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<ri:Resource created="2016-04-21T13:35:40Z" 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>Galaxies in X-ray clusters with DES. I. Stellar mass</title><shortName>J/ApJ/816/98</shortName><identifier>ivo://CDS.VizieR/J/ApJ/816/98</identifier><altIdentifier>doi:10.26093/cds/vizier.18160098</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhang Y.</name></creator><creator><name>Miller C.</name></creator><creator><name>McKay T.</name></creator><creator><name>Rooney P.</name></creator><creator><name>Evrard A.E.</name></creator><creator><name>Romer A.K.,Perfecto R.</name></creator><creator><name>Song J.</name></creator><creator><name>Desai S.</name></creator><creator><name>Mohr J.</name></creator><creator><name>Wilcox H.</name></creator><creator><name>Bermeo-Hernandez A.,Jeltema T.</name></creator><creator><name>Hollowood D.</name></creator><creator><name>Bacon D.</name></creator><creator><name>Capozzi D.</name></creator><creator><name>Collins C.</name></creator><creator><name>Das R.,Gerdes D.</name></creator><creator><name>Hennig C.</name></creator><creator><name>Hilton M.</name></creator><creator><name>Hoyle B.</name></creator><creator><name>Kay S.</name></creator><creator><name>Liddle A.</name></creator><creator><name>Mann R.G.,Mehrtens N.</name></creator><creator><name>Nichol R.C.</name></creator><creator><name>Papovich C.</name></creator><creator><name>Sahlen M.</name></creator><creator><name>Soares-Santos M.,Stott J.</name></creator><creator><name>Viana P.T.</name></creator><creator><name>Abbott T.</name></creator><creator><name>Abdalla F.B.</name></creator><creator><name>Banerji M.</name></creator><creator><name>Bauer A.H.,Benoit-Levy A.</name></creator><creator><name>Bertin E.</name></creator><creator><name>Brooks D.</name></creator><creator><name>Buckley-Geer E.</name></creator><creator><name>Burke D.L.,Carnero Rosell A.</name></creator><creator><name>Castander F.J.</name></creator><creator><name>Diehl H.T.</name></creator><creator><name>Doel P.</name></creator><creator><name>Cunha C.E.,Eifler T.F.</name></creator><creator><name>Fausti Neto A.</name></creator><creator><name>Fernandez E.</name></creator><creator><name>Flaugher B.</name></creator><creator><name>Fosalba P.,Frieman J.</name></creator><creator><name>Gaztanaga E.</name></creator><creator><name>Gruen D.</name></creator><creator><name>Gruendl R.A.</name></creator><creator><name>Honscheid K.</name></creator><creator><name>James D.,Kuehn K.</name></creator><creator><name>Kuropatkin N.</name></creator><creator><name>Lahav O.</name></creator><creator><name>Maia M.A.G.</name></creator><creator><name>Makler M.</name></creator><creator><name>Marshall J.L.,Martini P.</name></creator><creator><name>Miquel R.</name></creator><creator><name>Ogando R.</name></creator><creator><name>Plazas A.A.</name></creator><creator><name>Roodman A.</name></creator><creator><name>Rykoff E.S.,Sako M.</name></creator><creator><name>Sanchez E.</name></creator><creator><name>Scarpine V.</name></creator><creator><name>Schubnell M.</name></creator><creator><name>Sevilla I.</name></creator><creator><name>Smith R.C.,Sobreira F.</name></creator><creator><name>Suchyta E.</name></creator><creator><name>Swanson M.E.C.</name></creator><creator><name>Tarle G.</name></creator><creator><name>Thaler J.</name></creator><creator><name>Tucker D.,Vikram V.</name></creator><creator><name>da Costa L.N.</name></creator><date role="Updated">2017-01-23T22:00:00Z</date><date role="Created">2016-04-21T13:35:40Z</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>x-ray-sources</subject><subject>galaxies</subject><subject>visible-astronomy</subject><subject>redshifted</subject><subject>surveys</subject><description>Using the science verification data of the Dark Energy Survey for a new sample of 106 X-ray selected clusters and groups, we study the stellar mass growth of bright central galaxies (BCGs) since redshift z~1.2. Compared with the expectation in a semi-analytical model applied to the Millennium Simulation, the observed BCGs become under-massive/under-luminous with decreasing redshift. We incorporate the uncertainties associated with cluster mass, redshift, and BCG stellar mass measurements into an analysis of a redshift-dependent BCG-cluster mass relation, m_*_{propto}(M_200_/1.5x10^14^M_{sun}_)^0.24+/-0.08^(1+z)^-0.19+/-0.34, and compare the observed relation to the model prediction. We estimate the average growth rate since z=1.0 for BCGs hosted by clusters of M_200,z_=10^13.8^M_{sun}_; at z=1.0: m_*,BCG_ appears to have grown by 0.13+/-0.11dex, in tension at the ~2.5{sigma} significance level with the 0.40 dex growth rate expected from the semi-analytic model. We show that the build-up of extended intracluster light after z=1.0 may alleviate this tension in BCG growth rates.</description><source format="bibcode">2016ApJ...816...98Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/816/98</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/xmm">B/xmm : XMM-Newton Observation Log (XMM-Newton Science Operation Center, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/446/3943">J/MNRAS/446/3943 : galaxies 2D phot. decompositions in SDSS-DR7 (Meert+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/444/L63">J/MNRAS/444/L63 : SFRs of Brightest Cluster Galaxies (Fraser-McKelvie+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/424/2086">J/MNRAS/424/2086 : LX-T relation in galaxy clusters (Hilton+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/423/1024">J/MNRAS/423/1024 : XCS-DR1 Cluster Catalogue (Mehrtens+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/423/422">J/MNRAS/423/422 : Early-type BCGs with star formation (Liu+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/172/615">J/ApJS/172/615 : GALFIT result for GEMS galaxies (Haussler+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/379/867">J/MNRAS/379/867 : BCG C4 cluster catalog (von der Linden+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/662/808">J/ApJ/662/808 : Cusp radius in luminous elliptical galaxies (Lauer+, 2007)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/816/98</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/816/98</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/816/98</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/816/98</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/816/98</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/816/98</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/816/98/table3 (Bright central galaxies (BCGs) and their host cluster properties)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/816/98/table3?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/816/98/table3?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/816/98/table3?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>8.9395833</ra><dec>-43.2996111</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/4420 4423 11539 6/17677 17686 17688 17689 17690 17712 17717 27256 27258 27259 33235 33894 33912 33945 33946 33947 33955 33971 33980 33984 33986 35390 35935 36098 38973 46151 46155 46162 46163 46168 46170 46174 46177 46181 46192</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/816/98?format=ascii</footprint><waveband>X-ray</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/816/98/table3</name><description>Bright central galaxies (BCGs) and their host cluster properties</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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