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<ri:Resource created="2013-07-01T13:23:52Z" 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>T1C photometry of NGC7507</title><shortName>J/A+A/555/A56</shortName><identifier>ivo://CDS.VizieR/J/A+A/555/A56</identifier><altIdentifier>doi:10.26093/cds/vizier.35550056</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Caso J.P.</name></creator><creator><name>Richtler T.</name></creator><creator><name>Bassino L.P.</name></creator><creator><name>Salinas R.</name></creator><creator><name>Lane R.R.</name></creator><creator><name>Romanowsky A.</name></creator><date role="Updated">2014-01-11T16:18:13Z</date><date role="Created">2013-07-01T13:23:52Z</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>photometry</subject><subject>globular-star-clusters</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>There is strong evidence that globular cluster systems (GCSs) of massive galaxies are largely assembled by infall/accretion processes. Therefore, we expect the GCSs of isolated elliptical galaxies to be poor. Although not completely isolated, NGC 7507 is a massive field elliptical galaxy with an apparently very low dark matter content. We determine the richness, the colour distribution, and the structural properties of the GCS of NGC 7507. 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