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<ri:Resource created="2012-08-20T11:59:35Z" 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>MgII absorbing gas around galaxies</title><shortName>J/ApJ/724/L176</shortName><identifier>ivo://CDS.VizieR/J/ApJ/724/L176</identifier><altIdentifier>doi:10.26093/cds/vizier.17249176</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chen H.-W.</name></creator><creator><name>Wild V.</name></creator><creator><name>Tinker J.L.</name></creator><creator><name>Gauthier J.-R.</name></creator><creator><name>Helsby J.E.,Shectman S.A.</name></creator><creator><name>Thompson I.B.</name></creator><date role="Updated">2013-01-03T13:12:25Z</date><date role="Created">2012-08-20T11:59:35Z</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>line-intensities</subject><subject>galaxies</subject><subject>spectroscopy</subject><subject>redshifted</subject><subject>quasars</subject><description>We study the connections between ongoing star formation, galaxy mass, and extended halo gas, in order to distinguish between starburst-driven outflows and infalling clouds that produce the majority of observed MgII absorbers at large galactic radii (&gt;~10h^-1^kpc) and to gain insights into halo gas contents around galaxies. We present new measurements of total stellar mass (M_star_), H{alpha} emission line strength (EW(H{alpha})), and specific star formation rate (sSFR) for the 94 galaxies described by Chen et al.'s 2010 paper (Cat. 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