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<ri:Resource created="2009-10-26T10:08:41Z" 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>NGC 3610 globular clusters HST BVI photometry</title><shortName>J/AJ/133/2737</shortName><identifier>ivo://CDS.VizieR/J/AJ/133/2737</identifier><altIdentifier>doi:10.26093/cds/vizier.51332737</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Goudfrooij P.</name></creator><creator><name>Schweizer F.</name></creator><creator><name>Gilmore D.</name></creator><creator><name>Whitmore B.C.</name></creator><date role="Updated">2018-01-04T08:22:03Z</date><date role="Created">2009-10-26T10:08:41Z</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>hst-photometry</subject><description>The Advanced Camera for Surveys on board the Hubble Space Telescope has been used to obtain deep, high-resolution images of the giant elliptical galaxy NGC 3610, a well-established remnant of a dissipative galaxy merger. These observations supersede previous, shallower observations that revealed the presence of a population of metal-rich globular clusters of intermediate age (~1.5-4Gyr). We detect a total of 580 cluster candidates, 46% more than from the previous WFPC2 images. 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