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  <title>NGC 4649 Chandra X-Ray Point Source Catalog 2</title>
  <shortName>NGC4649CX2</shortName>
  <identifier>ivo://nasa.heasarc/ngc4649cx2</identifier>
  <curation>
    <publisher ivo-id="ivo://nasa.heasarc/ASD">NASA/GSFC HEASARC</publisher>
    <creator>
      <name>Luo 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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    <subject>Survey Source</subject>
    <description>
      This table contains the main X-ray source catalog for the Chandra monitoring observations of the 16.5-Mpc distant elliptical galaxy, NGC 4649. The galaxy has been observed with Chandra ACIS-S3 in six separate pointings, reaching a total exposure of 299 ks. There are 501 X-ray sources detected in the 0.3-8.0 keV band in the merged observation or in one of the six individual observations; 399 sources are located within the D&amp;lt;sub&amp;gt;25&amp;lt;/sub&amp;gt; ellipse. The observed 0.3-8.0 keV luminosities of these 501 sources range from 9.3 x 10&amp;lt;sup&amp;gt;36&amp;lt;/sup&amp;gt; erg s&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; to 5.4 x 10&amp;lt;sup&amp;gt;39&amp;lt;/sup&amp;gt; erg s&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. The 90% detection completeness limit within the D&amp;lt;sub&amp;gt;25&amp;lt;/sub&amp;gt; ellipse is 5.5 x 10&amp;lt;sup&amp;gt;37&amp;lt;/sup&amp;gt; erg s&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. Based on the surface density of background active galactic nuclei (AGNs) and the detection completeness, we expect ~ 45 background AGNs among the catalog sources (~ 15 within the D&amp;lt;sub&amp;gt;25&amp;lt;/sub&amp;gt; ellipse). There are nine sources with luminosities greater than 10&amp;lt;sup&amp;gt;39&amp;lt;/sup&amp;gt; erg s&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, which are candidates for ultraluminous X-ray sources. The nuclear source of NGC 4649 is a low-luminosity AGN, with an intrinsic 2.0-8.0 keV X-ray luminosity of 1.5 x 10&amp;lt;sup&amp;gt;38&amp;lt;/sup&amp;gt; erg s&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. The X-ray colors suggest that the majority of the catalog sources are low-mass X-ray binaries (LMXBs). The authors find that 164 of the 501 X-ray sources show long-term variability, indicating that they are accreting compact objects, and discover four transient candidates and another four potential transients. They also identify 173 X-ray sources (141 within the D&amp;lt;sub&amp;gt;25&amp;lt;/sub&amp;gt; ellipse) that are associated with globular clusters (GCs) based on Hubble Space Telescope and ground-based data; these LMXBs tend to be hosted by red GCs. Although NGC 4649 has a much larger population of X-ray sources than the structurally similar early-type galaxies, NGC 3379 and NGC 4278, the X-ray source properties are comparable in all three systems. This HEASARC table contains the main Chandra source catalog of the basic properties of the 501 X-ray detected sources (Table 3 in the reference paper which includes both sources detected in the merged X-ray image as well as a number only detected in the individual observations), and also the information on source counts, hardness ratios and soft and hard X-ray colors in the merged observation for the same 501 X-ray detected sources (Table 4 in the reference paper). It does not contain the information on source counts, hardness ratios and soft and hard X-ray colors for these same sources in the six individual observations that were contained in Tables 5 - 10 of the reference paper. This table was created by the HEASARC in March 2013 based on the electronic version of Tables 3 and 4 from the reference paper which were obtained from the ApJS website.. This is a service provided by NASA HEASARC .
    </description>
    <source format="">
      2013ApJS..204...14L
    </source>
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          NGC 4649 Chandra X-Ray Point Source Catalog 2
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            Upper 1-Sigma Uncertainty in Net 1-2 keV Counts
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            Upper 1-Sigma Uncertainty in Hard X-Ray Color
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            Radial Distance of Source from Nucleus
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            Net 0.3-2 keV Counts
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            Lower 1-Sigma Uncertainty in Net 0.3-1 keV Counts
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            Upper 1-Sigma Uncertainty in Hardness Ratio
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            Lower 1-Sigma Uncertainty in Net 2-8 keV Counts
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            Net 2-8 keV Counts
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            Lower 1-Sigma Uncertainty in Net 0.3-8 keV Counts
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          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>opt_ctrpart_flag</name>
          <description>
            Flag [0-9] Indicates Optical Association Note
          </description>
          <ucd>
            meta.code;src;em.opt
          </ucd>
          <dataType xsi:type="vs:VOTableType">short</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>"__x_ra_dec"</name>
          <description>
            System unit vector column
          </description>
          <dataType xsi:type="vs:VOTableType">double</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>"__y_ra_dec"</name>
          <description>
            System unit vector column
          </description>
          <dataType xsi:type="vs:VOTableType">double</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>"__z_ra_dec"</name>
          <description>
            System unit vector column
          </description>
          <dataType xsi:type="vs:VOTableType">double</dataType>
          <flag>
            nullable
          </flag>
        </column>
        <column>
          <name>"__row"</name>
          <description>
            System index column
          </description>
          <dataType xsi:type="vs:VOTableType">char</dataType>
          <flag>
            nullable
          </flag>
        </column>
      </table>
    </schema>
  </tableset>
</ri:Resource>