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<ri:Resource created="2026-10-02T00:00:00" status="active" updated="2026-10-02T00:00:00" 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>X-Ray Selected High-z AGN Catalog</title>
  <shortName>XSHZAGNCXO</shortName>
  <identifier>ivo://nasa.heasarc/xshzagncxo</identifier>
  <curation>
    <publisher ivo-id="ivo://nasa.heasarc/ASD">NASA/GSFC HEASARC</publisher>
    <creator>
      <name>Kalfountzou et al.</name>
    </creator>
    <contributor/>
    <date>2026-10-02</date>
    <contact>
      <name>NASA/GSFC HEASARC help desk</name>
      <email>heasarc-vo at athena.gsfc.nasa.gov</email>
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  <content>
    <subject>AGN</subject>
    <description>
      This table contains the results from an analysis of the largest high-redshift (z &amp;gt; 3) X-ray-selected active galactic nucleus (AGN) sample to date, combining the Chandra Cosmological Evolution Survey and Chandra Multi-wavelength Project surveys and doubling the previous samples. The sample comprises 209 X-ray-detected AGNs, over a wide range of rest-frame 2-10 keV luminosities log L&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt; = 43.3 - 46.0 erg/s. X-ray hardness ratios show that ~39 per cent of the sources are highly obscured, N&amp;lt;sub&amp;gt;H&amp;lt;/sub&amp;gt; &amp;gt; 10&amp;lt;sup&amp;gt;22&amp;lt;/sup&amp;gt; cm&amp;lt;sup&amp;gt;-2&amp;lt;/sup&amp;gt;, in agreement with the ~37 per cent of type-2 AGNs found in this sample based on their optical classification. For ~26 per cent of objects, there are mismatched optical and X-ray classifications. Utilizing the 1/V&amp;lt;sub&amp;gt;max&amp;lt;/sub&amp;gt; method, the authors confirm that the comoving space density of all luminosity ranges of AGNs decreases with redshift above z &amp;gt; 3 and up to z ~ 7. With a significant sample of AGNs (N = 27) at z &amp;gt; 4, it is found that both source number counts in the 0.5-2 keV band and comoving space density are consistent with the expectation of a luminosity-dependent density evolution (LDDE) model at all redshifts, while they exclude the luminosity and density evolution (LADE) model. The measured comoving space density of type-1 and type-2 AGNs shows a constant ratio between the two types at z &amp;gt; 3. These results for both AGN types at these redshifts are consistent with the expectations of LDDE model. The high-redshift AGN sample used in this work has been selected from the C-COSMOS X-ray catalog, combining the spectroscopic and photometric information available from the identification catalogue of X-ray C-COSMOS sources (Civano et al. 2011, ApJ, 741, 91; 2012, ApJS, 201, 30) and the ChaMP (Chandra Multi-wavelength Project) X-ray catalog using only the 323 ChaMP ObsIDs overlapping with Sloan Digital Sky Survey (SDSS; Richards et al. 2006, AJ, 131, 2766) DR5 imaging. This table was created by the HEASARC in March 2016 based on the &amp;lt;a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/MNRAS/445/1430"&amp;gt;CDS catalog J/MNRAS/445/1430&amp;lt;/a&amp;gt; file tablea1.dat. This is a service provided by NASA HEASARC .
    </description>
    <source format="">
      2014MNRAS.445.1430K
    </source>
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  <facility>GALAXY CATALOG</facility>
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    <waveband>X-ray</waveband>
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        <name>xshzagncxo</name>
        <description>
          X-Ray Selected High-z AGN Catalog
        </description>
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            Source Designation
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            Declination
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            Photometric Redshift
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          <name>sb_flux</name>
          <description>
            The 0.5-2keV Flux Converted to Gamma=1.8
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          <unit>erg/s/cm^2</unit>
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            phot.flux;em.X-ray.soft
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        <column>
          <name>log_lx</name>
          <description>
            The 2-10keV Luminosity
          </description>
          <unit>log(erg/s)</unit>
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            phys.luminosity;em.X-ray
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          <name>nh</name>
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            The Absorption Column Density
          </description>
          <unit>cm^-2</unit>
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            phys.columnDensity
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        <column>
          <name>bii</name>
          <description>
            Galactic Latitude
          </description>
          <unit>degree</unit>
          <ucd>
            pos.galactic.lat
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        <column>
          <name>hardness_ratio_max</name>
          <description>
            Hardness Ratio Upper Bound
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            phot.flux;arith.ratio;em.X-ray.medium;stat.max
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        <column>
          <name>lii</name>
          <description>
            Galactic Longitude
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          <unit>degree</unit>
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            pos.galactic.lon
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          <name>xray_type_code</name>
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            Number Code [1/2] Indicates X-Ray Type Based on N_H=10^22 cm^-2 Limit
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            meta.code
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            meta.code;phys.columnDensity
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          <name>optical_type_code</name>
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            Number Code [1/2] Indicates Optical Type
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            meta.code;src.class
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            Number Code [1/2] Indicates Survey: 1=ChaMP; 2=C-COSMOS
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            meta.code
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            Number Code [1/2] Indicates 1=Detection in Soft Band; 2=Estimated from HB or FB
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            Hardness Ratio Lower Bound
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            phot.flux;arith.ratio;em.X-ray.medium;stat.min
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            Hardness Ratio
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            phot.flux;arith.ratio;em.X-ray.medium
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            System unit vector column
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            System unit vector column
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