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The Sloan Digital Sky Survey Quasar Catalog. V. Seventh Data Release

  • Authors: Donald P. Schneider, Gordon T. Richards, Patrick B. Hall, Michael A. Strauss, Scott F. Anderson, Todd A. Boroson, Nicholas P. Ross, Yue Shen, W. N. Brandt, Xiaohui Fan, Naohisa Inada, Sebastian Jester, G. R. Knapp, Coleman M. Krawczyk, Anirudda R. Thakar, Daniel E. Vanden Berk, Wolfgang Voges, Brian Yanny, Donald G. York, Neta A. Bahcall, Dmitry Bizyaev, Michael R. Blanton, Howard Brewington, J. Brinkmann, Daniel Eisenstein, Joshua A. Frieman, Masataka Fukugita, Jim Gray, James E. Gunn, Pascale Hibon, Željko Ivezić, Stephen M. Kent, Richard G. Kron, Myung Gyoon Lee, Robert H. Lupton, Elena Malanushenko, Viktor Malanushenko, Dan Oravetz, K. Pan, Jeffrey R. Pier, Ted N. Price III, David H. Saxe, David J. Schlegel, Audry Simmons, Stephanie A. Snedden, Mark U. SubbaRao, Alexander S. Szalay, and David H. Weinberg

SCHNEIDER et al. 2010 The Astronomical Journal 139 2360.

  • Provider: AAS Journals

Caption: Figure 4.

Observed i magnitude as a function of redshift for the 105,783 objects in the catalog. Open circles indicate quasars that were recovered, but not discovered, by the SDSS. The distribution is represented by a set of linear contours when the density of points in this two-dimensional space would cause the points to overlap. The steep gradients at i ≈ 19.1 and i ≈ 20.2 are due to the flux limit for the targeted low- and high-redshift parts of the survey; the dip in the counts at z ≈ 2.7 arises because of the high incompleteness of the SDSS Quasar Survey at redshifts between 2.5 and 3.0 (also see Figure 5).

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