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<ri:Resource created="2015-07-31T12:35:23Z" status="active" updated="2026-01-13T18:57:57Z" 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>SFRs of Brightest Cluster Galaxies</title><shortName>J/MNRAS/444/L63</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/444/L63</identifier><altIdentifier>doi:10.26093/cds/vizier.74449063</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fraser-McKelvie A.</name></creator><creator><name>Brown M.J.I.</name></creator><creator><name>Pimbblet K.A.</name></creator><date role="Updated">2026-01-13T18:57:57Z</date><date role="Created">2015-07-31T12:35:23Z</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>infrared-photometry</subject><description>We present the mid-infrared star formation rates of 245 X-ray selected, nearby (z&lt;0.1) brightest cluster galaxies (BCGs). A homogeneous and volume limited sample of BCGs was created by X-ray selecting clusters with Lx&gt;1x10^44^erg/s. The Wide-Field Infrared Survey Explorer (WISE) All WISE Data Release provides the first measurement of the 12{mu}m star formation indicator for all BCGs in the nearby Universe. Perseus A and Cygnus A are the only galaxies in our sample to have star formation rates of &gt;40M_{sun}_/yr, indicating that these two galaxies are highly unusual at current times. Stellar populations of 99+/-0.6 per cent of local BCGs are (approximately) passively evolving, with star formation rates of &lt;10M_{sun}_/yr. We find that in general, star formation produces only modest BCG growth at the current epoch.</description><source format="bibcode">2014MNRAS.444L..63F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/444/L63</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/J/MNRAS/384/1502">J/MNRAS/384/1502 : NIR photometry of X-ray luminous BCGs (Stott+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/4795">J/AJ/137/4795 : Dynamical state of brightest cluster galaxies (Coziol+ 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/34">J/ApJS/199/34 : Clusters of galaxies in SDSS-III (Wen+, 2012)</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/MNRAS/444/L63</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/444/L63</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/444/L63</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/444/L63</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/444/L63</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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BCG Stellar Mass</description><unit>1e+10solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Mstar</name><description>[0.02/5]? Error on Mstar (upper value)</description><unit>1e+10solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Mstar</name><description>[0.02/5]? Error on Mstar (lower value)</description><unit>1e+10solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_SFR</name><description>[&lt;] Upper Limit on SFR flag</description><ucd>meta.code.error;phys.SFR</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>SFR</name><description>[0/70]? 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