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1. http://www.stsci.edu/documents/dhb/web/c32_wfpc2dataanal.fm3.html
... WFPC2 has a polarizer filter which can be used for wide-field polarimetric imaging from about 200 through 700 nm. This filter is a quad , meaning that it consists of four panes, each with the polarization angle oriented in a different direction, in steps of 45o. The panes are aligned with the edges of the pyramid, thus each pane corresponds to a chip. ... Accurate calibration of WFPC2 polarimetric data is rather complex, due to the design of both the polarizer filter and the instrument itself. ...
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Ссылки http://www.stsci.edu/documents/dhb/web/c32_wfpc2dataanal.fm3.html -- 6.2 Кб -- 01.07.1998
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2. http://www.stsci.edu/~dejong/gzip/proc184.ps.gz
CORES OR CUSPS IN ELLIPTICAL GALAXIES: LUMINOSITY OR ENVIRONMENT? ... The low lumi nosity disky galaxies have `hard' cores with a steep slope in the luminosity profile at small radii, whereas the luminous galaxies have `soft' cores with flat profiles at small radii (e.g. Faber et al. ... Coma Cluster cores In the gas/stellar continuum paradigm, one would expect that in the outer parts of a cluster it is more likely that the last merger was gaseous than in its central regions. ...
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Ссылки http://www.stsci.edu/~dejong/gzip/proc184.ps.gz -- 26.2 Кб -- 18.12.2007
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3. http://www.stsci.edu/hst/wfc3/documents/ISRs/WFC3-2009-17.pdf
ST-ECF Instrument Science Report WFC3-2009-17 WFC3 SMOV proposal 11552: Calibration of the G141 grism H. Kuntschner, H. Bushouse, M. KЭmmel, J. R. Walsh October 16, 2009 A BSTR A C T Based on the SMOV observations, the performance of the WFC3 near-IR grism G141 has been assessed. ... Figure 2: Image of the G141 grism exposure (iab908s4q_flt.fits). ... 12 2 ST-ECF Technical Instrument Report WFC3-2009-17 Figure 5: Linear fit for the wavelength solution of the G141 grism. ...
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Ссылки http://www.stsci.edu/hst/wfc3/documents/ISRs/WFC3-2009-17.pdf -- 1634.9 Кб -- 19.11.2009
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4. http://www.stsci.edu/ftp/meetings/apn3/LatexSummary.ps
... Some of these commands are L A T E X macros, while oth ers belong to plain T E X; no attempt to differen tiate them is made. ``/ --- ordinary space after period. ``! --- negative thin space = \Gamma 1 6 quad; xx``!x yields xxx (math mode). ``'' makes an umlaut, as Ёo. ``# prints a pound sign: #. ``$ prints a dollar sign: $. ``% prints a percent sign: %. ``& prints an ampersand: &. ``' in tabbing environment moves current column to the right of the previous column. ... math mode). ``phi is OE. ...
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Ссылки http://www.stsci.edu/ftp/meetings/apn3/LatexSummary.ps -- 218.6 Кб -- 09.09.2003
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5. http://www.stsci.edu/~mutchler/documents/ASP_Ceres_Pluto.pdf
... 70 · Winter 2007 www.astrosociety.org/uitc © 2007, Astronomical Society of the Pacific 390 Ashton Avenue, San Francisco, CA 94112 Hubble Observations of Ceres and Pluto: A Closer Look at the "Ugly Ducklings" of the Solar System by Max Mutchler Space Telescope Science Institute Introduction regret that my 4th Grade teacher, Mrs. Hadley, doesn't know that she provided me with the very first astronomy book that I ever read, because it had a profound impact on me. ... Planet count 7 6 7 11 12 13 8 9 9? ...
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Ссылки http://www.stsci.edu/~mutchler/documents/ASP_Ceres_Pluto.pdf -- 2511.9 Кб -- 19.02.2007
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6. http://www.stsci.edu/ftp/software/tex/aasmacros/aaspp4.sty
... Use 11pt or 12pt documentstyle option.} \fi \fi \ def \ps@plaintop{\let\@mkboth\@gobbletwo \ def \@oddfoot{}\ def \@oddhead{\rm\hfil--\ space \thepage\ space --\hfil} \ def \@evenfoot{}\let\@evenhead\@oddhead} \ps@plaintop \pretolerance=10000 \@rightskip=\z@ plus 4em\rightskip\@rightskip \textwidth=6 ... \textheight=8.4in \topmargin=0in \headheight=.15in \headsep=.35in \oddsidemargin=0in \evensidemargin=0in \parindent=2em \parskip=1.5ex \ def \@tightleading{1.1} \ ... B$}} \def\bv{\hbox{$B\!- ...
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Ссылки http://www.stsci.edu/ftp/software/tex/aasmacros/aaspp4.sty -- 18.2 Кб -- 14.08.1995
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7. http://www.stsci.edu/~ariess/documents/1998.pdf
THE ASTRONOMICAL JOURNAL, 116 : 1009 х1038, 1998 September ( 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A. OBSERVATIONAL EVIDENCE FROM SUPERNOVAE FOR AN ACCELERATING UNIVERSE AND A COSMOLOGICAL CONSTANT ADAM G. RIESS,1 ALEXEI PETER M. GARNAVICH,2 B. LEIBUNDGUT,6 M. R. V. FILIPPENKO,1 PETER CHALLIS,2 ALEJANDRO CLOCCHIATTI,3 ALAN DIERCKS,4 RON L. GILLILAND,5 CRAIG J. HOGAN,4 SAURABH JHA,2 ROBERT P. KIRSHNER,2 M. PHILLIPS,7 DAVID REISS,4 BRIAN P. SCHMIDT,8,9 ROBERT A.
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Ссылки http://www.stsci.edu/~ariess/documents/1998.pdf -- 1319.8 Кб -- 26.07.2007
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8. http://www.stsci.edu/~marel/decadal/sc/352.pdf
... Complex astrophysical phenomena could now be studied spectroscopically: the X-ray absorption line forest intrinsic to Seyfert galaxies; the interaction between AGN jets and intracluster media; hot winds of starburst galaxies; stellar coronal plasmas; the charge -exchange emission of Mars' exosphere; the X-ray irradiation of protoplanetary disks; and the myst erious flat-topped spectral line shapes of O star winds. ... We estimate that Gen-X will be able to detect and resolve 20, 000 stars in NGC...
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Ссылки http://www.stsci.edu/~marel/decadal/sc/352.pdf -- 434.2 Кб -- 20.02.2009
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