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<ri:Resource created="2011-10-07T10:48:19Z" 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>Luminosity profiles of BCGs</title><shortName>J/ApJS/195/15</shortName><identifier>ivo://CDS.VizieR/J/ApJS/195/15</identifier><altIdentifier>doi:10.26093/cds/vizier.21950015</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Donzelli C.J.</name></creator><creator><name>Muriel H.</name></creator><creator><name>Madrid J.P.</name></creator><date role="Updated">2017-09-20T05:14:07Z</date><date role="Created">2011-10-07T10:48:19Z</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>absolute-magnitude</subject><subject>galaxies</subject><subject>photometry</subject><description>We have derived detailed R-band luminosity profiles and structural parameters for a total of 430 brightest cluster galaxies (BCGs), down to a limiting surface brightness of 24.5mag/arcsec^2^. Light profiles were initially fitted with a Sersic's R^1/n^ model, but we found that 205 (~48%) BCGs require a double component model to accurately match their light profiles. The best fit for these 205 galaxies is an inner Sersic model, with indices n~1-7, plus an outer exponential component. Thus, we establish the existence of two categories of the BCG luminosity profiles: single and double component profiles. We found that double profile BCGs are brighter (~0.2mag) than single profile BCGs. From a subsample of 24 BCGs, we found strong evidence that extra-light at intermediate radii in double profile BCGs is related to the presence of a faint stellar envelope. Similarly, from another subsample of 12 BCGs we also found that extra-light is related to star formation.</description><source format="bibcode">2011ApJS..195...15D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/195/15</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/VII/165">VII/165 : Measured Redshifts of Abell Clusters of Galaxies (Andernach 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/87">VII/87 : Data on 1889 Abell's clusters of galaxies (Leir+ 1977)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/125/478">J/AJ/125/478 : HST imaging of brightest cluster galaxies (Laine+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/440/28">J/ApJ/440/28 : Brightest Cluster Galaxies velocities (Postman+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/425/418">J/ApJ/425/418 : Absoulue R mag of brightest clusters galaxies (Lauer+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/241/486">J/ApJ/241/486 : Absolute magnitudes in 116 nearby Abell clusters (Hoessel+,</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/ApJS/195/15</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/195/15</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Abell cluster name (ANNNN)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>mue</name><description>Effective surface magnitude (in Rc band)</description><unit>mag.arcsec**-2</unit><ucd>phot.mag.sb</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>re</name><description>Effective radius (in Rc band)</description><unit>kpc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n</name><description>Sersic n parameter</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>mu0</name><description>? Central Rc surface magnitude</description><unit>mag.arcsec**-2</unit><ucd>phot.mag.sb;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r0</name><description>? Scale length</description><unit>kpc</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MAGS</name><description>Absolute magnitude of the Sersic component</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>MAGexp</name><description>? Absolute Rc magnitude of the exponential component</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MAGtot</name><description>Total Rc absolute magnitude of the BCG</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S/e</name><description>? Sersic to exponential component light ratio</description><ucd>phys.luminosity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>alpha</name><description>The {alpha} parameter (1)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>elli</name><description>Inner ellipticity (2)</description><ucd>src.ellipticity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ello</name><description>Outer ellipticity (2)</description><ucd>src.ellipticity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PAi</name><description>Inner position angle of the isophote (2)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PAo</name><description>Outer position angle of the isophote (2)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>MAGM</name><description>Metric absolute magnitude, calculated at r=14.5kpc</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>NED</name><description>Simbad column added by the CDS</description><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Positions of the cluster from Simbad (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions of the cluster from Simbad (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>