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http://www.stsci.edu/instruments/wfpc2/Wfpc2_hand2/ch5_psf5.html.
http://www.stsci.edu/instruments/wfpc2/Wfpc2_hand2/ch5_psf5.html.
1. CCD Pixel Response Function
... Further testing, by covering a flight spare CCD with a 2 ? m pinhole grid in an opaque metallic mask and illuminating it with a flat field source, showed that even when a pinhole was centered over a pixel only about 70% of the light was detected in that pixel. ... Alternatively, at least in the V band, it can be modeled by convolving a simulated image by the following kernel, which gives the pixel response function averaged within pixels: . ... m pinhole grid test get worse at longer wavelengths. ...
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Ссылки http://www.stsci.edu/instruments/wfpc2/Wfpc2_hand4/ch5_psf5.html -- 6.1 Кб -- 04.09.2001
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2. http://www.stsci.edu/hst/acs/analysis/STECF/isr/isr0603.pdf
ST-ECF Instrument Science Report ACS-2006-03 Wavelength and Flux calibration of the ACS/HRC PR200L prism S. S. Larsen, J. Walsh and M. KЭmmel, March 2006 ABSTRACT Wavelength- and flux calibrations are presented for the ACS/HRC PR200L slitless spectroscopy mode. ... Wavelength solutions for the PR200L prism. ... Wavelength. ... 12 ST-ECF Instrument Science Report ACS-2006-03 Figure 7: Comparison of the aXe-extracted prism spectra of the two flux standards with the reference spectra. ...
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Ссылки http://www.stsci.edu/hst/acs/analysis/STECF/isr/isr0603.pdf -- 788.6 Кб -- 02.12.2010
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3. 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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4. 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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5. 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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6. 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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7. 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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