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The Sloan Digital Sky Survey Quasar Catalog. IV. Fifth Data Release

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Donald P. Schneider1, Patrick B. Hall2, Gordon T. Richards3,4, Michael A. Strauss5, Daniel E. Vanden Berk1, Scott F. Anderson6, W. N. Brandt1, Xiaohui Fan7, Sebastian Jester8,9, Jim Gray10, James E. Gunn5, Mark U. SubbaRao11, Anirudda R. Thakar3, Chris Stoughton12, Alexander S. Szalay3, Brian Yanny12, Donald G. York13,14, Neta A. Bahcall5, J. Barentine15, Michael R. Blanton16, Howard Brewington15, J. Brinkmann15, Robert J. Brunner17, Francisco J. Castander18, István Csabai19, Joshua A. Frieman12,13,20, Masataka Fukugita21, Michael Harvanek15, David W. Hogg16, Željko Ivezić6, Stephen M. Kent12,13, S. J. Kleinman15, G. R. Knapp5, Richard G. Kron12,13, Jurek Krzesiński22, Daniel C. Long15, Robert H. Lupton5, Atsuko Nitta23, Jeffrey R. Pier24, David H. Saxe25, Yue Shen5, Stephanie A. Snedden15, David H. Weinberg26 and Jian Wu1

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We present the fourth edition of the Sloan Digital Sky Survey (SDSS) Quasar Catalog. The catalog contains 77,429 objects; this is an increase of over 30,000 entries since the previous edition. The catalog consists of the objects in the SDSS Fifth Data Release that have luminosities larger than Mi = -22.0 (in a cosmology with H0 = 70 km s-1 Mpc-1, ΩM = 0.3, and ΩΛ = 0.7), have at least one emission line with FWHM larger than 1000 km s-1 or have interesting/complex absorption features, are fainter than i ≈ 15.0, and have highly reliable redshifts. The area covered by the catalog is ≈5740 deg2. The quasar redshifts range from 0.08 to 5.41, with a median value of 1.48; the catalog includes 891 quasars at redshifts greater than 4, of which 36 are at redshifts greater than 5. Approximately half of the catalog quasars have i < 19; nearly all have i < 21. For each object the catalog presents positions accurate to better than 0.2'' rms per coordinate, five-band (ugriz) CCD-based photometry with typical accuracy of 0.03 mag, and information on the morphology and selection method. The catalog also contains basic radio, near-infrared, and X-ray emission properties of the quasars, when available, from other large-area surveys. The calibrated digital spectra cover the wavelength region 3800-9200 Å at a spectral resolution of simeq2000; the spectra can be retrieved from the public database using the information provided in the catalog. The average SDSS colors of quasars as a function of redshift, derived from the catalog entries, are presented in tabular form. Approximately 96% of the objects in the catalog were discovered by the SDSS.


Keywords

catalogs; quasars: general; surveys


Dates

Issue 1 (2007 July)

Received 2006 December 1, accepted for publication 2007 March 25

Published 2007 May 11



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