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<ri:Resource created="2011-02-16T07:53:39Z" 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>LMXBs and globulars in early-type galaxies. II.</title><shortName>J/ApJ/690/512</shortName><identifier>ivo://CDS.VizieR/J/ApJ/690/512</identifier><altIdentifier>doi:10.26093/cds/vizier.16900512</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Humphrey P.J.</name></creator><date role="Updated">2018-01-02T13:43:12Z</date><date role="Created">2011-02-16T07:53:39Z</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>hst-photometry</subject><subject>galaxies</subject><subject>visible-astronomy</subject><subject>globular-star-clusters</subject><description>We present an astrometry and photometry catalogue of globular cluster (GC) candidates detected with the Hubble Space Telescope Wide Field Planetary Camera 2 in a sample of 19 early-type galaxies, appropriate for comparison with the low-mass X-ray binary populations observed with Chandra. In a companion paper (Cat. J/ApJ/689/983), we present the Chandra data and investigate the relation between these populations. We demonstrate that, although there is little evidence of a color-magnitude correlation for the GCs, after estimating mass and metallicity from the photometry under the assumption of a single-age simple stellar population, there is a significant positive correlation between mass and metallicity.</description><source format="bibcode">2009ApJ...690..512H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/690/512</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/VII/176">VII/176 : Photometry and Spectroscopy of Elliptical Galaxies (Faber+ 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/586/814">J/ApJ/586/814 : NGC 4472 Chandra/HST study (Maccarone+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/455/453">J/A+A/455/453 : Globular Cluster System of NGC5846 (Chies-Santos+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/671/1624">J/ApJ/671/1624 : NGC 1533 globular cluster candidates (Degraaff+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/689/983">J/ApJ/689/983 : LMXBs in early-type galaxies. 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