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<ri:Resource created="2021-09-01T12:45:09Z" status="active" updated="2025-05-19T09:50:00Z" 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 binaries in M101 with HST optical data</title><shortName>J/ApJ/890/150</shortName><identifier>ivo://CDS.VizieR/J/ApJ/890/150</identifier><altIdentifier>doi:10.26093/cds/vizier.18900150</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chandar R.</name></creator><creator><name>Johns P.</name></creator><creator><name>Mok A.</name></creator><creator><name>Prestwich A.</name></creator><creator><name>Gallo E.</name></creator><creator><name>Hunt Q.</name></creator><date role="Updated">2024-04-19T13:57:38Z</date><date role="Created">2021-09-01T12:45:09Z</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>galaxies</subject><subject>visible-astronomy</subject><subject>x-ray-binary-stars</subject><subject>hst-photometry</subject><subject>x-ray-sources</subject><description>The high-energy emission from nearby, star-forming galaxies is dominated by X-ray binaries, where a neutron star or black hole is accreting mass from either a low-mass (&lt;~M_{sun}_) or high-mass (&gt;~8M_{sun}_) star. Donor stars with intermediate masses ~3-7M_{sun}_ are also possible, but rarer in our Galaxy. Since it is not possible to separate low-, intermediate-, and high-mass X-ray binaries (LMXBs, IMXBs, and HMXBs) from their X-ray properties alone, we use optical images of M101 taken with the Hubble Space Telescope to directly constrain the masses of donor stars in X-ray binaries down to ~3M_{sun}_. For X-ray binaries that still live within their parent star cluster, the age of the cluster provides strong constraints on the mass of the donor and hence type of binary. We present the classification, on a source-by-source basis, of 140 X-ray point sources in the nearby spiral galaxy M101 (D=6.4+/-0.2Mpc). We find that, overall, HMXBs appear to follow the spiral arms, while LMXBs dominate the bulge region as expected, but also appear to form an inter-arm disk population. The X-ray luminosity functions for HMXBs and LMXBs are well fit by a power-law distribution, dN/dL_X_{propto}L^{alpha}^, with {alpha}=-1.71+/-0.06 (HMXBs) and {alpha}=-1.96+/-0.08 (LMXBs), and the brightest sources are consistent with the expectations from sampling statistics without requiring a physical cutoff. Overall, our results for HMXB and LMXB populations agree well with the specific star formation rate map presented for M101 recently by Lehmer and collaborators.</description><source format="bibcode">2020ApJ...890..150C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/890/150</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, 1999-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/57">IX/57 : The Chandra Source Catalog (CSC), Release 2.0 (Evans+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/613/279">J/ApJ/613/279 : ACS Virgo Cluster Survey. III. M87 (Jordan+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/662/525">J/ApJ/662/525 : LMXBs in globular clusters of 5 galaxies (Kundu+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/689/983">J/ApJ/689/983 : LMXBs in early-type galaxies. I. Chandra (Humphrey+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/392/L55">J/MNRAS/392/L55 : Globular clusters in M31 from K-band phot. (Peacock+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/693/8">J/ApJ/693/8 : High-redshift QSOs in the COSMOS survey (Brusa+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/733/124">J/ApJ/733/124 : Cepheids in M101 observed with HST (Shappee+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/741/86">J/ApJ/741/86 : XRBs and star clusters in NGC 4449 (Rangelov+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/419/2095">J/MNRAS/419/2095 : HMXBs in nearby galaxies (Mineo+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/805/160">J/ApJ/805/160 : Old star clusters in M101 from HST (Simanton+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/228/2">J/ApJS/228/2 : Chandra Deep Field-South survey: 7Ms sources (Luo+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/239/13">J/ApJS/239/13 : Chandra PHAT X-ray catalog of the M31 disk (Williams+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/243/3">J/ApJS/243/3 : Chandra observations of SINGS galaxies (Lehmer+, 2019)</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/890/150</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/890/150</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/890/150</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/890/150</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/890/150</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/890/150</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/890/150/table1 (M101 X-ray point source properties)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/890/150/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/890/150/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/890/150/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>210.80459478</ra><dec>54.34798659</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/11434</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/890/150?format=ascii</footprint><waveband>X-ray</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/890/150/table1</name><description>M101 X-ray point source properties</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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