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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>AT Large Area Survey (ATLAS) E-CDF-S 5.5-GHz Components Catalog</title>
  <shortName>ATLAS5P5GH</shortName>
  <identifier>ivo://nasa.heasarc/atlas5p5gh</identifier>
  <curation>
    <publisher ivo-id="ivo://nasa.heasarc/ASD">NASA/GSFC HEASARC</publisher>
    <creator>
      <name>Huynh 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>
      Star-forming galaxies are thought to dominate the sub-mJy radio population, but recent work has shown that low-luminosity active galactic nuclei (AGNs) can still make a significant contribution to the faint radio source population. Spectral indices are an important tool for understanding the emission mechanism of the faint radio sources. The authors have observed the extended Chandra Deep Field South at 5.5 GHz using a mosaic of 42 pointings with the Australia Telescope Compact Array (ATCA). Their image reaches an almost uniform sensitivity of ~ 12 &amp;micro;Jy (&amp;micro;Jy) rms over 0.25 deg&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; with a restoring beam of 4.9 arcsec x 2.0 arcsec, making the ATLAS 5.5-GHz survey one of the deepest 6-cm surveys to date. This table contains the 5.5 GHz catalog of 142 source components corresponding to the 123 sources in this field: the source counts from this field are discussed in the reference paper. This table was created by the HEASARC in February 2013 based on the electronic 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="">
      2012MNRAS.426.2342H
    </source>
    <referenceURL>https://heasarc.gsfc.nasa.gov/W3Browse/all/atlas5p5gh.html</referenceURL>
    <type>Catalog</type>
    <contentLevel>Research</contentLevel>
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        HEASARC TAP
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    </interface>
    <maxSR>180</maxSR>
    <maxRecords>99999</maxRecords>
    <verbosity>true</verbosity>
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  </capability>
  <facility>RADIO CATALOG</facility>
  <coverage>
    <stc:STCResourceProfile>
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        <name>atlas5p5gh</name>
        <description>
          AT Large Area Survey (ATLAS) E-CDF-S 5.5-GHz Components Catalog
        </description>
        <column>
          <name>name</name>
          <description>
            IAU-Style Source Designation
          </description>
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            meta.id;meta.main
          </ucd>
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            Right Ascension
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            pos.eq.ra;meta.main
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          <name>dec</name>
          <description>
            Declination
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            Peak Source Flux Density
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            Uncertainty in Peak Source Flux Density
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            Integrated Flux Density
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          <name>rms_5p5_ghz</name>
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            Local Noise Level
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            stat.error;phot.flux.density;em.radio.3-6GHz
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        <column>
          <name>bii</name>
          <description>
            Galactic Latitude
          </description>
          <unit>degree</unit>
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            pos.galactic.lat
          </ucd>
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            nullable
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          <name>resolved_flag</name>
          <description>
            Boolean Flag Indicates Source Successfully Deconvolved
          </description>
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            meta.code;src
          </ucd>
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            nullable
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        <column>
          <name>source_id</name>
          <description>
            Unique Source Identifier
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            meta.id;src
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            nullable
          </flag>
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        <column>
          <name>lii</name>
          <description>
            Galactic Longitude
          </description>
          <unit>degree</unit>
          <ucd>
            pos.galactic.lon
          </ucd>
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          <flag>
            nullable
          </flag>
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        <column>
          <name>position_angle</name>
          <description>
            Deconvolved Position Angle, Measured from North to East
          </description>
          <unit>degree</unit>
          <ucd>
            pos.posAng
          </ucd>
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          <flag>
            nullable
          </flag>
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        <column>
          <name>major_axis</name>
          <description>
            Deconvolved Major Axis
          </description>
          <unit>arcsec</unit>
          <ucd>
            phys.angSize.smajAxis
          </ucd>
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            nullable
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        <column>
          <name>minor_axis</name>
          <description>
            Deconvolved Minor Axis
          </description>
          <unit>arcsec</unit>
          <ucd>
            phys.angSize.sminAxis
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          <name>"__x_ra_dec"</name>
          <description>
            System unit vector column
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            System unit vector column
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            System index column
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