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The FIRST Bright Quasar Survey. II. 60 Nights and 1200 Spectra Later

  • Authors: Richard L. White, Robert H. Becker, Michael D. Gregg, Sally A. Laurent-Muehleisen, Michael S. Brotherton, Chris D. Impey, Catherine E. Petry, Craig B. Foltz, Frederic H. Chaffee, Gordon T. Richards, William R. Oegerle, David J. Helfand, Richard G. McMahon, and Juan E. Cabanela

White et al. 2000 The Astrophysical Journal Supplement Series 126 133.

  • Provider: AAS Journals

Caption: Fig. 11.

Completeness, C, and reliability, R, of the sample as a function of the threshold selected for the probability ﹩P( Q) ﹩. The completeness is the fraction of quasars from the complete FBQS sample that are included at the selected ﹩P( Q) ﹩ threshold; the reliability is the fraction of selected candidates that are quasars. The solid line is computed using all parameters; the dashed line excludes color. The FBQS sample presented in this paper is the point at ﹩C=1﹩, ﹩R=0.55﹩ (i.e., the sample is complete but only 55% of the candidates turn out to be quasars.) The efficiency of the quasar search (determined by the reliability of the prediction) can be increased to ~89% using color (85% without color), if completeness is not important. Even with completeness greater than 90%, the reliability can be higher than 80%.

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