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  <title>M 37 Chandra X-Ray Point Source Catalog</title>
  <shortName>M37CXO</shortName>
  <identifier>ivo://nasa.heasarc/m37cxo</identifier>
  <curation>
    <publisher ivo-id="ivo://nasa.heasarc/ASD">NASA/GSFC HEASARC</publisher>
    <creator>
      <name>Nunez 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>
      Empirical calibrations of the stellar age-rotation-activity relation (ARAR) rely on observations of the co-eval populations of stars in open clusters. The authors used the Chandra X-ray Observatory to study M 37 (NGC 2099), a 500-Myr-old open cluster that has been extensively surveyed for rotation periods (P&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt;). M 37 was observed almost continuously for five days, for a total of 440.5 ks, to measure stellar X-ray luminosities (L&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;), a proxy for coronal activity, across a wide range of masses. The cluster&amp;#39;s membership catalog was revisited to calculate updated membership probabilities from photometric data and each star&amp;#39;s distance to the cluster center. The result is a comprehensive sample of 1699 M 37 members: 426 with P&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt;, 278 with X-ray detections, and 76 with both. The authors calculate Rossby numbers, R&amp;lt;sub&amp;gt;o&amp;lt;/sub&amp;gt;= P&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt;/tau , where tau is the convective turnover time, and ratios of the X-ray-to-bolometric luminosity, L&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;/L&amp;lt;sub&amp;gt;bol&amp;lt;/sub&amp;gt;, to minimize mass dependencies in their characterization of the rotation-coronal activity relation at 500 Myr. They find that fast rotators, for which R&amp;lt;sub&amp;gt;o&amp;lt;/sub&amp;gt; &amp;lt; 0.09 +/- 0.01, show saturated levels of activity, with log(L&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt;/L&amp;lt;sub&amp;gt;bol&amp;lt;/sub&amp;gt;) = -3.06 +/- 0.04. For R&amp;lt;sub&amp;gt;o&amp;lt;/sub&amp;gt; &amp;gt;= 0.09 +/- 0.01, activity is unsaturated and follows a power law of the form R&amp;lt;sup&amp;gt;beta&amp;lt;/sup&amp;gt;&amp;lt;sub&amp;gt;o&amp;lt;/sub&amp;gt; , where beta = -2.03 (-0.14, +0.17). This is the largest sample available for analyzing the dependence of coronal emission on rotation for a single-aged population, covering stellar masses in the range 0.4 - 1.3 solar masses, P&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; in the range 0.4 - 12.8 days, and L&amp;lt;sub&amp;gt;X&amp;lt;/sub&amp;gt; in the range 10&amp;lt;sup&amp;gt;28.4&amp;lt;/sup&amp;gt; - 10&amp;lt;sup&amp;gt;30.5&amp;lt;/sup&amp;gt; erg s&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. These results make M 37 a new benchmark open cluster for calibrating the ARAR at ages of ~ 500 Myr. The central field of M 37 was observed five separate times between 2011 November 14 20:58 and 2011 November 1915:31 UTC for a total of 440.5 ks with the Advanced CCD Imaging Spectrometer (ACIS). The four ACIS-I chips and the ACIS-S3 chip were used in Very Faint telemetry mode to improve the screening of background events and thus increase the sensitivity of ACIS to faint sources. The exposure-weighted average aimpoint of the 16.9 x 16.9 arcmin&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; ACIS-I field of view is RA = 05&amp;lt;sup&amp;gt;h&amp;lt;/sup&amp;gt; 52&amp;lt;sup&amp;gt;m&amp;lt;/sup&amp;gt; 17.86&amp;lt;sup&amp;gt;s&amp;lt;/sup&amp;gt;,Dec = +32&amp;lt;sup&amp;gt;o&amp;lt;/sup&amp;gt; 33&amp;#39; 48.23&amp;quot; (J2000). The pitch angle for four observations was 103 degrees; due to scheduling constraints, it was 253 degrees for the fifth. Table 1 in the reference paper provides the basic information for the 5 Chandra observations and Figure 1 in that paper shows their footprints superimposed on a 40&amp;#39; x 40&amp;#39; i&amp;#39; image centered on M 37 obtained by Hartman et al. (2008, ApJ, 675, 1233, hereafter HA08) with the Megacam on the MMT telescope. This HEASARC table contains all of the data from Table 3 of the reference paper, the M 37 Chandra catalog of 774 X-ray sources, and the data from Table 5, the catalog of optical objects, for those objects which have been identified as optical counterparts to the X-ray sources. It does not contain entries for those optical objects in Table 5 which lack X-ray counterparts. This online catalog was created by the HEASARC in December 2015 based on machine-readable versions of tables 3 and 5 from the paper which were obtained from the ApJ website. This is a service provided by NASA HEASARC .
    </description>
    <source format="">
      2015ApJ...809..161N
    </source>
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    <type>Catalog</type>
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        <name>m37cxo</name>
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          M 37 Chandra X-Ray Point Source Catalog
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          <description>
            Sequential Identification Number for Each Source in the Catalog
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          <description>
            80%-Confidence Level X-Ray Positional Uncertainty
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          <unit>arcsec</unit>
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            Net Source Counts in the 0.5-7 keV Band
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          <unit>ct</unit>
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          <description>
            1-Sigma Negative Error of Net Source Counts in the 0.5-7 keV Band
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          <unit>ct</unit>
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            stat.error;phot;em.X-ray
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            1-Sigma Positive Error of Net Source Counts in the 0.5-7 keV Band
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            Absorbed Energy Flux in the 0.5-7 keV Band
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          <unit>erg/s/cm^2</unit>
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            phot.flux;em.X-ray
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          <name>sb_lx</name>
          <description>
            X-Ray Luminosity in the 0.1-2.4 keV Band
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          <unit>erg/s</unit>
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          <name>optical_cxo_offset</name>
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            Offset Between X-Ray Source and Optical Match
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          <unit>arcsec</unit>
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            g Magnitude
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            g Magnitude Standard Deviation
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          <unit>mag</unit>
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          </ucd>
          <dataType xsi:type="vs:VOTableType">double</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>me08_optical_offset</name>
          <description>
            Offset Between Optical Object and ME08 Match
          </description>
          <unit>arcsec</unit>
          <ucd>
            pos.angDistance;em.opt
          </ucd>
          <dataType xsi:type="vs:VOTableType">double</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>lii</name>
          <description>
            Galactic Longitude
          </description>
          <unit>degree</unit>
          <ucd>
            pos.galactic.lon
          </ucd>
          <dataType xsi:type="vs:VOTableType">double</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>source_anomaly_flags</name>
          <description>
            Flags Indicates Source Anomalies
          </description>
          <ucd>
            meta.code;src
          </ucd>
          <dataType xsi:type="vs:VOTableType">char</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>sb_counts_pos_err</name>
          <description>
            1-Sigma Positive Error of Net Source Counts in the 0.5-2 keV Band
          </description>
          <unit>ct</unit>
          <ucd>
            stat.error;phot;em.X-ray.soft
          </ucd>
          <dataType xsi:type="vs:VOTableType">double</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>lbol</name>
          <description>
            Bolometric Luminosity
          </description>
          <unit>erg/s</unit>
          <ucd>
            phys.luminosity
          </ucd>
          <dataType xsi:type="vs:VOTableType">double</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>psf_fraction</name>
          <description>
            Fraction of the PSF Enclosed within Extraction Region
          </description>
          <ucd>
            instr.det.psf
          </ucd>
          <dataType xsi:type="vs:VOTableType">double</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>me08_ra</name>
          <description>
            Right Ascension of ME08 Match
          </description>
          <unit>degree</unit>
          <ucd>
            pos.eq.ra;em.opt
          </ucd>
          <dataType xsi:type="vs:VOTableType">double</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>rmag_error</name>
          <description>
            r Magnitude Standard Deviation
          </description>
          <unit>mag</unit>
          <ucd>
            stat.error;phot.mag;em.opt.R
          </ucd>
          <dataType xsi:type="vs:VOTableType">double</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>stellar_mass</name>
          <description>
            Stellar Mass
          </description>
          <unit>Solar_Mass</unit>
          <ucd>
            phys.mass
          </ucd>
          <dataType xsi:type="vs:VOTableType">double</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>ks_var_flag</name>
          <description>
            Variability Based on K-S Statistic
          </description>
          <ucd>
            meta.code;src.var
          </ucd>
          <dataType xsi:type="vs:VOTableType">char</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>optical_id</name>
          <description>
            Identification of Optical Match
          </description>
          <ucd>
            meta.id.cross;em.opt
          </ucd>
          <dataType xsi:type="vs:VOTableType">char</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>prob_binary_member</name>
          <description>
            Probability That Object Is Likely Binary Member
          </description>
          <ucd>
            stat.probability
          </ucd>
          <dataType xsi:type="vs:VOTableType">double</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>optical_notes</name>
          <description>
            Additional Notes Concerning Optical Match
          </description>
          <ucd>
            meta.note;em.opt
          </ucd>
          <dataType xsi:type="vs:VOTableType">char</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>imag_error</name>
          <description>
            i Magnitude Standard Deviation
          </description>
          <unit>mag</unit>
          <ucd>
            stat.error;phot.mag;em.opt.I
          </ucd>
          <dataType xsi:type="vs:VOTableType">double</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>prob_member</name>
          <description>
            Probability That Object Is Member
          </description>
          <ucd>
            stat.probability
          </ucd>
          <dataType xsi:type="vs:VOTableType">double</dataType>
          <flag>
            nullable
          </flag>
        </column>
      </table>
    </schema>
  </tableset>
</ri:Resource>