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<ri:Resource created="2010-04-23T10:40:41Z" 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>Cepheids in 3 host galaxies</title><shortName>J/ApJS/183/109</shortName><identifier>ivo://CDS.VizieR/J/ApJS/183/109</identifier><altIdentifier>doi:10.26093/cds/vizier.21830109</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Riess A.G.</name></creator><creator><name>Macri L.</name></creator><creator><name>Li W.</name></creator><creator><name>Lampeitl H.</name></creator><creator><name>Casertano S.</name></creator><creator><name>Ferguson H.C.,Filippenko A.V.</name></creator><creator><name>Jha S.W.</name></creator><creator><name>Chornock R.</name></creator><creator><name>Greenhill L.</name></creator><creator><name>Mutchler M.,Ganeshalingam M.</name></creator><creator><name>Hicken M.</name></creator><date role="Updated">2017-07-11T13:08:31Z</date><date role="Created">2010-04-23T10:40:41Z</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>hst-photometry</subject><subject>variable-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><description>This is the first of two papers reporting measurements from a program to determine the Hubble constant to ~5% precision from a refurbished distance ladder. 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