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  <title>SDSS NBCKDE Catalog of Photometrically Selected Quasar Candidates</title>
  <shortName>SDSSNBCKDE</shortName>
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    <publisher ivo-id="ivo://nasa.heasarc/ASD">NASA/GSFC HEASARC</publisher>
    <creator>
      <name>Richards et al.</name>
    </creator>
    <contributor/>
    <date>2026-10-09</date>
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      <email>heasarc-vo at athena.gsfc.nasa.gov</email>
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    <subject>Survey Source</subject>
    <description>
      This table contains a catalog of 1,015,082 quasar candidates selected from the photometric imaging data of the Sloan Digital Sky Survey (SDSS) using a non-parametric Bayesian classification kernel density estimator (NBC-KDE). It excludes 157,075 initial candidates that were culled as known or likely contaminants. The objects are all point sources to a limiting magnitude of i = 21.3 from 8417 deg&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; of imaging from SDSS Data Release 6 (DR6). This sample extends the previous catalog (Paper I: Richards et al. 2004, ApJS, 155, 257) by using the latest SDSS public release data and probing both ultraviolet (UV)-excess and high-redshift quasars. While the addition of high-redshift candidates reduces the overall efficiency (quasars:quasar candidates) of the catalog to ~80%, it is expected to contain no fewer than 850,000 bona fide quasars, which is ~8 times the number of the previous sample and ~10 times the size of the largest spectroscopic quasar catalog. Cross-matching between this photometric catalog and spectroscopic quasar catalogs from both the SDSS and 2dF survey yields 88,879 spectroscopically confirmed quasars. For judicious selection of the most robust UV-excess sources (~500,000 objects in all), the efficiency is nearly 97 - more than sufficient for detailed statistical analyses. The catalog&amp;#39;s completeness to type 1 (broad-line) quasars is expected to be no worse than 70%, with most missing objects occurring at z &amp;lt; 0.7 and 2.5 &amp;lt; z &amp;lt; 3.0. In addition to classification information, the authors provide photometric redshift estimates (typically good to Delta(z) +/- 0.3 [2-sigma]) and cross-matching with radio, X-ray, and proper-motion catalogs. Finally, the authors have considered the catalog&amp;#39;s utility for determining the optical luminosity function of quasars and are able to confirm the flattening of the bright-end slope of the quasar luminosity function at z ~ 4 as compared to z ~ 2. Much more information on the SDSS is available at the project&amp;#39;s web site at &amp;lt;a href="http://www.sdss.org/"&amp;gt;http://www.sdss.org/&amp;lt;/a&amp;gt;. This table was created by the HEASARC based on an electronic version of Table 1 in the reference paper which was obtained from the ApJ web site. This is a service provided by NASA HEASARC .
    </description>
    <source format="">
      2009ApJS..180...67R
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        <description>
          SDSS NBCKDE Catalog of Photometrically Selected Quasar Candidate
        </description>
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            SDSS Source Designation (SDSS Jhhmmss.ss+-ddmmss.s)
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        <column>
          <name>reddening</name>
          <description>
            The (B-V) Extinction
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          <unit>mag</unit>
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            phot.color.excess
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          <name>redshift_probability</name>
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            Photometric Redshift Range Probability
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            stat.probability;src.redshift
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          <name>uvxts_flag</name>
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            UV-Excess Flag, 88% Star Prior; See Paper I
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          <name>proper_motion</name>
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            Proper Motion (mas/yr)
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          <unit>mas/yr</unit>
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            Previous Catalog Object Classification
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            Logarithm of KDE Star Density
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            Low z Range Flag (z &lt;= 2.2), 98% Star Prior
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            z-band PSF-ubercalibrated asinh Magnitude
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          <ucd>
            phot.mag;em.opt.I
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            Galactic Longitude
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            Error in gmag
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            Error in zmag
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            Lower Limit of Photometric Redshift
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            Galactic Latitude
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