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<ri:Resource created="2022-11-16T09:36:55Z" 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>M83 X-ray binary classifications from HST</title><shortName>J/ApJ/912/31</shortName><identifier>ivo://CDS.VizieR/J/ApJ/912/31</identifier><altIdentifier>doi:10.26093/cds/vizier.19120031</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hunt Q.</name></creator><creator><name>Gallo E.</name></creator><creator><name>Chandar R.</name></creator><creator><name>Johns Mulia P.</name></creator><creator><name>Mok A.</name></creator><creator><name>Prestwich A.</name></creator><creator><name>Liu S.</name></creator><date role="Updated">2023-08-16T15:45:09Z</date><date role="Created">2022-11-16T09:36:55Z</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-binary-stars</subject><subject>hst-photometry</subject><subject>astronomical-object-identification</subject><subject>absolute-magnitude</subject><subject>two-color-diagrams</subject><subject>x-ray-sources</subject><subject>visible-astronomy</subject><description>Building on recent work by Chandar+ (2020, J/ApJ/890/150), we construct X-ray luminosity functions (XLFs) for different classes of X-ray binary (XRB) donors in the nearby star-forming galaxy M83 through a novel methodology. Rather than classifying low-versus high-mass XRBs based on the scaling of the number of X-ray sources with stellar mass and star formation rate, respectively, we utilize multiband Hubble Space Telescope imaging data to classify each Chandra-detected compact X-ray source as a low-mass (i.e., donor mass &lt;~3M_{sun}_), high-mass (donor mass &gt;~8M_{sun}_), or intermediate-mass XRB based on either the location of its candidate counterpart on optical color-magnitude diagrams or the age of its host star cluster. In addition to the standard (single and/or truncated) power-law functional shape, we approximate the resulting XLFs with a Schechter function. We identify a marginally significant (at the 1{sigma}-to-2{sigma} level) exponential downturn for the high-mass XRB XLF, at l~38.48_-0.33_^+0.52^ (in log CGS units). In contrast, the low- and intermediate-mass XRB XLFs, as well as the total XLF of M83, are formally consistent with sampling statistics from a single power law. Our method suggests a non-negligible contribution from low- and possibly intermediate-mass XRBs to the total XRB XLF of M83, i.e., between 20% and 50%, in broad agreement with X-ray-based XLFs. More generally, we caution against considerable contamination from X-ray emitting supernova remnants to the published, X-ray-based XLFs of M83, and possibly all actively star-forming galaxies.</description><source format="bibcode">2021ApJ...912...31H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/912/31</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/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/chandra">B/chandra : The Chandra Archive Log (CXC, 1999-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/76">VIII/76 : Leiden/Argentine/Bonn (LAB) Survey of Galactic HI (Kalberla+ 2005)</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/A+A/410/53">J/A+A/410/53 : M83 X-ray sources (Soria+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/602/231">J/ApJ/602/231 : Chandra X-ray point sources in nearby gal. 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