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http://www.stsci.edu/~golim/papers/leggett2007.pdf.

1. What effect does the color index of the target have on the observed Transfer
... HST . What effect does the color index of the target have on the observed Transfer Function? ... HST Peer Review Process . ... HST Overview . Overview . ... Phase I Proposing . ... Phase II Cycle 23 . ... Retrieving HST Data . ... HST Science Year in Review . ... A: The effect of color index on the Transfer Function is an expansion (for red stars) and a contraction (for blue stars) of the observed Transfer Function with respect to a Transfer Function of a target of moderate (B-V=0.5) color. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/fgs/faqs/calib2.faq -- 14.6 Кб -- 10.04.2016
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2. http://www.stsci.edu/hst/acs/documents/isrs/isr0103.pdf
ST-ECF Instrument Science Report ACS 2001-003 ACS Grism Simulations using SLIM 1.0 N. Pirzkal, A. Pasquali, J. R. Walsh, R. N. Hook, W. Freudling, R. Albrecht, R.A.E. Fosbury April 4, 2001 ABSTRACT We introduce SLIM, a slitless spectroscopy simulator written in Python which can be used to simulate the ACS grism and prism modes. ... We have thus developed a simulator called SLIM which is able to disperse an input spectrum in a well-controlled manner. ... Can simulate multiple order grism observations. ...
[ Текст ]  Ссылки http://www.stsci.edu/hst/acs/documents/isrs/isr0103.pdf -- 278.5 Кб -- 08.01.2007
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3. 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. ...
[ Текст ]  Ссылки http://www.stsci.edu/~dejong/gzip/proc184.ps.gz -- 26.2 Кб -- 18.12.2007
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4. 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.
[ Текст ]  Ссылки http://www.stsci.edu/~ariess/documents/1998.pdf -- 1319.8 Кб -- 26.07.2007
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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? ...
[ Текст ]  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/~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...
[ Текст ]  Ссылки http://www.stsci.edu/~marel/decadal/sc/352.pdf -- 434.2 Кб -- 20.02.2009
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7. 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: $. ``% prints a percent sign: %. ``& prints an ampersand: &. ``' in tabbing environment moves current column to the right of the previous column. ... math mode). ``phi is OE. ...
[ Текст ]  Ссылки http://www.stsci.edu/ftp/meetings/apn3/LatexSummary.ps -- 218.6 Кб -- 09.09.2003
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8. http://www.stsci.edu/ftp/software/tex/aasmacros/aaspp4.sty
... Use 11pt or 12pt documentstyle option.} \fi \fi \ def \ps@plaintop{\let\@mkboth\@gobbletwo \ def \@oddfoot{}\ def \@oddhead{\rm\hfil--\ space \thepage\ space --\hfil} \ def \@evenfoot{}\let\@evenhead\@oddhead} \ps@plaintop \pretolerance=10000 \@rightskip=\z@ plus 4em\rightskip\@rightskip \textwidth=6 ... \textheight=8.4in \topmargin=0in \headheight=.15in \headsep=.35in \oddsidemargin=0in \evensidemargin=0in \parindent=2em \parskip=1.5ex \ def \@tightleading{1.1} \ ... B$}} \def\bv{\hbox{$B\!- ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/software/tex/aasmacros/aaspp4.sty -- 18.2 Кб -- 14.08.1995
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