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<ri:Resource created="2017-11-17T14:11:46Z" 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>Groups of galaxies from from SDSS-DR7</title><shortName>J/AJ/154/96</shortName><identifier>ivo://CDS.VizieR/J/AJ/154/96</identifier><altIdentifier>doi:10.26093/cds/vizier.51540096</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>de Carvalho R.R.</name></creator><creator><name>Ribeiro A.L.B.</name></creator><creator><name>Stalder D.H.</name></creator><creator><name>Rosa R.R.</name></creator><creator><name>Costa A.P.,Moura T.C.</name></creator><date role="Updated">2017-12-15T18:24:47Z</date><date role="Created">2017-11-17T14:11:46Z</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>redshifted</subject><subject>x-ray-sources</subject><description>We investigate the dependence of stellar population properties of galaxies on group dynamical stage for a subsample of the Yang catalog. We classify groups according to their galaxy velocity distribution into Gaussian (G) and Non-Gaussian (NG). Using two totally independent approaches, we have shown that our measurement of Gaussianity is robust and reliable. Our sample covers Yang's groups in the redshift range 0.03{&lt;=}z{&lt;=}0.1, with mass {&gt;=}10^14^M_{Sun}_. The new method, called Hellinger Distance, to determine whether a group has a velocity distribution Gaussian or NG is very effective in distinguishing between the two families. NG groups present halo masses higher than the G ones, confirming previous findings. Examining the skewness and kurtosis of the velocity distribution of G and NG groups, we find that faint galaxies in NG groups are mainly infalling, for the first time, into the groups. We show that considering only faint galaxies in the outskirts; those in NG groups are older and more metal-rich than those in G groups. Also, examining the Projected Phase Space of cluster galaxies, we see that bright and faint galactic systems in G groups are in dynamical equilibrium-which does not seem to be the case in NG groups. These findings suggest that NG systems have a higher infall rate, assembling more galaxies that have experienced preprocessing before entering the group.</description><source format="bibcode">2017AJ....154...96D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/154/96</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/V/147">V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/294">II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/776/71">J/ApJ/776/71 : Galaxies in groups along the cosmic web. I. (Carollo+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/542/A36">J/A+A/542/A36 : Rich clusters from SDSS DR8 (Einasto+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/540/A123">J/A+A/540/A123 : Galaxy clusters from SDSS DR8 (Einasto+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/425/367">J/A+A/425/367 : REFLEX Galaxy Cluster Survey catalogue (Boehringer+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/129/435">J/ApJS/129/435 : NORAS galaxy cluster survey. I. 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