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<ri:Resource created="2020-02-05T09:19:18Z" 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>Chandra observations of SINGS galaxies</title><shortName>J/ApJS/243/3</shortName><identifier>ivo://CDS.VizieR/J/ApJS/243/3</identifier><altIdentifier>doi:10.26093/cds/vizier.22430003</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lehmer B.D.</name></creator><creator><name>Eufrasio R.T.</name></creator><creator><name>Tzanavaris P.</name></creator><creator><name>Basu-Zych A.</name></creator><creator><name>Fragos T.,Prestwich A.</name></creator><creator><name>Yukita M.</name></creator><creator><name>Zezas A.</name></creator><creator><name>Hornschemeier A.E.</name></creator><creator><name>Ptak A.</name></creator><date role="Updated">2020-09-30T10:33:58Z</date><date role="Created">2020-02-05T09:19:18Z</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>x-ray-binary-stars</subject><subject>x-ray-sources</subject><description>We present new Chandra constraints on the X-ray luminosity functions (XLFs) of X-ray binary (XRB) populations, as well as their scaling relations, for a sample of 38 nearby galaxies (D=3.4-29Mpc). Our galaxy sample is drawn primarily from the Spitzer Infrared Nearby Galaxies Survey (SINGS) and contains a wealth of Chandra (5.8Ms total) and multiwavelength data, allowing for star formation rates (SFRs) and stellar masses (M_*_) to be measured on subgalactic scales. We divided the 2478 X-ray-detected sources into 21 subsamples in bins of specific SFR (sSFR=SFR/M_*_) and constructed XLFs. To model the XLF dependence on sSFR, we fit a global XLF model, containing contributions from high-mass XRBs (HMXBs), low-mass XRBs (LMXBs), and background sources from the cosmic X-ray background that respectively scale with SFR, M_*_, and sky area. We find an HMXB XLF that is more complex in shape than previously reported and an LMXB XLF that likely varies with sSFR, potentially due to an age dependence. When applying our global model to XLF data for each individual galaxy, we discover a few galaxy XLFs that significantly deviate from our model beyond statistical scatter. Most notably, relatively low-metallicity galaxies have an excess of HMXBs above ~10^38^erg/s, and elliptical galaxies that have relatively rich populations of globular clusters (GCs) show excesses of LMXBs compared to the global model. Additional modeling of how the XRB XLF depends on stellar age, metallicity, and GC specific frequency is required to sufficiently characterize the XLFs of galaxies.</description><source format="bibcode">2019ApJS..243....3L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/243/3</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/J/ApJ/586/794">J/ApJ/586/794 : Multiwavelength luminosities of galaxies (Bell, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/602/231">J/ApJ/602/231 : Chandra X-ray point sources in nearby gal. (Colbert+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/617/240">J/ApJ/617/240 : Oxygen abundances in the GOODS-North field (Kobulnicky+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/681/197">J/ApJ/681/197 : ACS Virgo Cluster Survey. XV (Peng+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/695/580">J/ApJ/695/580 : Oxygen abundance in M83 (Bresolin+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/190/233">J/ApJS/190/233 : Spectroscopy and abundances of SINGS gal. (Moustakas+, 2010)</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/764/41">J/ApJ/764/41 : X-ray binary evolution across cosmic time (Fragos+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/772/82">J/ApJ/772/82 : A catalog of globular cluster systems (Harris+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/774/136">J/ApJ/774/136 : SINGS gal. 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(Miralles-Caballero+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/212/21">J/ApJS/212/21 : A deep Chandra ACIS survey of M83 (Long+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/817/95">J/ApJ/817/95 : X-ray observations of HCG galaxies (Tzanavaris+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/825/7">J/ApJ/825/7 : Evolution of ~6Ms CDF-S galaxies (Lehmer+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/466/1019">J/MNRAS/466/1019 : Bright HMXBs in THINGS galaxies (Sazonov+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/865/43">J/ApJ/865/43 : X-ray analysis of Chandra-COSMOS gal. 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