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  <title>Chandra Lockman Area North Survey (CLANS) X-Ray Source Catalog</title>
  <shortName>CLANS</shortName>
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    <publisher ivo-id="ivo://nasa.heasarc/ASD">NASA/GSFC HEASARC</publisher>
    <creator>
      <name>Trouille et al.</name>
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    <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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    <subject>Survey Source</subject>
    <description>
      This table contains the catalogs for the X-ray sources detected in the Chandra Lockman Area North Survey (CLANS). (The information on the optical and infrared counterparts to these sources is contained in the CLANSOID table.) The nine ACIS-I fields which constitute the CLANS cover a solid angle of ~0.6 deg&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; and reach fluxes of 7 x 10&amp;lt;sup&amp;gt;-16&amp;lt;/sup&amp;gt; ergs cm&amp;lt;sup&amp;gt;-2&amp;lt;/sup&amp;gt; s&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (0.5-2 keV) and 3.5 x 10&amp;lt;sup&amp;gt;-15&amp;lt;/sup&amp;gt; ergs cm&amp;lt;sup&amp;gt;-2&amp;lt;/sup&amp;gt; s&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (2-8 keV). The authors find a total of 761 X-ray point sources. The CLANS and CLASXS surveys bridge the gap between the ultra-deep pencil-beam surveys, such as the CDFs, and the shallower, very large-area surveys. As a result, they probe the X-ray sources that contribute the bulk of the 2-8 keV X-ray background and cover the flux range of the observed break in the log N-log S distribution. CLANS consists of nine separate 70 ks Chandra ACIS-I exposures centered at J2000.0 RA and Dec of (10 46,+59 01) (see Table 2 of the reference paper for the full observational details) which were combined to create an 0.6 deg&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; image containing 761 sources. The CLANS observations consist of a raster with an ~2 arcminute overlap between contiguous pointings. Following the prescription in Yang et al. (2004, AJ, 128, 1501) for the CLASXS field, the authors merged the nine individual pointing catalogs to create the final CLANS X-ray catalog. For sources with more than one detection in the nine fields, they used the detection from the observation in which the effective area of the source was the largest. This table was created by the HEASARC in December 2008 based on the electronic versions of Tables 4 and 5 from the paper which were obtained from the ApJ web site. This is a service provided by NASA HEASARC .
    </description>
    <source format="">
      2008ApJS..179....1T
    </source>
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        <description>
          Chandra Lockman Area North Survey (CLANS) X-Ray Source Catalog
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          <name>name</name>
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            Source Designation
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            1-Sigma Poisson Upper Error in Full-Band Flux (erg/s/cm^2)
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            1-Sigma Poisson Lower Error in Full-Band Flux (erg/s/cm^2)
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            Hardness Ratio
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            1-Sigma Upper Error in Hardness Ratio
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            1-Sigma Lower Error in Hardness Ratio
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            System unit vector column
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            System unit vector column
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            Limit Flag for Hard-Band Flux
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            1-Sigma Poisson Upper Error in Soft-Band counts
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            Net 0.5-2 keV (Soft-Band) Counts
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            1-Sigma Poisson Lower Error in Hard-Band Counts
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            1-Sigma Poisson Upper Error in Soft-Band Flux (erg/s/cm^2)
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            Source Distance From Pointing Center (arcmin)
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            The 0.5-2 keV (Soft-Band) Flux (erg/s/cm^2)
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            phot.flux;em.X-ray.soft
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            Limit Flag for Soft-Band Flux
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            Power Law Photon Index
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            1-Sigma Poisson Lower Error in Hard-Band Flux (erg/s/cm^2)
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            stat.error;phot.flux;em.X-ray.medium
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            1-Sigma Poisson Lower Error in Full-Band Counts
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            Limit Flag for Hardness Ratio
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        <column>
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            Galactic Longitude
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            1-Sigma Poisson Upper Error in Hard-Band Counts
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            Net 5-8 keV (Full-Band) Counts
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            Galactic Latitude
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