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<ri:Resource created="2010-03-29T13:09:47Z" 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>Central galaxies in groups and clusters</title><shortName>J/MNRAS/398/1129</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/398/1129</identifier><altIdentifier>doi:10.26093/cds/vizier.73981129</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Guo Y.</name></creator><creator><name>McIntosh D.H.</name></creator><creator><name>Mo H.J.</name></creator><creator><name>Katz N.</name></creator><creator><name>van den Bosch F.C.</name></creator><creator><name>Weinberg M.,Weinmann S.M.</name></creator><creator><name>Pasquali A.</name></creator><creator><name>Yang X.</name></creator><date role="Updated">2024-07-09T20:15:36Z</date><date role="Created">2010-03-29T13:09:47Z</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>galaxy-classification-systems</subject><subject>apparent-magnitude</subject><description>Using a statistically representative sample of 911 central galaxies (CENs) from the Sloan Digital Sky Survey (SDSS) Data Release 4 group catalogue, we study how the structure (shape and size) of the first rank (by stellar mass) group and cluster members depends on (1) galaxy stellar mass (M_star_), (2) the global environment defined by the dark matter halo mass (M_halo_) of the host group and (3) the local environment defined by their special halocentric position. We quantify the structure of SDSS galaxies with a galfit-based pipeline that fits two-dimensional Sersic models to the r-band image data. Through tests with simulated and real galaxy images, we demonstrate that our pipeline can recover Sersic parameters without significant bias. Moreover, to test the impact of local environment on CENs, we compare the structure of CENs with that satellite galaxies (SATs) of comparable M_star_.</description><source format="bibcode">2009MNRAS.398.1129G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/398/1129</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/II/267">II/267 : The SDSS Photometric Catalog, Release 4 (Adelman-McCarthy+, 2006)</relatedResource><relatedResource>http://www.sdss.org : SDSS Home 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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>Sam</name><description>Sample (CEN, S1 or S3)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Gal</name><description>Galaxy ID number (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Right ascension in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>mag</name><description>Apparent total magnitude</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a50</name><description>Semimajor axis</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n</name><description>Sersic index</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PA</name><description>[-180/180] Position angle</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sky</name><description>SDSS global sky background (in unit of ADU) used in image fitting</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>chi2v</name><description>Reduced chi^2^ of the best-fitting model</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>MAG</name><description>Absolute magnitude (2)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mstar</name><description>Stellar mass (in h^-2^*solMass unit)</description><unit>log(solMass)</unit><ucd>meta.unit;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rhl</name><description>Half-light radius (in h^-1^*kpc unit)</description><unit>kpc</unit><ucd>meta.unit;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>g-r</name><description>g−r colour index corrected to z=0.1</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mhalo</name><description>Host halo mass of the galaxy in (h^-2^*solMass unit)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>TT</name><description>[-1/1] Visual type of galaxy: 0=late-type, 1=early-type, -1=peculiar</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Sloan</name><description>Display the SDSS data: DR4 (2006) and DR7 (2009)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>