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<ri:Resource created="2002-08-23T07:00:56Z" 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>HST photometry of M4</title><shortName>J/ApJS/120/265</shortName><identifier>ivo://CDS.VizieR/J/ApJS/120/265</identifier><altIdentifier>doi:10.26093/cds/vizier.21200265</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ibata R.A.</name></creator><creator><name>Richer H.B.</name></creator><creator><name>Fahlman G.G.</name></creator><creator><name>Bolte M.</name></creator><creator><name>Bond H.E.</name></creator><creator><name>Hesser J.E.,Pryor C.</name></creator><creator><name>Stetson P.B.</name></creator><date role="Updated">2002-08-23T07:01:58Z</date><date role="Created">2002-08-23T07:00:56Z</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>globular-star-clusters</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>This paper presents a detailed description of the acquisition and processing of a large body of imaging data for three fields in the globular cluster M4 taken with the Wide Field and Planetary Camera 2 aboard the Hubble Space Telescope. Analysis with the ALLFRAME package yielded the deepest photometry yet obtained for this cluster. The resulting data set for 4708 stars (positions and calibrated photometry in V, I, and, in two fields, U) spanning approximately six cluster core radii is presented. 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