|
Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://mavr.sao.ru/hq/lsfvo/devices/mpfs/MPFS_V1/node45.html
Дата изменения: Unknown Дата индексирования: Fri Dec 28 19:24:50 2007 Кодировка: koi8-r Поисковые слова: cygnus |
Program for masking `hot spots` on CCD data
(C) SAO AS USSR VLVSoft 1991
Usage : COSMETIC.EXE [-x sizex] [-y sizey] [namein] [nameout] [maskname]
where sizex - size of input image along X-direction( default= 512)
sizey - size of input image along Y-direction( default= 512)
namein - name of input file
nameout - name of output result file
maskname - name of text file with masks of 'hot spots' and defects
COSPAR
Program for analysing cosmic hits on CCD data
(C) SAO Russian AS VLVSoft 1993
Usage : COSPAR.EXE [-x sizex][-y sizey][namein1][namein2][maskname][-d dev]
where sizex - size of input image along X-direction( default= 530)
dev - deviation parameter ( default - from console)
sizey - size of input image along Y-direction( default= 580)
namein1 - name of input file N1
namein2 - name of input file N2
maskname - name of result file with mask of hits
CREATSP
Program for creating of image with spectra' strobes
(C) SAO Russian AS,Marseille Observatory VLVSoft v.01 18-11-1994
Usage : CREATSP.EXE [-w wid] [-x sizex] [-y sizey] [filgeo]
where filgeo - name of text file with coefficients of polynoms
(default name - geometry.exa)
sizex,sizey - size of result image on both coordinates
(default = 530 580)
wid - width of modelled spetra ( by default = sigma*3.0)
CVIZ
Program for CIGALE/TIGER/PYTHEAS data cubes managing and processing
(C) SAO Russian AS VLVSoft v.1.03 08-02-95
Usage : CVIZ.EXE [-e] [-s] [-w wmin wmax] [-x xleft xright] [-y ytop ybot]
[-r][-f widfact][-d][-a][-c contnam][name1][name2][...nameN]
where wmin,wmax - limits of argument for all profiles
xleft,xright,ytop,ybot - leftmost,rightmost,upper
and lower showed profiles
name1,name2,...nameN - name of files with data cubes
contnam - name of cube with continuum values
widfact - factor of component widths transform (default = 1)
Key -e indicates on work in EGA-mode with VGA adapter
Key -s suggests fixed order of components (as set in GAUSAN.EXE)
Key -r provides automatical restoring of last approximation in GAUSAN
Key -d provides using of variable doublet parameters in GAUSAN
Key -a provides quiet mode for wavelength in GAUSAN
FVIZ
Program for image vizualization and some processing
(C) SAO Russian AS VLVSoft v.05 27-01-95
Usage : FVIZ.EXE [-e] [-w] [-f|l] [-x Xcen] [-y Xcen] [-s Scale] [-n|N]
[-h hdlen][-m][-p Numpal][-t Twait][name1] [name2]...
where Xcen,Ycen,Scale - coordinates of center and scale for image fragment
hdlen - length of image file header (default=0)
name1 - name of file with image
name2,..- names of next workfiles(default - no)
Numpal - number of palette will be used by default
Twait - time of waiting for any user's action (default - no)
Key -e indicates on work in EGA-mode with VGA adapter
Key -w permits writing to image file
Keys -f & -l indicate on output first or last image fragment
Keys -n and -N allow output symbol data while repers coordinates
re-reading from disk file
Key -m provides definition of color level even service file exists
GAUEXT
Program for gaussian spectra extraction from detector frame
(C) SAO Russian AS VLVSoft v.02 09-02-1995
Usage: GAUEXT.EXE [-b left right] [-n numsp]inpimage resfile
[filgeo] [-d] [-y shiftY][-w AddWid]
where left,right - borders for integrating (default = 5 MX-0)
numsp - amount of adjacent spectra ( default = 3)
inpimage - name of file with input image
filgeo - file with spectra' geometrical params(default - geometry.exa)
resfile - file with result spectra
shiftY - shift of extration zone on Y (default = 0)
AddWid - additional part into spectra width ( default = 0.0)
Key -d using for producing of additional information
GEOPREP
Program for preparing of geometry data for bidimensional spectra
(C) SAO Russian AS,KPNO,Marseille VLVSoft v.02 1993
Usage: GEOPREP.EXE [-f] [-r numrep] [-p power] [-x sizex] [-y sizey]
[-nosort] [filgeo] [filpos] [filnum] [geores]
where filgeo - name of text file with repers' coordinates
filpos - name of text file with measured position of individual spectra
filnum - name of text file with associated numbers of spectra
geores - name of file with result : coefficients for each spectrum
(default - geometry.pol)
numrep - amount of repers in one line of repers' grid (default = 7)
power - power of approximating bidimensional polynom (default = 3)
sizex,sizey - size of result image on both coordinates
(default = 512 512)
Using of key -nosort prevents sorting of input file with
repers' coordinates
Key -f provides writing additional data to file geometry.tmp
Using -F produce additonal image file strobe.dat (512 by 512 px)
with predicted spectra' position
GAUSAN
Program for Gauss-decomposition of vector data
(C) SAO Russian AS VLVSoft v.04 10-02-1995
Usage : GAUSAN.EXE [-x xmin xmax] [-w wave0] [-d dist relamp relwid] [-e]
[-r] [-f widfact] [-a] [-F] filnam
where xmin,xmax - min&max argument values (default - from file *.PAR)
wave0 - restframe wavelength
dist,relamp,relwid - distance and relations for doublet's components
widfact - factor of width transform while it restoring
filnam - name of input file
Key -e indicates on using EGA-mode (default - VGA)
Using of key -r provide restoring of parameters from gaus_sol.res
Using of key -D instead of -d provides FIXED values for doublets !
The same for key -F : first entered parameters will be used everythere
Using of key -a allows to avoid question about rest wavelength
IMAR
Program for image arithmetics
(C) SAO Russian AS VLVSoft 18-11-1994
Usage: IMAR.EXE [operation] [filnam1] [filnam2] [filnam3]
[const1] [const2] [const3]
where operation - (+,-,/,*,-lg,-ln)
filnam1 - name of input image 1
filnam2 - name of input image 2
filnam3 - name of output image
const1,const2,const3 - constants for calculation
Size of output image equals size of original
LINID
(C) SAO Russian AS VLVSoft v.05 24-01-1995
Usage: LINID.EXE [-p pow][-l len][-w wid][-d|-D disp][-a][-s][-f][-z]
[-e][-m maskfil][-y min max][-c filcoef]
[compspec lintab] [inspec outspec]
where pow - power of dispersion approximating polynom(max=6) (default=2)
len - length of input spectrum ( default - from file)
wid - width of instrumental profile(default=5)
min,max - limits for comparison spectrum respresentation
filcoef - file with coefficients channels = > wavelength
compspec - name of file with comparison spectrum
lintab - table of spectral lines wavelength
inspec - input spectrum to be linearized
outspec - result of linearization
maskfil - file with lines' positions
Key -d indicates on input value of dispersion by user
When key -D is using, necessary set dispersion value(in A/pix)
Key -a executes automatic procedure with lines` mask
and wavelength from lintab
Key -f provides precise background estimating in each line centering
Key -s indicates on using details in object`s spectrum in forming
disp.curve only in manual program mode
Key -z provides using same values (x0,dx,step) for all linearizes data
When key -c is applying, comspec & lintab must be omitted
PRFTEST
Program for spectra parameters determination over detector frame
(C) SAO Russian AS VLVSoft v.02 09-01-1995
Usage : PRFTEST.EXE [-w width][-b left right] [-n numsp] inpimage
[filgeo][-d][-a AmpLim][-y YcrdLim][-f FWHMLim][-p power]
where width - height of integration aperture(default=5,<30)
left,right - borders for integrating (default = 10 MX-0)
numsp - amount of adjacent spectra ( default = 3)
inpimage - name of file with input image
filgeo - file with spectra' geometrical params(default - geometry.pol)
AmpLim, YcrdLim, FWHMLim - limits for max.variation of profile params
by defaults - 0.9 1.0 0.5
power - order of approximating polynoms ( default - 3)
Using of key -d provides extended output of results
PRFTESTO
Program for spectra parameters determination over detector frame
(C) SAO Russian AS VLVSoft v.03 08-02-1995
Usage: PRFTESTO.EXE [-w width][-b left right] [-n numsp][-p Numfrag]inpimage
[filgeo][-a AmpLim][-y YcrdLim][-f FWHMLim]
where width - height of integration aperture(default=5,<30)
left,right - borders for integrating (default = 5 MX-0)
numsp - amount of adjacent spectra ( default = 3)
Numfrag - number of fragments for spectra dividing (default = 21)
inpimage - name of file with input image
filgeo - file with spectra' geometrical params(default - geometry.pol)
AmpLim, YcrdLim, FWHMLim - limits for max.variation of profile params
by defaults - 1.00 0.50 0.75
SPEXTR
Program for spectra extraction from detector frame
(C) SAO Russian AS VLVSoft v.02 1993
Usage: SPEXTR.EXE [-w width][-b left right][-s SlitStep]
[inpimage][resfile][filgeo]
where width - height of integration aperture(default=5,<100)
left,right - borders for integrating (default = 20 MX-0)
SlitStep - step for slit function producing (default = 1)
inpimage - name of file with input image
filgeo - file with spectra' geometrical params(default - geometry.pol)
resfile - file with result spectra
<
/SMALL>