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<ri:Resource created="2015-04-29T13:49:59Z" 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>Velocity distributions in galaxy clusters</title><shortName>J/other/NewA/27.</shortName><identifier>ivo://CDS.VizieR/J/other/NewA/27.41</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sampaio F.S.</name></creator><creator><name>Ribeiro A.L.B.</name></creator><date role="Updated">2017-11-29T11:48:28Z</date><date role="Created">2015-04-29T13:49:59Z</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-kinematics</subject><description>We study 416 galaxy systems with more than 7 members selected from the 2MASS catalog. We applied five well known normality tests to the velocity distributions of these systems to distinguish Gaussian and non-Gaussian clusters. Using controlled samples, we estimated type I and II errors for each test. We verified that individual tests minimize the chances of classifying a Gaussian system as non-Gaussian, while the Fisher's meta-analysis method, a procedure to combine p-values from several statistical tests, minimizes the chances of classifying a non-Gaussian system as Gaussian. Taking the positive elements of each method and also including a modality analysis of the velocity distribution, we defined objective criteria to split up the sample into Gaussian and non-Gaussian clusters. Our analysis indicates that 50-58% of groups have Gaussian distribution, a lower fraction than that we found using individual normality tests, 71-87%. We also found that some properties of galaxy clusters are significantly different between Gaussian and non-Gaussian systems. For instance, non-Gaussian clusters have larger radii and contain more galaxies than Gaussian clusters. Finally, we discussed the importance of choosing the adequate methodology to classify galaxy systems from their velocity distributions and also the dependence of the results on the criteria used to identify clusters in galaxy surveys.</description><source format="bibcode">2014NewA...27...41S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/NewA/27.41</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/ApJ/655/790">J/ApJ/655/790 : Groups of galaxies in 2MASS survey (Crook+, 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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>Group</name><description>[LDC HDC] Low or High Density Contrast group</description><ucd>meta.id.part;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>ID</name><description>[6/1260] Group number (1)</description><ucd>meta.id.part;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>N200</name><description>[8/300] Number of galaxies within R200</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>sigma</name><description>[43/950] Velocity dispersion {sigma}</description><unit>km/s</unit><ucd>phys.veloc.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R200</name><description>[0.1/3] Virial radius, R200</description><unit>Mpc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM200</name><description>[11.2/15.3] Mass of galaxies within R200</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>m12</name><description>[-4.3/0] Magnitude difference between the first and second brightest galaxies</description><unit>mag</unit><ucd>stat.variance;phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>v200</name><description>[0.6/4.2] Number density of galaxies (in N200*Mpc^-3^ unit)</description><unit>Mpc**-3</unit><ucd>meta.number;phys.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DP</name><description>[0/1] Gaussian (0) or non-Gaussian (1) group according to the DP test</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MA</name><description>[0/1] Gaussian (0) or non-Gaussian (1) group according to the metanalysis</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>mod</name><description>[0/1] Gaussian (0) or non-Gaussian (1) group according to the modality analysis</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>