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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>Omega Centauri Globular Cluster Chandra Deep Survey X-Ray Point Source Catalog</title>
  <shortName>OMEGCENCX2</shortName>
  <identifier>ivo://nasa.heasarc/omegcencx2</identifier>
  <curation>
    <publisher ivo-id="ivo://nasa.heasarc/ASD">NASA/GSFC HEASARC</publisher>
    <creator>
      <name>Henleywillis 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>
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  <content>
    <subject>Survey Source</subject>
    <description>
      The authors identify 233 X-ray sources, of which 95 are new, in a 222-ks exposure of omega Centauri with the Chandra X-ray Observatory&amp;#39;s Advanced CCD Imaging Spectrometer detector. The limiting unabsorbed flux in the core is f&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;(0.5-6.0keV) ~= 3 x 10&amp;lt;sup&amp;gt;-16&amp;lt;/sup&amp;gt; erg/s/cm&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; (L&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt; ~= 1 x 10&amp;lt;sup&amp;gt;30&amp;lt;/sup&amp;gt; erg/s at 5.2kpc). The authors estimate that ~60 +/- 20 of these are cluster members, of which ~30 lie within the core (r&amp;lt;sub&amp;gt;c&amp;lt;/sub&amp;gt; = 155 arcsec), and another ~30 between 1-2 core radii. They identify four new optical counterparts, for a total of 45 likely identifications. Probable cluster members include 18 cataclysmic variables (CVs) and CV candidates, one quiescent low-mass X-ray binary, four variable stars, and five stars that are either associated with omega Cen&amp;#39;s anomalous red giant branch or are sub-subgiants. The authors estimate that the cluster contains 40 +/- 10 CVs with L_x_&amp;gt; 10&amp;lt;sup&amp;gt;31&amp;lt;/sup&amp;gt; erg/s, confirming that CVs are underabundant in omega Cen relative to the field. Intrinsic absorption is required to fit X-ray spectra of six of the nine brightest CVs, suggesting magnetic CVs, or high-inclination systems. Though no radio millisecond pulsars (MSPs) are currently known in omega Cen, more than 30 unidentified sources have luminosities and X-ray colors like those of MSPs found in other globular clusters; these could be responsible for the Fermi-detected gamma-ray emission from the cluster. The authors identify a CH star as the counterpart to the second brightest X-ray source in the cluster and argue that it is a symbiotic star. This is the first such giant/white dwarf binary to be identified in a globular cluster. The data were obtained over two long exposures of omega Cen using the imaging array of the Chandra X-ray Observatory&amp;#39;s ACIS-I on 2012 April 16 and 17. The data sets have a combined exposure time of ~222ks (173.7 and 48.5ks for ObsIDs 13726 and 13727, respectively). This table was created by the HEASARC in June 2018 based upon the &amp;lt;a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/MNRAS/479/2834"&amp;gt;CDS Catalog J/MNRAS/479/2834&amp;lt;/a&amp;gt; file table1.dat. This is a service provided by NASA HEASARC .
    </description>
    <source format="">
      2018MNRAS.479.2834H
    </source>
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    <type>Catalog</type>
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        <description>
          Omega Centauri Globular Cluster Chandra Deep Survey X-Ray Point
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            Catalog Source Designation
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          <unit>erg/s/cm^2</unit>
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            Soft (0.5-2.0keV) Band X-Ray Flux
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          <unit>erg/s/cm^2</unit>
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            Optical Identification
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          <ucd>
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        <column>
          <name>bii</name>
          <description>
            Galactic Latitude
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          <unit>degree</unit>
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            95% Confidence Error Radius
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          <unit>arcsec</unit>
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          <description>
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          <name>hardness_ratio</name>
          <description>
            Logarithm of the Soft-to-Hard X-Ray Count Ratio
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          <name>hb_total_counts</name>
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            Detected Hard (1.5-6.0keV) Band X-Ray Counts
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            Detected Soft (0.5-1.5keV) Band X-Ray Counts
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            Detected Medium (0.5-4.5keV) Band X-Ray Counts
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            Corrected Medium (0.5-4.5keV) Band X-Ray Counts
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            Corrected Soft (0.5-1.5keV) Band X-Ray Counts
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          <unit>ct</unit>
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            phot;em.X-ray
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        <column>
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          <description>
            Galactic Longitude
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          <unit>degree</unit>
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