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<ri:Resource created="2009-09-26T16:58:30Z" 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 sources in 5 galaxy clusters</title><shortName>J/ApJS/168/19</shortName><identifier>ivo://CDS.VizieR/J/ApJS/168/19</identifier><altIdentifier>doi:10.26093/cds/vizier.21680019</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Martel A.R.</name></creator><creator><name>Menanteau F.</name></creator><creator><name>Tozzi P.</name></creator><creator><name>Ford H.C.</name></creator><creator><name>Infante L.</name></creator><date role="Updated">2018-01-26T07:38:00Z</date><date role="Created">2009-09-26T16:58:30Z</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>galaxy-clusters</subject><subject>active-galactic-nuclei</subject><subject>x-ray-sources</subject><subject>hst-photometry</subject><subject>redshifted</subject><description>We present catalogs and images of optical counterparts to the Chandra-selected X-ray sources found in the fields of the five clusters RX J0152-1357, RX J0849+4452, RDCS J0910+5422, MS 1054-0321, and RDCS J1252-2927, which were imaged with the Advanced Camera for Surveys as part of the ACS Guaranteed Time Observer programs. A total of 98 X-ray sources fall within the ACS mosaics, and positive identifications are made for ~96% of them, including confirmed cluster members. 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