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<ri:Resource created="2012-01-09T07:50:58Z" status="active" updated="2026-05-19T14:25:37Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" 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/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" xsi:type="vs:CatalogService"><title>X-ray point sources near the Galactic Center</title><shortName>J/ApJ/706/223</shortName><identifier>ivo://CDS.VizieR/J/ApJ/706/223</identifier><altIdentifier>doi:10.26093/cds/vizier.17060223</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hong J.</name></creator><creator><name>van den Berg M.</name></creator><creator><name>Grindlay J.E.</name></creator><creator><name>Laycock S.</name></creator><date role="Updated">2026-05-19T14:25:37Z</date><date role="Created">2012-01-09T07:50:58Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>x-ray-sources</subject><subject>surveys</subject><description>We present the log N-logS and spatial distributions of X-ray point sources in seven Galactic bulge (GB) fields within 4{deg} from the Galactic center (GC). We compare the properties of 1159 X-ray point sources discovered in our deep (100ks) Chandra observations of three low extinction Window fields near the GC with the X-ray sources in the other GB fields centered around Sgr B2, Sgr C, the Arches Cluster, and Sgr A* using Chandra archival data. To reduce the systematic errors induced by the uncertain X-ray spectra of the sources coupled with field-and-distance-dependent extinction, we classify the X-ray sources using quantile analysis and estimate their fluxes accordingly. We also compare the total X-ray and infrared surface brightness using the Chandra and Spitzer observations of the regions. GB X-ray sources can be of the same or similar type. Their X-ray luminosity and spectral properties support the idea that the most likely candidate is magnetic cataclysmic variables (CVs), primarily intermediate polars (IPs).</description><source format="bibcode">2009ApJ...706..223H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/706/223</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/chandra">B/chandra : The Chandra Archive Log (CXC, 1999-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/18">J/ApJS/194/18 : The Galactic Bulge Survey: X-ray observations (Jonker+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/700/1702">J/ApJ/700/1702 : ChaMPlane deep galactic bulge survey. I. (van den Berg+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/703/30">J/ApJ/703/30 : NIR counterparts to Chandra X-ray sources. I. (Mauerhan+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/685/463">J/ApJ/685/463 : ChaMPlane X-ray sources in the Galactic bulge (Koenig+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/685/958">J/ApJ/685/958 : Spitzer and Chandra sources in galactic center (Arendt+ 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/371/38">J/MNRAS/371/38 : X-ray observations of the Galaxy center (Wang+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/613/1179">J/ApJ/613/1179 : X-ray sources in Galactic Center (Muno+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/589/225">J/ApJ/589/225 : Chandra X-ray sources toward Galactic Center (Feigelson+,</relatedResource><relatedResource>http://hea-www.harvard.edu/ChaMPlane/ : ChaMPlane home page</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/706/223</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/706/223</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/706/223</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/706/223</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/706/223</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/706/223</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/706/223/table2 (Catalog of X-ray point sources in the Window and four Galactic bulge (GB) fields)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/706/223/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/706/223/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/706/223/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>270.62693389</ra><dec>-29.94649694</dec><sr>0.005555555555555556</sr></testQuery></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/706/223/table1 (Selected Galactic Bulge (GB) fields)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/706/223/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/706/223/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/706/223/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>270.8157</ra><dec>-29.9565</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/28778 28821-28823 28827 28830-28831</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/706/223?format=ascii</footprint><waveband>X-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/706/223/table2</name><description>Catalog of X-ray point sources in the Window and four Galactic bulge (GB) fields</description><column><name>e_E50</name><description>Error in E50</description><unit>keV</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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