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<ri:Resource created="2010-11-26T12:07:57Z" 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>Photometry of globulars in early galaxies</title><shortName>J/A+A/525/A19</shortName><identifier>ivo://CDS.VizieR/J/A+A/525/A19</identifier><altIdentifier>doi:10.26093/cds/vizier.35250019</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chies-Santos A.L.</name></creator><creator><name>Larsen S.S.</name></creator><creator><name>Wehner E.M.</name></creator><creator><name>Kuntschner H.</name></creator><creator><name>Strader J.,Brodie J.P.</name></creator><date role="Updated">2011-02-14T20:26:06Z</date><date role="Created">2010-11-26T12:07:57Z</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>globular-star-clusters</subject><subject>photometry</subject><description>The combination of optical and near-infrared (NIR) colours has the potential to break the age/metallicity degeneracy and offers a better metallicity sensitivity than optical colours alone. Previous studies of extragalactic globular clusters (GCs) with this colour combination, however, have suffered from small samples or have been restricted to a few galaxies. 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