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<ri:Resource created="2009-09-22T09:47:18Z" 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>HST imaging of brightest cluster galaxies</title><shortName>J/AJ/125/478</shortName><identifier>ivo://CDS.VizieR/J/AJ/125/478</identifier><altIdentifier>doi:10.26093/cds/vizier.51250478</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Laine S.</name></creator><creator><name>Van Der Marel R.P.</name></creator><creator><name>Lauer T.R.</name></creator><creator><name>Postman M.</name></creator><creator><name>O'Dea C.P.</name></creator><creator><name>Owen F.N.</name></creator><date role="Updated">2023-04-06T16:50:56Z</date><date role="Created">2009-09-22T09:47:18Z</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>galaxies</subject><subject>photometry</subject><description>We used the Hubble Space Telescope Wide Field Planetary Camera 2 to obtain Iband images of the centers of 81 brightest cluster galaxies (BCGs), drawn from a volume-limited sample of nearby BCGs. The images show a rich variety of morphological features, including multiple or double nuclei, dust, stellar disks, point-source nuclei, and central surface brightness depressions. Highresolution surface brightness profiles could be inferred for 60 galaxies. 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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>Cluster</name><description>Cluster name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>OName</name><description>Other name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension of the BCG center (J2000.0) (1)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination of the BCG center (J2000.0) (1)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>cz</name><description>Heliocentric velocity cz for the BCG</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Dist</name><description>Angular diameter distance of the BCG</description><unit>Mpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rmet</name><description>R-band metric magnitude in an aperture of 10h^-1^kpc</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VMAG</name><description>Total absolute V-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logLV</name><description>Total V-band luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F4</name><description>[YSN] Profiles are shown in Fig.4 (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>North</name><description>Orientation on the sky of the images that are shown in Fig. 1.</description><ucd>obs.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E(B-V)</name><description>Foreground reddening E(BV)</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Notes</name><description>Identifies any special features seen in the HST images (3)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>BM</name><description>Bautz-Morgan cluster morphology classification</description><ucd>src.class.struct</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>RMAG</name><description>Absolute R-band metric magnitude of the BCG inside an aperture of 10kpc radius</description><unit>mag</unit><ucd>phot.mag;em.opt.R;instr.fov</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>alpha</name><description>Parameter {alpha}, which measures the logarithmic slope of the metric luminosity as a function of radius, determined at a physical radius of 10kpc</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>delta</name><description>Residual {delta} between the observed metric luminosity and that predicted by the BCG standard-candle relation between metric luminosity and alpha</description><ucd>stat.fit.residual</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B-R</name><description>B-R color index at the metric radius after correcting for Galactic extinction and Kdimming</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rich</name><description>Richness Abell richness count</description><ucd>src.class.richness</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Sep</name><description>Projected separation of the BCG from the cluster center</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VelDiff</name><description>Difference between the line of sight velocity of the BCG and the systemic velocity of the cluster</description><unit>km/s</unit><ucd>phys.veloc;arith.diff</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>sigma</name><description>? 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