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  <title>M 83 XMM-Newton X-Ray Point Source Catalog</title>
  <shortName>M83XMM</shortName>
  <identifier>ivo://nasa.heasarc/m83xmm</identifier>
  <curation>
    <publisher ivo-id="ivo://nasa.heasarc/ASD">NASA/GSFC HEASARC</publisher>
    <creator>
      <name>Ducci 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>
      This database table contains results obtained from the analysis of three XMM-Newton observations of the grand-design barred spiral galaxy M 83. The aims of this study were to study the X-ray source populations in M 83 and to calculate the X-ray luminosity functions of X-ray binaries for different regions of the galaxy. The authors detected 189 sources in the XMM-Newton field of view in the energy range of 0.2-12 keV. They constrained their nature by means of spectral analysis, hardness ratios, studies of the X-ray variability, and cross-correlations with catalogs in X-ray, optical, infrared, and radio wavelengths. The authors identified and classified 12 background objects, five foreground stars, two X-ray binaries, one supernova remnant candidate, one super-soft source candidate and one ultra-luminous X-ray source. Among these sources, they classified for the first time three active galactic nuclei (AGN) candidates. the authors derived X-ray luminosity functions for the X-ray sources in M 83 in the 2-10 keV energy range, within and outside the D&amp;lt;sub&amp;gt;25&amp;lt;/sub&amp;gt; ellipse, correcting the total X-ray luminosity function for incompleteness and subtracting the AGN contribution. The X-ray luminosity function inside the D25 ellipse is consistent with that previously observed by Chandra. The Kolmogorov-Smirnov test shows that the X-ray luminosity function of the outer disc and the AGN luminosity distribution are uncorrelated with a probability of ~99.3%. The authors also found that the X-ray sources detected outside the D&amp;lt;sub&amp;gt;25&amp;lt;/sub&amp;gt; ellipse and the uniform spatial distribution of AGNs are spatially uncorrelated with a significance of 99.5%. They interpret these results as an indication that part of the observed X-ray sources are X-ray binaries in the outer disc of M 83. The authors analyzed the public archival XMM-Newton data of M 83 (PIs: Watson, Kuntz). Three observations were analyzed, one pointing at the center of the galaxy (obs.1) and two in the south, which covered the outer arms with a young population of stars discovered with GALEX. The details of these observations are given in Table 1 of the reference paper (summarized below): &amp;lt;pre&amp;gt; EPIC EPIC EPIC No ObsID Date RA DE PN MOS1 MOS2 Mode F Texp F Texp F Texp PN MOS 1 0110910201 2003-01-27 13:37:05.16 -29:51:46.1 t 21.2 m 24.6 m 24.6 EFF FF 2 0503230101 2008-01-16 13:37:01.09 -30:03:49.9 m 15.4 m 19.0 m 19.0 EFF FF 3 0552080101 2008-08-16 13:36:50.87 -30:03:55.2 m 25.0 m 28.8 m 28.8 EFF FF &amp;lt;/pre&amp;gt; where F is the filter (t for thin, m for medium), T&amp;lt;sub&amp;gt;exp&amp;lt;/sub&amp;gt; is the exposure time in ks, EFF = extended full frame imaging mode, and FF = full frame imaging mode. This table was created by the HEASARC in April 2013 based on &amp;lt;a href="https://cdsarc.cds.unistra.fr/ftp/cats/J/A+A/553/A7"&amp;gt;CDS Catalog J/A+A/553/A7&amp;lt;/a&amp;gt; files tableb1.dat and tableb2.dat. This is a service provided by NASA HEASARC .
    </description>
    <source format="">
      2013A&amp;amp;A...553A...7D
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    <type>Catalog</type>
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        <name>m83xmm</name>
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          M 83 XMM-Newton X-Ray Point Source Catalog
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            Sequential Identification Number for Each Source in Catalog
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            Source Designation
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          <name>ra</name>
          <description>
            Right Ascension
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          <unit>degree</unit>
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            pos.eq.ra;meta.main
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          <name>dec</name>
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            Declination
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          <name>error_radius</name>
          <description>
            Positional Error
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          <unit>arcsec</unit>
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          <name>count_rate_1</name>
          <description>
            Observation 1 Count Rate (in 0.2-12keV)
          </description>
          <unit>ct/s</unit>
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            phot.count;em.X-ray
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            RMS Uncertainty in Observation 1 Count Rate
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          <unit>ct/s</unit>
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            stat.error;phot.count;em.X-ray
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          <name>count_rate_2</name>
          <description>
            Observation 2 Count Rate (in 0.2-12keV)
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          <unit>ct/s</unit>
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            phot.count;em.X-ray
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          <description>
            RMS Uncertainty in Observation 2 Count Rate
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          <unit>ct/s</unit>
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            stat.error;phot.count;em.X-ray
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            Observation 3 Count Rate (in 0.2-12keV)
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          <unit>ct/s</unit>
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            phot.count;em.X-ray
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          <description>
            RMS Uncertainty in Observation 3 Count Rate
          </description>
          <unit>ct/s</unit>
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            stat.error;phot.count;em.X-ray
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        <column>
          <name>broad_type</name>
          <description>
            Classification
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          <ucd>
            src.class
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          <dataType xsi:type="vs:VOTableType">char</dataType>
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        <column>
          <name>detect_likelihood_1</name>
          <description>
            Likelihood from Observation 1
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            stat.likelihood;em.X-ray
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            RMS Uncertainty in Hardness Ratio 3
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            stat.error;phot.flux;arith.ratio;em.X-ray
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          <name>optical_name</name>
          <description>
            Optical Identification
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          <ucd>
            meta.id.cross
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            RMS Uncertainty in Hardness Ratio 4
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            stat.error;phot.flux;arith.ratio;em.X-ray
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            Hardness Ratio 1, (R2-R1)/(R2+R1)
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            phot.flux;arith.ratio;em.X-ray
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          <name>radio_matches</name>
          <description>
            Radio Identification(s) with Grade(s)
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          <ucd>
            meta.id.cross
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          <name>twomass_name</name>
          <description>
            2MASS (II/246) Identification
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            meta.id.cross
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          <description>
            Flag Indicates the Grade for the USNO-B1 Match
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          <name>lii</name>
          <description>
            Galactic Longitude
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          <unit>degree</unit>
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            pos.galactic.lon
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            RMS Uncertainty in Hardness Ratio 2
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