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<ri:Resource created="2026-05-29T00:00:00" status="active" updated="2026-05-29T00:00:00" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:stc="http://www.ivoa.net/xml/STC/stc-v1.30.xsd" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/STC/stc-v1.30.xsd http://vo.ari.uni-heidelberg.de/docs/schemata/stc-v1.30.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd http://www.w3.org/1999/xlink http://vo.ari.uni-heidelberg.de/docs/schemata/xlink.xsd" xsi:type="vs:CatalogService">
  <title>Sloan Digital Sky Survey (DR5)/XMM-Newton Quasar Survey Catalog</title>
  <shortName>SDSSXMMQSO</shortName>
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  <curation>
    <publisher ivo-id="ivo://nasa.heasarc/ASD">NASA/GSFC HEASARC</publisher>
    <creator>
      <name>Young et al.</name>
    </creator>
    <contributor/>
    <date>2026-05-29</date>
    <contact>
      <name>NASA/GSFC HEASARC help desk</name>
      <email>heasarc-vo at athena.gsfc.nasa.gov</email>
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    <subject>AGN</subject>
    <description>
      This table contains the 5th Data Release Sloan Digital Sky Survey (DR5 SDSS)/XMM-Newton Quasar Survey Catalog. This catalog contains 792 SDSS DR5 quasars with optical spectra that have been observed serendipitously in the X-rays with XMM-Newton. These quasars cover a redshift range of z = 0.11 - 5.41 and a magnitude range of i = 15.3 - 20.7. Substantial numbers of radio-loud (70) and broad absorption line (51) quasars exist within this sample. Significant X-ray detections at &amp;gt;=2 sigma account for 87% of the sample (685 quasars), and 473 quasars are detected at &amp;gt;=6 sigma, sufficient to allow X-ray spectral fits. For detected sources, ~60% have X-ray fluxes between F(2-10 keV) = (1-10) x 10&amp;lt;sup&amp;gt;-14&amp;lt;/sup&amp;gt; erg cm&amp;lt;sup&amp;gt;-2&amp;lt;/sup&amp;gt; s&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. The authors fit a single power law, a fixed power law with intrinsic absorption left free to vary, and an absorbed power-law model to all quasars with X-ray signal-to-noise ratio &amp;gt;= 6, resulting in a weighted mean photon index Gamma = 1.91 +/- 0.08, with an intrinsic dispersion sigma(Gamma) = 0.38. For the 55 sources (11.6%) that prefer intrinsic absorption, the authors find a weighted mean N&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; = 1.5 +/- 0.3 x 10&amp;lt;sup&amp;gt;21&amp;lt;/sup&amp;gt; cm&amp;lt;sup&amp;gt;-2&amp;lt;/sup&amp;gt;. They find that Gamma correlates significantly with optical color, Delta(g-i), the optical-to-X-ray spectral index (alpha&amp;lt;sub&amp;gt;ox&amp;lt;/sub&amp;gt;), and the X-ray luminosity. While the first two correlations can be explained as artifacts of undetected intrinsic absorption, the correlation between Gamma and X-ray luminosity appears to be a real physical correlation, indicating a pivot in the X-ray slope. This table was created by the HEASARC in July 2009 based on electronic versions of Tables 1 and 2 from the paper which were obtained from the Astrophysical Journal web site. This is a service provided by NASA HEASARC .
    </description>
    <source format="">
      2009ApJS..183...17Y
    </source>
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        <name>sdssxmmqso</name>
        <description>
          Sloan Digital Sky Survey (DR5)/XMM-Newton Quasar Survey Catalog
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            Source Designation
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            Rest-Frame Luminosity in 2-10 keV Band
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        <column>
          <name>spectral_index</name>
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            X-Ray Photon Index for Best-Fit Model
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          <ucd>
            spect.index
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          <dataType xsi:type="vs:VOTableType">double</dataType>
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        <column>
          <name>chi_squared</name>
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            Chi-Squared Value for Best-Fit Model
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            stat.fit.chi2
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        <column>
          <name>nh_min</name>
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            The 90% Lower Error on Intrinsic X-Ray Absorption
          </description>
          <unit>H-atoms/cm^2</unit>
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            phys.columnDensity;stat.min
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            The 90% Lower Error on X-Ray Photon Index
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            Radio-Loud Flag
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        <column>
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            Observed-Frame Flux in 0.5-2 keV Band
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            phot.flux;em.X-ray.soft
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            Background Counts; Scaled to Source Extraction Region
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          <unit>ct</unit>
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            Live Exposure Time of X-Ray Observation (s)
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        <column>
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            Galactic Hydrogen Column Density in the Direction of the Source
          </description>
          <unit>H-atoms/cm^2</unit>
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            phys.columnDensity
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          <flag>
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          <description>
            The 90% Upper Error on Intrinsic X-Ray Absorption
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          <unit>H-atoms/cm^2</unit>
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            phys.columnDensity;stat.max
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          <description>
            The 90% Upper Error on X-Ray Photon Index
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            stat.error;spect.index
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            Degrees of Freedom for Best-Fit Model
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            Off-Axis Angle (arcmin)
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            Observed-Frame Flux in 2-10 keV Band
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            Flag Indicating Quality of the X-Ray Fit: -1=non-detection
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            Galactic Latitude
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