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<ri:Resource created="2016-03-07T08:23:53Z" status="active" updated="2025-06-13T15:25:00Z" 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>Rich galaxy clusters richness-based masses</title><shortName>J/A+A/587/A158</shortName><identifier>ivo://CDS.VizieR/J/A+A/587/A158</identifier><altIdentifier>doi:10.26093/cds/vizier.35870158</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Andreon S.</name></creator><date role="Updated">2016-03-07T08:16:02Z</date><date role="Created">2016-03-07T08:23:53Z</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>stellar-masses</subject><description>We present a catalog of galaxy cluster masses derived by exploiting the tight correlation between mass and richness, i.e., a properly computed number of bright cluster galaxies. The richness definition adopted in this work is properly calibrated, shows a small scatter with mass, and has a known evolution, which means that we can estimate accurate (0.16dex) masses more precisely than by adopting any other richness estimates or X-ray or SZ-based proxies based on survey data. We measured a few hundred galaxy clusters at 0.05&lt;z&lt;0.22 in the low-extinction part of the Sloan Digital Sky Survey footprint that are in the 2015 catalog of Planck-detected clusters, that have a known X-ray emission, that are in the Abell catalog, or that are among the most most cited in the literature. The derived cluster mass values are included in the distributed value-added cluster catalog of the 275 clusters with a derived mass larger than 10^14^M_{sun}_. A web front-end is available at the URL http://www.brera.mi.astro.it/~andreon/famous.html</description><source format="bibcode">2016A&amp;A...587A.158A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/587/A158</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/110">VII/110 : Rich Clusters of Galaxies (Abell+, 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/91">VIII/91 : Planck Catalog of Compact Sources Release 1 (Planck, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/534/A109">J/A+A/534/A109 : MCXC 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