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<ri:Resource created="2026-10-09T00:00:00" status="active" updated="2026-10-09T00:00:00" 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>VLA Extended-Chandra Deep Field-South Classification Catalog</title>
  <shortName>VLAECDFSCLS</shortName>
  <identifier>ivo://nasa.heasarc/vlaecdfscls</identifier>
  <curation>
    <publisher ivo-id="ivo://nasa.heasarc/ASD">NASA/GSFC HEASARC</publisher>
    <creator>
      <name>Bonzini et al.</name>
    </creator>
    <contributor/>
    <date>2026-10-09</date>
    <contact>
      <name>NASA/GSFC HEASARC help desk</name>
      <email>heasarc-vo at athena.gsfc.nasa.gov</email>
    </contact>
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  <content>
    <subject>Survey Source</subject>
    <description>
      The sub-mJy radio population is a mixture of active systems, that is star-forming galaxies (SFGs) and active galactic nuclei (AGNs). In their paper, the authors study a sample of 883 radio sources detected at 1.4 GHz in a deep Very Large Array (VLA) survey of the Extended Chandra Deep Field-South (E-CDF-S) that reaches a best rms sensitivity of 6 microJansky (&amp;micro;Jy). The authors have used a simple scheme to disentangle SFGs, radio-quiet (RQ), and radio-loud (RL) AGNs based on the combination of radio data with Chandra X-ray data and mid-infrared observations from Spitzer. They find that at flux densities between about 30 and 100 uJy, the radio population is dominated by SFGs (~60%) and that RQ AGNs become increasingly important over RL ones below 100 uJy. In the paper, the authors also compare the host galaxy properties of the three classes in terms of morphology, optical colors and stellar masses. Their results show that both SFG and RQ AGN host galaxies have blue colors and late-type morphology while RL AGNs tend to be hosted by massive red galaxies with early-type morphology. This supports the hypothesis that radio emission in SFGs and RQ AGNs mainly comes from the same physical process: star formation in the host galaxy. This table was created by the HEASARC in January 2014 based on the machine-readable version of Table 1 from the reference paper which was obtained from the MNRAS web site. This is a service provided by NASA HEASARC .
    </description>
    <source format="">
      2013MNRAS.436.3759B
    </source>
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    <type>Catalog</type>
    <contentLevel>Research</contentLevel>
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  <facility>RADIO CATALOG</facility>
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    <waveband>Infrared</waveband>
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        <name>vlaecdfscls</name>
        <description>
          VLA Extended-Chandra Deep Field-South Classification Catalog
        </description>
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          <name>name</name>
          <description>
            Source Designation
          </description>
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            meta.id;meta.main
          </ucd>
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            pos.eq.ra;meta.main
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            Logarithm of the X-Ray Luminosity in the Hard Band (2-10 keV)
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            phys.luminosity;em.X-ray
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            Logarithm of the Radio Power
          </description>
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          </ucd>
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            Quality Flag of the Classification: from 3=Secure to 1=Insecure
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            System unit vector column
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          <name>"__y_ra_dec"</name>
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            System unit vector column
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            System unit vector column
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          <description>
            System index column
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          <name>class</name>
          <description>
            Browse Object Classification
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            src.class
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          <name>source_number</name>
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            Sequential Identification Number for Each Source in Catalog
          </description>
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          <name>log_ratio_8p0_4p5_um</name>
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            IRAC Color: Logarithm of the Ratio of 8.0- and 4.5-um Flux Densities
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          <name>abs_bmag</name>
          <description>
            Rest-Frame Absolute B Magnitude
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            Logarithm of the Ratio of the Observed 24-micron and 1.4-Ghz Luminosities
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          <description>
            Galactic Longitude
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          <unit>degree</unit>
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            pos.galactic.lon
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            Limit Flag for Logarithm of the Ratio of the 24-micron and 1.4-Ghz Luminosities
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          <description>
            Galactic Latitude
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            pos.galactic.lat
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