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<ri:Resource created="2023-11-06T08:56:30Z" status="active" updated="2026-08-03T07:30:13Z" 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>Ultraluminous X-ray sources in local Universe</title><shortName>J/MNRAS/498/4790</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/498/4790</identifier><altIdentifier>doi:10.26093/cds/vizier/bg-fj-4np</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kovlakas K.</name></creator><creator><name>Zezas A.</name></creator><creator><name>Andrews J.J.</name></creator><creator><name>Basu-Zych A.</name></creator><creator><name>Fragos T.,Hornschemeier A.</name></creator><creator><name>Lehmer B.</name></creator><creator><name>Ptak A.</name></creator><date role="Updated">2026-08-03T07:30:13Z</date><date role="Created">2023-11-06T08:56:30Z</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>galaxies</subject><subject>catalogs</subject><subject>astrometry</subject><description>Using the Chandra Source Catalog 2.0 and a newly compiled catalogue of galaxies in the local Universe, we deliver a census of ultraluminous X-ray source (ULX) populations in nearby galaxies. We find 629 ULX candidates in 309 galaxies with distance smaller than 40Mpc. The foreground/background contamination is ~20 per cent. The ULX populations in bona fide star-forming galaxies scale on average with star formation rate and stellar mass (M_*_) such that the number of ULXs per galaxy is 0.45^+0.06^_-0.09_xSFR/(M_{sun}_/yr)+3.3^+3.8^_-3.2_xM_*_/M_{sun}_. The scaling depends strongly on the morphological type. This analysis shows that early spiral galaxies contain an additional population of ULXs that scales with M_*_. We also confirm the strong anticorrelation of the ULX rate with the host galaxy's metallicity. In the case of early-type galaxies, we find that there is a non-linear dependence of the number of ULXs with M_*_, which is interpreted as the result of star formation history differences. Taking into account age and metallicity effects, we find that the predictions from X-ray binary population synthesis models are consistent with the observed ULX rates in early-type galaxies, as well as spiral/irregular galaxies.</description><source format="bibcode">2020MNRAS.498.4790K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/498/4790</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/IX/57">IX/57 : The Chandra Source Catalog (CSC), Release 2.0 (Evans+, 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Number of ULXs by subtracting interlopers</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Nulx</name><description>? Upper error on Nulx</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Nulx</name><description>? Lower error on Nulx</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AGN</name><description>[Y/N/ ] Indicates if the galaxy hosts an AGN (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ID</name><description>[92/6740437] Source identifier from HyperLEDA and HECATE (1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Galaxy name (1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="28*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000) (1)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000) (1)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>R1</name><description>Semimajor axis (1)</description><unit>arcmin</unit><ucd>phys.angSize.smajAxis</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R2</name><description>? 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ID</name><description>[92/6740437] Host galaxy identifier from HyperLEDA and HECATE</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>X-ray source name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="22*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>Flux</name><description>? 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Upper bound on Flux</description><unit>mW.m**-2</unit><ucd>phot.flux;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Flagp</name><description>[0/1] Flag indicating if the source is a pile-up source (2)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Flagu</name><description>[0/1] Flag indicating if the source is unreliable (0:reliable, 1:unreliable) (3)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Flagn</name><description>[0/1] Flag indicating if the source is nuclear (4)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>c</name><description>Galactocentric scale parameter (5)</description><ucd>instr.scale;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LX</name><description>? X-ray luminosity converted from Flux adopting the distance of the host galaxy in the HECATE</description><unit>1e-07W</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_LX</name><description>? Lower bound on LX</description><unit>1e-07W</unit><ucd>phys.luminosity;em.X-ray;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_LX</name><description>? Upper bound on LX</description><unit>1e-07W</unit><ucd>phys.luminosity;em.X-ray;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>