~ SR M AQT~ D ATUF SR
M @jVV D @mVJ SR M @mVJ D @sVB SR M @sVB D @|U~ SR M @|U~ D ABU~ SR
M ABU~ D AKVB SR M AKVB D AQVJ SR M AQVJ D ATVV SR M ATVV D ATV^ SR
M ATV^ D AQVk SR M AQVk D AKVs SR M AKVs D ABVw SR M ABVw D @|Vw SR
M @|Vw D @sVs SR M @sVs D @mVk SR M @mVk D @jV^ SR M @jV^ D @jVV SR
M @jVV D @mVN SR M @mVN D @sVF SR M @sVF D @|VB SR M @|VB D ABVB SR
M ABVB D AKVF SR M AKVF D AQVN SR M AQVN D ATVV SR M ATV^ D AQVf SR
M AQVf D AKVo SR M AKVo D ABVs SR M ABVs D @|Vs SR M @|Vs D @sVo SR
M @sVo D @mVf SR M @mVf D @jV^ SR M @jWW D AKWW SR M AKWW D AQW[ SR
M AQW[ D ATWg SR M ATWg D ATWo SR M ATWo D AQW{ SR M AQW{ D AKXC SR
M @jW[ D AKW[ SR M AKW[ D AQW_ SR M AQW_ D ATWg SR M @jXC D ATXC SR
M @jXG D ATXG SR M @jWK D @jW[ SR M @jWw D @jXG SR M ATXC D ATXS SR
M @jXp D ATXp SR M @jXt D ATXt SR M @sXt D @mX| SR M @mX| D @jYH SR
M @jYH D @jYP SR M @jYP D @mY\ SR M @mY\ D @sY` SR M @sY` D ATY` SR
M @jYP D @mYX SR M @mYX D @sY\ SR M @sY\ D ATY\ SR M @jXd D @jXt SR
M ATXd D ATY@ SR M ATYP D ATYl SR M @TZH D AHZH SR M AHZH D AQZM SR
M AQZM D ATZU SR M ATZU D ATZ] SR M ATZ] D AQZe SR M AQZe D AKZi SR
M @TZM D AHZM SR M AHZM D AQZQ SR M AQZQ D ATZU SR M @jY| D @jZ] SR
M @T\N D AT\N SR M @T\R D AT\R SR M @T\A D @T\r SR M @T\r D @W\~ SR
M @W\~ D @Z]B SR M @Z]B D @a]F SR M @a]F D @g]F SR M @g]F D @m]B SR
M @m]B D @p\~ SR M @p\~ D @s\r SR M @s\r D @s\R SR M @T\r D @W\z SR
M @W\z D @Z\~ SR M @Z\~ D @a]B SR M @a]B D @g]B SR M @g]B D @m\~ SR
M @m\~ D @p\z SR M @p\z D @s\r SR M AT\A D AT\^ SR M @s\j D AN\z SR
M AN\z D AT]B SR M AT]B D AT]J SR M AT]J D AN]N SR M @s\j D @y\r SR
M @y\r D AT]B SR M @p]f D @s]f SR M @s]f D @s]b SR M @s]b D @p]b SR
M @p]b D @m]f SR M @m]f D @j]n SR M @j]n D @j]? SR M @j]? D @m^G SR
M @m^G D @p^K SR M @p^K D @v^O SR M @v^O D AK^O SR M AK^O D AQ^S SR
M AQ^S D AT^W SR M @p^K D AK^K SR M AK^K D AQ^O SR M AQ^O D AT^W SR
M AT^W D AT^[ SR M @v^K D @y^G SR M @y^G D @|]n SR M @|]n D @?]b SR
M @?]b D AE]^ SR M AE]^ D AK]^ SR M AK]^ D AQ]b SR M AQ]b D AT]n SR
M AT]n D AT]z SR M AT]z D AQ^C SR M AQ^C D AK^K SR M @|]n D @?]f SR
M @?]f D AE]b SR M AE]b D AK]b SR M AK]b D AQ]f SR M AQ]f D AT]n SR
M @T^w D AH^w SR M AH^w D AQ^{ SR M AQ^{ D AT_C SR M AT_C D AT_K SR
M AT_K D AQ_S SR M AQ_S D AK_W SR M @T^{ D AH^{ SR M AH^{ D AQ^? SR
M AQ^? D AT_C SR M @j^k D @j_K SR M @|_p D @|`` SR M @|`` D @v`` SR
M @v`` D @p`\ SR M @p`\ D @m`X SR M @m`X D @j`P SR M @j`P D @j`D SR
M @j`D D @m_x SR M @m_x D @s_p SR M @s_p D @|_k SR M @|_k D AB_k SR
M AB_k D AK_p SR M AK_p D AQ_x SR M AQ_x D AT`D SR M AT`D D AT`L SR
M AT`L D AQ`X SR M AQ`X D AK`` SR M @|`\ D @s`\ SR M @s`\ D @m`X SR
M @j`D D @m_| SR M @m_| D @s_t SR M @s_t D @|_p SR M @|_p D AB_p SR
M AB_p D AK_t SR M AK_t D AQ_| SR M AQ_| D AT`D SR M @Hba D @NbY SR
M @NbY D @WbQ SR M @WbQ D @dbI SR M @dbI D @sbE SR M @sbE D @?bE SR
M @?bE D ANbI SR M ANbI D AZbQ SR M AZbQ D AdbY SR M AdbY D Ajba SR
M @NbY D @ZbQ SR M @ZbQ D @dbM SR M @dbM D @sbI SR M @sbI D @?bI SR
M @?bI D ANbM SR M ANbM D AWbQ SR M AWbQ D AdbY SR M @scj D @vcf SR
M @vcf D @ycj SR M @ycj D @vcn SR M @vcn D @scn SR M @scn D @mcf SR
M @mcf D @jc^ SR M @jc^ D @jcQ SR M @jcQ D @mcE SR M @mcE D @sb} SR
M @sb} D @|by SR M @|by D ABby SR M ABby D AKb} SR M AKb} D AQcE SR
M AQcE D ATcQ SR M ATcQ D ATcZ SR M ATcZ D AQcf SR M AQcf D AKcn SR
M @jcQ D @mcI SR M @mcI D @scA SR M @scA D @|b} SR M @|b} D ABb} SR
M ABb} D AKcA SR M AKcA D AQcI SR M AQcI D ATcQ SR M @jd^ D @mdR SR
M @mdR D @sdJ SR M @sdJ D @|dF SR M @|dF D ABdF SR M ABdF D AKdJ SR
M AKdJ D AQdR SR M AQdR D ATd^ SR M ATd^ D ATdf SR M ATdf D AQdr SR
M AQdr D AKdz SR M AKdz D ABd~ SR M ABd~ D @|d~ SR M @|d~ D @sdz SR
M @sdz D @mdr SR M @mdr D @jdf SR M @jdf D @jd^ SR M @jd^ D @mdV SR
M @mdV D @sdN SR M @sdN D @|dJ SR M @|dJ D ABdJ SR M ABdJ D AKdN SR
M AKdN D AQdV SR M AQdV D ATd^ SR M ATdf D AQdn SR M AQdn D AKdv SR
M AKdv D ABdz SR M ABdz D @|dz SR M @|dz D @sdv SR M @sdv D @mdn SR
M @mdn D @jdf SR M @je_ D AKe_ SR M AKe_ D AQec SR M AQec D ATeo SR
M ATeo D ATew SR M ATew D AQfC SR M AQfC D AKfK SR M @jec D AKec SR
M AKec D AQeg SR M AQeg D ATeo SR M @jfK D ATfK SR M @jfO D ATfO SR
M @jeR D @jec SR M @je? D @jfO SR M ATfK D ATf[ SR M @jfw D ATfw SR
M @jf{ D ATf{ SR M @sf{ D @mgC SR M @mgC D @jgP SR M @jgP D @jgX SR
M @jgX D @mgd SR M @mgd D @sgh SR M @sgh D ATgh SR M @jgX D @mg` SR
M @mg` D @sgd SR M @sgd D ATgd SR M @jfk D @jf{ SR M ATfk D ATgH SR
M ATgX D ATgt SR M @ThP D AHhP SR M AHhP D AQhT SR M AQhT D ATh\ SR
M ATh\ D AThd SR M AThd D AQhl SR M AQhl D AKhp SR M @ThT D AHhT SR
M AHhT D AQhX SR M AQhX D ATh\ SR M @jhD D @jhd SR M @mim D @jiq SR
M @jiq D @siq SR M @siq D @mim SR M @mim D @jia SR M @jia D @jiU SR
M @jiU D @miI SR M @miI D @piE SR M @piE D @siE SR M @siE D @yiI SR
M @yiI D @|iQ SR M @|iQ D ABie SR M ABie D AEim SR M AEim D AHiq SR
M @siE D @viI SR M @viI D @yiQ SR M @yiQ D @?ie SR M @?ie D ABim SR
M ABim D AHiq SR M AHiq D ANiq SR M ANiq D AQim SR M AQim D ATia SR
M ATia D ATiU SR M ATiU D AQiI SR M AQiI D AKiE SR M AKiE D ATiE SR
M ATiE D AQiI SR M @mkz D @jk~ SR M @jk~ D @sk~ SR M @sk~ D @mkz SR
M @mkz D @jkn SR M @jkn D @jkb SR M @jkb D @mkV SR M @mkV D @pkR SR
M @pkR D @skR SR M @skR D @ykV SR M @ykV D @|k^ SR M @|k^ D ABkr SR
M ABkr D AEkz SR M AEkz D AHk~ SR M @skR D @vkV SR M @vkV D @yk^ SR
M @yk^ D @?kr SR M @?kr D ABkz SR M ABkz D AHk~ SR M AHk~ D ANk~ SR
M ANk~ D AQkz SR M AQkz D ATkn SR M ATkn D ATkb SR M ATkb D AQkV SR
M AQkV D AKkR SR M AKkR D ATkR SR M ATkR D AQkV SR M @HlR D @Hl} SR
M @@mS D @@mX SR M @@mX D @@m_ SR M @@m_ D @Ym_ SR M @@m] D @Ym] SR
M @YmS D @Ymi SR M @HnA D @NnI SR M @NnI D @WnQ SR M @WnQ D @dnY SR
M @dnY D @sn] SR M @sn] D @?n] SR M @?n] D ANnY SR M ANnY D AZnQ SR
M AZnQ D AdnI SR M AdnI D AjnA SR M @NnI D @ZnQ SR M @ZnQ D @dnU SR
M @dnU D @snY SR M @snY D @?nY SR M @?nY D ANnU SR M ANnU D AWnQ SR
M AWnQ D AdnI SR
M _bBo D _\Bg SR M _\Bg D _VB[ SR M _VB[ D _PBK SR M _PBK D _MAw SR
M _MAw D _MAg SR M _MAg D _PAR SR M _PAR D _VAB SR M _VAB D _\@v SR
M _\@v D _b@n SR M _\Bg D _VBW SR M _VBW D _SBK SR M _SBK D _PAw SR
M _PAw D _PAg SR M _PAg D _SAR SR M _SAR D _VAF SR M _VAF D _\@v SR
M _{B_ D _{AJ SR M _~B_ D _~AJ SR M _rB_ D `VB_ SR M `VB_ D `_B[ SR
M `_B[ D `bBW SR M `bBW D `eBO SR M `eBO D `eBG SR M `eBG D `bA? SR
M `bA? D `_A{ SR M `_A{ D `VAw SR M `VB_ D `\B[ SR M `\B[ D `_BW SR
M `_BW D `bBO SR M `bBO D `bBG SR M `bBG D `_A? SR M `_A? D `\A{ SR
M `\A{ D `VAw SR M _~Aw D `VAw SR M `VAw D `_As SR M `_As D `bAo SR
M `bAo D `eAg SR M `eAg D `eAZ SR M `eAZ D `bAR SR M `bAR D `_AN SR
M `_AN D `VAJ SR M `VAJ D _rAJ SR M `VAw D `\As SR M `\As D `_Ao SR
M `_Ao D `bAg SR M `bAg D `bAZ SR M `bAZ D `_AR SR M `_AR D `\AN SR
M `\AN D `VAJ SR M `xAo D anAo SR M bDB_ D bYAJ SR M bGB_ D bYAV SR
M bnB_ D bYAJ SR M a{B_ D bPB_ SR M beB_ D bxB_ SR M cDBo D cJBg SR
M cJBg D cPB[ SR M cPB[ D cVBK SR M cVBK D cYAw SR M cYAw D cYAg SR
M cYAg D cVAR SR M cVAR D cPAB SR M cPAB D cJ@v SR M cJ@v D cD@n SR
M cJBg D cPBW SR M cPBW D cSBK SR M cSBK D cVAw SR M cVAw D cVAg SR
M cVAg D cSAR SR M cSAR D cPAF SR M cPAF D cJ@v SR M cvAe D cpAb SR
M cpAb D cmA[ SR M cmA[ D ckAO SR M ckAO D ckAH SR M ckAH D cm@| SR
M cm@| D cp@t SR M cp@t D cv@r SR M cv@r D cy@r SR M cy@r D c?@t SR
M c?@t D dC@| SR M dC@| D dDAH SR M dDAH D dDAO SR M dDAO D dCA[ SR
M dCA[ D c?Ab SR M c?Ab D cyAe SR M cyAe D cvAe SR M cvAe D crAb SR
M crAb D cpA` SR M cpA` D cnA[ SR M cnA[ D cmAO SR M cmAO D cmAH SR
M cmAH D cn@| SR M cn@| D cp@w SR M cp@w D cr@t SR M cr@t D cv@r SR
M cy@r D c}@t SR M c}@t D c?@w SR M c?@w D dA@| SR M dA@| D dCAH SR
M dCAH D dCAO SR M dCAO D dAA[ SR M dAA[ D c?A` SR M c?A` D c}Ab SR
M c}Ab D cyAe SR
M mtpF D mZn` SR M mtpF D nMn` SR M mtow D nJn` SR M mbnx D nFnx SR
M mOn` D men` SR M m?n` D nXn` SR M nnor D nvow SR M nvow D o@pF SR
M o@pF D o@n` SR M n}pA D n}n` SR M nnn` D oOn` SR
M HUxr D JQwi D LNv^ D NJuQ D PFtB D RCrq D S?q^ D U{pJ D Wxns D YtmZ
D [pk? D ]mjc D _iiD D aegc D cbf@ D e^d\ D gZbu D iVaL D kS_b D mO]u
D oK\G D qHZV D sDXc D u@Vo D v}Tx SR
M yOU^ D yHU[ SR M yHU[ D yCUQ SR M yCUQ D y@UA SR M y@UA D y@Tx SR
M y@Tx D yCTh SR M yCTh D yHT^ SR M yHT^ D yOT[ SR M yOT[ D yTT[ SR
M yTT[ D y[T^ SR M y[T^ D y`Th SR M y`Th D ybTx SR M ybTx D ybUA SR
M ybUA D y`UQ SR M y`UQ D y[U[ SR M y[U[ D yTU^ SR M yTU^ D yOU^ SR
M yOU^ D yJU[ SR M yJU[ D yHUX SR M yHUX D yEUQ SR M yEUQ D yCUA SR
M yCUA D yCTx SR M yCTx D yETh SR M yETh D yHTa SR M yHTa D yJT^ SR
M yJT^ D yOT[ SR M yTT[ D yYT^ SR M yYT^ D y[Ta SR M y[Ta D y^Th SR
M y^Th D y`Tx SR M y`Tx D y`UA SR M y`UA D y^UQ SR M y^UQ D y[UX SR
M y[UX D yYU[ SR M yYU[ D yTU^ SR M ytTa D yqT^ SR M yqT^ D ytT[ SR
M ytT[ D yvT^ SR M yvT^ D ytTa SR M zSU^ D zLU[ SR M zLU[ D zGUQ SR
M zGUQ D zEUA SR M zEUA D zETx SR M zETx D zGTh SR M zGTh D zLT^ SR
M zLT^ D zST[ SR M zST[ D zXT[ SR M zXT[ D z_T^ SR M z_T^ D zdTh SR
M zdTh D zgTx SR M zgTx D zgUA SR M zgUA D zdUQ SR M zdUQ D z_U[ SR
M z_U[ D zXU^ SR M zXU^ D zSU^ SR M zSU^ D zNU[ SR M zNU[ D zLUX SR
M zLUX D zIUQ SR M zIUQ D zGUA SR M zGUA D zGTx SR M zGTx D zITh SR
M zITh D zLTa SR M zLTa D zNT^ SR M zNT^ D zST[ SR M zXT[ D z]T^ SR
M z]T^ D z_Ta SR M z_Ta D zbTh SR M zbTh D zdTx SR M zdTx D zdUA SR
M zdUA D zbUQ SR M zbUQ D z_UX SR M z_UX D z]U[ SR M z]U[ D zXU^ SR
M HUvi D JQu` D LNtU D NJsH D PFqz D RCpi D S?oV D U{nA D Wxlj D YtkQ
D [piw D ]mhZ D _if{ D aeeZ D cbcx D e^bS D gZ`l D iV_C D kS]Y D mO[l
D oKY~ D qHXM D sDVZ D u@Tf D v}Ro SR
M yOSW D yHST SR M yHST D yCSK SR M yCSK D y@Rz SR M y@Rz D y@Rq SR
M y@Rq D yCRa SR M yCRa D yHRW SR M yHRW D yORT SR M yORT D yTRT SR
M yTRT D y[RW SR M y[RW D y`Ra SR M y`Ra D ybRq SR M ybRq D ybRz SR
M ybRz D y`SK SR M y`SK D y[ST SR M y[ST D yTSW SR M yTSW D yOSW SR
M yOSW D yJST SR M yJST D yHSQ SR M yHSQ D yESK SR M yESK D yCRz SR
M yCRz D yCRq SR M yCRq D yERa SR M yERa D yHRZ SR M yHRZ D yJRW SR
M yJRW D yORT SR M yTRT D yYRW SR M yYRW D y[RZ SR M y[RZ D y^Ra SR
M y^Ra D y`Rq SR M y`Rq D y`Rz SR M y`Rz D y^SK SR M y^SK D y[SQ SR
M y[SQ D yYST SR M yYST D yTSW SR M ytRZ D yqRW SR M yqRW D ytRT SR
M ytRT D yvRW SR M yvRW D ytRZ SR M zLSK D zQSN SR M zQSN D zXSW SR
M zXSW D zXRT SR M zVST D zVRT SR M zLRT D zbRT SR
M HUta D JQsX D LNrM D NJq@ D PFoq D RCn` D S?mM D U{kx D Wxja D YtiI
D [pgn D ]mfQ D _idr D aecQ D cbao D e^`J D gZ^c D iV\z D kS[P D mOYc
D oKWu D qHVD D sDTQ D u@R] D v}Pf SR
M yOQQ D yHQM SR M yHQM D yCQD SR M yCQD D y@Pt SR M y@Pt D y@Pj SR
M y@Pj D yCPZ SR M yCPZ D yHPP SR M yHPP D yOPM SR M yOPM D yTPM SR
M yTPM D y[PP SR M y[PP D y`PZ SR M y`PZ D ybPj SR M ybPj D ybPt SR
M ybPt D y`QD SR M y`QD D y[QM SR M y[QM D yTQQ SR M yTQQ D yOQQ SR
M yOQQ D yJQM SR M yJQM D yHQJ SR M yHQJ D yEQD SR M yEQD D yCPt SR
M yCPt D yCPj SR M yCPj D yEPZ SR M yEPZ D yHPS SR M yHPS D yJPP SR
M yJPP D yOPM SR M yTPM D yYPP SR M yYPP D y[PS SR M y[PS D y^PZ SR
M y^PZ D y`Pj SR M y`Pj D y`Pt SR M y`Pt D y^QD SR M y^QD D y[QJ SR
M y[QJ D yYQM SR M yYQM D yTQQ SR M ytPS D yqPP SR M yqPP D ytPM SR
M ytPM D yvPP SR M yvPP D ytPS SR M zGQD D zIQA SR M zIQA D zGP} SR
M zGP} D zEQA SR M zEQA D zEQD SR M zEQD D zGQJ SR M zGQJ D zIQM SR
M zIQM D zQQQ SR M zQQQ D z[QQ SR M z[QQ D zbQM SR M zbQM D zdQJ SR
M zdQJ D zgQD SR M zgQD D zgP} SR M zgP} D zdPw SR M zdPw D z]Pp SR
M z]Pp D zQPj SR M zQPj D zLPg SR M zLPg D zGP` SR M zGP` D zEPW SR
M zEPW D zEPM SR M z[QQ D z_QM SR M z_QM D zbQJ SR M zbQJ D zdQD SR
M zdQD D zdP} SR M zdP} D zbPw SR M zbPw D z[Pp SR M z[Pp D zQPj SR
M zEPS D zGPW SR M zGPW D zLPW SR M zLPW D zXPP SR M zXPP D z_PP SR
M z_PP D zdPS SR M zdPS D zgPW SR M zLPW D zXPM SR M zXPM D zbPM SR
M zbPM D zdPP SR M zdPP D zgPW SR M zgPW D zgP] SR
M HUrY D JQqO D LNpD D NJnw D PFmi D RClX D S?kE D U{ip D WxhY D Ytg@
D [pee D ]mdH D _ibi D aeaI D cb_f D e^^A D gZ\Z D iVZr D kSYG D mOWZ
D oKUk D qHS{ D sDRH D u@PT D v}N] SR
M yOOE D yHOB SR M yHOB D yCNy SR M yCNy D y@Nh SR M y@Nh D y@N_ SR
M y@N_ D yCNO SR M yCNO D yHNE SR M yHNE D yONB SR M yONB D yTNB SR
M yTNB D y[NE SR M y[NE D y`NO SR M y`NO D ybN_ SR M ybN_ D ybNh SR
M ybNh D y`Ny SR M y`Ny D y[OB SR M y[OB D yTOE SR M yTOE D yOOE SR
M yOOE D yJOB SR M yJOB D yHN? SR M yHN? D yENy SR M yENy D yCNh SR
M yCNh D yCN_ SR M yCN_ D yENO SR M yENO D yHNH SR M yHNH D yJNE SR
M yJNE D yONB SR M yTNB D yYNE SR M yYNE D y[NH SR M y[NH D y^NO SR
M y^NO D y`N_ SR M y`N_ D y`Nh SR M y`Nh D y^Ny SR M y^Ny D y[N? SR
M y[N? D yYOB SR M yYOB D yTOE SR M ytNH D yqNE SR M yqNE D ytNB SR
M ytNB D yvNE SR M yvNE D ytNH SR M zGN| D zINy SR M zINy D zGNu SR
M zGNu D zENy SR M zENy D zEN| SR M zEN| D zIOB SR M zIOB D zQOE SR
M zQOE D z[OE SR M z[OE D zbOB SR M zbOB D zdN| SR M zdN| D zdNr SR
M zdNr D zbNl SR M zbNl D z[Nh SR M z[Nh D zSNh SR M z[OE D z_OB SR
M z_OB D zbN| SR M zbN| D zbNr SR M zbNr D z_Nl SR M z_Nl D z[Nh SR
M z[Nh D z_Ne SR M z_Ne D zdN_ SR M zdN_ D zgNX SR M zgNX D zgNO SR
M zgNO D zdNH SR M zdNH D zbNE SR M zbNE D z[NB SR M z[NB D zQNB SR
M zQNB D zINE SR M zINE D zGNH SR M zGNH D zENO SR M zENO D zENR SR
M zENR D zGNU SR M zGNU D zINR SR M zINR D zGNO SR M zbNb D zdNX SR
M zdNX D zdNO SR M zdNO D zbNH SR M zbNH D z_NE SR M z_NE D z[NB SR
M HUpP D JQoG D LNm| D NJlo D PFk` D RCjO D S?h| D U{gg D WxfP D Ytdw
D [pc\ D ]ma? D _i`a D ae_@ D cb]] D e^[x D gZZQ D iVXi D kSV~ D mOUQ
D oKSb D qHQr D sDO? D u@NK D v}LT SR
M yOLz D yHLw SR M yHLw D yCLm SR M yCLm D y@L] SR M y@L] D y@LS SR
M y@LS D yCLC SR M yCLC D yHKz SR M yHKz D yOKv SR M yOKv D yTKv SR
M yTKv D y[Kz SR M y[Kz D y`LC SR M y`LC D ybLS SR M ybLS D ybL] SR
M ybL] D y`Lm SR M y`Lm D y[Lw SR M y[Lw D yTLz SR M yTLz D yOLz SR
M yOLz D yJLw SR M yJLw D yHLt SR M yHLt D yELm SR M yELm D yCL] SR
M yCL] D yCLS SR M yCLS D yELC SR M yELC D yHK} SR M yHK} D yJKz SR
M yJKz D yOKv SR M yTKv D yYKz SR M yYKz D y[K} SR M y[K} D y^LC SR
M y^LC D y`LS SR M y`LS D y`L] SR M y`L] D y^Lm SR M y^Lm D y[Lt SR
M y[Lt D yYLw SR M yYLw D yTLz SR M ytK} D yqKz SR M yqKz D ytKv SR
M ytKv D yvKz SR M yvKz D ytK} SR M z[Lt D z[Kv SR M z]Lz D z]Kv SR
M z]Lz D zBLJ SR M zBLJ D ziLJ SR M zSKv D zdKv SR
M HUnH D JQl? D LNkt D NJjg D PFiX D RChF D S?fs D U{e^ D WxdH D Ytbo
D [paT D ]m_w D _i^X D ae\w D cb[T D e^Yo D gZXI D iVV` D kSTu D mOSH
D oKQZ D qHOi D sDMv D u@LB D v}JK SR
M yOJs D yHJp SR M yHJp D yCJf SR M yCJf D y@JV SR M y@JV D y@JM SR
M y@JM D yCI| SR M yCI| D yHIs SR M yHIs D yOIo SR M yOIo D yTIo SR
M yTIo D y[Is SR M y[Is D y`I| SR M y`I| D ybJM SR M ybJM D ybJV SR
M ybJV D y`Jf SR M y`Jf D y[Jp SR M y[Jp D yTJs SR M yTJs D yOJs SR
M yOJs D yJJp SR M yJJp D yHJm SR M yHJm D yEJf SR M yEJf D yCJV SR
M yCJV D yCJM SR M yCJM D yEI| SR M yEI| D yHIv SR M yHIv D yJIs SR
M yJIs D yOIo SR M yTIo D yYIs SR M yYIs D y[Iv SR M y[Iv D y^I| SR
M y^I| D y`JM SR M y`JM D y`JV SR M y`JV D y^Jf SR M y^Jf D y[Jm SR
M y[Jm D yYJp SR M yYJp D yTJs SR M ytIv D yqIs SR M yqIs D ytIo SR
M ytIo D yvIs SR M yvIs D ytIv SR M zIJs D zEJS SR M zEJS D zIJV SR
M zIJV D zQJY SR M zQJY D zXJY SR M zXJY D z_JV SR M z_JV D zdJP SR
M zdJP D zgJF SR M zgJF D zgJC SR M zgJC D zdIy SR M zdIy D z_Is SR
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M zGIv D zEI| SR M zEI| D zEJ@ SR M zEJ@ D zGJC SR M zGJC D zIJ@ SR
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M zdJF D zdJC SR M zdJC D zbIy SR M zbIy D z]Is SR M z]Is D zXIo SR
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%PSKCloseWorkStation
%PSKOpenWorkStation
CL
%%Trailer
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%DocumentFonts: Times-Bold Times-Italic Symbol Times-Roman
%%Pages: 1
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%%EndDocument
FMENDEPSF
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%%BeginDocument: /pongo/data2/drs/ghrs/handbook/ih5/figs/mirror_n1.epsi
%!PS-Adobe-2.0 EPSF-1.2
%%BoundingBox: 56 29 576 730
%!PS-Adobe-1.0
%%Creator: PSIKern - An IRAF GKI Translator
%%CreationDate: Thu 15:33:07 28-Apr-94
%%DocumentFonts: (atend)
%%Pages: (atend)
%%BoundingBox: 28 28 583 763
%%EndComments
/MAXNDC 4095 def /PageSizeXMeter 0.2594 def /PageSizeYMeter 0.1959 def
/PageOffXMeter 0.01 def /PageOffYMeter 0.01 def
/PortraitMode false def /PortraitRotation 0. def
/LandScapeRotation 90. def /GT_LEFT 2 def /GT_RIGHT 3 def
/GT_TOP 6 def /GT_BOTTOM 7 def /GT_UP 4 def /GT_DOWN 5 def
/GT_CENTER 1 def /RF /Times-Roman def /GF /Symbol def
/IF /Times-Italic def /BF /Times-Bold def /DASH 49 def /DOT 4 def
/SPACE 24 def

% How to define things.
/BD { bind def } bind def
/LD { load def } bind def

% Constants
/yes true def
/no false def

% Define some shorthand instructions.
/GRS /grestore LD
/GS /gsave LD
/MK /mark LD
/R /restore LD
/S /save LD
/SH /showpage LD
/SW /setlinewidth LD

% Measurement conversions.
/PointperMeter 2834.64 def
/MonoScale .7 def

% SR: Set current path to page: - -> -
/SR { currentpoint stroke moveto } BD

% CL: CLear the page: - -> -
/CL { restore showpage grestore gsave save } BD

% RC: Read Coordinates: string -> x y
/RC {
currentfile read pop 8#77 and 6 bitshift
currentfile read pop 8#77 and or
currentfile read pop 8#77 and 6 bitshift
currentfile read pop 8#77 and or
} BD

% DO - Determine Offset: length -> offset
/DO { DS dup 0 eq { pop pop 0 } { mod } ifelse } BD

% M: Move: M string -> -
% Move to a point and clear length of path.
/M { RC moveto CT OF setdash } BD

% D: Draw: D string -> -
% This also calculates the length of the current path.
/OF 0 def
/D { RC DS 0 ne { 2 copy currentpoint exch 4 1 roll sub dup mul 3 1 roll
sub dup mul add sqrt round OF add cvi DO /OF exch store } if lineto
} BD

% Character/Font definitions.

% FS -- Define the current font size: xsize ysize FS -
/FontXSize 0 def /FontYSize 0 def /NewFont true def
/FS { /FontYSize exch MonoScale mul store /FontXSize exch MonoScale mul store
/NewFont true store } BD

% PH -- Set the current path: path PH -
/Path 0 def
/PH { /Path exch store } BD

% PA -- Set the path angle of the text: angle PA -
/Angle 0 def
/PA { 360 mod dup 0 lt { 360 add } if /Angle exch store /NewFont true store } BD

% HJ, VJ -- Set Horizontal/Verticle Justification: just HJ/VJ -
/HorzJust 0 def /VertJust 0 def
/HJ { /HorzJust exch store } BD /VJ { /VertJust exch store } BD

% VT -- Use mono- or variable-spaced fonts: flag VT -
/VT true def
/VT { /Variable exch store } BD

% SetFont -- Make the required font the default: font SetFont -
% Note scale factor- This is to fill out monospaced better and match other
% IRAF output.
/Font () def
/FontMatrix matrix def
/SetFont {
dup Font ne NewFont or
{ dup /Font exch store findfont
Angle matrix rotate FontXSize MonoScale div FontYSize MonoScale div
matrix scale matrix concatmatrix makefont setfont Angle matrix rotate
FontXSize FontYSize matrix scale matrix concatmatrix /FontMatrix exch
store
}
{ pop } ifelse /NewFont false store
} BD

% StringWidth -- Determine path length of string: string StringWidth - xs ys
/StringWidth { Path GT_RIGHT eq Variable and { stringwidth }
{ Path GT_RIGHT eq { length } { pop 1 } ifelse 0 FontMatrix transform }
ifelse
} BD

% MonoShow -- Write the string out in mono-spaced: string MonoShow -
/MonoShow {
/t 1 string def 1 0 FontMatrix transform
/dy exch def /dx exch def Path GT_RIGHT eq { /mx dx def /my dy def }
{ 0 1 FontMatrix transform /my exch def /mx exch def } ifelse
{ t 0 3 -1 roll put t dup stringwidth dy exch sub 2 div exch dx exch
sub 2 div exch gsave rmoveto show grestore mx my rmoveto
} forall
} BD

% WS -- Draw the string: string font string ... DS -
/*WSDict 13 dict def
/WS { *WSDict begin
counttomark 2 idiv dup dup array /FontArray exch def
array /StringArray exch def 1 sub /NStrings exch def

NStrings -1 0 {
dup 4 1 roll exch StringArray 3 1 roll put FontArray 3 1 roll put
} for
pop

/XSize 0 def /YSize 0 def /NChars 0 def
0 1 NStrings {
dup FontArray exch get SetFont StringArray exch get dup
length NChars add /NChars exch def StringWidth
YSize add /YSize exch def XSize add /XSize exch def
} for

/TAngle HorzJust GT_RIGHT eq
{ Angle 180 add dup 360 ge { 360 sub } if } { Angle } ifelse def
0 TAngle 180 le HorzJust GT_CENTER eq or
{ Angle sin FontYSize mul Path GT_UP eq { NChars mul } if add } if
TAngle 90 ge TAngle 270 le and HorzJust GT_CENTER eq or
{ Path GT_RIGHT eq { XSize } { Angle cos FontXSize mul } ifelse sub } if
HorzJust GT_CENTER eq { .5 mul } if

/TAngle
VertJust GT_TOP eq { Angle 180 sub dup 0 lt { 360 add } if } { Angle } ifelse
def
0 TAngle 90 ge TAngle 270 le and VertJust GT_CENTER eq or
{ Angle cos FontYSize mul Path GT_UP eq { NChars mul } if sub } if
TAngle 180 ge TAngle 360 le and VertJust GT_CENTER eq or
{ Path GT_RIGHT eq { YSize } { Angle sin FontXSize mul } ifelse sub } if
VertJust GT_CENTER eq { .5 mul } if
rmoveto

0 1 NStrings {
dup FontArray exch get SetFont StringArray exch get
Path GT_RIGHT eq Variable and { show } { MonoShow } ifelse
} for

end
} BD

% Define the DASHED, DOTTED, DOTDASH patterns.
/DS 0 def
/LPS {
/OF 0 store /DS 0 store 0 array
} BD
/LPD {
/OF 0 store DASH SPACE 2 copy add /DS exch store 2 array astore
} BD
/LPP {
/OF 0 store DOT SPACE 2 copy add /DS exch store 2 array astore
} BD
/LDD {
/OF 0 store DOT SPACE DASH SPACE 4 copy add add add /DS exch store
4 array astore
} BD

% LT - Set Line Type - array -> -
/CT { currentdash pop } BD
/LT { /CT exch store /OF 0 store } BD

% SC - Set Color: color -> -
/*SCDict 1 dict def
/SC { *SCDict begin
1 sub /color exch def
GR color get 255 div GG color get 255 div GB color get 255 div setrgbcolor
end
} BD

% MI - Make Image LUT: table-name size MI hexstring -> -
/MI { currentfile exch string readhexstring pop def } BD

% Define the graphics color lookup table.
/GR 16 MI 00FFFF0000FF00FFFFB0FFF0D940F0F5
/GG 16 MI 00FF00FF00FFFF0080D0A6E670E082DE
/GB 16 MI 00FF0000FF00FFFF4F61008CD6D1EFB3

% Render an image when no image LUT has been define.
/DefaultGrey {
{ currentfile inarr readhexstring pop } image
} BD

% ColorImage - Produce an image by indexing into the Image Lookup Table.
% There are two versions of this code- one for PostScript that has
% the colorimage operator and one that doesn't. If the PostScript doesn't
% have colorimage, it is assumed that it can only produce black & white,
% in which the Image LUT is combined to produce a single grey which is
% then used as the image for the image operator.
/colorimage where
{ pop
/ColorImage {
{ currentfile inarr readhexstring pop dup /inarr exch def
length 3 mul string /oarr exch def
0 1 inarr length 1 sub
{ /iindex exch def
/oindex iindex 3 mul def
oarr oindex IR inarr iindex get get put
oarr oindex 1 add IG inarr iindex get get put
oarr oindex 2 add IB inarr iindex get get put
} for
oarr
}
false 3 colorimage
} BD
}
{ /ColorImage {
{ currentfile inarr readhexstring pop dup /inarr exch def
length string /oarr exch def
0 1 inarr length 1 sub
{ /iindex exch def
oarr iindex
IR inarr iindex get get 0.3 mul
IG inarr iindex get get 0.59 mul
IB inarr iindex get get 0.11 mul
add add round cvi dup 255 gt { pop 255 } if
put
} for
oarr
}
image
} BD
}
ifelse

% PC: Put Cellarray: width height bitspersample matrix -> -
/*PCdict 10 dict def
/PC {
*PCdict begin
4 -1 roll dup /inarr exch string def 4 1 roll
/IR where {pop ColorImage} {DefaultGrey} ifelse
end
} BD

% Define the Hatch (fill area) styles. H1 and H2 are handled internally
% by PSIKern. Feel free to define more; there is no limit.
/H3 <8888888888888888> def
/H4 def
/H5 <8844221188442211> def
/H6 <1122448811224488> def

% Setup for fill patterns. This whole section of code is taken almost
% directly from _PostScript Language: Tutorial and Cookbook_, Adobe Systems,
% 1986 (the blue book).
/setuserscreendict 22 dict def
setuserscreendict begin
/tempctm matrix def
/temprot matrix def
/tempscale matrix def

/concatprocs
{ /proc2 exch cvlit def
/proc1 exch cvlit def
/newproc proc1 length proc2 length add
array def
newproc 0 proc1 putinterval
newproc proc1 length proc2 putinterval
newproc cvx
} def

/resmatrix matrix def
/findresolution
{ 72 0 resmatrix defaultmatrix dtransform
/yres exch def /xres exch def
xres dup mul yres dup mul add sqrt
} def
end

/setuserscreen
{ setuserscreendict begin
/spotfunction exch def
/screenangle exch def
/cellsize exch def

/m tempctm currentmatrix def
/rm screenangle temprot rotate def
/sm cellsize dup tempscale scale def

sm rm m m concatmatrix m concatmatrix pop
1 0 m dtransform /y1 exch def /x1 exch def

/veclength x1 dup mul y1 dup mul add sqrt def
/frequency findresolution veclength div def

/newscreenangle y1 x1 atan def

m 2 get m 1 get mul m 0 get m 3 get mul sub
0 gt
{ {neg} /spotfunction load concatprocs
/spotfunction exch def
} if

frequency newscreenangle /spotfunction load
setscreen
end
} def

/setpatterndict 18 dict def
setpatterndict begin
/bitison
{ /ybit exch def /xbit exch def
/bytevalue bstring ybit bwidth mul xbit 8 idiv
add get def

/mask 1 7 xbit 8 mod sub bitshift def
bytevalue mask and 0 ne
} def
end

/bitpatternspotfunction
{ setpatterndict begin
/y exch def /x exch def

/xindex x 1 add 2 div bpside mul cvi def
/yindex y 1 add 2 div bpside mul cvi def

xindex yindex bitison
{ /onbits onbits 1 add def 1 }
{ /offbits offbits 1 add def 0 }
ifelse
end
} def

/setpattern
{ setpatterndict begin
/cellsz exch def
/angle exch def
/bwidth exch def
/bpside exch def
/bstring exch def

/onbits 0 def /offbits 0 def
cellsz angle /bitpatternspotfunction load
setuserscreen
{ } settransfer
offbits offbits onbits add div setgray
end
} def

% SP: Set Pattern: pattern -> -
/SP { 8 1 0 MAXNDC 100 div setpattern } BD

% FI: Fill with Pattern: - -> -
/FI { fill grestore } BD

% Set the transformation matrix.
PointperMeter dup scale
PageOffXMeter
PortraitMode not
{ PageSizeYMeter add }
if
PageOffYMeter translate
PortraitMode
{ PortraitRotation rotate }
{ LandScapeRotation rotate}
ifelse
PageSizeXMeter MAXNDC div PageSizeYMeter MAXNDC div scale
1 setlinejoin 1 setlinecap

% Save the current graphics state (to restore after showpage) and the
% VM state to recover after a showpage.
GS S

%%EndProlog
%PSKOpenWorkStation
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M NPEd D NMEh SR M NMEh D NGEl SR M NoD_ D NlD[ SR M NlD[ D NoDW SR
M NoDW D NrD[ SR M NrD[ D NoD_ SR M OGE\ D OJEX SR M OJEX D OGET SR
M OGET D ODEX SR M ODEX D ODE\ SR M ODE\ D OGEd SR M OGEd D OJEh SR
M OJEh D OSEl SR M OSEl D O`El SR M O`El D OiEh SR M OiEh D OlEd SR
M OlEd D OoE\ SR M OoE\ D OoET SR M OoET D OlEL SR M OlEL D OcEC SR
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M ODDc D ODDW SR M O`El D OfEh SR M OfEh D OiEd SR M OiEd D OlE\ SR
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M ODD_ D OGDc SR M OGDc D OMDc SR M OMDc D O\D[ SR M O\D[ D OfD[ SR
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M OiDW D OlD[ SR M OlD[ D OoDc SR M OoDc D OoDk SR M UxEl D UoEh SR
M UoEh D UiE\ SR M UiE\ D UfEG SR M UfEG D UfD{ SR M UfD{ D UiDg SR
M UiDg D UoD[ SR M UoD[ D UxDW SR M UxDW D U~DW SR M U~DW D VHD[ SR
M VHD[ D VNDg SR M VNDg D VQD{ SR M VQD{ D VQEG SR M VQEG D VNE\ SR
M VNE\ D VHEh SR M VHEh D U~El SR M U~El D UxEl SR M UxEl D UrEh SR
M UrEh D UoEd SR M UoEd D UlE\ SR M UlE\ D UiEG SR M UiEG D UiD{ SR
M UiD{ D UlDg SR M UlDg D UoD_ SR M UoD_ D UrD[ SR M UrD[ D UxDW SR
M U~DW D VED[ SR M VED[ D VHD_ SR M VHD_ D VKDg SR M VKDg D VND{ SR
M VND{ D VNEG SR M VNEG D VKE\ SR M VKE\ D VHEd SR M VHEd D VEEh SR
M VEEh D U~El SR M \?El D \vEh SR M \vEh D \pE\ SR M \pE\ D \mEG SR
M \mEG D \mD{ SR M \mD{ D \pDg SR M \pDg D \vD[ SR M \vD[ D \?DW SR
M \?DW D ]EDW SR M ]EDW D ]ND[ SR M ]ND[ D ]TDg SR M ]TDg D ]WD{ SR
M ]WD{ D ]WEG SR M ]WEG D ]TE\ SR M ]TE\ D ]NEh SR M ]NEh D ]EEl SR
M ]EEl D \?El SR M \?El D \yEh SR M \yEh D \vEd SR M \vEd D \sE\ SR
M \sE\ D \pEG SR M \pEG D \pD{ SR M \pD{ D \sDg SR M \sDg D \vD_ SR
M \vD_ D \yD[ SR M \yD[ D \?DW SR M ]EDW D ]KD[ SR M ]KD[ D ]ND_ SR
M ]ND_ D ]QDg SR M ]QDg D ]TD{ SR M ]TD{ D ]TEG SR M ]TEG D ]QE\ SR
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M thD{ D thEG SR M thEG D teE\ SR M teE\ D tbEd SR M tbEd D t_Eh SR
M t_Eh D tYEl SR M u@D_ D t}D[ SR M t}D[ D u@DW SR M u@DW D uDD[ SR
M uDD[ D u@D_ SR M ueEl D u\Eh SR M u\Eh D uYE` SR M uYE` D uYET SR
M uYET D u\EL SR M u\EL D ueEG SR M ueEG D uqEG SR M uqEG D uzEL SR
M uzEL D u}ET SR M u}ET D u}E` SR M u}E` D uzEh SR M uzEh D uqEl SR
M uqEl D ueEl SR M ueEl D u_Eh SR M u_Eh D u\E` SR M u\E` D u\ET SR
M u\ET D u_EL SR M u_EL D ueEG SR M uqEG D uwEL SR M uwEL D uzET SR
M uzET D uzE` SR M uzE` D uwEh SR M uwEh D uqEl SR M ueEG D u\EC SR
M u\EC D uYD? SR M uYD? D uVDw SR M uVDw D uVDg SR M uVDg D uYD_ SR
M uYD_ D u\D[ SR M u\D[ D ueDW SR M ueDW D uqDW SR M uqDW D uzD[ SR
M uzD[ D u}D_ SR M u}D_ D v@Dg SR M v@Dg D v@Dw SR M v@Dw D u}D? SR
M u}D? D uzEC SR M uzEC D uqEG SR M ueEG D u_EC SR M u_EC D u\D? SR
M u\D? D uYDw SR M uYDw D uYDg SR M uYDg D u\D_ SR M u\D_ D u_D[ SR
M u_D[ D ueDW SR M uqDW D uwD[ SR M uwD[ D uzD_ SR M uzD_ D u}Dg SR
M u}Dg D u}Dw SR M u}Dw D uzD? SR M uzD? D uwEC SR M uwEC D uqEG SR
M |fE\ D |lE` SR M |lE` D |uEl SR M |uEl D |uDW SR M |rEh D |rDW SR
M |fDW D }ADW SR M FY|r D |r|r SR M FY|r D FY{r SR M HU|r D HU|R SR
M JQ|r D JQ|R SR M LN|r D LN|R SR M NJ|r D NJ{r SR M PF|r D PF|R SR
M RC|r D RC|R SR M S?|r D S?|R SR M U{|r D U{{r SR M Wx|r D Wx|R SR
M Yt|r D Yt|R SR M [p|r D [p|R SR M ]m|r D ]m{r SR M _i|r D _i|R SR
M ae|r D ae|R SR M cb|r D cb|R SR M e^|r D e^{r SR M gZ|r D gZ|R SR
M iV|r D iV|R SR M kS|r D kS|R SR M mO|r D mO{r SR M oK|r D oK|R SR
M qH|r D qH|R SR M sD|r D sD|R SR M u@|r D u@{r SR M v}|r D v}|R SR
M xy|r D xy|R SR M zu|r D zu|R SR M |r|r D |r{r SR M FYFY D FY|r SR
M FYFY D FyFY SR M FYFY D GYFY SR M FYHG D FyHG SR M FYIH D FyIH SR
M FYIu D FyIu SR M FYJY D FyJY SR M FYJv D FyJv SR M FYKN D FyKN SR
M FYKd D FyKd SR M FYKv D FyKv SR M FYLG D FyLG SR M FYLG D GYLG SR
M FYMv D FyMv SR M FYNv D FyNv SR M FYOd D FyOd SR M FYPG D FyPG SR
M FYPd D FyPd SR M FYP} D FyP} SR M FYQR D FyQR SR M FYQe D FyQe SR
M FYQv D FyQv SR M FYQv D GYQv SR M FYSd D FySd SR M FYTd D FyTd SR
M FYUR D FyUR SR M FYUv D FyUv SR M FYVS D FyVS SR M FYVk D FyVk SR
M FYWA D FyWA SR M FYWS D FyWS SR M FYWd D FyWd SR M FYWd D GYWd SR
M FYYR D FyYR SR M FYZS D FyZS SR M FY[A D Fy[A SR M FY[d D Fy[d SR
M FY\A D Fy\A SR M FY\Z D Fy\Z SR M FY\o D Fy\o SR M FY]B D Fy]B SR
M FY]R D Fy]R SR M FY]R D GY]R SR M FY_A D Fy_A SR M FY`A D Fy`A SR
M FY`o D Fy`o SR M FYaS D FyaS SR M FYap D Fyap SR M FYbH D FybH SR
M FYb] D Fyb] SR M FYbp D Fybp SR M FYcA D FycA SR M FYcA D GYcA SR
M FYdo D Fydo SR M FYep D Fyep SR M FYf] D Fyf] SR M FYgA D FygA SR
M FYg^ D Fyg^ SR M FYgv D Fygv SR M FYhL D FyhL SR M FYh^ D Fyh^ SR
M FYho D Fyho SR M FYho D GYho SR M FYj^ D Fyj^ SR M FYk^ D Fyk^ SR
M FYlL D FylL SR M FYlo D Fylo SR M FYmL D FymL SR M FYme D Fyme SR
M FYmz D Fymz SR M FYnM D FynM SR M FYn^ D Fyn^ SR M FYn^ D GYn^ SR
M FYpL D FypL SR M FYqL D FyqL SR M FYqz D Fyqz SR M FYr^ D Fyr^ SR
M FYr{ D Fyr{ SR M FYsS D FysS SR M FYsi D Fysi SR M FYs{ D Fys{ SR
M FYtL D FytL SR M FYtL D GYtL SR M FYuz D Fyuz SR M FYv{ D Fyv{ SR
M FYwi D Fywi SR M FYxL D FyxL SR M FYxi D Fyxi SR M FYyB D FyyB SR
M FYyW D FyyW SR M FYyj D Fyyj SR M FYyz D Fyyz SR M FYyz D GYyz SR
M FY{i D Fy{i SR M FY|i D Fy|i SR M ByFy D B?F} SR M B?F} D CHGI SR
M CHGI D CHEu SR M CEGE D CEEu SR M ByEu D CTEu SR M C?GI D CvGE SR
M CvGE D CpFy SR M CpFy D ClFe SR M ClFe D ClFY SR M ClFY D CpFE SR
M CpFE D CvEy SR M CvEy D C?Eu SR M C?Eu D DEEu SR M DEEu D DNEy SR
M DNEy D DTFE SR M DTFE D DWFY SR M DWFY D DWFe SR M DWFe D DTFy SR
M DTFy D DNGE SR M DNGE D DEGI SR M DEGI D C?GI SR M C?GI D CyGE SR
M CyGE D CvGA SR M CvGA D CsFy SR M CsFy D CpFe SR M CpFe D CpFY SR
M CpFY D CsFE SR M CsFE D CvE} SR M CvE} D CyEy SR M CyEy D C?Eu SR
M DEEu D DKEy SR M DKEy D DNE} SR M DNE} D DQFE SR M DQFE D DTFY SR
M DTFY D DTFe SR M DTFe D DQFy SR M DQFy D DNGA SR M DNGA D DKGE SR
M DKGE D DEGI SR M ERGw D ELGt SR M ELGt D EIGm SR M EIGm D EGGa SR
M EGGa D EGGZ SR M EGGZ D EIGM SR M EIGM D ELGF SR M ELGF D ERGD SR
M ERGD D EUGD SR M EUGD D E[GF SR M E[GF D E^GM SR M E^GM D E`GZ SR
M E`GZ D E`Ga SR M E`Ga D E^Gm SR M E^Gm D E[Gt SR M E[Gt D EUGw SR
M EUGw D ERGw SR M ERGw D ENGt SR M ENGt D ELGr SR M ELGr D EJGm SR
M EJGm D EIGa SR M EIGa D EIGZ SR M EIGZ D EJGM SR M EJGM D ELGI SR
M ELGI D ENGF SR M ENGF D ERGD SR M EUGD D EYGF SR M EYGF D E[GI SR
M E[GI D E]GM SR M E]GM D E^GZ SR M E^GZ D E^Ga SR M E^Ga D E]Gm SR
M E]Gm D E[Gr SR M E[Gr D EYGt SR M EYGt D EUGw SR M ByLh D B?Ll SR
M B?Ll D CHLx SR M CHLx D CHKc SR M CELt D CEKc SR M ByKc D CTKc SR
M C?Lx D CvLt SR M CvLt D CpLh SR M CpLh D ClLS SR M ClLS D ClLG SR
M ClLG D CpKs SR M CpKs D CvKg SR M CvKg D C?Kc SR M C?Kc D DEKc SR
M DEKc D DNKg SR M DNKg D DTKs SR M DTKs D DWLG SR M DWLG D DWLS SR
M DWLS D DTLh SR M DTLh D DNLt SR M DNLt D DELx SR M DELx D C?Lx SR
M C?Lx D CyLt SR M CyLt D CvLp SR M CvLp D CsLh SR M CsLh D CpLS SR
M CpLS D CpLG SR M CpLG D CsKs SR M CsKs D CvKk SR M CvKk D CyKg SR
M CyKg D C?Kc SR M DEKc D DKKg SR M DKKg D DNKk SR M DNKk D DQKs SR
M DQKs D DTLG SR M DTLG D DTLS SR M DTLS D DQLh SR M DQLh D DNLp SR
M DNLp D DKLt SR M DKLt D DELx SR M ELM[ D EPM^ SR M EPM^ D EUMe SR
M EUMe D EULr SR M ESMc D ESLr SR M ELLr D E]Lr SR M ByRV D B?RZ SR
M B?RZ D CHRf SR M CHRf D CHQQ SR M CERb D CEQQ SR M ByQQ D CTQQ SR
M C?Rf D CvRb SR M CvRb D CpRV SR M CpRV D ClRB SR M ClRB D ClQv SR
M ClQv D CpQb SR M CpQb D CvQV SR M CvQV D C?QQ SR M C?QQ D DEQQ SR
M DEQQ D DNQV SR M DNQV D DTQb SR M DTQb D DWQv SR M DWQv D DWRB SR
M DWRB D DTRV SR M DTRV D DNRb SR M DNRb D DERf SR M DERf D C?Rf SR
M C?Rf D CyRb SR M CyRb D CvR^ SR M CvR^ D CsRV SR M CsRV D CpRB SR
M CpRB D CpQv SR M CpQv D CsQb SR M CsQb D CvQZ SR M CvQZ D CyQV SR
M CyQV D C?QQ SR M DEQQ D DKQV SR M DKQV D DNQZ SR M DNQZ D DQQb SR
M DQQb D DTQv SR M DTQv D DTRB SR M DTRB D DQRV SR M DQRV D DNR^ SR
M DNR^ D DKRb SR M DKRb D DERf SR M EISJ D EJSG SR M EJSG D EISE SR
M EISE D EGSG SR M EGSG D EGSJ SR M EGSJ D EISN SR M EISN D EJSQ SR
M EJSQ D EPSS SR M EPSS D EWSS SR M EWSS D E]SQ SR M E]SQ D E^SN SR
M E^SN D E`SJ SR M E`SJ D E`SE SR M E`SE D E^S@ SR M E^S@ D EYR{ SR
M EYR{ D EPRv SR M EPRv D ELRt SR M ELRt D EIRo SR M EIRo D EGRh SR
M EGRh D EGR` SR M EWSS D E[SQ SR M E[SQ D E]SN SR M E]SN D E^SJ SR
M E^SJ D E^SE SR M E^SE D E]S@ SR M E]S@ D EWR{ SR M EWR{ D EPRv SR
M EGRe D EIRh SR M EIRh D ELRh SR M ELRh D EURc SR M EURc D E[Rc SR
M E[Rc D E^Re SR M E^Re D E`Rh SR M ELRh D EUR` SR M EUR` D E]R` SR
M E]R` D E^Rc SR M E^Rc D E`Rh SR M E`Rh D E`Rm SR M ByXD D B?XH SR
M B?XH D CHXU SR M CHXU D CHW@ SR M CEXQ D CEW@ SR M ByW@ D CTW@ SR
M C?XU D CvXQ SR M CvXQ D CpXD SR M CpXD D ClWp SR M ClWp D ClWd SR
M ClWd D CpWP SR M CpWP D CvWD SR M CvWD D C?W@ SR M C?W@ D DEW@ SR
M DEW@ D DNWD SR M DNWD D DTWP SR M DTWP D DWWd SR M DWWd D DWWp SR
M DWWp D DTXD SR M DTXD D DNXQ SR M DNXQ D DEXU SR M DEXU D C?XU SR
M C?XU D CyXQ SR M CyXQ D CvXL SR M CvXL D CsXD SR M CsXD D CpWp SR
M CpWp D CpWd SR M CpWd D CsWP SR M CsWP D CvWH SR M CvWH D CyWD SR
M CyWD D C?W@ SR M DEW@ D DKWD SR M DKWD D DNWH SR M DNWH D DQWP SR
M DQWP D DTWd SR M DTWd D DTWp SR M DTWp D DQXD SR M DQXD D DNXL SR
M DNXL D DKXQ SR M DKXQ D DEXU SR M EIXz D EJXx SR M EJXx D EIXv SR
M EIXv D EGXx SR M EGXx D EGXz SR M EGXz D EJX? SR M EJX? D EPYB SR
M EPYB D EWYB SR M EWYB D E]X? SR M E]X? D E^Xz SR M E^Xz D E^Xs SR
M E^Xs D E]Xn SR M E]Xn D EWXl SR M EWXl D ERXl SR M EWYB D E[X? SR
M E[X? D E]Xz SR M E]Xz D E]Xs SR M E]Xs D E[Xn SR M E[Xn D EWXl SR
M EWXl D E[Xj SR M E[Xj D E^Xe SR M E^Xe D E`X` SR M E`X` D E`XY SR
M E`XY D E^XT SR M E^XT D E]XQ SR M E]XQ D EWXO SR M EWXO D EPXO SR
M EPXO D EJXQ SR M EJXQ D EIXT SR M EIXT D EGXY SR M EGXY D EGX[ SR
M EGX[ D EIX] SR M EIX] D EJX[ SR M EJX[ D EIXY SR M E]Xg D E^X` SR
M E^X` D E^XY SR M E^XY D E]XT SR M E]XT D E[XQ SR M E[XQ D EWXO SR
M By]s D B?]w SR M B?]w D CH^C SR M CH^C D CH\n SR M CE]? D CE\n SR
M By\n D CT\n SR M C?^C D Cv]? SR M Cv]? D Cp]s SR M Cp]s D Cl]_ SR
M Cl]_ D Cl]R SR M Cl]R D Cp\~ SR M Cp\~ D Cv\r SR M Cv\r D C?\n SR
M C?\n D DE\n SR M DE\n D DN\r SR M DN\r D DT\~ SR M DT\~ D DW]R SR
M DW]R D DW]_ SR M DW]_ D DT]s SR M DT]s D DN]? SR M DN]? D DE^C SR
M DE^C D C?^C SR M C?^C D Cy]? SR M Cy]? D Cv]{ SR M Cv]{ D Cs]s SR
M Cs]s D Cp]_ SR M Cp]_ D Cp]R SR M Cp]R D Cs\~ SR M Cs\~ D Cv\v SR
M Cv\v D Cy\r SR M Cy\r D C?\n SR M DE\n D DK\r SR M DK\r D DN\v SR
M DN\v D DQ\~ SR M DQ\~ D DT]R SR M DT]R D DT]_ SR M DT]_ D DQ]s SR
M DQ]s D DN]{ SR M DN]{ D DK]? SR M DK]? D DE^C SR M EW^k D EW]} SR
M EY^p D EY]} SR M EY^p D EE^L SR M EE^L D Eb^L SR M ER]} D E^]} SR
M Byca D B?ce SR M B?ce D CHcq SR M CHcq D CHb] SR M CEcm D CEb] SR
M Byb] D CTb] SR M C?cq D Cvcm SR M Cvcm D Cpca SR M Cpca D ClcM SR
M ClcM D ClcA SR M ClcA D Cpbm SR M Cpbm D Cvba SR M Cvba D C?b] SR
M C?b] D DEb] SR M DEb] D DNba SR M DNba D DTbm SR M DTbm D DWcA SR
M DWcA D DWcM SR M DWcM D DTca SR M DTca D DNcm SR M DNcm D DEcq SR
M DEcq D C?cq SR M C?cq D Cycm SR M Cycm D Cvci SR M Cvci D Csca SR
M Csca D CpcM SR M CpcM D CpcA SR M CpcA D Csbm SR M Csbm D Cvbe SR
M Cvbe D Cyba SR M Cyba D C?b] SR M DEb] D DKba SR M DKba D DNbe SR
M DNbe D DQbm SR M DQbm D DTcA SR M DTcA D DTcM SR M DTcM D DQca SR
M DQca D DNci SR M DNci D DKcm SR M DKcm D DEcq SR M EJd_ D EGdF SR
M EGdF D EJdI SR M EJdI D EPdK SR M EPdK D EUdK SR M EUdK D E[dI SR
M E[dI D E^dD SR M E^dD D E`c} SR M E`c} D E`cz SR M E`cz D E^cs SR
M E^cs D E[cn SR M E[cn D EUcl SR M EUcl D EPcl SR M EPcl D EJcn SR
M EJcn D EIcq SR M EIcq D EGcu SR M EGcu D EGcx SR M EGcx D EIcz SR
M EIcz D EJcx SR M EJcx D EIcu SR M EUdK D EYdI SR M EYdI D E]dD SR
M E]dD D E^c} SR M E^c} D E^cz SR M E^cz D E]cs SR M E]cs D EYcn SR
M EYcn D EUcl SR M EJd_ D E]d_ SR M EJd\ D ESd\ SR M ESd\ D E]d_ SR
M ByiP D B?iT SR M B?iT D CHi` SR M CHi` D CHhK SR M CEi\ D CEhK SR
M ByhK D CThK SR M C?i` D Cvi\ SR M Cvi\ D CpiP SR M CpiP D Clh{ SR
M Clh{ D Clho SR M Clho D Cph[ SR M Cph[ D CvhO SR M CvhO D C?hK SR
M C?hK D DEhK SR M DEhK D DNhO SR M DNhO D DTh[ SR M DTh[ D DWho SR
M DWho D DWh{ SR M DWh{ D DTiP SR M DTiP D DNi\ SR M DNi\ D DEi` SR
M DEi` D C?i` SR M C?i` D Cyi\ SR M Cyi\ D CviX SR M CviX D CsiP SR
M CsiP D Cph{ SR M Cph{ D Cpho SR M Cpho D Csh[ SR M Csh[ D CvhS SR
M CvhS D CyhO SR M CyhO D C?hK SR M DEhK D DKhO SR M DKhO D DNhS SR
M DNhS D DQh[ SR M DQh[ D DTho SR M DTho D DTh{ SR M DTh{ D DQiP SR
M DQiP D DNiX SR M DNiX D DKi\ SR M DKi\ D DEi` SR M E]jF D E[jC SR
M E[jC D E]jA SR M E]jA D E^jC SR M E^jC D E^jF SR M E^jF D E]jJ SR
M E]jJ D EYjM SR M EYjM D ESjM SR M ESjM D ENjJ SR M ENjJ D EJjF SR
M EJjF D EIjA SR M EIjA D EGiw SR M EGiw D EGii SR M EGii D EIia SR
M EIia D ELi\ SR M ELi\ D ERiZ SR M ERiZ D EUiZ SR M EUiZ D E[i\ SR
M E[i\ D E^ia SR M E^ia D E`ii SR M E`ii D E`ik SR M E`ik D E^ir SR
M E^ir D E[iw SR M E[iw D EUiz SR M EUiz D ESiz SR M ESiz D ENiw SR
M ENiw D EJir SR M EJir D EIik SR M ESjM D EPjJ SR M EPjJ D ELjF SR
M ELjF D EJjA SR M EJjA D EIiw SR M EIiw D EIii SR M EIii D EJia SR
M EJia D ENi\ SR M ENi\ D ERiZ SR M EUiZ D EYi\ SR M EYi\ D E]ia SR
M E]ia D E^ii SR M E^ii D E^ik SR M E^ik D E]ir SR M E]ir D EYiw SR
M EYiw D EUiz SR M Byn~ D B?oB SR M B?oB D CHoN SR M CHoN D CHmy SR
M CEoJ D CEmy SR M Bymy D CTmy SR M C?oN D CvoJ SR M CvoJ D Cpn~ SR
M Cpn~ D Clnj SR M Clnj D Cln^ SR M Cln^ D CpnI SR M CpnI D Cvm} SR
M Cvm} D C?my SR M C?my D DEmy SR M DEmy D DNm} SR M DNm} D DTnI SR
M DTnI D DWn^ SR M DWn^ D DWnj SR M DWnj D DTn~ SR M DTn~ D DNoJ SR
M DNoJ D DEoN SR M DEoN D C?oN SR M C?oN D CyoJ SR M CyoJ D CvoF SR
M CvoF D Csn~ SR M Csn~ D Cpnj SR M Cpnj D Cpn^ SR M Cpn^ D CsnI SR
M CsnI D CvnA SR M CvnA D Cym} SR M Cym} D C?my SR M DEmy D DKm} SR
M DKm} D DNnA SR M DNnA D DQnI SR M DQnI D DTn^ SR M DTn^ D DTnj SR
M DTnj D DQn~ SR M DQn~ D DNoF SR M DNoF D DKoJ SR M DKoJ D DEoN SR
M EGo{ D EGom SR M EGor D EIov SR M EIov D ELo{ SR M ELo{ D EPo{ SR
M EPo{ D EYot SR M EYot D E]ot SR M E]ot D E^ov SR M E^ov D E`o{ SR
M EIov D ELoy SR M ELoy D EPoy SR M EPoy D EYot SR M E`o{ D E`ot SR
M E`ot D E^om SR M E^om D EWoa SR M EWoa D EUo\ SR M EUo\ D ESoU SR
M ESoU D ESoH SR M E^om D EUoa SR M EUoa D ESo\ SR M ESo\ D ERoU SR
M ERoU D ERoH SR M Bytl D B?tp SR M B?tp D CHt} SR M CHt} D CHsh SR
M CEty D CEsh SR M Bysh D CTsh SR M C?t} D Cvty SR M Cvty D Cptl SR
M Cptl D CltX SR M CltX D CltL SR M CltL D Cpsx SR M Cpsx D Cvsl SR
M Cvsl D C?sh SR M C?sh D DEsh SR M DEsh D DNsl SR M DNsl D DTsx SR
M DTsx D DWtL SR M DWtL D DWtX SR M DWtX D DTtl SR M DTtl D DNty SR
M DNty D DEt} SR M DEt} D C?t} SR M C?t} D Cyty SR M Cyty D Cvtt SR
M Cvtt D Cstl SR M Cstl D CptX SR M CptX D CptL SR M CptL D Cssx SR
M Cssx D Cvsp SR M Cvsp D Cysl SR M Cysl D C?sh SR M DEsh D DKsl SR
M DKsl D DNsp SR M DNsp D DQsx SR M DQsx D DTtL SR M DTtL D DTtX SR
M DTtX D DQtl SR M DQtl D DNtt SR M DNtt D DKty SR M DKty D DEt} SR
M EPuj D EJug SR M EJug D EIub SR M EIub D EIu[ SR M EIu[ D EJuV SR
M EJuV D EPuT SR M EPuT D EWuT SR M EWuT D E]uV SR M E]uV D E^u[ SR
M E^u[ D E^ub SR M E^ub D E]ug SR M E]ug D EWuj SR M EWuj D EPuj SR
M EPuj D ELug SR M ELug D EJub SR M EJub D EJu[ SR M EJu[ D ELuV SR
M ELuV D EPuT SR M EWuT D E[uV SR M E[uV D E]u[ SR M E]u[ D E]ub SR
M E]ub D E[ug SR M E[ug D EWuj SR M EPuT D EJuR SR M EJuR D EIuO SR
M EIuO D EGuJ SR M EGuJ D EGuA SR M EGuA D EIt| SR M EIt| D EJty SR
M EJty D EPtw SR M EPtw D EWtw SR M EWtw D E]ty SR M E]ty D E^t| SR
M E^t| D E`uA SR M E`uA D E`uJ SR M E`uJ D E^uO SR M E^uO D E]uR SR
M E]uR D EWuT SR M EPuT D ELuR SR M ELuR D EJuO SR M EJuO D EIuJ SR
M EIuJ D EIuA SR M EIuA D EJt| SR M EJt| D ELty SR M ELty D EPtw SR
M EWtw D E[ty SR M E[ty D E]t| SR M E]t| D E^uA SR M E^uA D E^uJ SR
M E^uJ D E]uO SR M E]uO D E[uR SR M E[uR D EWuT SR M Byz[ D B?z_ SR
M B?z_ D CHzk SR M CHzk D CHyV SR M CEzg D CEyV SR M ByyV D CTyV SR
M C?zk D Cvzg SR M Cvzg D Cpz[ SR M Cpz[ D ClzG SR M ClzG D Clyz SR
M Clyz D Cpyf SR M Cpyf D CvyZ SR M CvyZ D C?yV SR M C?yV D DEyV SR
M DEyV D DNyZ SR M DNyZ D DTyf SR M DTyf D DWyz SR M DWyz D DWzG SR
M DWzG D DTz[ SR M DTz[ D DNzg SR M DNzg D DEzk SR M DEzk D C?zk SR
M C?zk D Cyzg SR M Cyzg D Cvzc SR M Cvzc D Csz[ SR M Csz[ D CpzG SR
M CpzG D Cpyz SR M Cpyz D Csyf SR M Csyf D Cvy^ SR M Cvy^ D CyyZ SR
M CyyZ D C?yV SR M DEyV D DKyZ SR M DKyZ D DNy^ SR M DNy^ D DQyf SR
M DQyf D DTyz SR M DTyz D DTzG SR M DTzG D DQz[ SR M DQz[ D DNzc SR
M DNzc D DKzg SR M DKzg D DEzk SR M E^{G D E]{@ SR M E]{@ D EYz{ SR
M EYz{ D ESzy SR M ESzy D ERzy SR M ERzy D ELz{ SR M ELz{ D EI{@ SR
M EI{@ D EG{G SR M EG{G D EG{J SR M EG{J D EI{Q SR M EI{Q D EL{V SR
M EL{V D ER{X SR M ER{X D EU{X SR M EU{X D E[{V SR M E[{V D E^{Q SR
M E^{Q D E`{J SR M E`{J D E`z{ SR M E`z{ D E^zq SR M E^zq D E]zm SR
M E]zm D EYzh SR M EYzh D ESze SR M ESze D ENze SR M ENze D EJzh SR
M EJzh D EIzm SR M EIzm D EIzo SR M EIzo D EJzq SR M EJzq D ELzo SR
M ELzo D EJzm SR M ERzy D ENz{ SR M ENz{ D EJ{@ SR M EJ{@ D EI{G SR
M EI{G D EI{J SR M EI{J D EJ{Q SR M EJ{Q D EN{V SR M EN{V D ER{X SR
M EU{X D EY{V SR M EY{V D E]{Q SR M E]{Q D E^{J SR M E^{J D E^z{ SR
M E^z{ D E]zq SR M E]zq D E[zm SR M E[zm D EWzh SR M EWzh D ESze SR
M |rFY D |r|r SR M |rFY D |RFY SR M |rFY D {rFY SR M |rHG D |RHG SR
M |rIH D |RIH SR M |rIu D |RIu SR M |rJY D |RJY SR M |rJv D |RJv SR
M |rKN D |RKN SR M |rKd D |RKd SR M |rKv D |RKv SR M |rLG D |RLG SR
M |rLG D {rLG SR M |rMv D |RMv SR M |rNv D |RNv SR M |rOd D |ROd SR
M |rPG D |RPG SR M |rPd D |RPd SR M |rP} D |RP} SR M |rQR D |RQR SR
M |rQe D |RQe SR M |rQv D |RQv SR M |rQv D {rQv SR M |rSd D |RSd SR
M |rTd D |RTd SR M |rUR D |RUR SR M |rUv D |RUv SR M |rVS D |RVS SR
M |rVk D |RVk SR M |rWA D |RWA SR M |rWS D |RWS SR M |rWd D |RWd SR
M |rWd D {rWd SR M |rYR D |RYR SR M |rZS D |RZS SR M |r[A D |R[A SR
M |r[d D |R[d SR M |r\A D |R\A SR M |r\Z D |R\Z SR M |r\o D |R\o SR
M |r]B D |R]B SR M |r]R D |R]R SR M |r]R D {r]R SR M |r_A D |R_A SR
M |r`A D |R`A SR M |r`o D |R`o SR M |raS D |RaS SR M |rap D |Rap SR
M |rbH D |RbH SR M |rb] D |Rb] SR M |rbp D |Rbp SR M |rcA D |RcA SR
M |rcA D {rcA SR M |rdo D |Rdo SR M |rep D |Rep SR M |rf] D |Rf] SR
M |rgA D |RgA SR M |rg^ D |Rg^ SR M |rgv D |Rgv SR M |rhL D |RhL SR
M |rh^ D |Rh^ SR M |rho D |Rho SR M |rho D {rho SR M |rj^ D |Rj^ SR
M |rk^ D |Rk^ SR M |rlL D |RlL SR M |rlo D |Rlo SR M |rmL D |RmL SR
M |rme D |Rme SR M |rmz D |Rmz SR M |rnM D |RnM SR M |rn^ D |Rn^ SR
M |rn^ D {rn^ SR M |rpL D |RpL SR M |rqL D |RqL SR M |rqz D |Rqz SR
M |rr^ D |Rr^ SR M |rr{ D |Rr{ SR M |rsS D |RsS SR M |rsi D |Rsi SR
M |rs{ D |Rs{ SR M |rtL D |RtL SR M |rtL D {rtL SR M |ruz D |Ruz SR
M |rv{ D |Rv{ SR M |rwi D |Rwi SR M |rxL D |RxL SR M |rxi D |Rxi SR
M |ryB D |RyB SR M |ryW D |RyW SR M |ryj D |Ryj SR M |ryz D |Ryz SR
M |ryz D {ryz SR M |r{i D |R{i SR M |r|i D |R|i SR
M @^Ub D @dUf SR M @dUf D @TUf SR M @TUf D @^Ub SR M @^Ub D @WUZ SR
M @WUZ D @TUN SR M @TUN D @TUF SR M @TUF D @WTz SR M @WTz D @^Tq SR
M @^Tq D @dTm SR M @dTm D @mTi SR M @mTi D @|Ti SR M @|Ti D AETm SR
M AETm D AKTq SR M AKTq D AQTz SR M AQTz D ATUF SR M ATUF D ATUN SR
M ATUN D AQUZ SR M AQUZ D AKUb SR M AKUb D AEUf SR M @TUF D @WT~ SR
M @WT~ D @^Tv SR M @^Tv D @dTq SR M @dTq D @mTm SR M @mTm D @|Tm SR
M @|Tm D AETq SR M AETq D AKTv SR M AKTv D AQT~ SR M AQT~ D ATUF SR
M @jVV D @mVJ SR M @mVJ D @sVB SR M @sVB D @|U~ SR M @|U~ D ABU~ SR
M ABU~ D AKVB SR M AKVB D AQVJ SR M AQVJ D ATVV SR M ATVV D ATV^ SR
M ATV^ D AQVk SR M AQVk D AKVs SR M AKVs D ABVw SR M ABVw D @|Vw SR
M @|Vw D @sVs SR M @sVs D @mVk SR M @mVk D @jV^ SR M @jV^ D @jVV SR
M @jVV D @mVN SR M @mVN D @sVF SR M @sVF D @|VB SR M @|VB D ABVB SR
M ABVB D AKVF SR M AKVF D AQVN SR M AQVN D ATVV SR M ATV^ D AQVf SR
M AQVf D AKVo SR M AKVo D ABVs SR M ABVs D @|Vs SR M @|Vs D @sVo SR
M @sVo D @mVf SR M @mVf D @jV^ SR M @jWW D AKWW SR M AKWW D AQW[ SR
M AQW[ D ATWg SR M ATWg D ATWo SR M ATWo D AQW{ SR M AQW{ D AKXC SR
M @jW[ D AKW[ SR M AKW[ D AQW_ SR M AQW_ D ATWg SR M @jXC D ATXC SR
M @jXG D ATXG SR M @jWK D @jW[ SR M @jWw D @jXG SR M ATXC D ATXS SR
M @jXp D ATXp SR M @jXt D ATXt SR M @sXt D @mX| SR M @mX| D @jYH SR
M @jYH D @jYP SR M @jYP D @mY\ SR M @mY\ D @sY` SR M @sY` D ATY` SR
M @jYP D @mYX SR M @mYX D @sY\ SR M @sY\ D ATY\ SR M @jXd D @jXt SR
M ATXd D ATY@ SR M ATYP D ATYl SR M @TZH D AHZH SR M AHZH D AQZM SR
M AQZM D ATZU SR M ATZU D ATZ] SR M ATZ] D AQZe SR M AQZe D AKZi SR
M @TZM D AHZM SR M AHZM D AQZQ SR M AQZQ D ATZU SR M @jY| D @jZ] SR
M @T\N D AT\N SR M @T\R D AT\R SR M @T\A D @T\r SR M @T\r D @W\~ SR
M @W\~ D @Z]B SR M @Z]B D @a]F SR M @a]F D @g]F SR M @g]F D @m]B SR
M @m]B D @p\~ SR M @p\~ D @s\r SR M @s\r D @s\R SR M @T\r D @W\z SR
M @W\z D @Z\~ SR M @Z\~ D @a]B SR M @a]B D @g]B SR M @g]B D @m\~ SR
M @m\~ D @p\z SR M @p\z D @s\r SR M AT\A D AT\^ SR M @s\j D AN\z SR
M AN\z D AT]B SR M AT]B D AT]J SR M AT]J D AN]N SR M @s\j D @y\r SR
M @y\r D AT]B SR M @p]f D @s]f SR M @s]f D @s]b SR M @s]b D @p]b SR
M @p]b D @m]f SR M @m]f D @j]n SR M @j]n D @j]? SR M @j]? D @m^G SR
M @m^G D @p^K SR M @p^K D @v^O SR M @v^O D AK^O SR M AK^O D AQ^S SR
M AQ^S D AT^W SR M @p^K D AK^K SR M AK^K D AQ^O SR M AQ^O D AT^W SR
M AT^W D AT^[ SR M @v^K D @y^G SR M @y^G D @|]n SR M @|]n D @?]b SR
M @?]b D AE]^ SR M AE]^ D AK]^ SR M AK]^ D AQ]b SR M AQ]b D AT]n SR
M AT]n D AT]z SR M AT]z D AQ^C SR M AQ^C D AK^K SR M @|]n D @?]f SR
M @?]f D AE]b SR M AE]b D AK]b SR M AK]b D AQ]f SR M AQ]f D AT]n SR
M @T^w D AH^w SR M AH^w D AQ^{ SR M AQ^{ D AT_C SR M AT_C D AT_K SR
M AT_K D AQ_S SR M AQ_S D AK_W SR M @T^{ D AH^{ SR M AH^{ D AQ^? SR
M AQ^? D AT_C SR M @j^k D @j_K SR M @|_p D @|`` SR M @|`` D @v`` SR
M @v`` D @p`\ SR M @p`\ D @m`X SR M @m`X D @j`P SR M @j`P D @j`D SR
M @j`D D @m_x SR M @m_x D @s_p SR M @s_p D @|_k SR M @|_k D AB_k SR
M AB_k D AK_p SR M AK_p D AQ_x SR M AQ_x D AT`D SR M AT`D D AT`L SR
M AT`L D AQ`X SR M AQ`X D AK`` SR M @|`\ D @s`\ SR M @s`\ D @m`X SR
M @j`D D @m_| SR M @m_| D @s_t SR M @s_t D @|_p SR M @|_p D AB_p SR
M AB_p D AK_t SR M AK_t D AQ_| SR M AQ_| D AT`D SR M @Hba D @NbY SR
M @NbY D @WbQ SR M @WbQ D @dbI SR M @dbI D @sbE SR M @sbE D @?bE SR
M @?bE D ANbI SR M ANbI D AZbQ SR M AZbQ D AdbY SR M AdbY D Ajba SR
M @NbY D @ZbQ SR M @ZbQ D @dbM SR M @dbM D @sbI SR M @sbI D @?bI SR
M @?bI D ANbM SR M ANbM D AWbQ SR M AWbQ D AdbY SR M @scj D @vcf SR
M @vcf D @ycj SR M @ycj D @vcn SR M @vcn D @scn SR M @scn D @mcf SR
M @mcf D @jc^ SR M @jc^ D @jcQ SR M @jcQ D @mcE SR M @mcE D @sb} SR
M @sb} D @|by SR M @|by D ABby SR M ABby D AKb} SR M AKb} D AQcE SR
M AQcE D ATcQ SR M ATcQ D ATcZ SR M ATcZ D AQcf SR M AQcf D AKcn SR
M @jcQ D @mcI SR M @mcI D @scA SR M @scA D @|b} SR M @|b} D ABb} SR
M ABb} D AKcA SR M AKcA D AQcI SR M AQcI D ATcQ SR M @jd^ D @mdR SR
M @mdR D @sdJ SR M @sdJ D @|dF SR M @|dF D ABdF SR M ABdF D AKdJ SR
M AKdJ D AQdR SR M AQdR D ATd^ SR M ATd^ D ATdf SR M ATdf D AQdr SR
M AQdr D AKdz SR M AKdz D ABd~ SR M ABd~ D @|d~ SR M @|d~ D @sdz SR
M @sdz D @mdr SR M @mdr D @jdf SR M @jdf D @jd^ SR M @jd^ D @mdV SR
M @mdV D @sdN SR M @sdN D @|dJ SR M @|dJ D ABdJ SR M ABdJ D AKdN SR
M AKdN D AQdV SR M AQdV D ATd^ SR M ATdf D AQdn SR M AQdn D AKdv SR
M AKdv D ABdz SR M ABdz D @|dz SR M @|dz D @sdv SR M @sdv D @mdn SR
M @mdn D @jdf SR M @je_ D AKe_ SR M AKe_ D AQec SR M AQec D ATeo SR
M ATeo D ATew SR M ATew D AQfC SR M AQfC D AKfK SR M @jec D AKec SR
M AKec D AQeg SR M AQeg D ATeo SR M @jfK D ATfK SR M @jfO D ATfO SR
M @jeR D @jec SR M @je? D @jfO SR M ATfK D ATf[ SR M @jfw D ATfw SR
M @jf{ D ATf{ SR M @sf{ D @mgC SR M @mgC D @jgP SR M @jgP D @jgX SR
M @jgX D @mgd SR M @mgd D @sgh SR M @sgh D ATgh SR M @jgX D @mg` SR
M @mg` D @sgd SR M @sgd D ATgd SR M @jfk D @jf{ SR M ATfk D ATgH SR
M ATgX D ATgt SR M @ThP D AHhP SR M AHhP D AQhT SR M AQhT D ATh\ SR
M ATh\ D AThd SR M AThd D AQhl SR M AQhl D AKhp SR M @ThT D AHhT SR
M AHhT D AQhX SR M AQhX D ATh\ SR M @jhD D @jhd SR M @mim D @jiq SR
M @jiq D @siq SR M @siq D @mim SR M @mim D @jia SR M @jia D @jiU SR
M @jiU D @miI SR M @miI D @piE SR M @piE D @siE SR M @siE D @yiI SR
M @yiI D @|iQ SR M @|iQ D ABie SR M ABie D AEim SR M AEim D AHiq SR
M @siE D @viI SR M @viI D @yiQ SR M @yiQ D @?ie SR M @?ie D ABim SR
M ABim D AHiq SR M AHiq D ANiq SR M ANiq D AQim SR M AQim D ATia SR
M ATia D ATiU SR M ATiU D AQiI SR M AQiI D AKiE SR M AKiE D ATiE SR
M ATiE D AQiI SR M @mkz D @jk~ SR M @jk~ D @sk~ SR M @sk~ D @mkz SR
M @mkz D @jkn SR M @jkn D @jkb SR M @jkb D @mkV SR M @mkV D @pkR SR
M @pkR D @skR SR M @skR D @ykV SR M @ykV D @|k^ SR M @|k^ D ABkr SR
M ABkr D AEkz SR M AEkz D AHk~ SR M @skR D @vkV SR M @vkV D @yk^ SR
M @yk^ D @?kr SR M @?kr D ABkz SR M ABkz D AHk~ SR M AHk~ D ANk~ SR
M ANk~ D AQkz SR M AQkz D ATkn SR M ATkn D ATkb SR M ATkb D AQkV SR
M AQkV D AKkR SR M AKkR D ATkR SR M ATkR D AQkV SR M @HlR D @Hl} SR
M @@mS D @@mX SR M @@mX D @@m_ SR M @@m_ D @Ym_ SR M @@m] D @Ym] SR
M @YmS D @Ymi SR M @HnA D @NnI SR M @NnI D @WnQ SR M @WnQ D @dnY SR
M @dnY D @sn] SR M @sn] D @?n] SR M @?n] D ANnY SR M ANnY D AZnQ SR
M AZnQ D AdnI SR M AdnI D AjnA SR M @NnI D @ZnQ SR M @ZnQ D @dnU SR
M @dnU D @snY SR M @snY D @?nY SR M @?nY D ANnU SR M ANnU D AWnQ SR
M AWnQ D AdnI SR
M _bBo D _\Bg SR M _\Bg D _VB[ SR M _VB[ D _PBK SR M _PBK D _MAw SR
M _MAw D _MAg SR M _MAg D _PAR SR M _PAR D _VAB SR M _VAB D _\@v SR
M _\@v D _b@n SR M _\Bg D _VBW SR M _VBW D _SBK SR M _SBK D _PAw SR
M _PAw D _PAg SR M _PAg D _SAR SR M _SAR D _VAF SR M _VAF D _\@v SR
M _{B_ D _{AJ SR M _~B_ D _~AJ SR M _rB_ D `VB_ SR M `VB_ D `_B[ SR
M `_B[ D `bBW SR M `bBW D `eBO SR M `eBO D `eBG SR M `eBG D `bA? SR
M `bA? D `_A{ SR M `_A{ D `VAw SR M `VB_ D `\B[ SR M `\B[ D `_BW SR
M `_BW D `bBO SR M `bBO D `bBG SR M `bBG D `_A? SR M `_A? D `\A{ SR
M `\A{ D `VAw SR M _~Aw D `VAw SR M `VAw D `_As SR M `_As D `bAo SR
M `bAo D `eAg SR M `eAg D `eAZ SR M `eAZ D `bAR SR M `bAR D `_AN SR
M `_AN D `VAJ SR M `VAJ D _rAJ SR M `VAw D `\As SR M `\As D `_Ao SR
M `_Ao D `bAg SR M `bAg D `bAZ SR M `bAZ D `_AR SR M `_AR D `\AN SR
M `\AN D `VAJ SR M `xAo D anAo SR M bDB_ D bYAJ SR M bGB_ D bYAV SR
M bnB_ D bYAJ SR M a{B_ D bPB_ SR M beB_ D bxB_ SR M cDBo D cJBg SR
M cJBg D cPB[ SR M cPB[ D cVBK SR M cVBK D cYAw SR M cYAw D cYAg SR
M cYAg D cVAR SR M cVAR D cPAB SR M cPAB D cJ@v SR M cJ@v D cD@n SR
M cJBg D cPBW SR M cPBW D cSBK SR M cSBK D cVAw SR M cVAw D cVAg SR
M cVAg D cSAR SR M cSAR D cPAF SR M cPAF D cJ@v SR M cvAe D cpAb SR
M cpAb D cmA[ SR M cmA[ D ckAO SR M ckAO D ckAH SR M ckAH D cm@| SR
M cm@| D cp@t SR M cp@t D cv@r SR M cv@r D cy@r SR M cy@r D c?@t SR
M c?@t D dC@| SR M dC@| D dDAH SR M dDAH D dDAO SR M dDAO D dCA[ SR
M dCA[ D c?Ab SR M c?Ab D cyAe SR M cyAe D cvAe SR M cvAe D crAb SR
M crAb D cpA` SR M cpA` D cnA[ SR M cnA[ D cmAO SR M cmAO D cmAH SR
M cmAH D cn@| SR M cn@| D cp@w SR M cp@w D cr@t SR M cr@t D cv@r SR
M cy@r D c}@t SR M c}@t D c?@w SR M c?@w D dA@| SR M dA@| D dCAH SR
M dCAH D dCAO SR M dCAO D dAA[ SR M dAA[ D c?A` SR M c?A` D c}Ab SR
M c}Ab D cyAe SR
M mboX D mbmr SR M meoX D nQm| SR M meoN D nQmr SR M nQoX D nQmr SR
M mWoX D meoX SR M nFoX D n\oX SR M mWmr D mmmr SR M nyoD D o@oI SR
M o@oI D oKoX SR M oKoX D oKmr SR M oHoS D oHmr SR M nymr D oZmr SR
M HUyS D JQwo D LNvK D NJth D PFsE D RCqb D S?o? D U{n] D Wxl{ D YtkY
D [piw D ]mhV D _ifu D aeeT D cbct D e^bT D gZ`t D iV_U D kS]u D mO\V
D oKZx D qHYY D sDW{ D u@V] D v}U@ SR
M yOUf D yHUc SR M yHUc D yCUY SR M yCUY D y@UI SR M y@UI D y@T? SR
M y@T? D yCTo SR M yCTo D yHTe SR M yHTe D yOTb SR M yOTb D yTTb SR
M yTTb D y[Te SR M y[Te D y`To SR M y`To D ybT? SR M ybT? D ybUI SR
M ybUI D y`UY SR M y`UY D y[Uc SR M y[Uc D yTUf SR M yTUf D yOUf SR
M yOUf D yJUc SR M yJUc D yHU` SR M yHU` D yEUY SR M yEUY D yCUI SR
M yCUI D yCT? SR M yCT? D yETo SR M yETo D yHTi SR M yHTi D yJTe SR
M yJTe D yOTb SR M yTTb D yYTe SR M yYTe D y[Ti SR M y[Ti D y^To SR
M y^To D y`T? SR M y`T? D y`UI SR M y`UI D y^UY SR M y^UY D y[U` SR
M y[U` D yYUc SR M yYUc D yTUf SR M ytTi D yqTe SR M yqTe D ytTb SR
M ytTb D yvTe SR M yvTe D ytTi SR M zSUf D zLUc SR M zLUc D zGUY SR
M zGUY D zEUI SR M zEUI D zET? SR M zET? D zGTo SR M zGTo D zLTe SR
M zLTe D zSTb SR M zSTb D zXTb SR M zXTb D z_Te SR M z_Te D zdTo SR
M zdTo D zgT? SR M zgT? D zgUI SR M zgUI D zdUY SR M zdUY D z_Uc SR
M z_Uc D zXUf SR M zXUf D zSUf SR M zSUf D zNUc SR M zNUc D zLU` SR
M zLU` D zIUY SR M zIUY D zGUI SR M zGUI D zGT? SR M zGT? D zITo SR
M zITo D zLTi SR M zLTi D zNTe SR M zNTe D zSTb SR M zXTb D z]Te SR
M z]Te D z_Ti SR M z_Ti D zbTo SR M zbTo D zdT? SR M zdT? D zdUI SR
M zdUI D zbUY SR M zbUY D z_U` SR M z_U` D z]Uc SR M z]Uc D zXUf SR
M HUwS D JQup D LNtN D NJrl D PFqJ D RCoh D S?nF D U{le D WxkD D Ytib
D [phB D ]mfa D _ie@ D aec` D cbb@ D e^`` D gZ_@ D iV]` D kS\A D mOZb
D oKYC D qHWd D sDVE D u@Tf D v}SH SR
M yOSm D yHSj SR M yHSj D yCS` SR M yCS` D y@SP SR M y@SP D y@SF SR
M y@SF D yCRv SR M yCRv D yHRl SR M yHRl D yORi SR M yORi D yTRi SR
M yTRi D y[Rl SR M y[Rl D y`Rv SR M y`Rv D ybSF SR M ybSF D ybSP SR
M ybSP D y`S` SR M y`S` D y[Sj SR M y[Sj D yTSm SR M yTSm D yOSm SR
M yOSm D yJSj SR M yJSj D yHSg SR M yHSg D yES` SR M yES` D yCSP SR
M yCSP D yCSF SR M yCSF D yERv SR M yERv D yHRp SR M yHRp D yJRl SR
M yJRl D yORi SR M yTRi D yYRl SR M yYRl D y[Rp SR M y[Rp D y^Rv SR
M y^Rv D y`SF SR M y`SF D y`SP SR M y`SP D y^S` SR M y^S` D y[Sg SR
M y[Sg D yYSj SR M yYSj D yTSm SR M ytRp D yqRl SR M yqRl D ytRi SR
M ytRi D yvRl SR M yvRl D ytRp SR M zLS` D zQSc SR M zQSc D zXSm SR
M zXSm D zXRi SR M zVSj D zVRi SR M zLRi D zbRi SR
M HUuQ D JQsp D LNrO D NJpo D PFoN D RCmn D S?lN D U{jn D WxiN D Ytgo
D [pfO D ]mdp D _icQ D aeaq D cb`R D e^^t D gZ]U D iV[v D kSZX D mOXy
D oKW[ D qHU} D sDT_ D u@SA D v}Qd SR
M yORJ D yHRG SR M yHRG D yCQ} SR M yCQ} D y@Qm SR M y@Qm D y@Qc SR
M y@Qc D yCQS SR M yCQS D yHQJ SR M yHQJ D yOQF SR M yOQF D yTQF SR
M yTQF D y[QJ SR M y[QJ D y`QS SR M y`QS D ybQc SR M ybQc D ybQm SR
M ybQm D y`Q} SR M y`Q} D y[RG SR M y[RG D yTRJ SR M yTRJ D yORJ SR
M yORJ D yJRG SR M yJRG D yHRD SR M yHRD D yEQ} SR M yEQ} D yCQm SR
M yCQm D yCQc SR M yCQc D yEQS SR M yEQS D yHQM SR M yHQM D yJQJ SR
M yJQJ D yOQF SR M yTQF D yYQJ SR M yYQJ D y[QM SR M y[QM D y^QS SR
M y^QS D y`Qc SR M y`Qc D y`Qm SR M y`Qm D y^Q} SR M y^Q} D y[RD SR
M y[RD D yYRG SR M yYRG D yTRJ SR M ytQM D yqQJ SR M yqQJ D ytQF SR
M ytQF D yvQJ SR M yvQJ D ytQM SR M zGQ} D zIQz SR M zIQz D zGQw SR
M zGQw D zEQz SR M zEQz D zEQ} SR M zEQ} D zGRD SR M zGRD D zIRG SR
M zIRG D zQRJ SR M zQRJ D z[RJ SR M z[RJ D zbRG SR M zbRG D zdRD SR
M zdRD D zgQ} SR M zgQ} D zgQw SR M zgQw D zdQp SR M zdQp D z]Qj SR
M z]Qj D zQQc SR M zQQc D zLQ` SR M zLQ` D zGQZ SR M zGQZ D zEQP SR
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M zdQ} D zdQw SR M zdQw D zbQp SR M zbQp D z[Qj SR M z[Qj D zQQc SR
M zEQM D zGQP SR M zGQP D zLQP SR M zLQP D zXQJ SR M zXQJ D z_QJ SR
M z_QJ D zdQM SR M zdQM D zgQP SR M zLQP D zXQF SR M zXQF D zbQF SR
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M yTOQ D y[OT SR M y[OT D y`O^ SR M y`O^ D ybOn SR M ybOn D ybOx SR
M ybOx D y`PH SR M y`PH D y[PR SR M y[PR D yTPU SR M yTPU D yOPU SR
M yOPU D yJPR SR M yJPR D yHPN SR M yHPN D yEPH SR M yEPH D yCOx SR
M yCOx D yCOn SR M yCOn D yEO^ SR M yEO^ D yHOX SR M yHOX D yJOT SR
M yJOT D yOOQ SR M yTOQ D yYOT SR M yYOT D y[OX SR M y[OX D y^O^ SR
M y^O^ D y`On SR M y`On D y`Ox SR M y`Ox D y^PH SR M y^PH D y[PN SR
M y[PN D yYPR SR M yYPR D yTPU SR M ytOX D yqOT SR M yqOT D ytOQ SR
M ytOQ D yvOT SR M yvOT D ytOX SR M zGPK D zIPH SR M zIPH D zGPE SR
M zGPE D zEPH SR M zEPH D zEPK SR M zEPK D zIPR SR M zIPR D zQPU SR
M zQPU D z[PU SR M z[PU D zbPR SR M zbPR D zdPK SR M zdPK D zdPB SR
M zdPB D zbO{ SR M zbO{ D z[Ox SR M z[Ox D zSOx SR M z[PU D z_PR SR
M z_PR D zbPK SR M zbPK D zbPB SR M zbPB D z_O{ SR M z_O{ D z[Ox SR
M z[Ox D z_Ou SR M z_Ou D zdOn SR M zdOn D zgOh SR M zgOh D zgO^ SR
M zgO^ D zdOX SR M zdOX D zbOT SR M zbOT D z[OQ SR M z[OQ D zQOQ SR
M zQOQ D zIOT SR M zIOT D zGOX SR M zGOX D zEO^ SR M zEO^ D zEOa SR
M zEOa D zGOe SR M zGOe D zIOa SR M zIOa D zGO^ SR M zbOq D zdOh SR
M zdOh D zdO^ SR M zdO^ D zbOX SR M zbOX D z_OT SR M z_OT D z[OQ SR
M HUqT D JQov D LNnX D NJly D PFk[ D RCi} D S?h^ D U{g@ D Wxea D YtdC
D [pbe D ]maF D _i_g D ae^I D cb\j D e^[L D gZYm D iVXN D kSVp D mOUQ
D oKSr D qHRS D sDPt D u@OV D v}Mw SR
M yON\ D yHNY SR M yHNY D yCNO SR M yCNO D y@M? SR M y@M? D y@Mu SR
M y@Mu D yCMe SR M yCMe D yHM[ SR M yHM[ D yOMX SR M yOMX D yTMX SR
M yTMX D y[M[ SR M y[M[ D y`Me SR M y`Me D ybMu SR M ybMu D ybM? SR
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M yON\ D yJNY SR M yJNY D yHNV SR M yHNV D yENO SR M yENO D yCM? SR
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M y[NV D yYNY SR M yYNY D yTN\ SR M ytM_ D yqM[ SR M yqM[ D ytMX SR
M ytMX D yvM[ SR M yvM[ D ytM_ SR M z[NV D z[MX SR M z]N\ D z]MX SR
M z]N\ D zBMl SR M zBMl D ziMl SR M zSMX D zdMX SR
M HUoW D JQmz D LNl] D NJj? D PFib D RChD D S?fg D U{eI D Wxck D YtbM
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D oKQ~ D qHP_ D sDN? D u@M` D v}LA SR
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%PSKCloseWorkStation
%PSKOpenWorkStation
CL
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%DocumentFonts: Times-Bold Times-Italic Symbol Times-Roman
%%Pages: 1
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%%EndDocument
FMENDEPSF
0 56 29 576 727 208 279.2 74 424.4 FMBEGINEPSF
%%BeginDocument: /pongo/data2/drs/ghrs/handbook/ih5/figs/mirror_n2.epsi
%!PS-Adobe-2.0 EPSF-1.2
%%BoundingBox: 56 29 576 727
%!PS-Adobe-1.0
%%Creator: PSIKern - An IRAF GKI Translator
%%CreationDate: Thu 15:08:26 28-Apr-94
%%DocumentFonts: (atend)
%%Pages: (atend)
%%BoundingBox: 28 28 583 763
%%EndComments
/MAXNDC 4095 def /PageSizeXMeter 0.2594 def /PageSizeYMeter 0.1959 def
/PageOffXMeter 0.01 def /PageOffYMeter 0.01 def
/PortraitMode false def /PortraitRotation 0. def
/LandScapeRotation 90. def /GT_LEFT 2 def /GT_RIGHT 3 def
/GT_TOP 6 def /GT_BOTTOM 7 def /GT_UP 4 def /GT_DOWN 5 def
/GT_CENTER 1 def /RF /Times-Roman def /GF /Symbol def
/IF /Times-Italic def /BF /Times-Bold def /DASH 49 def /DOT 4 def
/SPACE 24 def

% How to define things.
/BD { bind def } bind def
/LD { load def } bind def

% Constants
/yes true def
/no false def

% Define some shorthand instructions.
/GRS /grestore LD
/GS /gsave LD
/MK /mark LD
/R /restore LD
/S /save LD
/SH /showpage LD
/SW /setlinewidth LD

% Measurement conversions.
/PointperMeter 2834.64 def
/MonoScale .7 def

% SR: Set current path to page: - -> -
/SR { currentpoint stroke moveto } BD

% CL: CLear the page: - -> -
/CL { restore showpage grestore gsave save } BD

% RC: Read Coordinates: string -> x y
/RC {
currentfile read pop 8#77 and 6 bitshift
currentfile read pop 8#77 and or
currentfile read pop 8#77 and 6 bitshift
currentfile read pop 8#77 and or
} BD

% DO - Determine Offset: length -> offset
/DO { DS dup 0 eq { pop pop 0 } { mod } ifelse } BD

% M: Move: M string -> -
% Move to a point and clear length of path.
/M { RC moveto CT OF setdash } BD

% D: Draw: D string -> -
% This also calculates the length of the current path.
/OF 0 def
/D { RC DS 0 ne { 2 copy currentpoint exch 4 1 roll sub dup mul 3 1 roll
sub dup mul add sqrt round OF add cvi DO /OF exch store } if lineto
} BD

% Character/Font definitions.

% FS -- Define the current font size: xsize ysize FS -
/FontXSize 0 def /FontYSize 0 def /NewFont true def
/FS { /FontYSize exch MonoScale mul store /FontXSize exch MonoScale mul store
/NewFont true store } BD

% PH -- Set the current path: path PH -
/Path 0 def
/PH { /Path exch store } BD

% PA -- Set the path angle of the text: angle PA -
/Angle 0 def
/PA { 360 mod dup 0 lt { 360 add } if /Angle exch store /NewFont true store } BD

% HJ, VJ -- Set Horizontal/Verticle Justification: just HJ/VJ -
/HorzJust 0 def /VertJust 0 def
/HJ { /HorzJust exch store } BD /VJ { /VertJust exch store } BD

% VT -- Use mono- or variable-spaced fonts: flag VT -
/VT true def
/VT { /Variable exch store } BD

% SetFont -- Make the required font the default: font SetFont -
% Note scale factor- This is to fill out monospaced better and match other
% IRAF output.
/Font () def
/FontMatrix matrix def
/SetFont {
dup Font ne NewFont or
{ dup /Font exch store findfont
Angle matrix rotate FontXSize MonoScale div FontYSize MonoScale div
matrix scale matrix concatmatrix makefont setfont Angle matrix rotate
FontXSize FontYSize matrix scale matrix concatmatrix /FontMatrix exch
store
}
{ pop } ifelse /NewFont false store
} BD

% StringWidth -- Determine path length of string: string StringWidth - xs ys
/StringWidth { Path GT_RIGHT eq Variable and { stringwidth }
{ Path GT_RIGHT eq { length } { pop 1 } ifelse 0 FontMatrix transform }
ifelse
} BD

% MonoShow -- Write the string out in mono-spaced: string MonoShow -
/MonoShow {
/t 1 string def 1 0 FontMatrix transform
/dy exch def /dx exch def Path GT_RIGHT eq { /mx dx def /my dy def }
{ 0 1 FontMatrix transform /my exch def /mx exch def } ifelse
{ t 0 3 -1 roll put t dup stringwidth dy exch sub 2 div exch dx exch
sub 2 div exch gsave rmoveto show grestore mx my rmoveto
} forall
} BD

% WS -- Draw the string: string font string ... DS -
/*WSDict 13 dict def
/WS { *WSDict begin
counttomark 2 idiv dup dup array /FontArray exch def
array /StringArray exch def 1 sub /NStrings exch def

NStrings -1 0 {
dup 4 1 roll exch StringArray 3 1 roll put FontArray 3 1 roll put
} for
pop

/XSize 0 def /YSize 0 def /NChars 0 def
0 1 NStrings {
dup FontArray exch get SetFont StringArray exch get dup
length NChars add /NChars exch def StringWidth
YSize add /YSize exch def XSize add /XSize exch def
} for

/TAngle HorzJust GT_RIGHT eq
{ Angle 180 add dup 360 ge { 360 sub } if } { Angle } ifelse def
0 TAngle 180 le HorzJust GT_CENTER eq or
{ Angle sin FontYSize mul Path GT_UP eq { NChars mul } if add } if
TAngle 90 ge TAngle 270 le and HorzJust GT_CENTER eq or
{ Path GT_RIGHT eq { XSize } { Angle cos FontXSize mul } ifelse sub } if
HorzJust GT_CENTER eq { .5 mul } if

/TAngle
VertJust GT_TOP eq { Angle 180 sub dup 0 lt { 360 add } if } { Angle } ifelse
def
0 TAngle 90 ge TAngle 270 le and VertJust GT_CENTER eq or
{ Angle cos FontYSize mul Path GT_UP eq { NChars mul } if sub } if
TAngle 180 ge TAngle 360 le and VertJust GT_CENTER eq or
{ Path GT_RIGHT eq { YSize } { Angle sin FontXSize mul } ifelse sub } if
VertJust GT_CENTER eq { .5 mul } if
rmoveto

0 1 NStrings {
dup FontArray exch get SetFont StringArray exch get
Path GT_RIGHT eq Variable and { show } { MonoShow } ifelse
} for

end
} BD

% Define the DASHED, DOTTED, DOTDASH patterns.
/DS 0 def
/LPS {
/OF 0 store /DS 0 store 0 array
} BD
/LPD {
/OF 0 store DASH SPACE 2 copy add /DS exch store 2 array astore
} BD
/LPP {
/OF 0 store DOT SPACE 2 copy add /DS exch store 2 array astore
} BD
/LDD {
/OF 0 store DOT SPACE DASH SPACE 4 copy add add add /DS exch store
4 array astore
} BD

% LT - Set Line Type - array -> -
/CT { currentdash pop } BD
/LT { /CT exch store /OF 0 store } BD

% SC - Set Color: color -> -
/*SCDict 1 dict def
/SC { *SCDict begin
1 sub /color exch def
GR color get 255 div GG color get 255 div GB color get 255 div setrgbcolor
end
} BD

% MI - Make Image LUT: table-name size MI hexstring -> -
/MI { currentfile exch string readhexstring pop def } BD

% Define the graphics color lookup table.
/GR 16 MI 00FFFF0000FF00FFFFB0FFF0D940F0F5
/GG 16 MI 00FF00FF00FFFF0080D0A6E670E082DE
/GB 16 MI 00FF0000FF00FFFF4F61008CD6D1EFB3

% Render an image when no image LUT has been define.
/DefaultGrey {
{ currentfile inarr readhexstring pop } image
} BD

% ColorImage - Produce an image by indexing into the Image Lookup Table.
% There are two versions of this code- one for PostScript that has
% the colorimage operator and one that doesn't. If the PostScript doesn't
% have colorimage, it is assumed that it can only produce black & white,
% in which the Image LUT is combined to produce a single grey which is
% then used as the image for the image operator.
/colorimage where
{ pop
/ColorImage {
{ currentfile inarr readhexstring pop dup /inarr exch def
length 3 mul string /oarr exch def
0 1 inarr length 1 sub
{ /iindex exch def
/oindex iindex 3 mul def
oarr oindex IR inarr iindex get get put
oarr oindex 1 add IG inarr iindex get get put
oarr oindex 2 add IB inarr iindex get get put
} for
oarr
}
false 3 colorimage
} BD
}
{ /ColorImage {
{ currentfile inarr readhexstring pop dup /inarr exch def
length string /oarr exch def
0 1 inarr length 1 sub
{ /iindex exch def
oarr iindex
IR inarr iindex get get 0.3 mul
IG inarr iindex get get 0.59 mul
IB inarr iindex get get 0.11 mul
add add round cvi dup 255 gt { pop 255 } if
put
} for
oarr
}
image
} BD
}
ifelse

% PC: Put Cellarray: width height bitspersample matrix -> -
/*PCdict 10 dict def
/PC {
*PCdict begin
4 -1 roll dup /inarr exch string def 4 1 roll
/IR where {pop ColorImage} {DefaultGrey} ifelse
end
} BD

% Define the Hatch (fill area) styles. H1 and H2 are handled internally
% by PSIKern. Feel free to define more; there is no limit.
/H3 <8888888888888888> def
/H4 def
/H5 <8844221188442211> def
/H6 <1122448811224488> def

% Setup for fill patterns. This whole section of code is taken almost
% directly from _PostScript Language: Tutorial and Cookbook_, Adobe Systems,
% 1986 (the blue book).
/setuserscreendict 22 dict def
setuserscreendict begin
/tempctm matrix def
/temprot matrix def
/tempscale matrix def

/concatprocs
{ /proc2 exch cvlit def
/proc1 exch cvlit def
/newproc proc1 length proc2 length add
array def
newproc 0 proc1 putinterval
newproc proc1 length proc2 putinterval
newproc cvx
} def

/resmatrix matrix def
/findresolution
{ 72 0 resmatrix defaultmatrix dtransform
/yres exch def /xres exch def
xres dup mul yres dup mul add sqrt
} def
end

/setuserscreen
{ setuserscreendict begin
/spotfunction exch def
/screenangle exch def
/cellsize exch def

/m tempctm currentmatrix def
/rm screenangle temprot rotate def
/sm cellsize dup tempscale scale def

sm rm m m concatmatrix m concatmatrix pop
1 0 m dtransform /y1 exch def /x1 exch def

/veclength x1 dup mul y1 dup mul add sqrt def
/frequency findresolution veclength div def

/newscreenangle y1 x1 atan def

m 2 get m 1 get mul m 0 get m 3 get mul sub
0 gt
{ {neg} /spotfunction load concatprocs
/spotfunction exch def
} if

frequency newscreenangle /spotfunction load
setscreen
end
} def

/setpatterndict 18 dict def
setpatterndict begin
/bitison
{ /ybit exch def /xbit exch def
/bytevalue bstring ybit bwidth mul xbit 8 idiv
add get def

/mask 1 7 xbit 8 mod sub bitshift def
bytevalue mask and 0 ne
} def
end

/bitpatternspotfunction
{ setpatterndict begin
/y exch def /x exch def

/xindex x 1 add 2 div bpside mul cvi def
/yindex y 1 add 2 div bpside mul cvi def

xindex yindex bitison
{ /onbits onbits 1 add def 1 }
{ /offbits offbits 1 add def 0 }
ifelse
end
} def

/setpattern
{ setpatterndict begin
/cellsz exch def
/angle exch def
/bwidth exch def
/bpside exch def
/bstring exch def

/onbits 0 def /offbits 0 def
cellsz angle /bitpatternspotfunction load
setuserscreen
{ } settransfer
offbits offbits onbits add div setgray
end
} def

% SP: Set Pattern: pattern -> -
/SP { 8 1 0 MAXNDC 100 div setpattern } BD

% FI: Fill with Pattern: - -> -
/FI { fill grestore } BD

% Set the transformation matrix.
PointperMeter dup scale
PageOffXMeter
PortraitMode not
{ PageSizeYMeter add }
if
PageOffYMeter translate
PortraitMode
{ PortraitRotation rotate }
{ LandScapeRotation rotate}
ifelse
PageSizeXMeter MAXNDC div PageSizeYMeter MAXNDC div scale
1 setlinejoin 1 setlinecap

% Save the current graphics state (to restore after showpage) and the
% VM state to recover after a showpage.
GS S

%%EndProlog
%PSKOpenWorkStation
%%Page: 1 1
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M KiFY D KiFy SR M NQFY D NQFy SR M PzFY D PzGY SR M SbFY D SbFy SR
M VJFY D VJFy SR M XrFY D XrFy SR M [ZFY D [ZFy SR M ^BFY D ^BGY SR
M `jFY D `jFy SR M cSFY D cSFy SR M e{FY D e{Fy SR M hcFY D hcFy SR
M kKFY D kKGY SR M msFY D msFy SR M p[FY D p[Fy SR M sCFY D sCFy SR
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M QCEh D P}El SR M ]UEl D ]KEh SR M ]KEh D ]EE\ SR M ]EE\ D ]BEG SR
M ]BEG D ]BD{ SR M ]BD{ D ]EDg SR M ]EDg D ]KD[ SR M ]KD[ D ]UDW SR
M ]UDW D ][DW SR M ][DW D ]dD[ SR M ]dD[ D ]jDg SR M ]jDg D ]mD{ SR
M ]mD{ D ]mEG SR M ]mEG D ]jE\ SR M ]jE\ D ]dEh SR M ]dEh D ][El SR
M ][El D ]UEl SR M ]UEl D ]NEh SR M ]NEh D ]KEd SR M ]KEd D ]HE\ SR
M ]HE\ D ]EEG SR M ]EEG D ]ED{ SR M ]ED{ D ]HDg SR M ]HDg D ]KD_ SR
M ]KD_ D ]ND[ SR M ]ND[ D ]UDW SR M ][DW D ]aD[ SR M ]aD[ D ]dD_ SR
M ]dD_ D ]gDg SR M ]gDg D ]jD{ SR M ]jD{ D ]jEG SR M ]jEG D ]gE\ SR
M ]gE\ D ]dEd SR M ]dEd D ]aEh SR M ]aEh D ][El SR M ^BD_ D ]?D[ SR
M ]?D[ D ^BDW SR M ^BDW D ^ED[ SR M ^ED[ D ^BD_ SR M ^^El D ^XEC SR
M ^XEC D ^^EG SR M ^^EG D ^gEL SR M ^gEL D ^pEL SR M ^pEL D ^yEG SR
M ^yEG D ^?D? SR M ^?D? D _BDs SR M _BDs D _BDo SR M _BDo D ^?Dc SR
M ^?Dc D ^yD[ SR M ^yD[ D ^pDW SR M ^pDW D ^gDW SR M ^gDW D ^^D[ SR
M ^^D[ D ^[D_ SR M ^[D_ D ^XDg SR M ^XDg D ^XDk SR M ^XDk D ^[Do SR
M ^[Do D ^^Dk SR M ^^Dk D ^[Dg SR M ^pEL D ^vEG SR M ^vEG D ^|D? SR
M ^|D? D ^?Ds SR M ^?Ds D ^?Do SR M ^?Do D ^|Dc SR M ^|Dc D ^vD[ SR
M ^vD[ D ^pDW SR M ^^El D ^|El SR M ^^Eh D ^mEh SR M ^mEh D ^|El SR
M j?E\ D kEE` SR M kEE` D kNEl SR M kNEl D kNDW SR M kKEh D kKDW SR
M j?DW D kZDW SR M w]E\ D wcE` SR M wcE` D wlEl SR M wlEl D wlDW SR
M wiEh D wiDW SR M w]DW D wxDW SR M xTD_ D xQD[ SR M xQD[ D xTDW SR
M xTDW D xWD[ SR M xWD[ D xTD_ SR M xoEl D xiEC SR M xiEC D xoEG SR
M xoEG D xxEL SR M xxEL D yAEL SR M yAEL D yKEG SR M yKEG D yQD? SR
M yQD? D yTDs SR M yTDs D yTDo SR M yTDo D yQDc SR M yQDc D yKD[ SR
M yKD[ D yADW SR M yADW D xxDW SR M xxDW D xoD[ SR M xoD[ D xlD_ SR
M xlD_ D xiDg SR M xiDg D xiDk SR M xiDk D xlDo SR M xlDo D xoDk SR
M xoDk D xlDg SR M yAEL D yHEG SR M yHEG D yND? SR M yND? D yQDs SR
M yQDs D yQDo SR M yQDo D yNDc SR M yNDc D yHD[ SR M yHD[ D yADW SR
M xoEl D yNEl SR M xoEh D x~Eh SR M x~Eh D yNEl SR M FY|r D |r|r SR
M FY|r D FY|R SR M IA|r D IA|R SR M Ki|r D Ki|R SR M NQ|r D NQ|R SR
M Pz|r D Pz{r SR M Sb|r D Sb|R SR M VJ|r D VJ|R SR M Xr|r D Xr|R SR
M [Z|r D [Z|R SR M ^B|r D ^B{r SR M `j|r D `j|R SR M cS|r D cS|R SR
M e{|r D e{|R SR M hc|r D hc|R SR M kK|r D kK{r SR M ms|r D ms|R SR
M p[|r D p[|R SR M sC|r D sC|R SR M ul|r D ul|R SR M xT|r D xT{r SR
M z||r D z||R SR M FYFY D FY|r SR M FYGT D FyGT SR M FYHL D FyHL SR
M FYHz D FyHz SR M FYIa D FyIa SR M FYJC D FyJC SR M FYJ` D FyJ` SR
M FYJ{ D FyJ{ SR M FYJ{ D GYJ{ SR M FYMj D FyMj SR M FYOP D FyOP SR
M FYPX D FyPX SR M FYQP D FyQP SR M FYQ~ D FyQ~ SR M FYRe D FyRe SR
M FYSG D FySG SR M FYSd D FySd SR M FYS? D FyS? SR M FYS? D GYS? SR
M FYVn D FyVn SR M FYXT D FyXT SR M FYY\ D FyY\ SR M FYZU D FyZU SR
M FY[C D Fy[C SR M FY[i D Fy[i SR M FY\K D Fy\K SR M FY\i D Fy\i SR
M FY]C D Fy]C SR M FY]C D GY]C SR M FY_r D Fy_r SR M FYaX D FyaX SR
M FYb` D Fyb` SR M FYcY D FycY SR M FYdG D FydG SR M FYdm D Fydm SR
M FYeO D FyeO SR M FYem D Fyem SR M FYfG D FyfG SR M FYfG D GYfG SR
M FYhv D Fyhv SR M FYj\ D Fyj\ SR M FYke D Fyke SR M FYl] D Fyl] SR
M FYmK D FymK SR M FYmq D Fymq SR M FYnS D FynS SR M FYnq D Fynq SR
M FYoK D FyoK SR M FYoK D GYoK SR M FYqz D Fyqz SR M FYs` D Fys` SR
M FYti D Fyti SR M FYua D Fyua SR M FYvO D FyvO SR M FYvv D Fyvv SR
M FYwW D FywW SR M FYwu D Fywu SR M FYxO D FyxO SR M FYxO D GYxO SR
M FYz~ D Fyz~ SR M FY|d D Fy|d SR M ByK[ D B?K_ SR M B?K_ D CHKk SR
M CHKk D CHJW SR M CEKg D CEJW SR M ByJW D CTJW SR M C?Kk D CvKg SR
M CvKg D CpK[ SR M CpK[ D ClKG SR M ClKG D ClJ{ SR M ClJ{ D CpJg SR
M CpJg D CvJ[ SR M CvJ[ D C?JW SR M C?JW D DEJW SR M DEJW D DNJ[ SR
M DNJ[ D DTJg SR M DTJg D DWJ{ SR M DWJ{ D DWKG SR M DWKG D DTK[ SR
M DTK[ D DNKg SR M DNKg D DEKk SR M DEKk D C?Kk SR M C?Kk D CyKg SR
M CyKg D CvKc SR M CvKc D CsK[ SR M CsK[ D CpKG SR M CpKG D CpJ{ SR
M CpJ{ D CsJg SR M CsJg D CvJ_ SR M CvJ_ D CyJ[ SR M CyJ[ D C?JW SR
M DEJW D DKJ[ SR M DKJ[ D DNJ_ SR M DNJ_ D DQJg SR M DQJg D DTJ{ SR
M DTJ{ D DTKG SR M DTKG D DQK[ SR M DQK[ D DNKc SR M DNKc D DKKg SR
M DKKg D DEKk SR M EJLY D EGL@ SR M EGL@ D EJLC SR M EJLC D EPLE SR
M EPLE D EULE SR M EULE D E[LC SR M E[LC D E^K~ SR M E^K~ D E`Kw SR
M E`Kw D E`Kt SR M E`Kt D E^Km SR M E^Km D E[Kh SR M E[Kh D EUKf SR
M EUKf D EPKf SR M EPKf D EJKh SR M EJKh D EIKk SR M EIKk D EGKo SR
M EGKo D EGKr SR M EGKr D EIKt SR M EIKt D EJKr SR M EJKr D EIKo SR
M EULE D EYLC SR M EYLC D E]K~ SR M E]K~ D E^Kw SR M E^Kw D E^Kt SR
M E^Kt D E]Km SR M E]Km D EYKh SR M EYKh D EUKf SR M EJLY D E]LY SR
M EJLV D ESLV SR M ESLV D E]LY SR M ByT_ D B?Tc SR M B?Tc D CHTp SR
M CHTp D CHS[ SR M CETk D CES[ SR M ByS[ D CTS[ SR M C?Tp D CvTk SR
M CvTk D CpT_ SR M CpT_ D ClTK SR M ClTK D ClS? SR M ClS? D CpSk SR
M CpSk D CvS_ SR M CvS_ D C?S[ SR M C?S[ D DES[ SR M DES[ D DNS_ SR
M DNS_ D DTSk SR M DTSk D DWS? SR M DWS? D DWTK SR M DWTK D DTT_ SR
M DTT_ D DNTk SR M DNTk D DETp SR M DETp D C?Tp SR M C?Tp D CyTk SR
M CyTk D CvTg SR M CvTg D CsT_ SR M CsT_ D CpTK SR M CpTK D CpS? SR
M CpS? D CsSk SR M CsSk D CvSc SR M CvSc D CyS_ SR M CyS_ D C?S[ SR
M DES[ D DKS_ SR M DKS_ D DNSc SR M DNSc D DQSk SR M DQSk D DTS? SR
M DTS? D DTTK SR M DTTK D DQT_ SR M DQT_ D DNTg SR M DNTg D DKTk SR
M DKTk D DETp SR M E]UU D E[US SR M E[US D E]UQ SR M E]UQ D E^US SR
M E^US D E^UU SR M E^UU D E]UZ SR M E]UZ D EYU] SR M EYU] D ESU] SR
M ESU] D ENUZ SR M ENUZ D EJUU SR M EJUU D EIUQ SR M EIUQ D EGUG SR
M EGUG D EGTx SR M EGTx D EITq SR M EITq D ELTl SR M ELTl D ERTj SR
M ERTj D EUTj SR M EUTj D E[Tl SR M E[Tl D E^Tq SR M E^Tq D E`Tx SR
M E`Tx D E`T{ SR M E`T{ D E^UB SR M E^UB D E[UG SR M E[UG D EUUI SR
M EUUI D ESUI SR M ESUI D ENUG SR M ENUG D EJUB SR M EJUB D EIT{ SR
M ESU] D EPUZ SR M EPUZ D ELUU SR M ELUU D EJUQ SR M EJUQ D EIUG SR
M EIUG D EITx SR M EITx D EJTq SR M EJTq D ENTl SR M ENTl D ERTj SR
M EUTj D EYTl SR M EYTl D E]Tq SR M E]Tq D E^Tx SR M E^Tx D E^T{ SR
M E^T{ D E]UB SR M E]UB D EYUG SR M EYUG D EUUI SR M By]c D B?]h SR
M B?]h D CH]t SR M CH]t D CH\_ SR M CE]p D CE\_ SR M By\_ D CT\_ SR
M C?]t D Cv]p SR M Cv]p D Cp]c SR M Cp]c D Cl]O SR M Cl]O D Cl]C SR
M Cl]C D Cp\o SR M Cp\o D Cv\c SR M Cv\c D C?\_ SR M C?\_ D DE\_ SR
M DE\_ D DN\c SR M DN\c D DT\o SR M DT\o D DW]C SR M DW]C D DW]O SR
M DW]O D DT]c SR M DT]c D DN]p SR M DN]p D DE]t SR M DE]t D C?]t SR
M C?]t D Cy]p SR M Cy]p D Cv]l SR M Cv]l D Cs]c SR M Cs]c D Cp]O SR
M Cp]O D Cp]C SR M Cp]C D Cs\o SR M Cs\o D Cv\g SR M Cv\g D Cy\c SR
M Cy\c D C?\_ SR M DE\_ D DK\c SR M DK\c D DN\g SR M DN\g D DQ\o SR
M DQ\o D DT]C SR M DT]C D DT]O SR M DT]O D DQ]c SR M DQ]c D DN]l SR
M DN]l D DK]p SR M DK]p D DE]t SR M EG^a D EG^R SR M EG^W D EI^\ SR
M EI^\ D EL^a SR M EL^a D EP^a SR M EP^a D EY^Z SR M EY^Z D E]^Z SR
M E]^Z D E^^\ SR M E^^\ D E`^a SR M EI^\ D EL^^ SR M EL^^ D EP^^ SR
M EP^^ D EY^Z SR M E`^a D E`^Z SR M E`^Z D E^^R SR M E^^R D EW^F SR
M EW^F D EU^A SR M EU^A D ES]z SR M ES]z D ES]n SR M E^^R D EU^F SR
M EU^F D ES^A SR M ES^A D ER]z SR M ER]z D ER]n SR M Byfh D B?fl SR
M B?fl D CHfx SR M CHfx D CHec SR M CEft D CEec SR M Byec D CTec SR
M C?fx D Cvft SR M Cvft D Cpfh SR M Cpfh D ClfS SR M ClfS D ClfG SR
M ClfG D Cpes SR M Cpes D Cveg SR M Cveg D C?ec SR M C?ec D DEec SR
M DEec D DNeg SR M DNeg D DTes SR M DTes D DWfG SR M DWfG D DWfS SR
M DWfS D DTfh SR M DTfh D DNft SR M DNft D DEfx SR M DEfx D C?fx SR
M C?fx D Cyft SR M Cyft D Cvfp SR M Cvfp D Csfh SR M Csfh D CpfS SR
M CpfS D CpfG SR M CpfG D Cses SR M Cses D Cvek SR M Cvek D Cyeg SR
M Cyeg D C?ec SR M DEec D DKeg SR M DKeg D DNek SR M DNek D DQes SR
M DQes D DTfG SR M DTfG D DTfS SR M DTfS D DQfh SR M DQfh D DNfp SR
M DNfp D DKft SR M DKft D DEfx SR M EPge D EJgc SR M EJgc D EIg^ SR
M EIg^ D EIgV SR M EIgV D EJgR SR M EJgR D EPgO SR M EPgO D EWgO SR
M EWgO D E]gR SR M E]gR D E^gV SR M E^gV D E^g^ SR M E^g^ D E]gc SR
M E]gc D EWge SR M EWge D EPge SR M EPge D ELgc SR M ELgc D EJg^ SR
M EJg^ D EJgV SR M EJgV D ELgR SR M ELgR D EPgO SR M EWgO D E[gR SR
M E[gR D E]gV SR M E]gV D E]g^ SR M E]g^ D E[gc SR M E[gc D EWge SR
M EPgO D EJgM SR M EJgM D EIgJ SR M EIgJ D EGgE SR M EGgE D EGf| SR
M EGf| D EIfw SR M EIfw D EJfu SR M EJfu D EPfr SR M EPfr D EWfr SR
M EWfr D E]fu SR M E]fu D E^fw SR M E^fw D E`f| SR M E`f| D E`gE SR
M E`gE D E^gJ SR M E^gJ D E]gM SR M E]gM D EWgO SR M EPgO D ELgM SR
M ELgM D EJgJ SR M EJgJ D EIgE SR M EIgE D EIf| SR M EIf| D EJfw SR
M EJfw D ELfu SR M ELfu D EPfr SR M EWfr D E[fu SR M E[fu D E]fw SR
M E]fw D E^f| SR M E^f| D E^gE SR M E^gE D E]gJ SR M E]gJ D E[gM SR
M E[gM D EWgO SR M Byol D B?op SR M B?op D CHo| SR M CHo| D CHng SR
M CEox D CEng SR M Byng D CTng SR M C?o| D Cvox SR M Cvox D Cpol SR
M Cpol D CloX SR M CloX D CloK SR M CloK D Cpnw SR M Cpnw D Cvnk SR
M Cvnk D C?ng SR M C?ng D DEng SR M DEng D DNnk SR M DNnk D DTnw SR
M DTnw D DWoK SR M DWoK D DWoX SR M DWoX D DTol SR M DTol D DNox SR
M DNox D DEo| SR M DEo| D C?o| SR M C?o| D Cyox SR M Cyox D Cvot SR
M Cvot D Csol SR M Csol D CpoX SR M CpoX D CpoK SR M CpoK D Csnw SR
M Csnw D Cvno SR M Cvno D Cynk SR M Cynk D C?ng SR M DEng D DKnk SR
M DKnk D DNno SR M DNno D DQnw SR M DQnw D DToK SR M DToK D DToX SR
M DToX D DQol SR M DQol D DNot SR M DNot D DKox SR M DKox D DEo| SR
M E^pX D E]pQ SR M E]pQ D EYpL SR M EYpL D ESpJ SR M ESpJ D ERpJ SR
M ERpJ D ELpL SR M ELpL D EIpQ SR M EIpQ D EGpX SR M EGpX D EGp[ SR
M EGp[ D EIpb SR M EIpb D ELpg SR M ELpg D ERpi SR M ERpi D EUpi SR
M EUpi D E[pg SR M E[pg D E^pb SR M E^pb D E`p[ SR M E`p[ D E`pL SR
M E`pL D E^pB SR M E^pB D E]o} SR M E]o} D EYoy SR M EYoy D ESov SR
M ESov D ENov SR M ENov D EJoy SR M EJoy D EIo} SR M EIo} D EIp@ SR
M EIp@ D EJpB SR M EJpB D ELp@ SR M ELp@ D EJo} SR M ERpJ D ENpL SR
M ENpL D EJpQ SR M EJpQ D EIpX SR M EIpX D EIp[ SR M EIp[ D EJpb SR
M EJpb D ENpg SR M ENpg D ERpi SR M EUpi D EYpg SR M EYpg D E]pb SR
M E]pb D E^p[ SR M E^p[ D E^pL SR M E^pL D E]pB SR M E]pB D E[o} SR
M E[o} D EWoy SR M EWoy D ESov SR M Buxp D B{xt SR M B{xt D CDy@ SR
M CDy@ D CDwk SR M CAx| D CAwk SR M Buwk D CPwk SR M C{y@ D Crx| SR
M Crx| D Clxp SR M Clxp D Cix\ SR M Cix\ D CixP SR M CixP D Clw{ SR
M Clw{ D Crwo SR M Crwo D C{wk SR M C{wk D DAwk SR M DAwk D DJwo SR
M DJwo D DPw{ SR M DPw{ D DSxP SR M DSxP D DSx\ SR M DSx\ D DPxp SR
M DPxp D DJx| SR M DJx| D DAy@ SR M DAy@ D C{y@ SR M C{y@ D Cux| SR
M Cux| D Crxx SR M Crxx D Coxp SR M Coxp D Clx\ SR M Clx\ D ClxP SR
M ClxP D Cow{ SR M Cow{ D Crws SR M Crws D Cuwo SR M Cuwo D C{wk SR
M DAwk D DGwo SR M DGwo D DJws SR M DJws D DMw{ SR M DMw{ D DPxP SR
M DPxP D DPx\ SR M DPx\ D DMxp SR M DMxp D DJxx SR M DJxx D DGx| SR
M DGx| D DAy@ SR M Dhyd D Dkyf SR M Dkyf D Dqym SR M Dqym D Dqxz SR
M Doyk D Doxz SR M Dhxz D Dxxz SR M ERym D ELyk SR M ELyk D EIyd SR
M EIyd D EGyW SR M EGyW D EGyP SR M EGyP D EIyD SR M EIyD D ELx} SR
M ELx} D ERxz SR M ERxz D EUxz SR M EUxz D E[x} SR M E[x} D E^yD SR
M E^yD D E`yP SR M E`yP D E`yW SR M E`yW D E^yd SR M E^yd D E[yk SR
M E[yk D EUym SR M EUym D ERym SR M ERym D ENyk SR M ENyk D ELyh SR
M ELyh D EJyd SR M EJyd D EIyW SR M EIyW D EIyP SR M EIyP D EJyD SR
M EJyD D ELx? SR M ELx? D ENx} SR M ENx} D ERxz SR M EUxz D EYx} SR
M EYx} D E[x? SR M E[x? D E]yD SR M E]yD D E^yP SR M E^yP D E^yW SR
M E^yW D E]yd SR M E]yd D E[yh SR M E[yh D EYyk SR M EYyk D EUym SR
M |rFY D |r|r SR M |rGT D |RGT SR M |rHL D |RHL SR M |rHz D |RHz SR
M |rIa D |RIa SR M |rJC D |RJC SR M |rJ` D |RJ` SR M |rJ{ D |RJ{ SR
M |rJ{ D {rJ{ SR M |rMj D |RMj SR M |rOP D |ROP SR M |rPX D |RPX SR
M |rQP D |RQP SR M |rQ~ D |RQ~ SR M |rRe D |RRe SR M |rSG D |RSG SR
M |rSd D |RSd SR M |rS? D |RS? SR M |rS? D {rS? SR M |rVn D |RVn SR
M |rXT D |RXT SR M |rY\ D |RY\ SR M |rZU D |RZU SR M |r[C D |R[C SR
M |r[i D |R[i SR M |r\K D |R\K SR M |r\i D |R\i SR M |r]C D |R]C SR
M |r]C D {r]C SR M |r_r D |R_r SR M |raX D |RaX SR M |rb` D |Rb` SR
M |rcY D |RcY SR M |rdG D |RdG SR M |rdm D |Rdm SR M |reO D |ReO SR
M |rem D |Rem SR M |rfG D |RfG SR M |rfG D {rfG SR M |rhv D |Rhv SR
M |rj\ D |Rj\ SR M |rke D |Rke SR M |rl] D |Rl] SR M |rmK D |RmK SR
M |rmq D |Rmq SR M |rnS D |RnS SR M |rnq D |Rnq SR M |roK D |RoK SR
M |roK D {roK SR M |rqz D |Rqz SR M |rs` D |Rs` SR M |rti D |Rti SR
M |rua D |Rua SR M |rvO D |RvO SR M |rvv D |Rvv SR M |rwW D |RwW SR
M |rwu D |Rwu SR M |rxO D |RxO SR M |rxO D {rxO SR M |rz~ D |Rz~ SR
M |r|d D |R|d SR
M @^Ub D @dUf SR M @dUf D @TUf SR M @TUf D @^Ub SR M @^Ub D @WUZ SR
M @WUZ D @TUN SR M @TUN D @TUF SR M @TUF D @WTz SR M @WTz D @^Tq SR
M @^Tq D @dTm SR M @dTm D @mTi SR M @mTi D @|Ti SR M @|Ti D AETm SR
M AETm D AKTq SR M AKTq D AQTz SR M AQTz D ATUF SR M ATUF D ATUN SR
M ATUN D AQUZ SR M AQUZ D AKUb SR M AKUb D AEUf SR M @TUF D @WT~ SR
M @WT~ D @^Tv SR M @^Tv D @dTq SR M @dTq D @mTm SR M @mTm D @|Tm SR
M @|Tm D AETq SR M AETq D AKTv SR M AKTv D AQT~ SR M AQT~ D ATUF SR
M @jVV D @mVJ SR M @mVJ D @sVB SR M @sVB D @|U~ SR M @|U~ D ABU~ SR
M ABU~ D AKVB SR M AKVB D AQVJ SR M AQVJ D ATVV SR M ATVV D ATV^ SR
M ATV^ D AQVk SR M AQVk D AKVs SR M AKVs D ABVw SR M ABVw D @|Vw SR
M @|Vw D @sVs SR M @sVs D @mVk SR M @mVk D @jV^ SR M @jV^ D @jVV SR
M @jVV D @mVN SR M @mVN D @sVF SR M @sVF D @|VB SR M @|VB D ABVB SR
M ABVB D AKVF SR M AKVF D AQVN SR M AQVN D ATVV SR M ATV^ D AQVf SR
M AQVf D AKVo SR M AKVo D ABVs SR M ABVs D @|Vs SR M @|Vs D @sVo SR
M @sVo D @mVf SR M @mVf D @jV^ SR M @jWW D AKWW SR M AKWW D AQW[ SR
M AQW[ D ATWg SR M ATWg D ATWo SR M ATWo D AQW{ SR M AQW{ D AKXC SR
M @jW[ D AKW[ SR M AKW[ D AQW_ SR M AQW_ D ATWg SR M @jXC D ATXC SR
M @jXG D ATXG SR M @jWK D @jW[ SR M @jWw D @jXG SR M ATXC D ATXS SR
M @jXp D ATXp SR M @jXt D ATXt SR M @sXt D @mX| SR M @mX| D @jYH SR
M @jYH D @jYP SR M @jYP D @mY\ SR M @mY\ D @sY` SR M @sY` D ATY` SR
M @jYP D @mYX SR M @mYX D @sY\ SR M @sY\ D ATY\ SR M @jXd D @jXt SR
M ATXd D ATY@ SR M ATYP D ATYl SR M @TZH D AHZH SR M AHZH D AQZM SR
M AQZM D ATZU SR M ATZU D ATZ] SR M ATZ] D AQZe SR M AQZe D AKZi SR
M @TZM D AHZM SR M AHZM D AQZQ SR M AQZQ D ATZU SR M @jY| D @jZ] SR
M @T\N D AT\N SR M @T\R D AT\R SR M @T\A D @T\r SR M @T\r D @W\~ SR
M @W\~ D @Z]B SR M @Z]B D @a]F SR M @a]F D @g]F SR M @g]F D @m]B SR
M @m]B D @p\~ SR M @p\~ D @s\r SR M @s\r D @s\R SR M @T\r D @W\z SR
M @W\z D @Z\~ SR M @Z\~ D @a]B SR M @a]B D @g]B SR M @g]B D @m\~ SR
M @m\~ D @p\z SR M @p\z D @s\r SR M AT\A D AT\^ SR M @s\j D AN\z SR
M AN\z D AT]B SR M AT]B D AT]J SR M AT]J D AN]N SR M @s\j D @y\r SR
M @y\r D AT]B SR M @p]f D @s]f SR M @s]f D @s]b SR M @s]b D @p]b SR
M @p]b D @m]f SR M @m]f D @j]n SR M @j]n D @j]? SR M @j]? D @m^G SR
M @m^G D @p^K SR M @p^K D @v^O SR M @v^O D AK^O SR M AK^O D AQ^S SR
M AQ^S D AT^W SR M @p^K D AK^K SR M AK^K D AQ^O SR M AQ^O D AT^W SR
M AT^W D AT^[ SR M @v^K D @y^G SR M @y^G D @|]n SR M @|]n D @?]b SR
M @?]b D AE]^ SR M AE]^ D AK]^ SR M AK]^ D AQ]b SR M AQ]b D AT]n SR
M AT]n D AT]z SR M AT]z D AQ^C SR M AQ^C D AK^K SR M @|]n D @?]f SR
M @?]f D AE]b SR M AE]b D AK]b SR M AK]b D AQ]f SR M AQ]f D AT]n SR
M @T^w D AH^w SR M AH^w D AQ^{ SR M AQ^{ D AT_C SR M AT_C D AT_K SR
M AT_K D AQ_S SR M AQ_S D AK_W SR M @T^{ D AH^{ SR M AH^{ D AQ^? SR
M AQ^? D AT_C SR M @j^k D @j_K SR M @|_p D @|`` SR M @|`` D @v`` SR
M @v`` D @p`\ SR M @p`\ D @m`X SR M @m`X D @j`P SR M @j`P D @j`D SR
M @j`D D @m_x SR M @m_x D @s_p SR M @s_p D @|_k SR M @|_k D AB_k SR
M AB_k D AK_p SR M AK_p D AQ_x SR M AQ_x D AT`D SR M AT`D D AT`L SR
M AT`L D AQ`X SR M AQ`X D AK`` SR M @|`\ D @s`\ SR M @s`\ D @m`X SR
M @j`D D @m_| SR M @m_| D @s_t SR M @s_t D @|_p SR M @|_p D AB_p SR
M AB_p D AK_t SR M AK_t D AQ_| SR M AQ_| D AT`D SR M @Hba D @NbY SR
M @NbY D @WbQ SR M @WbQ D @dbI SR M @dbI D @sbE SR M @sbE D @?bE SR
M @?bE D ANbI SR M ANbI D AZbQ SR M AZbQ D AdbY SR M AdbY D Ajba SR
M @NbY D @ZbQ SR M @ZbQ D @dbM SR M @dbM D @sbI SR M @sbI D @?bI SR
M @?bI D ANbM SR M ANbM D AWbQ SR M AWbQ D AdbY SR M @scj D @vcf SR
M @vcf D @ycj SR M @ycj D @vcn SR M @vcn D @scn SR M @scn D @mcf SR
M @mcf D @jc^ SR M @jc^ D @jcQ SR M @jcQ D @mcE SR M @mcE D @sb} SR
M @sb} D @|by SR M @|by D ABby SR M ABby D AKb} SR M AKb} D AQcE SR
M AQcE D ATcQ SR M ATcQ D ATcZ SR M ATcZ D AQcf SR M AQcf D AKcn SR
M @jcQ D @mcI SR M @mcI D @scA SR M @scA D @|b} SR M @|b} D ABb} SR
M ABb} D AKcA SR M AKcA D AQcI SR M AQcI D ATcQ SR M @jd^ D @mdR SR
M @mdR D @sdJ SR M @sdJ D @|dF SR M @|dF D ABdF SR M ABdF D AKdJ SR
M AKdJ D AQdR SR M AQdR D ATd^ SR M ATd^ D ATdf SR M ATdf D AQdr SR
M AQdr D AKdz SR M AKdz D ABd~ SR M ABd~ D @|d~ SR M @|d~ D @sdz SR
M @sdz D @mdr SR M @mdr D @jdf SR M @jdf D @jd^ SR M @jd^ D @mdV SR
M @mdV D @sdN SR M @sdN D @|dJ SR M @|dJ D ABdJ SR M ABdJ D AKdN SR
M AKdN D AQdV SR M AQdV D ATd^ SR M ATdf D AQdn SR M AQdn D AKdv SR
M AKdv D ABdz SR M ABdz D @|dz SR M @|dz D @sdv SR M @sdv D @mdn SR
M @mdn D @jdf SR M @je_ D AKe_ SR M AKe_ D AQec SR M AQec D ATeo SR
M ATeo D ATew SR M ATew D AQfC SR M AQfC D AKfK SR M @jec D AKec SR
M AKec D AQeg SR M AQeg D ATeo SR M @jfK D ATfK SR M @jfO D ATfO SR
M @jeR D @jec SR M @je? D @jfO SR M ATfK D ATf[ SR M @jfw D ATfw SR
M @jf{ D ATf{ SR M @sf{ D @mgC SR M @mgC D @jgP SR M @jgP D @jgX SR
M @jgX D @mgd SR M @mgd D @sgh SR M @sgh D ATgh SR M @jgX D @mg` SR
M @mg` D @sgd SR M @sgd D ATgd SR M @jfk D @jf{ SR M ATfk D ATgH SR
M ATgX D ATgt SR M @ThP D AHhP SR M AHhP D AQhT SR M AQhT D ATh\ SR
M ATh\ D AThd SR M AThd D AQhl SR M AQhl D AKhp SR M @ThT D AHhT SR
M AHhT D AQhX SR M AQhX D ATh\ SR M @jhD D @jhd SR M @mim D @jiq SR
M @jiq D @siq SR M @siq D @mim SR M @mim D @jia SR M @jia D @jiU SR
M @jiU D @miI SR M @miI D @piE SR M @piE D @siE SR M @siE D @yiI SR
M @yiI D @|iQ SR M @|iQ D ABie SR M ABie D AEim SR M AEim D AHiq SR
M @siE D @viI SR M @viI D @yiQ SR M @yiQ D @?ie SR M @?ie D ABim SR
M ABim D AHiq SR M AHiq D ANiq SR M ANiq D AQim SR M AQim D ATia SR
M ATia D ATiU SR M ATiU D AQiI SR M AQiI D AKiE SR M AKiE D ATiE SR
M ATiE D AQiI SR M @mkz D @jk~ SR M @jk~ D @sk~ SR M @sk~ D @mkz SR
M @mkz D @jkn SR M @jkn D @jkb SR M @jkb D @mkV SR M @mkV D @pkR SR
M @pkR D @skR SR M @skR D @ykV SR M @ykV D @|k^ SR M @|k^ D ABkr SR
M ABkr D AEkz SR M AEkz D AHk~ SR M @skR D @vkV SR M @vkV D @yk^ SR
M @yk^ D @?kr SR M @?kr D ABkz SR M ABkz D AHk~ SR M AHk~ D ANk~ SR
M ANk~ D AQkz SR M AQkz D ATkn SR M ATkn D ATkb SR M ATkb D AQkV SR
M AQkV D AKkR SR M AKkR D ATkR SR M ATkR D AQkV SR M @HlR D @Hl} SR
M @@mS D @@mX SR M @@mX D @@m_ SR M @@m_ D @Ym_ SR M @@m] D @Ym] SR
M @YmS D @Ymi SR M @HnA D @NnI SR M @NnI D @WnQ SR M @WnQ D @dnY SR
M @dnY D @sn] SR M @sn] D @?n] SR M @?n] D ANnY SR M ANnY D AZnQ SR
M AZnQ D AdnI SR M AdnI D AjnA SR M @NnI D @ZnQ SR M @ZnQ D @dnU SR
M @dnU D @snY SR M @snY D @?nY SR M @?nY D ANnU SR M ANnU D AWnQ SR
M AWnQ D AdnI SR
M _bBo D _\Bg SR M _\Bg D _VB[ SR M _VB[ D _PBK SR M _PBK D _MAw SR
M _MAw D _MAg SR M _MAg D _PAR SR M _PAR D _VAB SR M _VAB D _\@v SR
M _\@v D _b@n SR M _\Bg D _VBW SR M _VBW D _SBK SR M _SBK D _PAw SR
M _PAw D _PAg SR M _PAg D _SAR SR M _SAR D _VAF SR M _VAF D _\@v SR
M _{B_ D _{AJ SR M _~B_ D _~AJ SR M _rB_ D `VB_ SR M `VB_ D `_B[ SR
M `_B[ D `bBW SR M `bBW D `eBO SR M `eBO D `eBG SR M `eBG D `bA? SR
M `bA? D `_A{ SR M `_A{ D `VAw SR M `VB_ D `\B[ SR M `\B[ D `_BW SR
M `_BW D `bBO SR M `bBO D `bBG SR M `bBG D `_A? SR M `_A? D `\A{ SR
M `\A{ D `VAw SR M _~Aw D `VAw SR M `VAw D `_As SR M `_As D `bAo SR
M `bAo D `eAg SR M `eAg D `eAZ SR M `eAZ D `bAR SR M `bAR D `_AN SR
M `_AN D `VAJ SR M `VAJ D _rAJ SR M `VAw D `\As SR M `\As D `_Ao SR
M `_Ao D `bAg SR M `bAg D `bAZ SR M `bAZ D `_AR SR M `_AR D `\AN SR
M `\AN D `VAJ SR M `xAo D anAo SR M bDB_ D bYAJ SR M bGB_ D bYAV SR
M bnB_ D bYAJ SR M a{B_ D bPB_ SR M beB_ D bxB_ SR M cDBo D cJBg SR
M cJBg D cPB[ SR M cPB[ D cVBK SR M cVBK D cYAw SR M cYAw D cYAg SR
M cYAg D cVAR SR M cVAR D cPAB SR M cPAB D cJ@v SR M cJ@v D cD@n SR
M cJBg D cPBW SR M cPBW D cSBK SR M cSBK D cVAw SR M cVAw D cVAg SR
M cVAg D cSAR SR M cSAR D cPAF SR M cPAF D cJ@v SR M cvAe D cpAb SR
M cpAb D cmA[ SR M cmA[ D ckAO SR M ckAO D ckAH SR M ckAH D cm@| SR
M cm@| D cp@t SR M cp@t D cv@r SR M cv@r D cy@r SR M cy@r D c?@t SR
M c?@t D dC@| SR M dC@| D dDAH SR M dDAH D dDAO SR M dDAO D dCA[ SR
M dCA[ D c?Ab SR M c?Ab D cyAe SR M cyAe D cvAe SR M cvAe D crAb SR
M crAb D cpA` SR M cpA` D cnA[ SR M cnA[ D cmAO SR M cmAO D cmAH SR
M cmAH D cn@| SR M cn@| D cp@w SR M cp@w D cr@t SR M cr@t D cv@r SR
M cy@r D c}@t SR M c}@t D c?@w SR M c?@w D dA@| SR M dA@| D dCAH SR
M dCAH D dCAO SR M dCAO D dAA[ SR M dAA[ D c?A` SR M c?A` D c}Ab SR
M c}Ab D cyAe SR
M k]pF D k]n` SR M kapF D lMnj SR M kao| D lMn` SR M lMpF D lMn` SR
M kRpF D kapF SR M lBpF D lXpF SR M kRn` D khn` SR M lnor D lqom SR
M lqom D lnoi SR M lnoi D ljom SR M ljom D ljor SR M ljor D lno| SR
M lno| D lqpA SR M lqpA D l|pF SR M l|pF D mKpF SR M mKpF D mVpA SR
M mVpA D mZo| SR M mZo| D m]or SR M m]or D m]oi SR M m]oi D mZo_ SR
M mZo_ D mOoU SR M mOoU D l|oK SR M l|oK D luoG SR M luoG D lnn} SR
M lnn} D ljnn SR M ljnn D ljn` SR M mKpF D mRpA SR M mRpA D mVo| SR
M mVo| D mZor SR M mZor D mZoi SR M mZoi D mVo_ SR M mVo_ D mKoU SR
M mKoU D l|oK SR M ljnj D lnnn SR M lnnn D lunn SR M lunn D mGne SR
M mGne D mRne SR M mRne D mZnj SR M mZnj D m]nn SR M lunn D mGn` SR
M mGn` D mVn` SR M mVn` D mZne SR M mZne D m]nn SR M m]nn D m]nx SR
M Gm{b D IAxX D JUui D KisQ D L}qO D NQo` D Oen@ D Pzlo D RNki D Sbjm
D Tviy D VJiK D W^hb D Xrg| D ZFgW D [Zft D \nfP D ^Bek D _VeC D `jdZ
D a~cm D cSb} D dgbI D e{aR D gO`W D hc_Z D iw^Y D kK]V D l_\Q D ms[L
D oGZG D p[YC D qoXA D sCWD D tXVK D ulUZ D w@Tq D xTTS SR
M y~T} D ywTz SR M ywTz D yrTp SR M yrTp D yoT` SR M yoT` D yoTV SR
M yoTV D yrTF SR M yrTF D ywS| SR M ywS| D y~Sy SR M y~Sy D zCSy SR
M zCSy D zJS| SR M zJS| D zOTF SR M zOTF D zQTV SR M zQTV D zQT` SR
M zQT` D zOTp SR M zOTp D zJTz SR M zJTz D zCT} SR M zCT} D y~T} SR
M y~T} D yyTz SR M yyTz D ywTw SR M ywTw D ytTp SR M ytTp D yrT` SR
M yrT` D yrTV SR M yrTV D ytTF SR M ytTF D ywT@ SR M ywT@ D yyS| SR
M yyS| D y~Sy SR M zCSy D zHS| SR M zHS| D zJT@ SR M zJT@ D zLTF SR
M zLTF D zOTV SR M zOTV D zOT` SR M zOT` D zLTp SR M zLTp D zJTw SR
M zJTw D zHTz SR M zHTz D zCT} SR M zbT@ D z`S| SR M z`S| D zbSy SR
M zbSy D zeS| SR M zeS| D zbT@ SR M {BT} D z{Tz SR M z{Tz D zvTp SR
M zvTp D zsT` SR M zsT` D zsTV SR M zsTV D zvTF SR M zvTF D z{S| SR
M z{S| D {BSy SR M {BSy D {GSy SR M {GSy D {NS| SR M {NS| D {STF SR
M {STF D {VTV SR M {VTV D {VT` SR M {VT` D {STp SR M {STp D {NTz SR
M {NTz D {GT} SR M {GT} D {BT} SR M {BT} D z}Tz SR M z}Tz D z{Tw SR
M z{Tw D zxTp SR M zxTp D zvT` SR M zvT` D zvTV SR M zvTV D zxTF SR
M zxTF D z{T@ SR M z{T@ D z}S| SR M z}S| D {BSy SR M {GSy D {LS| SR
M {LS| D {NT@ SR M {NT@ D {QTF SR M {QTF D {STV SR M {STV D {ST` SR
M {ST` D {QTp SR M {QTp D {NTw SR M {NTw D {LTz SR M {LTz D {GT} SR
M Gmxr D IAuh D JUry D Kipc D L}nb D NQlt D OekV D PzjG D RNiC D SbhJ
D TvgX D VJfm D W^fF D Xreb D ZFe@ D [Zd_ D \nc} D ^BcZ D _Vbu D `jbM
D a~ab D cS`s D dg`A D e{_K D gO^Q D hc]T D iw\U D kK[R D l_ZN D msYI
D oGXE D p[WA D qoV@ D sCUB D tXTJ D ulSY D w@Rq D xTRT SR
M y~Rx D ywRt SR M ywRt D yrRk SR M yrRk D yoR[ SR M yoR[ D yoRQ SR
M yoRQ D yrRA SR M yrRA D ywQw SR M ywQw D y~Qt SR M y~Qt D zCQt SR
M zCQt D zJQw SR M zJQw D zORA SR M zORA D zQRQ SR M zQRQ D zQR[ SR
M zQR[ D zORk SR M zORk D zJRt SR M zJRt D zCRx SR M zCRx D y~Rx SR
M y~Rx D yyRt SR M yyRt D ywRq SR M ywRq D ytRk SR M ytRk D yrR[ SR
M yrR[ D yrRQ SR M yrRQ D ytRA SR M ytRA D ywQz SR M ywQz D yyQw SR
M yyQw D y~Qt SR M zCQt D zHQw SR M zHQw D zJQz SR M zJQz D zLRA SR
M zLRA D zORQ SR M zORQ D zOR[ SR M zOR[ D zLRk SR M zLRk D zJRq SR
M zJRq D zHRt SR M zHRt D zCRx SR M zbQz D z`Qw SR M z`Qw D zbQt SR
M zbQt D zeQw SR M zeQw D zbQz SR M z{Rk D {@Rn SR M {@Rn D {GRx SR
M {GRx D {GQt SR M {ERt D {EQt SR M z{Qt D {QQt SR
M GmvE D IAr{ D JUpM D Kimx D L}ky D NQjL D Oehq D Pzgc D RNfb D Sbej
D Tvd{ D VJdR D W^cm D XrcL D ZFbl D [ZbL D \nam D ^BaK D _V`h D `j`B
D a~_X D cS^k D dg]z D e{]E D gO\L D hc[P D iwZQ D kKYO D l_XL D msWG
D oGVC D p[T? D qoS~ D sCSA D tXRJ D ulQY D w@Pq D xTPU SR
M y~P~ D ywP{ SR M ywP{ D yrPq SR M yrPq D yoPa SR M yoPa D yoPW SR
M yoPW D yrPG SR M yrPG D ywO} SR M ywO} D y~Oz SR M y~Oz D zCOz SR
M zCOz D zJO} SR M zJO} D zOPG SR M zOPG D zQPW SR M zQPW D zQPa SR
M zQPa D zOPq SR M zOPq D zJP{ SR M zJP{ D zCP~ SR M zCP~ D y~P~ SR
M y~P~ D yyP{ SR M yyP{ D ywPw SR M ywPw D ytPq SR M ytPq D yrPa SR
M yrPa D yrPW SR M yrPW D ytPG SR M ytPG D ywPA SR M ywPA D yyO} SR
M yyO} D y~Oz SR M zCOz D zHO} SR M zHO} D zJPA SR M zJPA D zLPG SR
M zLPG D zOPW SR M zOPW D zOPa SR M zOPa D zLPq SR M zLPq D zJPw SR
M zJPw D zHP{ SR M zHP{ D zCP~ SR M zbPA D z`O} SR M z`O} D zbOz SR
M zbOz D zeO} SR M zeO} D zbPA SR M zvPq D zxPn SR M zxPn D zvPj SR
M zvPj D zsPn SR M zsPn D zsPq SR M zsPq D zvPw SR M zvPw D zxP{ SR
M zxP{ D {@P~ SR M {@P~ D {IP~ SR M {IP~ D {QP{ SR M {QP{ D {SPw SR
M {SPw D {VPq SR M {VPq D {VPj SR M {VPj D {SPd SR M {SPd D {LP^ SR
M {LP^ D {@PW SR M {@PW D z{PT SR M z{PT D zvPM SR M zvPM D zsPD SR
M zsPD D zsOz SR M {IP~ D {NP{ SR M {NP{ D {QPw SR M {QPw D {SPq SR
M {SPq D {SPj SR M {SPj D {QPd SR M {QPd D {IP^ SR M {IP^ D {@PW SR
M zsPA D zvPD SR M zvPD D z{PD SR M z{PD D {GO} SR M {GO} D {NO} SR
M {NO} D {SPA SR M {SPA D {VPD SR M z{PD D {GOz SR M {GOz D {QOz SR
M {QOz D {SO} SR M {SO} D {VPD SR M {VPD D {VPJ SR
M GmsZ D IApR D JUme D KikQ D L}iS D NQgi D OefO D PzeC D RNdD D SbcO
D Tvba D VJaz D W^aX D Xr`x D ZF`Z D [Z_} D \n__ D ^B^? D _V^] D `j]x
D a~]P D cS\d D dg[t D e{[@ D gOZH D hcYM D iwXN D kKWM D l_VJ D msUF
D oGTB D p[R? D qoQ~ D sCQA D tXPJ D ulOZ D w@Nr D xTNV SR
M y~Nx D ywNu SR M ywNu D yrNk SR M yrNk D yoN[ SR M yoN[ D yoNR SR
M yoNR D yrNB SR M yrNB D ywMx SR M ywMx D y~Mu SR M y~Mu D zCMu SR
M zCMu D zJMx SR M zJMx D zONB SR M zONB D zQNR SR M zQNR D zQN[ SR
M zQN[ D zONk SR M zONk D zJNu SR M zJNu D zCNx SR M zCNx D y~Nx SR
M y~Nx D yyNu SR M yyNu D ywNr SR M ywNr D ytNk SR M ytNk D yrN[ SR
M yrN[ D yrNR SR M yrNR D ytNB SR M ytNB D ywM{ SR M ywM{ D yyMx SR
M yyMx D y~Mu SR M zCMu D zHMx SR M zHMx D zJM{ SR M zJM{ D zLNB SR
M zLNB D zONR SR M zONR D zON[ SR M zON[ D zLNk SR M zLNk D zJNr SR
M zJNr D zHNu SR M zHNu D zCNx SR M zbM{ D z`Mx SR M z`Mx D zbMu SR
M zbMu D zeMx SR M zeMx D zbM{ SR M zvNo D zxNk SR M zxNk D zvNh SR
M zvNh D zsNk SR M zsNk D zsNo SR M zsNo D zxNu SR M zxNu D {@Nx SR
M {@Nx D {INx SR M {INx D {QNu SR M {QNu D {SNo SR M {SNo D {SNe SR
M {SNe D {QN_ SR M {QN_ D {IN[ SR M {IN[ D {BN[ SR M {INx D {NNu SR
M {NNu D {QNo SR M {QNo D {QNe SR M {QNe D {NN_ SR M {NN_ D {IN[ SR
M {IN[ D {NNX SR M {NNX D {SNR SR M {SNR D {VNK SR M {VNK D {VNB SR
M {VNB D {SM{ SR M {SM{ D {QMx SR M {QMx D {IMu SR M {IMu D {@Mu SR
M {@Mu D zxMx SR M zxMx D zvM{ SR M zvM{ D zsNB SR M zsNB D zsNE SR
M zsNE D zvNH SR M zvNH D zxNE SR M zxNE D zvNB SR M {QNU D {SNK SR
M {SNK D {SNB SR M {SNB D {QM{ SR M {QM{ D {NMx SR M {NMx D {IMu SR
M Gmps D IAmk D JUk@ D Kihn D L}fq D NQeI D Oecq D Pzbg D RNaj D Sb`v
D Tv`K D VJ_f D W^_E D Xr^g D ZF^K D [Z]o D \n]S D ^B\t D _V\T D `j[p
D a~[I D cSZ^ D dgYo D e{X| D gOXE D hcWJ D iwVL D kKUK D l_TI D msSE
D oGRA D p[P~ D qoO~ D sCOA D tXNJ D ulM[ D w@Lt D xTLY SR
M y~L? D ywL{ SR M ywL{ D yrLr SR M yrLr D yoLa SR M yoLa D yoLX SR
M yoLX D yrLH SR M yrLH D ywK~ SR M ywK~ D y~K{ SR M y~K{ D zCK{ SR
M zCK{ D zJK~ SR M zJK~ D zOLH SR M zOLH D zQLX SR M zQLX D zQLa SR
M zQLa D zOLr SR M zOLr D zJL{ SR M zJL{ D zCL? SR M zCL? D y~L? SR
M y~L? D yyL{ SR M yyL{ D ywLx SR M ywLx D ytLr SR M ytLr D yrLa SR
M yrLa D yrLX SR M yrLX D ytLH SR M ytLH D ywLA SR M ywLA D yyK~ SR
M yyK~ D y~K{ SR M zCK{ D zHK~ SR M zHK~ D zJLA SR M zJLA D zLLH SR
M zLLH D zOLX SR M zOLX D zOLa SR M zOLa D zLLr SR M zLLr D zJLx SR
M zJLx D zHL{ SR M zHL{ D zCL? SR M zbLA D z`K~ SR M z`K~ D zbK{ SR
M zbK{ D zeK~ SR M zeK~ D zbLA SR M {ILx D {IK{ SR M {LL? D {LK{ SR
M {LL? D zqLN SR M zqLN D {XLN SR M {BK{ D {SK{ SR
M GmnN D IAkH D JUh^ D KifN D L}dS D NQbl D OeaV D Pz`N D RN_R D Sb^a
D Tv]w D VJ]S D W^\t D Xr\X D ZF[~ D [Z[c D \n[H D ^BZk D _VZL D `jYi
D a~YC D cSXY D dgWk D e{Vy D gOVB D hcUH D iwTJ D kKSJ D l_RH D msQD
D oGPA D p[N~ D qoM~ D sCMB D tXLK D ulK\ D w@Jv D xTJ[ SR
M y~J? D ywJ| SR M ywJ| D yrJr SR M yrJr D yoJb SR M yoJb D yoJX SR
M yoJX D yrJH SR M yrJH D ywI~ SR M ywI~ D y~I{ SR M y~I{ D zCI{ SR
M zCI{ D zJI~ SR M zJI~ D zOJH SR M zOJH D zQJX SR M zQJX D zQJb SR
M zQJb D zOJr SR M zOJr D zJJ| SR M zJJ| D zCJ? SR M zCJ? D y~J? SR
M y~J? D yyJ| SR M yyJ| D ywJx SR M ywJx D ytJr SR M ytJr D yrJb SR
M yrJb D yrJX SR M yrJX D ytJH SR M ytJH D ywJB SR M ywJB D yyI~ SR
M yyI~ D y~I{ SR M zCI{ D zHI~ SR M zHI~ D zJJB SR M zJJB D zLJH SR
M zLJH D zOJX SR M zOJX D zOJb SR M zOJb D zLJr SR M zLJr D zJJx SR
M zJJx D zHJ| SR M zHJ| D zCJ? SR M zbJB D z`I~ SR M z`I~ D zbI{ SR
M zbI{ D zeI~ SR M zeI~ D zbJB SR M zxJ? D zsJ_ SR M zsJ_ D zxJb SR
M zxJb D {@Je SR M {@Je D {GJe SR M {GJe D {NJb SR M {NJb D {SJ[ SR
M {SJ[ D {VJR SR M {VJR D {VJN SR M {VJN D {SJE SR M {SJE D {NI~ SR
M {NI~ D {GI{ SR M {GI{ D {@I{ SR M {@I{ D zxI~ SR M zxI~ D zvJB SR
M zvJB D zsJH SR M zsJH D zsJK SR M zsJK D zvJN SR M zvJN D zxJK SR
M zxJK D zvJH SR M {GJe D {LJb SR M {LJb D {QJ[ SR M {QJ[ D {SJR SR
M {SJR D {SJN SR M {SJN D {QJE SR M {QJE D {LI~ SR M {LI~ D {GI{ SR
M zxJ? D {QJ? SR M zxJ| D {EJ| SR M {EJ| D {QJ? SR
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FMENDEPSF
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (71) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(T) 207 736.18 T
(arget Acquisition Reference Information) 211.83 736.18 T
0 10 Q
0.57 (Figure 7-2.) 126 434.33 P
3 F
0.57 (Fraction of counts detected as a function of the true count rate,) 183.83 434.33 P
(i.e., before the paired pulse correction.) 126 422.33 T
54 379 540 382 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 380.5 540 380.5 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 380.5 180 380.5 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(7.2) 163.32 386 T
(Constraints on the V) 189 386 T
(alue of the) 305.69 386 T
8 F
(STEP-TIME) 369.04 386 T
0 F
( Parameter) 433.84 386 T
5 10 Q
-0.22 (Once you have the predicted countrate, you then need to extract the piece of information) 189 358.33 P
-0.02 (required to plan your tar) 189 346.33 P
-0.02 (get acquisition:) 285.93 346.33 P
6 F
-0.05 (STEP-TIME) 349.77 346.33 P
5 F
-0.02 (. This is necessary to calculate the) 403.77 346.33 P
0.7 (time per exposure that is entered on the proposal logsheet. The goal is to have GHRS) 189 334.33 P
-0.2 (see 10) 189 322.33 P
5 8 Q
-0.16 (3) 214.07 326.33 P
5 10 Q
-0.2 ( to 10) 218.07 322.33 P
5 8 Q
-0.16 (4) 240.46 326.33 P
5 10 Q
-0.2 ( counts at the peak dwell point of the spiral search for either an acquisition) 244.46 322.33 P
0.16 (or a peakup. A minimum of 100 counts are needed to have a chance at a successful tar-) 189 310.33 P
0.13 (get acquisition. The) 189 298.33 P
6 F
0.31 (STEP-TIME) 271.05 298.33 P
5 F
0.13 ( then is just the number of counts desired \05010) 325.05 298.33 P
5 8 Q
0.1 (3) 506.46 302.33 P
5 10 Q
0.13 ( to 10) 510.46 298.33 P
5 8 Q
0.1 (5) 533.5 302.33 P
5 10 Q
0.13 (,) 537.5 298.33 P
-0.09 (but at least 100\051 divided by the predicted count rate. Remember) 189 286.33 P
-0.09 (, however) 442.42 286.33 P
-0.09 (, that the mini-) 481.37 286.33 P
0.76 (mum) 189 274.33 P
6 F
1.82 (STEP-TIME) 212.82 274.33 P
5 F
0.76 ( permitted is 0.2 seconds. Also bear in mind that the) 266.82 274.33 P
6 F
1.82 (STEP-TIME) 486 274.33 P
5 F
(may not exceed 12.75 seconds.) 189 262.33 T
-0.24 (T) 189 238.33 P
-0.24 (o avoid the possibility of a failed tar) 194.41 238.33 P
-0.24 (get acquisition, it is important that the combination) 337.24 238.33 P
0.21 (of your tar) 189 226.33 P
0.21 (get \337ux and the acquisition mirror used should not result in the eight science) 231.45 226.33 P
0.82 (diodes used for the tar) 189 214.33 P
0.82 (get acquisition seeing more than a total of about 65,000 counts) 280.98 214.33 P
-0.23 (\050the number accommodated in a 16 bit register\051 in a given) 189 202.33 P
6 F
-0.55 (STEP-TIME) 421.17 202.33 P
5 F
-0.23 (. Counting more) 475.17 202.33 P
0.98 (than 65,000 counts ef) 189 190.33 P
0.98 (fectively causes the register to wrap back to zero and thus con-) 277.87 190.33 P
-0.03 (founds the tar) 189 178.33 P
-0.03 (get acquisition algorithm.) 243.76 178.33 P
11 F
-0.03 (This pr) 348.68 178.33 P
-0.03 (oblem is avoided if) 379.87 178.33 P
8 F
-0.06 (BRIGHT=RETURN) 462 178.33 P
11 F
0.62 (is speci\336ed) 189 166.33 P
5 F
0.62 (because a 32-bit on-board register is used. If a) 238.57 166.33 P
6 F
1.48 (BRIGHT) 431.3 166.33 P
5 F
0.62 ( limit is explicitly) 467.3 166.33 P
(given, the register that holds it is limited to 16 bits.) 189 154.33 T
-0.11 (Figure) 189 130.33 P
-0.11 (7-3 and Figure) 217.61 130.33 P
-0.11 (7-4 are provided to allow for a visual check of potential problems) 278.77 130.33 P
0.38 (arising from the choice of) 189 118.33 P
6 F
0.91 (STEP-TIME) 296.71 118.33 P
5 F
0.38 (. These Figures show the constraints placed on) 350.71 118.33 P
0.35 (using a particular mirror and) 189 106.33 P
6 F
0.84 (STEP-TIME) 307.67 106.33 P
5 F
0.35 (. Figure) 361.67 106.33 P
0.35 (7-4 is analogous for the Side 1 mir-) 395.62 106.33 P
(rors.) 189 94.33 T
54 87.98 540 686.02 C
54 450 540 679.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
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600 1998 r 696 1997 d 753 1995 d 793 1993 d 824 1992 d 849 1990 d
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0 9 Q
(T) 189 736.18 T
(arget Acquisition Reference Information) 193.83 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(72) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
(Figure 7-3.) 126 326.33 T
3 F
(T) 182.13 326.33 T
(arget acquisition constraints for the Side 2 mirrors N2 and A2.) 187.13 326.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 9 Q
(N2R:) 114 299 T
(Constraints and Restrictions Document \050CARD\051 upper limit for use of Mirror) 186 299 T
(-N2. Observing) 465.3 299 T
(objects that are bluer and brighter than indicated by this line would result in degraded perfor-) 186 288 T
-0.33 (mance and possible damage to the instrument. Brighter and bluer objects should be acquired with) 186 277 P
(mirrors A2 or A1.) 186 266 T
(N2-0.2:) 114 247 T
-0.17 (GHRS will count 65,000 counts in 0.2 seconds with the N2 mirror for objects on this contour) 186 247 P
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-0.17 (o) 527.42 247 P
(the left of this curve, more than 65,000 counts will be detected leading to a probable failure to) 186 236 T
(acquire the object if a) 186 225 T
6 F
(BRIGHT) 266.23 225 T
5 F
( value is speci\336ed. However) 298.63 225 T
(, use of) 399.99 225 T
6 F
(BRIGHT=RETURN) 428.49 225 T
5 F
( will) 498.69 225 T
(result in a satisfactory acquisition.) 186 214 T
(A2-0.2:) 114 195 T
-0.17 (GHRS will count 65,000 counts in 0.2 seconds with the A2 mirror for objects on this contour) 186 195 P
-0.17 (. T) 518.23 195 P
-0.17 (o) 527.42 195 P
(the left of this curve, more than 65,000 counts will be detected leading to a probable failure to) 186 184 T
(acquire the object if a) 186 173 T
6 F
(BRIGHT) 266.23 173 T
5 F
( value is speci\336ed. However) 298.63 173 T
(, use of) 399.99 173 T
6 F
(BRIGHT=RETURN) 428.49 173 T
5 F
( will) 498.69 173 T
(result in a satisfactory acquisition.) 186 162 T
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0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (73) 546.88 60.29 P
72 750.02 558 750.02 2 L
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3 F
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0 0 0 1 0 0 0 K
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(objects that are bluer and brighter than indicated by this line would result in degraded perfor-) 204 297 T
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(acquire the object if a) 204 234 T
6 F
(BRIGHT) 284.23 234 T
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( value is speci\336ed. However) 316.63 234 T
(, use of) 417.99 234 T
6 F
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5 F
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(result in a satisfactory acquisition.!) 204 223 T
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9270 667 M 105 0 R 35 -11 R 12 -12 R 12 -23 R 0 -24 R -12 -23 R -12 -12 R
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93 245 R D 10018 714 M 23 -23 R 24 -35 R 23 -47 R 12 -59 R 0 -46 R -12 -59 R
-23 -58 R -24 -35 R -23 -24 R D 10200 479 M -16 -5 R -10 -15 R -6 -26 R
0 -16 R 6 -26 R 10 -15 R 16 -6 R 10 0 R 15 6 R 11 15 R 5 26 R 0 16 R -5 26 R
-11 15 R -15 5 R -10 0 R D 2220 11996 M 14894 0 R D 2220 11996 M 0 -212 R D
4603 11996 M 0 -212 R D 6986 11996 M 0 -212 R D 9369 11996 M 0 -212 R D
11752 11996 M 0 -212 R D 14135 11996 M 0 -212 R D 16518 11996 M 0 -212 R D
2815 11996 M 0 -106 R D 3411 11996 M 0 -106 R D 4007 11996 M 0 -106 R D
5198 11996 M 0 -106 R D 5794 11996 M 0 -106 R D 6390 11996 M 0 -106 R D
7581 11996 M 0 -106 R D 8177 11996 M 0 -106 R D 8773 11996 M 0 -106 R D
9964 11996 M 0 -106 R D 10560 11996 M 0 -106 R D 11156 11996 M 0 -106 R D
12348 11996 M 0 -106 R D 12943 11996 M 0 -106 R D 13539 11996 M 0 -106 R D
14731 11996 M 0 -106 R D 15326 11996 M 0 -106 R D 15922 11996 M 0 -106 R D
2220 1408 M 0 10588 R D 2220 1408 M 297 0 R D 1957 1653 M -35 -12 R
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0 35 R 12 24 R 23 23 R 35 12 R 47 11 R 23 12 R 12 24 R 0 23 R -12 23 R
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0 -23 R -12 -24 R -23 -35 R -117 -116 R 164 0 R D 2220 9878 M 297 0 R D
1968 9983 M -35 -12 R -23 -35 R -12 -59 R 0 -35 R 12 -58 R 23 -35 R 35 -12 R
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17114 4055 M -149 0 R D 17114 4584 M -149 0 R D 17114 5113 M -149 0 R D
17114 6172 M -149 0 R D 17114 6702 M -149 0 R D 17114 7231 M -149 0 R D
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23 -35 R 35 -12 R 24 0 R 35 12 R 23 35 R 12 59 R 0 35 R -12 58 R -23 35 R
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FMENDEPSF
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0 0 612 792 C
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7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(T) 189 736.18 T
(arget Acquisition Reference Information) 193.83 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(74) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
36 96 542.02 717 R
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
36 96 542.02 717 R
55 152.01 68 717 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
61 287.01 61 638.01 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
61 152.01 61 278.01 2 L
0 Z
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 0 -270 74 152.01 TF
(ABLE 7-1) 0 -270 74 156.84 TF
3 F
(Predicted target acquisition count rates for stars, reduced to) 0 -270 74 287.01 TF
4 F
(V) 0 -270 74 527.62 TF
4 7.2 Q
(0) 0 -270 76.25 533.62 TF
3 9 Q
(= 0.) 0 -270 74 540.13 TF
0 8 Q
(Star Name) 0 -270 100.33 161.69 TF
(Spectral) 0 -270 95.33 221.97 TF
(T) 0 -270 105.33 228.71 TF
(ype) 0 -270 105.33 233.01 TF
10 F
(\050B\320V\051) 0 -270 100.33 270.82 TF
10 6.4 Q
(0) 0 -270 102.33 291.71 TF
0 8 Q
(count rate for mirror) 0 -270 92.33 365.08 TF
(reddening reduction factor) 0 -270 92.33 530.82 TF
0 6.4 Q
(a) 0 -270 89.13 632.61 TF
0 8 Q
(N2) 0 -270 108.33 321.96 TF
(A2) 0 -270 108.33 373.08 TF
(N1) 0 -270 108.33 424.21 TF
(A1) 0 -270 108.33 475.33 TF
(N2) 0 -270 108.33 520.26 TF
(A2) 0 -270 108.33 559.01 TF
(N1) 0 -270 108.33 597.76 TF
(A1) 0 -270 108.33 636.51 TF
5 9 Q
(9 Sgr) 0 -270 123 185.68 TF
(O5) 0 -270 123 232.25 TF
(-0.337) 0 -270 123 271.42 TF
(8.595E9) 0 -270 123 311.95 TF
(2.098E7) 0 -270 123 363.07 TF
(4.598E8) 0 -270 123 414.19 TF
(2.657E5) 0 -270 123 465.32 TF
(-3.034) 0 -270 123 513.75 TF
(-3.108) 0 -270 123 552.5 TF
(-3.428) 0 -270 123 591.25 TF
(-3.130) 0 -270 123 630 TF
(HR 8023) 0 -270 136 172.18 TF
(O6) 0 -270 136 232.25 TF
(-0.313) 0 -270 136 271.42 TF
(5.684E9) 0 -270 136 311.95 TF
(1.348E7) 0 -270 136 363.07 TF
(2.545E8) 0 -270 136 414.19 TF
(1.690E5) 0 -270 136 465.32 TF
(-2.955) 0 -270 136 513.75 TF
(-3.021) 0 -270 136 552.5 TF
(-3.382) 0 -270 136 591.25 TF
(-3.1) 0 -270 136 630.16 TF
(14) 0 -270 136 644.08 TF
(60 Cyg) 0 -270 149 178.68 TF
(B1V) 0 -270 149 229.25 TF
(-0.269) 0 -270 149 271.42 TF
(5.367E9) 0 -270 149 311.95 TF
(1.293E7) 0 -270 149 363.07 TF
(2.794E8) 0 -270 149 414.19 TF
(1.767E5) 0 -270 149 465.32 TF
(-3.002) 0 -270 149 513.75 TF
(-3.070) 0 -270 149 552.5 TF
(-3.393) 0 -270 149 591.25 TF
(-3.123) 0 -270 149 630 TF
(69 Cyg) 0 -270 162 178.68 TF
(B0IB) 0 -270 162 228 TF
(-0.234) 0 -270 162 271.42 TF
(4.192E9) 0 -270 162 311.95 TF
(9.901E6) 0 -270 162 363.07 TF
(1.869E8) 0 -270 162 414.19 TF
(1.209E5) 0 -270 162 465.32 TF
(-2.935) 0 -270 162 513.75 TF
(-3.003) 0 -270 162 552.5 TF
(-3.384) 0 -270 162 591.25 TF
(-3.1) 0 -270 162 630.16 TF
(10) 0 -270 162 644.08 TF
9 10 Q
(i) 0 -270 175 185.65 TF
5 9 Q
(Her) 0 -270 175 191.44 TF
(B3V) 0 -270 175 229.25 TF
(-0.203) 0 -270 175 271.42 TF
(2.764E9) 0 -270 175 311.95 TF
(6.529E6) 0 -270 175 363.07 TF
(1.232E8) 0 -270 175 414.19 TF
(7.970E4) 0 -270 175 465.32 TF
(-2.935) 0 -270 175 513.75 TF
(-3.003) 0 -270 175 552.5 TF
(-3.384) 0 -270 175 591.25 TF
(-3.1) 0 -270 175 630.16 TF
(10) 0 -270 175 644.08 TF
(HR 7467) 0 -270 188 172.18 TF
(B3III) 0 -270 188 228.01 TF
(-0.182) 0 -270 188 271.42 TF
(2.436E9) 0 -270 188 311.95 TF
(5.755E6) 0 -270 188 363.07 TF
(1.087E8) 0 -270 188 414.19 TF
(7.028E4) 0 -270 188 465.32 TF
(-2.936) 0 -270 188 513.75 TF
(-3.004) 0 -270 188 552.5 TF
(-3.384) 0 -270 188 591.25 TF
(-3.1) 0 -270 188 630.16 TF
(10) 0 -270 188 644.08 TF
(20 Aql) 0 -270 201 180.18 TF
(B3IV) 0 -270 201 227.75 TF
(-0.156) 0 -270 201 271.42 TF
(2.268E9) 0 -270 201 311.95 TF
(5.357E6) 0 -270 201 363.07 TF
(1.012E8) 0 -270 201 414.19 TF
(6.542E4) 0 -270 201 465.32 TF
(-2.936) 0 -270 201 513.75 TF
(-3.004) 0 -270 201 552.5 TF
(-3.384) 0 -270 201 591.25 TF
(-3.1) 0 -270 201 630.16 TF
(10) 0 -270 201 644.08 TF
(38 Oph) 0 -270 214 178.19 TF
(A1V) 0 -270 214 229 TF
(-0.139) 0 -270 214 271.42 TF
(1.776E9) 0 -270 214 311.95 TF
(4.108E6) 0 -270 214 363.07 TF
(6.421E7) 0 -270 214 414.19 TF
(4.582E4) 0 -270 214 465.32 TF
(-2.891) 0 -270 214 513.75 TF
(-2.953) 0 -270 214 552.5 TF
(-3.347) 0 -270 214 591.25 TF
(-3.101) 0 -270 214 630 TF
(HR 7346) 0 -270 227 172.18 TF
(B7III) 0 -270 227 228.01 TF
(-0.108) 0 -270 227 271.42 TF
(1.368E9) 0 -270 227 311.95 TF
(3.165E6) 0 -270 227 363.07 TF
(4.948E7) 0 -270 227 414.19 TF
(3.531E4) 0 -270 227 465.32 TF
(-2.892) 0 -270 227 513.75 TF
(-2.953) 0 -270 227 552.5 TF
(-3.347) 0 -270 227 591.25 TF
(-3.101) 0 -270 227 630 TF
(HD 189689) 0 -270 240 162.69 TF
(B9V) 0 -270 240 229.25 TF
(-0.081) 0 -270 240 271.42 TF
(1.008E9) 0 -270 240 311.95 TF
(2.303E6) 0 -270 240 363.07 TF
(2.763E7) 0 -270 240 414.19 TF
(2.306E4) 0 -270 240 465.32 TF
(-2.864) 0 -270 240 513.75 TF
(-2.921) 0 -270 240 552.5 TF
(-3.317) 0 -270 240 591.25 TF
(-3.097) 0 -270 240 630 TF
(59 Her) 0 -270 253 180.19 TF
(A3III) 0 -270 253 227.76 TF
(-0.045) 0 -270 253 271.42 TF
(5.948E8) 0 -270 253 311.95 TF
(1.363E6) 0 -270 253 363.07 TF
(1.700E7) 0 -270 253 414.19 TF
(1.407E4) 0 -270 253 465.32 TF
(-2.873) 0 -270 253 513.75 TF
(-2.932) 0 -270 253 552.5 TF
(-3.320) 0 -270 253 591.25 TF
(-3.099) 0 -270 253 630 TF
(1) 0 -270 266 180.52 TF
(1 Sge) 0 -270 266 184.68 TF
(B9IV) 0 -270 266 227.75 TF
(-0.027) 0 -270 266 271.42 TF
(5.745E8) 0 -270 266 311.95 TF
(1.293E6) 0 -270 266 363.07 TF
(1.168E7) 0 -270 266 414.19 TF
(1.182E4) 0 -270 266 465.32 TF
(-2.819) 0 -270 266 513.75 TF
(-2.873) 0 -270 266 552.5 TF
(-3.281) 0 -270 266 591.25 TF
(-3.088) 0 -270 266 630 TF
(69 Her) 0 -270 279 180.19 TF
(A2V) 0 -270 279 229 TF
(0.000) 0 -270 279 272.92 TF
(4.918E8) 0 -270 279 311.95 TF
(1.107E6) 0 -270 279 363.07 TF
(9.997E6) 0 -270 279 414.19 TF
(1.01) 0 -270 279 465.48 TF
(1E4) 0 -270 279 480.9 TF
(-2.819) 0 -270 279 513.75 TF
(-2.873) 0 -270 279 552.5 TF
(-3.281) 0 -270 279 591.25 TF
(-3.088) 0 -270 279 630 TF
(HR 8020) 0 -270 292 172.18 TF
(B8IA) 0 -270 292 227.75 TF
(0.027) 0 -270 292 272.92 TF
(1.063E9) 0 -270 292 311.95 TF
(2.386E6) 0 -270 292 363.07 TF
(1.940E7) 0 -270 292 414.19 TF
(2.154E4) 0 -270 292 465.32 TF
(-2.820) 0 -270 292 513.75 TF
(-2.872) 0 -270 292 552.5 TF
(-3.255) 0 -270 292 591.25 TF
(-3.089) 0 -270 292 630 TF
(78 Her) 0 -270 305 180.19 TF
(B9V) 0 -270 305 229.25 TF
(0.036) 0 -270 305 272.92 TF
(4.532E8) 0 -270 305 311.95 TF
(1.018E6) 0 -270 305 363.07 TF
(8.272E6) 0 -270 305 414.19 TF
(9.187E3) 0 -270 305 465.32 TF
(-2.820) 0 -270 305 513.75 TF
(-2.872) 0 -270 305 552.5 TF
(-3.255) 0 -270 305 591.25 TF
(-3.089) 0 -270 305 630 TF
(58 Aql) 0 -270 318 180.18 TF
(A0V) 0 -270 318 229 TF
(0.057) 0 -270 318 272.92 TF
(4.291E8) 0 -270 318 311.95 TF
(9.634E5) 0 -270 318 363.07 TF
(7.830E6) 0 -270 318 414.19 TF
(8.696E3) 0 -270 318 465.32 TF
(-2.820) 0 -270 318 513.75 TF
(-2.872) 0 -270 318 552.5 TF
(-3.255) 0 -270 318 591.25 TF
(-3.089) 0 -270 318 630 TF
(60 Her) 0 -270 331 180.19 TF
(A3IV) 0 -270 331 227.51 TF
(0.085) 0 -270 331 272.92 TF
(3.197E8) 0 -270 331 311.95 TF
(7.086E5) 0 -270 331 363.07 TF
(3.280E6) 0 -270 331 414.19 TF
(5.497E3) 0 -270 331 465.32 TF
(-2.758) 0 -270 331 513.75 TF
(-2.810) 0 -270 331 552.5 TF
(-3.217) 0 -270 331 591.25 TF
(-3.077) 0 -270 331 630 TF
(HR 6570) 0 -270 344 172.18 TF
(A7V) 0 -270 344 229 TF
(0.107) 0 -270 344 272.92 TF
(2.999E8) 0 -270 344 311.95 TF
(6.647E5) 0 -270 344 363.07 TF
(3.079E6) 0 -270 344 414.19 TF
(5.161E3) 0 -270 344 465.32 TF
(-2.759) 0 -270 344 513.75 TF
(-2.81) 0 -270 344 552.67 TF
(1) 0 -270 344 571.08 TF
(-3.217) 0 -270 344 591.25 TF
(-3.077) 0 -270 344 630 TF
(HD192285) 0 -270 357 164.94 TF
(A4IV) 0 -270 357 227.51 TF
(0.124) 0 -270 357 272.92 TF
(2.628E8) 0 -270 357 311.95 TF
(5.771E5) 0 -270 357 363.07 TF
(1.444E6) 0 -270 357 414.19 TF
(3.569E3) 0 -270 357 465.32 TF
(-2.719) 0 -270 357 513.75 TF
(-2.771) 0 -270 357 552.5 TF
(-3.184) 0 -270 357 591.25 TF
(-3.071) 0 -270 357 630 TF
9 10 Q
(q) 0 -270 370 182.33 TF
5 7.2 Q
(1) 0 -270 366.4 187.54 TF
5 9 Q
(Ser) 0 -270 370 192.94 TF
(A5V) 0 -270 370 229 TF
(0.143) 0 -270 370 272.92 TF
(2.669E8) 0 -270 370 311.95 TF
(5.862E5) 0 -270 370 363.07 TF
(1.466E6) 0 -270 370 414.19 TF
(3.623E3) 0 -270 370 465.32 TF
(-2.718) 0 -270 370 513.75 TF
(-2.770) 0 -270 370 552.5 TF
(-3.184) 0 -270 370 591.25 TF
(-3.071) 0 -270 370 630 TF
(KW 1) 0 -270 383 174.52 TF
(14) 0 -270 383 195.93 TF
(0.175) 0 -270 383 272.92 TF
(2.395E8) 0 -270 383 311.95 TF
(5.240E5) 0 -270 383 363.07 TF
(9.954E5) 0 -270 383 414.19 TF
(2.843E3) 0 -270 383 465.32 TF
(-2.703) 0 -270 383 513.75 TF
(-2.755) 0 -270 383 552.5 TF
(-3.168) 0 -270 383 591.25 TF
(-3.069) 0 -270 383 630 TF
(KW 154) 0 -270 396 174.19 TF
(0.219) 0 -270 396 272.92 TF
(2.050E8) 0 -270 396 311.95 TF
(4.439E5) 0 -270 396 363.07 TF
(4.497E5) 0 -270 396 414.19 TF
(1.636E3) 0 -270 396 465.32 TF
(-2.666) 0 -270 396 513.75 TF
(-2.715) 0 -270 396 552.5 TF
(-3.166) 0 -270 396 591.25 TF
(-3.063) 0 -270 396 630 TF
9 10 Q
(c) 0 -270 409 184.95 TF
5 9 Q
(Ser) 0 -270 409 192.94 TF
(F0IV) 0 -270 409 228.25 TF
(0.240) 0 -270 409 272.92 TF
(1.829E8) 0 -270 409 311.95 TF
(3.958E5) 0 -270 409 363.07 TF
(4.004E5) 0 -270 409 414.19 TF
(1.457E3) 0 -270 409 465.32 TF
(-2.665) 0 -270 409 513.75 TF
(-2.714) 0 -270 409 552.5 TF
(-3.166) 0 -270 409 591.25 TF
(-3.062) 0 -270 409 630 TF
(HD5132) 0 -270 422 173.94 TF
(F0IV) 0 -270 422 228.25 TF
(0.287) 0 -270 422 272.92 TF
(2.01) 0 -270 422 312.12 TF
(1E8) 0 -270 422 327.53 TF
(4.354E5) 0 -270 422 363.07 TF
(4.412E5) 0 -270 422 414.19 TF
(1.605E3) 0 -270 422 465.32 TF
(-2.666) 0 -270 422 513.75 TF
(-2.715) 0 -270 422 552.5 TF
(-3.166) 0 -270 422 591.25 TF
(-3.063) 0 -270 422 630 TF
(HD508) 0 -270 435 178.44 TF
(A9IV) 0 -270 435 227.51 TF
(0.305) 0 -270 435 272.92 TF
(1.718E8) 0 -270 435 311.95 TF
(3.720E5) 0 -270 435 363.07 TF
(3.771E5) 0 -270 435 414.19 TF
(1.372E3) 0 -270 435 465.32 TF
(-2.666) 0 -270 435 513.75 TF
(-2.716) 0 -270 435 552.5 TF
(-3.166) 0 -270 435 591.25 TF
(-3.063) 0 -270 435 630 TF
9 10 Q
(r) 0 -270 448 182.45 TF
5 9 Q
(Cap) 0 -270 448 190.43 TF
(F2IV) 0 -270 448 228.25 TF
(0.339) 0 -270 448 272.92 TF
(1.125E8) 0 -270 448 311.95 TF
(2.322E5) 0 -270 448 363.07 TF
(2.619E4) 0 -270 448 414.19 TF
(1.014E2) 0 -270 448 465.32 TF
(-2.484) 0 -270 448 513.75 TF
(-2.517) 0 -270 448 552.5 TF
(-3.181) 0 -270 448 591.25 TF
(-3.023) 0 -270 448 630 TF
(KW 332) 0 -270 461 174.19 TF
(0.389) 0 -270 461 272.92 TF
(1.177E8) 0 -270 461 311.95 TF
(2.431E5) 0 -270 461 363.07 TF
(2.751E4) 0 -270 461 414.19 TF
(1.065E2) 0 -270 461 465.32 TF
(-2.486) 0 -270 461 513.75 TF
(-2.519) 0 -270 461 552.5 TF
(-3.181) 0 -270 461 591.25 TF
(-3.023) 0 -270 461 630 TF
(HD7331) 0 -270 474 173.94 TF
(F7IV) 0 -270 474 228.25 TF
(0.427) 0 -270 474 272.92 TF
(9.807E7) 0 -270 474 311.95 TF
(2.012E5) 0 -270 474 363.07 TF
(2.256E4) 0 -270 474 414.19 TF
(8.772E1) 0 -270 474 465.32 TF
(-2.451) 0 -270 474 513.75 TF
(-2.482) 0 -270 474 552.5 TF
(-3.179) 0 -270 474 591.25 TF
(-3.015) 0 -270 474 630 TF
(BD+63) 0 -270 487 165.76 TF
5 7.2 Q
(o) 0 -270 483.4 192.33 TF
5 9 Q
(13) 0 -270 487 195.93 TF
(F5IV) 0 -270 487 228.25 TF
(0.444) 0 -270 487 272.92 TF
(1.139E8) 0 -270 487 311.95 TF
(2.362E5) 0 -270 487 363.07 TF
(6.070E4) 0 -270 487 414.19 TF
(2.395E2) 0 -270 487 465.32 TF
(-2.488) 0 -270 487 513.75 TF
(-2.523) 0 -270 487 552.5 TF
(-3.171) 0 -270 487 591.25 TF
(-3.024) 0 -270 487 630 TF
(HD35296) 0 -270 500 169.44 TF
(F8V) 0 -270 500 229.75 TF
(0.489) 0 -270 500 272.92 TF
(1.089E8) 0 -270 500 311.95 TF
(2.259E5) 0 -270 500 363.07 TF
(5.804E4) 0 -270 500 414.19 TF
(2.290E2) 0 -270 500 465.32 TF
(-2.488) 0 -270 500 513.75 TF
(-2.523) 0 -270 500 552.5 TF
(-3.171) 0 -270 500 591.25 TF
(-3.024) 0 -270 500 630 TF
(vB 1) 0 -270 513 187.68 TF
(0.530) 0 -270 513 272.92 TF
(6.757E7) 0 -270 513 311.95 TF
(1.374E5) 0 -270 513 363.07 TF
(2.147E4) 0 -270 513 414.19 TF
(8.448E1) 0 -270 513 465.32 TF
(-2.407) 0 -270 513 513.75 TF
(-2.437) 0 -270 513 552.5 TF
(-3.175) 0 -270 513 591.25 TF
(-3.006) 0 -270 513 630 TF
(HD154760) 0 -270 526 164.94 TF
(G2V) 0 -270 526 229 TF
(0.586) 0 -270 526 272.92 TF
(6.393E7) 0 -270 526 311.95 TF
(1.285E5) 0 -270 526 363.07 TF
(3.1) 0 -270 526 414.36 TF
(15E3) 0 -270 526 425.28 TF
(1.151E1) 0 -270 526 465.32 TF
(-2.365) 0 -270 526 513.75 TF
(-2.386) 0 -270 526 552.5 TF
(-3.206) 0 -270 526 591.25 TF
(-2.998) 0 -270 526 630 TF
83.12 152.01 530.88 152.01 2 L
V
0.25 H
0 Z
N
82.88 210.93 531.12 210.93 2 L
V
N
82.88 264.57 531.12 264.57 2 L
V
N
82.88 301.51 531.12 301.51 2 L
V
2 H
N
98.88 352.64 531.12 352.64 2 L
V
0.25 H
N
98.88 403.76 531.12 403.76 2 L
V
N
98.88 454.88 531.12 454.88 2 L
V
N
82.88 506 531.12 506 2 L
V
N
98.88 544.75 531.12 544.75 2 L
V
N
98.88 583.5 531.12 583.5 2 L
V
N
98.88 622.24 531.12 622.24 2 L
V
N
83.12 660.99 530.88 660.99 2 L
V
N
83 151.88 83 661.12 2 L
V
N
99 300.51 99 661.12 2 L
V
N
115 151.88 115 661.12 2 L
V
0.5 H
N
180 151.88 180 661.12 2 L
V
0.25 H
N
245 151.88 245 661.12 2 L
V
N
310 151.88 310 661.12 2 L
V
N
375 151.88 375 661.12 2 L
V
N
440 151.88 440 661.12 2 L
V
N
505 151.88 505 661.12 2 L
V
N
531 151.88 531 661.12 2 L
V
N
FMENDPAGE
%%EndPage: "74" 8
%%Page: "75" 9
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (75) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(T) 207 736.18 T
(arget Acquisition Reference Information) 211.83 736.18 T
30.49 78 563.51 699 R
519.49 134.01 526.49 642.99 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 612 792 C
5 9 Q
0 X
0 0 0 1 0 0 0 K
(a. use factor) 0 -270 532.49 281.01 TF
7 F
(f) 0 -270 532.49 326.99 TF
5 F
( to reduce count rate by) 0 -270 532.49 329.49 TF
(.) 0 -270 532.49 466.45 TF
30.49 78 563.51 699 R
(HD139777A) 0 -270 98.49 140.44 TF
(K0V) 0 -270 98.49 211 TF
(0.631) 0 -270 98.49 254.92 TF
(6.040E7) 0 -270 98.49 293.95 TF
(1.215E5) 0 -270 98.49 345.07 TF
(2.954E3) 0 -270 98.49 396.19 TF
(1.091E1) 0 -270 98.49 447.32 TF
(-2.367) 0 -270 98.49 495.75 TF
(-2.387) 0 -270 98.49 534.5 TF
(-3.206) 0 -270 98.49 573.25 TF
(-2.998) 0 -270 98.49 612 TF
(HR 6516) 0 -270 111.49 154.18 TF
(G6IV) 0 -270 111.49 209.51 TF
(0.651) 0 -270 111.49 254.92 TF
(5.167E7) 0 -270 111.49 293.95 TF
(1.039E5) 0 -270 111.49 345.07 TF
(2.518E3) 0 -270 111.49 396.19 TF
(9.301E0) 0 -270 111.49 447.32 TF
(-2.365) 0 -270 111.49 495.75 TF
(-2.386) 0 -270 111.49 534.5 TF
(-3.206) 0 -270 111.49 573.25 TF
(-2.998) 0 -270 111.49 612 TF
(HD136274) 0 -270 124.49 146.94 TF
(G8V) 0 -270 124.49 211 TF
(0.672) 0 -270 124.49 254.92 TF
(4.901E7) 0 -270 124.49 293.95 TF
(9.855E4) 0 -270 124.49 345.07 TF
(2.392E3) 0 -270 124.49 396.19 TF
(8.837E0) 0 -270 124.49 447.32 TF
(-2.366) 0 -270 124.49 495.75 TF
(-2.387) 0 -270 124.49 534.5 TF
(-3.206) 0 -270 124.49 573.25 TF
(-2.998) 0 -270 124.49 612 TF
(HD150205) 0 -270 137.49 146.94 TF
(G5V) 0 -270 137.49 211 TF
(0.700) 0 -270 137.49 254.92 TF
(4.650E7) 0 -270 137.49 293.95 TF
(9.352E4) 0 -270 137.49 345.07 TF
(2.275E3) 0 -270 137.49 396.19 TF
(8.404E0) 0 -270 137.49 447.32 TF
(-2.367) 0 -270 137.49 495.75 TF
(-2.388) 0 -270 137.49 534.5 TF
(-3.206) 0 -270 137.49 573.25 TF
(-2.998) 0 -270 137.49 612 TF
(31 Aql) 0 -270 150.49 162.18 TF
(G8IV) 0 -270 150.49 209.51 TF
(0.732) 0 -270 150.49 254.92 TF
(4.042E7) 0 -270 150.49 293.95 TF
(8.123E4) 0 -270 150.49 345.07 TF
(1.960E3) 0 -270 150.49 396.19 TF
(7.242E0) 0 -270 150.49 447.32 TF
(-2.364) 0 -270 150.49 495.75 TF
(-2.384) 0 -270 150.49 534.5 TF
(-3.206) 0 -270 150.49 573.25 TF
(-2.997) 0 -270 150.49 612 TF
(vB 21) 0 -270 163.49 165.18 TF
(0.766) 0 -270 163.49 254.92 TF
(3.890E7) 0 -270 163.49 293.95 TF
(7.818E4) 0 -270 163.49 345.07 TF
(1.887E3) 0 -270 163.49 396.19 TF
(6.972E0) 0 -270 163.49 447.32 TF
(-2.364) 0 -270 163.49 495.75 TF
(-2.385) 0 -270 163.49 534.5 TF
(-3.206) 0 -270 163.49 573.25 TF
(-2.997) 0 -270 163.49 612 TF
(BD\3202) 0 -270 176.49 143.83 TF
5 7.2 Q
(o) 0 -270 172.89 165.33 TF
5 9 Q
(4018) 0 -270 176.49 168.93 TF
(G5IV) 0 -270 176.49 209.51 TF
(0.791) 0 -270 176.49 254.92 TF
(3.516E7) 0 -270 176.49 293.95 TF
(7.068E4) 0 -270 176.49 345.07 TF
(1.713E3) 0 -270 176.49 396.19 TF
(6.328E0) 0 -270 176.49 447.32 TF
(-2.365) 0 -270 176.49 495.75 TF
(-2.386) 0 -270 176.49 534.5 TF
(-3.206) 0 -270 176.49 573.25 TF
(-2.998) 0 -270 176.49 612 TF
(HD190571) 0 -270 189.49 146.94 TF
(G8V) 0 -270 189.49 211 TF
(0.816) 0 -270 189.49 254.92 TF
(1.587E7) 0 -270 189.49 293.95 TF
(3.086E4) 0 -270 189.49 345.07 TF
(1.165E1) 0 -270 189.49 396.19 TF
(4.76E-4) 0 -270 189.49 448.07 TF
(-2.233) 0 -270 189.49 495.75 TF
(-2.244) 0 -270 189.49 534.5 TF
(-3.719) 0 -270 189.49 573.25 TF
(-3.247) 0 -270 189.49 612 TF
(HD1) 0 -270 202.49 151.77 TF
(1004) 0 -270 202.49 168.93 TF
(G5IV) 0 -270 202.49 209.51 TF
(0.825) 0 -270 202.49 254.92 TF
(1.587E7) 0 -270 202.49 293.95 TF
(3.086E4) 0 -270 202.49 345.07 TF
(1.169E1) 0 -270 202.49 396.19 TF
(4.78E-4) 0 -270 202.49 448.07 TF
(-2.234) 0 -270 202.49 495.75 TF
(-2.244) 0 -270 202.49 534.5 TF
(-3.719) 0 -270 202.49 573.25 TF
(-3.247) 0 -270 202.49 612 TF
(HD56176) 0 -270 215.49 151.44 TF
(G7IV) 0 -270 215.49 209.51 TF
(0.857) 0 -270 215.49 254.92 TF
(1.510E7) 0 -270 215.49 293.95 TF
(2.937E4) 0 -270 215.49 345.07 TF
(1.109E1) 0 -270 215.49 396.19 TF
(4.54E-4) 0 -270 215.49 448.07 TF
(-2.233) 0 -270 215.49 495.75 TF
(-2.244) 0 -270 215.49 534.5 TF
(-3.719) 0 -270 215.49 573.25 TF
(-3.247) 0 -270 215.49 612 TF
(HD190470) 0 -270 228.49 146.94 TF
(K3V) 0 -270 228.49 211 TF
(0.895) 0 -270 228.49 254.92 TF
(1.237E7) 0 -270 228.49 293.95 TF
(2.403E4) 0 -270 228.49 345.07 TF
(8.968E0) 0 -270 228.49 396.19 TF
(3.67E-4) 0 -270 228.49 448.07 TF
(-2.230) 0 -270 228.49 495.75 TF
(-2.241) 0 -270 228.49 534.5 TF
(-3.719) 0 -270 228.49 573.25 TF
(-3.246) 0 -270 228.49 612 TF
9 10 Q
(q) 0 -270 241.49 162.96 TF
5 7.2 Q
(1) 0 -270 237.89 168.17 TF
5 9 Q
(T) 0 -270 241.49 173.57 TF
(au) 0 -270 241.49 178.44 TF
(G8III) 0 -270 241.49 209.76 TF
(0.904) 0 -270 241.49 254.92 TF
(1.950E7) 0 -270 241.49 293.95 TF
(3.862E4) 0 -270 241.49 345.07 TF
(2.639E1) 0 -270 241.49 396.19 TF
(2.67E-4) 0 -270 241.49 448.07 TF
(-2.306) 0 -270 241.49 495.75 TF
(-2.320) 0 -270 241.49 534.5 TF
(-3.750) 0 -270 241.49 573.25 TF
(-3.262) 0 -270 241.49 612 TF
(HD170527) 0 -270 254.49 146.94 TF
(G5IV) 0 -270 254.49 209.51 TF
(0.918) 0 -270 254.49 254.92 TF
(2.157E7) 0 -270 254.49 293.95 TF
(4.277E4) 0 -270 254.49 345.07 TF
(2.944E1) 0 -270 254.49 396.19 TF
(2.98E-4) 0 -270 254.49 448.07 TF
(-2.309) 0 -270 254.49 495.75 TF
(-2.323) 0 -270 254.49 534.5 TF
(-3.750) 0 -270 254.49 573.25 TF
(-3.263) 0 -270 254.49 612 TF
(HD191615) 0 -270 267.49 146.94 TF
(G8IV) 0 -270 267.49 209.51 TF
(0.947) 0 -270 267.49 254.92 TF
(1.596E7) 0 -270 267.49 293.95 TF
(3.159E4) 0 -270 267.49 345.07 TF
(2.136E1) 0 -270 267.49 396.19 TF
(2.16E-4) 0 -270 267.49 448.07 TF
(-2.303) 0 -270 267.49 495.75 TF
(-2.317) 0 -270 267.49 534.5 TF
(-3.750) 0 -270 267.49 573.25 TF
(-3.261) 0 -270 267.49 612 TF
(HD4744) 0 -270 280.49 155.94 TF
(G8IV) 0 -270 280.49 209.51 TF
(0.989) 0 -270 280.49 254.92 TF
(1.087E7) 0 -270 280.49 293.95 TF
(2.1) 0 -270 280.49 345.24 TF
(19E4) 0 -270 280.49 356.15 TF
(8.241E0) 0 -270 280.49 396.19 TF
(3.37E-4) 0 -270 280.49 448.07 TF
(-2.240) 0 -270 280.49 495.75 TF
(-2.250) 0 -270 280.49 534.5 TF
(-3.719) 0 -270 280.49 573.25 TF
(-3.248) 0 -270 280.49 612 TF
(91 Aqr) 0 -270 293.49 161.69 TF
(K0III) 0 -270 293.49 209.76 TF
(1.010) 0 -270 293.49 254.92 TF
(8.535E6) 0 -270 293.49 293.95 TF
(1.662E4) 0 -270 293.49 345.07 TF
(6.381E0) 0 -270 293.49 396.19 TF
(2.61E-4) 0 -270 293.49 448.07 TF
(-2.237) 0 -270 293.49 495.75 TF
(-2.247) 0 -270 293.49 534.5 TF
(-3.719) 0 -270 293.49 573.25 TF
(-3.247) 0 -270 293.49 612 TF
(HD95272) 0 -270 306.49 151.44 TF
(K0III) 0 -270 306.49 209.76 TF
(1.041) 0 -270 306.49 254.92 TF
(8.184E6) 0 -270 306.49 293.95 TF
(1.593E4) 0 -270 306.49 345.07 TF
(6.086E0) 0 -270 306.49 396.19 TF
(2.49E-4) 0 -270 306.49 448.07 TF
(-2.236) 0 -270 306.49 495.75 TF
(-2.246) 0 -270 306.49 534.5 TF
(-3.719) 0 -270 306.49 573.25 TF
(-3.247) 0 -270 306.49 612 TF
9 10 Q
(y) 0 -270 319.49 159.08 TF
5 9 Q
(UMa) 0 -270 319.49 168.44 TF
(K1III) 0 -270 319.49 209.76 TF
(1.081) 0 -270 319.49 254.92 TF
(6.894E6) 0 -270 319.49 293.95 TF
(1.342E4) 0 -270 319.49 345.07 TF
(5.143E0) 0 -270 319.49 396.19 TF
(2.10E-4) 0 -270 319.49 448.07 TF
(-2.237) 0 -270 319.49 495.75 TF
(-2.247) 0 -270 319.49 534.5 TF
(-3.719) 0 -270 319.49 573.25 TF
(-3.247) 0 -270 319.49 612 TF
(BD+1) 0 -270 332.49 143.26 TF
5 7.2 Q
(o) 0 -270 328.89 165.33 TF
5 9 Q
(3131) 0 -270 332.49 168.93 TF
(K0III) 0 -270 332.49 209.76 TF
(1.143) 0 -270 332.49 254.92 TF
(4.403E6) 0 -270 332.49 293.95 TF
(8.51) 0 -270 332.49 345.24 TF
(1E3) 0 -270 332.49 360.65 TF
(7.928E0) 0 -270 332.49 396.19 TF
(2.54E-4) 0 -270 332.49 448.07 TF
(-2.210) 0 -270 332.49 495.75 TF
(-2.221) 0 -270 332.49 534.5 TF
(-3.718) 0 -270 332.49 573.25 TF
(-3.242) 0 -270 332.49 612 TF
(vB 173) 0 -270 345.49 160.68 TF
(1.202) 0 -270 345.49 254.92 TF
(6.753E6) 0 -270 345.49 293.95 TF
(1.337E4) 0 -270 345.49 345.07 TF
(2.396E1) 0 -270 345.49 396.19 TF
(7.80E-4) 0 -270 345.49 448.07 TF
(-2.296) 0 -270 345.49 495.75 TF
(-2.31) 0 -270 345.49 534.67 TF
(1) 0 -270 345.49 553.08 TF
(-3.721) 0 -270 345.49 573.25 TF
(-3.260) 0 -270 345.49 612 TF
(HD166780) 0 -270 358.49 146.94 TF
(K5III) 0 -270 358.49 209.76 TF
(1.323) 0 -270 358.49 254.92 TF
(2.059E6) 0 -270 358.49 293.95 TF
(3.986E3) 0 -270 358.49 345.07 TF
(3.791E0) 0 -270 358.49 396.19 TF
(1.21E-4) 0 -270 358.49 448.07 TF
(-2.214) 0 -270 358.49 495.75 TF
(-2.225) 0 -270 358.49 534.5 TF
(-3.718) 0 -270 358.49 573.25 TF
(-3.243) 0 -270 358.49 612 TF
(RZ Her) 0 -270 371.49 159.69 TF
(M6III) 0 -270 371.49 209.01 TF
(1.380) 0 -270 371.49 254.92 TF
(5.352E6) 0 -270 371.49 293.95 TF
(1.042E4) 0 -270 371.49 345.07 TF
(1.057E1) 0 -270 371.49 396.19 TF
(3.39E-4) 0 -270 371.49 448.07 TF
(-2.228) 0 -270 371.49 495.75 TF
(-2.239) 0 -270 371.49 534.5 TF
(-3.718) 0 -270 371.49 573.25 TF
(-3.246) 0 -270 371.49 612 TF
(HD1) 0 -270 384.49 147.27 TF
(16870) 0 -270 384.49 164.43 TF
(M0III) 0 -270 384.49 209.01 TF
(1.413) 0 -270 384.49 254.92 TF
(1.414E6) 0 -270 384.49 293.95 TF
(2.734E3) 0 -270 384.49 345.07 TF
(2.228E0) 0 -270 384.49 396.19 TF
(7.87E-5) 0 -270 384.49 448.07 TF
(-2.207) 0 -270 384.49 495.75 TF
(-2.218) 0 -270 384.49 534.5 TF
(-3.717) 0 -270 384.49 573.25 TF
(-3.241) 0 -270 384.49 612 TF
(M67 IV) 0 -270 397.49 142.52 TF
(-202) 0 -270 397.49 170.44 TF
(1.463) 0 -270 397.49 254.92 TF
(1.170E6) 0 -270 397.49 293.95 TF
(2.263E3) 0 -270 397.49 345.07 TF
(1.857E0) 0 -270 397.49 396.19 TF
(6.56E-5) 0 -270 397.49 448.07 TF
(-2.208) 0 -270 397.49 495.75 TF
(-2.219) 0 -270 397.49 534.5 TF
(-3.717) 0 -270 397.49 573.25 TF
(-3.242) 0 -270 397.49 612 TF
(HD104216) 0 -270 410.49 146.94 TF
(M2III) 0 -270 410.49 209.01 TF
(1.523) 0 -270 410.49 254.92 TF
(1.423E6) 0 -270 410.49 293.95 TF
(2.795E3) 0 -270 410.49 345.07 TF
(4.603E0) 0 -270 410.49 396.19 TF
(1.50E-4) 0 -270 410.49 448.07 TF
(-2.271) 0 -270 410.49 495.75 TF
(-2.287) 0 -270 410.49 534.5 TF
(-3.721) 0 -270 410.49 573.25 TF
(-3.255) 0 -270 410.49 612 TF
(BD\3201) 0 -270 423.49 144.17 TF
5 7.2 Q
(o) 0 -270 419.89 165.67 TF
5 9 Q
(31) 0 -270 423.49 169.27 TF
(13) 0 -270 423.49 177.93 TF
(K5III) 0 -270 423.49 209.76 TF
(1.609) 0 -270 423.49 254.92 TF
(8.070E5) 0 -270 423.49 293.95 TF
(1.588E3) 0 -270 423.49 345.07 TF
(2.681E0) 0 -270 423.49 396.19 TF
(8.72E-5) 0 -270 423.49 448.07 TF
(-2.277) 0 -270 423.49 495.75 TF
(-2.293) 0 -270 423.49 534.5 TF
(-3.721) 0 -270 423.49 573.25 TF
(-3.256) 0 -270 423.49 612 TF
(HD142804) 0 -270 436.49 146.94 TF
(M1III) 0 -270 436.49 209.01 TF
(1.694) 0 -270 436.49 254.92 TF
(7.419E5) 0 -270 436.49 293.95 TF
(1.463E3) 0 -270 436.49 345.07 TF
(2.517E0) 0 -270 436.49 396.19 TF
(8.19E-5) 0 -270 436.49 448.07 TF
(-2.283) 0 -270 436.49 495.75 TF
(-2.299) 0 -270 436.49 534.5 TF
(-3.721) 0 -270 436.49 573.25 TF
(-3.258) 0 -270 436.49 612 TF
(Gl 15B) 0 -270 449.49 160.68 TF
(M6V) 0 -270 449.49 210.25 TF
(1.707) 0 -270 449.49 254.92 TF
(2.391E6) 0 -270 449.49 293.95 TF
(4.742E3) 0 -270 449.49 345.07 TF
(8.704E0) 0 -270 449.49 396.19 TF
(2.83E-4) 0 -270 449.49 448.07 TF
(-2.303) 0 -270 449.49 495.75 TF
(-2.318) 0 -270 449.49 534.5 TF
(-3.721) 0 -270 449.49 573.25 TF
(-3.262) 0 -270 449.49 612 TF
(Gl 65) 0 -270 462.49 166.68 TF
(M5V) 0 -270 462.49 210.25 TF
(1.768) 0 -270 462.49 254.92 TF
(1.075E7) 0 -270 462.49 293.95 TF
(2.122E4) 0 -270 462.49 345.07 TF
(3.642E1) 0 -270 462.49 396.19 TF
(1.18E-3) 0 -270 462.49 448.07 TF
(-2.284) 0 -270 462.49 495.75 TF
(-2.300) 0 -270 462.49 534.5 TF
(-3.721) 0 -270 462.49 573.25 TF
(-3.258) 0 -270 462.49 612 TF
(HD 151658) 0 -270 475.49 144.69 TF
(M2III) 0 -270 475.49 209.01 TF
(1.770) 0 -270 475.49 254.92 TF
(7.242E5) 0 -270 475.49 293.95 TF
(1.423E3) 0 -270 475.49 345.07 TF
(2.359E0) 0 -270 475.49 396.19 TF
(7.67E-5) 0 -270 475.49 448.07 TF
(-2.272) 0 -270 475.49 495.75 TF
(-2.288) 0 -270 475.49 534.5 TF
(-3.721) 0 -270 475.49 573.25 TF
(-3.255) 0 -270 475.49 612 TF
(R Leo) 0 -270 488.49 164.69 TF
(1.918) 0 -270 488.49 254.92 TF
(4.550E6) 0 -270 488.49 293.95 TF
(8.879E3) 0 -270 488.49 345.07 TF
(1.308E1) 0 -270 488.49 396.19 TF
(4.26E-4) 0 -270 488.49 448.07 TF
(-2.245) 0 -270 488.49 495.75 TF
(-2.260) 0 -270 488.49 534.5 TF
(-3.721) 0 -270 488.49 573.25 TF
(-3.250) 0 -270 488.49 612 TF
(WZ Cas) 0 -270 501.49 157.19 TF
(N) 0 -270 501.49 216.5 TF
(2.636) 0 -270 501.49 254.92 TF
(1.987E5) 0 -270 501.49 293.95 TF
(3.867E2) 0 -270 501.49 345.07 TF
(5.89E-1) 0 -270 501.49 396.95 TF
(1.92E-5) 0 -270 501.49 448.07 TF
(-2.246) 0 -270 501.49 495.75 TF
(-2.263) 0 -270 501.49 534.5 TF
(-3.721) 0 -270 501.49 573.25 TF
(-3.250) 0 -270 501.49 612 TF
(A) 0 -270 514.49 155.41 TF
(W Cyg) 0 -270 514.49 161.18 TF
(N) 0 -270 514.49 216.5 TF
(3.790) 0 -270 514.49 254.92 TF
(1.951E5) 0 -270 514.49 293.95 TF
(3.796E2) 0 -270 514.49 345.07 TF
(5.70E-1) 0 -270 514.49 396.95 TF
(1.85E-5) 0 -270 514.49 448.07 TF
(-2.243) 0 -270 514.49 495.75 TF
(-2.260) 0 -270 514.49 534.5 TF
(-3.721) 0 -270 514.49 573.25 TF
(-3.249) 0 -270 514.49 612 TF
30.49 134.01 43.49 699 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
36.49 269.01 36.49 620.01 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
36.49 134.01 36.49 260.01 2 L
0 Z
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 0 -270 49.49 134.01 TF
(ABLE 7-1) 0 -270 49.49 138.84 TF
3 F
(Predicted target acquisition count rates for stars, reduced to) 0 -270 49.49 269.01 TF
4 F
(V) 0 -270 49.49 509.62 TF
4 7.2 Q
(0) 0 -270 51.74 515.62 TF
3 9 Q
(= 0. \050Continued\051) 0 -270 49.49 522.13 TF
0 8 Q
(Star Name) 0 -270 75.83 143.69 TF
(Spectral) 0 -270 70.83 203.97 TF
(T) 0 -270 80.83 210.71 TF
(ype) 0 -270 80.83 215.01 TF
10 F
(\050B\320V\051) 0 -270 75.83 252.82 TF
10 6.4 Q
(0) 0 -270 77.83 273.71 TF
0 8 Q
(count rate for mirror) 0 -270 67.83 347.08 TF
(reddening reduction factor) 0 -270 67.83 512.82 TF
0 6.4 Q
(a) 0 -270 64.63 614.61 TF
0 8 Q
(N2) 0 -270 83.83 303.96 TF
(A2) 0 -270 83.83 355.08 TF
(N1) 0 -270 83.83 406.21 TF
(A1) 0 -270 83.83 457.33 TF
(N2) 0 -270 83.83 502.26 TF
(A2) 0 -270 83.83 541.01 TF
(N1) 0 -270 83.83 579.76 TF
(A1) 0 -270 83.83 618.51 TF
58.62 134.01 519.37 134.01 2 L
V
0.25 H
0 Z
N
58.37 192.93 519.62 192.93 2 L
V
N
58.37 246.57 519.62 246.57 2 L
V
N
58.37 283.51 519.62 283.51 2 L
V
2 H
N
74.37 334.64 519.62 334.64 2 L
V
0.25 H
N
74.37 385.76 519.62 385.76 2 L
V
N
74.37 436.88 519.62 436.88 2 L
V
N
58.37 488 519.62 488 2 L
V
N
74.37 526.75 519.62 526.75 2 L
V
N
74.37 565.5 519.62 565.5 2 L
V
N
74.37 604.24 519.62 604.24 2 L
V
N
58.62 642.99 519.37 642.99 2 L
V
N
58.49 133.88 58.49 643.12 2 L
V
N
74.49 282.51 74.49 643.12 2 L
V
N
90.49 133.88 90.49 643.12 2 L
V
0.5 H
N
129.49 133.88 129.49 643.12 2 L
V
0.25 H
N
194.49 133.88 194.49 643.12 2 L
V
N
259.49 133.88 259.49 643.12 2 L
V
N
324.49 133.88 324.49 643.12 2 L
V
N
389.49 133.88 389.49 643.12 2 L
V
N
454.49 133.88 454.49 643.12 2 L
V
N
519.49 133.88 519.49 643.12 2 L
V
N
520.77 416.46 536.74 466.45 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 9 Q
0 X
0 0 0 1 0 0 0 K
(1) 0 -270 532.49 417.47 TF
(0) 0 -270 532.49 421.97 TF
7 7 Q
(f) 0 -270 527.02 426.81 TF
(E) 0 -270 527.02 436.09 TF
(B) 0 -270 527.02 445.08 TF
(V) 0 -270 527.02 456.35 TF
5 F
(\320) 0 -270 527.02 451.1 TF
9 F
(\050) 0 -270 527.02 442.08 TF
(\051) 0 -270 527.02 460.95 TF
(\264) 0 -270 527.02 430.5 TF
0 0 612 792 C
FMENDPAGE
%%EndPage: "75" 9
%%Page: "76" 10
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(T) 189 736.18 T
(arget Acquisition Reference Information) 193.83 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(76) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
72 669 558 672 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 670.5 558 670.5 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 670.5 198 670.5 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(7.3) 181.32 676 T
(Acquisition Count Rates for Extended Objects) 207 676 T
5 10 Q
0.62 (Chapter 4 mentions acquisition methodologies for extended objects, and, in particular) 207 648.33 P
0.62 (,) 555.5 648.33 P
-0.06 (the use of the) 207 636.33 P
6 F
-0.16 (EXTENDED) 262.84 636.33 P
5 F
-0.06 ( optional parameter) 310.84 636.33 P
-0.06 (. In this section we provide some guidance) 387.92 636.33 P
-0.06 (on predicting the count rates to be expected during an acquisition of an extended object,) 207 624.33 P
-0.14 (especially one beyond our own Galaxy) 207 612.33 P
-0.14 (. The renewed availability of Side 1 of the GHRS) 361.47 612.33 P
0.48 (and its G140L grating make it possible to get high-quality spectra of faint objects ef) 207 600.33 P
0.48 (\336-) 549.11 600.33 P
(ciently) 207 588.33 T
(.) 233.57 588.33 T
0.68 (Whenever possible, we recommend that faint objects be acquired by of) 207 564.33 P
0.68 (fsetting from a) 497.75 564.33 P
-0.09 (nearby and brighter point source. If accurate coordinates are used this method should be) 207 552.33 P
0.74 (reliable. However) 207 540.33 P
0.74 (, such objects are not always present next to tar) 278.98 540.33 P
0.74 (gets of astrophysical) 474.31 540.33 P
0.49 (interest. Also, obtaining a good astrometric position of an extended source can be pre-) 207 528.33 P
0.13 (vented by its lar) 207 516.33 P
0.13 (ge saturated area on the photographic plates upon which the Guide Star) 271.37 516.33 P
-0.08 (Catalog is based. In these cases a direct tar) 207 504.33 P
-0.08 (get acquisition will need to be attempted, and) 376.94 504.33 P
2.02 (it should succeed if the object provides enough ultraviolet photons. The procedure) 207 492.33 P
(closely follows that for point sources just described:) 207 480.33 T
8 11 Q
(\245) 207 462.33 T
5 10 Q
-0.15 (Find a star in T) 221.4 462.33 P
-0.15 (able) 281.22 462.33 P
-0.15 (7-1 with a spectral ener) 300.38 462.33 P
-0.15 (gy distribution like that of your object, or) 393.48 462.33 P
0.52 (consult the IUE Atlas of Star) 221.4 450.33 P
0.52 (-Forming Galaxies, by Kinney et al. \0501993, ApJS, 86,) 339.65 450.33 P
0.25 (5\051. This publication provides representative spectra of many classes of galaxies and) 221.4 438.33 P
(compares their shapes to ones of stellar spectra \050whence the \322spectral types\323 listed\051.) 221.4 426.33 T
8 11 Q
(\245) 207 411.33 T
5 10 Q
0.14 (Estimate the \337ux that will fall within the LSA from either T) 221.4 411.33 P
0.14 (able) 461.37 411.33 P
0.14 (7-1 or T) 480.53 411.33 P
0.14 (able) 512.87 411.33 P
0.14 (7-2 on) 532.03 411.33 P
(page) 221.4 399.33 T
(77, as appropriate.) 242.78 399.33 T
8 11 Q
(\245) 207 384.33 T
5 10 Q
0.62 (Calculate) 221.4 384.33 P
6 F
1.48 (STEP-TIME) 262.29 384.33 P
5 F
0.62 ( in the same manner as for stars. If necessary) 316.29 384.33 P
0.62 (, you may use) 500.59 384.33 P
-0.12 (mirror N2 on Side 2 for your acquisition, even if Side 1 is being used to observe, but) 221.4 372.33 P
(doing so will add about 40 minutes of overhead time.) 221.4 360.33 T
8 11 Q
(\245) 207 345.33 T
5 10 Q
(If your object does not fall within these categories, please consult us.) 221.4 345.33 T
FMENDPAGE
%%EndPage: "76" 10
%%Page: "77" 11
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (77) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(T) 207 736.18 T
(arget Acquisition Reference Information) 211.83 736.18 T
88.7 104.02 505.3 111.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 612 792 C
5 9 Q
0 X
0 0 0 1 0 0 0 K
(a. use factor) 235.7 98.02 T
7 F
(f) 281.68 98.02 T
5 F
( to reduce count rate by) 284.18 98.02 T
(.) 421.14 98.02 T
88.7 665.02 540 678.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
223.7 672.02 574.7 672.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
88.7 672.02 214.7 672.02 2 L
0 Z
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 88.7 659.02 T
(ABLE 7-2) 93.53 659.02 T
3 F
(Predicted count rates for non-stellar objects) 223.7 659.02 T
0 8 Q
(\322Spectral) 99.48 637.68 T
(T) 106.22 627.68 T
(ype\323) 110.52 627.68 T
(count rate for mirror) 209.4 640.68 T
(reddening reduction factor) 375.13 640.68 T
0 6.4 Q
(a) 476.92 643.88 T
0 8 Q
(N2) 166.27 624.68 T
(A2) 217.39 624.68 T
(N1) 268.52 624.68 T
(A1) 319.64 624.68 T
(N2) 364.57 624.68 T
(A2) 403.32 624.68 T
(N1) 442.07 624.68 T
(A1) 480.82 624.68 T
5 9 Q
(o3_6v) 106.01 610.02 T
(8.843E9) 156.26 610.02 T
(2.1) 207.55 610.02 T
(16E7) 218.46 610.02 T
(3.990E8) 258.5 610.02 T
(2.726E5) 309.62 610.02 T
(-3.059) 358.06 610.02 T
(-3.1) 396.98 610.02 T
(12) 410.89 610.02 T
(-3.362) 435.56 610.02 T
(-3.134) 474.31 610.02 T
(o4_9i) 107.01 597.02 T
(8.047E9) 156.26 597.02 T
(1.934E7) 207.38 597.02 T
(3.731E8) 258.5 597.02 T
(2.427E5) 309.62 597.02 T
(-3.054) 358.06 597.02 T
(-3.109) 396.81 597.02 T
(-3.380) 435.56 597.02 T
(-3.133) 474.31 597.02 T
(o5_6iii) 104.51 584.02 T
(8.935E9) 156.26 584.02 T
(2.140E7) 207.38 584.02 T
(3.961E8) 258.5 584.02 T
(2.687E5) 309.62 584.02 T
(-3.068) 358.06 584.02 T
(-3.121) 396.81 584.02 T
(-3.364) 435.56 584.02 T
(-3.136) 474.31 584.02 T
(o7_b0v) 103.76 571.02 T
(7.407E9) 156.26 571.02 T
(1.771E7) 207.38 571.02 T
(3.282E8) 258.5 571.02 T
(2.065E5) 309.62 571.02 T
(-3.028) 358.06 571.02 T
(-3.086) 396.81 571.02 T
(-3.388) 435.56 571.02 T
(-3.129) 474.31 571.02 T
(o9_b0iv) 102.51 558.02 T
(6.413E9) 156.26 558.02 T
(1.533E7) 207.38 558.02 T
(2.931E8) 258.5 558.02 T
(1.784E5) 309.62 558.02 T
(-3.012) 358.06 558.02 T
(-3.072) 396.81 558.02 T
(-3.396) 435.56 558.02 T
(-3.125) 474.31 558.02 T
(b0_2i) 107.01 545.02 T
(4.314E9) 156.26 545.02 T
(1.005E7) 207.38 545.02 T
(1.372E8) 258.5 545.02 T
(9.530E4) 309.62 545.02 T
(-2.949) 358.06 545.02 T
(-3.005) 396.81 545.02 T
(-3.378) 435.56 545.02 T
(-3.1) 474.47 545.02 T
(13) 488.39 545.02 T
(b0_2iii) 104.51 532.02 T
(5.144E9) 156.26 532.02 T
(1.214E7) 207.38 532.02 T
(1.908E8) 258.5 532.02 T
(1.231E5) 309.62 532.02 T
(-2.994) 358.06 532.02 T
(-3.051) 396.81 532.02 T
(-3.388) 435.56 532.02 T
(-3.122) 474.31 532.02 T
(b2_4v) 106.01 519.02 T
(2.889E9) 156.26 519.02 T
(6.765E6) 207.38 519.02 T
(1.037E8) 258.5 519.02 T
(7.131E4) 309.62 519.02 T
(-2.964) 358.06 519.02 T
(-3.021) 396.81 519.02 T
(-3.364) 435.56 519.02 T
(-3.1) 474.47 519.02 T
(16) 488.39 519.02 T
(b2_5iv) 104.76 506.02 T
(2.754E9) 156.26 506.02 T
(6.444E6) 207.38 506.02 T
(9.673E7) 258.5 506.02 T
(6.712E4) 309.62 506.02 T
(-2.960) 358.06 506.02 T
(-3.017) 396.81 506.02 T
(-3.367) 435.56 506.02 T
(-3.1) 474.47 506.02 T
(15) 488.39 506.02 T
(b3_5i) 107.01 493.02 T
(1.694E9) 156.26 493.02 T
(3.836E6) 207.38 493.02 T
(3.581E7) 258.5 493.02 T
(3.042E4) 309.62 493.02 T
(-2.859) 358.06 493.02 T
(-2.910) 396.81 493.02 T
(-3.328) 435.56 493.02 T
(-3.095) 474.31 493.02 T
(b3_6iii) 104.51 480.02 T
(2.344E9) 156.26 480.02 T
(5.448E6) 207.38 480.02 T
(7.404E7) 258.5 480.02 T
(5.400E4) 309.62 480.02 T
(-2.943) 358.06 480.02 T
(-2.998) 396.81 480.02 T
(-3.353) 435.56 480.02 T
(-3.1) 474.47 480.02 T
(12) 488.39 480.02 T
(b5_8v) 106.01 467.02 T
(1.713E9) 156.26 467.02 T
(3.952E6) 207.38 467.02 T
(4.849E7) 258.5 467.02 T
(3.716E4) 309.62 467.02 T
(-2.922) 358.06 467.02 T
(-2.976) 396.81 467.02 T
(-3.337) 435.56 467.02 T
(-3.108) 474.31 467.02 T
(b6_9i) 107.01 454.02 T
(9.689E8) 156.26 454.02 T
(2.187E6) 207.38 454.02 T
(2.021E7) 258.5 454.02 T
(1.765E4) 309.62 454.02 T
(-2.831) 358.06 454.02 T
(-2.882) 396.81 454.02 T
(-3.313) 435.56 454.02 T
(-3.089) 474.31 454.02 T
(b7_9iii) 104.51 441.02 T
(8.700E8) 156.26 441.02 T
(1.975E6) 207.38 441.02 T
(1.845E7) 258.5 441.02 T
(1.663E4) 309.62 441.02 T
(-2.867) 358.06 441.02 T
(-2.918) 396.81 441.02 T
(-3.305) 435.56 441.02 T
(-3.098) 474.31 441.02 T
(b8_9iv) 104.76 428.02 T
(9.701E8) 156.26 428.02 T
(2.216E6) 207.38 428.02 T
(2.337E7) 258.5 428.02 T
(1.984E4) 309.62 428.02 T
(-2.889) 358.06 428.02 T
(-2.941) 396.81 428.02 T
(-3.316) 435.56 428.02 T
(-3.102) 474.31 428.02 T
(f2_7iv) 105.51 415.02 T
(1.007E8) 156.26 415.02 T
(2.108E5) 207.38 415.02 T
(2.968E4) 258.5 415.02 T
(1.206E2) 309.62 415.02 T
(-2.547) 358.06 415.02 T
(-2.580) 396.81 415.02 T
(-3.201) 435.56 415.02 T
(-3.043) 474.31 415.02 T
(f2_8i) 107.76 402.02 T
(4.536E7) 156.26 402.02 T
(9.480E4) 207.38 402.02 T
(1.403E4) 258.5 402.02 T
(5.634E1) 309.62 402.02 T
(-2.535) 358.06 402.02 T
(-2.569) 396.81 402.02 T
(-3.201) 435.56 402.02 T
(-3.041) 474.31 402.02 T
(f5_7v) 106.76 389.02 T
(1.079E8) 156.26 389.02 T
(2.254E5) 207.38 389.02 T
(1.782E4) 258.5 389.02 T
(-2.538) 358.06 389.02 T
(-2.571) 396.81 389.02 T
(-3.238) 435.56 389.02 T
(f6iii) 109.76 376.02 T
(9.009E7) 156.26 376.02 T
(1.862E5) 207.38 376.02 T
(8.586E2) 258.5 376.02 T
(-2.499) 358.06 376.02 T
(-2.526) 396.81 376.02 T
(-3.830) 435.56 376.02 T
(f8_9v) 106.76 363.02 T
(6.664E7) 156.26 363.02 T
(1.367E5) 207.38 363.02 T
(3.996E3) 258.5 363.02 T
(-2.460) 358.06 363.02 T
(-2.484) 396.81 363.02 T
(-3.245) 435.56 363.02 T
(g0_2iv) 104.76 350.02 T
(4.451E7) 156.26 350.02 T
(9.041E4) 207.38 350.02 T
(3.614E2) 258.5 350.02 T
(-2.415) 358.06 350.02 T
(-2.434) 396.81 350.02 T
(-3.604) 435.56 350.02 T
(g0_3i) 107.01 337.02 T
(1.971E7) 156.26 337.02 T
(4.015E4) 207.38 337.02 T
(-2.429) 358.06 337.02 T
(-2.444) 396.81 337.02 T
(g0_5iii) 104.51 324.02 T
(3.349E7) 156.26 324.02 T
(6.822E4) 207.38 324.02 T
(-2.431) 358.06 324.02 T
(-2.450) 396.81 324.02 T
(g0_5v) 106.01 311.02 T
(5.372E7) 156.26 311.02 T
(1.095E5) 207.38 311.02 T
(-2.428) 358.06 311.02 T
(-2.449) 396.81 311.02 T
(g5_8i) 107.01 298.02 T
(4.802E6) 156.26 298.02 T
(9.721E3) 207.38 298.02 T
(-2.399) 358.06 298.02 T
(-2.414) 396.81 298.02 T
(g5_8iv) 104.76 285.02 T
(2.123E7) 156.26 285.02 T
(4.242E4) 207.38 285.02 T
(-2.344) 358.06 285.02 T
(-2.354) 396.81 285.02 T
(g5_k0iii) 102.26 272.02 T
(6.969E6) 156.26 272.02 T
(1.384E4) 207.38 272.02 T
(-2.320) 358.06 272.02 T
(-2.330) 396.81 272.02 T
(g6_9v) 106.01 259.02 T
(2.588E7) 156.26 259.02 T
(5.189E4) 207.38 259.02 T
(-2.360) 358.06 259.02 T
(-2.372) 396.81 259.02 T
(g8_k1iv) 102.51 246.02 T
(8.008E6) 156.26 246.02 T
(1.583E4) 207.38 246.02 T
(-2.297) 358.06 246.02 T
(-2.304) 396.81 246.02 T
(k0_1v) 106.01 233.02 T
(1.307E7) 156.26 233.02 T
(2.606E4) 207.38 233.02 T
(-2.337) 358.06 233.02 T
(-2.348) 396.81 233.02 T
(k0_2iii) 104.51 220.02 T
(5.918E6) 156.26 220.02 T
(1.165E4) 207.38 220.02 T
(-2.285) 358.06 220.02 T
(-2.290) 396.81 220.02 T
(k1_3i) 107.01 207.02 T
(2.497E6) 156.26 207.02 T
(5.057E3) 207.38 207.02 T
(-2.397) 358.06 207.02 T
(-2.41) 396.98 207.02 T
(1) 415.39 207.02 T
(k2_3v) 106.01 194.02 T
(9.035E6) 156.26 194.02 T
(1.800E4) 207.38 194.02 T
(-2.327) 358.06 194.02 T
(-2.336) 396.81 194.02 T
(k2iii) 109.01 181.02 T
(2.092E6) 156.26 181.02 T
(4.107E3) 207.38 181.02 T
(-2.268) 358.06 181.02 T
(-2.273) 396.81 181.02 T
(k3iii) 109.01 168.02 T
(1.157E6) 156.26 168.02 T
(2.266E3) 207.38 168.02 T
(-2.259) 358.06 168.02 T
(-2.264) 396.81 168.02 T
(k4_5iii) 104.51 155.02 T
(5.490E5) 156.26 155.02 T
(1.085E3) 207.38 155.02 T
(-2.290) 358.06 155.02 T
(-2.296) 396.81 155.02 T
(k5_m0v) 102.51 142.02 T
(2.607E6) 156.26 142.02 T
(5.167E3) 207.38 142.02 T
(-2.304) 358.06 142.02 T
(-2.31) 396.98 142.02 T
(1) 415.39 142.02 T
(k5_m5i) 103.51 129.02 T
(9.714E5) 156.26 129.02 T
(1.976E3) 207.38 129.02 T
(-2.413) 358.06 129.02 T
(-2.426) 396.81 129.02 T
(k7_m3iii) 101.01 116.02 T
(5.420E5) 156.26 116.02 T
(1.081E3) 207.38 116.02 T
(-2.323) 358.06 116.02 T
(-2.330) 396.81 116.02 T
88.7 649.89 88.7 111.14 2 L
V
0.25 H
0 Z
N
145.82 650.14 145.82 110.89 2 L
V
N
196.95 634.14 196.95 110.89 2 L
V
N
248.07 634.14 248.07 110.89 2 L
V
N
299.19 634.14 299.19 110.89 2 L
V
N
350.31 650.14 350.31 110.89 2 L
V
N
389.06 634.14 389.06 110.89 2 L
V
N
427.81 634.14 427.81 110.89 2 L
V
N
466.55 634.14 466.55 110.89 2 L
V
N
505.3 649.89 505.3 111.14 2 L
V
N
88.57 650.02 505.43 650.02 2 L
V
N
145.7 634.02 505.43 634.02 2 L
V
N
88.57 618.02 505.43 618.02 2 L
V
0.5 H
N
88.57 553.02 505.43 553.02 2 L
V
0.25 H
N
88.57 488.02 505.43 488.02 2 L
V
N
88.57 423.02 505.43 423.02 2 L
V
N
88.57 358.02 505.43 358.02 2 L
V
N
88.57 293.02 505.43 293.02 2 L
V
N
88.57 228.02 505.43 228.02 2 L
V
N
88.57 163.02 505.43 163.02 2 L
V
N
88.57 111.02 505.43 111.02 2 L
V
N
371.16 93.77 421.14 109.74 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 9 Q
0 X
0 0 0 1 0 0 0 K
(1) 372.16 98.02 T
(0) 376.66 98.02 T
7 7 Q
(f) 381.5 103.49 T
(E) 390.78 103.49 T
(B) 399.77 103.49 T
(V) 411.04 103.49 T
5 F
(\320) 405.79 103.49 T
9 F
(\050) 396.77 103.49 T
(\051) 415.64 103.49 T
(\264) 385.19 103.49 T
0 0 612 792 C
FMENDPAGE
%%EndPage: "77" 11
%%Page: "78" 12
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(T) 189 736.18 T
(arget Acquisition Reference Information) 193.83 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(78) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
72 671.02 558 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 672.52 558 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 672.52 198 672.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(7.4) 181.32 678.02 T
(Other Acquisition Information) 207 678.02 T
0 10 Q
(7.4.1) 175.76 644.35 T
(Effective Areas of the Acquisition Mirrors) 207 644.35 T
5 F
0.04 (T) 207 620.35 P
0.04 (able) 212.41 620.35 P
0.04 (7-3 on page) 231.57 620.35 P
0.04 (79 lists the ef) 281.35 620.35 P
0.04 (fective areas of the four acquisition mirrors \050in) 334.89 620.35 P
0.04 (\051 as) 543.8 620.35 P
1.38 (a function of wavelength, to use to predict acquisition count rates. These values are) 207 608.35 P
-0.17 (those from the Science V) 207 596.35 P
-0.17 (eri\336cation Report for the GHRS, adjusted by the observed ratio) 306.28 596.35 P
-0.09 (of post- to pre-COST) 207 584.35 P
-0.09 (AR sensitivities \050see Section) 291.19 584.35 P
-0.09 (8.1 on page) 408.13 584.35 P
-0.09 (82\051. Note that A1 and N1) 456.82 584.35 P
(may only be used with detector D1 and A2 and N2 with detector D2.) 207 572.35 T
0.33 (Also note that the proper use of this table requires compensation for the dif) 207 548.35 P
0.33 (ferent ener-) 511.31 548.35 P
-0.18 (gies of photons of dif) 207 536.35 P
-0.18 (ferent wavelengths, hence the last column, which is in picoer) 291.66 536.35 P
-0.18 (gs per) 534.02 536.35 P
(photon.) 207 524.35 T
0 F
0.19 (Figure 7-5.) 144 179.33 P
3 F
0.19 (Relative sensitivities of the GHRS acquisition mirrors. The ef) 200.7 179.33 P
0.19 (fec-) 469.33 179.33 P
(tive areas shown are from T) 144 167.33 T
(able) 266.82 167.33 T
(7-3 on page) 288.5 167.33 T
(79.) 344.65 167.33 T
524.58 615.85 543.8 629.47 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(c) 525.58 620.35 T
(m) 530.02 620.35 T
5 7 Q
(2) 538.3 623.22 T
0 0 612 792 C
72 87.98 558 686.02 C
72 195 558 506.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
270 29 38 538 744 285.03 395.35 172.48 152.83 FMBEGINEPSF
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987 2316 d 1011 2292 d 1011 2326 d 783 1453 r 834 1453 d 783 1453 r
834 1486 d 783 1486 r 834 1486 d 793 1510 r 790 1515 d 783 1522 d
834 1522 d 230 2248 r 281 2248 d 230 2248 r 281 2281 d 230 2281 r
281 2281 d 242 2300 r 240 2300 d 235 2303 d 233 2305 d 230 2310 d
230 2320 d 233 2324 d 235 2327 d 240 2329 d 245 2329 d 249 2327 d
257 2322 d 281 2298 d 281 2332 d
e
%%Trailer
EndPSPlot

%%EndDocument
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0 0 612 792 C
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612 792 0 FMBEGINPAGE
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7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (79) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(T) 207 736.18 T
(arget Acquisition Reference Information) 211.83 736.18 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 660.02 540 673.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 667.02 540 667.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 667.02 180 667.02 2 L
0 Z
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 654.02 T
(ABLE 7-3.) 58.83 654.02 T
3 F
(Ef) 189 654.02 T
(fective areas of the four GHRS acquisition mirrors) 197.34 654.02 T
0 8 Q
(W) 203.14 613.68 T
(avelength) 210.39 613.68 T
(\050\201\051) 249.96 613.68 T
(Effective Area \050cm) 342.89 630.68 T
0 6.4 Q
(2) 412.69 633.88 T
0 8 Q
(\051) 416.25 630.68 T
(perg) 504.33 622.68 T
(photon) 496.6 613.68 T
0 6.4 Q
(-1) 523.71 616.88 T
0 8 Q
(A1) 294.79 613.68 T
(N1) 345.89 613.68 T
(A2) 399.89 613.68 T
(N2) 453.89 613.68 T
5 9 Q
(1) 223.27 599.02 T
(100) 227.43 599.02 T
(0.0025) 338.62 599.02 T
(0.00085) 390.38 599.02 T
(0.175) 448.88 599.02 T
(18.1) 505.12 599.02 T
(1) 223.27 584.02 T
(150) 227.43 584.02 T
(4.89) 343.12 584.02 T
(0.12) 397.12 584.02 T
(23.36) 448.88 584.02 T
(17.3) 505.12 584.02 T
(1200) 223.1 569.02 T
(16.79) 340.88 569.02 T
(0.29) 397.12 569.02 T
(54.18) 448.88 569.02 T
(16.6) 505.12 569.02 T
(1250) 223.1 554.02 T
(28.54) 340.88 554.02 T
(0.34) 397.12 554.02 T
(76.50) 448.88 554.02 T
(15.9) 505.12 554.02 T
(1300) 223.1 539.02 T
(34.10) 340.88 539.02 T
(0.37) 397.12 539.02 T
(96.22) 448.88 539.02 T
(15.3) 505.12 539.02 T
(1350) 223.1 524.02 T
(36.64) 340.88 524.02 T
(0.34) 397.12 524.02 T
(97.03) 448.88 524.02 T
(14.7) 505.12 524.02 T
(1400) 223.1 509.02 T
(36.05) 340.88 509.02 T
(0.28) 397.12 509.02 T
(96.88) 448.88 509.02 T
(14.2) 505.12 509.02 T
(1450) 223.1 494.02 T
(35.35) 340.88 494.02 T
(0.28) 397.12 494.02 T
(105.46) 446.62 494.02 T
(13.7) 505.12 494.02 T
(1500) 223.1 479.02 T
(35.49) 340.88 479.02 T
(0.27) 397.12 479.02 T
(1) 446.79 479.02 T
(13.43) 450.96 479.02 T
(13.2) 505.12 479.02 T
(1550) 223.1 464.02 T
(0.000172) 283.02 464.02 T
(34.43) 340.88 464.02 T
(0.29) 397.12 464.02 T
(133.84) 446.62 464.02 T
(12.8) 505.12 464.02 T
(1600) 223.1 449.02 T
(0.00298) 285.27 449.02 T
(30.18) 340.88 449.02 T
(0.31) 397.12 449.02 T
(155.76) 446.62 449.02 T
(12.4) 505.12 449.02 T
(1650) 223.1 434.02 T
(0.0317) 287.52 434.02 T
(29.37) 340.88 434.02 T
(0.37) 397.12 434.02 T
(165.92) 446.62 434.02 T
(12.0) 505.12 434.02 T
(1700) 223.1 419.02 T
(0.0843) 287.52 419.02 T
(25.91) 340.88 419.02 T
(0.44) 397.12 419.02 T
(176.10) 446.62 419.02 T
(1) 505.29 419.02 T
(1.7) 509.46 419.02 T
(1750) 223.1 404.02 T
(0.0923) 287.52 404.02 T
(18.1) 341.04 404.02 T
(1) 356.46 404.02 T
(0.56) 397.12 404.02 T
(216.91) 446.62 404.02 T
(1) 505.29 404.02 T
(1.4) 509.46 404.02 T
(1800) 223.1 389.02 T
(0.0680) 287.52 389.02 T
(1) 341.04 389.02 T
(1.82) 345.21 389.02 T
(0.68) 397.12 389.02 T
(259.65) 446.62 389.02 T
(1) 505.29 389.02 T
(1.0) 509.46 389.02 T
(1850) 223.1 374.02 T
(0.0261) 287.52 374.02 T
(7.38) 343.12 374.02 T
(0.74) 397.12 374.02 T
(281.80) 446.62 374.02 T
(10.7) 505.12 374.02 T
(1900) 223.1 359.02 T
(0.0094) 287.52 359.02 T
(3.04) 343.12 359.02 T
(0.79) 397.12 359.02 T
(302.40) 446.62 359.02 T
(10.5) 505.12 359.02 T
(1950) 223.1 344.02 T
(0.0021) 287.52 344.02 T
(1.04) 343.12 344.02 T
(1.04) 397.12 344.02 T
(362.78) 446.62 344.02 T
(10.2) 505.12 344.02 T
(2000) 223.1 329.02 T
(0.55) 343.12 329.02 T
(1.04) 397.12 329.02 T
(363.32) 446.62 329.02 T
(9.93) 505.12 329.02 T
(2050) 223.1 314.02 T
(0.30) 343.12 314.02 T
(1.08) 397.12 314.02 T
(406.51) 446.62 314.02 T
(9.69) 505.12 314.02 T
(2100) 223.1 299.02 T
(0.16) 343.12 299.02 T
(1.13) 397.12 299.02 T
(449.71) 446.62 299.02 T
(9.46) 505.12 299.02 T
(2200) 223.1 284.02 T
(1.43) 397.12 284.02 T
(594.61) 446.62 284.02 T
(9.03) 505.12 284.02 T
(2300) 223.1 269.02 T
(1.55) 397.12 269.02 T
(663.74) 446.62 269.02 T
(8.64) 505.12 269.02 T
(2400) 223.1 254.02 T
(1.75) 397.12 254.02 T
(776.52) 446.62 254.02 T
(8.28) 505.12 254.02 T
(2500) 223.1 239.02 T
(1.87) 397.12 239.02 T
(847.76) 446.62 239.02 T
(7.95) 505.12 239.02 T
(2600) 223.1 224.02 T
(1.85) 397.12 224.02 T
(854.42) 446.62 224.02 T
(7.64) 505.12 224.02 T
(2700) 223.1 209.02 T
(1.83) 397.12 209.02 T
(866.65) 446.62 209.02 T
(7.36) 505.12 209.02 T
(2800) 223.1 194.02 T
(1.68) 397.12 194.02 T
(813.29) 446.62 194.02 T
(7.09) 505.12 194.02 T
(2900) 223.1 179.02 T
(1.50) 397.12 179.02 T
(754.81) 446.62 179.02 T
(6.85) 505.12 179.02 T
(3000) 223.1 164.02 T
(0.76) 397.12 164.02 T
(398.89) 446.62 164.02 T
(6.62) 505.12 164.02 T
(3100) 223.1 149.02 T
(0.58) 397.12 149.02 T
(309.31) 446.62 149.02 T
(6.41) 505.12 149.02 T
(3200) 223.1 134.02 T
(0.38) 397.12 134.02 T
(194.15) 446.62 134.02 T
(6.21) 505.12 134.02 T
(3300) 223.1 119.02 T
(0.21) 397.12 119.02 T
(1) 446.79 119.02 T
(16.67) 450.96 119.02 T
(6.02) 505.12 119.02 T
(3400) 223.1 104.02 T
(0.14) 397.12 104.02 T
(80.) 453.38 104.02 T
(5.84) 505.12 104.02 T
188.4 642.89 188.4 99.14 2 L
V
0.25 H
0 Z
N
275.8 643.14 275.8 98.89 2 L
V
N
324 626.14 324 98.89 2 L
V
N
378 626.14 378 98.89 2 L
V
N
432 626.14 432 98.89 2 L
V
N
486 643.14 486 98.89 2 L
V
N
540 642.89 540 99.14 2 L
V
N
188.27 643.02 540.12 643.02 2 L
V
N
275.68 626.02 486.12 626.02 2 L
V
N
188.27 609.02 540.12 609.02 2 L
V
0.5 H
N
188.27 594.02 540.12 594.02 2 L
V
0.25 H
N
188.27 579.02 540.12 579.02 2 L
V
N
188.27 564.02 540.12 564.02 2 L
V
N
188.27 549.02 540.12 549.02 2 L
V
N
188.27 534.02 540.12 534.02 2 L
V
N
188.27 519.02 540.12 519.02 2 L
V
N
188.27 504.02 540.12 504.02 2 L
V
N
188.27 489.02 540.12 489.02 2 L
V
N
188.27 474.02 540.12 474.02 2 L
V
N
188.27 459.02 540.12 459.02 2 L
V
N
188.27 444.02 540.12 444.02 2 L
V
N
188.27 429.02 540.12 429.02 2 L
V
N
188.27 414.02 540.12 414.02 2 L
V
N
188.27 399.02 540.12 399.02 2 L
V
N
188.27 384.02 540.12 384.02 2 L
V
N
188.27 369.02 540.12 369.02 2 L
V
N
188.27 354.02 540.12 354.02 2 L
V
N
188.27 339.02 540.12 339.02 2 L
V
N
188.27 324.02 540.12 324.02 2 L
V
N
188.27 309.02 540.12 309.02 2 L
V
N
188.27 294.02 540.12 294.02 2 L
V
N
188.27 279.02 540.12 279.02 2 L
V
N
188.27 264.02 540.12 264.02 2 L
V
N
188.27 249.02 540.12 249.02 2 L
V
N
188.27 234.02 540.12 234.02 2 L
V
N
188.27 219.02 540.12 219.02 2 L
V
N
188.27 204.02 540.12 204.02 2 L
V
N
188.27 189.02 540.12 189.02 2 L
V
N
188.27 174.02 540.12 174.02 2 L
V
N
188.27 159.02 540.12 159.02 2 L
V
N
188.27 144.02 540.12 144.02 2 L
V
N
188.27 129.02 540.12 129.02 2 L
V
N
188.27 114.02 540.12 114.02 2 L
V
N
188.27 99.02 540.12 99.02 2 L
V
N
FMENDPAGE
%%EndPage: "79" 13
%%Page: "80" 14
612 792 0 FMBEGINPAGE
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[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(T) 189 736.18 T
(arget Acquisition Reference Information) 193.83 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(80) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
(7.4.2) 157.76 679.35 T
(Geocoronal L) 189 679.35 T
(yman-) 253.09 679.35 T
9 F
(a) 282.54 679.35 T
0 F
( Background) 288.85 679.35 T
5 F
1.33 (The acquisition mirror sensitivity curves illustrated above show that the mirrors still) 189 655.35 P
0.28 (re\337ect well at the L) 189 643.35 P
0.28 (yman-) 267.34 643.35 P
9 F
0.28 (a) 292.89 643.35 P
5 F
0.28 ( line at 1216 \201. Note that L) 299.2 643.35 P
0.28 (y-) 410.62 643.35 P
9 F
0.28 (a) 418.95 643.35 P
5 F
0.28 ( is suppressed by mirror A1.) 425.26 643.35 P
0.98 (T) 189 631.35 P
0.98 (ests have shown that the count rate from geocoronal L) 194.41 631.35 P
0.98 (yman-) 419.53 631.35 P
9 F
0.98 (a) 445.08 631.35 P
5 F
0.98 ( can be as high as 12) 451.39 631.35 P
0.95 (counts per second per diode. If you wish to acquire a faint tar) 189 619.35 P
0.95 (get with the least L) 445.45 619.35 P
0.95 (y-) 525.36 619.35 P
9 F
0.95 (a) 533.69 619.35 P
5 F
0.92 (contamination, we suggest that you specify) 189 607.35 P
6 F
2.22 (DARK) 369.8 607.35 P
2.22 (TIME) 397.23 607.35 P
5 F
0.92 ( as a Special Requirement in) 421.23 607.35 P
(Phase II.) 189 595.35 T
FMENDPAGE
%%EndPage: "80" 14
%%Trailer
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%%PageOrder: Ascend
%%Pages: 14
%%DocumentFonts: Helvetica-Bold
%%+ Palatino-BoldItalic
%%+ Palatino-Italic
%%+ Helvetica
%%+ Helvetica-Oblique
%%+ Times-Roman
%%+ Courier
%%+ Times-Italic
%%+ Courier-Bold
%%+ Symbol
%%+ Helvetica-BoldOblique
%%+ Times-Bold
%%EOF
%!PS-Adobe-3.0
%%BoundingBox: (atend)
%%Pages: (atend)
%%PageOrder: (atend)
%%DocumentFonts: (atend)
%%Creator: Frame 4.0
%%DocumentData: Clean7Bit
%%EndComments
%%BeginProlog
%
% Frame ps_prolog 4.0, for use with Frame 4.0 products
% This ps_prolog file is Copyright (c) 1986-1993 Frame Technology
% Corporation. All rights reserved. This ps_prolog file may be
% freely copied and distributed in conjunction with documents created
% using FrameMaker, FrameBuilder and FrameViewer as long as this
% copyright notice is preserved.
%
% Frame products normally print colors as their true color on a color printer
% or as shades of gray, based on luminance, on a black-and white printer. The
% following flag, if set to True, forces all non-white colors to print as pure
% black. This has no effect on bitmap images.
/FMPrintAllColorsAsBlack false def
%
% Frame products can either set their own line screens or use a printer's
% default settings. Three flags below control this separately for no
% separations, spot separations and process separations. If a flag
% is true, then the default printer settings will not be changed. If it is
% false, Frame products will use their own settings from a table based on
% the printer's resolution.
/FMUseDefaultNoSeparationScreen true def
/FMUseDefaultSpotSeparationScreen true def
/FMUseDefaultProcessSeparationScreen false def
%
% For any given PostScript printer resolution, Frame products have two sets of
% screen angles and frequencies for printing process separations, which are
% recomended by Adobe. The following variable chooses the higher frequencies
% when set to true or the lower frequencies when set to false. This is only
% effective if the appropriate FMUseDefault...SeparationScreen flag is false.
/FMUseHighFrequencyScreens true def
%
% PostScript Level 2 printers contain an "Accurate Screens" feature which can
% improve process separation rendering at the expense of compute time. This
% flag is ignored by PostScript Level 1 printers.
/FMUseAcccurateScreens true def
%
% The following PostScript procedure defines the spot function that Frame
% products will use for process separations. You may un-comment-out one of
% the alternative functions below, or use your own.
%
% Dot function
/FMSpotFunction {abs exch abs 2 copy add 1 gt
{1 sub dup mul exch 1 sub dup mul add 1 sub }
{dup mul exch dup mul add 1 exch sub }ifelse } def
%
% Line function
% /FMSpotFunction { pop } def
%
% Elipse function
% /FMSpotFunction { dup 5 mul 8 div mul exch dup mul exch add
% sqrt 1 exch sub } def
%
%
/FMversion (4.0) def
/FMLevel1 /languagelevel where {pop languagelevel} {1} ifelse 2 lt def
/FMPColor
FMLevel1 {
false
/colorimage where {pop pop true} if
} {
true
} ifelse
def
/FrameDict 400 dict def
systemdict /errordict known not {/errordict 10 dict def
errordict /rangecheck {stop} put} if
% The readline in PS 23.0 doesn't recognize cr's as nl's on AppleTalk
FrameDict /tmprangecheck errordict /rangecheck get put
errordict /rangecheck {FrameDict /bug true put} put
FrameDict /bug false put
mark
% Some PS machines read past the CR, so keep the following 3 lines together!
currentfile 5 string readline
00
0000000000
cleartomark
errordict /rangecheck FrameDict /tmprangecheck get put
FrameDict /bug get {
/readline {
/gstring exch def
/gfile exch def
/gindex 0 def
{
gfile read pop
dup 10 eq {exit} if
dup 13 eq {exit} if
gstring exch gindex exch put
/gindex gindex 1 add def
} loop
pop
gstring 0 gindex getinterval true
} bind def
} if
/FMshowpage /showpage load def
/FMquit /quit load def
/FMFAILURE {
dup = flush
FMshowpage
/Helvetica findfont 12 scalefont setfont
72 200 moveto
show FMshowpage
FMquit
} def
/FMVERSION {
FMversion ne {
(Frame product version does not match ps_prolog!) FMFAILURE
} if
} def
/FMBADEPSF {
(PostScript Lang. Ref. Man., 2nd Ed., H.2.4 says EPS must not call X )
dup dup (X) search pop exch pop exch pop length
4 -1 roll
putinterval
FMFAILURE
} def
/FMLOCAL {
FrameDict begin
0 def
end
} def
/concatprocs
{
/proc2 exch cvlit def/proc1 exch cvlit def/newproc proc1 length proc2 length add array def
newproc 0 proc1 putinterval newproc proc1 length proc2 putinterval newproc cvx
}def
FrameDict begin
/FMnone 0 def
/FMcyan 1 def
/FMmagenta 2 def
/FMyellow 3 def
/FMblack 4 def
/FMcustom 5 def
/FrameNegative false def
/FrameSepIs FMnone def
/FrameSepBlack 0 def
/FrameSepYellow 0 def
/FrameSepMagenta 0 def
/FrameSepCyan 0 def
/FrameSepRed 1 def
/FrameSepGreen 1 def
/FrameSepBlue 1 def
/FrameCurGray 1 def
/FrameCurPat null def
/FrameCurColors [ 0 0 0 1 0 0 0 ] def
/FrameColorEpsilon .001 def
/eqepsilon {
sub dup 0 lt {neg} if
FrameColorEpsilon le
} bind def
/FrameCmpColorsCMYK {
2 copy 0 get exch 0 get eqepsilon {
2 copy 1 get exch 1 get eqepsilon {
2 copy 2 get exch 2 get eqepsilon {
3 get exch 3 get eqepsilon
} {pop pop false} ifelse
}{pop pop false} ifelse
} {pop pop false} ifelse
} bind def
/FrameCmpColorsRGB {
2 copy 4 get exch 0 get eqepsilon {
2 copy 5 get exch 1 get eqepsilon {
6 get exch 2 get eqepsilon
}{pop pop false} ifelse
} {pop pop false} ifelse
} bind def
/RGBtoCMYK {
1 exch sub
3 1 roll
1 exch sub
3 1 roll
1 exch sub
3 1 roll
3 copy
2 copy
le { pop } { exch pop } ifelse
2 copy
le { pop } { exch pop } ifelse
dup dup dup
6 1 roll
4 1 roll
7 1 roll
sub
6 1 roll
sub
5 1 roll
sub
4 1 roll
} bind def
/CMYKtoRGB {
dup dup 4 -1 roll add
5 1 roll 3 -1 roll add
4 1 roll add
1 exch sub dup 0 lt {pop 0} if 3 1 roll
1 exch sub dup 0 lt {pop 0} if exch
1 exch sub dup 0 lt {pop 0} if exch
} bind def
/FrameSepInit {
1.0 RealSetgray
} bind def
/FrameSetSepColor {
/FrameSepBlue exch def
/FrameSepGreen exch def
/FrameSepRed exch def
/FrameSepBlack exch def
/FrameSepYellow exch def
/FrameSepMagenta exch def
/FrameSepCyan exch def
/FrameSepIs FMcustom def
setCurrentScreen
} bind def
/FrameSetCyan {
/FrameSepBlue 1.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 1.0 def
/FrameSepIs FMcyan def
setCurrentScreen
} bind def

/FrameSetMagenta {
/FrameSepBlue 1.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 1.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMmagenta def
setCurrentScreen
} bind def

/FrameSetYellow {
/FrameSepBlue 0.0 def
/FrameSepGreen 1.0 def
/FrameSepRed 1.0 def
/FrameSepBlack 0.0 def
/FrameSepYellow 1.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMyellow def
setCurrentScreen
} bind def

/FrameSetBlack {
/FrameSepBlue 0.0 def
/FrameSepGreen 0.0 def
/FrameSepRed 0.0 def
/FrameSepBlack 1.0 def
/FrameSepYellow 0.0 def
/FrameSepMagenta 0.0 def
/FrameSepCyan 0.0 def
/FrameSepIs FMblack def
setCurrentScreen
} bind def

/FrameNoSep {
/FrameSepIs FMnone def
setCurrentScreen
} bind def
/FrameSetSepColors {
FrameDict begin
[ exch 1 add 1 roll ]
/FrameSepColors
exch def end
} bind def
/FrameColorInSepListCMYK {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsCMYK
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/FrameColorInSepListRGB {
FrameSepColors {
exch dup 3 -1 roll
FrameCmpColorsRGB
{ pop true exit } if
} forall
dup true ne {pop false} if
} bind def
/RealSetgray /setgray load def
/RealSetrgbcolor /setrgbcolor load def
/RealSethsbcolor /sethsbcolor load def
end
/setgray {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetgray }
{
FrameSepIs FMblack eq
{ RealSetgray }
{ FrameSepIs FMcustom eq
FrameSepRed 0 eq and
FrameSepGreen 0 eq and
FrameSepBlue 0 eq and {
RealSetgray
} {
1 RealSetgray pop
} ifelse
} ifelse
} ifelse
end
} bind def
/setrgbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetrgbcolor }
{
3 copy [ 4 1 roll ]
FrameColorInSepListRGB
{
FrameSepBlue eq exch
FrameSepGreen eq and exch
FrameSepRed eq and
{ 0 } { 1 } ifelse
}
{
FMPColor {
RealSetrgbcolor
currentcmykcolor
} {
RGBtoCMYK
} ifelse
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
RealSetgray
}
ifelse
end
} bind def
/sethsbcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSethsbcolor }
{
RealSethsbcolor
currentrgbcolor
setrgbcolor
}
ifelse
end
} bind def
FrameDict begin
/setcmykcolor where {
pop /RealSetcmykcolor /setcmykcolor load def
} {
/RealSetcmykcolor {
4 1 roll
3 { 3 index add 0 max 1 min 1 exch sub 3 1 roll} repeat
setrgbcolor pop
} bind def
} ifelse
userdict /setcmykcolor {
FrameDict begin
FrameSepIs FMnone eq
{ RealSetcmykcolor }
{
4 copy [ 5 1 roll ]
FrameColorInSepListCMYK
{
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
{ 0 } { 1 } ifelse
}
{
FrameSepIs FMblack eq
{1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
RealSetgray
}
ifelse
end
} bind put
FMLevel1 not {

/patProcDict 5 dict dup begin
<0f1e3c78f0e1c387> { 3 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<0f87c3e1f0783c1e> { 3 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
<8142241818244281> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-1 -1 moveto 9 9 lineto stroke } bind def
<03060c183060c081> { 1 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<8040201008040201> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
end def
/patDict 15 dict dup begin
/PatternType 1 def
/PaintType 2 def
/TilingType 3 def
/BBox [ 0 0 8 8 ] def
/XStep 8 def
/YStep 8 def
/PaintProc {
begin
patProcDict bstring known {
patProcDict bstring get exec
} {
8 8 true [1 0 0 -1 0 8] bstring imagemask
} ifelse
end
} bind def
end def
} if
/combineColor {
FrameSepIs FMnone eq
{
graymode FMLevel1 or not {

[/Pattern [/DeviceCMYK]] setcolorspace
FrameCurColors 0 4 getinterval aload pop FrameCurPat setcolor
} {
FrameCurColors 3 get 1.0 ge {
FrameCurGray RealSetgray
} {
FMPColor graymode and {
0 1 3 {
FrameCurColors exch get
1 FrameCurGray sub mul
} for
RealSetcmykcolor
} {
4 1 6 {
FrameCurColors exch get
graymode {
1 exch sub 1 FrameCurGray sub mul 1 exch sub
} {
1.0 lt {FrameCurGray} {1} ifelse
} ifelse
} for
RealSetrgbcolor
} ifelse
} ifelse
} ifelse
} {
FrameCurColors 0 4 getinterval aload
FrameColorInSepListCMYK {
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
FrameSepIs FMcustom eq and
{ FrameCurGray } { 1 } ifelse
} {
FrameSepIs FMblack eq
{FrameCurGray 1.0 exch sub mul 1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop FrameCurGray 1.0 exch sub mul 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
graymode FMLevel1 or not {

[/Pattern [/DeviceGray]] setcolorspace
FrameCurPat setcolor
} {
graymode not FMLevel1 and {

dup 1 lt {pop FrameCurGray} if
} if
RealSetgray
} ifelse
} ifelse
} bind def
/savematrix {
orgmatrix currentmatrix pop
} bind def
/restorematrix {
orgmatrix setmatrix
} bind def
/dmatrix matrix def
/dpi 72 0 dmatrix defaultmatrix dtransform
dup mul exch dup mul add sqrt def

/freq dpi dup 72 div round dup 0 eq {pop 1} if 8 mul div def
/sangle 1 0 dmatrix defaultmatrix dtransform exch atan def
/dpiranges [ 2540 2400 1693 1270 1200 635 600 0 ] def
/CMLowFreqs [ 100.402 94.8683 89.2289 100.402 94.8683 66.9349 63.2456 47.4342 ] def
/YLowFreqs [ 95.25 90.0 84.65 95.25 90.0 70.5556 66.6667 50.0 ] def
/KLowFreqs [ 89.8026 84.8528 79.8088 89.8026 84.8528 74.8355 70.7107 53.033 ] def
/CLowAngles [ 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 ] def
/MLowAngles [ 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 ] def
/YLowTDot [ true true false true true false false false ] def
/CMHighFreqs [ 133.87 126.491 133.843 108.503 102.523 100.402 94.8683 63.2456 ] def
/YHighFreqs [ 127.0 120.0 126.975 115.455 109.091 95.25 90.0 60.0 ] def
/KHighFreqs [ 119.737 113.137 119.713 128.289 121.218 89.8026 84.8528 63.6395 ] def
/CHighAngles [ 71.5651 71.5651 71.5651 70.0169 70.0169 71.5651 71.5651 71.5651 ] def
/MHighAngles [ 18.4349 18.4349 18.4349 19.9831 19.9831 18.4349 18.4349 18.4349 ] def
/YHighTDot [ false false true false false true true false ] def
/PatFreq [ 10.5833 10.0 9.4055 10.5833 10.0 10.5833 10.0 9.375 ] def
/screenIndex {
0 1 dpiranges length 1 sub { dup dpiranges exch get 1 sub dpi le {exit} {pop} ifelse } for
} bind def
/getCyanScreen {
FMUseHighFrequencyScreens { CHighAngles CMHighFreqs} {CLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getMagentaScreen {
FMUseHighFrequencyScreens { MHighAngles CMHighFreqs } {MLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getYellowScreen {
FMUseHighFrequencyScreens { YHighTDot YHighFreqs} { YLowTDot YLowFreqs } ifelse
screenIndex dup 3 1 roll get 3 1 roll get { 3 div
{2 { 1 add 2 div 3 mul dup floor sub 2 mul 1 sub exch} repeat
FMSpotFunction } } {/FMSpotFunction load } ifelse
0.0 exch
} bind def
/getBlackScreen {
FMUseHighFrequencyScreens { KHighFreqs } { KLowFreqs } ifelse
screenIndex get 45.0 /FMSpotFunction load
} bind def
/getSpotScreen {
getBlackScreen
} bind def
/getCompositeScreen {
getBlackScreen
} bind def
/FMSetScreen
FMLevel1 { /setscreen load
}{ {
8 dict begin
/HalftoneType 1 def
/SpotFunction exch def
/Angle exch def
/Frequency exch def
/AccurateScreens FMUseAcccurateScreens def
currentdict end sethalftone
} bind } ifelse
def
/setDefaultScreen {
FMPColor {
orgrxfer cvx orggxfer cvx orgbxfer cvx orgxfer cvx setcolortransfer
}
{
orgxfer cvx settransfer
} ifelse
orgfreq organgle orgproc cvx setscreen
} bind def
/setCurrentScreen {
FrameSepIs FMnone eq {
FMUseDefaultNoSeparationScreen {
setDefaultScreen
} {
getCompositeScreen FMSetScreen
} ifelse
} {
FrameSepIs FMcustom eq {
FMUseDefaultSpotSeparationScreen {
setDefaultScreen
} {
getSpotScreen FMSetScreen
} ifelse
} {
FMUseDefaultProcessSeparationScreen {
setDefaultScreen
} {
FrameSepIs FMcyan eq {
getCyanScreen FMSetScreen
} {
FrameSepIs FMmagenta eq {
getMagentaScreen FMSetScreen
} {
FrameSepIs FMyellow eq {
getYellowScreen FMSetScreen
} {
getBlackScreen FMSetScreen
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} bind def
end
/gstring FMLOCAL
/gfile FMLOCAL
/gindex FMLOCAL
/orgrxfer FMLOCAL
/orggxfer FMLOCAL
/orgbxfer FMLOCAL
/orgxfer FMLOCAL
/orgproc FMLOCAL
/orgrproc FMLOCAL
/orggproc FMLOCAL
/orgbproc FMLOCAL
/organgle FMLOCAL
/orgrangle FMLOCAL
/orggangle FMLOCAL
/orgbangle FMLOCAL
/orgfreq FMLOCAL
/orgrfreq FMLOCAL
/orggfreq FMLOCAL
/orgbfreq FMLOCAL
/yscale FMLOCAL
/xscale FMLOCAL
/edown FMLOCAL
/manualfeed FMLOCAL
/paperheight FMLOCAL
/paperwidth FMLOCAL
/FMDOCUMENT {
array /FMfonts exch def
/#copies exch def
FrameDict begin
0 ne /manualfeed exch def
/paperheight exch def
/paperwidth exch def
0 ne /FrameNegative exch def
0 ne /edown exch def
/yscale exch def
/xscale exch def
FMLevel1 {
manualfeed {setmanualfeed} if
/FMdicttop countdictstack 1 add def
/FMoptop count def
% setpapername
% manualfeed {true} {papersize} ifelse
% {manualpapersize} {false} ifelse
% {desperatepapersize} {false} ifelse
% { (Can't select requested paper size for Frame print job!) FMFAILURE } if
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
}
{{1 dict dup /PageSize [paperwidth paperheight]put setpagedevice}stopped
{ (Can't select requested paper size for Frame print job!) FMFAILURE } if
{1 dict dup /ManualFeed manualfeed put setpagedevice } stopped pop }
ifelse

FMPColor {
currentcolorscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def
cvlit /orgbproc exch def
/orgbangle exch def
/orgbfreq exch def
cvlit /orggproc exch def
/orggangle exch def
/orggfreq exch def
cvlit /orgrproc exch def
/orgrangle exch def
/orgrfreq exch def
currentcolortransfer
FrameNegative {
1 1 4 {
pop { 1 exch sub } concatprocs 4 1 roll
} for
4 copy
setcolortransfer
} if
cvlit /orgxfer exch def
cvlit /orgbxfer exch def
cvlit /orggxfer exch def
cvlit /orgrxfer exch def
} {
currentscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def

currenttransfer
FrameNegative {
{ 1 exch sub } concatprocs
dup settransfer
} if
cvlit /orgxfer exch def
} ifelse
end
} def
/pagesave FMLOCAL
/orgmatrix FMLOCAL
/landscape FMLOCAL
/pwid FMLOCAL
/FMBEGINPAGE {
FrameDict begin
/pagesave save def
3.86 setmiterlimit
/landscape exch 0 ne def
landscape {
90 rotate 0 exch dup /pwid exch def neg translate pop
}{
pop /pwid exch def
} ifelse
edown { [-1 0 0 1 pwid 0] concat } if
0 0 moveto paperwidth 0 lineto paperwidth paperheight lineto
0 paperheight lineto 0 0 lineto 1 setgray fill
xscale yscale scale
/orgmatrix matrix def
gsave
} def
/FMENDPAGE {
grestore
pagesave restore
end
showpage
} def
/FMFONTDEFINE {
FrameDict begin
findfont
ReEncode
1 index exch
definefont
FMfonts 3 1 roll
put
end
} def
/FMFILLS {
FrameDict begin dup
array /fillvals exch def
dict /patCache exch def
end
} def
/FMFILL {
FrameDict begin
fillvals 3 1 roll put
end
} def
/FMNORMALIZEGRAPHICS {
newpath
0.0 0.0 moveto
1 setlinewidth
0 setlinecap
0 0 0 sethsbcolor
0 setgray
} bind def
/fx FMLOCAL
/fy FMLOCAL
/fh FMLOCAL
/fw FMLOCAL
/llx FMLOCAL
/lly FMLOCAL
/urx FMLOCAL
/ury FMLOCAL
/FMBEGINEPSF {
end
/FMEPSF save def
/showpage {} def
% See Adobe's "PostScript Language Reference Manual, 2nd Edition", page 714.
% "...the following operators MUST NOT be used in an EPS file:" (emphasis ours)
/banddevice {(banddevice) FMBADEPSF} def
/clear {(clear) FMBADEPSF} def
/cleardictstack {(cleardictstack) FMBADEPSF} def
/copypage {(copypage) FMBADEPSF} def
/erasepage {(erasepage) FMBADEPSF} def
/exitserver {(exitserver) FMBADEPSF} def
/framedevice {(framedevice) FMBADEPSF} def
/grestoreall {(grestoreall) FMBADEPSF} def
/initclip {(initclip) FMBADEPSF} def
/initgraphics {(initgraphics) FMBADEPSF} def
/initmatrix {(initmatrix) FMBADEPSF} def
/quit {(quit) FMBADEPSF} def
/renderbands {(renderbands) FMBADEPSF} def
/setglobal {(setglobal) FMBADEPSF} def
/setpagedevice {(setpagedevice) FMBADEPSF} def
/setshared {(setshared) FMBADEPSF} def
/startjob {(startjob) FMBADEPSF} def
/lettertray {(lettertray) FMBADEPSF} def
/letter {(letter) FMBADEPSF} def
/lettersmall {(lettersmall) FMBADEPSF} def
/11x17tray {(11x17tray) FMBADEPSF} def
/11x17 {(11x17) FMBADEPSF} def
/ledgertray {(ledgertray) FMBADEPSF} def
/ledger {(ledger) FMBADEPSF} def
/legaltray {(legaltray) FMBADEPSF} def
/legal {(legal) FMBADEPSF} def
/statementtray {(statementtray) FMBADEPSF} def
/statement {(statement) FMBADEPSF} def
/executivetray {(executivetray) FMBADEPSF} def
/executive {(executive) FMBADEPSF} def
/a3tray {(a3tray) FMBADEPSF} def
/a3 {(a3) FMBADEPSF} def
/a4tray {(a4tray) FMBADEPSF} def
/a4 {(a4) FMBADEPSF} def
/a4small {(a4small) FMBADEPSF} def
/b4tray {(b4tray) FMBADEPSF} def
/b4 {(b4) FMBADEPSF} def
/b5tray {(b5tray) FMBADEPSF} def
/b5 {(b5) FMBADEPSF} def
FMNORMALIZEGRAPHICS
[/fy /fx /fh /fw /ury /urx /lly /llx] {exch def} forall
fx fw 2 div add fy fh 2 div add translate
rotate
fw 2 div neg fh 2 div neg translate
fw urx llx sub div fh ury lly sub div scale
llx neg lly neg translate
/FMdicttop countdictstack 1 add def
/FMoptop count def
} bind def
/FMENDEPSF {
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
FMEPSF restore
FrameDict begin
} bind def
FrameDict begin
/setmanualfeed {
%%BeginFeature *ManualFeed True
statusdict /manualfeed true put
%%EndFeature
} bind def
/max {2 copy lt {exch} if pop} bind def
/min {2 copy gt {exch} if pop} bind def
/inch {72 mul} def
/pagedimen {
paperheight sub abs 16 lt exch
paperwidth sub abs 16 lt and
{/papername exch def} {pop} ifelse
} bind def
/papersizedict FMLOCAL
/setpapername {
/papersizedict 14 dict def
papersizedict begin
/papername /unknown def
/Letter 8.5 inch 11.0 inch pagedimen
/LetterSmall 7.68 inch 10.16 inch pagedimen
/Tabloid 11.0 inch 17.0 inch pagedimen
/Ledger 17.0 inch 11.0 inch pagedimen
/Legal 8.5 inch 14.0 inch pagedimen
/Statement 5.5 inch 8.5 inch pagedimen
/Executive 7.5 inch 10.0 inch pagedimen
/A3 11.69 inch 16.5 inch pagedimen
/A4 8.26 inch 11.69 inch pagedimen
/A4Small 7.47 inch 10.85 inch pagedimen
/B4 10.125 inch 14.33 inch pagedimen
/B5 7.16 inch 10.125 inch pagedimen
end
} bind def
/papersize {
papersizedict begin
/Letter {lettertray letter} def
/LetterSmall {lettertray lettersmall} def
/Tabloid {11x17tray 11x17} def
/Ledger {ledgertray ledger} def
/Legal {legaltray legal} def
/Statement {statementtray statement} def
/Executive {executivetray executive} def
/A3 {a3tray a3} def
/A4 {a4tray a4} def
/A4Small {a4tray a4small} def
/B4 {b4tray b4} def
/B5 {b5tray b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
statusdict begin stopped end
} bind def
/manualpapersize {
papersizedict begin
/Letter {letter} def
/LetterSmall {lettersmall} def
/Tabloid {11x17} def
/Ledger {ledger} def
/Legal {legal} def
/Statement {statement} def
/Executive {executive} def
/A3 {a3} def
/A4 {a4} def
/A4Small {a4small} def
/B4 {b4} def
/B5 {b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
stopped
} bind def
/desperatepapersize {
statusdict /setpageparams known
{
paperwidth paperheight 0 1
statusdict begin
{setpageparams} stopped
end
} {true} ifelse
} bind def
/DiacriticEncoding [
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /space /exclam /quotedbl
/numbersign /dollar /percent /ampersand /quotesingle /parenleft
/parenright /asterisk /plus /comma /hyphen /period /slash /zero /one
/two /three /four /five /six /seven /eight /nine /colon /semicolon
/less /equal /greater /question /at /A /B /C /D /E /F /G /H /I /J /K
/L /M /N /O /P /Q /R /S /T /U /V /W /X /Y /Z /bracketleft /backslash
/bracketright /asciicircum /underscore /grave /a /b /c /d /e /f /g /h
/i /j /k /l /m /n /o /p /q /r /s /t /u /v /w /x /y /z /braceleft /bar
/braceright /asciitilde /.notdef /Adieresis /Aring /Ccedilla /Eacute
/Ntilde /Odieresis /Udieresis /aacute /agrave /acircumflex /adieresis
/atilde /aring /ccedilla /eacute /egrave /ecircumflex /edieresis
/iacute /igrave /icircumflex /idieresis /ntilde /oacute /ograve
/ocircumflex /odieresis /otilde /uacute /ugrave /ucircumflex
/udieresis /dagger /.notdef /cent /sterling /section /bullet
/paragraph /germandbls /registered /copyright /trademark /acute
/dieresis /.notdef /AE /Oslash /.notdef /.notdef /.notdef /.notdef
/yen /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/ordfeminine /ordmasculine /.notdef /ae /oslash /questiondown
/exclamdown /logicalnot /.notdef /florin /.notdef /.notdef
/guillemotleft /guillemotright /ellipsis /.notdef /Agrave /Atilde
/Otilde /OE /oe /endash /emdash /quotedblleft /quotedblright
/quoteleft /quoteright /.notdef /.notdef /ydieresis /Ydieresis
/fraction /currency /guilsinglleft /guilsinglright /fi /fl /daggerdbl
/periodcentered /quotesinglbase /quotedblbase /perthousand
/Acircumflex /Ecircumflex /Aacute /Edieresis /Egrave /Iacute
/Icircumflex /Idieresis /Igrave /Oacute /Ocircumflex /.notdef /Ograve
/Uacute /Ucircumflex /Ugrave /dotlessi /circumflex /tilde /macron
/breve /dotaccent /ring /cedilla /hungarumlaut /ogonek /caron
] def
/ReEncode {
dup
length
dict begin
{
1 index /FID ne
{def}
{pop pop} ifelse
} forall
0 eq {/Encoding DiacriticEncoding def} if
currentdict
end
} bind def
FMPColor

{
/BEGINBITMAPCOLOR {
BITMAPCOLOR} def
/BEGINBITMAPCOLORc {
BITMAPCOLORc} def
/BEGINBITMAPTRUECOLOR {
BITMAPTRUECOLOR } def
/BEGINBITMAPTRUECOLORc {
BITMAPTRUECOLORc } def
}

{
/BEGINBITMAPCOLOR {
BITMAPGRAY} def
/BEGINBITMAPCOLORc {
BITMAPGRAYc} def
/BEGINBITMAPTRUECOLOR {
BITMAPTRUEGRAY } def
/BEGINBITMAPTRUECOLORc {
BITMAPTRUEGRAYc } def
}
ifelse
/K {
FMPrintAllColorsAsBlack {
dup 1 eq 2 index 1 eq and 3 index 1 eq and not
{7 {pop} repeat 0 0 0 1 0 0 0} if
} if
FrameCurColors astore
pop combineColor
} bind def
/graymode true def
/bwidth FMLOCAL
/bpside FMLOCAL
/bstring FMLOCAL
/onbits FMLOCAL
/offbits FMLOCAL
/xindex FMLOCAL
/yindex FMLOCAL
/x FMLOCAL
/y FMLOCAL
/setPatternMode {
FMLevel1 {
/bwidth exch def
/bpside exch def
/bstring exch def
/onbits 0 def /offbits 0 def
freq sangle landscape {90 add} if
{/y exch def
/x exch def
/xindex x 1 add 2 div bpside mul cvi def
/yindex y 1 add 2 div bpside mul cvi def
bstring yindex bwidth mul xindex 8 idiv add get
1 7 xindex 8 mod sub bitshift and 0 ne FrameNegative {not} if
{/onbits onbits 1 add def 1}
{/offbits offbits 1 add def 0}
ifelse
}
setscreen
offbits offbits onbits add div FrameNegative {1.0 exch sub} if
/FrameCurGray exch def
} {
pop pop
dup patCache exch known {
patCache exch get
} {
dup
patDict /bstring 3 -1 roll put
patDict
9 PatFreq screenIndex get div dup matrix scale
makepattern
dup
patCache 4 -1 roll 3 -1 roll put
} ifelse
/FrameCurGray 0 def
/FrameCurPat exch def
} ifelse
/graymode false def
combineColor
} bind def
/setGrayScaleMode {
graymode not {
/graymode true def
FMLevel1 {
setCurrentScreen
} if
} if
/FrameCurGray exch def
combineColor
} bind def
/normalize {
transform round exch round exch itransform
} bind def
/dnormalize {
dtransform round exch round exch idtransform
} bind def
/lnormalize {
0 dtransform exch cvi 2 idiv 2 mul 1 add exch idtransform pop
} bind def
/H {
lnormalize setlinewidth
} bind def
/Z {
setlinecap
} bind def

/PFill {
graymode FMLevel1 or not {
gsave 1 setgray eofill grestore
} if
} bind def
/PStroke {
graymode FMLevel1 or not {
gsave 1 setgray stroke grestore
} if
stroke
} bind def
/fillvals FMLOCAL
/X {
fillvals exch get
dup type /stringtype eq
{8 1 setPatternMode}
{setGrayScaleMode}
ifelse
} bind def
/V {
PFill gsave eofill grestore
} bind def
/Vclip {
clip
} bind def
/Vstrk {
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/N {
PStroke
} bind def
/Nclip {
strokepath clip newpath
} bind def
/Nstrk {
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/M {newpath moveto} bind def
/E {lineto} bind def
/D {curveto} bind def
/O {closepath} bind def
/n FMLOCAL
/L {
/n exch def
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%%EndProlog
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( Properties of the First-Order Gratings) 164.02 397 T
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( 83) 508.1 364.33 T
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( Sensitivity Functions for the First-Order Gratings) 187.02 348.33 T
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( 85) 508.1 348.33 T
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( Properties of the Echelle Gratings) 164.02 331 T
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( 87) 505.32 331 T
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( W) 187.02 314.33 T
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( 87) 508.1 314.33 T
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( 89) 508.1 298.33 T
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( Echelle Blaze Function) 187.02 282.33 T
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( 91) 508.1 282.33 T
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( Standard Patterns for Substepping and Background Measurement) 164.02 265 T
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( 92) 525.54 265 T
3 F
(8.5) 144 247 T
( The Ef) 164.02 247 T
(fects of Reddening in the Ultraviolet) 202.49 247 T
4 F
( 93) 505.32 247 T
3 F
(8.6) 144 229 T
( Instrumental Properties) 164.02 229 T
4 F
( 94) 505.32 229 T
3 10 Q
(8.6.1) 162 212.33 T
( The Point Spread Function) 187.02 212.33 T
4 F
( 94) 508.1 212.33 T
3 F
(8.6.2) 162 196.33 T
( Detector Dark Count and the CENSOR Option) 187.02 196.33 T
4 F
( 95) 508.1 196.33 T
3 F
(8.6.3) 162 180.33 T
( Noise Rejection with FL) 187.02 180.33 T
(YLIM) 294.09 180.33 T
4 F
( 97) 508.1 180.33 T
3 F
(8.6.4) 162 164.33 T
( Count Rate Linearity) 187.02 164.33 T
4 F
( 98) 508.1 164.33 T
3 F
(8.6.5) 162 148.33 T
( Image Stability) 187.02 148.33 T
4 F
( 98) 508.1 148.33 T
3 F
(8.6.6) 162 132.33 T
( W) 187.02 132.33 T
(avelength Calibrations) 198.87 132.33 T
4 F
( 98) 508.1 132.33 T
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(AR on the GHRS) 315.46 678.02 T
5 10 Q
-0.21 (Prior to the Servicing Mission, it was believed that the COST) 207 654.35 P
-0.21 (AR mirrors would have lit-) 449.95 654.35 P
1.02 (tle ef) 207 642.35 P
1.02 (fect on the throughput of the GHRS. It was known that the magnesium \337uoride) 228.11 642.35 P
1.16 (coatings would severely attenuate light below 1) 207 630.35 P
1.16 (150 \201, but at longer wavelengths we) 404.12 630.35 P
0.62 (anticipated that the light lost from the extra two re\337ections would be compensated for) 207 618.35 P
(by the improved throughput of the restored Point Spread Function.) 207 606.35 T
0.5 (The actual situation is more complex, as shown below) 207 586.35 P
0.5 (. What is plotted is a mean rela-) 427.29 586.35 P
-0.11 (tion that was \336tted to observations of the same star that were made both before and after) 207 574.35 P
0.27 (the Servicing Mission. The most prominent feature is the dip at 2000 \201. The high ratio) 207 562.35 P
0.34 (at longer wavelengths is just due to the improved PSF) 207 550.35 P
0.34 (, but the peak near 1300 \201 is not) 425.05 550.35 P
(understood.) 207 538.35 T
0 F
0.44 (Figure 8-1.) 144 187.35 P
3 F
0.44 (The observed ratio of counts for) 201.44 187.35 P
6 F
0.39 (m) 348.01 187.35 P
3 F
0.44 ( Col, made before the Servic-) 353.77 187.35 P
(ing Mission \050in Cycle 2\051 and after the deployment of the COST) 144 175.35 T
(AR mirrors.) 418.37 175.35 T
72 87.98 558 686.02 C
126 203.02 558 520.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 87.98 558 686.02 C
0 0 612 792 C
270 35 25 549 744 287.83 402.63 192.08 164.68 FMBEGINEPSF
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3 lw lt0 2050 500 r 2050 3100 d 2050 557 r 2018 557 d 2050 670 r
2018 670 d 2050 783 r 2018 783 d 2050 896 r 2018 896 d 2050 1009 r
1986 1009 d 2050 1122 r 2018 1122 d 2050 1235 r 2018 1235 d 2050 1348 r
2018 1348 d 2050 1461 r 2018 1461 d 2050 1574 r 1986 1574 d 2050 1687 r
2018 1687 d 2050 1800 r 2018 1800 d 2050 1913 r 2018 1913 d 2050 2026 r
2018 2026 d 2050 2139 r 1986 2139 d 2050 2252 r 2018 2252 d 2050 2365 r
2018 2365 d 2050 2478 r 2018 2478 d 2050 2591 r 2018 2591 d 2050 2704 r
1986 2704 d 2050 2817 r 2018 2817 d 2050 2930 r 2018 2930 d 2050 3043 r
2018 3043 d 2098 941 r 2096 945 d 2090 951 d 2132 951 d 2090 999 r
2090 979 d 2108 977 d 2106 979 d 2104 985 d 2104 991 d 2106 997 d
2110 1001 d 2116 1003 d 2120 1003 d 2126 1001 d 2130 997 d 2132 991 d
2132 985 d 2130 979 d 2128 977 d 2124 975 d 2090 1027 r 2092 1021 d
2098 1017 d 2108 1015 d 2114 1015 d 2124 1017 d 2130 1021 d 2132 1027 d
2132 1031 d 2130 1037 d 2124 1041 d 2114 1043 d 2108 1043 d 2098 1041 d
2092 1037 d 2090 1031 d 2090 1027 d 2090 1067 r 2092 1061 d 2098 1057 d
2108 1055 d 2114 1055 d 2124 1057 d 2130 1061 d 2132 1067 d 2132 1071 d
2130 1077 d 2124 1081 d 2114 1083 d 2108 1083 d 2098 1081 d 2092 1077 d
2090 1071 d 2090 1067 d 2100 1502 r 2098 1502 d 2094 1504 d 2092 1506 d
2090 1510 d 2090 1518 d 2092 1522 d 2094 1524 d 2098 1526 d 2102 1526 d
2106 1524 d 2112 1520 d 2132 1500 d 2132 1528 d 2090 1552 r 2092 1546 d
2098 1542 d 2108 1540 d 2114 1540 d 2124 1542 d 2130 1546 d 2132 1552 d
2132 1556 d 2130 1562 d 2124 1566 d 2114 1568 d 2108 1568 d 2098 1566 d
2092 1562 d 2090 1556 d 2090 1552 d 2090 1592 r 2092 1586 d 2098 1582 d
2108 1580 d 2114 1580 d 2124 1582 d 2130 1586 d 2132 1592 d 2132 1596 d
2130 1602 d 2124 1606 d 2114 1608 d 2108 1608 d 2098 1606 d 2092 1602 d
2090 1596 d 2090 1592 d 2090 1632 r 2092 1626 d 2098 1622 d 2108 1620 d
2114 1620 d 2124 1622 d 2130 1626 d 2132 1632 d 2132 1636 d 2130 1642 d
2124 1646 d 2114 1648 d 2108 1648 d 2098 1646 d 2092 1642 d 2090 1636 d
2090 1632 d 2100 2067 r 2098 2067 d 2094 2069 d 2092 2071 d 2090 2075 d
2090 2083 d 2092 2087 d 2094 2089 d 2098 2091 d 2102 2091 d 2106 2089 d
2112 2085 d 2132 2065 d 2132 2093 d 2090 2129 r 2090 2109 d 2108 2107 d
2106 2109 d 2104 2115 d 2104 2121 d 2106 2127 d 2110 2131 d 2116 2133 d
2120 2133 d 2126 2131 d 2130 2127 d 2132 2121 d 2132 2115 d 2130 2109 d
2128 2107 d 2124 2105 d 2090 2157 r 2092 2151 d 2098 2147 d 2108 2145 d
2114 2145 d 2124 2147 d 2130 2151 d 2132 2157 d 2132 2161 d 2130 2167 d
2124 2171 d 2114 2173 d 2108 2173 d 2098 2171 d 2092 2167 d 2090 2161 d
2090 2157 d 2090 2197 r 2092 2191 d 2098 2187 d 2108 2185 d 2114 2185 d
2124 2187 d 2130 2191 d 2132 2197 d 2132 2201 d 2130 2207 d 2124 2211 d
2114 2213 d 2108 2213 d 2098 2211 d 2092 2207 d 2090 2201 d 2090 2197 d
2090 2634 r 2090 2656 d 2106 2644 d 2106 2650 d 2108 2654 d 2110 2656 d
2116 2658 d 2120 2658 d 2126 2656 d 2130 2652 d 2132 2646 d 2132 2640 d
2130 2634 d 2128 2632 d 2124 2630 d 2090 2682 r 2092 2676 d 2098 2672 d
2108 2670 d 2114 2670 d 2124 2672 d 2130 2676 d 2132 2682 d 2132 2686 d
2130 2692 d 2124 2696 d 2114 2698 d 2108 2698 d 2098 2696 d 2092 2692 d
2090 2686 d 2090 2682 d 2090 2722 r 2092 2716 d 2098 2712 d 2108 2710 d
2114 2710 d 2124 2712 d 2130 2716 d 2132 2722 d 2132 2726 d 2130 2732 d
2124 2736 d 2114 2738 d 2108 2738 d 2098 2736 d 2092 2732 d 2090 2726 d
2090 2722 d 2090 2762 r 2092 2756 d 2098 2752 d 2108 2750 d 2114 2750 d
2124 2752 d 2130 2756 d 2132 2762 d 2132 2766 d 2130 2772 d 2124 2776 d
2114 2778 d 2108 2778 d 2098 2776 d 2092 2772 d 2090 2766 d 2090 2762 d
150 500 r 150 3100 d 150 557 r 182 557 d 150 670 r 182 670 d
150 783 r 182 783 d 150 896 r 182 896 d 150 1009 r 214 1009 d
150 1122 r 182 1122 d 150 1235 r 182 1235 d 150 1348 r 182 1348 d
150 1461 r 182 1461 d 150 1574 r 214 1574 d 150 1687 r 182 1687 d
150 1800 r 182 1800 d 150 1913 r 182 1913 d 150 2026 r 182 2026 d
150 2139 r 214 2139 d 150 2252 r 182 2252 d 150 2365 r 182 2365 d
150 2478 r 182 2478 d 150 2591 r 182 2591 d 150 2704 r 214 2704 d
150 2817 r 182 2817 d 150 2930 r 182 2930 d 150 3043 r 182 3043 d
2050 500 r 150 500 d 2050 500 r 2050 564 d 1898 500 r 1898 532 d
1746 500 r 1746 532 d 1594 500 r 1594 532 d 1442 500 r 1442 532 d
1290 500 r 1290 564 d 1138 500 r 1138 532 d 986 500 r 986 532 d
834 500 r 834 532 d 682 500 r 682 532 d 530 500 r 530 564 d
378 500 r 378 532 d 226 500 r 226 532 d 2026 386 r 2028 380 d
2034 376 d 2044 374 d 2050 374 d 2060 376 d 2066 380 d 2068 386 d
2068 390 d 2066 396 d 2060 400 d 2050 402 d 2044 402 d 2034 400 d
2028 396 d 2026 390 d 2026 386 d 2064 418 r 2066 416 d 2068 418 d
2066 420 d 2064 418 d 2026 446 r 2028 440 d 2034 436 d 2044 434 d
2050 434 d 2060 436 d 2066 440 d 2068 446 d 2068 450 d 2066 456 d
2060 460 d 2050 462 d 2044 462 d 2034 460 d 2028 456 d 2026 450 d
2026 446 d 1266 386 r 1268 380 d 1274 376 d 1284 374 d 1290 374 d
1300 376 d 1306 380 d 1308 386 d 1308 390 d 1306 396 d 1300 400 d
1290 402 d 1284 402 d 1274 400 d 1268 396 d 1266 390 d 1266 386 d
1304 418 r 1306 416 d 1308 418 d 1306 420 d 1304 418 d 1266 458 r
1266 438 d 1284 436 d 1282 438 d 1280 444 d 1280 450 d 1282 456 d
1286 460 d 1292 462 d 1296 462 d 1302 460 d 1306 456 d 1308 450 d
1308 444 d 1306 438 d 1304 436 d 1300 434 d 514 380 r 512 384 d
506 390 d 548 390 d 544 418 r 546 416 d 548 418 d 546 420 d
544 418 d 506 446 r 508 440 d 514 436 d 524 434 d 530 434 d
540 436 d 546 440 d 548 446 d 548 450 d 546 456 d 540 460 d
530 462 d 524 462 d 514 460 d 508 456 d 506 450 d 506 446 d
2050 3100 r 150 3100 d 2050 3100 r 2050 3036 d 1898 3100 r 1898 3068 d
1746 3100 r 1746 3068 d 1594 3100 r 1594 3068 d 1442 3100 r 1442 3068 d
1290 3100 r 1290 3036 d 1138 3100 r 1138 3068 d 986 3100 r 986 3068 d
834 3100 r 834 3068 d 682 3100 r 682 3068 d 530 3100 r 530 3036 d
378 3100 r 378 3068 d 226 3100 r 226 3068 d 2227 1260 r 2269 1272 d
2227 1284 r 2269 1272 d 2227 1284 r 2269 1296 d 2227 1308 r 2269 1296 d
2227 1362 r 2269 1362 d 2236 1362 r 2230 1356 d 2227 1350 d 2227 1341 d
2230 1335 d 2236 1329 d 2245 1326 d 2251 1326 d 2260 1329 d 2266 1335 d
2269 1341 d 2269 1350 d 2266 1356 d 2260 1362 d 2227 1377 r 2269 1395 d
2227 1413 r 2269 1395 d 2245 1428 r 2245 1464 d 2239 1464 d 2233 1461 d
2230 1458 d 2227 1452 d 2227 1443 d 2230 1437 d 2236 1431 d 2245 1428 d
2251 1428 d 2260 1431 d 2266 1437 d 2269 1443 d 2269 1452 d 2266 1458 d
2260 1464 d 2206 1485 r 2269 1485 d 2245 1506 r 2245 1542 d 2239 1542 d
2233 1539 d 2230 1536 d 2227 1530 d 2227 1521 d 2230 1515 d 2236 1509 d
2245 1506 d 2251 1506 d 2260 1509 d 2266 1515 d 2269 1521 d 2269 1530 d
2266 1536 d 2260 1542 d 2227 1563 r 2269 1563 d 2239 1563 r 2230 1572 d
2227 1578 d 2227 1587 d 2230 1593 d 2239 1596 d 2269 1596 d 2227 1650 r
2275 1650 d 2284 1647 d 2287 1644 d 2290 1638 d 2290 1629 d 2287 1623 d
2236 1650 r 2230 1644 d 2227 1638 d 2227 1629 d 2230 1623 d 2236 1617 d
2245 1614 d 2251 1614 d 2260 1617 d 2266 1623 d 2269 1629 d 2269 1638 d
2266 1644 d 2260 1650 d 2206 1674 r 2257 1674 d 2266 1677 d 2269 1683 d
2269 1689 d 2227 1665 r 2227 1686 d 2206 1701 r 2269 1701 d 2239 1701 r
2230 1710 d 2227 1716 d 2227 1725 d 2230 1731 d 2239 1734 d 2269 1734 d
2194 1824 r 2200 1818 d 2209 1812 d 2221 1806 d 2236 1803 d 2248 1803 d
2263 1806 d 2275 1812 d 2284 1818 d 2290 1824 d 2206 1860 r 2269 1836 d
2206 1860 r 2269 1884 d 2248 1845 r 2248 1875 d 2227 1899 r 2269 1899 d
2239 1899 r 2230 1908 d 2227 1914 d 2227 1923 d 2230 1929 d 2239 1932 d
2269 1932 d 2227 1986 r 2275 1986 d 2284 1983 d 2287 1980 d 2290 1974 d
2290 1965 d 2287 1959 d 2236 1986 r 2230 1980 d 2227 1974 d 2227 1965 d
2230 1959 d 2236 1953 d 2245 1950 d 2251 1950 d 2260 1953 d 2266 1959 d
2269 1965 d 2269 1974 d 2266 1980 d 2260 1986 d 2236 2037 r 2230 2034 d
2227 2025 d 2227 2016 d 2230 2007 d 2236 2004 d 2242 2007 d 2245 2013 d
2248 2028 d 2251 2034 d 2257 2037 d 2260 2037 d 2266 2034 d 2269 2025 d
2269 2016 d 2266 2007 d 2260 2004 d 2206 2058 r 2257 2058 d 2266 2061 d
2269 2067 d 2269 2073 d 2227 2049 r 2227 2070 d 2227 2085 r 2269 2085 d
2245 2085 r 2236 2088 d 2230 2094 d 2227 2100 d 2227 2109 d 2227 2139 r
2230 2133 d 2236 2127 d 2245 2124 d 2251 2124 d 2260 2127 d 2266 2133 d
2269 2139 d 2269 2148 d 2266 2154 d 2260 2160 d 2251 2163 d 2245 2163 d
2236 2160 d 2230 2154 d 2227 2148 d 2227 2139 d 2227 2181 r 2269 2181 d
2239 2181 r 2230 2190 d 2227 2196 d 2227 2205 d 2230 2211 d 2239 2214 d
2269 2214 d 2239 2214 r 2230 2223 d 2227 2229 d 2227 2238 d 2230 2244 d
2239 2247 d 2269 2247 d 2236 2301 r 2230 2298 d 2227 2289 d 2227 2280 d
2230 2271 d 2236 2268 d 2242 2271 d 2245 2277 d 2248 2292 d 2251 2298 d
2257 2301 d 2260 2301 d 2266 2298 d 2269 2289 d 2269 2280 d 2266 2271 d
2260 2268 d 2194 2316 r 2200 2322 d 2209 2328 d 2221 2334 d 2236 2337 d
2248 2337 d 2263 2334 d 2275 2328 d 2284 2322 d 2290 2316 d 1496 125 r
1496 167 d 1496 143 r 1493 134 d 1487 128 d 1481 125 d 1472 125 d
1421 125 r 1421 167 d 1421 134 r 1427 128 d 1433 125 d 1442 125 d
1448 128 d 1454 134 d 1457 143 d 1457 149 d 1454 158 d 1448 164 d
1442 167 d 1433 167 d 1427 164 d 1421 158 d 1397 104 r 1397 155 d
1394 164 d 1388 167 d 1382 167 d 1406 125 r 1385 125 d 1373 104 r
1370 107 d 1367 104 d 1370 101 d 1373 104 d 1370 125 r 1370 167 d
1334 125 r 1340 128 d 1346 134 d 1349 143 d 1349 149 d 1346 158 d
1340 164 d 1334 167 d 1325 167 d 1319 164 d 1313 158 d 1310 149 d
1310 143 d 1313 134 d 1319 128 d 1325 125 d 1334 125 d 1232 125 r
1238 128 d 1244 134 d 1247 143 d 1247 149 d 1244 158 d 1238 164 d
1232 167 d 1223 167 d 1217 164 d 1211 158 d 1208 149 d 1208 143 d
1211 134 d 1217 128 d 1223 125 d 1232 125 d 1172 104 r 1178 104 d
1184 107 d 1187 116 d 1187 167 d 1196 125 r 1175 125 d 1082 134 r
1085 128 d 1094 125 d 1103 125 d 1112 128 d 1115 134 d 1112 140 d
1106 143 d 1091 146 d 1085 149 d 1082 155 d 1082 158 d 1085 164 d
1094 167 d 1103 167 d 1112 164 d 1115 158 d 1067 143 r 1031 143 d
1031 137 d 1034 131 d 1037 128 d 1043 125 d 1052 125 d 1058 128 d
1064 134 d 1067 143 d 1067 149 d 1064 158 d 1058 164 d 1052 167 d
1043 167 d 1037 164 d 1031 158 d 1010 125 r 1010 167 d 1010 137 r
1001 128 d 995 125 d 986 125 d 980 128 d 977 137 d 977 167 d
926 134 r 929 128 d 938 125 d 947 125 d 956 128 d 959 134 d
956 140 d 950 143 d 935 146 d 929 149 d 926 155 d 926 158 d
929 164 d 938 167 d 947 167 d 956 164 d 959 158 d 911 104 r
908 107 d 905 104 d 908 101 d 911 104 d 908 125 r 908 167 d
881 104 r 881 155 d 878 164 d 872 167 d 866 167 d 890 125 r
869 125 d 857 104 r 854 107 d 851 104 d 854 101 d 857 104 d
854 125 r 854 167 d 836 125 r 818 167 d 800 125 r 818 167 d
785 104 r 782 107 d 779 104 d 782 101 d 785 104 d 782 125 r
782 167 d 755 104 r 755 155 d 752 164 d 746 167 d 740 167 d
764 125 r 743 125 d 734 125 r 716 167 d 698 125 r 716 167 d
722 179 d 728 185 d 734 188 d 737 188 d 2037 557 r 1072 613 d
538 670 d 315 726 d 284 783 d 327 839 d 389 896 d 457 952 d
521 1009 d 569 1065 d 598 1122 d 614 1178 d 627 1235 d 647 1291 d
682 1348 d 725 1404 d 766 1461 d 791 1517 d 789 1574 d 758 1630 d
708 1687 d 650 1743 d 596 1800 d 554 1857 d 523 1913 d 500 1970 d
482 2026 d 465 2083 d 448 2139 d 431 2196 d 414 2252 d 396 2309 d
378 2365 d 359 2422 d 341 2478 d 323 2535 d 306 2591 d 290 2648 d
273 2704 d 255 2761 d 236 2817 d 219 2874 d 211 2930 d 223 2987 d
263 3043 d
e
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%%EndDocument
FMENDEPSF
FMENDPAGE
%%EndPage: "82" 2
%%Page: "83" 3
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (83) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Reference T) 207 736.18 T
(ables for Instrument Performance) 257.85 736.18 T
54 671.02 540 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 672.52 540 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 672.52 180 672.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(8.2) 163.32 678.02 T
(Properties of the First-Order Gratings) 189 678.02 T
0 10 Q
(8.2.1) 157.76 644.35 T
(Useful W) 189 644.35 T
(avelength Ranges) 231.41 644.35 T
5 F
0.32 (The following table summarizes the useful wavelength range for each of the \336rst-order) 189 624.35 P
0.28 (gratings of GHRS. More precise sensitivity values are enumerated below) 189 612.35 P
0.28 (. Note that lit-) 483.05 612.35 P
-0.24 (tle or no \337ux below 1) 189 600.35 P
-0.24 (150 \201 is re\337ected by the COST) 273.24 600.35 P
-0.24 (AR mirrors because of their magne-) 397.09 600.35 P
(sium \337uoride coatings.) 189 588.35 T
1.64 (The last three gratings are used with detector D2, which admits some second-order) 189 429.35 P
0.08 (light, hence the comments. For example, L) 189 417.35 P
0.08 (yman-) 360.3 417.35 P
6 F
0.08 (a) 385.85 417.35 P
5 F
0.08 ( light \0501216 \201\051 can appear at 2432 \201) 392.16 417.35 P
1.58 (in second order) 189 405.35 P
1.58 (. Except for this possibility of geocoronal contamination, many cool) 253.27 405.35 P
0.51 (stars have very little short-wavelength \337ux, so that the best resolution can be achieved) 189 393.35 P
1.48 (without undue extraneous light by observing in \336rst order near the high-wavelength) 189 381.35 P
(limit.) 189 369.35 T
1.08 (Note that the G270M grating has an order) 189 349.35 P
1.08 (-sorting \336lter which eliminates light below) 363.8 349.35 P
(about 1650 \201 so that no cross-order contamination occurs below 3300 \201.) 189 337.35 T
0 F
(8.2.2) 157.76 307.35 T
(Resolving Power) 189 307.35 T
5 F
1.25 (The following \336gures illustrate the resolving power as measured for each of GHRS\325) 189 287.35 P
0.38 (gratings. In this case the resolving power was computed as) 189 275.35 P
7 F
0.33 (R) 430.21 275.35 P
5 F
0.38 ( =) 436.21 275.35 P
6 F
0.38 ( l) 444.73 275.35 P
5 F
0.38 (/) 453.09 275.35 P
6 F
0.38 (Dl) 455.87 275.35 P
5 F
0.38 (, where) 467.48 275.35 P
0.38 ( is the) 515.36 275.35 P
1.05 (measured full-width-at-half-maximum \050FWHM\051 of lines from an exposure of a spec-) 189 263.35 P
-0.17 (trum calibration lamp. T) 189 251.35 P
-0.17 (ests have shown that the measured FWHM does not change sig-) 285.58 251.35 P
0.73 (ni\336cantly with wavelength \050for the \336rst-order gratings\051 or with) 189 239.35 P
8 F
0.73 (m) 448.56 239.35 P
6 F
0.73 (l) 455.78 239.35 P
5 F
0.73 (, the product of the) 461.27 239.35 P
0.45 (wavelength and order number \050for the echelle gratings\051. The nominal design speci\336ca-) 189 227.35 P
-0.15 (tion for the GHRS was) 189 215.35 P
7 F
-0.13 (R) 282.42 215.35 P
5 F
-0.15 ( = 20,000 for the \336rst-order gratings, but in fact one can exceed) 288.42 215.35 P
0.61 (a resolving power of 25,000 at virtually all wavelengths. Similarly) 189 203.35 P
0.61 (, the low-dispersion) 459.62 203.35 P
0.42 (grating G140L has R in excess of 2,000 over most of its useful wavelength range. The) 189 191.35 P
1.45 (true resolving powers for the echelle gratings are closer to 80,000 than the nominal) 189 179.35 P
(100,000.) 189 167.35 T
0.27 (By providing a sharper image of a point source, COST) 189 147.35 P
0.27 (AR restores the resolving power) 409.5 147.35 P
0.36 (achieved with the LSA to within about 20% of that possible with the SSA. There is no) 189 135.35 P
(ef) 189 123.35 T
(fective change for the SSA, however) 196.59 123.35 T
(.) 343.22 123.35 T
54 566.02 540 579.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 573.02 540 573.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 573.02 180 573.02 2 L
0 Z
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 560.02 T
(ABLE 8-1) 58.83 560.02 T
3 F
(Useful wavelength ranges for \336rst-order gratings.) 189 549.02 T
0 8 Q
(Grating) 115.12 525.68 T
(Useful Range \050\201\051) 172.05 525.68 T
(\201 per diode) 266.19 525.68 T
(Bandpass \050\201\051) 340.06 525.68 T
(Comment) 410.4 525.68 T
5 9 Q
(G140L) 115.12 511.02 T
(1) 185.25 511.02 T
(100 \320 1900) 189.41 511.02 T
(0.572 \320 0.573) 263.45 511.02 T
(286 \320 287) 347.84 511.02 T
(G140M) 115.12 496.02 T
(1) 185.25 496.02 T
(100 \320 1900) 189.41 496.02 T
(0.056 \320 0.052) 263.45 496.02 T
(28 \320 26) 352.34 496.02 T
(G160M) 115.12 481.02 T
(1) 185.25 481.02 T
(150 \320 2300) 189.41 481.02 T
(0.072 \320 0.066) 263.45 481.02 T
(36 \320 33) 352.34 481.02 T
(2nd order overlap above 2300 \201) 410.4 481.02 T
(G200M) 115.12 466.02 T
(1600 \320 2300) 185.08 466.02 T
(0.081 \320 0.075) 263.45 466.02 T
(41 \320 38) 352.34 466.02 T
(2nd order overlap above 2300 \201) 410.4 466.02 T
(G270M) 115.12 451.02 T
(2000 \320 3300) 185.08 451.02 T
(0.096 \320 0.087) 263.45 451.02 T
(48 \320 44) 352.34 451.02 T
(2nd order overlap above 3300 \201) 410.4 451.02 T
109.12 537.89 109.12 446.14 2 L
V
0.25 H
0 Z
N
166.05 538.14 166.05 445.89 2 L
V
N
249.11 538.14 249.11 445.89 2 L
V
N
327.29 538.14 327.29 445.89 2 L
V
N
404.4 538.14 404.4 445.89 2 L
V
N
540 537.89 540 446.14 2 L
V
N
109 538.02 540.12 538.02 2 L
V
N
109 521.02 540.12 521.02 2 L
V
0.5 H
N
109 506.02 540.12 506.02 2 L
V
0.25 H
N
109 491.02 540.12 491.02 2 L
V
N
109 476.02 540.12 476.02 2 L
V
N
109 461.02 540.12 461.02 2 L
V
N
109 446.02 540.12 446.02 2 L
V
N
500.16 270.85 515.36 283.85 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
6 10 Q
0 X
0 0 0 1 0 0 0 K
(D) 501.16 275.35 T
(l) 507.87 275.35 T
0 0 612 792 C
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7 FrameSetSepColors
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(84) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
1.27 (Figure 8-2.) 144 414.32 P
3 F
1.27 (Spectrum resolving power as a function of wavelength for the) 203.93 414.32 P
0.15 (GHRS medium-resolution \050holographic\051 gratings. From left to right the curves) 144 402.32 P
(are for G140M, G160M, G200M, and G270M, respectively) 144 390.32 T
(.) 400.59 390.32 T
0 F
(Figure 8-3.) 144 108.32 T
3 F
(Resolving power for grating G140L.) 200.13 108.32 T
72 85.97 558 684 C
72 429.98 558 677 C
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911 1166 d 910 1172 d 908 1175 d 904 1176 d 902 1176 d 959 1172 r
962 1173 d 965 1176 d 965 1151 d 981 1170 r 981 1172 d 982 1174 d
983 1175 d 986 1176 d 990 1176 d 993 1175 d 994 1174 d 995 1172 d
995 1169 d 994 1167 d 992 1163 d 980 1151 d 996 1151 d 1011 1176 r
1007 1175 d 1005 1172 d 1004 1166 d 1004 1162 d 1005 1156 d 1007 1152 d
1011 1151 d 1013 1151 d 1017 1152 d 1019 1156 d 1020 1162 d 1020 1166 d
1019 1172 d 1017 1175 d 1013 1176 d 1011 1176 d 1035 1176 r 1031 1175 d
1029 1172 d 1028 1166 d 1028 1162 d 1029 1156 d 1031 1152 d 1035 1151 d
1037 1151 d 1041 1152 d 1043 1156 d 1044 1162 d 1044 1166 d 1043 1172 d
1041 1175 d 1037 1176 d 1035 1176 d 1092 1172 r 1095 1173 d 1098 1176 d
1098 1151 d 1115 1176 r 1128 1176 d 1121 1167 d 1125 1167 d 1127 1166 d
1128 1164 d 1129 1161 d 1129 1158 d 1128 1155 d 1126 1152 d 1122 1151 d
1119 1151 d 1115 1152 d 1114 1154 d 1113 1156 d 1144 1176 r 1140 1175 d
1138 1172 d 1137 1166 d 1137 1162 d 1138 1156 d 1140 1152 d 1144 1151 d
1146 1151 d 1150 1152 d 1152 1156 d 1153 1162 d 1153 1166 d 1152 1172 d
1150 1175 d 1146 1176 d 1144 1176 d 1168 1176 r 1164 1175 d 1162 1172 d
1161 1166 d 1161 1162 d 1162 1156 d 1164 1152 d 1168 1151 d 1170 1151 d
1174 1152 d 1176 1156 d 1177 1162 d 1177 1166 d 1176 1172 d 1174 1175 d
1170 1176 d 1168 1176 d 1226 1172 r 1229 1173 d 1232 1176 d 1232 1151 d
1259 1176 r 1247 1160 d 1265 1160 d 1259 1176 r 1259 1151 d 1278 1176 r
1274 1175 d 1272 1172 d 1271 1166 d 1271 1162 d 1272 1156 d 1274 1152 d
1278 1151 d 1280 1151 d 1284 1152 d 1286 1156 d 1287 1162 d 1287 1166 d
1286 1172 d 1284 1175 d 1280 1176 d 1278 1176 d 1302 1176 r 1298 1175 d
1296 1172 d 1295 1166 d 1295 1162 d 1296 1156 d 1298 1152 d 1302 1151 d
1304 1151 d 1308 1152 d 1310 1156 d 1311 1162 d 1311 1166 d 1310 1172 d
1308 1175 d 1304 1176 d 1302 1176 d 1359 1172 r 1362 1173 d 1365 1176 d
1365 1151 d 1394 1176 r 1382 1176 d 1381 1166 d 1382 1167 d 1386 1168 d
1389 1168 d 1393 1167 d 1395 1164 d 1396 1161 d 1396 1158 d 1395 1155 d
1393 1152 d 1389 1151 d 1386 1151 d 1382 1152 d 1381 1154 d 1380 1156 d
1411 1176 r 1407 1175 d 1405 1172 d 1404 1166 d 1404 1162 d 1405 1156 d
1407 1152 d 1411 1151 d 1413 1151 d 1417 1152 d 1419 1156 d 1420 1162 d
1420 1166 d 1419 1172 d 1417 1175 d 1413 1176 d 1411 1176 d 1435 1176 r
1431 1175 d 1429 1172 d 1428 1166 d 1428 1162 d 1429 1156 d 1431 1152 d
1435 1151 d 1437 1151 d 1441 1152 d 1443 1156 d 1444 1162 d 1444 1166 d
1443 1172 d 1441 1175 d 1437 1176 d 1435 1176 d 1492 1172 r 1495 1173 d
1498 1176 d 1498 1151 d 1528 1173 r 1527 1175 d 1523 1176 d 1521 1176 d
1517 1175 d 1515 1172 d 1514 1166 d 1514 1160 d 1515 1155 d 1517 1152 d
1521 1151 d 1522 1151 d 1526 1152 d 1528 1155 d 1529 1158 d 1529 1160 d
1528 1163 d 1526 1166 d 1522 1167 d 1521 1167 d 1517 1166 d 1515 1163 d
1514 1160 d 1544 1176 r 1540 1175 d 1538 1172 d 1537 1166 d 1537 1162 d
1538 1156 d 1540 1152 d 1544 1151 d 1546 1151 d 1550 1152 d 1552 1156 d
1553 1162 d 1553 1166 d 1552 1172 d 1550 1175 d 1546 1176 d 1544 1176 d
1568 1176 r 1564 1175 d 1562 1172 d 1561 1166 d 1561 1162 d 1562 1156 d
1564 1152 d 1568 1151 d 1570 1151 d 1574 1152 d 1576 1156 d 1577 1162 d
1577 1166 d 1576 1172 d 1574 1175 d 1570 1176 d 1568 1176 d 1626 1172 r
1629 1173 d 1632 1176 d 1632 1151 d 1663 1176 r 1651 1151 d 1647 1176 r
1663 1176 d 1678 1176 r 1674 1175 d 1672 1172 d 1671 1166 d 1671 1162 d
1672 1156 d 1674 1152 d 1678 1151 d 1680 1151 d 1684 1152 d 1686 1156 d
1687 1162 d 1687 1166 d 1686 1172 d 1684 1175 d 1680 1176 d 1678 1176 d
1702 1176 r 1698 1175 d 1696 1172 d 1695 1166 d 1695 1162 d 1696 1156 d
1698 1152 d 1702 1151 d 1704 1151 d 1708 1152 d 1710 1156 d 1711 1162 d
1711 1166 d 1710 1172 d 1708 1175 d 1704 1176 d 1702 1176 d 1759 1172 r
1762 1173 d 1765 1176 d 1765 1151 d 1786 1176 r 1782 1175 d 1781 1173 d
1781 1170 d 1782 1168 d 1784 1167 d 1789 1166 d 1793 1164 d 1795 1162 d
1796 1160 d 1796 1156 d 1795 1154 d 1794 1152 d 1790 1151 d 1786 1151 d
1782 1152 d 1781 1154 d 1780 1156 d 1780 1160 d 1781 1162 d 1783 1164 d
1787 1166 d 1792 1167 d 1794 1168 d 1795 1170 d 1795 1173 d 1794 1175 d
1790 1176 d 1786 1176 d 1811 1176 r 1807 1175 d 1805 1172 d 1804 1166 d
1804 1162 d 1805 1156 d 1807 1152 d 1811 1151 d 1813 1151 d 1817 1152 d
1819 1156 d 1820 1162 d 1820 1166 d 1819 1172 d 1817 1175 d 1813 1176 d
1811 1176 d 1835 1176 r 1831 1175 d 1829 1172 d 1828 1166 d 1828 1162 d
1829 1156 d 1831 1152 d 1835 1151 d 1837 1151 d 1841 1152 d 1843 1156 d
1844 1162 d 1844 1166 d 1843 1172 d 1841 1175 d 1837 1176 d 1835 1176 d
1892 1172 r 1895 1173 d 1898 1176 d 1898 1151 d 1928 1168 r 1927 1164 d
1925 1162 d 1921 1161 d 1920 1161 d 1916 1162 d 1914 1164 d 1913 1168 d
1913 1169 d 1914 1173 d 1916 1175 d 1920 1176 d 1921 1176 d 1925 1175 d
1927 1173 d 1928 1168 d 1928 1162 d 1927 1156 d 1925 1152 d 1921 1151 d
1919 1151 d 1915 1152 d 1914 1155 d 1944 1176 r 1940 1175 d 1938 1172 d
1937 1166 d 1937 1162 d 1938 1156 d 1940 1152 d 1944 1151 d 1946 1151 d
1950 1152 d 1952 1156 d 1953 1162 d 1953 1166 d 1952 1172 d 1950 1175 d
1946 1176 d 1944 1176 d 1968 1176 r 1964 1175 d 1962 1172 d 1961 1166 d
1961 1162 d 1962 1156 d 1964 1152 d 1968 1151 d 1970 1151 d 1974 1152 d
1976 1156 d 1977 1162 d 1977 1166 d 1976 1172 d 1974 1175 d 1970 1176 d
1968 1176 d 800 1700 r 2000 1700 d 800 1700 r 800 1681 d 867 1700 r
867 1662 d 933 1700 r 933 1681 d 1000 1700 r 1000 1662 d 1067 1700 r
1067 1681 d 1133 1700 r 1133 1662 d 1200 1700 r 1200 1681 d 1267 1700 r
1267 1662 d 1333 1700 r 1333 1681 d 1400 1700 r 1400 1662 d 1467 1700 r
1467 1681 d 1533 1700 r 1533 1662 d 1600 1700 r 1600 1681 d 1667 1700 r
1667 1662 d 1733 1700 r 1733 1681 d 1800 1700 r 1800 1662 d 1867 1700 r
1867 1681 d 1933 1700 r 1933 1662 d 2000 1700 r 2000 1681 d 800 1200 r
800 1700 d 800 1200 r 819 1200 d 800 1228 r 838 1228 d 800 1256 r
819 1256 d 800 1283 r 819 1283 d 800 1311 r 819 1311 d 800 1339 r
819 1339 d 800 1367 r 838 1367 d 800 1394 r 819 1394 d 800 1422 r
819 1422 d 800 1450 r 819 1450 d 800 1478 r 819 1478 d 800 1506 r
838 1506 d 800 1533 r 819 1533 d 800 1561 r 819 1561 d 800 1589 r
819 1589 d 800 1617 r 819 1617 d 800 1644 r 838 1644 d 800 1672 r
819 1672 d 800 1700 r 819 1700 d 692 1238 r 695 1239 d 698 1242 d
698 1217 d 727 1242 r 715 1242 d 714 1232 d 715 1233 d 719 1234 d
722 1234 d 726 1233 d 728 1230 d 729 1227 d 729 1224 d 728 1221 d
726 1218 d 722 1217 d 719 1217 d 715 1218 d 714 1220 d 713 1222 d
744 1242 r 740 1241 d 738 1238 d 737 1232 d 737 1228 d 738 1222 d
740 1218 d 744 1217 d 746 1217 d 750 1218 d 752 1222 d 753 1228 d
753 1232 d 752 1238 d 750 1241 d 746 1242 d 744 1242 d 768 1242 r
764 1241 d 762 1238 d 761 1232 d 761 1228 d 762 1222 d 764 1218 d
768 1217 d 770 1217 d 774 1218 d 776 1222 d 777 1228 d 777 1232 d
776 1238 d 774 1241 d 770 1242 d 768 1242 d 690 1375 r 690 1377 d
691 1379 d 692 1380 d 695 1381 d 699 1381 d 702 1380 d 703 1379 d
704 1377 d 704 1374 d 703 1372 d 701 1368 d 689 1356 d 705 1356 d
720 1381 r 716 1380 d 714 1377 d 713 1371 d 713 1367 d 714 1361 d
716 1357 d 720 1356 d 722 1356 d 726 1357 d 728 1361 d 729 1367 d
729 1371 d 728 1377 d 726 1380 d 722 1381 d 720 1381 d 744 1381 r
740 1380 d 738 1377 d 737 1371 d 737 1367 d 738 1361 d 740 1357 d
744 1356 d 746 1356 d 750 1357 d 752 1361 d 753 1367 d 753 1371 d
752 1377 d 750 1380 d 746 1381 d 744 1381 d 768 1381 r 764 1380 d
762 1377 d 761 1371 d 761 1367 d 762 1361 d 764 1357 d 768 1356 d
770 1356 d 774 1357 d 776 1361 d 777 1367 d 777 1371 d 776 1377 d
774 1380 d 770 1381 d 768 1381 d 690 1514 r 690 1516 d 691 1518 d
692 1519 d 695 1520 d 699 1520 d 702 1519 d 703 1518 d 704 1516 d
704 1513 d 703 1511 d 701 1507 d 689 1495 d 705 1495 d 727 1520 r
715 1520 d 714 1510 d 715 1511 d 719 1512 d 722 1512 d 726 1511 d
728 1508 d 729 1505 d 729 1502 d 728 1499 d 726 1496 d 722 1495 d
719 1495 d 715 1496 d 714 1498 d 713 1500 d 744 1520 r 740 1519 d
738 1516 d 737 1510 d 737 1506 d 738 1500 d 740 1496 d 744 1495 d
746 1495 d 750 1496 d 752 1500 d 753 1506 d 753 1510 d 752 1516 d
750 1519 d 746 1520 d 744 1520 d 768 1520 r 764 1519 d 762 1516 d
761 1510 d 761 1506 d 762 1500 d 764 1496 d 768 1495 d 770 1495 d
774 1496 d 776 1500 d 777 1506 d 777 1510 d 776 1516 d 774 1519 d
770 1520 d 768 1520 d 691 1658 r 704 1658 d 697 1649 d 701 1649 d
703 1648 d 704 1646 d 705 1643 d 705 1640 d 704 1637 d 702 1634 d
698 1633 d 695 1633 d 691 1634 d 690 1636 d 689 1638 d 720 1658 r
716 1657 d 714 1654 d 713 1648 d 713 1644 d 714 1638 d 716 1634 d
720 1633 d 722 1633 d 726 1634 d 728 1638 d 729 1644 d 729 1648 d
728 1654 d 726 1657 d 722 1658 d 720 1658 d 744 1658 r 740 1657 d
738 1654 d 737 1648 d 737 1644 d 738 1638 d 740 1634 d 744 1633 d
746 1633 d 750 1634 d 752 1638 d 753 1644 d 753 1648 d 752 1654 d
750 1657 d 746 1658 d 744 1658 d 768 1658 r 764 1657 d 762 1654 d
761 1648 d 761 1644 d 762 1638 d 764 1634 d 768 1633 d 770 1633 d
774 1634 d 776 1638 d 777 1644 d 777 1648 d 776 1654 d 774 1657 d
770 1658 d 768 1658 d 2000 1200 r 2000 1700 d 2000 1200 r 1981 1200 d
2000 1228 r 1962 1228 d 2000 1256 r 1981 1256 d 2000 1283 r 1981 1283 d
2000 1311 r 1981 1311 d 2000 1339 r 1981 1339 d 2000 1367 r 1962 1367 d
2000 1394 r 1981 1394 d 2000 1422 r 1981 1422 d 2000 1450 r 1981 1450 d
2000 1478 r 1981 1478 d 2000 1506 r 1962 1506 d 2000 1533 r 1981 1533 d
2000 1561 r 1981 1561 d 2000 1589 r 1981 1589 d 2000 1617 r 1981 1617 d
2000 1644 r 1962 1644 d 2000 1672 r 1981 1672 d 2000 1700 r 1981 1700 d
1109 1117 r 1117 1084 d 1125 1117 r 1117 1084 d 1125 1117 r 1133 1084 d
1141 1117 r 1133 1084 d 1168 1106 r 1168 1084 d 1168 1101 r 1165 1104 d
1162 1106 d 1157 1106 d 1154 1104 d 1151 1101 d 1149 1096 d 1149 1093 d
1151 1088 d 1154 1085 d 1157 1084 d 1162 1084 d 1165 1085 d 1168 1088 d
1176 1106 r 1186 1084 d 1196 1106 r 1186 1084 d 1204 1096 r 1223 1096 d
1223 1100 d 1221 1103 d 1220 1104 d 1216 1106 d 1212 1106 d 1208 1104 d
1205 1101 d 1204 1096 d 1204 1093 d 1205 1088 d 1208 1085 d 1212 1084 d
1216 1084 d 1220 1085 d 1223 1088 d 1234 1117 r 1234 1084 d 1245 1096 r
1264 1096 d 1264 1100 d 1263 1103 d 1261 1104 d 1258 1106 d 1253 1106 d
1250 1104 d 1247 1101 d 1245 1096 d 1245 1093 d 1247 1088 d 1250 1085 d
1253 1084 d 1258 1084 d 1261 1085 d 1264 1088 d 1276 1106 r 1276 1084 d
1276 1100 r 1280 1104 d 1284 1106 d 1288 1106 d 1292 1104 d 1293 1100 d
1293 1084 d 1322 1106 r 1322 1080 d 1320 1076 d 1319 1074 d 1316 1072 d
1311 1072 d 1308 1074 d 1322 1101 r 1319 1104 d 1316 1106 d 1311 1106 d
1308 1104 d 1304 1101 d 1303 1096 d 1303 1093 d 1304 1088 d 1308 1085 d
1311 1084 d 1316 1084 d 1319 1085 d 1322 1088 d 1335 1117 r 1335 1090 d
1336 1085 d 1340 1084 d 1343 1084 d 1330 1106 r 1341 1106 d 1349 1117 r
1349 1084 d 1349 1100 r 1354 1104 d 1357 1106 d 1362 1106 d 1365 1104 d
1367 1100 d 1367 1084 d 1415 1124 r 1412 1120 d 1408 1116 d 1405 1109 d
1404 1101 d 1404 1095 d 1405 1087 d 1408 1080 d 1412 1076 d 1415 1072 d
1434 1117 r 1421 1084 d 1434 1117 r 1447 1084 d 1426 1095 r 1442 1095 d
1455 1106 r 1455 1084 d 1455 1100 r 1460 1104 d 1463 1106 d 1468 1106 d
1471 1104 d 1472 1100 d 1472 1084 d 1501 1106 r 1501 1080 d 1500 1076 d
1498 1074 d 1495 1072 d 1490 1072 d 1487 1074 d 1501 1101 r 1498 1104 d
1495 1106 d 1490 1106 d 1487 1104 d 1484 1101 d 1482 1096 d 1482 1093 d
1484 1088 d 1487 1085 d 1490 1084 d 1495 1084 d 1498 1085 d 1501 1088 d
1528 1101 r 1527 1104 d 1522 1106 d 1517 1106 d 1512 1104 d 1511 1101 d
1512 1098 d 1516 1096 d 1524 1095 d 1527 1093 d 1528 1090 d 1528 1088 d
1527 1085 d 1522 1084 d 1517 1084 d 1512 1085 d 1511 1088 d 1540 1117 r
1540 1090 d 1541 1085 d 1544 1084 d 1548 1084 d 1535 1106 r 1546 1106 d
1554 1106 r 1554 1084 d 1554 1096 r 1556 1101 d 1559 1104 d 1562 1106 d
1567 1106 d 1583 1106 r 1580 1104 d 1576 1101 d 1575 1096 d 1575 1093 d
1576 1088 d 1580 1085 d 1583 1084 d 1588 1084 d 1591 1085 d 1594 1088 d
1596 1093 d 1596 1096 d 1594 1101 d 1591 1104 d 1588 1106 d 1583 1106 d
1605 1106 r 1605 1084 d 1605 1100 r 1610 1104 d 1613 1106 d 1618 1106 d
1621 1104 d 1623 1100 d 1623 1084 d 1623 1100 r 1628 1104 d 1631 1106 d
1636 1106 d 1639 1104 d 1640 1100 d 1640 1084 d 1669 1101 r 1668 1104 d
1663 1106 d 1658 1106 d 1653 1104 d 1652 1101 d 1653 1098 d 1656 1096 d
1664 1095 d 1668 1093 d 1669 1090 d 1669 1088 d 1668 1085 d 1663 1084 d
1658 1084 d 1653 1085 d 1652 1088 d 1677 1124 r 1680 1120 d 1684 1116 d
1687 1109 d 1688 1101 d 1688 1095 d 1687 1087 d 1684 1080 d 1680 1076 d
1677 1072 d 589 1254 r 622 1254 d 589 1254 r 589 1269 d 590 1274 d
592 1275 d 595 1277 d 598 1277 d 602 1275 d 603 1274 d 605 1269 d
605 1254 d 605 1266 r 622 1277 d 610 1288 r 610 1307 d 606 1307 d
603 1306 d 602 1304 d 600 1301 d 600 1296 d 602 1293 d 605 1290 d
610 1288 d 613 1288 d 618 1290 d 621 1293 d 622 1296 d 622 1301 d
621 1304 d 618 1307 d 605 1334 r 602 1333 d 600 1328 d 600 1323 d
602 1318 d 605 1317 d 608 1318 d 610 1322 d 611 1330 d 613 1333 d
616 1334 d 618 1334 d 621 1333 d 622 1328 d 622 1323 d 621 1318 d
618 1317 d 600 1350 r 602 1347 d 605 1344 d 610 1342 d 613 1342 d
618 1344 d 621 1347 d 622 1350 d 622 1355 d 621 1358 d 618 1362 d
613 1363 d 610 1363 d 605 1362 d 602 1358 d 600 1355 d 600 1350 d
589 1373 r 622 1373 d 600 1382 r 622 1392 d 600 1402 r 622 1392 d
589 1410 r 590 1411 d 589 1413 d 587 1411 d 589 1410 d 600 1411 r
622 1411 d 600 1424 r 622 1424 d 606 1424 r 602 1429 d 600 1432 d
600 1437 d 602 1440 d 606 1442 d 622 1442 d 600 1470 r 626 1470 d
630 1469 d 632 1467 d 634 1464 d 634 1459 d 632 1456 d 605 1470 r
602 1467 d 600 1464 d 600 1459 d 602 1456 d 605 1453 d 610 1451 d
613 1451 d 618 1453 d 621 1456 d 622 1459 d 622 1464 d 621 1467 d
618 1470 d 589 1507 r 622 1507 d 589 1507 r 589 1522 d 590 1526 d
592 1528 d 595 1530 d 600 1530 d 603 1528 d 605 1526 d 606 1522 d
606 1507 d 600 1549 r 602 1546 d 605 1542 d 610 1541 d 613 1541 d
618 1542 d 621 1546 d 622 1549 d 622 1554 d 621 1557 d 618 1560 d
613 1562 d 610 1562 d 605 1560 d 602 1557 d 600 1554 d 600 1549 d
600 1570 r 622 1576 d 600 1582 r 622 1576 d 600 1582 r 622 1589 d
600 1595 r 622 1589 d 610 1605 r 610 1624 d 606 1624 d 603 1622 d
602 1621 d 600 1618 d 600 1613 d 602 1610 d 605 1606 d 610 1605 d
613 1605 d 618 1606 d 621 1610 d 622 1613 d 622 1618 d 621 1621 d
618 1624 d 600 1635 r 622 1635 d 610 1635 r 605 1637 d 602 1640 d
600 1643 d 600 1648 d 867 1283 r 933 1303 d 1067 1346 d 1200 1388 d
1333 1431 d 1467 1475 d 1600 1518 d 1733 1562 d 1867 1604 d 1973 1632 d
e
%%Trailer
EndPSPlot

%%EndDocument
FMENDEPSF
72 85.97 558 684 C
0 0 612 792 C
FMENDPAGE
%%EndPage: "84" 4
%%Page: "85" 5
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (85) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Reference T) 207 736.18 T
(ables for Instrument Performance) 257.85 736.18 T
0 10 Q
(8.2.3) 157.76 679.35 T
(Sensitivity Functions for the First-Order Gratings) 189 679.35 T
5 F
0.27 (Below are given sensitivities for the \336rst-order gratings, using the Lar) 189 659.35 P
0.27 (ge Science Aper-) 470.61 659.35 P
0.43 (ture, in units of) 189 647.35 P
0.43 (. These) 510.69 647.35 P
0.83 (values will be updated with precise numbers determined in Cycle 4 but what is listed) 189 635.35 P
-0.11 (here has been adjusted for the known ef) 189 623.35 P
-0.11 (fects of the COST) 347.14 623.35 P
-0.11 (AR mirrors. SSA sensitivity is) 418.49 623.35 P
(about 50 to 70% of these values, with the lar) 189 611.35 T
(ger value applying at longer wavelengths.) 367.13 611.35 T
54 589.02 540 602.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 596.02 540 596.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 596.02 180 596.02 2 L
0 Z
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 583.02 T
(ABLE 8-2) 58.83 583.02 T
3 F
(Sensitivities for \336rst-order gratings.) 189 572.02 T
0 8 Q
(Grating) 277.48 548.68 T
(W) 200.4 531.68 T
(avelength \050\201\051) 207.66 531.68 T
(G140L) 277.48 531.68 T
(G140M) 331.48 531.68 T
(G160M) 385.48 531.68 T
(G200M) 439.48 531.68 T
(G270M) 493.48 531.68 T
5 9 Q
(1) 224.1 517.02 T
(100) 228.27 517.02 T
(0.20) 303.73 517.02 T
(0.006) 331.48 517.02 T
(1) 224.1 502.02 T
(150) 228.27 502.02 T
(20.9) 303.73 502.02 T
(0.75) 331.48 502.02 T
(0.64) 411.73 502.02 T
(1200) 223.94 487.02 T
(82.3) 303.73 487.02 T
(2.27) 331.48 487.02 T
(2.87) 411.73 487.02 T
(1250) 223.94 472.02 T
(152.) 303.73 472.02 T
(4.95) 331.48 472.02 T
(5.77) 411.73 472.02 T
(1300) 223.94 457.02 T
(168.) 303.73 457.02 T
(7.13) 331.48 457.02 T
(7.96) 411.73 457.02 T
(1350) 223.94 442.02 T
(166.) 303.73 442.02 T
(5.89) 331.48 442.02 T
(7.33) 411.73 442.02 T
(1400) 223.94 427.02 T
(146.) 303.73 427.02 T
(5.23) 331.48 427.02 T
(6.41) 411.73 427.02 T
(1450) 223.94 412.02 T
(1) 304.06 412.02 T
(14.) 308.23 412.02 T
(4.74) 331.48 412.02 T
(6.08) 411.73 412.02 T
(1500) 223.94 397.02 T
(89.3) 303.73 397.02 T
(3.41) 331.48 397.02 T
(4.34) 411.73 397.02 T
(1550) 223.94 382.02 T
(67.0) 303.73 382.02 T
(2.34) 331.48 382.02 T
(4.87) 411.73 382.02 T
(1600) 223.94 367.02 T
(43.9) 303.73 367.02 T
(1.36) 331.48 367.02 T
(5.17) 411.73 367.02 T
(4.48) 465.73 367.02 T
(1650) 223.94 352.02 T
(40.0) 303.73 352.02 T
(1.14) 331.48 352.02 T
(4.89) 411.73 352.02 T
(4.63) 465.73 352.02 T
(1700) 223.94 337.02 T
(32.0) 303.73 337.02 T
(0.88) 331.48 337.02 T
(4.74) 411.73 337.02 T
(5.56) 465.73 337.02 T
(1750) 223.94 322.02 T
(20.7) 303.73 322.02 T
(4.80) 411.73 322.02 T
(6.53) 465.73 322.02 T
(1800) 223.94 307.02 T
(10.8) 303.73 307.02 T
(4.78) 411.73 307.02 T
(7.42) 465.73 307.02 T
(1850) 223.94 292.02 T
(4.03) 303.73 292.02 T
(5.02) 411.73 292.02 T
(8.21) 465.73 292.02 T
(1900) 223.94 277.02 T
(1.09) 303.73 277.02 T
(5.20) 411.73 277.02 T
(8.61) 465.73 277.02 T
(1950) 223.94 262.02 T
(5.20) 411.73 262.02 T
(8.40) 465.73 262.02 T
(3.64) 519.73 262.02 T
(2000) 223.94 247.02 T
(5.00) 411.73 247.02 T
(8.23) 465.73 247.02 T
(4.72) 519.73 247.02 T
(2050) 223.94 232.02 T
(4.75) 411.73 232.02 T
(8.57) 465.73 232.02 T
(6.72) 519.73 232.02 T
(2100) 223.94 217.02 T
(4.68) 411.73 217.02 T
(8.92) 465.73 217.02 T
(9.25) 519.73 217.02 T
(2150) 223.94 202.02 T
(9.18) 465.73 202.02 T
(12.31) 515.23 202.02 T
(2200) 223.94 187.02 T
(9.35) 465.73 187.02 T
(16.19) 515.23 187.02 T
(2250) 223.94 172.02 T
(9.02) 465.73 172.02 T
(20.87) 515.23 172.02 T
(2300) 223.94 157.02 T
(8.57) 465.73 157.02 T
(23.82) 515.23 157.02 T
(2350) 223.94 142.02 T
(8.14) 465.73 142.02 T
(23.98) 515.23 142.02 T
(2400) 223.94 127.02 T
(8.70) 465.73 127.02 T
(26.29) 515.23 127.02 T
(2450) 223.94 112.02 T
(9.24) 465.73 112.02 T
(32.34) 515.23 112.02 T
(2500) 223.94 97.02 T
(9.76) 465.73 97.02 T
(41.63) 515.23 97.02 T
194.4 560.89 194.4 92.14 2 L
V
0.25 H
0 Z
N
271.48 561.14 271.48 91.89 2 L
V
N
325.48 544.27 325.48 91.89 2 L
V
N
379.48 544.27 379.48 91.89 2 L
V
N
433.48 544.27 433.48 91.89 2 L
V
N
487.48 544.27 487.48 91.89 2 L
V
N
541.48 560.89 541.48 92.14 2 L
V
N
194.27 561.02 541.6 561.02 2 L
V
N
194.27 544.02 271.6 544.02 2 L
V
N
271.35 544.02 541.6 544.02 2 L
V
0.5 H
N
194.27 527.02 541.6 527.02 2 L
V
N
194.27 512.02 541.6 512.02 2 L
V
0.25 H
N
194.27 497.02 541.6 497.02 2 L
V
N
194.27 482.02 541.6 482.02 2 L
V
N
194.27 467.02 541.6 467.02 2 L
V
N
194.27 452.02 541.6 452.02 2 L
V
N
194.27 437.02 541.6 437.02 2 L
V
N
194.27 422.02 541.6 422.02 2 L
V
N
194.27 407.02 541.6 407.02 2 L
V
N
194.27 392.02 541.6 392.02 2 L
V
N
194.27 377.02 541.6 377.02 2 L
V
N
194.27 362.02 541.6 362.02 2 L
V
N
194.27 347.02 541.6 347.02 2 L
V
N
194.27 332.02 541.6 332.02 2 L
V
N
194.27 317.02 541.6 317.02 2 L
V
N
194.27 302.02 541.6 302.02 2 L
V
N
194.27 287.02 541.6 287.02 2 L
V
N
194.27 272.02 541.6 272.02 2 L
V
N
194.27 257.02 541.6 257.02 2 L
V
N
194.27 242.02 541.6 242.02 2 L
V
N
194.27 227.02 541.6 227.02 2 L
V
N
194.27 212.02 541.6 212.02 2 L
V
N
194.27 197.02 541.6 197.02 2 L
V
N
194.27 182.02 541.6 182.02 2 L
V
N
194.27 167.02 541.6 167.02 2 L
V
N
194.27 152.02 541.6 152.02 2 L
V
N
194.27 137.02 541.6 137.02 2 L
V
N
194.27 122.02 541.6 122.02 2 L
V
N
194.27 107.02 541.6 107.02 2 L
V
N
194.27 92.02 541.6 92.02 2 L
V
N
254.33 644.18 510.69 658.31 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 10 Q
0 X
0 0 0 1 0 0 0 K
(1) 259.88 647.35 T
(0) 264.88 647.35 T
5 7 Q
(1) 270.38 650.22 T
(1) 273.88 650.22 T
5 10 Q
(\050) 277.97 647.35 T
(c) 281.3 647.35 T
(o) 285.74 647.35 T
(u) 290.74 647.35 T
(n) 295.74 647.35 T
(t) 300.74 647.35 T
(s) 303.52 647.35 T
(s) 309.91 647.35 T
(e) 313.8 647.35 T
(c) 318.24 647.35 T
5 7 Q
(1) 326.95 650.22 T
(\320) 323.18 650.22 T
5 10 Q
(d) 333.54 647.35 T
(i) 338.54 647.35 T
(o) 341.32 647.35 T
(d) 346.32 647.35 T
(e) 351.32 647.35 T
5 7 Q
(1) 360.02 650.22 T
(\320) 356.26 650.22 T
5 10 Q
(\051) 364.11 647.35 T
(p) 369.94 647.35 T
(e) 374.94 647.35 T
(r) 379.38 647.35 T
(i) 385.21 647.35 T
(n) 387.99 647.35 T
(c) 392.99 647.35 T
(i) 397.43 647.35 T
(d) 400.21 647.35 T
(e) 405.21 647.35 T
(n) 409.65 647.35 T
(t) 414.65 647.35 T
(\050) 419.93 647.35 T
(e) 423.26 647.35 T
(r) 427.7 647.35 T
(g) 431.03 647.35 T
(c) 438.53 647.35 T
(m) 442.97 647.35 T
5 7 Q
(2) 455.02 650.22 T
(\320) 451.25 650.22 T
5 10 Q
(s) 461.61 647.35 T
(e) 465.5 647.35 T
(c) 469.94 647.35 T
5 7 Q
(1) 478.64 650.22 T
(\320) 474.88 650.22 T
5 10 Q
(\201) 485.23 647.35 T
5 7 Q
(1) 496.72 650.22 T
(\320) 492.95 650.22 T
5 10 Q
(\051) 500.81 647.35 T
0 0 612 792 C
FMENDPAGE
%%EndPage: "85" 5
%%Page: "86" 6
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(86) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
5 9 Q
(2550) 241.94 601.02 T
(49.06) 533.23 601.02 T
(2600) 241.94 586.02 T
(53.21) 533.23 586.02 T
(2650) 241.94 571.02 T
(54.37) 533.23 571.02 T
(2700) 241.94 556.02 T
(53.01) 533.23 556.02 T
(2750) 241.94 541.02 T
(50.28) 533.23 541.02 T
(2800) 241.94 526.02 T
(46.73) 533.23 526.02 T
(2850) 241.94 511.02 T
(42.44) 533.23 511.02 T
(2900) 241.94 496.02 T
(37.71) 533.23 496.02 T
(2950) 241.94 481.02 T
(32.19) 533.23 481.02 T
(3000) 241.94 466.02 T
(25.76) 533.23 466.02 T
(3050) 241.94 451.02 T
(19.46) 533.23 451.02 T
(3100) 241.94 436.02 T
(14.14) 533.23 436.02 T
(3150) 241.94 421.02 T
(10.07) 533.23 421.02 T
(3200) 241.94 406.02 T
(6.53) 537.73 406.02 T
(3250) 241.94 391.02 T
(3.83) 537.73 391.02 T
(3300) 241.94 376.02 T
(2.64) 537.73 376.02 T
72 673.02 558 686.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
207 680.02 558 680.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
72 680.02 198 680.02 2 L
0 Z
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 72 667.02 T
(ABLE 8-2) 76.83 667.02 T
3 F
( \050Continued\051) 207 667.02 T
(Sensitivities for \336rst-order gratings.) 207 656.02 T
0 8 Q
(Grating) 295.48 632.68 T
(W) 218.4 615.68 T
(avelength \050\201\051) 225.66 615.68 T
(G140L) 295.48 615.68 T
(G140M) 349.48 615.68 T
(G160M) 403.48 615.68 T
(G200M) 457.48 615.68 T
(G270M) 511.48 615.68 T
212.4 644.89 212.4 371.14 2 L
V
0.25 H
0 Z
N
289.48 645.14 289.48 370.89 2 L
V
N
343.48 628.27 343.48 370.89 2 L
V
N
397.48 628.27 397.48 370.89 2 L
V
N
451.48 628.27 451.48 370.89 2 L
V
N
505.48 628.27 505.48 370.89 2 L
V
N
559.48 644.89 559.48 371.14 2 L
V
N
212.27 645.02 559.6 645.02 2 L
V
N
212.27 628.02 289.6 628.02 2 L
V
N
289.35 628.02 559.6 628.02 2 L
V
0.5 H
N
212.27 611.02 559.6 611.02 2 L
V
N
212.27 596.02 559.6 596.02 2 L
V
0.25 H
N
212.27 581.02 559.6 581.02 2 L
V
N
212.27 566.02 559.6 566.02 2 L
V
N
212.27 551.02 559.6 551.02 2 L
V
N
212.27 536.02 559.6 536.02 2 L
V
N
212.27 521.02 559.6 521.02 2 L
V
N
212.27 506.02 559.6 506.02 2 L
V
N
212.27 491.02 559.6 491.02 2 L
V
N
212.27 476.02 559.6 476.02 2 L
V
N
212.27 461.02 559.6 461.02 2 L
V
N
212.27 446.02 559.6 446.02 2 L
V
N
212.27 431.02 559.6 431.02 2 L
V
N
212.27 416.02 559.6 416.02 2 L
V
N
212.27 401.02 559.6 401.02 2 L
V
N
212.27 386.02 559.6 386.02 2 L
V
N
212.27 371.02 559.6 371.02 2 L
V
N
FMENDPAGE
%%EndPage: "86" 6
%%Page: "87" 7
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (87) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Reference T) 207 736.18 T
(ables for Instrument Performance) 257.85 736.18 T
54 671.02 540 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 672.52 540 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 672.52 180 672.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(8.3) 163.32 678.02 T
(Properties of the Echelle Gratings) 189 678.02 T
0 10 Q
(8.3.1) 157.76 644.35 T
(W) 189 644.35 T
(avelength Coverage, Bandpass, and Sensitivity) 198.07 644.35 T
5 F
0.81 (The following tables summarize basic properties of the two echelle gratings. The dis-) 189 624.35 P
0.14 (persion in each order has not been listed but does not change if it is computed in veloc-) 189 612.35 P
0.17 (ity units. At the center of each order) 189 600.35 P
0.17 (, the dispersion is 3.0 km s) 334.22 600.35 P
5 8 Q
0.14 (-1) 441.93 604.35 P
5 10 Q
0.17 ( per diode, at the long-) 448.59 600.35 P
-0.04 (wavelength end of each order it is 2.9 km s) 189 588.35 P
5 8 Q
-0.03 (-1) 360.86 592.35 P
5 10 Q
-0.04 ( per diode, and at the short-wavelength end) 367.52 588.35 P
(of each order it is 3.1 km s) 189 576.35 T
5 8 Q
(-1) 295.65 580.35 T
5 10 Q
( per diode.) 302.31 576.35 T
135.06 208.02 540 215.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 612 792 C
5 9 Q
0 X
0 0 0 1 0 0 0 K
-0.08 (a.) 135.06 202.02 P
8 F
-0.08 (\322d\323) 143.48 202.02 P
5 F
-0.08 ( coef) 157.99 202.02 P
-0.08 (\336cient of Cardelli, Ebbets, and Savage \0501993; see Section) 175.48 202.02 P
-0.08 (9.2 on page) 384.07 202.02 P
-0.08 (102\051. These apply only to) 427.9 202.02 P
(the SSA.) 171.06 192.02 T
-0.08 (b. Sensitivity function at blaze peak, in units of 10) 135.06 179.02 P
5 7.2 Q
-0.07 (1) 315.55 182.62 P
-0.07 (1) 318.88 182.62 P
5 9 Q
-0.08 ( \050counts diode) 322.48 179.02 P
5 7.2 Q
-0.07 (-1) 373.3 182.62 P
5 9 Q
-0.08 ( sec) 379.3 179.02 P
5 7.2 Q
-0.07 (-1) 392.96 182.62 P
5 9 Q
-0.08 (\051 per incident \050er) 398.96 179.02 P
-0.08 (g cm) 458.77 179.02 P
5 7.2 Q
-0.07 (-2) 476.44 182.62 P
5 9 Q
-0.08 ( sec) 482.43 179.02 P
5 7.2 Q
-0.07 (-1) 496.09 182.62 P
5 9 Q
-0.08 ( \201) 502.09 179.02 P
5 7.2 Q
-0.07 (-1) 510.76 182.62 P
5 9 Q
-0.08 (\051.) 516.75 179.02 P
54 554.02 540 567.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 561.02 540 561.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 561.02 180 561.02 2 L
0 Z
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 548.02 T
(ABLE 8-3) 58.83 548.02 T
3 F
(Properties of Grating Echelle-A) 189 537.02 T
0 8 Q
(Order) 150.99 504.68 T
(Central) 215.57 513.68 T
(W) 200.39 504.68 T
(avelength \050\201\051) 207.64 504.68 T
(Order) 295.11 513.68 T
(Coverage \050\201\051) 281.11 504.68 T
(Bandpass per) 360.55 513.68 T
(exposure \050\201\051) 362.55 504.68 T
(Scattered) 440.77 513.68 T
(Light) 447.45 504.68 T
0 6.4 Q
(a) 467 507.88 T
0 8 Q
(S) 506.18 504.68 T
6 F
(l) 511.52 502.18 T
0 6.4 Q
(b) 515.91 507.88 T
5 9 Q
(51) 157.38 490.02 T
(1) 220.52 490.02 T
(102) 224.68 490.02 T
(1091 \320 1) 283.83 490.02 T
(1) 315 490.02 T
(13) 319.17 490.02 T
(5.90 \320 5.55) 366.75 490.02 T
432.25 485.27 485.75 499.77 R
7 X
V
0 X
(50) 157.38 475.02 T
(1) 220.52 475.02 T
(124) 224.68 475.02 T
(1) 284 475.02 T
(1) 288.17 475.02 T
(13 \320 1) 292.33 475.02 T
(135) 314.5 475.02 T
(6.05 \320 5.65) 366.75 475.02 T
432.25 470.27 485.75 484.77 R
7 X
V
0 X
(49) 157.38 460.02 T
(1) 220.52 460.02 T
(147) 224.68 460.02 T
(1) 283.83 460.02 T
(135 \320 1) 288 460.02 T
(159) 314.67 460.02 T
(6.15 \320 5.75) 366.75 460.02 T
432.25 455.27 485.75 469.77 R
7 X
V
0 X
(0.061) 448.88 460.02 T
(0.12) 505.12 460.02 T
(48) 157.38 445.02 T
(1) 220.52 445.02 T
(171) 224.68 445.02 T
(1) 283.83 445.02 T
(159 \320 1) 288 445.02 T
(183) 314.67 445.02 T
(6.25 \320 5.90) 366.75 445.02 T
432.25 440.27 485.75 454.77 R
7 X
V
0 X
(0.058) 448.88 445.02 T
(0.27) 505.12 445.02 T
(47) 157.38 430.02 T
(1) 220.52 430.02 T
(196) 224.68 430.02 T
(1) 283.67 430.02 T
(183 \320 1209) 287.83 430.02 T
(6.40 \320 6.00) 366.75 430.02 T
432.25 425.27 485.75 439.77 R
7 X
V
0 X
(0.055) 448.88 430.02 T
(0.46) 505.12 430.02 T
(46) 157.38 415.02 T
(1222) 220.35 415.02 T
(1209 \320 1235) 283.5 415.02 T
(6.55 \320 6.10) 366.75 415.02 T
432.25 410.27 485.75 424.77 R
7 X
V
0 X
(0.052) 448.88 415.02 T
(0.8) 507.38 415.02 T
(45) 157.38 400.02 T
(1249) 220.35 400.02 T
(1235 \320 1263) 283.5 400.02 T
(6.70 \320 6.25) 366.75 400.02 T
432.25 395.27 485.75 409.77 R
7 X
V
0 X
(0.049) 448.88 400.02 T
(0.92) 505.12 400.02 T
(44) 157.38 385.02 T
(1277) 220.35 385.02 T
(1263 \320 1292) 283.5 385.02 T
(6.85 \320 6.40) 366.75 385.02 T
432.25 380.27 485.75 394.77 R
7 X
V
0 X
(0.046) 448.88 385.02 T
(1.15) 505.12 385.02 T
(43) 157.38 370.02 T
(1307) 220.35 370.02 T
(1292 \320 1322) 283.5 370.02 T
(7.05 \320 6.55) 366.75 370.02 T
432.25 365.27 485.75 379.77 R
7 X
V
0 X
(0.044) 448.88 370.02 T
(1.16) 505.12 370.02 T
(42) 157.38 355.02 T
(1338) 220.35 355.02 T
(1322 \320 1354) 283.5 355.02 T
(7.20 \320 6.70) 366.75 355.02 T
432.25 350.27 485.75 364.77 R
7 X
V
0 X
(0.041) 448.88 355.02 T
(1.34) 505.12 355.02 T
(41) 157.38 340.02 T
(1371) 220.35 340.02 T
(1354 \320 1387) 283.5 340.02 T
(7.40 \320 6.85) 366.75 340.02 T
432.25 335.27 485.75 349.77 R
7 X
V
0 X
(0.039) 448.88 340.02 T
(1.23) 505.12 340.02 T
(40) 157.38 325.02 T
(1405) 220.35 325.02 T
(1387 \320 1423) 283.5 325.02 T
(7.55 \320 7.00) 366.75 325.02 T
432.25 320.27 485.75 334.77 R
7 X
V
0 X
(0.037) 448.88 325.02 T
(1.47) 505.12 325.02 T
(39) 157.38 310.02 T
(1441) 220.35 310.02 T
(1423 \320 1460) 283.5 310.02 T
(7.80 \320 7.20) 366.75 310.02 T
432.25 305.27 485.75 319.77 R
7 X
V
0 X
(0.035) 448.88 310.02 T
(1.04) 505.12 310.02 T
(38) 157.38 295.02 T
(1479) 220.35 295.02 T
(1460 \320 1498) 283.5 295.02 T
(8.00 \320 7.40) 366.75 295.02 T
432.25 290.27 485.75 304.77 R
7 X
V
0 X
(0.034) 448.88 295.02 T
(0.91) 505.12 295.02 T
(37) 157.38 280.02 T
(1519) 220.35 280.02 T
(1498 \320 1539) 283.5 280.02 T
(8.25 \320 7.55) 366.75 280.02 T
432.25 275.27 485.75 289.77 R
7 X
V
0 X
(0.032) 448.88 280.02 T
(0.77) 505.12 280.02 T
(36) 157.38 265.02 T
(1561) 220.35 265.02 T
(1539 \320 1583) 283.5 265.02 T
(8.45 \320 7.75) 366.75 265.02 T
432.25 260.27 485.75 274.77 R
7 X
V
0 X
(0.031) 448.88 265.02 T
(0.64) 505.12 265.02 T
(35) 157.38 250.02 T
(1606) 220.35 250.02 T
(1583 \320 1629) 283.5 250.02 T
(8.70 \320 7.95) 366.75 250.02 T
432.25 245.27 485.75 259.77 R
7 X
V
0 X
(0.030) 448.88 250.02 T
(0.56) 505.12 250.02 T
(34) 157.38 235.02 T
(1653) 220.35 235.02 T
(1629 \320 1677) 283.5 235.02 T
(8.95 \320 8.20) 366.75 235.02 T
432.25 230.27 485.75 244.77 R
7 X
V
0 X
(0.030) 448.88 235.02 T
(0.44) 505.12 235.02 T
(33) 157.38 220.02 T
(1703) 220.35 220.02 T
(1677 \320 1729) 283.5 220.02 T
(9.25 \320 8.40) 366.75 220.02 T
432.25 215.27 485.75 229.77 R
7 X
V
0 X
(0.029) 448.88 220.02 T
(0.40) 505.12 220.02 T
135.06 525.89 135.06 215.14 2 L
V
0.25 H
0 Z
N
188.7 526.14 188.7 214.89 2 L
V
N
270 526.14 270 214.89 2 L
V
N
342 526.14 342 214.89 2 L
V
N
432 526.14 432 499.77 2 L
V
N
432 500.27 432 214.77 2 L
V
0.5 H
N
486 526.14 486 499.77 2 L
V
0.25 H
N
486 500.27 486 214.77 2 L
V
0.5 H
N
540 525.89 540 215.14 2 L
V
0.25 H
N
134.93 526.02 540.12 526.02 2 L
V
N
134.93 500.02 540.12 500.02 2 L
V
0.5 H
N
134.93 485.02 432.25 485.02 2 L
V
0.25 H
N
431.75 485.02 486.25 485.02 2 L
V
0.5 H
N
485.75 485.02 540.12 485.02 2 L
V
0.25 H
N
134.93 470.02 432.25 470.02 2 L
V
N
431.75 470.02 486.25 470.02 2 L
V
0.5 H
N
485.75 470.02 540.12 470.02 2 L
V
0.25 H
N
134.93 455.02 432.25 455.02 2 L
V
N
431.75 455.02 486.25 455.02 2 L
V
0.5 H
N
485.75 455.02 540.12 455.02 2 L
V
0.25 H
N
134.93 440.02 432.25 440.02 2 L
V
N
431.75 440.02 486.25 440.02 2 L
V
0.5 H
N
485.75 440.02 540.12 440.02 2 L
V
0.25 H
N
134.93 425.02 432.25 425.02 2 L
V
N
431.75 425.02 486.25 425.02 2 L
V
0.5 H
N
485.75 425.02 540.12 425.02 2 L
V
0.25 H
N
134.93 410.02 432.25 410.02 2 L
V
N
431.75 410.02 486.25 410.02 2 L
V
0.5 H
N
485.75 410.02 540.12 410.02 2 L
V
0.25 H
N
134.93 395.02 432.25 395.02 2 L
V
N
431.75 395.02 486.25 395.02 2 L
V
0.5 H
N
485.75 395.02 540.12 395.02 2 L
V
0.25 H
N
134.93 380.02 432.25 380.02 2 L
V
N
431.75 380.02 486.25 380.02 2 L
V
0.5 H
N
485.75 380.02 540.12 380.02 2 L
V
0.25 H
N
134.93 365.02 432.25 365.02 2 L
V
N
431.75 365.02 486.25 365.02 2 L
V
0.5 H
N
485.75 365.02 540.12 365.02 2 L
V
0.25 H
N
134.93 350.02 432.25 350.02 2 L
V
N
431.75 350.02 486.25 350.02 2 L
V
0.5 H
N
485.75 350.02 540.12 350.02 2 L
V
0.25 H
N
134.93 335.02 432.25 335.02 2 L
V
N
431.75 335.02 486.25 335.02 2 L
V
0.5 H
N
485.75 335.02 540.12 335.02 2 L
V
0.25 H
N
134.93 320.02 432.25 320.02 2 L
V
N
431.75 320.02 486.25 320.02 2 L
V
0.5 H
N
485.75 320.02 540.12 320.02 2 L
V
0.25 H
N
134.93 305.02 432.25 305.02 2 L
V
N
431.75 305.02 486.25 305.02 2 L
V
0.5 H
N
485.75 305.02 540.12 305.02 2 L
V
0.25 H
N
134.93 290.02 432.25 290.02 2 L
V
N
431.75 290.02 486.25 290.02 2 L
V
0.5 H
N
485.75 290.02 540.12 290.02 2 L
V
0.25 H
N
134.93 275.02 432.25 275.02 2 L
V
N
431.75 275.02 486.25 275.02 2 L
V
0.5 H
N
485.75 275.02 540.12 275.02 2 L
V
0.25 H
N
134.93 260.02 432.25 260.02 2 L
V
N
431.75 260.02 486.25 260.02 2 L
V
0.5 H
N
485.75 260.02 540.12 260.02 2 L
V
0.25 H
N
134.93 245.02 432.25 245.02 2 L
V
N
431.75 245.02 486.25 245.02 2 L
V
0.5 H
N
485.75 245.02 540.12 245.02 2 L
V
0.25 H
N
134.93 230.02 432.25 230.02 2 L
V
N
431.75 230.02 486.25 230.02 2 L
V
0.5 H
N
485.75 230.02 540.12 230.02 2 L
V
0.25 H
N
134.93 215.02 431.75 215.02 2 L
V
N
432.25 215.02 485.75 215.02 2 L
V
0.5 H
N
486.25 215.02 540.12 215.02 2 L
V
0.25 H
N
FMENDPAGE
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(88) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
135.06 356.02 540 363.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 612 792 C
5 9 Q
0 X
0 0 0 1 0 0 0 K
-0.08 (a.) 135.06 350.02 P
8 F
-0.08 (\322d\323) 143.48 350.02 P
5 F
-0.08 ( coef) 157.99 350.02 P
-0.08 (\336cient of Cardelli, Ebbets, and Savage \0501993; see Section) 175.48 350.02 P
-0.08 (9.2 on page) 384.07 350.02 P
-0.08 (102\051. These apply only to) 427.9 350.02 P
(the SSA.) 171.06 340.02 T
-0.08 (b. Sensitivity function at blaze peak, in units of 10) 135.06 327.02 P
5 7.2 Q
-0.07 (1) 315.55 330.62 P
-0.07 (1) 318.88 330.62 P
5 9 Q
-0.08 ( \050counts diode) 322.48 327.02 P
5 7.2 Q
-0.07 (-1) 373.3 330.62 P
5 9 Q
-0.08 ( sec) 379.3 327.02 P
5 7.2 Q
-0.07 (-1) 392.96 330.62 P
5 9 Q
-0.08 (\051 per incident \050er) 398.96 327.02 P
-0.08 (g cm) 458.77 327.02 P
5 7.2 Q
-0.07 (-2) 476.44 330.62 P
5 9 Q
-0.08 ( sec) 482.43 327.02 P
5 7.2 Q
-0.07 (-1) 496.09 330.62 P
5 9 Q
-0.08 ( \201) 502.09 327.02 P
5 7.2 Q
-0.07 (-1) 510.76 330.62 P
5 9 Q
-0.08 (\051.) 516.75 327.02 P
54 657.02 540 670.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 664.02 540 664.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 664.02 180 664.02 2 L
0 Z
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 651.02 T
(ABLE 8-4) 58.83 651.02 T
3 F
(Properties of Grating Echelle-B) 189 640.02 T
0 8 Q
(Order) 150.99 607.68 T
(Central) 215.57 616.68 T
(W) 200.39 607.68 T
(avelength \050\201\051) 207.64 607.68 T
(Order) 295.11 616.68 T
(Coverage \050\201\051) 281.11 607.68 T
(Bandpass per) 360.55 616.68 T
(exposure \050\201\051) 362.55 607.68 T
(Scattered) 440.77 616.68 T
(Light) 447.45 607.68 T
0 6.4 Q
(a) 467 610.88 T
0 8 Q
(S) 506.18 616.68 T
6 F
(l) 511.52 614.18 T
0 6.4 Q
(b) 515.91 619.88 T
5 9 Q
(33) 157.38 593.02 T
(1703) 220.35 593.02 T
(1677 \320 1729) 283.5 593.02 T
(9.3 \320 8.4) 371.25 593.02 T
432.25 588.27 485.75 602.77 R
7 X
V
0 X
(0.045) 448.88 593.02 T
(0.35) 505.12 593.02 T
(32) 157.38 578.02 T
(1756) 220.35 578.02 T
(1729 \320 1784) 283.5 578.02 T
(9.6 \320 8.6) 371.25 578.02 T
432.25 573.27 485.75 587.77 R
7 X
V
0 X
(0.043) 448.88 578.02 T
(0.74) 505.12 578.02 T
(31) 157.38 563.02 T
(1813) 220.35 563.02 T
(1784 \320 1842) 283.5 563.02 T
(9.9 \320 8.9) 371.25 563.02 T
432.25 558.27 485.75 572.77 R
7 X
V
0 X
(0.041) 448.88 563.02 T
(1.06) 505.12 563.02 T
(30) 157.38 548.02 T
(1873) 220.35 548.02 T
(1842 \320 1905) 283.5 548.02 T
(10.3 \320 9.2) 369 548.02 T
432.25 543.27 485.75 557.77 R
7 X
V
0 X
(0.039) 448.88 548.02 T
(1.62) 505.12 548.02 T
(29) 157.38 533.02 T
(1938) 220.35 533.02 T
(1905 \320 1971) 283.5 533.02 T
(10.7 \320 9.5) 369 533.02 T
432.25 528.27 485.75 542.77 R
7 X
V
0 X
(0.037) 448.88 533.02 T
(2.26) 505.12 533.02 T
(28) 157.38 518.02 T
(2007) 220.35 518.02 T
(1971 \320 2043) 283.5 518.02 T
(1) 369.17 518.02 T
(1.1 \320 9.8) 373.33 518.02 T
432.25 513.27 485.75 527.77 R
7 X
V
0 X
(0.035) 448.88 518.02 T
(3.04) 505.12 518.02 T
(27) 157.38 503.02 T
(2082) 220.35 503.02 T
(2043 \320 2120) 283.5 503.02 T
(1) 366.92 503.02 T
(1.5 \320 10.1) 371.08 503.02 T
432.25 498.27 485.75 512.77 R
7 X
V
0 X
(0.033) 448.88 503.02 T
(4.29) 505.12 503.02 T
(26) 157.38 488.02 T
(2162) 220.35 488.02 T
(2120 \320 2203) 283.5 488.02 T
(1) 366.92 488.02 T
(1.9 \320 10.5) 371.08 488.02 T
432.25 483.27 485.75 497.77 R
7 X
V
0 X
(0.031) 448.88 488.02 T
(6.18) 505.12 488.02 T
(25) 157.38 473.02 T
(2248) 220.35 473.02 T
(2203 \320 2293) 283.5 473.02 T
(12.4 \320 10.9) 366.75 473.02 T
432.25 468.27 485.75 482.77 R
7 X
V
0 X
(0.030) 448.88 473.02 T
(8.59) 505.12 473.02 T
(24) 157.38 458.02 T
(2342) 220.35 458.02 T
(2293 \320 2391) 283.5 458.02 T
(13.0 \320 1) 366.92 458.02 T
(1.3) 395.83 458.02 T
432.25 453.27 485.75 467.77 R
7 X
V
0 X
(0.028) 448.88 458.02 T
(9.96) 505.12 458.02 T
(23) 157.38 443.02 T
(2444) 220.35 443.02 T
(2390 \320 2497) 283.5 443.02 T
(13.6 \320 1) 366.92 443.02 T
(1.7) 395.83 443.02 T
432.25 438.27 485.75 452.77 R
7 X
V
0 X
(0.026) 448.88 443.02 T
(1) 505.29 443.02 T
(1.2) 509.46 443.02 T
(22) 157.38 428.02 T
(2555) 220.35 428.02 T
(2497 \320 2613) 283.5 428.02 T
(14.2 \320 12.2) 366.75 428.02 T
432.25 423.27 485.75 437.77 R
7 X
V
0 X
(0.024) 448.88 428.02 T
(13.0) 505.12 428.02 T
(21) 157.38 413.02 T
(2676) 220.35 413.02 T
(2613 \320 2740) 283.5 413.02 T
(14.9 \320 12.7) 366.75 413.02 T
432.25 408.27 485.75 422.77 R
7 X
V
0 X
(0.022) 448.88 413.02 T
(13.4) 505.12 413.02 T
(20) 157.38 398.02 T
(2810) 220.35 398.02 T
(2740 \320 2880) 283.5 398.02 T
(15.8 \320 13.3) 366.75 398.02 T
432.25 393.27 485.75 407.77 R
7 X
V
0 X
(0.020) 448.88 398.02 T
(12.8) 505.12 398.02 T
(19) 157.38 383.02 T
(2958) 220.35 383.02 T
(2880 \320 3036) 283.5 383.02 T
(16.7 \320 13.9) 366.75 383.02 T
432.25 378.27 485.75 392.77 R
7 X
V
0 X
(0.018) 448.88 383.02 T
(9.57) 505.12 383.02 T
(18) 157.38 368.02 T
(3122) 220.35 368.02 T
(3036 \320 3209) 283.5 368.02 T
(17.6 \320 14.6) 366.75 368.02 T
432.25 363.27 485.75 377.77 R
7 X
V
0 X
(0.016) 448.88 368.02 T
(4.20) 505.12 368.02 T
135.06 628.89 135.06 363.14 2 L
V
0.25 H
0 Z
N
188.7 629.14 188.7 362.89 2 L
V
N
270 629.14 270 362.89 2 L
V
N
342 629.14 342 362.89 2 L
V
N
432 629.14 432 602.77 2 L
V
N
432 603.27 432 362.77 2 L
V
0.5 H
N
486 629.14 486 602.77 2 L
V
0.25 H
N
486 603.27 486 362.77 2 L
V
0.5 H
N
540 628.89 540 363.14 2 L
V
0.25 H
N
134.93 629.02 540.12 629.02 2 L
V
N
134.93 603.02 540.12 603.02 2 L
V
0.5 H
N
134.93 588.02 432.25 588.02 2 L
V
0.25 H
N
431.75 588.02 486.25 588.02 2 L
V
0.5 H
N
485.75 588.02 540.12 588.02 2 L
V
0.25 H
N
134.93 573.02 432.25 573.02 2 L
V
N
431.75 573.02 486.25 573.02 2 L
V
0.5 H
N
485.75 573.02 540.12 573.02 2 L
V
0.25 H
N
134.93 558.02 432.25 558.02 2 L
V
N
431.75 558.02 486.25 558.02 2 L
V
0.5 H
N
485.75 558.02 540.12 558.02 2 L
V
0.25 H
N
134.93 543.02 432.25 543.02 2 L
V
N
431.75 543.02 486.25 543.02 2 L
V
0.5 H
N
485.75 543.02 540.12 543.02 2 L
V
0.25 H
N
134.93 528.02 432.25 528.02 2 L
V
N
431.75 528.02 486.25 528.02 2 L
V
0.5 H
N
485.75 528.02 540.12 528.02 2 L
V
0.25 H
N
134.93 513.02 432.25 513.02 2 L
V
N
431.75 513.02 486.25 513.02 2 L
V
0.5 H
N
485.75 513.02 540.12 513.02 2 L
V
0.25 H
N
134.93 498.02 432.25 498.02 2 L
V
N
431.75 498.02 486.25 498.02 2 L
V
0.5 H
N
485.75 498.02 540.12 498.02 2 L
V
0.25 H
N
134.93 483.02 432.25 483.02 2 L
V
N
431.75 483.02 486.25 483.02 2 L
V
0.5 H
N
485.75 483.02 540.12 483.02 2 L
V
0.25 H
N
134.93 468.02 432.25 468.02 2 L
V
N
431.75 468.02 486.25 468.02 2 L
V
0.5 H
N
485.75 468.02 540.12 468.02 2 L
V
0.25 H
N
134.93 453.02 432.25 453.02 2 L
V
N
431.75 453.02 486.25 453.02 2 L
V
0.5 H
N
485.75 453.02 540.12 453.02 2 L
V
0.25 H
N
134.93 438.02 432.25 438.02 2 L
V
N
431.75 438.02 486.25 438.02 2 L
V
0.5 H
N
485.75 438.02 540.12 438.02 2 L
V
0.25 H
N
134.93 423.02 432.25 423.02 2 L
V
N
431.75 423.02 486.25 423.02 2 L
V
0.5 H
N
485.75 423.02 540.12 423.02 2 L
V
0.25 H
N
134.93 408.02 432.25 408.02 2 L
V
N
431.75 408.02 486.25 408.02 2 L
V
0.5 H
N
485.75 408.02 540.12 408.02 2 L
V
0.25 H
N
134.93 393.02 432.25 393.02 2 L
V
N
431.75 393.02 486.25 393.02 2 L
V
0.5 H
N
485.75 393.02 540.12 393.02 2 L
V
0.25 H
N
134.93 378.02 432.25 378.02 2 L
V
N
431.75 378.02 486.25 378.02 2 L
V
0.5 H
N
485.75 378.02 540.12 378.02 2 L
V
0.25 H
N
134.93 363.02 431.75 363.02 2 L
V
N
432.25 363.02 485.75 363.02 2 L
V
0.5 H
N
486.25 363.02 540.12 363.02 2 L
V
0.25 H
N
FMENDPAGE
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0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (89) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Reference T) 207 736.18 T
(ables for Instrument Performance) 257.85 736.18 T
0 10 Q
(8.3.2) 157.76 679.35 T
(Echelle W) 189 679.35 T
(avelength Formats) 235.87 679.35 T
5 F
-0.03 (The illustrations below provide a means of estimating where particular wavelengths fall) 189 663.35 P
0.22 (within the echelle formats and where they lie relative to the blaze peak. Note that these) 189 651.35 P
0.53 (layouts are purely schematic; the actual length of the free spectral range changes from) 189 639.35 P
(order to order) 189 627.35 T
(. The center of each order is at) 243.43 627.35 T
8 F
(m) 367.55 627.35 T
6 F
(l) 374.77 627.35 T
5 F
( = 56200.) 380.26 627.35 T
0 F
(Figure 8-4.) 126 129.33 T
3 F
(Schematic format of wavelengths for Echelle-B.) 182.13 129.33 T
54 87.98 540 686.02 C
54 145 540 609.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
107 517 125 533 R
0 0 0 0 1 1 1 K
105 151 126 167 R
126 556.02 522 646.02 R
7 X
V
106 178 125 197 R
V
1 H
2 Z
N
105 549 124 562 R
V
N
0 0 0 1 0 0 0 K
0 56 82 551 624 445.5 487.8 74.25 153.11 FMBEGINEPSF
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1598 2581 d 1715 2600 r 1715 2562 d 1832 2600 r 1832 2581 d 1949 2600 r
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878 1462 d 878 1466 d 877 1472 d 875 1475 d 871 1476 d 869 1476 d
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805 1651 d 807 1651 d 811 1652 d 813 1656 d 814 1662 d 814 1666 d
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1388 1676 d 1388 1651 d 1418 1668 r 1417 1664 d 1415 1662 d 1411 1661 d
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54 726.98 540 726.98 2 L
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54 726.98 540 726.98 2 L
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1840 2556 d 1842 2552 d 1846 2551 d 1848 2551 d 1852 2552 d 1854 2556 d
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7 X
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2 Z
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N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
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N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (91) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
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72 726.98 558 726.98 2 L
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72 74.02 558 74.02 2 L
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72 750.02 558 750.02 2 L
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0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
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(ables for Instrument Performance) 257.85 736.18 T
0 10 Q
(8.3.3) 157.76 679.35 T
(Echelle Blaze Function) 189 679.35 T
5 F
1.04 (The \336gure below shows the echelle blaze function \050also known as the \322Ripple Func-) 189 659.35 P
0.11 (tion\323\051 in the form of sensitivity relative to the peak of the blaze as the product of wave-) 189 647.35 P
(length and order number) 189 635.35 T
(.) 287.04 635.35 T
0 F
(Figure 8-6.) 126 330.33 T
3 F
(Normalized blaze function for the GHRS echelle gratings.) 182.13 330.33 T
54 87.98 540 686.02 C
54 346 540 617.02 C
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499 1405 d 499 1400 d 500 1392 d 504 1387 d 508 1386 d 512 1386 d
516 1387 d 520 1392 d 521 1400 d 521 1405 d 520 1413 d 516 1418 d
512 1419 d 508 1419 d 534 1389 r 532 1387 d 534 1386 d 536 1387 d
534 1389 d 566 1419 r 550 1419 d 548 1405 d 550 1406 d 555 1408 d
560 1408 d 564 1406 d 568 1403 d 569 1398 d 569 1395 d 568 1390 d
564 1387 d 560 1386 d 555 1386 d 550 1387 d 548 1389 d 547 1392 d
504 1813 r 507 1814 d 512 1819 d 512 1786 d 534 1789 r 532 1787 d
534 1786 d 536 1787 d 534 1789 d 556 1819 r 552 1818 d 548 1813 d
547 1805 d 547 1800 d 548 1792 d 552 1787 d 556 1786 d 560 1786 d
564 1787 d 568 1792 d 569 1800 d 569 1805 d 568 1813 d 564 1818 d
560 1819 d 556 1819 d 2200 1000 r 2200 1800 d 2200 1000 r 2149 1000 d
2200 1080 r 2174 1080 d 2200 1160 r 2174 1160 d 2200 1240 r 2174 1240 d
2200 1320 r 2174 1320 d 2200 1400 r 2149 1400 d 2200 1480 r 2174 1480 d
2200 1560 r 2174 1560 d 2200 1640 r 2174 1640 d 2200 1720 r 2174 1720 d
2200 1800 r 2149 1800 d 336 1126 r 378 1126 d 336 1126 r 336 1144 d
338 1150 d 340 1152 d 344 1154 d 348 1154 d 352 1152 d 354 1150 d
356 1144 d 356 1126 d 356 1140 r 378 1154 d 362 1168 r 362 1192 d
358 1192 d 354 1190 d 352 1188 d 350 1184 d 350 1178 d 352 1174 d
356 1170 d 362 1168 d 366 1168 d 372 1170 d 376 1174 d 378 1178 d
378 1184 d 376 1188 d 372 1192 d 336 1206 r 378 1206 d 350 1244 r
378 1244 d 356 1244 r 352 1240 d 350 1236 d 350 1230 d 352 1226 d
356 1222 d 362 1220 d 366 1220 d 372 1222 d 376 1226 d 378 1230 d
378 1236 d 376 1240 d 372 1244 d 336 1260 r 370 1260 d 376 1262 d
378 1266 d 378 1270 d 350 1254 r 350 1268 d 336 1276 r 338 1278 d
336 1280 d 334 1278 d 336 1276 d 350 1278 r 378 1278 d 350 1290 r
378 1302 d 350 1314 r 378 1302 d 362 1324 r 362 1348 d 358 1348 d
354 1346 d 352 1344 d 350 1340 d 350 1334 d 352 1330 d 356 1326 d
362 1324 d 366 1324 d 372 1326 d 376 1330 d 378 1334 d 378 1340 d
376 1344 d 372 1348 d 342 1420 r 338 1416 d 336 1410 d 336 1402 d
338 1396 d 342 1392 d 346 1392 d 350 1394 d 352 1396 d 354 1400 d
358 1412 d 360 1416 d 362 1418 d 366 1420 d 372 1420 d 376 1416 d
378 1410 d 378 1402 d 376 1396 d 372 1392 d 362 1432 r 362 1456 d
358 1456 d 354 1454 d 352 1452 d 350 1448 d 350 1442 d 352 1438 d
356 1434 d 362 1432 d 366 1432 d 372 1434 d 376 1438 d 378 1442 d
378 1448 d 376 1452 d 372 1456 d 350 1470 r 378 1470 d 358 1470 r
352 1476 d 350 1480 d 350 1486 d 352 1490 d 358 1492 d 378 1492 d
356 1526 r 352 1524 d 350 1518 d 350 1512 d 352 1506 d 356 1504 d
360 1506 d 362 1510 d 364 1520 d 366 1524 d 370 1526 d 372 1526 d
376 1524 d 378 1518 d 378 1512 d 376 1506 d 372 1504 d 336 1536 r
338 1538 d 336 1540 d 334 1538 d 336 1536 d 350 1538 r 378 1538 d
336 1556 r 370 1556 d 376 1558 d 378 1562 d 378 1566 d 350 1550 r
350 1564 d 336 1572 r 338 1574 d 336 1576 d 334 1574 d 336 1572 d
350 1574 r 378 1574 d 350 1586 r 378 1598 d 350 1610 r 378 1598 d
336 1620 r 338 1622 d 336 1624 d 334 1622 d 336 1620 d 350 1622 r
378 1622 d 336 1640 r 370 1640 d 376 1642 d 378 1646 d 378 1650 d
350 1634 r 350 1648 d 350 1654 r 378 1666 d 350 1678 r 378 1666 d
386 1662 d 390 1658 d 392 1654 d 392 1652 d 1156 882 r 1156 854 d
1156 874 r 1162 880 d 1166 882 d 1172 882 d 1176 880 d 1178 874 d
1178 854 d 1178 874 r 1184 880 d 1188 882 d 1194 882 d 1198 880 d
1200 874 d 1200 854 d 1214 896 r 1218 896 d 1222 894 d 1224 892 d
1228 882 d 1240 856 d 1242 854 d 1218 896 r 1222 892 d 1226 882 d
1238 856 d 1242 854 d 1244 854 d 1226 882 r 1212 854 d 1226 882 r
1214 854 d 1302 904 r 1298 900 d 1294 894 d 1290 886 d 1288 876 d
1288 868 d 1290 858 d 1294 850 d 1298 844 d 1302 840 d 1326 896 r
1310 854 d 1326 896 r 1342 854 d 1316 868 r 1336 868 d 1352 882 r
1352 854 d 1352 874 r 1358 880 d 1362 882 d 1368 882 d 1372 880 d
1374 874 d 1374 854 d 1410 882 r 1410 850 d 1408 844 d 1406 842 d
1402 840 d 1396 840 d 1392 842 d 1410 876 r 1406 880 d 1402 882 d
1396 882 d 1392 880 d 1388 876 d 1386 870 d 1386 866 d 1388 860 d
1392 856 d 1396 854 d 1402 854 d 1406 856 d 1410 860 d 1444 876 r
1442 880 d 1436 882 d 1430 882 d 1424 880 d 1422 876 d 1424 872 d
1428 870 d 1438 868 d 1442 866 d 1444 862 d 1444 860 d 1442 856 d
1436 854 d 1430 854 d 1424 856 d 1422 860 d 1458 896 r 1458 862 d
1460 856 d 1464 854 d 1468 854 d 1452 882 r 1466 882 d 1476 882 r
1476 854 d 1476 870 r 1478 876 d 1482 880 d 1486 882 d 1492 882 d
1512 882 r 1508 880 d 1504 876 d 1502 870 d 1502 866 d 1504 860 d
1508 856 d 1512 854 d 1518 854 d 1522 856 d 1526 860 d 1528 866 d
1528 870 d 1526 876 d 1522 880 d 1518 882 d 1512 882 d 1540 882 r
1540 854 d 1540 874 r 1546 880 d 1550 882 d 1556 882 d 1560 880 d
1562 874 d 1562 854 d 1562 874 r 1568 880 d 1572 882 d 1578 882 d
1582 880 d 1584 874 d 1584 854 d 1620 876 r 1618 880 d 1612 882 d
1606 882 d 1600 880 d 1598 876 d 1600 872 d 1604 870 d 1614 868 d
1618 866 d 1620 862 d 1620 860 d 1618 856 d 1612 854 d 1606 854 d
1600 856 d 1598 860 d 1630 904 r 1634 900 d 1638 894 d 1642 886 d
1644 876 d 1644 868 d 1642 858 d 1638 850 d 1634 844 d 1630 840 d
747 1266 r 813 1378 d 867 1474 d 920 1550 d 973 1616 d 1027 1672 d
1080 1728 d 1133 1762 d 1187 1786 d 1240 1797 d 1256 1800 d 1293 1794 d
1347 1773 d 1400 1741 d 1453 1700 d 1507 1646 d 1560 1584 d 1613 1522 d
1667 1471 d 1720 1408 d 1773 1354 d 1827 1300 d 1880 1248 d 1933 1200 d
e
%%Trailer
EndPSPlot

%%EndDocument
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54 87.98 540 686.02 C
0 0 612 792 C
FMENDPAGE
%%EndPage: "91" 11
%%Page: "92" 12
612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(92) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
0 12 Q
(8.4) 163.32 678.02 T
(Standard Patterns for Substepping and Background) 189 678.02 T
54 657.02 540 660.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 658.52 540 658.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 658.52 180 658.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(Measurement) 189 664.02 T
5 10 Q
-0.06 (This table shows how each) 189 640.35 P
9 F
-0.14 (STEP-PATT) 298.97 640.35 P
5 F
-0.06 ( pattern measures the background for a science) 352.97 640.35 P
0.48 (exposure. Listed are the) 189 628.35 P
9 F
1.16 (STEP-PATT) 288.96 628.35 P
5 F
0.48 ( number) 342.96 628.35 P
0.48 (, the number of spectrum bins for which) 376.09 628.35 P
0.37 (substepping occurs, the number of background bins measured, the diodes used to mea-) 189 616.35 P
0.57 (sure the background, the fraction of the total time spent measuring \337ux on the science) 189 604.35 P
-0.25 (diodes, the gratings for which the) 189 592.35 P
9 F
-0.59 (STEP-PATT) 323.89 592.35 P
5 F
-0.25 ( is appropriate, and the shortest exposure) 377.89 592.35 P
0.98 (that can be used for that pattern. The shortest exposure has been computed assuming) 189 580.35 P
9 F
0.68 (COMB=4) 189 568.35 P
5 F
0.28 (, which is the recommended value. These minimum exposures can be reduced) 225 568.35 P
(by half if) 189 556.35 T
9 F
(COMB=2) 228.16 556.35 T
5 F
( is used and by a factor of four for) 264.16 556.35 T
9 F
(COMB=NO) 403.01 556.35 T
5 F
(.) 445.01 556.35 T
54 519.02 540 532.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 526.02 540 526.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 526.02 180 526.02 2 L
0 Z
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 513.02 T
(ABLE 8-5) 58.83 513.02 T
3 F
(STEP-P) 189 502.02 T
(A) 220.84 502.02 T
(TT speci\336cations) 226.18 502.02 T
10 F
(STEP-) 67.46 478.68 T
(PATT) 70.16 469.68 T
0 8 Q
(number) 66.29 460.68 T
(Bins Measured) 136.11 478.68 T
(Spectrum/) 236.94 478.68 T
(Backgr) 242.94 469.68 T
(Ratio) 246.5 460.68 T
(Diodes used for) 298.27 474.18 T
(Background) 305.16 465.18 T
(On-target) 380.25 474.18 T
(Ef\336ciency) 379.35 465.18 T
(Appropriate) 434.08 474.18 T
( Gratings) 439.19 465.18 T
(Minimum) 495.44 478.68 T
(Exposure) 494.77 469.68 T
(T) 493.29 460.68 T
(ime \050sec\051) 498.03 460.68 T
(Spectrum) 114.61 460.68 T
(Background) 170.16 460.68 T
9 9 Q
(1) 78.26 446.02 T
5 F
(1) 130.81 446.02 T
(0) 191.25 446.02 T
(1) 254.25 446.02 T
(1.00) 390.38 446.02 T
(all) 452.25 446.02 T
(0.8) 507.38 446.02 T
9 F
(2) 78.26 431.02 T
5 F
(2) 130.81 431.02 T
(0) 191.25 431.02 T
(1) 254.25 431.02 T
(1.00) 390.38 431.02 T
(all) 452.25 431.02 T
(1.6) 507.38 431.02 T
9 F
(3) 78.26 416.02 T
5 F
(4) 130.81 416.02 T
(0) 191.25 416.02 T
(1) 254.25 416.02 T
(1.00) 390.38 416.02 T
(all) 452.25 416.02 T
(3.2) 507.38 416.02 T
9 F
(4) 78.26 401.02 T
5 F
(2) 130.81 401.02 T
(2) 191.25 401.02 T
(8) 254.25 401.02 T
(science) 315.26 401.02 T
(0.89) 390.38 401.02 T
(\336rst-order) 438.76 401.02 T
(14.4) 505.12 401.02 T
9 F
(5) 78.26 386.02 T
5 F
(4) 130.81 386.02 T
(2) 191.25 386.02 T
(8) 254.25 386.02 T
(science) 315.26 386.02 T
(0.94) 390.38 386.02 T
(\336rst-order) 438.76 386.02 T
(27.2) 505.12 386.02 T
9 F
(6) 78.26 371.02 T
5 F
(2) 130.81 371.02 T
(2) 191.25 371.02 T
(8) 254.25 371.02 T
(science) 315.26 371.02 T
(0.89) 390.38 371.02 T
(echelle) 444.01 371.02 T
(14.4) 505.12 371.02 T
9 F
(7) 78.26 356.02 T
5 F
(4) 130.81 356.02 T
(2) 191.25 356.02 T
(8) 254.25 356.02 T
(science) 315.26 356.02 T
(0.94) 390.38 356.02 T
(echelle) 444.01 356.02 T
(27.2) 505.12 356.02 T
9 F
(8) 78.26 341.02 T
5 F
(2) 130.81 341.02 T
(2) 191.25 341.02 T
(8) 254.25 341.02 T
(corner) 317.01 341.02 T
(0.89) 390.38 341.02 T
(echelle) 444.01 341.02 T
(14.4) 505.12 341.02 T
9 F
(9) 78.26 326.02 T
5 F
(4) 130.81 326.02 T
(2) 191.25 326.02 T
(8) 254.25 326.02 T
(corner) 317.01 326.02 T
(0.94) 390.38 326.02 T
(echelle) 444.01 326.02 T
(27.2) 505.12 326.02 T
9 F
(10) 75.56 311.02 T
5 F
(2) 130.81 311.02 T
(2) 191.25 311.02 T
(1) 254.25 311.02 T
(science) 315.26 311.02 T
(0.50) 390.38 311.02 T
(\336rst-order) 438.76 311.02 T
(3.2) 507.38 311.02 T
9 F
(11) 75.56 296.02 T
5 F
(4) 130.81 296.02 T
(2) 191.25 296.02 T
(1) 254.25 296.02 T
(science) 315.26 296.02 T
(0.67) 390.38 296.02 T
(\336rst-order) 438.76 296.02 T
(4.8) 507.38 296.02 T
9 F
(12) 75.56 281.02 T
5 F
(2) 130.81 281.02 T
(2) 191.25 281.02 T
(1) 254.25 281.02 T
(science) 315.26 281.02 T
(0.50) 390.38 281.02 T
(echelle) 444.01 281.02 T
(3.2) 507.38 281.02 T
9 F
(13) 75.56 266.02 T
5 F
(4) 130.81 266.02 T
(2) 191.25 266.02 T
(1) 254.25 266.02 T
(science) 315.26 266.02 T
(0.67) 390.38 266.02 T
(echelle) 444.01 266.02 T
(4.8) 507.38 266.02 T
9 F
(14) 75.56 251.02 T
5 F
(2) 130.81 251.02 T
(2) 191.25 251.02 T
(1) 254.25 251.02 T
(corner) 317.01 251.02 T
(0.50) 390.38 251.02 T
(echelle) 444.01 251.02 T
(3.2) 507.38 251.02 T
9 F
(15) 75.56 236.02 T
5 F
(4) 130.81 236.02 T
(2) 191.25 236.02 T
(1) 254.25 236.02 T
(corner) 317.01 236.02 T
(0.67) 390.38 236.02 T
(echelle) 444.01 236.02 T
(4.8) 507.38 236.02 T
54 195.02 540 208.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 202.02 540 202.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 202.02 180 202.02 2 L
0 Z
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 189.02 T
(ABLE 8-6) 58.83 189.02 T
3 F
(Default STEP-P) 189 189.02 T
(A) 251.86 189.02 T
(TT for science modes) 257.19 189.02 T
3 8 Q
(Grating) 326.62 172.68 T
(Order) 407.15 172.68 T
9 9 Q
(STEP-PATT) 466.76 172.02 T
5 F
(First-order) 326.62 159.02 T
(1) 415.12 159.02 T
9 F
(5) 488.36 159.02 T
5 F
(Ech-A) 326.62 146.02 T
6 10 Q
(\263) 409.01 146.02 T
5 9 Q
( 51) 414.49 146.02 T
9 F
(9) 488.36 146.02 T
5 F
(< 51) 409.21 133.02 T
9 F
(7) 488.36 133.02 T
5 F
(Ech-B) 326.62 120.02 T
6 10 Q
(\263) 409.01 120.02 T
5 9 Q
( 31) 414.49 120.02 T
9 F
(9) 488.36 120.02 T
5 F
(< 31) 409.21 107.02 T
9 F
(7) 488.36 107.02 T
57.8 490.89 57.8 231.14 2 L
V
0.25 H
0 Z
N
104.12 491.14 104.12 230.89 2 L
V
N
162 474.14 162 230.89 2 L
V
N
225 491.14 225 230.89 2 L
V
N
288 491.14 288 230.89 2 L
V
N
369 491.14 369 230.89 2 L
V
N
427.5 491.14 427.5 230.89 2 L
V
N
486 491.14 486 230.89 2 L
V
N
540 490.89 540 231.14 2 L
V
N
57.67 491.02 540.12 491.02 2 L
V
N
104 474.02 225.12 474.02 2 L
V
N
57.67 456.02 540.12 456.02 2 L
V
0.5 H
N
57.67 441.02 540.12 441.02 2 L
V
0.25 H
N
57.67 426.02 540.12 426.02 2 L
V
N
57.67 411.02 540.12 411.02 2 L
V
N
57.67 396.02 540.12 396.02 2 L
V
N
57.67 381.02 540.12 381.02 2 L
V
N
57.67 366.02 540.12 366.02 2 L
V
N
57.67 351.02 540.12 351.02 2 L
V
N
57.67 336.02 540.12 336.02 2 L
V
N
57.67 321.02 540.12 321.02 2 L
V
N
57.67 306.02 540.12 306.02 2 L
V
N
57.67 291.02 540.12 291.02 2 L
V
N
57.67 276.02 540.12 276.02 2 L
V
N
57.67 261.02 540.12 261.02 2 L
V
N
57.67 246.02 540.12 246.02 2 L
V
N
57.67 231.02 540.12 231.02 2 L
V
N
320.62 179.89 320.62 102.14 2 L
V
N
392.62 180.14 392.62 101.89 2 L
V
N
442.12 180.14 442.12 101.89 2 L
V
N
540 179.89 540 102.14 2 L
V
N
320.5 180.02 540.12 180.02 2 L
V
N
320.5 167.02 540.12 167.02 2 L
V
N
320.5 154.02 540.12 154.02 2 L
V
N
392.5 141.02 540.12 141.02 2 L
V
N
320.5 128.02 540.12 128.02 2 L
V
N
392.5 115.02 540.12 115.02 2 L
V
N
320.5 102.02 540.12 102.02 2 L
V
N
FMENDPAGE
%%EndPage: "92" 12
%%Page: "93" 13
612 792 0 FMBEGINPAGE
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[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (93) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Reference T) 207 736.18 T
(ables for Instrument Performance) 257.85 736.18 T
54 671.02 540 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 672.52 540 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 672.52 180 672.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(8.5) 163.32 678.02 T
(The Effects of Reddening in the Ultraviolet) 189 678.02 T
5 10 Q
0.8 (The table above lists extinction from interstellar reddening at ultraviolet wavelengths.) 189 423.35 P
-0.23 (More information on the ef) 189 411.35 P
-0.23 (fects of reddening may be found in the bibliography in Chap-) 296.77 411.35 P
0.11 (ter 9. The above values are from Code et al. \0501976\051. Seaton \0501979\051 has provided conve-) 189 399.35 P
(nient \336ts to ultraviolet extinction for) 189 387.35 T
8 F
(x) 336.78 387.35 T
5 F
( =) 341.22 387.35 T
6 F
(1/l) 351.86 387.35 T
5 F
(, with) 365.13 387.35 T
6 F
(l) 390.41 387.35 T
5 F
( in microns:) 395.9 387.35 T
54 650.02 540 663.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 657.02 540 657.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 657.02 180 657.02 2 L
0 Z
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 644.02 T
(ABLE 8-7) 58.83 644.02 T
3 F
(A) 189 633.02 T
(verage normalized ultraviolet extinction as a function of wavelength.) 194.84 633.02 T
0 8 Q
(W) 231.77 609.68 T
(avelength \050\201\051) 239.02 609.68 T
4 9 Q
(A) 318.82 609.68 T
6 8 Q
(l) 324.82 607.18 T
11 F
(/E\050B-V\051) 329.22 609.68 T
0 F
(W) 385.04 609.68 T
(avelength \050\201\051) 392.29 609.68 T
4 9 Q
(A) 476.47 609.68 T
6 8 Q
(l) 482.47 607.18 T
11 F
(/E\050B-V\051) 486.86 609.68 T
5 9 Q
(1) 251.9 595.02 T
(100) 256.06 595.02 T
(1) 327.39 595.02 T
(1.70) 331.56 595.02 T
(2160) 405 595.02 T
(10.10) 484.88 595.02 T
(1200) 251.73 580.02 T
(10.20) 327.23 580.02 T
(2200) 405 580.02 T
(9.85) 487.12 580.02 T
(1300) 251.73 565.02 T
(9.19) 329.48 565.02 T
(2300) 405 565.02 T
(8.75) 487.12 565.02 T
(1400) 251.73 550.02 T
(8.54) 329.48 550.02 T
(2400) 405 550.02 T
(7.92) 487.12 550.02 T
(1500) 251.73 535.02 T
(8.29) 329.48 535.02 T
(2500) 405 535.02 T
(7.30) 487.12 535.02 T
(1600) 251.73 520.02 T
(8.03) 329.48 520.02 T
(2600) 405 520.02 T
(6.82) 487.12 520.02 T
(1700) 251.73 505.02 T
(7.85) 329.48 505.02 T
(2700) 405 505.02 T
(6.41) 487.12 505.02 T
(1800) 251.73 490.02 T
(7.90) 329.48 490.02 T
(2800) 405 490.02 T
(6.10) 487.12 490.02 T
(1900) 251.73 475.02 T
(8.38) 329.48 475.02 T
(2900) 405 475.02 T
(5.85) 487.12 475.02 T
(2000) 251.73 460.02 T
(9.05) 329.48 460.02 T
(3000) 405 460.02 T
(5.65) 487.12 460.02 T
(2100) 251.73 445.02 T
(9.90) 329.48 445.02 T
(3300) 405 445.02 T
(5.16) 487.12 445.02 T
8 10 Q
(x) 205.93 342.35 T
5 F
( range) 210.37 342.35 T
8 F
(X\050x\051 = A) 372.26 342.35 T
6 8 Q
(l) 407.33 339.85 T
8 10 Q
(/E\050B\320V\051) 411.72 342.35 T
5 9 Q
(2.70) 170.25 321.02 T
6 F
(\243) 188.25 321.02 T
8 F
(x) 195.44 321.02 T
6 F
(\243) 201.69 321.02 T
5 F
( 3.65) 206.63 321.02 T
(3.65) 170.25 299.02 T
6 F
( \243) 186 299.02 T
8 F
(x) 195.44 299.02 T
6 F
(\243) 201.69 299.02 T
5 F
( 7.14) 206.63 299.02 T
(7.14) 170.25 277.02 T
6 F
(\243) 188.25 277.02 T
8 F
(x) 195.44 277.02 T
6 F
(\243) 201.69 277.02 T
5 F
( 10) 206.63 277.02 T
224.76 621.89 224.76 440.14 2 L
V
0.25 H
0 Z
N
296.7 622.14 296.7 559.89 2 L
V
N
296.7 560.14 296.7 544.89 2 L
V
0.5 H
N
296.7 545.14 296.7 439.89 2 L
V
0.25 H
N
378 622.14 378 439.77 2 L
V
2 H
N
450 622.14 450 439.77 2 L
V
0.25 H
N
540 621.89 540 440.14 2 L
V
N
224.63 622.02 540.12 622.02 2 L
V
N
224.63 605.02 540.12 605.02 2 L
V
0.5 H
N
224.63 590.02 540.12 590.02 2 L
V
0.25 H
N
224.63 575.02 540.12 575.02 2 L
V
N
224.63 560.02 540.12 560.02 2 L
V
N
224.63 545.02 540.12 545.02 2 L
V
N
224.63 530.02 540.12 530.02 2 L
V
N
224.63 515.02 540.12 515.02 2 L
V
N
224.63 500.02 540.12 500.02 2 L
V
N
224.63 485.02 540.12 485.02 2 L
V
N
224.63 470.02 540.12 470.02 2 L
V
N
224.63 455.02 379 455.02 2 L
V
N
377 455.02 450.12 455.02 2 L
V
0.5 H
N
449.88 455.02 540.12 455.02 2 L
V
0.25 H
N
224.63 440.02 377 440.02 2 L
V
N
379 440.02 449.88 440.02 2 L
V
0.5 H
N
450.12 440.02 540.12 440.02 2 L
V
0.25 H
N
164.25 356.89 164.25 267.14 2 L
V
N
276.75 357.14 276.75 266.89 2 L
V
N
540 356.89 540 267.14 2 L
V
N
164.12 357.02 540.12 357.02 2 L
V
N
164.12 333.02 540.12 333.02 2 L
V
0.5 H
N
164.12 311.02 540.12 311.02 2 L
V
0.25 H
N
164.12 289.02 540.12 289.02 2 L
V
N
164.12 267.02 540.12 267.02 2 L
V
N
282.75 314.77 449.78 328.03 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 9 Q
0 X
0 0 0 1 0 0 0 K
(1) 283.53 319.02 T
(.) 288.03 319.02 T
(5) 290.28 319.02 T
(6) 294.78 319.02 T
(1) 308.85 319.02 T
(.) 313.35 319.02 T
(0) 315.6 319.02 T
(4) 320.1 319.02 T
(8) 324.6 319.02 T
8 F
(x) 329.63 319.02 T
5 F
(1) 343.2 319.02 T
(.) 347.7 319.02 T
(0) 349.95 319.02 T
(1) 354.45 319.02 T
8 F
(x) 375.67 319.02 T
5 F
(4) 388.66 319.02 T
(.) 393.16 319.02 T
(6) 395.41 319.02 T
(0) 399.91 319.02 T
(\320) 381.91 319.02 T
6 F
(\050) 371.81 319.02 T
(\051) 404.82 319.02 T
5 7 Q
(2) 409.77 321.78 T
5 9 Q
(0) 422.84 319.02 T
(.) 427.34 319.02 T
(2) 429.59 319.02 T
(8) 434.09 319.02 T
(0) 438.59 319.02 T
(+) 415.52 319.02 T
6 F
([) 366.45 319.02 T
(]) 443.5 319.02 T
(\244) 361.2 319.02 T
5 F
(+) 301.53 319.02 T
(+) 335.88 319.02 T
0 0 612 792 C
282.75 292.77 449.78 306.03 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 9 Q
0 X
0 0 0 1 0 0 0 K
(2) 283.53 297.02 T
(.) 288.03 297.02 T
(2) 290.28 297.02 T
(9) 294.78 297.02 T
(0) 308.85 297.02 T
(.) 313.35 297.02 T
(8) 315.6 297.02 T
(4) 320.1 297.02 T
(8) 324.6 297.02 T
8 F
(x) 329.63 297.02 T
5 F
(1) 343.2 297.02 T
(.) 347.7 297.02 T
(0) 349.95 297.02 T
(1) 354.45 297.02 T
8 F
(x) 375.67 297.02 T
5 F
(4) 388.66 297.02 T
(.) 393.16 297.02 T
(6) 395.41 297.02 T
(0) 399.91 297.02 T
(\320) 381.91 297.02 T
6 F
(\050) 371.81 297.02 T
(\051) 404.82 297.02 T
5 7 Q
(2) 409.77 299.78 T
5 9 Q
(0) 422.84 297.02 T
(.) 427.34 297.02 T
(2) 429.59 297.02 T
(8) 434.09 297.02 T
(0) 438.59 297.02 T
(+) 415.52 297.02 T
6 F
([) 366.45 297.02 T
(]) 443.5 297.02 T
(\244) 361.2 297.02 T
5 F
(+) 301.53 297.02 T
(+) 335.88 297.02 T
0 0 612 792 C
282.75 270.77 377.63 284.03 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
5 9 Q
0 X
0 0 0 1 0 0 0 K
(1) 283.53 275.02 T
(6) 288.03 275.02 T
(.) 292.53 275.02 T
(1) 294.78 275.02 T
(7) 299.28 275.02 T
(3) 312.78 275.02 T
(.) 317.28 275.02 T
(2) 319.53 275.02 T
(0) 324.03 275.02 T
8 F
(x) 329.06 275.02 T
5 F
(\320) 306.03 275.02 T
(0) 342.62 275.02 T
(.) 347.12 275.02 T
(2) 349.37 275.02 T
(9) 353.87 275.02 T
(7) 358.37 275.02 T
(5) 362.87 275.02 T
8 F
(x) 367.9 275.02 T
5 7 Q
(2) 372.35 277.78 T
5 9 Q
(+) 335.3 275.02 T
0 0 612 792 C
FMENDPAGE
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FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(94) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 671.02 540 674.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 672.52 540 672.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 672.52 180 672.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(8.6) 163.32 678.02 T
(Instrumental Properties) 189 678.02 T
0 10 Q
(8.6.1) 157.76 644.35 T
(The Point Spread Function) 189 644.35 T
5 F
0.71 (The illustration below shows the PSF for the GHRS after the installation of the COS-) 189 624.35 P
0.24 (T) 189 612.35 P
0.24 (AR mirrors, to allow for estimation of the degree of scattered light in the vicinity of a) 194.31 612.35 P
0.95 (bright object. Note that this PSF is only one-dimensional, and was only measured on) 189 600.35 P
0.59 (one side of the center of the aperture at that; in fact the true PSF has two-dimensional) 189 588.35 P
0.34 (structure. The relative throughput of the SSA at the wavelength at which this measure-) 189 576.35 P
(ment was done \0501450 \201\051 is 0.55.) 189 564.35 T
0 F
1.79 (Figure 8-7.) 126 228.33 P
3 F
1.79 (Normalized Point Spread Function for the GHRS. The upper) 187.49 228.33 P
0.36 (curve is for the LSA and the lower for the SSA, both normalized to 1.0 at the) 126 216.33 P
(origin.) 126 204.33 T
54 87.98 540 686.02 C
54 244 540 546.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
270 35 25 549 744 287.83 402.63 153.08 193.69 FMBEGINEPSF
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1514 125 r 1520 128 d 1526 134 d 1529 143 d 1529 149 d 1526 158 d
1520 164 d 1514 167 d 1505 167 d 1499 164 d 1493 158 d 1490 149 d
1490 143 d 1493 134 d 1499 128 d 1505 125 d 1514 125 d 1439 125 r
1439 173 d 1442 182 d 1445 185 d 1451 188 d 1460 188 d 1466 185 d
1439 134 r 1445 128 d 1451 125 d 1460 125 d 1466 128 d 1472 134 d
1475 143 d 1475 149 d 1472 158 d 1466 164 d 1460 167 d 1451 167 d
1445 164 d 1439 158 d 1370 125 r 1370 167 d 1370 143 r 1367 134 d
1361 128 d 1355 125 d 1346 125 d 1331 143 r 1295 143 d 1295 137 d
1298 131 d 1301 128 d 1307 125 d 1316 125 d 1322 128 d 1328 134 d
1331 143 d 1331 149 d 1328 158 d 1322 164 d 1316 167 d 1307 167 d
1301 164 d 1295 158 d 1274 104 r 1274 167 d 1217 125 r 1217 167 d
1217 134 r 1223 128 d 1229 125 d 1238 125 d 1244 128 d 1250 134 d
1253 143 d 1253 149 d 1250 158 d 1244 164 d 1238 167 d 1229 167 d
1223 164 d 1217 158 d 1193 104 r 1193 155 d 1190 164 d 1184 167 d
1178 167 d 1202 125 r 1181 125 d 1169 104 r 1166 107 d 1163 104 d
1166 101 d 1169 104 d 1166 125 r 1166 167 d 1148 125 r 1130 167 d
1112 125 r 1130 167 d 1097 143 r 1061 143 d 1061 137 d 1064 131 d
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1061 158 d 995 104 r 992 107 d 989 104 d 992 101 d 995 104 d
992 125 r 992 167 d 968 125 r 968 167 d 968 137 r 959 128 d
953 125 d 944 125 d 938 128 d 935 137 d 935 167 d 911 104 r
911 155 d 908 164 d 902 167 d 896 167 d 920 125 r 899 125 d
887 143 r 851 143 d 851 137 d 854 131 d 857 128 d 863 125 d
872 125 d 878 128 d 884 134 d 887 143 d 887 149 d 884 158 d
878 164 d 872 167 d 863 167 d 857 164 d 851 158 d 830 125 r
830 167 d 830 137 r 821 128 d 815 125 d 806 125 d 800 128 d
797 137 d 797 167 d 746 134 r 749 128 d 758 125 d 767 125 d
776 128 d 779 134 d 776 140 d 770 143 d 755 146 d 749 149 d
746 155 d 746 158 d 749 164 d 758 167 d 767 167 d 776 164 d
779 158 d 731 104 r 728 107 d 725 104 d 728 101 d 731 104 d
728 125 r 728 167 d 701 104 r 701 155 d 698 164 d 692 167 d
686 167 d 710 125 r 689 125 d 680 125 r 662 167 d 644 125 r
662 167 d 668 179 d 674 185 d 680 188 d 683 188 d 201 505 r
201 500 d 200 507 r 200 500 d 199 510 r 199 500 d 198 511 r
198 500 d 197 512 r 197 500 d 196 513 r 196 500 d 195 514 r
195 500 d 194 515 r 194 500 d 193 516 r 193 500 d 192 516 r
192 500 d 191 516 r 191 500 d 190 517 r 190 500 d 189 517 r
189 500 d 188 517 r 188 500 d 187 518 r 187 500 d 186 518 r
186 500 d 185 518 r 185 500 d 184 518 r 184 500 d 183 518 r
183 500 d 182 517 r 182 500 d 181 517 r 181 500 d 180 517 r
180 500 d 179 517 r 179 500 d 178 517 r 178 500 d 177 516 r
177 500 d 176 516 r 176 500 d 175 515 r 175 500 d 174 515 r
174 500 d 173 514 r 173 500 d 172 513 r 172 500 d 171 512 r
171 500 d 170 511 r 170 500 d 169 509 r 169 500 d 168 508 r
168 500 d 167 505 r 167 500 d 166 500 p 588 811 r 588 801 d
587 813 r 587 799 d 586 816 r 586 796 d 585 817 r 585 795 d
584 818 r 584 794 d 583 819 r 583 793 d 582 820 r 582 792 d
581 821 r 581 791 d 580 822 r 580 790 d 579 822 r 579 790 d
578 822 r 578 790 d 577 823 r 577 789 d 576 823 r 576 789 d
575 823 r 575 789 d 574 824 r 574 788 d 573 824 r 573 788 d
572 824 r 572 788 d 571 824 r 571 788 d 570 824 r 570 788 d
569 823 r 569 789 d 568 823 r 568 789 d 567 823 r 567 789 d
566 823 r 566 789 d 565 823 r 565 789 d 564 822 r 564 790 d
563 822 r 563 790 d 562 821 r 562 791 d 561 821 r 561 791 d
560 820 r 560 792 d 559 819 r 559 793 d 558 818 r 558 794 d
557 817 r 557 795 d 556 815 r 556 797 d 555 814 r 555 798 d
554 811 r 554 801 d 553 806 p 1088 1117 r 1088 1107 d 1087 1119 r
1087 1105 d 1086 1122 r 1086 1102 d 1085 1123 r 1085 1101 d 1084 1124 r
1084 1100 d 1083 1125 r 1083 1099 d 1082 1126 r 1082 1098 d 1081 1127 r
1081 1097 d 1080 1128 r 1080 1096 d 1079 1128 r 1079 1096 d 1078 1128 r
1078 1096 d 1077 1129 r 1077 1095 d 1076 1129 r 1076 1095 d 1075 1129 r
1075 1095 d 1074 1130 r 1074 1094 d 1073 1130 r 1073 1094 d 1072 1130 r
1072 1094 d 1071 1130 r 1071 1094 d 1070 1130 r 1070 1094 d 1069 1129 r
1069 1095 d 1068 1129 r 1068 1095 d 1067 1129 r 1067 1095 d 1066 1129 r
1066 1095 d 1065 1129 r 1065 1095 d 1064 1128 r 1064 1096 d 1063 1128 r
1063 1096 d 1062 1127 r 1062 1097 d 1061 1127 r 1061 1097 d 1060 1126 r
1060 1098 d 1059 1125 r 1059 1099 d 1058 1124 r 1058 1100 d 1057 1123 r
1057 1101 d 1056 1121 r 1056 1103 d 1055 1120 r 1055 1104 d 1054 1117 r
1054 1107 d 1053 1112 p 1425 1729 r 1425 1719 d 1424 1731 r 1424 1717 d
1423 1734 r 1423 1714 d 1422 1735 r 1422 1713 d 1421 1736 r 1421 1712 d
1420 1737 r 1420 1711 d 1419 1738 r 1419 1710 d 1418 1739 r 1418 1709 d
1417 1740 r 1417 1708 d 1416 1740 r 1416 1708 d 1415 1740 r 1415 1708 d
1414 1741 r 1414 1707 d 1413 1741 r 1413 1707 d 1412 1741 r 1412 1707 d
1411 1742 r 1411 1706 d 1410 1742 r 1410 1706 d 1409 1742 r 1409 1706 d
1408 1742 r 1408 1706 d 1407 1742 r 1407 1706 d 1406 1741 r 1406 1707 d
1405 1741 r 1405 1707 d 1404 1741 r 1404 1707 d 1403 1741 r 1403 1707 d
1402 1741 r 1402 1707 d 1401 1740 r 1401 1708 d 1400 1740 r 1400 1708 d
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1396 1737 r 1396 1711 d 1395 1736 r 1395 1712 d 1394 1735 r 1394 1713 d
1393 1733 r 1393 1715 d 1392 1732 r 1392 1716 d 1391 1729 r 1391 1719 d
1390 1724 p 1650 2952 r 1650 2942 d 1649 2954 r 1649 2940 d 1648 2957 r
1648 2937 d 1647 2958 r 1647 2936 d 1646 2959 r 1646 2935 d 1645 2960 r
1645 2934 d 1644 2961 r 1644 2933 d 1643 2962 r 1643 2932 d 1642 2963 r
1642 2931 d 1641 2963 r 1641 2931 d 1640 2963 r 1640 2931 d 1639 2964 r
1639 2930 d 1638 2964 r 1638 2930 d 1637 2964 r 1637 2930 d 1636 2965 r
1636 2929 d 1635 2965 r 1635 2929 d 1634 2965 r 1634 2929 d 1633 2965 r
1633 2929 d 1632 2965 r 1632 2929 d 1631 2964 r 1631 2930 d 1630 2964 r
1630 2930 d 1629 2964 r 1629 2930 d 1628 2964 r 1628 2930 d 1627 2964 r
1627 2930 d 1626 2963 r 1626 2931 d 1625 2963 r 1625 2931 d 1624 2962 r
1624 2932 d 1623 2962 r 1623 2932 d 1622 2961 r 1622 2933 d 1621 2960 r
1621 2934 d 1620 2959 r 1620 2935 d 1619 2958 r 1619 2936 d 1618 2956 r
1618 2938 d 1617 2955 r 1617 2939 d 1616 2952 r 1616 2942 d 1615 2947 p
184 500 r 571 806 d 1071 1112 d 1408 1724 d 1633 2947 d 197 513 r
171 513 d 171 500 d 197 500 r 197 513 d 714 574 r 688 574 d
688 548 d 714 548 d 714 574 d 865 635 r 839 635 d 839 609 d
865 609 d 865 635 d 1244 758 r 1218 758 d 1218 732 d 1244 732 d
1244 758 d 1558 1002 r 1532 1002 d 1532 976 d 1558 976 d 1558 1002 d
2032 1492 r 2006 1492 d 2006 1466 d 2032 1466 d 2032 1492 d 184 500 r
701 561 d 852 622 d 1231 745 d 1545 989 d 2019 1479 d
e
%%Trailer
EndPSPlot

%%EndDocument
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FMENDPAGE
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612 792 0 FMBEGINPAGE
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[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
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7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (95) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Reference T) 207 736.18 T
(ables for Instrument Performance) 257.85 736.18 T
0 10 Q
(8.6.2) 157.76 679.35 T
(Detector Dark Count and the CENSOR Option) 189 679.35 T
5 F
-0.24 (Each Digicon diode has its own discriminator) 189 659.35 P
-0.24 (, and if they are properly set the dark count) 369.94 659.35 P
0.3 (rate measured is very low) 189 647.35 P
0.3 (. On-orbit measurement has shown that both GHRS detectors) 292.32 647.35 P
0.61 (have a dark rate less than the design goal of 0.01 counts diode) 189 635.35 P
5 8 Q
0.48 (-1) 444.27 639.35 P
5 10 Q
0.61 ( sec) 450.93 635.35 P
5 8 Q
0.48 (-1) 466.81 639.35 P
5 10 Q
0.61 ( at low geomag-) 473.47 635.35 P
0.19 (netic latitudes and that the dominant noise source is cosmic rays. During SAA passage,) 189 623.35 P
0.53 (the noise increases to a maximum of about 1 count diode) 189 611.35 P
5 8 Q
0.43 (-1) 422.07 615.35 P
5 10 Q
0.53 ( sec) 428.73 611.35 P
5 8 Q
0.43 (-1) 444.53 615.35 P
5 10 Q
0.53 (. The scheduling soft-) 451.2 611.35 P
0.63 (ware for) 189 599.35 P
8 F
0.63 (HST) 226.35 599.35 P
5 F
0.63 ( uses known contours of the SAA and does not accumulate counts when) 244.13 599.35 P
(the spacecraft is within those contours.) 189 587.35 T
1.08 (Even outside the SAA, observations show that \322dark\323 counts tend to come in bursts.) 189 567.35 P
-0.06 (Approximately 15% of dark counts are produced by events that occur within a time of) 189 555.35 P
-0.06 (8) 535 555.35 P
6 F
0.48 (m) 189 543.35 P
5 F
0.48 (s or less. The) 194.76 543.35 P
9 F
1.15 ( CENSOR) 248.97 543.35 P
5 F
0.48 ( feature in Accumulation Mode allows you to ignore integra-) 292.12 543.35 P
1.09 (tions with such high dark rates.) 189 531.35 P
9 F
2.62 (CENSOR) 323.05 531.35 P
5 F
1.09 ( works by summing all 512 channels of the) 359.05 531.35 P
0.3 (Digicon every 8) 189 519.35 P
6 F
0.3 (m) 256.83 519.35 P
5 F
0.3 (s, and if that sum exceeds a threshold a coincident event is recorded.) 262.59 519.35 P
-0.05 (The \337ight software maintains a record of how many coincidence events occurred within) 189 507.35 P
-0.16 (a given) 189 495.35 P
9 F
-0.38 (STEP-TIME) 220.34 495.35 P
5 F
-0.16 ( and can reject and repeat a subexposure for which the coincidence) 274.34 495.35 P
0.38 (sum exceeds a speci\336ed level. The coincidence circuit reacts only to strong events that) 189 483.35 P
1.69 (trigger about 8 diodes simultaneously) 189 471.35 P
1.69 (, so that only the high-amplitude tail of back-) 345.66 471.35 P
1.1 (ground events can be rejected, even if the speci\336cation is to reject any) 189 459.35 P
9 F
2.64 (STEP-TIME) 486 459.35 P
5 F
1.06 (with a non-zero coincidence sum. It is estimated that use of) 189 447.35 P
9 F
2.54 (CENSOR) 440.58 447.35 P
5 F
1.06 ( can reduce the) 476.58 447.35 P
0.29 (dark count rate by about 20%. Using) 189 435.35 P
9 F
0.71 (CENSOR=YES) 340.48 435.35 P
5 F
0.29 ( is unlikely to degrade an observa-) 400.48 435.35 P
0.33 (tion \050unless the object is bright enough to cause a consistently high count rate\051, but the) 189 423.35 P
(bene\336t is also low: only about a 10% gain in S/N in favorable cases.) 189 411.35 T
0.19 (The dark count rate is highly uniform over the diodes, so that a mean dark count rate is) 189 391.35 P
(an excellent representation of what happens at the detector) 189 379.35 T
(.) 422.83 379.35 T
(Summary:) 189 359.35 T
10 11 Q
(\245) 189 341.35 T
5 10 Q
0.73 (The pre-\337ight noise speci\336cation was 0.01 counts diode) 203.4 341.35 P
5 8 Q
0.59 (-1) 431.84 345.35 P
5 10 Q
0.73 ( sec) 438.5 341.35 P
5 8 Q
0.59 (-1) 454.51 345.35 P
5 10 Q
0.73 (. The average mea-) 461.17 341.35 P
(sured value is 0.005 for D1 and 0.008 for D2.) 203.4 329.35 T
10 11 Q
(\245) 189 314.35 T
5 10 Q
(The background is sensibly constant between \32020 and +20) 203.4 314.35 T
5 8 Q
(o) 437.34 318.35 T
5 10 Q
( geomagnetic latitude.) 441.34 314.35 T
10 11 Q
(\245) 189 299.35 T
5 10 Q
-0.17 (At) 203.4 299.35 P
6 F
-0.17 (\261) 215.73 299.35 P
5 F
-0.17 (40) 221.22 299.35 P
5 8 Q
-0.14 (o) 231.22 303.35 P
5 10 Q
-0.17 ( geomagnetic latitude, the extrema of) 235.22 299.35 P
8 F
-0.17 (HST) 385.55 299.35 P
5 F
-0.17 (\325) 403.33 299.35 P
-0.17 (s orbit, the rate is twice that at the) 406.11 299.35 P
0.9 (geomagnetic equator) 203.4 287.35 P
0.9 (. T) 287.34 287.35 P
0.9 (ypical average rates are 0.007 counts per diode per second) 298.65 287.35 P
(for D1 and 0.01) 203.4 275.35 T
(1 for D2.) 266.35 275.35 T
10 11 Q
(\245) 189 260.35 T
5 10 Q
-0.09 (The background rate is correlated with the cosmic ray and trapped particle \337ux. Cal-) 203.4 260.35 P
0.05 (culations show that the dark noise can be accounted for by cosmic-ray-induced Cer-) 203.4 248.35 P
(enkov radiation in the faceplates of the Digicons.) 203.4 236.35 T
10 11 Q
(\245) 189 221.35 T
5 10 Q
0.16 (The background due to the direct penetration of cosmic rays into diodes is very low) 203.4 221.35 P
(\0500.0004 counts diode) 203.4 209.35 T
5 8 Q
(-1) 287.56 213.35 T
5 10 Q
( sec) 294.22 209.35 T
5 8 Q
(-1) 309.49 213.35 T
5 10 Q
(\051.) 316.16 209.35 T
(When using) 189 189.35 T
9 F
(CENSOR) 239.55 189.35 T
5 F
(:) 275.55 189.35 T
10 11 Q
(\245) 189 171.35 T
5 10 Q
(Use the default) 203.4 171.35 T
9 F
(STEP-TIME) 266.44 171.35 T
5 F
(of 0.2 sec.) 326.44 171.35 T
10 11 Q
(\245) 189 156.35 T
5 10 Q
0.05 (Do not use) 203.4 156.35 P
9 F
0.12 (CENSOR) 249.37 156.35 P
5 F
0.05 ( if the expected count rate exceeds about 100 counts per second) 285.37 156.35 P
0.54 (per diode because real photon events will be rejected. In a severe case, all the data) 203.4 144.35 P
(could be lost.) 203.4 132.35 T
10 11 Q
(\245) 189 117.35 T
5 10 Q
1.06 (Using) 203.4 117.35 P
9 F
2.54 (CENSOR) 230.85 117.35 P
5 F
1.06 ( can drop the noise level by about 20%. The nominal Side 2 dark) 266.85 117.35 P
0.9 (count rate is 0.01) 203.4 105.35 P
0.9 (1 counts per second per diode, so) 274.6 105.35 P
9 F
2.15 (CENSOR=YES) 416.42 105.35 P
5 F
0.9 ( can lower it to) 476.42 105.35 P
(0.0088.) 203.4 93.35 T
FMENDPAGE
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
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FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
54 750.02 540 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
0 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(96) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
54 726.98 540 726.98 2 L
0 Z
N
54 74.02 540 74.02 2 L
2 Z
N
10 11 Q
(\245) 189 679.35 T
5 10 Q
-0.01 (The following table shows the expected ef) 203.4 679.35 P
-0.01 (fects of using) 372.58 679.35 P
9 F
-0.02 (CENSOR) 428.93 679.35 P
5 F
-0.01 (.) 464.93 679.35 P
3 F
-0.01 (Rate) 469.92 679.35 P
5 F
-0.01 ( is the tar) 491.05 679.35 P
-0.01 (get) 527.78 679.35 P
0.2 (count rate per diode per second; the second column shows the standard S/N and the) 203.4 667.35 P
1.19 (third column lists the S/N achieved with) 203.4 655.35 P
9 F
2.85 (CENSOR=YES) 375.32 655.35 P
5 F
1.19 ( if the dark is 80% of its) 435.32 655.35 P
1.1 (value without) 203.4 643.35 P
9 F
2.63 (CENSOR) 262.81 643.35 P
5 F
1.1 (. Signal-to-noise was calculated on a per diode basis for a) 298.81 643.35 P
0.37 (nominal exposure time of 10,000 seconds \050which is reduced to 9,800 if) 203.4 415.35 P
9 F
0.89 (CENSOR) 494.46 415.35 P
5 F
0.37 ( is) 530.46 415.35 P
(used because of the loss of 2% of the exposures\051.) 203.4 403.35 T
-0.1 (Note that for rates exceeding one per second the ef) 203.4 388.35 P
-0.1 (fective loss of exposure time \050due) 405.27 388.35 P
0.15 (to 2% of the exposures being rejected\051 more than of) 203.4 376.35 P
0.15 (fsets any reduction of the noise.) 412.04 376.35 P
0.41 (At a rate of 0.1) 203.4 364.35 P
9 F
0.98 (CENSOR) 268.21 364.35 P
5 F
0.41 ( has essentially no ef) 304.21 364.35 P
0.41 (fect on S/N but for lower rates) 388.99 364.35 P
9 F
0.98 (CEN-) 516 364.35 P
(SOR) 203.4 352.35 T
5 F
( can help.) 221.4 352.35 T
54 615.02 540 628.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 622.02 540 622.02 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 622.02 180 622.02 2 L
0 Z
N
0 0 612 792 C
0 9 Q
0 X
0 0 0 1 0 0 0 K
(T) 54 609.02 T
(ABLE 8-8) 58.83 609.02 T
3 F
(Ef) 189 609.02 T
(fects of CENSOR) 197.34 609.02 T
(Rate) 249.25 586.02 T
(Standard S/N) 335.24 586.02 T
(S/N with CENSOR=YES) 428.11 586.02 T
5 F
(100) 252 565.02 T
(999.94) 349.88 565.02 T
(989.91) 464.62 565.02 T
(10) 254.25 546.02 T
(316.05) 349.88 546.02 T
(312.91) 464.62 546.02 T
(1) 256.5 527.02 T
(99.45) 352.12 527.02 T
(98.56) 466.88 527.02 T
(0.1) 253.12 508.02 T
(30.02) 352.12 508.02 T
(30.01) 466.88 508.02 T
(0.01) 250.88 489.02 T
(6.90) 354.38 489.02 T
(7.22) 469.12 489.02 T
(0.005) 248.62 470.02 T
(3.95) 354.38 470.02 T
(4.21) 469.12 470.02 T
(0.001) 248.62 451.02 T
(0.91) 354.38 451.02 T
(1.00) 469.12 451.02 T
207 599.89 207 444.14 2 L
V
0.25 H
0 Z
N
310.5 600.14 310.5 443.89 2 L
V
N
414 600.14 414 443.89 2 L
V
N
540 599.89 540 444.14 2 L
V
N
206.88 600.02 540.12 600.02 2 L
V
N
206.88 577.02 540.12 577.02 2 L
V
0.5 H
N
206.88 558.02 540.12 558.02 2 L
V
0.25 H
N
206.88 539.02 540.12 539.02 2 L
V
N
206.88 520.02 540.12 520.02 2 L
V
N
206.88 501.02 540.12 501.02 2 L
V
N
206.88 482.02 540.12 482.02 2 L
V
N
206.88 463.02 540.12 463.02 2 L
V
N
206.88 444.02 540.12 444.02 2 L
V
N
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612 792 0 FMBEGINPAGE
[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
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[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
72 750.02 558 750.02 2 L
2 H
0 Z
0 X
0 0 0 1 0 0 0 K
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (97) 546.88 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(Reference T) 207 736.18 T
(ables for Instrument Performance) 257.85 736.18 T
0 10 Q
(8.6.3) 157.76 679.35 T
(Noise Rejection with FL) 189 679.35 T
(YLIM) 300.88 679.35 T
9 F
1.19 (FLYLIM) 189 659.35 P
5 F
0.5 ( is a special commanding option for rejecting noise in cases where the source) 225 659.35 P
0.52 (signal is much weaker than the noise level. The idea is that as) 189 647.35 P
8 F
0.52 (HST) 444.6 647.35 P
5 F
0.52 ( circles the Earth it) 462.38 647.35 P
0.31 (\336nds itself in dif) 189 635.35 P
0.31 (ferent noise environments due to the changing magnetic \336eld, and that) 255.58 635.35 P
-0.08 (in\337uences the detected noise background. Also, the background noise occurs as discrete) 189 623.35 P
0.37 (events from radiation in the space environment. If the source count level is well below) 189 611.35 P
0.17 (the background noise, then spectra integrated over a suf) 189 599.35 P
0.17 (\336ciently short interval that con-) 413.21 599.35 P
1.25 (tain multiple counts are probably just noise, and should be rejected, whereas spectra) 189 587.35 P
0.43 (with single counts are more likely to contain real information. The rejected spectra are) 189 575.35 P
-0.22 (discarded, which wastes observing time, but there is a net gain in signal-to-noise. A test-) 189 563.35 P
-0.06 (in-principle run in 1993 showed that the net background rate could be reduced to as low) 189 551.35 P
2.3 (as 0.002 counts sec) 189 539.35 P
5 8 Q
1.84 (-1) 273.12 543.35 P
5 10 Q
2.3 ( diode) 279.78 539.35 P
5 8 Q
1.84 (-1) 306.8 543.35 P
5 10 Q
2.3 ( for the Side 2 detector) 313.47 539.35 P
2.3 (, which was a factor of four) 415.95 539.35 P
0.29 (improvement over the mean dark rate. This gain was achieved at the cost of the loss of) 189 527.35 P
(about 25% of the individual 0.2 second) 189 515.35 T
9 F
(STEP-TIME) 348.43 515.35 T
5 F
( integrations.) 402.43 515.35 T
1.26 (By \322special commanding\323 we mean that) 189 495.35 P
9 F
3.04 (FLYLIM) 360.45 495.35 P
5 F
1.26 ( is requested as a comment on the) 396.45 495.35 P
0.55 (Phase) 189 483.35 P
0.55 (II proposal, rather than as an optional parameter) 214.83 483.35 P
0.55 (. The normal scheduling system) 410.31 483.35 P
1.93 (cannot automatically invoke) 189 471.35 P
9 F
4.63 (FLYLIM) 310.61 471.35 P
5 F
1.93 (; manual intervention is necessary) 346.61 471.35 P
1.93 (. A detailed) 489.76 471.35 P
0.14 (description of) 189 459.35 P
9 F
0.34 (FLYLIM) 247.05 459.35 P
5 F
0.14 ( cannot be provided here, but if users believe that) 283.05 459.35 P
9 F
0.34 (FLYLIM) 484.14 459.35 P
5 F
0.14 ( may) 520.14 459.35 P
(be of help in their science program they should note the following:) 189 447.35 T
10 11 Q
(\245) 189 429.35 T
5 10 Q
0.28 (The use of the) 203.4 429.35 P
9 F
0.68 (FLYLIM) 263.97 429.35 P
5 F
0.28 ( parameter may not be assumed by the proposer but instead) 299.97 429.35 P
-0.13 (must be arranged in advance, i.e., before the Phase I proposal deadline, through con-) 203.4 417.35 P
1.89 (sultation with a GHRS Instrument Scientist. The T) 203.4 405.35 P
1.89 (AC will be made aware that) 418.62 405.35 P
9 F
(FLYLIM) 203.4 393.35 T
5 F
( may require additional resources to implement.) 239.4 393.35 T
10 11 Q
(\245) 189 378.35 T
5 10 Q
0.67 (If your program that uses) 203.4 378.35 P
9 F
1.61 (FLYLIM) 310.35 378.35 P
5 F
0.67 ( is approved, we will attempt to execute it on a) 346.35 378.35 P
(best ef) 203.4 366.35 T
(forts basis, but limited resources may prevent that.) 229.6 366.35 T
10 11 Q
(\245) 189 351.35 T
5 10 Q
1.07 (At the time this is written) 203.4 351.35 P
9 F
2.56 (FLYLIM) 314.24 351.35 P
5 F
1.07 ( has not been fully tested and its use is at the) 350.24 351.35 P
(observer) 203.4 339.35 T
(\325) 238.2 339.35 T
(s risk.) 240.98 339.35 T
FMENDPAGE
%%EndPage: "97" 17
%%Page: "98" 18
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(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
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(GHRS Instrument Handbook 5.0) 189 60.29 T
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54 726.98 540 726.98 2 L
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(8.6.4) 157.76 679.35 T
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0.35 (Deviations from linearity in the way in which the Digicons count photons at high rates) 189 659.35 P
0.54 (were illustrated above in Figure) 189 647.35 P
0.54 (7-2 on page) 320.88 647.35 P
0.54 (71. The ef) 371.67 647.35 P
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0.93 (detectors has been measured to be 10.2) 189 635.35 P
6 F
0.93 (m) 354.36 635.35 P
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0.93 (s for detector D1. The same value has been) 360.11 635.35 P
0.16 (assumed to hold for D2. Deviations from linearity are imperceptible below 10) 189 623.35 P
5 8 Q
0.13 (3) 502.36 627.35 P
5 10 Q
0.16 ( and can) 506.36 623.35 P
0.88 (be corrected to an accuracy of 1% up to a measured count rate of 20,000 \050in units of) 189 611.35 P
(counts diode) 189 599.35 T
5 8 Q
(-1) 239.83 603.35 T
5 10 Q
( s) 246.49 599.35 T
5 8 Q
(-1) 252.88 603.35 T
5 10 Q
(\051.) 259.55 599.35 T
0 F
(8.6.5) 157.76 569.35 T
(Image Stability) 189 569.35 T
5 F
-0.11 (The images formed by the Digicons are vulnerable to the ef) 189 549.35 P
-0.11 (fects of the Earth\325) 426.01 549.35 P
-0.11 (s magnetic) 497.06 549.35 P
-0.18 (\336eld. Over the course of a full orbit, the amplitude of the motion is about 50 microns per) 189 537.35 P
0.61 (Gauss for D2 \050about 15 microns peak-to-peak\051 and 10 microns per Gauss for D1. The) 189 525.35 P
0.21 (50 micron motion seen in D2 corresponds to the size of a diode. This geomagnetically-) 189 513.35 P
-0.22 (induced image motion \050\322GIMP\323\051, together with thermal ef) 189 501.35 P
-0.22 (fects, is the underlying reason) 421.16 501.35 P
(for breaking up long exposures into segments of no more than about 5 minutes each.) 189 489.35 T
0 F
(8.6.6) 157.76 459.35 T
(W) 189 459.35 T
(avelength Calibrations) 198.07 459.35 T
5 F
0.13 (The GHRS has two spectrum calibration lamps, although only lamp SC2 now operates.) 189 439.35 P
1.11 (Lamp SC1 should not be speci\336ed under any circumstances. Both are platinum-neon) 189 427.35 P
0.68 (hollow cathode lamps manufactured by W) 189 415.35 P
0.68 (estinghouse, providing a rich array of emis-) 361.26 415.35 P
-0.14 (sion lines throughout the ultraviolet region that the GHRS observes. The lines are bright) 189 403.35 P
0.51 (enough so that a 30 second exposure will yield a good comparison spectrum at almost) 189 391.35 P
0.5 (any wavelength, although longer times are needed at some echelle settings. The lamps) 189 379.35 P
0.17 (are designated) 189 367.35 P
9 F
0.41 (SC1) 249.32 367.35 P
5 F
0.17 ( and) 267.32 367.35 P
9 F
0.41 (SC2) 287.09 367.35 P
5 F
0.17 ( and are selected by using) 305.09 367.35 P
9 F
0.41 (WAVE) 411.64 367.35 P
5 F
0.17 ( as the tar) 435.64 367.35 P
0.17 (get speci\336cation) 474.56 367.35 P
0.5 (with) 189 355.35 P
9 F
1.2 (SC1) 209.78 355.35 P
5 F
0.5 ( or) 227.78 355.35 P
9 F
1.2 (SC2) 242.12 355.35 P
5 F
0.5 ( as the aperture. Each lamp, in fact, has its own aperture, of) 260.12 355.35 P
0.5 (fset from) 503.12 355.35 P
-0 (the two science apertures of the GHRS. SC2 forms its spectrum at the same) 189 343.35 P
8 F
-0 (y) 493.62 343.35 P
5 F
-0 ( de\337ection) 498.06 343.35 P
0.46 (as the SSA, but displaced in) 189 331.35 P
8 F
0.46 (x) 306.46 331.35 P
5 F
0.46 ( \050the direction of dispersion\051. SC1 is nearly aligned with) 310.9 331.35 P
0.17 (the SSA in) 189 319.35 P
8 F
0.17 (x) 235.35 319.35 P
5 F
0.17 ( but dif) 239.79 319.35 P
0.17 (fers in) 268.85 319.35 P
8 F
0.17 (y) 296.96 319.35 P
5 F
0.17 ( by about 130 de\337ection steps. The lamp apertures are each) 301.4 319.35 P
1.35 (67 microns square and they form Gaussian-shaped images with FWHM = 1.1 diode) 189 307.35 P
(widths.) 189 295.35 T
0.1 (A wavelength calibration exposure made with the star in the SSA may be contaminated) 189 275.35 P
-0.04 (by the stellar spectrum. This is because the SSA has no shutter and the fact that the SC2) 189 263.35 P
0.63 (aperture is in line with the SSA. This contamination is rarely a serious problem, how-) 189 251.35 P
0.58 (ever) 189 239.35 P
0.58 (, because it is possible to subtract the stellar component. Also, such exposures are) 205.81 239.35 P
1.38 (usually used to only con\336rm the zero-point of the spectrum and not to obtain a full) 189 227.35 P
(wavelength solution.) 189 215.35 T
(For a comprehensive listing of the platinum lines, see Reader et al. \0501990\051.) 189 195.35 T
0 9 Q
(8.6.6.1) 152.48 172.02 T
(Aperture Offsets) 189 172.02 T
5 10 Q
0.02 (The light from the spectrum calibration lamps does not enter the spectrograph along the) 189 151.35 P
0.08 (same path that starlight takes. This introduces a wavelength shift that must be corrected) 189 139.35 P
-0.21 (for in solving for the wavelength solution. The data reduction software incorporates cor-) 189 127.35 P
1.28 (rections that were determined during pre-\337ight ground testing \050new values are being) 189 115.35 P
(measured in Cycle 4\051.) 189 103.35 T
FMENDPAGE
%%EndPage: "98" 18
%%Page: "99" 19
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0 0 0 1 0 0 0 K
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0 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(99) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
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54 74.02 540 74.02 2 L
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54 726.98 540 726.98 2 L
0 Z
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54 74.02 540 74.02 2 L
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(8.6.6.2) 152.48 680.02 T
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5 10 Q
0.59 (The image formed by the Digicons is also af) 189 659.35 P
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-0.04 (the GHRS, which in turn is in\337uenced by whatever electronics happen to be on or of) 189 647.35 P
-0.04 (f in) 526.43 647.35 P
0.76 (the GHRS and the other instruments. The temperature inside the GHRS can be moni-) 189 635.35 P
0.65 (tored and the image motion calibrated. This correction is also provided for in the data) 189 623.35 P
0.63 (reduction software. However) 189 611.35 P
0.63 (, this correction is applied only once to a given Exposure) 306.21 611.35 P
-0.23 (Logsheet line. W) 189 599.35 P
-0.23 (e recommend that the exposure times for individual Exposure Logsheet) 256.33 599.35 P
-0.07 (lines be kept shorter than about one hour as long as you do not encounter problems with) 189 587.35 P
(using too much on-board memory \050see Section) 189 575.35 T
(4.6 on page) 378.7 575.35 T
(47\051.) 427.58 575.35 T
0 9 Q
(8.6.6.3) 152.48 552.02 T
(Geomagnetic Effects) 189 552.02 T
5 10 Q
0.14 (As for overall image stability) 189 531.35 P
0.14 (, geomagnetic ef) 306.13 531.35 P
0.14 (fects in\337uence wavelength stability) 372.6 531.35 P
0.14 (. Long) 513.75 531.35 P
-0 (exposures should be divided into units of about 5 minutes each, the time over which the) 189 519.35 P
(wavelength scale does not change measurably) 189 507.35 T
(.) 372.47 507.35 T
FMENDPAGE
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0 9 Q
(Reference T) 189 736.18 T
(ables for Instrument Performance) 239.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
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54 74.02 540 74.02 2 L
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0 10 Q
(100) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 726.98 540 726.98 2 L
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54 74.02 540 74.02 2 L
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54 726.98 540 726.98 2 L
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% Frame ps_prolog 4.0, for use with Frame 4.0 products
% This ps_prolog file is Copyright (c) 1986-1993 Frame Technology
% Corporation. All rights reserved. This ps_prolog file may be
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% using FrameMaker, FrameBuilder and FrameViewer as long as this
% copyright notice is preserved.
%
% Frame products normally print colors as their true color on a color printer
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FrameSepCyan eq and
FrameSepIs FMcustom eq and
{ FrameCurGray } { 1 } ifelse
} {
FrameSepIs FMblack eq
{FrameCurGray 1.0 exch sub mul 1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop FrameCurGray 1.0 exch sub mul 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
graymode FMLevel1 or not {

[/Pattern [/DeviceGray]] setcolorspace
FrameCurPat setcolor
} {
graymode not FMLevel1 and {

dup 1 lt {pop FrameCurGray} if
} if
RealSetgray
} ifelse
} ifelse
} bind def
/savematrix {
orgmatrix currentmatrix pop
} bind def
/restorematrix {
orgmatrix setmatrix
} bind def
/dmatrix matrix def
/dpi 72 0 dmatrix defaultmatrix dtransform
dup mul exch dup mul add sqrt def

/freq dpi dup 72 div round dup 0 eq {pop 1} if 8 mul div def
/sangle 1 0 dmatrix defaultmatrix dtransform exch atan def
/dpiranges [ 2540 2400 1693 1270 1200 635 600 0 ] def
/CMLowFreqs [ 100.402 94.8683 89.2289 100.402 94.8683 66.9349 63.2456 47.4342 ] def
/YLowFreqs [ 95.25 90.0 84.65 95.25 90.0 70.5556 66.6667 50.0 ] def
/KLowFreqs [ 89.8026 84.8528 79.8088 89.8026 84.8528 74.8355 70.7107 53.033 ] def
/CLowAngles [ 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 ] def
/MLowAngles [ 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 ] def
/YLowTDot [ true true false true true false false false ] def
/CMHighFreqs [ 133.87 126.491 133.843 108.503 102.523 100.402 94.8683 63.2456 ] def
/YHighFreqs [ 127.0 120.0 126.975 115.455 109.091 95.25 90.0 60.0 ] def
/KHighFreqs [ 119.737 113.137 119.713 128.289 121.218 89.8026 84.8528 63.6395 ] def
/CHighAngles [ 71.5651 71.5651 71.5651 70.0169 70.0169 71.5651 71.5651 71.5651 ] def
/MHighAngles [ 18.4349 18.4349 18.4349 19.9831 19.9831 18.4349 18.4349 18.4349 ] def
/YHighTDot [ false false true false false true true false ] def
/PatFreq [ 10.5833 10.0 9.4055 10.5833 10.0 10.5833 10.0 9.375 ] def
/screenIndex {
0 1 dpiranges length 1 sub { dup dpiranges exch get 1 sub dpi le {exit} {pop} ifelse } for
} bind def
/getCyanScreen {
FMUseHighFrequencyScreens { CHighAngles CMHighFreqs} {CLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getMagentaScreen {
FMUseHighFrequencyScreens { MHighAngles CMHighFreqs } {MLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getYellowScreen {
FMUseHighFrequencyScreens { YHighTDot YHighFreqs} { YLowTDot YLowFreqs } ifelse
screenIndex dup 3 1 roll get 3 1 roll get { 3 div
{2 { 1 add 2 div 3 mul dup floor sub 2 mul 1 sub exch} repeat
FMSpotFunction } } {/FMSpotFunction load } ifelse
0.0 exch
} bind def
/getBlackScreen {
FMUseHighFrequencyScreens { KHighFreqs } { KLowFreqs } ifelse
screenIndex get 45.0 /FMSpotFunction load
} bind def
/getSpotScreen {
getBlackScreen
} bind def
/getCompositeScreen {
getBlackScreen
} bind def
/FMSetScreen
FMLevel1 { /setscreen load
}{ {
8 dict begin
/HalftoneType 1 def
/SpotFunction exch def
/Angle exch def
/Frequency exch def
/AccurateScreens FMUseAcccurateScreens def
currentdict end sethalftone
} bind } ifelse
def
/setDefaultScreen {
FMPColor {
orgrxfer cvx orggxfer cvx orgbxfer cvx orgxfer cvx setcolortransfer
}
{
orgxfer cvx settransfer
} ifelse
orgfreq organgle orgproc cvx setscreen
} bind def
/setCurrentScreen {
FrameSepIs FMnone eq {
FMUseDefaultNoSeparationScreen {
setDefaultScreen
} {
getCompositeScreen FMSetScreen
} ifelse
} {
FrameSepIs FMcustom eq {
FMUseDefaultSpotSeparationScreen {
setDefaultScreen
} {
getSpotScreen FMSetScreen
} ifelse
} {
FMUseDefaultProcessSeparationScreen {
setDefaultScreen
} {
FrameSepIs FMcyan eq {
getCyanScreen FMSetScreen
} {
FrameSepIs FMmagenta eq {
getMagentaScreen FMSetScreen
} {
FrameSepIs FMyellow eq {
getYellowScreen FMSetScreen
} {
getBlackScreen FMSetScreen
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} bind def
end
/gstring FMLOCAL
/gfile FMLOCAL
/gindex FMLOCAL
/orgrxfer FMLOCAL
/orggxfer FMLOCAL
/orgbxfer FMLOCAL
/orgxfer FMLOCAL
/orgproc FMLOCAL
/orgrproc FMLOCAL
/orggproc FMLOCAL
/orgbproc FMLOCAL
/organgle FMLOCAL
/orgrangle FMLOCAL
/orggangle FMLOCAL
/orgbangle FMLOCAL
/orgfreq FMLOCAL
/orgrfreq FMLOCAL
/orggfreq FMLOCAL
/orgbfreq FMLOCAL
/yscale FMLOCAL
/xscale FMLOCAL
/edown FMLOCAL
/manualfeed FMLOCAL
/paperheight FMLOCAL
/paperwidth FMLOCAL
/FMDOCUMENT {
array /FMfonts exch def
/#copies exch def
FrameDict begin
0 ne /manualfeed exch def
/paperheight exch def
/paperwidth exch def
0 ne /FrameNegative exch def
0 ne /edown exch def
/yscale exch def
/xscale exch def
FMLevel1 {
manualfeed {setmanualfeed} if
/FMdicttop countdictstack 1 add def
/FMoptop count def
% setpapername
% manualfeed {true} {papersize} ifelse
% {manualpapersize} {false} ifelse
% {desperatepapersize} {false} ifelse
% { (Can't select requested paper size for Frame print job!) FMFAILURE } if
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
}
{{1 dict dup /PageSize [paperwidth paperheight]put setpagedevice}stopped
{ (Can't select requested paper size for Frame print job!) FMFAILURE } if
{1 dict dup /ManualFeed manualfeed put setpagedevice } stopped pop }
ifelse

FMPColor {
currentcolorscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def
cvlit /orgbproc exch def
/orgbangle exch def
/orgbfreq exch def
cvlit /orggproc exch def
/orggangle exch def
/orggfreq exch def
cvlit /orgrproc exch def
/orgrangle exch def
/orgrfreq exch def
currentcolortransfer
FrameNegative {
1 1 4 {
pop { 1 exch sub } concatprocs 4 1 roll
} for
4 copy
setcolortransfer
} if
cvlit /orgxfer exch def
cvlit /orgbxfer exch def
cvlit /orggxfer exch def
cvlit /orgrxfer exch def
} {
currentscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def

currenttransfer
FrameNegative {
{ 1 exch sub } concatprocs
dup settransfer
} if
cvlit /orgxfer exch def
} ifelse
end
} def
/pagesave FMLOCAL
/orgmatrix FMLOCAL
/landscape FMLOCAL
/pwid FMLOCAL
/FMBEGINPAGE {
FrameDict begin
/pagesave save def
3.86 setmiterlimit
/landscape exch 0 ne def
landscape {
90 rotate 0 exch dup /pwid exch def neg translate pop
}{
pop /pwid exch def
} ifelse
edown { [-1 0 0 1 pwid 0] concat } if
0 0 moveto paperwidth 0 lineto paperwidth paperheight lineto
0 paperheight lineto 0 0 lineto 1 setgray fill
xscale yscale scale
/orgmatrix matrix def
gsave
} def
/FMENDPAGE {
grestore
pagesave restore
end
showpage
} def
/FMFONTDEFINE {
FrameDict begin
findfont
ReEncode
1 index exch
definefont
FMfonts 3 1 roll
put
end
} def
/FMFILLS {
FrameDict begin dup
array /fillvals exch def
dict /patCache exch def
end
} def
/FMFILL {
FrameDict begin
fillvals 3 1 roll put
end
} def
/FMNORMALIZEGRAPHICS {
newpath
0.0 0.0 moveto
1 setlinewidth
0 setlinecap
0 0 0 sethsbcolor
0 setgray
} bind def
/fx FMLOCAL
/fy FMLOCAL
/fh FMLOCAL
/fw FMLOCAL
/llx FMLOCAL
/lly FMLOCAL
/urx FMLOCAL
/ury FMLOCAL
/FMBEGINEPSF {
end
/FMEPSF save def
/showpage {} def
% See Adobe's "PostScript Language Reference Manual, 2nd Edition", page 714.
% "...the following operators MUST NOT be used in an EPS file:" (emphasis ours)
/banddevice {(banddevice) FMBADEPSF} def
/clear {(clear) FMBADEPSF} def
/cleardictstack {(cleardictstack) FMBADEPSF} def
/copypage {(copypage) FMBADEPSF} def
/erasepage {(erasepage) FMBADEPSF} def
/exitserver {(exitserver) FMBADEPSF} def
/framedevice {(framedevice) FMBADEPSF} def
/grestoreall {(grestoreall) FMBADEPSF} def
/initclip {(initclip) FMBADEPSF} def
/initgraphics {(initgraphics) FMBADEPSF} def
/initmatrix {(initmatrix) FMBADEPSF} def
/quit {(quit) FMBADEPSF} def
/renderbands {(renderbands) FMBADEPSF} def
/setglobal {(setglobal) FMBADEPSF} def
/setpagedevice {(setpagedevice) FMBADEPSF} def
/setshared {(setshared) FMBADEPSF} def
/startjob {(startjob) FMBADEPSF} def
/lettertray {(lettertray) FMBADEPSF} def
/letter {(letter) FMBADEPSF} def
/lettersmall {(lettersmall) FMBADEPSF} def
/11x17tray {(11x17tray) FMBADEPSF} def
/11x17 {(11x17) FMBADEPSF} def
/ledgertray {(ledgertray) FMBADEPSF} def
/ledger {(ledger) FMBADEPSF} def
/legaltray {(legaltray) FMBADEPSF} def
/legal {(legal) FMBADEPSF} def
/statementtray {(statementtray) FMBADEPSF} def
/statement {(statement) FMBADEPSF} def
/executivetray {(executivetray) FMBADEPSF} def
/executive {(executive) FMBADEPSF} def
/a3tray {(a3tray) FMBADEPSF} def
/a3 {(a3) FMBADEPSF} def
/a4tray {(a4tray) FMBADEPSF} def
/a4 {(a4) FMBADEPSF} def
/a4small {(a4small) FMBADEPSF} def
/b4tray {(b4tray) FMBADEPSF} def
/b4 {(b4) FMBADEPSF} def
/b5tray {(b5tray) FMBADEPSF} def
/b5 {(b5) FMBADEPSF} def
FMNORMALIZEGRAPHICS
[/fy /fx /fh /fw /ury /urx /lly /llx] {exch def} forall
fx fw 2 div add fy fh 2 div add translate
rotate
fw 2 div neg fh 2 div neg translate
fw urx llx sub div fh ury lly sub div scale
llx neg lly neg translate
/FMdicttop countdictstack 1 add def
/FMoptop count def
} bind def
/FMENDEPSF {
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
FMEPSF restore
FrameDict begin
} bind def
FrameDict begin
/setmanualfeed {
%%BeginFeature *ManualFeed True
statusdict /manualfeed true put
%%EndFeature
} bind def
/max {2 copy lt {exch} if pop} bind def
/min {2 copy gt {exch} if pop} bind def
/inch {72 mul} def
/pagedimen {
paperheight sub abs 16 lt exch
paperwidth sub abs 16 lt and
{/papername exch def} {pop} ifelse
} bind def
/papersizedict FMLOCAL
/setpapername {
/papersizedict 14 dict def
papersizedict begin
/papername /unknown def
/Letter 8.5 inch 11.0 inch pagedimen
/LetterSmall 7.68 inch 10.16 inch pagedimen
/Tabloid 11.0 inch 17.0 inch pagedimen
/Ledger 17.0 inch 11.0 inch pagedimen
/Legal 8.5 inch 14.0 inch pagedimen
/Statement 5.5 inch 8.5 inch pagedimen
/Executive 7.5 inch 10.0 inch pagedimen
/A3 11.69 inch 16.5 inch pagedimen
/A4 8.26 inch 11.69 inch pagedimen
/A4Small 7.47 inch 10.85 inch pagedimen
/B4 10.125 inch 14.33 inch pagedimen
/B5 7.16 inch 10.125 inch pagedimen
end
} bind def
/papersize {
papersizedict begin
/Letter {lettertray letter} def
/LetterSmall {lettertray lettersmall} def
/Tabloid {11x17tray 11x17} def
/Ledger {ledgertray ledger} def
/Legal {legaltray legal} def
/Statement {statementtray statement} def
/Executive {executivetray executive} def
/A3 {a3tray a3} def
/A4 {a4tray a4} def
/A4Small {a4tray a4small} def
/B4 {b4tray b4} def
/B5 {b5tray b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
statusdict begin stopped end
} bind def
/manualpapersize {
papersizedict begin
/Letter {letter} def
/LetterSmall {lettersmall} def
/Tabloid {11x17} def
/Ledger {ledger} def
/Legal {legal} def
/Statement {statement} def
/Executive {executive} def
/A3 {a3} def
/A4 {a4} def
/A4Small {a4small} def
/B4 {b4} def
/B5 {b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
stopped
} bind def
/desperatepapersize {
statusdict /setpageparams known
{
paperwidth paperheight 0 1
statusdict begin
{setpageparams} stopped
end
} {true} ifelse
} bind def
/DiacriticEncoding [
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /space /exclam /quotedbl
/numbersign /dollar /percent /ampersand /quotesingle /parenleft
/parenright /asterisk /plus /comma /hyphen /period /slash /zero /one
/two /three /four /five /six /seven /eight /nine /colon /semicolon
/less /equal /greater /question /at /A /B /C /D /E /F /G /H /I /J /K
/L /M /N /O /P /Q /R /S /T /U /V /W /X /Y /Z /bracketleft /backslash
/bracketright /asciicircum /underscore /grave /a /b /c /d /e /f /g /h
/i /j /k /l /m /n /o /p /q /r /s /t /u /v /w /x /y /z /braceleft /bar
/braceright /asciitilde /.notdef /Adieresis /Aring /Ccedilla /Eacute
/Ntilde /Odieresis /Udieresis /aacute /agrave /acircumflex /adieresis
/atilde /aring /ccedilla /eacute /egrave /ecircumflex /edieresis
/iacute /igrave /icircumflex /idieresis /ntilde /oacute /ograve
/ocircumflex /odieresis /otilde /uacute /ugrave /ucircumflex
/udieresis /dagger /.notdef /cent /sterling /section /bullet
/paragraph /germandbls /registered /copyright /trademark /acute
/dieresis /.notdef /AE /Oslash /.notdef /.notdef /.notdef /.notdef
/yen /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/ordfeminine /ordmasculine /.notdef /ae /oslash /questiondown
/exclamdown /logicalnot /.notdef /florin /.notdef /.notdef
/guillemotleft /guillemotright /ellipsis /.notdef /Agrave /Atilde
/Otilde /OE /oe /endash /emdash /quotedblleft /quotedblright
/quoteleft /quoteright /.notdef /.notdef /ydieresis /Ydieresis
/fraction /currency /guilsinglleft /guilsinglright /fi /fl /daggerdbl
/periodcentered /quotesinglbase /quotedblbase /perthousand
/Acircumflex /Ecircumflex /Aacute /Edieresis /Egrave /Iacute
/Icircumflex /Idieresis /Igrave /Oacute /Ocircumflex /.notdef /Ograve
/Uacute /Ucircumflex /Ugrave /dotlessi /circumflex /tilde /macron
/breve /dotaccent /ring /cedilla /hungarumlaut /ogonek /caron
] def
/ReEncode {
dup
length
dict begin
{
1 index /FID ne
{def}
{pop pop} ifelse
} forall
0 eq {/Encoding DiacriticEncoding def} if
currentdict
end
} bind def
FMPColor

{
/BEGINBITMAPCOLOR {
BITMAPCOLOR} def
/BEGINBITMAPCOLORc {
BITMAPCOLORc} def
/BEGINBITMAPTRUECOLOR {
BITMAPTRUECOLOR } def
/BEGINBITMAPTRUECOLORc {
BITMAPTRUECOLORc } def
}

{
/BEGINBITMAPCOLOR {
BITMAPGRAY} def
/BEGINBITMAPCOLORc {
BITMAPGRAYc} def
/BEGINBITMAPTRUECOLOR {
BITMAPTRUEGRAY } def
/BEGINBITMAPTRUECOLORc {
BITMAPTRUEGRAYc } def
}
ifelse
/K {
FMPrintAllColorsAsBlack {
dup 1 eq 2 index 1 eq and 3 index 1 eq and not
{7 {pop} repeat 0 0 0 1 0 0 0} if
} if
FrameCurColors astore
pop combineColor
} bind def
/graymode true def
/bwidth FMLOCAL
/bpside FMLOCAL
/bstring FMLOCAL
/onbits FMLOCAL
/offbits FMLOCAL
/xindex FMLOCAL
/yindex FMLOCAL
/x FMLOCAL
/y FMLOCAL
/setPatternMode {
FMLevel1 {
/bwidth exch def
/bpside exch def
/bstring exch def
/onbits 0 def /offbits 0 def
freq sangle landscape {90 add} if
{/y exch def
/x exch def
/xindex x 1 add 2 div bpside mul cvi def
/yindex y 1 add 2 div bpside mul cvi def
bstring yindex bwidth mul xindex 8 idiv add get
1 7 xindex 8 mod sub bitshift and 0 ne FrameNegative {not} if
{/onbits onbits 1 add def 1}
{/offbits offbits 1 add def 0}
ifelse
}
setscreen
offbits offbits onbits add div FrameNegative {1.0 exch sub} if
/FrameCurGray exch def
} {
pop pop
dup patCache exch known {
patCache exch get
} {
dup
patDict /bstring 3 -1 roll put
patDict
9 PatFreq screenIndex get div dup matrix scale
makepattern
dup
patCache 4 -1 roll 3 -1 roll put
} ifelse
/FrameCurGray 0 def
/FrameCurPat exch def
} ifelse
/graymode false def
combineColor
} bind def
/setGrayScaleMode {
graymode not {
/graymode true def
FMLevel1 {
setCurrentScreen
} if
} if
/FrameCurGray exch def
combineColor
} bind def
/normalize {
transform round exch round exch itransform
} bind def
/dnormalize {
dtransform round exch round exch idtransform
} bind def
/lnormalize {
0 dtransform exch cvi 2 idiv 2 mul 1 add exch idtransform pop
} bind def
/H {
lnormalize setlinewidth
} bind def
/Z {
setlinecap
} bind def

/PFill {
graymode FMLevel1 or not {
gsave 1 setgray eofill grestore
} if
} bind def
/PStroke {
graymode FMLevel1 or not {
gsave 1 setgray stroke grestore
} if
stroke
} bind def
/fillvals FMLOCAL
/X {
fillvals exch get
dup type /stringtype eq
{8 1 setPatternMode}
{setGrayScaleMode}
ifelse
} bind def
/V {
PFill gsave eofill grestore
} bind def
/Vclip {
clip
} bind def
/Vstrk {
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/N {
PStroke
} bind def
/Nclip {
strokepath clip newpath
} bind def
/Nstrk {
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/M {newpath moveto} bind def
/E {lineto} bind def
/D {curveto} bind def
/O {closepath} bind def
/n FMLOCAL
/L {
/n exch def
newpath
normalize
moveto
2 1 n {pop normalize lineto} for
} bind def
/Y {
L
closepath
} bind def
/x1 FMLOCAL
/x2 FMLOCAL
/y1 FMLOCAL
/y2 FMLOCAL
/R {
/y2 exch def
/x2 exch def
/y1 exch def
/x1 exch def
x1 y1
x2 y1
x2 y2
x1 y2
4 Y
} bind def
/rad FMLOCAL
/rarc
{rad
arcto
} bind def
/RR {
/rad exch def
normalize
/y2 exch def
/x2 exch def
normalize
/y1 exch def
/x1 exch def
mark
newpath
{
x1 y1 rad add moveto
x1 y2 x2 y2 rarc
x2 y2 x2 y1 rarc
x2 y1 x1 y1 rarc
x1 y1 x1 y2 rarc
closepath
} stopped {x1 y1 x2 y2 R} if
cleartomark
} bind def
/RRR {
/rad exch def
normalize /y4 exch def /x4 exch def
normalize /y3 exch def /x3 exch def
normalize /y2 exch def /x2 exch def
normalize /y1 exch def /x1 exch def
newpath
normalize moveto
mark
{
x2 y2 x3 y3 rarc
x3 y3 x4 y4 rarc
x4 y4 x1 y1 rarc
x1 y1 x2 y2 rarc
closepath
} stopped
{x1 y1 x2 y2 x3 y3 x4 y4 newpath moveto lineto lineto lineto closepath} if
cleartomark
} bind def
/C {
grestore
gsave
R
clip
setCurrentScreen
} bind def
/CP {
grestore
gsave
Y
clip
setCurrentScreen
} bind def
/FMpointsize FMLOCAL
/F {
FMfonts exch get
FMpointsize scalefont
setfont
} bind def
/Q {
/FMpointsize exch def
F
} bind def
/T {
moveto show
} bind def
/RF {
rotate
0 ne {-1 1 scale} if
} bind def
/TF {
gsave
moveto
RF
show
grestore
} bind def
/P {
moveto
0 32 3 2 roll widthshow
} bind def
/PF {
gsave
moveto
RF
0 32 3 2 roll widthshow
grestore
} bind def
/S {
moveto
0 exch ashow
} bind def
/SF {
gsave
moveto
RF
0 exch ashow
grestore
} bind def
/B {
moveto
0 32 4 2 roll 0 exch awidthshow
} bind def
/BF {
gsave
moveto
RF
0 32 4 2 roll 0 exch awidthshow
grestore
} bind def
/G {
gsave
newpath
normalize translate 0.0 0.0 moveto
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
PFill fill
grestore
} bind def
/Gstrk {
savematrix
newpath
2 index 2 div add exch 3 index 2 div sub exch
normalize 2 index 2 div sub exch 3 index 2 div add exch
translate
scale
0.0 0.0 1.0 5 3 roll arc
restorematrix
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/Gclip {
newpath
savematrix
normalize translate 0.0 0.0 moveto
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
clip newpath
restorematrix
} bind def
/GG {
gsave
newpath
normalize translate 0.0 0.0 moveto
rotate
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
PFill
fill
grestore
} bind def
/GGclip {
savematrix
newpath
normalize translate 0.0 0.0 moveto
rotate
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
clip newpath
restorematrix
} bind def
/GGstrk {
savematrix
newpath
normalize translate 0.0 0.0 moveto
rotate
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
restorematrix
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/A {
gsave
savematrix
newpath
2 index 2 div add exch 3 index 2 div sub exch
normalize 2 index 2 div sub exch 3 index 2 div add exch
translate
scale
0.0 0.0 1.0 5 3 roll arc
restorematrix
PStroke
grestore
} bind def
/Aclip {
newpath
savematrix
normalize translate 0.0 0.0 moveto
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
strokepath clip newpath
restorematrix
} bind def
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1.2 (Chapter 9) 72 677 S
2 24 Q
-0.48 (GHRS Bibliography) 207 677 S
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(9.1) 144 424 T
( Ultraviolet Extinction) 164.02 424 T
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( 102) 498.65 424 T
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(9.2) 144 406 T
( GHRS-Related T) 164.02 406 T
(echnical Papers) 256.7 406 T
4 F
( 102) 498.65 406 T
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(9.3) 144 388 T
( GHRS Scienti\336c Papers) 164.02 388 T
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( 104) 498.65 388 T
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(9.4) 144 370 T
( Acknowledgments) 164.02 370 T
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( 109) 498.65 370 T
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1.45 (W) 189 679.35 P
1.45 (e have tried to make this) 197.64 679.35 P
6 F
1.45 (Handbook) 306.86 679.35 P
5 F
1.45 ( a comprehensive guide to using the Goddard) 348.52 679.35 P
0.39 (High Resolution Spectrograph, but some of the best information on the instrument and) 189 667.35 P
-0.2 (the uses to which it can be put can be found in the open literature. Here we provide three) 189 655.35 P
0.45 (lists. The \336rst provides additional information on interstellar reddening in the ultravio-) 189 643.35 P
0.32 (let. The next is technically oriented, and gives papers that provide detailed information) 189 631.35 P
1.29 (on speci\336c aspects of the GHRS. The \336nal list is of scienti\336c papers that have used) 189 619.35 P
(GHRS data.) 189 607.35 T
54 564.02 540 567.02 C
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0 0 0 1 0 0 0 K
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54 565.52 180 565.52 2 L
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N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(9.1) 163.32 571.02 T
(Ultraviolet Extinction) 189 571.02 T
6 10 Q
1.26 (\322Ultraviolet Photometry fr) 189 547.35 P
1.26 (om the Orbiting Astr) 298.93 547.35 P
1.26 (onomical Observatory) 385.4 547.35 P
1.26 (. II. Interstellar) 475.82 547.35 P
(Extinction.\323) 198 535.35 T
3 9 Q
(Bless, R.C., and Savage, B.D. 1972, ApJ, 171, 293\320308.) 207 518.02 T
6 10 Q
-0.15 (\322Studies of Ultraviolet Interstellar Extinction with the Sky-survey T) 189 498.35 P
-0.15 (elescope of the TD-1) 457.42 498.35 P
(Satellite.\323) 198 486.35 T
3 9 Q
0.77 (Nandy) 207 469.02 P
0.77 (, K., Thompson, G.I., Jamar) 232.34 469.02 P
0.77 (, C., Mon\336ls, A., and Wilson, R. 1976, A&A, 51,) 345.48 469.02 P
(63\32069.) 216 458.02 T
6 10 Q
(\322Empirical Effective T) 189 438.35 T
(emperatur) 279.19 438.35 T
(es and Bolometric Corr) 320.48 438.35 T
(ections for Early-T) 414.83 438.35 T
(ype Stars.\323) 490.2 438.35 T
3 9 Q
0.99 (Code, A.D., Davis, J., Bless, R.C., and Hanbury Brown, R. 1976, ApJ, 203, 417\320) 207 421.02 P
(434.) 216 410.02 T
6 10 Q
(\322Interstellar Extinction in the UV\323) 189 390.35 T
3 9 Q
(Seaton, M.J. 1979, MNRAS, 187, 73P\32076P) 207 373.02 T
(.) 378.43 373.02 T
6 10 Q
(\322Observed Pr) 189 353.35 T
(operties of Interstellar Dust\323) 245.01 353.35 T
3 9 Q
(Savage, B.D., and Mathis, J.S. 1979, ARA&A, 17, 73\3201) 207 336.02 T
(12.) 426.96 336.02 T
54 293.02 540 296.02 C
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
189 294.52 540 294.52 2 L
0.25 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
54 294.52 180 294.52 2 L
0 Z
N
0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(9.2) 163.32 300.02 T
(GHRS-Related T) 189 300.02 T
(echnical Papers) 280.79 300.02 T
6 10 Q
(\322Ultraviolet High-Resolution Spectr) 189 276.35 T
(oscopy fr) 334.74 276.35 T
(om the Space T) 371.31 276.35 T
(elescope.\323) 431.77 276.35 T
3 9 Q
0.29 (Ebbets, D.C., Brandt, J.C., and the HRS Investigation De\336nition T) 207 259.02 P
0.29 (eam 1983, P) 469.71 259.02 P
0.29 (ASP) 520.65 259.02 P
0.29 (,) 537.5 259.02 P
(95, 543\320549.) 216 248.02 T
6 10 Q
0.35 (\322W) 189 228.35 P
0.35 (avelengths and Intensities of a Platinum/Neon Hollow Cathode Lamp in the Region) 201.97 228.35 P
(1) 198 215.35 T
(100\3204000 \201\323) 202.26 215.35 T
3 9 Q
1.62 (Reader) 207 198.02 P
1.62 (, J., Acquista, N., Sansonetti, C.J., and Sansonetti, J.E. 1990, ApJS, 72,) 236.02 198.02 P
(831\320866.) 216 187.02 T
6 10 Q
(\322Status of the Goddar) 189 167.35 T
(d High Resolution Spectr) 277.25 167.35 T
(ograph in May 1991.\323) 377.71 167.35 T
3 9 Q
1.28 (Ebbets, D.C., Brandt, J., Heap, S. 1991, in The First Y) 207 150.02 P
1.28 (ear of) 434.61 150.02 P
4 F
1.28 (HST) 462.69 150.02 P
3 F
1.28 ( Observations,) 480.69 150.02 P
(edited by A.L. Kinney and J.C. Blades, p. 1) 216 139.02 T
(10-122,) 386.43 139.02 T
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6 10 Q
0.93 (\322Scatter) 189 679.35 P
0.93 (ed Light in the Echelle Modes of the Goddar) 222.52 679.35 P
0.93 (d High Resolution Spectr) 407.87 679.35 P
0.93 (ograph) 511.11 679.35 P
(Aboar) 198 667.35 T
(d the) 222.63 667.35 T
5 F
(Hubble Space T) 244.85 667.35 T
(elescope) 308.58 667.35 T
6 F
(. I. Analysis of Pr) 343.01 667.35 T
(elaunch Calibration Data.\323) 412.64 667.35 T
3 9 Q
(Cardelli, J.A., Ebbets, D.C., and Savage, B.D. 1990, 365, 789\320802.) 207 650.02 T
6 10 Q
0.93 (\322Scatter) 189 630.35 P
0.93 (ed Light in the Echelle Modes of the Goddar) 222.52 630.35 P
0.93 (d High Resolution Spectr) 407.87 630.35 P
0.93 (ograph) 511.11 630.35 P
0.68 (Aboar) 198 618.35 P
0.68 (d the) 222.63 618.35 P
5 F
0.68 (Hubble Space T) 246.22 618.35 P
0.68 (elescope) 311.31 618.35 P
6 F
0.68 (. II. Analysis of In\337ight Spectr) 345.74 618.35 P
0.68 (oscopic Observa-) 469.06 618.35 P
(tions.\323) 198 606.35 T
3 9 Q
(Cardelli, J.A., Ebbets, D.C., and Savage, B.D. 1993, ApJ, 413, 401\320415.) 207 589.02 T
6 10 Q
(\322Resolution and Noise Pr) 189 569.35 T
(operties of the Goddar) 292.25 569.35 T
(d High Resolution Spectr) 382.71 569.35 T
(ograph\323) 483.17 569.35 T
3 9 Q
1 (Gilliland, R.L., Morris, S.L., W) 207 552.02 P
1 (eymann, R.J., Ebbets, D.C., and Lindler) 328.88 552.02 P
1 (, D.J. 1992,) 491.97 552.02 P
(P) 216 541.02 T
(ASP) 221.34 541.02 T
(, 104, 367\320382.) 238.18 541.02 T
5 10 Q
-0.26 (This last paper is especially recommended for its discussion of the deconvolution of) 207 523.35 P
0.4 (the ef) 207 511.35 P
0.4 (fects of the Point Spread Function \050PSF\051 and Line Spread Function \050LSF\051 of) 229.71 511.35 P
6 F
(HST) 207 499.35 T
5 F
( and the GHRS.) 224.78 499.35 T
6 F
1.29 (\322Final Report of the Science V) 189 479.35 P
1.29 (eri\336cation Pr) 317.97 479.35 P
1.29 (ogram for the Goddar) 372.5 479.35 P
1.29 (d High Resolution) 464.63 479.35 P
(Spectr) 198 467.35 T
(ograph for the Hubble Space T) 223.18 467.35 T
(elescope\323) 346.42 467.35 T
3 9 Q
0.44 (Ebbets, D.C. 1992, prepared for NASA/Goddard Space Flight Center by Ball Aero-) 207 450.02 P
(space Systems Group.) 216 439.02 T
5 10 Q
-0.11 (This is a technical document prepared by Ball to ful\336ll a contractual requirement. It) 207 421.35 P
1.01 (provides a detailed description of the tests and calibrations performed during the) 207 409.35 P
0.62 (Science V) 207 397.35 P
0.62 (eri\336cation phase that occurred immediately after the launch of) 247.33 397.35 P
6 F
0.62 (HST) 504.26 397.35 P
5 F
0.62 (. W) 521.3 397.35 P
0.62 (e) 535.56 397.35 P
0.4 (cite it here for completeness, but a General Observer should usually be able to get) 207 385.35 P
(the information that he or she needs from this) 207 373.35 T
6 F
(Handbook) 391.7 373.35 T
5 F
( or by consulting us.) 433.36 373.35 T
FMENDPAGE
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(104) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
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54 672.52 180 672.52 2 L
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0 0 612 792 C
0 12 Q
0 X
0 0 0 1 0 0 0 K
(9.3) 163.32 678.02 T
(GHRS Scienti\336c Papers) 189 678.02 T
5 10 Q
1.44 (A number of GHRS-related papers are concentrated in three special volumes whose) 189 650.35 P
(contents will not be itemized here:) 189 638.35 T
7 11 Q
(\245) 189 620.35 T
6 10 Q
(The First Y) 203.4 620.35 T
(ear of HST Observations) 247.49 620.35 T
5 F
(, 1991, edited by A.L. Kinney and J.C. Blades,) 347.21 620.35 T
(and published by STScI.) 203.4 608.35 T
7 11 Q
(\245) 189 593.35 T
6 10 Q
(Astr) 203.4 593.35 T
(ophysical Journal Letters) 219.7 593.35 T
5 F
(, volume 377, number 1, 1991.) 321.92 593.35 T
7 11 Q
(\245) 189 578.35 T
6 10 Q
(Science with the Hubble Space T) 203.4 578.35 T
(elescope) 333.85 578.35 T
5 F
(, 1992, edited by P) 368.28 578.35 T
(. Benvenuti and E.) 442.17 578.35 T
(Schreier) 203.4 566.35 T
(, and published by ESO.) 236.32 566.35 T
8 12 Q
(1992:) 162 539.02 T
6 10 Q
(\322The Abundance of Bor) 189 518.35 T
(on in Thr) 284.46 518.35 T
(ee Halo Stars\323) 321.32 518.35 T
3 9 Q
(Duncan, D.K., Lambert, D.L., and Lemke, M. 1992, ApJ, 401, 584\320595.) 207 501.02 T
6 10 Q
0.38 (\322Ultraviolet Observations of the Gas Phase Abundances in the Diffuse Clouds T) 189 481.35 P
0.38 (owar) 514.81 481.35 P
0.38 (d) 535 481.35 P
(Zeta Ophiuchi at 3.5 Kilometers per Second Resolution\323) 198 469.35 T
3 9 Q
(Savage, B.D., Cardelli, J.A., and So\336a, U.J. 1992, ApJ, 401, 706\320723.) 207 452.02 T
6 10 Q
(\322Fractionation of CO in the Diffuse Clouds T) 189 432.35 T
(owar) 371.16 432.35 T
(d Zeta Ophiuchi\323) 391.35 432.35 T
3 9 Q
0.22 (Shef) 207 415.02 P
0.22 (fer) 225.35 415.02 P
0.22 (, Y) 235.36 415.02 P
0.22 (., Federman, S.R., Lambert, D.L., and Cardelli, J.A. 1992, ApJ, 397, 482\320) 245.43 415.02 P
(491.) 216 404.02 T
6 10 Q
(\322Highly Ionized Atoms T) 189 384.35 T
(owar) 288.36 384.35 T
(d HD 93521.\323) 308.55 384.35 T
3 9 Q
(Spitzer) 207 367.02 T
(, L., and Fitzpatrick, E.L. 1992, ApJ, 391, L41\320L44.) 234.51 367.02 T
6 10 Q
1.58 (\322Ultraviolet and Optical Spectral Morphology of Melnick 42 and Radcliffe 136a in) 189 347.35 P
(30) 198 335.35 T
(Doradus\323) 210.5 335.35 T
3 9 Q
0.06 (W) 207 318.02 P
0.06 (alborn, N.R., Ebbets, D.C., Parker) 215.16 318.02 P
0.06 (, J.W) 350.47 318.02 P
0.06 (., Nichols-Bohlin, J., and White, R.L. 1992,) 370.54 318.02 P
(ApJ, 393, L13\320L16.) 216 307.02 T
6 10 Q
(\322Detection of a Pr) 189 287.35 T
(oton Beam During the Impulsive Phase of a Stellar Flar) 263.35 287.35 T
(e\323) 487.69 287.35 T
3 9 Q
1.62 (W) 207 270.02 P
1.62 (oodgate, B.E., Robinson, R.D., Carpenter) 215.33 270.02 P
1.62 (, K.G., Maran, S.P) 386.89 270.02 P
1.62 (., and Shore, S.N.) 463.61 270.02 P
(1992, ApJ, 397, L95\320-L98.) 216 259.02 T
8 12 Q
(1993:) 162 232.02 T
6 10 Q
0.12 (\322Interstellar Mg) 189 211.35 P
6 9 Q
0.11 (II) 258.13 211.35 P
6 10 Q
0.12 ( and C) 264.12 211.35 P
6 9 Q
0.11 (IV) 293.66 211.35 P
6 10 Q
0.12 ( Absorption T) 302.15 211.35 P
0.12 (owar) 356.48 211.35 P
0.12 (d Mrk 205 by NGC 4319: An \324Optically-) 376.67 211.35 P
(Thick\325 QSO Absorption System\323) 198 199.35 T
3 9 Q
(Bowen D.V) 207 182.02 T
(., and Blades, J.C. ApJ, 403, L55\320L58.) 251.19 182.02 T
6 10 Q
0.24 (\322Observations of 3C 273 with the Goddar) 189 162.35 P
0.24 (d High Resolution Spectr) 358.95 162.35 P
0.24 (ograph on the Hub-) 460.13 162.35 P
(ble Space T) 198 150.35 T
(elescope\323) 243.74 150.35 T
3 9 Q
(Brandt, J.C., et al. 1993, AJ, 105, 831\320846.) 207 133.02 T
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0 X
0 0 0 1 0 0 0 K
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72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (105) 541.32 60.29 P
72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
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72 750.02 558 750.02 2 L
2 H
0 Z
N
72 726.98 558 726.98 2 L
0.25 H
N
72 74.02 558 74.02 2 L
2 Z
N
0 9 Q
(GHRS Bibliography) 207 736.18 T
6 10 Q
(\322The Galactic Halo and Local Inter) 189 679.35 T
(galactic Medium towar) 333.35 679.35 T
(d PKS 2155\320304\323) 426.31 679.35 T
3 9 Q
0.49 (Bruweiler) 207 662.02 P
0.49 (, F) 244.01 662.02 P
0.49 (.C., Boggess, A., Norman, D.J., Grady) 254 662.02 P
0.49 (, C.A., Urry) 408.34 662.02 P
0.49 (, C.M., and Kondo, Y) 453.16 662.02 P
0.49 (.) 537.5 662.02 P
(1993, ApJ, 409, 199\320204.) 216 651.02 T
6 10 Q
0.9 (\322Ultraviolet T) 189 631.35 P
0.9 (ransitions of Low Condensation T) 246.86 631.35 P
0.9 (emperatur) 385.68 631.35 P
0.9 (e Heavy Elements and New) 426.98 631.35 P
(Data for Interstellar Arsenic, Selenium, T) 198 619.35 T
(ellurium, and Lead\323) 364.02 619.35 T
3 9 Q
0.35 (Cardelli, J.A., Federman, S.R., Lambert, D., and Theodosiou, C.E. 1993, ApJ, 416,) 207 602.02 P
(L41\320L44.) 216 591.02 T
6 10 Q
(\322Abundance of Interstellar Carbon T) 189 571.35 T
(owar) 337.53 571.35 T
(d Zeta Ophiuchi\323) 357.72 571.35 T
3 9 Q
0.86 (Cardelli, J.A., Mathis, J.S., Ebbets, D.C., and Savage, B.D. 1993, ApJ, 403, L17\320) 207 554.02 P
(L20.) 216 543.02 T
6 10 Q
(\322Detection of Bor) 189 523.35 T
(on, Cobalt, and other W) 260.85 523.35 T
(eak Interstellar Lines towar) 356.6 523.35 T
(d) 467.62 523.35 T
9 F
(z) 475.12 523.35 T
6 F
( Ophiuchi\323) 480.06 523.35 T
3 9 Q
1.14 (Federman, S.R., Shef) 207 506.02 P
1.14 (fer) 296.15 506.02 P
1.14 (, Lambert, D.L., and Gilliland, R.L. 1993, ApJ, 413, L51\320) 306.16 506.02 P
(L54.) 216 495.02 T
6 10 Q
(\322Quantitative Spectr) 189 475.35 T
(oscopy of K647 \321 the PNN of Ps1 in the Globular Cluster M15\323) 272.24 475.35 T
3 9 Q
(Heber) 207 458.02 T
(, U., Dreizler) 231.01 458.02 T
(, S., and W) 280.52 458.02 T
(erner) 324.88 458.02 T
(, K. 1993, Acta Astron., 43, 337\320342.) 345.39 458.02 T
6 10 Q
(\322The Interstellar Abundances of T) 189 438.35 T
(in and Four Other Heavy Elements\323) 326.23 438.35 T
3 9 Q
0.44 (Hobbs, L.M., W) 207 421.02 P
0.44 (elty) 269.73 421.02 P
0.44 (, D.E., Morton, D.C., Spitzer) 283.07 421.02 P
0.44 (, L., and Y) 395.85 421.02 P
0.44 (ork, D.G. 1993, ApJ, 41) 437.36 421.02 P
0.44 (1,) 532.49 421.02 P
(750\320755.) 216 410.02 T
6 10 Q
1 (\322T) 189 390.35 P
1 (ime-Series Observations of O Stars. III. IUE and HST Spectr) 199.57 390.35 P
1 (oscopy of) 451.79 390.35 P
9 F
1 (z) 494.34 390.35 P
6 F
1 ( Ophiuchi) 499.28 390.35 P
(and Implications for the \324Photospheric Connection\325\323) 198 378.35 T
3 9 Q
(Howarth, I.D. et al., 1993, ApJ, 417, 338\320346.) 207 361.02 T
6 10 Q
1.36 (\322Hubble Space T) 189 341.35 P
1.36 (elescope Spectra of the Phase-Modulated W) 260.23 341.35 P
1.36 (ind in the SMC O+WR) 443.38 341.35 P
(Binary R31\323) 198 329.35 T
3 9 Q
(Hutchings, J.B., Morris, S.C., and Bianchi, L. 1993, ApJ, 410, 803\320807.) 207 312.02 T
6 10 Q
(\322Deceleration of Interstellar Hydr) 189 292.35 T
(ogen at the Heliospheric Interface\323) 327.23 292.35 T
3 9 Q
(Lallement, R., Bertaux, J.-L., and Clarke, J.T) 207 275.02 T
(. 1993, Science, 260, 1095\3201098.) 383.57 275.02 T
5 10 Q
(Provides a good illustration of geocoronal L) 207 257.35 T
(y-) 383.1 257.35 T
9 F
(a) 391.43 257.35 T
5 F
( with the LSA and Echelle-A.) 397.74 257.35 T
6 F
3.24 (\322High Resolution UV Stellar Spectr) 189 237.35 P
3.24 (oscopy with the HST/GHRS, Challenges and) 345.48 237.35 P
(Opportunities for Atomic Physics\323) 198 225.35 T
3 9 Q
0.62 (Leckrone, D.S., Johansson, S., W) 207 208.02 P
0.62 (ahlgren, G.M., and Adelman, S.J. 1993, Physica) 344.2 208.02 P
(Scripta, T47, 149\320156.) 216 197.02 T
6 10 Q
3.97 (\322Goddar) 189 177.35 P
3.97 (d High Resolution Spectr) 225.3 177.35 P
3.97 (ograph Observations of the Local Interstellar) 337.66 177.35 P
-0.15 (Medium and the Deuterium/Hydr) 198 165.35 P
-0.15 (ogen Ratio Along the Line of Sight T) 330.78 165.35 P
-0.15 (owar) 475.23 165.35 P
-0.15 (d Capella\323) 495.42 165.35 P
3 9 Q
-0.1 (Linsky) 207 148.02 P
-0.1 (, J.L., Brown, A., Gayley) 231.84 148.02 P
-0.1 (, K., Diplas, A., Savage, B.D., A) 327.33 148.02 P
-0.1 (yres, T) 452.66 148.02 P
-0.1 (.R., Landsman,) 479.07 148.02 P
(W) 216 137.02 T
(., Shore, S.N., and Heap, S.R. 1993, ApJ, 402, 694\320709.) 224 137.02 T
6 10 Q
(\322The Bor) 189 117.35 T
(on Abundance of Pr) 226.69 117.35 T
(ocyon\323) 306.59 117.35 T
3 9 Q
(Lemke, M., Lambert, D.L., and Edvardsson, B. 1993, P) 207 100.02 T
(ASP) 424.94 100.02 T
(, 105, 468\320475.) 441.79 100.02 T
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54 750.02 540 750.02 2 L
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0 X
0 0 0 1 0 0 0 K
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0 9 Q
(GHRS Bibliography) 189 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(106) 54 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
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54 750.02 540 750.02 2 L
2 H
0 Z
N
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
6 F
(\322Detection of [O II]) 189 679.35 T
9 F
(l) 272.88 679.35 T
6 F
(2471 fr) 278.37 679.35 T
(om the Io Plasma T) 307.17 679.35 T
(orus\323) 384.58 679.35 T
3 9 Q
0.23 (McGrath, M.A., Feldman, P) 207 662.02 P
0.23 (.D., Strobel, D.F) 315.56 662.02 P
0.23 (., Moos, H.W) 379.54 662.02 P
0.23 (., and Ballester) 431.52 662.02 P
0.23 (, G.E. 1993,) 491.51 662.02 P
(ApJ, 415, L55\320L58.) 216 651.02 T
6 10 Q
(\322A Sear) 189 631.35 T
(ch for Pr) 221.13 631.35 T
(oton Beams During Flar) 256.87 631.35 T
(es on AU Micr) 355.11 631.35 T
(oscopii\323) 413.34 631.35 T
3 9 Q
0.19 (Robinson, R.D., Carpenter) 207 614.02 P
0.19 (, K.G., W) 312.93 614.02 P
0.19 (oodgate, B.E., and Maran, S.P) 349.67 614.02 P
0.19 (. 1993, ApJ, 414,) 471.37 614.02 P
(872\320876.) 216 603.02 T
6 10 Q
1.28 (\322Observations of the Gaseous Galactic Halo T) 189 583.35 P
1.28 (owar) 384.07 583.35 P
1.28 (d 3C273 with the Goddar) 404.26 583.35 P
1.28 (d High) 511.22 583.35 P
(Resolution Spectr) 198 571.35 T
(ograph\323) 268.46 571.35 T
3 9 Q
(Savage, B.D., Lu, L., W) 207 554.02 T
(eymann, R.J., and Morris, S.L. 1993, ApJ, 404, 124\320143.) 300.89 554.02 T
6 10 Q
-0.25 (\322Goddar) 189 534.35 P
-0.25 (d High Resolution Spectr) 225.3 534.35 P
-0.25 (ograph Observations of Narr) 325.01 534.35 P
-0.25 (ow Discr) 440.84 534.35 P
-0.25 (ete Stellar W) 476.61 534.35 P
-0.25 (ind) 527.22 534.35 P
(Absorption Featur) 198 522.35 T
(es in the Ultraviolet Spectrum of the O7.5III Star) 271.8 522.35 T
9 F
(z) 470.67 522.35 T
6 F
( Persei\323) 475.61 522.35 T
3 9 Q
-0.08 (Shore, S.N., Altner) 207 505.02 P
-0.08 (, B., Bolton, C.T) 281.38 505.02 P
-0.08 (., Cardelli, J.A., and Ebbets, D.C. 1993, ApJ, 41) 343.68 505.02 P
-0.08 (1,) 532.49 505.02 P
(864\320868.) 216 494.02 T
6 10 Q
(\322The Early Ultraviolet Spectral Evolution of Nova Cygni 1992\323) 189 474.35 T
3 9 Q
2.14 (Shore, S.N., Sonneborn, G., Starr\336eld, S., Gonzalez-Riestra, R., and Ake, T) 207 457.02 P
2.14 (.B.) 528.99 457.02 P
(1993, AJ, 106, 2408\3202428.) 216 446.02 T
6 10 Q
1.49 (\322High-Resolution Ultraviolet Observations of the Interstellar Diffuse Clouds towar) 189 426.35 P
1.49 (d) 535 426.35 P
9 F
(m) 198 414.35 T
6 F
(Columbae\323) 206.26 414.35 T
3 9 Q
(So\336a, U.J., Savage, B.D., and Cardelli, J.A. 1993, ApJ, 413, 251\320267.) 207 397.02 T
6 10 Q
(\322Composition of Interstellar Clouds in the Disk and Halo. I. HD 93521\323) 189 377.35 T
3 9 Q
(Spitzer) 207 360.02 T
(, L., and Fitzpatrick, E.L. 1993, ApJ,409, 299\320318.) 234.51 360.02 T
8 12 Q
(1994:) 162 333.02 T
6 10 Q
(\322Interstellar and Inter) 189 312.35 T
(galactic Magnesium and Sodium Absorption towar) 278.63 312.35 T
(d SN 1993J\323) 482.43 312.35 T
3 9 Q
(Bowen, D.V) 207 295.02 T
(., Roth, K.C., Blades, J.C., and Meyer) 253.69 295.02 T
(, D.M. 1994, ApJ, 420, L71\320L74.) 403.26 295.02 T
6 10 Q
(\322Interstellar Detection of the Intersystem Line Si II] l 2335 towar) 189 275.35 T
(d) 451.4 275.35 T
9 F
(z) 458.9 275.35 T
6 F
( Ophiuchi\323) 463.84 275.35 T
3 9 Q
0.64 (Cardelli, J.A., So\336a, U.J., Savage, B.D., Keenan, F) 207 258.02 P
0.64 (.P) 412.55 258.02 P
0.64 (., and Dufton, P) 419.9 258.02 P
0.64 (.L. 1994, ApJ,) 483.19 258.02 P
(420, L29\320L32.) 216 247.02 T
6 10 Q
0.04 (\322GHRS Observations of Cool, Low-Gravity Stars. I. The Far) 189 227.35 P
0.04 (-Ultraviolet Spectrum of) 433.3 227.35 P
9 F
0.04 (a) 533.69 227.35 P
6 F
(Orionis \050M2Iab\051\323) 198 215.35 T
3 9 Q
0.08 (Carpenter) 207 198.02 P
0.08 (, K.G., Robinson, R.D., W) 246.52 198.02 P
0.08 (ahlgren, G.M., Linsky) 349.03 198.02 P
0.08 (, J.L., and Brown, A. 1994,) 433.55 198.02 P
(ApJ, in press.) 216 187.02 T
6 10 Q
(\322Composition of Interstellar Clouds in the Disk and Halo. II.) 189 167.35 T
9 F
(g) 436.79 167.35 T
6 8 Q
(2) 440.9 171.35 T
6 10 Q
( V) 444.9 167.35 T
(elorum\323) 452.4 167.35 T
3 9 Q
(Fitzpatrick, E.L., and Spitzer) 207 150.02 T
(, L. 1994, ApJ, in press.) 319.05 150.02 T
6 10 Q
(\322Sear) 189 130.35 T
(ch for CO Absorption Bands in IUE Far) 212.52 130.35 T
(-Ultraviolet Spectra of Cool Stars\323) 373.71 130.35 T
3 9 Q
(Gessner) 207 113.02 T
(, S.E., Carpenter) 240.52 113.02 T
(, K.G., and Robinson, R.D. 1994, AJ, 107, 747\320750.) 307.05 113.02 T
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0.79 (iallefond, F) 417.97 613.02 P
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0.58 (\322Interstellar Clouds towar) 207 582.35 P
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(of Sirius A\323) 216 570.35 T
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-0.14 (Lallement, R., Bertin, P) 225 553.02 P
-0.14 (., Ferlet, R., V) 315.95 553.02 P
-0.14 (idal-Madjar) 370.89 553.02 P
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(press.) 234 542.02 T
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(\322Interstellar Carbon Monoxide towar) 207 522.35 T
(d) 358.58 522.35 T
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(z) 366.08 522.35 T
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( Ophiuchi.\323) 371.02 522.35 T
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0.01 (Lambert, D.L., Shef) 225 505.02 P
0.01 (fer) 302.9 505.02 P
0.01 (, Y) 312.91 505.02 P
0.01 (., Gilliland, R.L., and Federman, S.R. 1994, ApJ, 420, 756\320) 322.77 505.02 P
(771.) 234 494.02 T
5 10 Q
0.02 (An especially good discussion of how to achieve very high signal-to-noise with the) 225 476.35 P
(GHRS.) 225 464.35 T
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0.35 (\322High V) 207 444.35 P
0.35 (elocity Plasma in the T) 240.41 444.35 P
0.35 (ransition Region of Au Micr) 333.46 444.35 P
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(Linsky) 225 403.02 T
(, J.L., and W) 249.84 403.02 T
(ood, B.E. 1994, ApJ, in press.) 300.2 403.02 T
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(\322Pr) 207 383.35 T
(obing the Galactic Disk and Halo. I. The NGC 3783 Sight Line\323) 222.19 383.35 T
3 9 Q
(Lu, L., Savage, B.D., and Sembach, K.R. 1994, ApJ, in press.) 225 366.02 T
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(\322Observing Stellar Cor) 207 346.35 T
(onae with the Goddar) 301.08 346.35 T
(d High Resolution Spectr) 388.21 346.35 T
(ograph.) 488.67 346.35 T
(I. The dMe Star AU Micr) 216 334.35 T
(oscopii\323) 316.17 334.35 T
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1.27 (Maran, S.P) 225 317.02 P
1.27 (., Robinson, R.D., Shore, S.N., Brosius, J.W) 270.13 317.02 P
1.27 (., Carpenter) 452.81 317.02 P
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1.27 (ood-) 539.99 317.02 P
0.93 (gate, B.E., Linsky) 234 306.02 P
0.93 (, J.L., Brown, A., Byrne, P) 305.23 306.02 P
0.93 (.B., Kundu, M.R., White, S., Brandt,) 411.78 306.02 P
(J.C., Shine, R.A., and W) 234 295.02 T
(alter) 331.21 295.02 T
(, F) 348.22 295.02 T
(.M. 1994, ApJ, 421, 800\320808.) 357.72 295.02 T
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0.51 (\322Highly Ionized Gas Absorption in the Disk and Halo towar) 207 275.35 P
0.51 (d HD) 453.18 275.35 P
0.51 (167756 at 3.5 Kilo-) 478.13 275.35 P
(meters per Second Resolution\323) 216 263.35 T
3 9 Q
(Savage, B.D., Sembach, K.R., and Cardelli, J.A., 1994, ApJ, 420, 183\320196.) 225 246.02 T
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0.39 (\322Al III, Si IV) 207 226.35 P
0.39 (, and C IV Absorption towar) 258.55 226.35 P
0.39 (d) 374.05 226.35 P
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0.39 (z) 381.94 226.35 P
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0.39 ( Ophiuchi: Evidence for Photoionized and) 386.88 226.35 P
(Collisionally Ionized Gas\323) 216 214.35 T
3 9 Q
(Sembach, K.R., Savage, B.D., and Jenkins, E.B. 1994, ApJ, 421, 585\320599.) 225 197.02 T
6 10 Q
0.22 (\322A Sear) 207 177.35 P
0.22 (ch for Chr) 239.35 177.35 P
0.22 (omospheric Emission in A-type Stars Using the Goddar) 281.1 177.35 P
0.22 (d High Reso-) 504.78 177.35 P
(lution Spectr) 216 165.35 T
(ograph\323) 267.02 165.35 T
3 9 Q
(Simon, T) 225 148.02 T
(., Landsman, W) 260.01 148.02 T
(.B., and Gilliland, R.L. 1994, ApJ, in press.) 322.54 148.02 T
6 10 Q
(\322The Abundant Elements in Interstellar Dust\323) 207 128.35 T
3 9 Q
(So\336a, U.J., Cardelli, J.A., and Savage, B.D. 1994, ApJ, in press.) 225 111.02 T
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(V) 207 553.02 T
(idal-Madjar) 212.84 553.02 T
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4 12 moveto 12 4 lineto stroke} bind def
<8142241818244281> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-1 -1 moveto 9 9 lineto stroke } bind def
<03060c183060c081> { 1 setlinewidth -1 -1 moveto 9 9 lineto stroke
4 -4 moveto 12 4 lineto stroke
-4 4 moveto 4 12 lineto stroke} bind def
<8040201008040201> { 1 setlinewidth -1 9 moveto 9 -1 lineto stroke
-4 4 moveto 4 -4 lineto stroke
4 12 moveto 12 4 lineto stroke} bind def
end def
/patDict 15 dict dup begin
/PatternType 1 def
/PaintType 2 def
/TilingType 3 def
/BBox [ 0 0 8 8 ] def
/XStep 8 def
/YStep 8 def
/PaintProc {
begin
patProcDict bstring known {
patProcDict bstring get exec
} {
8 8 true [1 0 0 -1 0 8] bstring imagemask
} ifelse
end
} bind def
end def
} if
/combineColor {
FrameSepIs FMnone eq
{
graymode FMLevel1 or not {

[/Pattern [/DeviceCMYK]] setcolorspace
FrameCurColors 0 4 getinterval aload pop FrameCurPat setcolor
} {
FrameCurColors 3 get 1.0 ge {
FrameCurGray RealSetgray
} {
FMPColor graymode and {
0 1 3 {
FrameCurColors exch get
1 FrameCurGray sub mul
} for
RealSetcmykcolor
} {
4 1 6 {
FrameCurColors exch get
graymode {
1 exch sub 1 FrameCurGray sub mul 1 exch sub
} {
1.0 lt {FrameCurGray} {1} ifelse
} ifelse
} for
RealSetrgbcolor
} ifelse
} ifelse
} ifelse
} {
FrameCurColors 0 4 getinterval aload
FrameColorInSepListCMYK {
FrameSepBlack eq exch
FrameSepYellow eq and exch
FrameSepMagenta eq and exch
FrameSepCyan eq and
FrameSepIs FMcustom eq and
{ FrameCurGray } { 1 } ifelse
} {
FrameSepIs FMblack eq
{FrameCurGray 1.0 exch sub mul 1.0 exch sub 4 1 roll pop pop pop} {
FrameSepIs FMyellow eq
{pop FrameCurGray 1.0 exch sub mul 1.0 exch sub 3 1 roll pop pop} {
FrameSepIs FMmagenta eq
{pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub exch pop } {
FrameSepIs FMcyan eq
{pop pop pop FrameCurGray 1.0 exch sub mul 1.0 exch sub }
{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
graymode FMLevel1 or not {

[/Pattern [/DeviceGray]] setcolorspace
FrameCurPat setcolor
} {
graymode not FMLevel1 and {

dup 1 lt {pop FrameCurGray} if
} if
RealSetgray
} ifelse
} ifelse
} bind def
/savematrix {
orgmatrix currentmatrix pop
} bind def
/restorematrix {
orgmatrix setmatrix
} bind def
/dmatrix matrix def
/dpi 72 0 dmatrix defaultmatrix dtransform
dup mul exch dup mul add sqrt def

/freq dpi dup 72 div round dup 0 eq {pop 1} if 8 mul div def
/sangle 1 0 dmatrix defaultmatrix dtransform exch atan def
/dpiranges [ 2540 2400 1693 1270 1200 635 600 0 ] def
/CMLowFreqs [ 100.402 94.8683 89.2289 100.402 94.8683 66.9349 63.2456 47.4342 ] def
/YLowFreqs [ 95.25 90.0 84.65 95.25 90.0 70.5556 66.6667 50.0 ] def
/KLowFreqs [ 89.8026 84.8528 79.8088 89.8026 84.8528 74.8355 70.7107 53.033 ] def
/CLowAngles [ 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 ] def
/MLowAngles [ 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 ] def
/YLowTDot [ true true false true true false false false ] def
/CMHighFreqs [ 133.87 126.491 133.843 108.503 102.523 100.402 94.8683 63.2456 ] def
/YHighFreqs [ 127.0 120.0 126.975 115.455 109.091 95.25 90.0 60.0 ] def
/KHighFreqs [ 119.737 113.137 119.713 128.289 121.218 89.8026 84.8528 63.6395 ] def
/CHighAngles [ 71.5651 71.5651 71.5651 70.0169 70.0169 71.5651 71.5651 71.5651 ] def
/MHighAngles [ 18.4349 18.4349 18.4349 19.9831 19.9831 18.4349 18.4349 18.4349 ] def
/YHighTDot [ false false true false false true true false ] def
/PatFreq [ 10.5833 10.0 9.4055 10.5833 10.0 10.5833 10.0 9.375 ] def
/screenIndex {
0 1 dpiranges length 1 sub { dup dpiranges exch get 1 sub dpi le {exit} {pop} ifelse } for
} bind def
/getCyanScreen {
FMUseHighFrequencyScreens { CHighAngles CMHighFreqs} {CLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getMagentaScreen {
FMUseHighFrequencyScreens { MHighAngles CMHighFreqs } {MLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getYellowScreen {
FMUseHighFrequencyScreens { YHighTDot YHighFreqs} { YLowTDot YLowFreqs } ifelse
screenIndex dup 3 1 roll get 3 1 roll get { 3 div
{2 { 1 add 2 div 3 mul dup floor sub 2 mul 1 sub exch} repeat
FMSpotFunction } } {/FMSpotFunction load } ifelse
0.0 exch
} bind def
/getBlackScreen {
FMUseHighFrequencyScreens { KHighFreqs } { KLowFreqs } ifelse
screenIndex get 45.0 /FMSpotFunction load
} bind def
/getSpotScreen {
getBlackScreen
} bind def
/getCompositeScreen {
getBlackScreen
} bind def
/FMSetScreen
FMLevel1 { /setscreen load
}{ {
8 dict begin
/HalftoneType 1 def
/SpotFunction exch def
/Angle exch def
/Frequency exch def
/AccurateScreens FMUseAcccurateScreens def
currentdict end sethalftone
} bind } ifelse
def
/setDefaultScreen {
FMPColor {
orgrxfer cvx orggxfer cvx orgbxfer cvx orgxfer cvx setcolortransfer
}
{
orgxfer cvx settransfer
} ifelse
orgfreq organgle orgproc cvx setscreen
} bind def
/setCurrentScreen {
FrameSepIs FMnone eq {
FMUseDefaultNoSeparationScreen {
setDefaultScreen
} {
getCompositeScreen FMSetScreen
} ifelse
} {
FrameSepIs FMcustom eq {
FMUseDefaultSpotSeparationScreen {
setDefaultScreen
} {
getSpotScreen FMSetScreen
} ifelse
} {
FMUseDefaultProcessSeparationScreen {
setDefaultScreen
} {
FrameSepIs FMcyan eq {
getCyanScreen FMSetScreen
} {
FrameSepIs FMmagenta eq {
getMagentaScreen FMSetScreen
} {
FrameSepIs FMyellow eq {
getYellowScreen FMSetScreen
} {
getBlackScreen FMSetScreen
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} bind def
end
/gstring FMLOCAL
/gfile FMLOCAL
/gindex FMLOCAL
/orgrxfer FMLOCAL
/orggxfer FMLOCAL
/orgbxfer FMLOCAL
/orgxfer FMLOCAL
/orgproc FMLOCAL
/orgrproc FMLOCAL
/orggproc FMLOCAL
/orgbproc FMLOCAL
/organgle FMLOCAL
/orgrangle FMLOCAL
/orggangle FMLOCAL
/orgbangle FMLOCAL
/orgfreq FMLOCAL
/orgrfreq FMLOCAL
/orggfreq FMLOCAL
/orgbfreq FMLOCAL
/yscale FMLOCAL
/xscale FMLOCAL
/edown FMLOCAL
/manualfeed FMLOCAL
/paperheight FMLOCAL
/paperwidth FMLOCAL
/FMDOCUMENT {
array /FMfonts exch def
/#copies exch def
FrameDict begin
0 ne /manualfeed exch def
/paperheight exch def
/paperwidth exch def
0 ne /FrameNegative exch def
0 ne /edown exch def
/yscale exch def
/xscale exch def
FMLevel1 {
manualfeed {setmanualfeed} if
/FMdicttop countdictstack 1 add def
/FMoptop count def
% setpapername
% manualfeed {true} {papersize} ifelse
% {manualpapersize} {false} ifelse
% {desperatepapersize} {false} ifelse
% { (Can't select requested paper size for Frame print job!) FMFAILURE } if
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
}
{{1 dict dup /PageSize [paperwidth paperheight]put setpagedevice}stopped
{ (Can't select requested paper size for Frame print job!) FMFAILURE } if
{1 dict dup /ManualFeed manualfeed put setpagedevice } stopped pop }
ifelse

FMPColor {
currentcolorscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def
cvlit /orgbproc exch def
/orgbangle exch def
/orgbfreq exch def
cvlit /orggproc exch def
/orggangle exch def
/orggfreq exch def
cvlit /orgrproc exch def
/orgrangle exch def
/orgrfreq exch def
currentcolortransfer
FrameNegative {
1 1 4 {
pop { 1 exch sub } concatprocs 4 1 roll
} for
4 copy
setcolortransfer
} if
cvlit /orgxfer exch def
cvlit /orgbxfer exch def
cvlit /orggxfer exch def
cvlit /orgrxfer exch def
} {
currentscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def

currenttransfer
FrameNegative {
{ 1 exch sub } concatprocs
dup settransfer
} if
cvlit /orgxfer exch def
} ifelse
end
} def
/pagesave FMLOCAL
/orgmatrix FMLOCAL
/landscape FMLOCAL
/pwid FMLOCAL
/FMBEGINPAGE {
FrameDict begin
/pagesave save def
3.86 setmiterlimit
/landscape exch 0 ne def
landscape {
90 rotate 0 exch dup /pwid exch def neg translate pop
}{
pop /pwid exch def
} ifelse
edown { [-1 0 0 1 pwid 0] concat } if
0 0 moveto paperwidth 0 lineto paperwidth paperheight lineto
0 paperheight lineto 0 0 lineto 1 setgray fill
xscale yscale scale
/orgmatrix matrix def
gsave
} def
/FMENDPAGE {
grestore
pagesave restore
end
showpage
} def
/FMFONTDEFINE {
FrameDict begin
findfont
ReEncode
1 index exch
definefont
FMfonts 3 1 roll
put
end
} def
/FMFILLS {
FrameDict begin dup
array /fillvals exch def
dict /patCache exch def
end
} def
/FMFILL {
FrameDict begin
fillvals 3 1 roll put
end
} def
/FMNORMALIZEGRAPHICS {
newpath
0.0 0.0 moveto
1 setlinewidth
0 setlinecap
0 0 0 sethsbcolor
0 setgray
} bind def
/fx FMLOCAL
/fy FMLOCAL
/fh FMLOCAL
/fw FMLOCAL
/llx FMLOCAL
/lly FMLOCAL
/urx FMLOCAL
/ury FMLOCAL
/FMBEGINEPSF {
end
/FMEPSF save def
/showpage {} def
% See Adobe's "PostScript Language Reference Manual, 2nd Edition", page 714.
% "...the following operators MUST NOT be used in an EPS file:" (emphasis ours)
/banddevice {(banddevice) FMBADEPSF} def
/clear {(clear) FMBADEPSF} def
/cleardictstack {(cleardictstack) FMBADEPSF} def
/copypage {(copypage) FMBADEPSF} def
/erasepage {(erasepage) FMBADEPSF} def
/exitserver {(exitserver) FMBADEPSF} def
/framedevice {(framedevice) FMBADEPSF} def
/grestoreall {(grestoreall) FMBADEPSF} def
/initclip {(initclip) FMBADEPSF} def
/initgraphics {(initgraphics) FMBADEPSF} def
/initmatrix {(initmatrix) FMBADEPSF} def
/quit {(quit) FMBADEPSF} def
/renderbands {(renderbands) FMBADEPSF} def
/setglobal {(setglobal) FMBADEPSF} def
/setpagedevice {(setpagedevice) FMBADEPSF} def
/setshared {(setshared) FMBADEPSF} def
/startjob {(startjob) FMBADEPSF} def
/lettertray {(lettertray) FMBADEPSF} def
/letter {(letter) FMBADEPSF} def
/lettersmall {(lettersmall) FMBADEPSF} def
/11x17tray {(11x17tray) FMBADEPSF} def
/11x17 {(11x17) FMBADEPSF} def
/ledgertray {(ledgertray) FMBADEPSF} def
/ledger {(ledger) FMBADEPSF} def
/legaltray {(legaltray) FMBADEPSF} def
/legal {(legal) FMBADEPSF} def
/statementtray {(statementtray) FMBADEPSF} def
/statement {(statement) FMBADEPSF} def
/executivetray {(executivetray) FMBADEPSF} def
/executive {(executive) FMBADEPSF} def
/a3tray {(a3tray) FMBADEPSF} def
/a3 {(a3) FMBADEPSF} def
/a4tray {(a4tray) FMBADEPSF} def
/a4 {(a4) FMBADEPSF} def
/a4small {(a4small) FMBADEPSF} def
/b4tray {(b4tray) FMBADEPSF} def
/b4 {(b4) FMBADEPSF} def
/b5tray {(b5tray) FMBADEPSF} def
/b5 {(b5) FMBADEPSF} def
FMNORMALIZEGRAPHICS
[/fy /fx /fh /fw /ury /urx /lly /llx] {exch def} forall
fx fw 2 div add fy fh 2 div add translate
rotate
fw 2 div neg fh 2 div neg translate
fw urx llx sub div fh ury lly sub div scale
llx neg lly neg translate
/FMdicttop countdictstack 1 add def
/FMoptop count def
} bind def
/FMENDEPSF {
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
FMEPSF restore
FrameDict begin
} bind def
FrameDict begin
/setmanualfeed {
%%BeginFeature *ManualFeed True
statusdict /manualfeed true put
%%EndFeature
} bind def
/max {2 copy lt {exch} if pop} bind def
/min {2 copy gt {exch} if pop} bind def
/inch {72 mul} def
/pagedimen {
paperheight sub abs 16 lt exch
paperwidth sub abs 16 lt and
{/papername exch def} {pop} ifelse
} bind def
/papersizedict FMLOCAL
/setpapername {
/papersizedict 14 dict def
papersizedict begin
/papername /unknown def
/Letter 8.5 inch 11.0 inch pagedimen
/LetterSmall 7.68 inch 10.16 inch pagedimen
/Tabloid 11.0 inch 17.0 inch pagedimen
/Ledger 17.0 inch 11.0 inch pagedimen
/Legal 8.5 inch 14.0 inch pagedimen
/Statement 5.5 inch 8.5 inch pagedimen
/Executive 7.5 inch 10.0 inch pagedimen
/A3 11.69 inch 16.5 inch pagedimen
/A4 8.26 inch 11.69 inch pagedimen
/A4Small 7.47 inch 10.85 inch pagedimen
/B4 10.125 inch 14.33 inch pagedimen
/B5 7.16 inch 10.125 inch pagedimen
end
} bind def
/papersize {
papersizedict begin
/Letter {lettertray letter} def
/LetterSmall {lettertray lettersmall} def
/Tabloid {11x17tray 11x17} def
/Ledger {ledgertray ledger} def
/Legal {legaltray legal} def
/Statement {statementtray statement} def
/Executive {executivetray executive} def
/A3 {a3tray a3} def
/A4 {a4tray a4} def
/A4Small {a4tray a4small} def
/B4 {b4tray b4} def
/B5 {b5tray b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
statusdict begin stopped end
} bind def
/manualpapersize {
papersizedict begin
/Letter {letter} def
/LetterSmall {lettersmall} def
/Tabloid {11x17} def
/Ledger {ledger} def
/Legal {legal} def
/Statement {statement} def
/Executive {executive} def
/A3 {a3} def
/A4 {a4} def
/A4Small {a4small} def
/B4 {b4} def
/B5 {b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
stopped
} bind def
/desperatepapersize {
statusdict /setpageparams known
{
paperwidth paperheight 0 1
statusdict begin
{setpageparams} stopped
end
} {true} ifelse
} bind def
/DiacriticEncoding [
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /space /exclam /quotedbl
/numbersign /dollar /percent /ampersand /quotesingle /parenleft
/parenright /asterisk /plus /comma /hyphen /period /slash /zero /one
/two /three /four /five /six /seven /eight /nine /colon /semicolon
/less /equal /greater /question /at /A /B /C /D /E /F /G /H /I /J /K
/L /M /N /O /P /Q /R /S /T /U /V /W /X /Y /Z /bracketleft /backslash
/bracketright /asciicircum /underscore /grave /a /b /c /d /e /f /g /h
/i /j /k /l /m /n /o /p /q /r /s /t /u /v /w /x /y /z /braceleft /bar
/braceright /asciitilde /.notdef /Adieresis /Aring /Ccedilla /Eacute
/Ntilde /Odieresis /Udieresis /aacute /agrave /acircumflex /adieresis
/atilde /aring /ccedilla /eacute /egrave /ecircumflex /edieresis
/iacute /igrave /icircumflex /idieresis /ntilde /oacute /ograve
/ocircumflex /odieresis /otilde /uacute /ugrave /ucircumflex
/udieresis /dagger /.notdef /cent /sterling /section /bullet
/paragraph /germandbls /registered /copyright /trademark /acute
/dieresis /.notdef /AE /Oslash /.notdef /.notdef /.notdef /.notdef
/yen /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/ordfeminine /ordmasculine /.notdef /ae /oslash /questiondown
/exclamdown /logicalnot /.notdef /florin /.notdef /.notdef
/guillemotleft /guillemotright /ellipsis /.notdef /Agrave /Atilde
/Otilde /OE /oe /endash /emdash /quotedblleft /quotedblright
/quoteleft /quoteright /.notdef /.notdef /ydieresis /Ydieresis
/fraction /currency /guilsinglleft /guilsinglright /fi /fl /daggerdbl
/periodcentered /quotesinglbase /quotedblbase /perthousand
/Acircumflex /Ecircumflex /Aacute /Edieresis /Egrave /Iacute
/Icircumflex /Idieresis /Igrave /Oacute /Ocircumflex /.notdef /Ograve
/Uacute /Ucircumflex /Ugrave /dotlessi /circumflex /tilde /macron
/breve /dotaccent /ring /cedilla /hungarumlaut /ogonek /caron
] def
/ReEncode {
dup
length
dict begin
{
1 index /FID ne
{def}
{pop pop} ifelse
} forall
0 eq {/Encoding DiacriticEncoding def} if
currentdict
end
} bind def
FMPColor

{
/BEGINBITMAPCOLOR {
BITMAPCOLOR} def
/BEGINBITMAPCOLORc {
BITMAPCOLORc} def
/BEGINBITMAPTRUECOLOR {
BITMAPTRUECOLOR } def
/BEGINBITMAPTRUECOLORc {
BITMAPTRUECOLORc } def
}

{
/BEGINBITMAPCOLOR {
BITMAPGRAY} def
/BEGINBITMAPCOLORc {
BITMAPGRAYc} def
/BEGINBITMAPTRUECOLOR {
BITMAPTRUEGRAY } def
/BEGINBITMAPTRUECOLORc {
BITMAPTRUEGRAYc } def
}
ifelse
/K {
FMPrintAllColorsAsBlack {
dup 1 eq 2 index 1 eq and 3 index 1 eq and not
{7 {pop} repeat 0 0 0 1 0 0 0} if
} if
FrameCurColors astore
pop combineColor
} bind def
/graymode true def
/bwidth FMLOCAL
/bpside FMLOCAL
/bstring FMLOCAL
/onbits FMLOCAL
/offbits FMLOCAL
/xindex FMLOCAL
/yindex FMLOCAL
/x FMLOCAL
/y FMLOCAL
/setPatternMode {
FMLevel1 {
/bwidth exch def
/bpside exch def
/bstring exch def
/onbits 0 def /offbits 0 def
freq sangle landscape {90 add} if
{/y exch def
/x exch def
/xindex x 1 add 2 div bpside mul cvi def
/yindex y 1 add 2 div bpside mul cvi def
bstring yindex bwidth mul xindex 8 idiv add get
1 7 xindex 8 mod sub bitshift and 0 ne FrameNegative {not} if
{/onbits onbits 1 add def 1}
{/offbits offbits 1 add def 0}
ifelse
}
setscreen
offbits offbits onbits add div FrameNegative {1.0 exch sub} if
/FrameCurGray exch def
} {
pop pop
dup patCache exch known {
patCache exch get
} {
dup
patDict /bstring 3 -1 roll put
patDict
9 PatFreq screenIndex get div dup matrix scale
makepattern
dup
patCache 4 -1 roll 3 -1 roll put
} ifelse
/FrameCurGray 0 def
/FrameCurPat exch def
} ifelse
/graymode false def
combineColor
} bind def
/setGrayScaleMode {
graymode not {
/graymode true def
FMLevel1 {
setCurrentScreen
} if
} if
/FrameCurGray exch def
combineColor
} bind def
/normalize {
transform round exch round exch itransform
} bind def
/dnormalize {
dtransform round exch round exch idtransform
} bind def
/lnormalize {
0 dtransform exch cvi 2 idiv 2 mul 1 add exch idtransform pop
} bind def
/H {
lnormalize setlinewidth
} bind def
/Z {
setlinecap
} bind def

/PFill {
graymode FMLevel1 or not {
gsave 1 setgray eofill grestore
} if
} bind def
/PStroke {
graymode FMLevel1 or not {
gsave 1 setgray stroke grestore
} if
stroke
} bind def
/fillvals FMLOCAL
/X {
fillvals exch get
dup type /stringtype eq
{8 1 setPatternMode}
{setGrayScaleMode}
ifelse
} bind def
/V {
PFill gsave eofill grestore
} bind def
/Vclip {
clip
} bind def
/Vstrk {
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/N {
PStroke
} bind def
/Nclip {
strokepath clip newpath
} bind def
/Nstrk {
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/M {newpath moveto} bind def
/E {lineto} bind def
/D {curveto} bind def
/O {closepath} bind def
/n FMLOCAL
/L {
/n exch def
newpath
normalize
moveto
2 1 n {pop normalize lineto} for
} bind def
/Y {
L
closepath
} bind def
/x1 FMLOCAL
/x2 FMLOCAL
/y1 FMLOCAL
/y2 FMLOCAL
/R {
/y2 exch def
/x2 exch def
/y1 exch def
/x1 exch def
x1 y1
x2 y1
x2 y2
x1 y2
4 Y
} bind def
/rad FMLOCAL
/rarc
{rad
arcto
} bind def
/RR {
/rad exch def
normalize
/y2 exch def
/x2 exch def
normalize
/y1 exch def
/x1 exch def
mark
newpath
{
x1 y1 rad add moveto
x1 y2 x2 y2 rarc
x2 y2 x2 y1 rarc
x2 y1 x1 y1 rarc
x1 y1 x1 y2 rarc
closepath
} stopped {x1 y1 x2 y2 R} if
cleartomark
} bind def
/RRR {
/rad exch def
normalize /y4 exch def /x4 exch def
normalize /y3 exch def /x3 exch def
normalize /y2 exch def /x2 exch def
normalize /y1 exch def /x1 exch def
newpath
normalize moveto
mark
{
x2 y2 x3 y3 rarc
x3 y3 x4 y4 rarc
x4 y4 x1 y1 rarc
x1 y1 x2 y2 rarc
closepath
} stopped
{x1 y1 x2 y2 x3 y3 x4 y4 newpath moveto lineto lineto lineto closepath} if
cleartomark
} bind def
/C {
grestore
gsave
R
clip
setCurrentScreen
} bind def
/CP {
grestore
gsave
Y
clip
setCurrentScreen
} bind def
/FMpointsize FMLOCAL
/F {
FMfonts exch get
FMpointsize scalefont
setfont
} bind def
/Q {
/FMpointsize exch def
F
} bind def
/T {
moveto show
} bind def
/RF {
rotate
0 ne {-1 1 scale} if
} bind def
/TF {
gsave
moveto
RF
show
grestore
} bind def
/P {
moveto
0 32 3 2 roll widthshow
} bind def
/PF {
gsave
moveto
RF
0 32 3 2 roll widthshow
grestore
} bind def
/S {
moveto
0 exch ashow
} bind def
/SF {
gsave
moveto
RF
0 exch ashow
grestore
} bind def
/B {
moveto
0 32 4 2 roll 0 exch awidthshow
} bind def
/BF {
gsave
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%%EndProlog
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72 750.02 558 750.02 2 L
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72 445.03 558 445.03 2 L
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N
72 74.02 558 74.02 2 L
0.25 H
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0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
-2.78 (1) 542.42 60.29 P
-2.78 (1) 547.43 60.29 P
-2.78 (1) 552.44 60.29 P
72 750.02 558 750.02 2 L
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72 445.03 558 445.03 2 L
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72 74.02 558 74.02 2 L
0.25 H
N
1 24 Q
-0.48 (Glossary of T) 207 677 S
-0.48 (erms and) 327.41 677 S
-0.48 (Abbr) 207 647 S
-0.48 (eviations) 253.54 647 S
2 10 Q
0.12 (Here we provide de\336nitions and explanations of technical terms and abbreviations used) 207 425.33 P
1.59 (in the text. The usual abbreviations found in HST) 207 413.33 P
1.59 (-related documents \050e.g., WFPC2,) 416.85 413.33 P
(FGS\051 are not repeated here.) 207 401.33 T
0 F
(Blaze Function) 189 377.33 T
2 F
-0.13 (The ef) 207 353.33 P
-0.13 (\336ciency of an echelle grating drops sharply as one moves away from blaze center) 232.51 353.33 P
-0.13 (.) 555.5 353.33 P
0.06 (The shape of the response function is virtually the same for the dif) 207 341.33 P
0.06 (ferent orders and this) 473.11 341.33 P
(function is known as the Ripple Function \050see Section) 207 329.33 T
(8.3.3 on page) 425.6 329.33 T
(91\051.) 481.98 329.33 T
0 F
(Corner diodes) 189 305.33 T
2 F
0.36 (The detector area of the Digicons is laid out into speci\336c diodes, each of which acts as) 207 281.33 P
0.18 (an independent detector) 207 269.33 P
0.18 (. There are 500 science diodes, each of which is skinny but tall,) 302.33 269.33 P
0.17 (four focus diodes \050see below\051, and four corner diodes. The corner diodes are lar) 207 257.33 P
0.17 (ge rect-) 527.57 257.33 P
0.47 (angles \0500.1) 207 245.33 P
3 F
0.47 (\264) 254.32 245.33 P
2 F
0.47 ( 1 mm\051 of detector area above and below the science diodes and are used) 259.81 245.33 P
(for measuring background.) 207 233.33 T
0 F
(Cycles) 189 209.33 T
2 F
0.31 (Proposals to use HST are solicited and reviewed on roughly an annual basis. However) 207 185.33 P
0.31 (,) 555.5 185.33 P
1.53 (because HST\325) 207 173.33 P
1.53 (s properties changed fundamentally when COST) 264.35 173.33 P
1.53 (AR and WFPC2 were) 465.91 173.33 P
-0.25 (installed, Cycle 3 was de\336ned to end at the time of the Servicing Mission. Cycle 4 began) 207 161.33 P
(at the end of SMOV) 207 149.33 T
(. Cycle 5 is due to begin in mid 1995.) 286.81 149.33 T
FMENDPAGE
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612 792 0 FMBEGINPAGE
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54 750.02 540 750.02 2 L
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0 Z
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0 9 Q
(Glossary of T) 189 736.18 T
(erms and Abbreviations) 245.85 736.18 T
54 726.98 540 726.98 2 L
0.25 H
N
54 74.02 540 74.02 2 L
2 Z
N
0 10 Q
(1) 54 60.29 T
(12) 59.01 60.29 T
(GHRS Instrument Handbook 5.0) 189 60.29 T
54 750.02 540 750.02 2 L
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0 Z
N
54 726.98 540 726.98 2 L
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N
54 74.02 540 74.02 2 L
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54 750.02 540 750.02 2 L
2 H
0 Z
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54 726.98 540 726.98 2 L
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N
54 74.02 540 74.02 2 L
2 Z
N
(CVZ) 171 679.35 T
2 F
0.55 (Continuous V) 189 655.35 P
0.55 (iewing Zones. The inclined orbit of HST allows for uninterrupted obser-) 244.79 655.35 P
-0.24 (vations of objects in some declination ranges at certain times. See the) 189 643.35 P
4 F
-0.24 (Call for Pr) 466.39 643.35 P
-0.24 (oposals) 509.44 643.35 P
2 F
(for further information.) 189 631.35 T
0 F
(DEFCAL) 171 607.35 T
2 F
0.58 (Short for De\337ection Calibration. All GHRS acquisitions begin with a) 189 583.35 P
5 F
1.4 (DEFCAL) 473.98 583.35 P
2 F
0.58 (, which) 509.98 583.35 P
0.5 (measures the instantaneous location of the images on the onboard spectrum lamps and) 189 571.35 P
0.44 (then compares that location to the nominal coordinates stored in the onboard database.) 189 559.35 P
0.08 (The dif) 189 547.35 P
0.08 (ferences can range over several de\337ection steps in response to thermal and mag-) 218.06 547.35 P
0.35 (netic drifts. The of) 189 535.35 P
0.35 (fsets are applied to the database coordinates of the science apertures) 264.31 535.35 P
0.4 (to provide an updated estimate of their location. In practice, only observations of lamp) 189 523.35 P
0.69 (SC2 are used because of the loss of Side 1 and because using SC2 decreases the time) 189 511.35 P
(interval between the) 189 499.35 T
5 F
(DEFCAL) 272.59 499.35 T
2 F
( and the tar) 308.59 499.35 T
(get locate phase of the acquisition.) 353.12 499.35 T
0 F
(Focus diodes) 171 475.35 T
2 F
-0.16 (See Chapter 7 to see how the diodes in the GHRS Digicons are con\336gured. At both ends) 189 451.35 P
0.74 (of the array of 500 science diodes are two focus diodes. The focus diodes are smaller) 189 439.35 P
0.43 (than the science diodes and are square. The image of the LSA is de\337ected to the focus) 189 427.35 P
(diodes to generate) 189 415.35 T
5 F
(MAP) 264.26 415.35 T
2 F
(s and) 282.26 415.35 T
5 F
(IMAGE) 305.59 415.35 T
2 F
(s. The focus diodes are 25 microns square.) 335.59 415.35 T
0 F
(GIMP) 171 391.35 T
2 F
1.21 (Geomagnetically-induced image motion problem. This problem underlies our recom-) 189 367.35 P
1.16 (mendation to have no single exposure be longer than about 5 minutes in length. See) 189 355.35 P
(Section) 189 343.35 T
(8.6.5 on page) 221.5 343.35 T
(98.) 277.88 343.35 T
0 F
(GSC) 171 319.35 T
2 F
-0.19 (Guide Star Catalog, the list used to \336nd stars upon which the Fine Guidance Sensors can) 189 295.35 P
(lock to control the pointing of HST) 189 283.35 T
(.) 329.37 283.35 T
0 F
(LSA) 171 259.35 T
2 F
0.34 (Lar) 189 235.35 P
0.34 (ge Science Aperture. This is a square opening at the front of the GHRS that is used) 202.7 235.35 P
1.52 (to acquire stars and for some science observations. Its dimensions were 2.00 arcsec) 189 223.35 P
0.57 (square before COST) 189 211.35 P
0.57 (AR is installed and 1.74 arcsec square afterwards. The name used) 271.55 211.35 P
(for the LSA will continue to be \322) 189 199.35 T
5 F
(2.0) 320.93 199.35 T
2 F
(\323.) 338.93 199.35 T
0 F
(OSS) 171 175.35 T
2 F
-0.21 (Observation Support System, which is the facility located at STScI for real-time interac-) 189 151.35 P
(tion between the ground and the) 189 139.35 T
4 F
(HST) 320.09 139.35 T
2 F
( spacecraft.) 337.87 139.35 T
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(GHRS Instrument Handbook 5.0) 207 60.29 T
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-2.78 (13) 546.88 60.29 P
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(Glossary of T) 207 736.18 T
(erms and Abbreviations) 263.85 736.18 T
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(Phase I) 189 679.35 T
2 F
0.01 (A Phase I proposal for) 207 655.35 P
4 F
0.01 (HST) 299.51 655.35 P
2 F
0.01 ( includes just the information need by the T) 317.29 655.35 P
0.01 (elescope Alloca-) 491.07 655.35 P
0.65 (tion Committee \050T) 207 643.35 P
0.65 (AC\051 and STScI to judge scienti\336c merit and technical feasibility) 281.94 643.35 P
0.65 (. In) 544.02 643.35 P
0.52 (addition to the scienti\336c justi\336cation, you are asked to provide a list of the tar) 207 631.35 P
0.52 (gets that) 523.86 631.35 P
0.31 (you wish to observe and a brief description of the observations themselves. W) 207 619.35 P
0.31 (e recom-) 522.42 619.35 P
-0.26 (mend adding comments to provide a clearer explanation of what you intend, even if they) 207 607.35 P
(are not required.) 207 595.35 T
0 F
(Phase II) 189 571.35 T
2 F
1.02 (The Phase II proposal is written once the Phase I proposal has been accepted for the) 207 547.35 P
-0.03 (HST science program. The Phase II proposal includes all the detailed speci\336cations that) 207 535.35 P
-0.12 (are needed to turn your science program into the commands that the spacecraft will exe-) 207 523.35 P
0.72 (cute. As with Phase I, we recommend the liberal use of comments to help ensure that) 207 511.35 P
(your goals will be achieved.) 207 499.35 T
0 F
(Ripple Function) 189 475.35 T
2 F
(See Blaze Function) 207 451.35 T
0 F
(SAA) 189 427.35 T
2 F
1.22 (South Atlantic Anomaly) 207 403.35 P
1.22 (. A region lying over southeastern South America where the) 306.56 403.35 P
0.17 (earth\325) 207 391.35 P
0.17 (s radiation belts dip low) 229.77 391.35 P
0.17 (, leading to high particle background rates for satellites in) 325.92 391.35 P
(Low Earth Orbit. GHRS observations are suspended during passage through the SAA.) 207 379.35 T
0 F
(Side 1, Side 2) 189 355.35 T
2 F
0.29 (GHRS is split into two \322sides,\323 one for the short-wavelength detector \050D1\051 and one for) 207 331.35 P
-0.1 (the long-wavelength detector \050D2\051. The sides operate independently but depend on each) 207 319.35 P
0.57 (other for communication with the spacecraft. The installation of the GHRS Repair Kit) 207 307.35 P
0.69 (during the HST Servicing Mission has meant that all GHRS communications are now) 207 295.35 P
1.07 (through Side 2. Moreover) 207 283.35 P
1.07 (, Side 2 now solely controls the grating carrousel and LSA) 313.14 283.35 P
(shutter) 207 271.35 T
(.) 233.67 271.35 T
0 F
(SMOV) 189 247.35 T
2 F
0.19 (Servicing Mission Orbital V) 207 223.35 P
0.19 (eri\336cation, the period of time immediately after the Servic-) 320.09 223.35 P
-0.09 (ing Mission in which the basic capabilities of the telescope and instruments are veri\336ed.) 207 211.35 P
0 F
(SPYBAL) 189 187.35 T
2 F
0 (SPectrum Y BALance. A) 207 163.35 P
5 F
0.01 (SPYBAL) 311.17 163.35 P
2 F
0 ( consists of a quick observation of the spectrum cali-) 347.17 163.35 P
0.43 (bration lamp SC2 at a standard wavelength setting to ensure that the spectrum is prop-) 207 151.35 P
1.83 (erly centered on the diodes in the cross-dispersion direction. The) 207 139.35 P
4 F
1.83 (y) 486.66 139.35 P
2 F
1.83 ( position at this) 491.1 139.35 P
0.61 (standard wavelength is compared to a stored value and the dif) 207 127.35 P
0.61 (ference is applied to the) 460.05 127.35 P
1.22 (observations made with the proposal con\336guration until another) 207 115.35 P
5 F
2.91 (SPYBAL) 475.03 115.35 P
2 F
1.22 ( is done. A) 511.03 115.35 P
5 F
-0.1 (SPYBAL) 207 103.35 P
2 F
-0.04 ( is normally done before each new use of a dif) 243 103.35 P
-0.04 (ferent spectrum element, such as) 427.36 103.35 P
FMENDPAGE
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(erms and Abbreviations) 245.85 736.18 T
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(0.25) 193.44 595.35 T
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(\323.) 217.44 595.35 T
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(STEIS) 171 571.35 T
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1.28 (Space T) 189 547.35 P
1.28 (elescope Electronic Information Service. This service provides on-line news,) 222.07 547.35 P
0.03 (information, and documents via anonymous ftp. T) 189 535.35 P
0.03 (o use it,) 389 535.35 P
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0.03 (ftp) 422.96 535.35 P
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0.03 ( to) 433.52 535.35 P
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0.03 (stsci.edu) 446.36 535.35 P
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0.03 (\050Internet node) 483.6 535.35 P
0.85 (130.167.1.2\051 and login with username) 189 523.35 P
4 F
0.85 (anonymous) 347.69 523.35 P
2 F
0.85 (, using your last name as password.) 393.24 523.35 P
0.42 (Use) 189 511.35 P
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0.42 (get) 207.47 511.35 P
2 F
0.42 ( to transfer the README \336le in the entry directory; this will provide a general) 219.69 511.35 P
1.34 (explanation of how to access STEIS information. For more details, consult the User) 189 499.35 P
(Support Branch.) 189 487.35 T
0 F
(STEP-P) 171 463.35 T
(A) 206.38 463.35 T
(TT) 212.86 463.35 T
5 F
2.35 (STEP-PATT) 189 439.35 P
2 F
0.98 ( is the pattern of operations undertaken in an) 243 439.35 P
5 F
2.35 (ACCUM) 432.62 439.35 P
2 F
0.98 (. A typical) 462.62 439.35 P
5 F
2.35 (STEP-) 510 439.35 P
0.3 (PATT) 189 427.35 P
2 F
0.12 ( de\336nes the relative proportions of time spent accumulating on the science diodes) 213 427.35 P
(versus time with the background diodes. See Section) 189 415.35 T
(8.4 on page) 402.59 415.35 T
(92.) 451.47 415.35 T
0 F
(STEP-TIME) 171 391.35 T
2 F
-0.24 (STEP-TIME is the exposure time for the smallest unit of an exposure. For example, dur-) 189 367.35 P
0.48 (ing an acquisition,) 189 355.35 P
5 F
1.15 (STEP-TIME) 266.55 355.35 P
2 F
0.48 ( is the amount of time spent at each dwell point while) 320.55 355.35 P
-0.19 (executing a spiral search pattern. During an) 189 343.35 P
5 F
-0.47 (ACCUM) 364.26 343.35 P
2 F
-0.19 (, the detector integrates for a) 394.26 343.35 P
5 F
-0.47 (STEP-) 510 343.35 P
3.18 (TIME) 189 331.35 P
2 F
1.32 ( before reading the diodes and adding their contents to the memory) 213 331.35 P
1.32 (. A unit of) 494.92 331.35 P
5 F
(STEP-TIME) 189 319.35 T
2 F
( is spent executing each portion of a) 243 319.35 T
5 F
(STEP-PATT) 389.64 319.35 T
2 F
(, for example.) 442.9 319.35 T
FMENDPAGE
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{pop pop pop pop 1} ifelse } ifelse } ifelse } ifelse
} ifelse
graymode FMLevel1 or not {

[/Pattern [/DeviceGray]] setcolorspace
FrameCurPat setcolor
} {
graymode not FMLevel1 and {

dup 1 lt {pop FrameCurGray} if
} if
RealSetgray
} ifelse
} ifelse
} bind def
/savematrix {
orgmatrix currentmatrix pop
} bind def
/restorematrix {
orgmatrix setmatrix
} bind def
/dmatrix matrix def
/dpi 72 0 dmatrix defaultmatrix dtransform
dup mul exch dup mul add sqrt def

/freq dpi dup 72 div round dup 0 eq {pop 1} if 8 mul div def
/sangle 1 0 dmatrix defaultmatrix dtransform exch atan def
/dpiranges [ 2540 2400 1693 1270 1200 635 600 0 ] def
/CMLowFreqs [ 100.402 94.8683 89.2289 100.402 94.8683 66.9349 63.2456 47.4342 ] def
/YLowFreqs [ 95.25 90.0 84.65 95.25 90.0 70.5556 66.6667 50.0 ] def
/KLowFreqs [ 89.8026 84.8528 79.8088 89.8026 84.8528 74.8355 70.7107 53.033 ] def
/CLowAngles [ 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 71.5651 ] def
/MLowAngles [ 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 18.4349 ] def
/YLowTDot [ true true false true true false false false ] def
/CMHighFreqs [ 133.87 126.491 133.843 108.503 102.523 100.402 94.8683 63.2456 ] def
/YHighFreqs [ 127.0 120.0 126.975 115.455 109.091 95.25 90.0 60.0 ] def
/KHighFreqs [ 119.737 113.137 119.713 128.289 121.218 89.8026 84.8528 63.6395 ] def
/CHighAngles [ 71.5651 71.5651 71.5651 70.0169 70.0169 71.5651 71.5651 71.5651 ] def
/MHighAngles [ 18.4349 18.4349 18.4349 19.9831 19.9831 18.4349 18.4349 18.4349 ] def
/YHighTDot [ false false true false false true true false ] def
/PatFreq [ 10.5833 10.0 9.4055 10.5833 10.0 10.5833 10.0 9.375 ] def
/screenIndex {
0 1 dpiranges length 1 sub { dup dpiranges exch get 1 sub dpi le {exit} {pop} ifelse } for
} bind def
/getCyanScreen {
FMUseHighFrequencyScreens { CHighAngles CMHighFreqs} {CLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getMagentaScreen {
FMUseHighFrequencyScreens { MHighAngles CMHighFreqs } {MLowAngles CMLowFreqs} ifelse
screenIndex dup 3 1 roll get 3 1 roll get /FMSpotFunction load
} bind def
/getYellowScreen {
FMUseHighFrequencyScreens { YHighTDot YHighFreqs} { YLowTDot YLowFreqs } ifelse
screenIndex dup 3 1 roll get 3 1 roll get { 3 div
{2 { 1 add 2 div 3 mul dup floor sub 2 mul 1 sub exch} repeat
FMSpotFunction } } {/FMSpotFunction load } ifelse
0.0 exch
} bind def
/getBlackScreen {
FMUseHighFrequencyScreens { KHighFreqs } { KLowFreqs } ifelse
screenIndex get 45.0 /FMSpotFunction load
} bind def
/getSpotScreen {
getBlackScreen
} bind def
/getCompositeScreen {
getBlackScreen
} bind def
/FMSetScreen
FMLevel1 { /setscreen load
}{ {
8 dict begin
/HalftoneType 1 def
/SpotFunction exch def
/Angle exch def
/Frequency exch def
/AccurateScreens FMUseAcccurateScreens def
currentdict end sethalftone
} bind } ifelse
def
/setDefaultScreen {
FMPColor {
orgrxfer cvx orggxfer cvx orgbxfer cvx orgxfer cvx setcolortransfer
}
{
orgxfer cvx settransfer
} ifelse
orgfreq organgle orgproc cvx setscreen
} bind def
/setCurrentScreen {
FrameSepIs FMnone eq {
FMUseDefaultNoSeparationScreen {
setDefaultScreen
} {
getCompositeScreen FMSetScreen
} ifelse
} {
FrameSepIs FMcustom eq {
FMUseDefaultSpotSeparationScreen {
setDefaultScreen
} {
getSpotScreen FMSetScreen
} ifelse
} {
FMUseDefaultProcessSeparationScreen {
setDefaultScreen
} {
FrameSepIs FMcyan eq {
getCyanScreen FMSetScreen
} {
FrameSepIs FMmagenta eq {
getMagentaScreen FMSetScreen
} {
FrameSepIs FMyellow eq {
getYellowScreen FMSetScreen
} {
getBlackScreen FMSetScreen
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} ifelse
} bind def
end
/gstring FMLOCAL
/gfile FMLOCAL
/gindex FMLOCAL
/orgrxfer FMLOCAL
/orggxfer FMLOCAL
/orgbxfer FMLOCAL
/orgxfer FMLOCAL
/orgproc FMLOCAL
/orgrproc FMLOCAL
/orggproc FMLOCAL
/orgbproc FMLOCAL
/organgle FMLOCAL
/orgrangle FMLOCAL
/orggangle FMLOCAL
/orgbangle FMLOCAL
/orgfreq FMLOCAL
/orgrfreq FMLOCAL
/orggfreq FMLOCAL
/orgbfreq FMLOCAL
/yscale FMLOCAL
/xscale FMLOCAL
/edown FMLOCAL
/manualfeed FMLOCAL
/paperheight FMLOCAL
/paperwidth FMLOCAL
/FMDOCUMENT {
array /FMfonts exch def
/#copies exch def
FrameDict begin
0 ne /manualfeed exch def
/paperheight exch def
/paperwidth exch def
0 ne /FrameNegative exch def
0 ne /edown exch def
/yscale exch def
/xscale exch def
FMLevel1 {
manualfeed {setmanualfeed} if
/FMdicttop countdictstack 1 add def
/FMoptop count def
% setpapername
% manualfeed {true} {papersize} ifelse
% {manualpapersize} {false} ifelse
% {desperatepapersize} {false} ifelse
% { (Can't select requested paper size for Frame print job!) FMFAILURE } if
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
}
{{1 dict dup /PageSize [paperwidth paperheight]put setpagedevice}stopped
{ (Can't select requested paper size for Frame print job!) FMFAILURE } if
{1 dict dup /ManualFeed manualfeed put setpagedevice } stopped pop }
ifelse

FMPColor {
currentcolorscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def
cvlit /orgbproc exch def
/orgbangle exch def
/orgbfreq exch def
cvlit /orggproc exch def
/orggangle exch def
/orggfreq exch def
cvlit /orgrproc exch def
/orgrangle exch def
/orgrfreq exch def
currentcolortransfer
FrameNegative {
1 1 4 {
pop { 1 exch sub } concatprocs 4 1 roll
} for
4 copy
setcolortransfer
} if
cvlit /orgxfer exch def
cvlit /orgbxfer exch def
cvlit /orggxfer exch def
cvlit /orgrxfer exch def
} {
currentscreen
cvlit /orgproc exch def
/organgle exch def
/orgfreq exch def

currenttransfer
FrameNegative {
{ 1 exch sub } concatprocs
dup settransfer
} if
cvlit /orgxfer exch def
} ifelse
end
} def
/pagesave FMLOCAL
/orgmatrix FMLOCAL
/landscape FMLOCAL
/pwid FMLOCAL
/FMBEGINPAGE {
FrameDict begin
/pagesave save def
3.86 setmiterlimit
/landscape exch 0 ne def
landscape {
90 rotate 0 exch dup /pwid exch def neg translate pop
}{
pop /pwid exch def
} ifelse
edown { [-1 0 0 1 pwid 0] concat } if
0 0 moveto paperwidth 0 lineto paperwidth paperheight lineto
0 paperheight lineto 0 0 lineto 1 setgray fill
xscale yscale scale
/orgmatrix matrix def
gsave
} def
/FMENDPAGE {
grestore
pagesave restore
end
showpage
} def
/FMFONTDEFINE {
FrameDict begin
findfont
ReEncode
1 index exch
definefont
FMfonts 3 1 roll
put
end
} def
/FMFILLS {
FrameDict begin dup
array /fillvals exch def
dict /patCache exch def
end
} def
/FMFILL {
FrameDict begin
fillvals 3 1 roll put
end
} def
/FMNORMALIZEGRAPHICS {
newpath
0.0 0.0 moveto
1 setlinewidth
0 setlinecap
0 0 0 sethsbcolor
0 setgray
} bind def
/fx FMLOCAL
/fy FMLOCAL
/fh FMLOCAL
/fw FMLOCAL
/llx FMLOCAL
/lly FMLOCAL
/urx FMLOCAL
/ury FMLOCAL
/FMBEGINEPSF {
end
/FMEPSF save def
/showpage {} def
% See Adobe's "PostScript Language Reference Manual, 2nd Edition", page 714.
% "...the following operators MUST NOT be used in an EPS file:" (emphasis ours)
/banddevice {(banddevice) FMBADEPSF} def
/clear {(clear) FMBADEPSF} def
/cleardictstack {(cleardictstack) FMBADEPSF} def
/copypage {(copypage) FMBADEPSF} def
/erasepage {(erasepage) FMBADEPSF} def
/exitserver {(exitserver) FMBADEPSF} def
/framedevice {(framedevice) FMBADEPSF} def
/grestoreall {(grestoreall) FMBADEPSF} def
/initclip {(initclip) FMBADEPSF} def
/initgraphics {(initgraphics) FMBADEPSF} def
/initmatrix {(initmatrix) FMBADEPSF} def
/quit {(quit) FMBADEPSF} def
/renderbands {(renderbands) FMBADEPSF} def
/setglobal {(setglobal) FMBADEPSF} def
/setpagedevice {(setpagedevice) FMBADEPSF} def
/setshared {(setshared) FMBADEPSF} def
/startjob {(startjob) FMBADEPSF} def
/lettertray {(lettertray) FMBADEPSF} def
/letter {(letter) FMBADEPSF} def
/lettersmall {(lettersmall) FMBADEPSF} def
/11x17tray {(11x17tray) FMBADEPSF} def
/11x17 {(11x17) FMBADEPSF} def
/ledgertray {(ledgertray) FMBADEPSF} def
/ledger {(ledger) FMBADEPSF} def
/legaltray {(legaltray) FMBADEPSF} def
/legal {(legal) FMBADEPSF} def
/statementtray {(statementtray) FMBADEPSF} def
/statement {(statement) FMBADEPSF} def
/executivetray {(executivetray) FMBADEPSF} def
/executive {(executive) FMBADEPSF} def
/a3tray {(a3tray) FMBADEPSF} def
/a3 {(a3) FMBADEPSF} def
/a4tray {(a4tray) FMBADEPSF} def
/a4 {(a4) FMBADEPSF} def
/a4small {(a4small) FMBADEPSF} def
/b4tray {(b4tray) FMBADEPSF} def
/b4 {(b4) FMBADEPSF} def
/b5tray {(b5tray) FMBADEPSF} def
/b5 {(b5) FMBADEPSF} def
FMNORMALIZEGRAPHICS
[/fy /fx /fh /fw /ury /urx /lly /llx] {exch def} forall
fx fw 2 div add fy fh 2 div add translate
rotate
fw 2 div neg fh 2 div neg translate
fw urx llx sub div fh ury lly sub div scale
llx neg lly neg translate
/FMdicttop countdictstack 1 add def
/FMoptop count def
} bind def
/FMENDEPSF {
count -1 FMoptop {pop pop} for
countdictstack -1 FMdicttop {pop end} for
FMEPSF restore
FrameDict begin
} bind def
FrameDict begin
/setmanualfeed {
%%BeginFeature *ManualFeed True
statusdict /manualfeed true put
%%EndFeature
} bind def
/max {2 copy lt {exch} if pop} bind def
/min {2 copy gt {exch} if pop} bind def
/inch {72 mul} def
/pagedimen {
paperheight sub abs 16 lt exch
paperwidth sub abs 16 lt and
{/papername exch def} {pop} ifelse
} bind def
/papersizedict FMLOCAL
/setpapername {
/papersizedict 14 dict def
papersizedict begin
/papername /unknown def
/Letter 8.5 inch 11.0 inch pagedimen
/LetterSmall 7.68 inch 10.16 inch pagedimen
/Tabloid 11.0 inch 17.0 inch pagedimen
/Ledger 17.0 inch 11.0 inch pagedimen
/Legal 8.5 inch 14.0 inch pagedimen
/Statement 5.5 inch 8.5 inch pagedimen
/Executive 7.5 inch 10.0 inch pagedimen
/A3 11.69 inch 16.5 inch pagedimen
/A4 8.26 inch 11.69 inch pagedimen
/A4Small 7.47 inch 10.85 inch pagedimen
/B4 10.125 inch 14.33 inch pagedimen
/B5 7.16 inch 10.125 inch pagedimen
end
} bind def
/papersize {
papersizedict begin
/Letter {lettertray letter} def
/LetterSmall {lettertray lettersmall} def
/Tabloid {11x17tray 11x17} def
/Ledger {ledgertray ledger} def
/Legal {legaltray legal} def
/Statement {statementtray statement} def
/Executive {executivetray executive} def
/A3 {a3tray a3} def
/A4 {a4tray a4} def
/A4Small {a4tray a4small} def
/B4 {b4tray b4} def
/B5 {b5tray b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
statusdict begin stopped end
} bind def
/manualpapersize {
papersizedict begin
/Letter {letter} def
/LetterSmall {lettersmall} def
/Tabloid {11x17} def
/Ledger {ledger} def
/Legal {legal} def
/Statement {statement} def
/Executive {executive} def
/A3 {a3} def
/A4 {a4} def
/A4Small {a4small} def
/B4 {b4} def
/B5 {b5} def
/unknown {unknown} def
papersizedict dup papername known {papername} {/unknown} ifelse get
end
stopped
} bind def
/desperatepapersize {
statusdict /setpageparams known
{
paperwidth paperheight 0 1
statusdict begin
{setpageparams} stopped
end
} {true} ifelse
} bind def
/DiacriticEncoding [
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/.notdef /.notdef /.notdef /.notdef /space /exclam /quotedbl
/numbersign /dollar /percent /ampersand /quotesingle /parenleft
/parenright /asterisk /plus /comma /hyphen /period /slash /zero /one
/two /three /four /five /six /seven /eight /nine /colon /semicolon
/less /equal /greater /question /at /A /B /C /D /E /F /G /H /I /J /K
/L /M /N /O /P /Q /R /S /T /U /V /W /X /Y /Z /bracketleft /backslash
/bracketright /asciicircum /underscore /grave /a /b /c /d /e /f /g /h
/i /j /k /l /m /n /o /p /q /r /s /t /u /v /w /x /y /z /braceleft /bar
/braceright /asciitilde /.notdef /Adieresis /Aring /Ccedilla /Eacute
/Ntilde /Odieresis /Udieresis /aacute /agrave /acircumflex /adieresis
/atilde /aring /ccedilla /eacute /egrave /ecircumflex /edieresis
/iacute /igrave /icircumflex /idieresis /ntilde /oacute /ograve
/ocircumflex /odieresis /otilde /uacute /ugrave /ucircumflex
/udieresis /dagger /.notdef /cent /sterling /section /bullet
/paragraph /germandbls /registered /copyright /trademark /acute
/dieresis /.notdef /AE /Oslash /.notdef /.notdef /.notdef /.notdef
/yen /.notdef /.notdef /.notdef /.notdef /.notdef /.notdef
/ordfeminine /ordmasculine /.notdef /ae /oslash /questiondown
/exclamdown /logicalnot /.notdef /florin /.notdef /.notdef
/guillemotleft /guillemotright /ellipsis /.notdef /Agrave /Atilde
/Otilde /OE /oe /endash /emdash /quotedblleft /quotedblright
/quoteleft /quoteright /.notdef /.notdef /ydieresis /Ydieresis
/fraction /currency /guilsinglleft /guilsinglright /fi /fl /daggerdbl
/periodcentered /quotesinglbase /quotedblbase /perthousand
/Acircumflex /Ecircumflex /Aacute /Edieresis /Egrave /Iacute
/Icircumflex /Idieresis /Igrave /Oacute /Ocircumflex /.notdef /Ograve
/Uacute /Ucircumflex /Ugrave /dotlessi /circumflex /tilde /macron
/breve /dotaccent /ring /cedilla /hungarumlaut /ogonek /caron
] def
/ReEncode {
dup
length
dict begin
{
1 index /FID ne
{def}
{pop pop} ifelse
} forall
0 eq {/Encoding DiacriticEncoding def} if
currentdict
end
} bind def
FMPColor

{
/BEGINBITMAPCOLOR {
BITMAPCOLOR} def
/BEGINBITMAPCOLORc {
BITMAPCOLORc} def
/BEGINBITMAPTRUECOLOR {
BITMAPTRUECOLOR } def
/BEGINBITMAPTRUECOLORc {
BITMAPTRUECOLORc } def
}

{
/BEGINBITMAPCOLOR {
BITMAPGRAY} def
/BEGINBITMAPCOLORc {
BITMAPGRAYc} def
/BEGINBITMAPTRUECOLOR {
BITMAPTRUEGRAY } def
/BEGINBITMAPTRUECOLORc {
BITMAPTRUEGRAYc } def
}
ifelse
/K {
FMPrintAllColorsAsBlack {
dup 1 eq 2 index 1 eq and 3 index 1 eq and not
{7 {pop} repeat 0 0 0 1 0 0 0} if
} if
FrameCurColors astore
pop combineColor
} bind def
/graymode true def
/bwidth FMLOCAL
/bpside FMLOCAL
/bstring FMLOCAL
/onbits FMLOCAL
/offbits FMLOCAL
/xindex FMLOCAL
/yindex FMLOCAL
/x FMLOCAL
/y FMLOCAL
/setPatternMode {
FMLevel1 {
/bwidth exch def
/bpside exch def
/bstring exch def
/onbits 0 def /offbits 0 def
freq sangle landscape {90 add} if
{/y exch def
/x exch def
/xindex x 1 add 2 div bpside mul cvi def
/yindex y 1 add 2 div bpside mul cvi def
bstring yindex bwidth mul xindex 8 idiv add get
1 7 xindex 8 mod sub bitshift and 0 ne FrameNegative {not} if
{/onbits onbits 1 add def 1}
{/offbits offbits 1 add def 0}
ifelse
}
setscreen
offbits offbits onbits add div FrameNegative {1.0 exch sub} if
/FrameCurGray exch def
} {
pop pop
dup patCache exch known {
patCache exch get
} {
dup
patDict /bstring 3 -1 roll put
patDict
9 PatFreq screenIndex get div dup matrix scale
makepattern
dup
patCache 4 -1 roll 3 -1 roll put
} ifelse
/FrameCurGray 0 def
/FrameCurPat exch def
} ifelse
/graymode false def
combineColor
} bind def
/setGrayScaleMode {
graymode not {
/graymode true def
FMLevel1 {
setCurrentScreen
} if
} if
/FrameCurGray exch def
combineColor
} bind def
/normalize {
transform round exch round exch itransform
} bind def
/dnormalize {
dtransform round exch round exch idtransform
} bind def
/lnormalize {
0 dtransform exch cvi 2 idiv 2 mul 1 add exch idtransform pop
} bind def
/H {
lnormalize setlinewidth
} bind def
/Z {
setlinecap
} bind def

/PFill {
graymode FMLevel1 or not {
gsave 1 setgray eofill grestore
} if
} bind def
/PStroke {
graymode FMLevel1 or not {
gsave 1 setgray stroke grestore
} if
stroke
} bind def
/fillvals FMLOCAL
/X {
fillvals exch get
dup type /stringtype eq
{8 1 setPatternMode}
{setGrayScaleMode}
ifelse
} bind def
/V {
PFill gsave eofill grestore
} bind def
/Vclip {
clip
} bind def
/Vstrk {
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/N {
PStroke
} bind def
/Nclip {
strokepath clip newpath
} bind def
/Nstrk {
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/M {newpath moveto} bind def
/E {lineto} bind def
/D {curveto} bind def
/O {closepath} bind def
/n FMLOCAL
/L {
/n exch def
newpath
normalize
moveto
2 1 n {pop normalize lineto} for
} bind def
/Y {
L
closepath
} bind def
/x1 FMLOCAL
/x2 FMLOCAL
/y1 FMLOCAL
/y2 FMLOCAL
/R {
/y2 exch def
/x2 exch def
/y1 exch def
/x1 exch def
x1 y1
x2 y1
x2 y2
x1 y2
4 Y
} bind def
/rad FMLOCAL
/rarc
{rad
arcto
} bind def
/RR {
/rad exch def
normalize
/y2 exch def
/x2 exch def
normalize
/y1 exch def
/x1 exch def
mark
newpath
{
x1 y1 rad add moveto
x1 y2 x2 y2 rarc
x2 y2 x2 y1 rarc
x2 y1 x1 y1 rarc
x1 y1 x1 y2 rarc
closepath
} stopped {x1 y1 x2 y2 R} if
cleartomark
} bind def
/RRR {
/rad exch def
normalize /y4 exch def /x4 exch def
normalize /y3 exch def /x3 exch def
normalize /y2 exch def /x2 exch def
normalize /y1 exch def /x1 exch def
newpath
normalize moveto
mark
{
x2 y2 x3 y3 rarc
x3 y3 x4 y4 rarc
x4 y4 x1 y1 rarc
x1 y1 x2 y2 rarc
closepath
} stopped
{x1 y1 x2 y2 x3 y3 x4 y4 newpath moveto lineto lineto lineto closepath} if
cleartomark
} bind def
/C {
grestore
gsave
R
clip
setCurrentScreen
} bind def
/CP {
grestore
gsave
Y
clip
setCurrentScreen
} bind def
/FMpointsize FMLOCAL
/F {
FMfonts exch get
FMpointsize scalefont
setfont
} bind def
/Q {
/FMpointsize exch def
F
} bind def
/T {
moveto show
} bind def
/RF {
rotate
0 ne {-1 1 scale} if
} bind def
/TF {
gsave
moveto
RF
show
grestore
} bind def
/P {
moveto
0 32 3 2 roll widthshow
} bind def
/PF {
gsave
moveto
RF
0 32 3 2 roll widthshow
grestore
} bind def
/S {
moveto
0 exch ashow
} bind def
/SF {
gsave
moveto
RF
0 exch ashow
grestore
} bind def
/B {
moveto
0 32 4 2 roll 0 exch awidthshow
} bind def
/BF {
gsave
moveto
RF
0 32 4 2 roll 0 exch awidthshow
grestore
} bind def
/G {
gsave
newpath
normalize translate 0.0 0.0 moveto
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
PFill fill
grestore
} bind def
/Gstrk {
savematrix
newpath
2 index 2 div add exch 3 index 2 div sub exch
normalize 2 index 2 div sub exch 3 index 2 div add exch
translate
scale
0.0 0.0 1.0 5 3 roll arc
restorematrix
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/Gclip {
newpath
savematrix
normalize translate 0.0 0.0 moveto
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
clip newpath
restorematrix
} bind def
/GG {
gsave
newpath
normalize translate 0.0 0.0 moveto
rotate
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
PFill
fill
grestore
} bind def
/GGclip {
savematrix
newpath
normalize translate 0.0 0.0 moveto
rotate
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
clip newpath
restorematrix
} bind def
/GGstrk {
savematrix
newpath
normalize translate 0.0 0.0 moveto
rotate
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
restorematrix
currentlinewidth exch setlinewidth PStroke setlinewidth
} bind def
/A {
gsave
savematrix
newpath
2 index 2 div add exch 3 index 2 div sub exch
normalize 2 index 2 div sub exch 3 index 2 div add exch
translate
scale
0.0 0.0 1.0 5 3 roll arc
restorematrix
PStroke
grestore
} bind def
/Aclip {
newpath
savematrix
normalize translate 0.0 0.0 moveto
dnormalize scale
0.0 0.0 1.0 5 3 roll arc
closepath
strokepath clip newpath
restorematrix
} bind def
/Astrk {
Gstrk
} bind def
/AA {
gsave
savematrix
newpath

3 index 2 div add exch 4 index 2 div sub exch

normalize 3 index 2 div sub exch 4 index 2 div add exch
translate
rotate
scale
0.0 0.0 1.0 5 3 roll arc
restorematrix
PStroke
grestore
} bind def
/AAclip {
savematrix
newpath
normalize translate 0.0 0.0 moveto
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(GHRS Instrument Handbook 5.0) 207 60.29 T
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-2.78 (1) 541.87 60.29 P
-2.78 (15) 546.88 60.29 P
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0 10 Q
(1) 54 60.29 T
(16) 59.01 60.29 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(GHRS Instrument Handbook 5.0) 189 60.29 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 9 Q
(A) 54 681.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(Accumulation Mode) 54 672.33 T
(13, 19, 34, 43\32045) 132.74 672.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(CENSOR) 63 662.33 T
2 9 Q
(44) 103.5 662.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(details) 72 652.33 T
(95\32096) 100 652.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(CENSOR) 63 642.33 T
2 9 Q
(, see also noise rejection) 99 642.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(COMB) 63 632.33 T
2 9 Q
(15, 44) 91.5 632.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(DOPPLER) 63 622.33 T
2 9 Q
(44) 109.5 622.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(FP-SPLIT) 63 612.33 T
2 9 Q
(14, 30, 43, 44) 115.5 612.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(high signal-to-noise methods) 63 602.33 T
(107) 172 602.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(parameter summary) 63 592.33 T
(44) 139.23 592.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(STEP-PATT) 63 582.33 T
2 9 Q
(15, 44, 92, 1) 121.5 582.33 T
(14) 166.17 582.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(STEP-TIME) 63 572.33 T
2 9 Q
(44) 121.5 572.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(substepping) 63 562.33 T
(19) 110.5 562.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(acquisition parameters) 54 552.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(ACQ/PEAKUP) 63 542.33 T
2 9 Q
(, see acquisition parameters,) 122 542.33 T
3 10 Q
(PEAKUP) 225.98 542.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(BRIGHT) 63 532.33 T
2 9 Q
( and) 99 532.33 T
3 10 Q
(FAINT) 116.5 532.33 T
2 9 Q
( limits) 146.5 532.33 T
(17, 26, 37, 41) 173.76 532.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(calculating) 72 522.33 T
(68) 115.99 522.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(BRIGHT=RETURN) 63 512.33 T
2 9 Q
(17, 25, 34, 37, 41, 71) 145.5 512.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(BRIGHT=RETURN) 63 502.33 T
2 9 Q
( compared to specifying limits) 141 502.33 T
(37) 254.99 502.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(DEC-OFF) 63 492.33 T
2 9 Q
(40) 109.5 492.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(ETA-OFF) 63 482.33 T
2 9 Q
(40) 109.5 482.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(EXTENDED) 63 472.33 T
2 9 Q
(39) 115.5 472.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(LOCATE) 63 462.33 T
2 9 Q
(17, 41) 103.5 462.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(LOCATE=EXTENDED) 63 452.33 T
2 9 Q
(8) 157.5 452.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(MAP) 63 442.33 T
2 9 Q
(37, 40, 41, 42) 85.5 442.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(MAP=ALL-POINTS) 63 432.33 T
2 9 Q
(40) 151.5 432.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(PEAKUP) 63 422.33 T
2 9 Q
(15, 34, 38, 40, 41) 103.5 422.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(STEP-TIME) 72 412.33 T
2 9 Q
(71) 130.5 412.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(RA-OFF) 63 402.33 T
2 9 Q
(40) 103.5 402.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(SEARCH-SIZE) 63 392.33 T
2 9 Q
(36, 37, 40) 133.5 392.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Special Requirements) 63 382.33 T
(41) 146.24 382.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(STEP-TIME) 63 372.33 T
2 9 Q
(71) 121.5 372.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(for) 72 362.33 T
3 10 Q
(PEAKUP) 84.74 362.33 T
2 9 Q
(71) 125.24 362.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(maximum permitted) 72 352.33 T
(38) 149.75 352.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(STEP-TIME) 63 342.33 T
2 9 Q
(as) 123 342.33 T
3 10 Q
(COMMENT) 132.75 342.33 T
2 9 Q
(41) 179.25 342.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(summary) 63 332.33 T
(40) 101 332.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(XI-OFF) 63 322.33 T
2 9 Q
(40) 103.5 322.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(acquisitions) 54 312.33 T
(15, 17, 24, 34, 35\32041, 68\32080) 101.5 312.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(early) 63 302.33 T
(16, 18, 25, 35, 36) 85.49 302.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(extended objects) 63 292.33 T
(39, 76) 127.74 292.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(faint objects) 63 282.33 T
(39) 111.74 282.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(DARK TIME) 72 272.33 T
2 9 Q
(39, 80) 130.5 272.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Side 2 acquisition for Side 1 observing) 72 262.33 T
(8, 38) 216.49 262.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(using FOS) 72 252.33 T
(8, 39) 114.76 252.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(\337ux measurement) 63 242.33 T
(17) 131.74 242.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(initial pointing) 63 232.33 T
(35) 120.76 232.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(interactive) 63 222.33 T
(16, 18, 24, 35) 105.49 222.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(of) 63 212.33 T
(fseting) 70.33 212.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(and guide stars) 72 202.33 T
(40) 130.49 202.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(of) 63 192.33 T
(fsetting) 70.33 192.33 T
(36, 39) 101.83 192.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(onboard) 63 182.33 T
(17, 36, 40) 96.99 182.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(parameter summary) 63 172.33 T
(40) 139.23 172.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(real time, see acquisitions, interactive) 63 162.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(reddening) 63 152.33 T
(68) 103.49 152.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(see also tar) 63 142.33 T
(gets) 102.82 142.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(spiral search) 63 132.33 T
(36, 37) 112.73 132.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(tar) 63 122.33 T
(gets, see tar) 72.33 122.33 T
(gets) 114.41 122.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(apertures) 306 681.33 T
(12) 343.48 681.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(angular scale) 315 671.33 T
(9) 366.73 671.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(LSA) 315 661.33 T
(9, 12, 17, 18, 28, 34, 35, 36, 38, 41, 42, 85, 1) 336.5 661.33 T
(12) 498.17 661.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(shutter) 324 651.33 T
(12, 28) 353 651.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(nomenclature) 315 641.33 T
(9) 368.49 641.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(physical locations) 315 631.33 T
(58) 384.25 631.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(physical size) 315 621.33 T
(60) 365.74 621.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(plate scale) 315 611.33 T
(9) 357.24 611.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(SSA) 315 601.33 T
(9, 12, 17, 28, 34, 38, 41, 42, 1) 336.01 601.33 T
(14) 443.67 601.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(B) 306 582.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(background) 306 573.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(echelle interorder) 315 563.33 T
(19) 382.73 563.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(geocoronal L) 315 553.33 T
(yman-) 362.24 553.33 T
4 10 Q
(a) 385.24 553.33 T
2 9 Q
(80) 396.05 553.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(LSA shutter) 315 543.33 T
(12) 363.25 543.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(measurement) 315 533.33 T
(92) 367.49 533.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(scattered light) 315 523.33 T
(87, 88) 370.24 523.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(echelles) 324 513.33 T
(103) 357.49 513.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(bandpass) 306 503.33 T
(87, 88) 343.49 503.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(blaze function) 306 493.33 T
(91, 1) 361.74 493.33 T
(1) 379.4 493.33 T
(1) 383.57 493.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(C) 306 474.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(calibrations) 306 465.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(precision and accuracy) 315 455.33 T
(46) 401.97 455.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(wavelength) 315 445.33 T
(34, 47, 98) 360.99 445.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(aperture of) 324 435.33 T
(fsets) 363.07 435.33 T
(98) 384.07 435.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(contamination from SSA) 324 425.33 T
(98) 418.5 425.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(geomagnetic ef) 324 415.33 T
(fects) 379.07 415.33 T
(99) 400.56 415.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(lamps) 324 405.33 T
(98) 350 405.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(line widths) 324 395.33 T
(98) 368.25 395.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(tables) 324 385.33 T
(102) 349.5 385.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(thermal ef) 324 375.33 T
(fects) 360.58 375.33 T
(99) 382.07 375.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(carrousel) 306 365.33 T
(14) 343.48 365.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(CENSOR) 306 355.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 9 Q
(see noise rejection) 315 345.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Continuous V) 306 335.33 T
(iewing Zone) 355.72 335.33 T
(16, 1) 405.46 335.33 T
(12) 423.13 335.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(conventions) 306 325.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(text) 315 315.33 T
(7) 333 315.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(units) 315 305.33 T
(8) 337.01 305.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(coordinated observations) 306 295.33 T
(47) 400.73 295.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(cosmic rays) 306 285.33 T
(95) 353.24 285.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(CVZ, see Continuous V) 306 275.33 T
(iewing Zone) 391.96 275.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Cycle 5) 306 265.33 T
(1) 338.25 265.33 T
(1) 342.41 265.33 T
(1) 346.58 265.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(D) 306 246.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(DARK TIME) 306 237.33 T
2 9 Q
( Special Requirement) 360 237.33 T
(39, 80) 441.99 237.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(data quality) 306 227.33 T
(43) 352.75 227.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(deadtime correction) 306 217.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(see paired pulse correction) 315 207.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(deconvolution) 306 197.33 T
(103) 362 197.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(DEFCAL) 306 187.33 T
2 9 Q
(1) 346.5 187.33 T
(12) 350.67 187.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(detectors) 306 177.33 T
(60) 342.99 177.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(count rate linearity) 315 167.33 T
(98) 387.49 167.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(D1) 315 157.33 T
(14) 330.5 157.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(D2) 315 147.33 T
(14) 330.5 147.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(dark count) 315 137.33 T
(95) 357.74 137.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Digicon, see Digicon) 315 127.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(granularity) 315 117.33 T
(14) 358.99 117.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(image stability) 315 107.33 T
(98) 372.75 107.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(sampling) 315 97.33 T
(15) 352.5 97.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
FMENDPAGE
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[0 0 0 1 0 0 0]
[ 0 1 1 0 1 0 0]
[ 1 0 1 0 0 1 0]
[ 1 1 0 0 0 0 1]
[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
72 72 558 72 2 L
0.5 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
(GHRS Instrument Handbook 5.0) 207 60.29 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
-2.78 (1) 541.87 60.29 P
-2.78 (17) 546.88 60.29 P
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 9 Q
(Digicon) 72 681.33 T
(14) 105.5 681.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(paired pulse correction) 81 671.33 T
(71) 167.98 671.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(diodes) 72 661.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(corner) 81 651.33 T
(28, 92) 108.49 651.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(focus) 81 641.33 T
(42, 43, 1) 104.99 641.33 T
(12) 136.16 641.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(science) 81 631.33 T
(92) 111.99 631.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(diodes, corner) 72 621.33 T
(1) 127.49 621.33 T
(1) 131.65 621.33 T
(1) 135.82 621.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Doppler shift) 72 611.33 T
(19, 44, 46) 124.25 611.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(E) 72 592.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(early acquisition, see acquisitions, early) 72 583.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(e-mail addresses) 72 573.33 T
(2) 136.23 573.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(exposure time calculation) 72 563.33 T
(26) 168.98 563.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(extinction, ultraviolet) 72 553.33 T
(93, 102) 154 553.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(F) 72 534.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(\337uxes, variable) 72 525.33 T
(18) 131.49 525.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(FLYLIM) 72 515.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 9 Q
(see noise rejection) 81 505.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(FOC) 72 495.33 T
(18, 24, 35, 36, 43) 94 495.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(G) 72 476.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(geocoronal L) 72 467.33 T
(yman-) 119.24 467.33 T
4 10 Q
(a) 142.24 467.33 T
2 9 Q
(27, 80, 105) 153.05 467.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(geomagnetically-induced image motion) 72 457.33 T
(47, 98, 1) 219.48 457.33 T
(12) 250.65 457.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(GHRS) 72 447.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(as slitless spectrograph) 81 437.33 T
(43) 168.49 437.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(paired pulse correction) 81 427.33 T
(71) 167.98 427.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(photometric precision) 81 417.33 T
(13) 164.24 417.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Point Spread Function) 81 407.33 T
(94) 166.01 407.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(resolving power) 81 397.33 T
(12, 83, 103) 143.74 397.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(scienti\336c papers) 81 387.33 T
(104) 143.74 387.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(STScI contacts) 81 377.33 T
(2) 139.74 377.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(technical papers) 81 367.33 T
(102) 143.73 367.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(time resolution) 81 357.33 T
(13) 139.75 357.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(useful wavelength range) 81 347.33 T
(12) 173.48 347.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(granularity) 72 337.33 T
(14) 115.99 337.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(gratings) 72 327.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(cross-dispersers) 81 317.33 T
(60) 142.98 317.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Ech-A) 81 307.33 T
(87) 108.99 307.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Ech-B) 81 297.33 T
(88) 108.5 297.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(echelle) 81 287.33 T
(12, 14, 60) 110.99 287.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(bandpass and sensitivity) 90 277.33 T
(87) 182 277.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(blaze function) 90 267.33 T
(91, 1) 145.74 267.33 T
(1) 163.4 267.33 T
(1) 167.57 267.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(resolving power) 90 257.33 T
(83) 152.74 257.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(scattered light) 90 247.33 T
(87) 145.24 247.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(wavelength format) 90 237.33 T
(89) 162.23 237.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(\336rst-order) 81 227.33 T
(12, 14, 60, 85) 121.49 227.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(resolving power) 90 217.33 T
(83) 152.74 217.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(useful ranges) 90 207.33 T
(83) 142.24 207.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(holographic) 81 197.33 T
(14) 128.49 197.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(GSC) 72 187.33 T
(35, 1) 94 187.33 T
(12) 111.67 187.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(H) 72 168.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(HST memory capacity) 72 159.33 T
(13, 16, 47) 157.99 159.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(I) 324 681.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(IMAGE Mode) 324 672.33 T
(16, 20, 40, 42\32043) 381.24 672.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(as slitless spectrograph) 333 662.33 T
(43) 420.49 662.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(critically sampling) 333 652.33 T
(42) 404.75 652.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(DELTA-X, DELTA-Y) 333 642.33 T
2 9 Q
(42) 433.5 642.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(maximum) 333 632.33 T
3 10 Q
(STEP-TIME) 371.75 632.33 T
2 9 Q
(43) 430.25 632.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(NX, NY) 333 622.33 T
2 9 Q
(42) 373.5 622.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(parameter summary) 333 612.33 T
(42) 409.23 612.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(PRECISION) 333 602.33 T
2 9 Q
(43) 391.5 602.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(interactive acquisitions, see acquisitions, interactive) 324 592.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(L) 324 573.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(Lar) 324 564.33 T
(ge Science Aperture, see apertures, LSA) 336.33 564.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Line Spread Function \050LSF\051) 324 554.33 T
(103) 430.24 554.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(M) 324 535.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(MAP) 324 526.33 T
(, see acquisition parameters,) 342.5 526.33 T
3 10 Q
(MAP) 446.48 526.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 9 Q
(mirrors) 324 516.33 T
(36, 40, 42, 60) 355 516.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(A1) 333 506.33 T
(14, 25) 348.5 506.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(A2) 333 496.33 T
(14) 348.5 496.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(attenuated) 333 486.33 T
(14) 374.49 486.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Cam-A) 333 476.33 T
(14) 364 476.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Cam-B) 333 466.33 T
(14) 363.5 466.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(ef) 333 456.33 T
(fective areas) 339.83 456.33 T
(78) 389.56 456.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(N1) 333 446.33 T
(14) 348.5 446.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(N2) 333 436.33 T
(14) 348.5 436.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(normal) 333 426.33 T
(14) 363 426.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(moving tar) 324 416.33 T
(ges, see tar) 363.09 416.33 T
(gets, moving) 402.66 416.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(N) 324 397.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(NO GAP) 324 388.33 T
2 9 Q
( Special Requirement) 360 388.33 T
(34) 441.99 388.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(noise rejection) 324 378.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(CENSOR) 333 368.33 T
2 9 Q
(27, 95) 373.5 368.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(FLYLIM) 333 358.33 T
2 9 Q
(9, 27, 45, 97) 373.5 358.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(noise, \336xed-pattern) 324 348.33 T
(30) 397.99 348.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(O) 324 329.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(OSCAN Mode) 324 320.33 T
(20, 45) 382.25 320.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(see also parameters for Accumulation Mode) 333 310.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(OSS) 324 300.33 T
(1) 345.01 300.33 T
(12) 349.17 300.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(P) 324 281.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(paired pulse correction) 324 272.33 T
(71) 410.98 272.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(peakup, see acquisition parameters,) 324 262.33 T
3 10 Q
(PEAKUP) 453.97 262.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 9 Q
(Phase I) 324 252.33 T
(22, 1) 354.74 252.33 T
(13) 372.41 252.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(acquisitions) 333 242.33 T
(24) 380.5 242.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Phase II) 324 232.33 T
(22, 1) 357.74 232.33 T
(13) 375.41 232.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(photometric precision) 324 222.33 T
(13) 407.24 222.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(plate scale) 324 212.33 T
(9) 366.24 212.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Point Spread Function) 324 202.33 T
(94, 103) 409.01 202.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(R) 324 183.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(RAPID Mode) 324 174.33 T
(13, 16, 20, 45, 46) 378.75 174.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(SAMPLE-TIME) 333 164.33 T
2 9 Q
(20, 46) 403.5 164.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Rapid Readout Mode, see RAPID Mode) 324 154.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(reddening) 324 144.33 T
(27, 93, 102) 364.49 144.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(ef) 333 134.33 T
(fect on acquisition count rates) 339.83 134.33 T
(68) 452.31 134.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(resolution, time) 324 124.33 T
(13) 385 124.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(resolving power) 324 114.33 T
(12, 83) 386.74 114.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(ripple function) 324 104.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(see blaze function) 333 94.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
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[ 0 1 1 0 1 0 0]
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[ 1 0 0 0 0 1 1]
[ 0 1 0 0 1 0 1]
[ 0 0 1 0 1 1 0]
7 FrameSetSepColors
FrameNoSep
0 0 0 1 0 0 0 K
54 72 540 72 2 L
0.5 H
2 Z
0 X
0 0 0 1 0 0 0 K
N
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 10 Q
(1) 54 60.29 T
(18) 59.01 60.29 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(GHRS Instrument Handbook 5.0) 189 60.29 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 9 Q
(S) 54 681.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(SAA, see South Atlantic Anomaly) 54 672.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(sampling) 54 662.33 T
(15) 91.5 662.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(scattered light) 54 652.33 T
(28, 87, 88) 109.24 652.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(SEARCH-SIZE) 54 642.33 T
2 9 Q
(, see acquisition parameters,) 120 642.33 T
3 10 Q
(SEARCH-) 223.98 642.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(SIZE) 72 632.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 9 Q
(sensitivity) 54 622.33 T
(26) 95.51 622.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(sensitivity function) 54 612.33 T
(85) 127.75 612.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Side 1) 54 602.33 T
(8, 12, 1) 81.25 602.33 T
(13) 107.92 602.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Side 2) 54 592.33 T
(12, 1) 81.25 592.33 T
(13) 98.92 592.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(signal-to-noise estimation) 54 582.33 T
(29) 151.75 582.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(slitless spectrograph mode) 54 572.33 T
(43) 153.99 572.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Small Science Aperture, see apertures, SSA) 54 562.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(South Atlantic Anomaly) 54 552.33 T
(16, 19, 27, 95, 1) 146.5 552.33 T
(13) 204.67 552.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(spectrograph temperature) 54 542.33 T
(47) 150.22 542.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(Spectrum Y Balance, see) 54 532.33 T
3 10 Q
(SPYBAL) 146.73 532.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 9 Q
(spiral search, see acquisitions, spiral search) 54 522.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(SPYBAL) 54 512.33 T
2 9 Q
(19, 1) 94.5 512.33 T
(13) 112.17 512.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(STEIS) 54 502.33 T
(10, 1) 82.5 502.33 T
(14) 100.17 502.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(STEP-TIME) 54 492.33 T
2 9 Q
(1) 112.5 492.33 T
(14) 116.67 492.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(substepping) 54 482.33 T
(92) 101.5 482.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(T) 54 463.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(tar) 54 454.33 T
(gets) 63.33 454.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(bright problems) 63 444.33 T
(25) 124.75 444.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(complex) 63 434.33 T
(38) 98.5 434.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(coordinates) 63 424.33 T
(18) 108.99 424.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(crowded \336elds) 63 414.33 T
(25, 35) 120.24 414.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(extended) 63 404.33 T
(8, 18, 26) 99.99 404.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(faint) 63 394.33 T
(26, 39) 84 394.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(moving) 63 384.33 T
(18, 25, 35) 95 384.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(nearby neighbors) 63 374.33 T
(18) 129.74 374.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(of) 63 364.33 T
(fsetting) 70.33 364.33 T
(36, 39) 101.83 364.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(point source) 63 354.33 T
(36) 111.74 354.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(variable) 63 344.33 T
(18, 26, 35) 96.49 344.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(T) 54 334.33 T
(ar) 58.87 334.33 T
(gets of Opportunity) 65.7 334.33 T
(47) 140.7 334.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(telephone numbers) 54 324.33 T
(2) 126.74 324.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(time resolution) 54 314.33 T
(13) 112.75 314.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 F
(W) 54 295.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
2 F
(wavelength tables) 54 286.33 T
(102) 123.24 286.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(WFPC2) 54 276.33 T
(18, 24, 35, 36) 87.51 276.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(WSCAN Mode) 54 266.33 T
(20, 45) 114.25 266.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
(see also parameters for Accumulation Mode) 63 256.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
3 10 Q
(WAVE-STEP) 63 246.33 T
2 9 Q
(45) 121.5 246.33 T
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
0 0 0 1 0 0 0 K
FMENDPAGE
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