/ftp/cats/J_other/PASP/106/646



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J/PASP/106/646   HST quasar absorption-line key project. VIII. (Kirhakos+, 1994)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table1.dat table2.dat notes.dat
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Query from: http://vizier.cds.unistra.fr/cgi-bin/VizieR?-source=J/PASP/106/646
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drwxr-xr-x 12 cats archive 231 Jul 15 2016 [Up] drwxr-xr-x 2 cats archive 319 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 493 Dec 19 2022 .message -r--r--r-- 1 cats archive 6326 Mar 23 2001 ReadMe -rw-r--r-- 1 cats archive 494 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 3831 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 1834 Jun 30 2000 notes.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 3681 Nov 7 2000 table1.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 29563 Mar 23 2001 table2.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/PASP/106/646 HST quasar absorption-line key project. VIII. (Kirhakos+, 1994) ================================================================================ The HST quasar absorption-line key project. VIII. CCD imaging of Hubble Space Telescope quasar fields. Kirhakos S., Sargent W.L.W., Schneider D.P., Bahcall J.N., Jannuzi B.T., Maoz D., Small T.A. <Publ. Astron. Soc. Pac. 106, 646 (1994)> =1994PASP..106..646K ================================================================================ ADC_Keywords: QSOs ; Redshifts ; Photometry, CCD Abstract: We present an analysis of CCD images (obtained at the Palomar 1.5m telescope) of more than 100 quasars; many of the objects have been or will be observed in the HST Key Project Quasar Absorption-Line Survey. The data set consists of B, g, and i photometry of 117 quasars and deeper g (limiting magnitude of  22) images of 101 quasar fields. Positions accurate to  1", measured with the Space Telescope Science Institute's Astrometric Support Program, are listed for all of the quasars in this study. Positions, magnitudes, and classifications of stars and galaxies located within  100" of the quasars are given for all of the deep g data. The positions of the stars and galaxies relative to the quasar are accurate to  0.5". The results presented here can be used to prepare spectroscopic programs designed to obtain redshifts of galaxies in the fields of these quasars.