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<ri:Resource created="2018-04-03T09:08:35Z" 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>Cool-core clusters with Chandra obs.</title><shortName>J/ApJ/843/76</shortName><identifier>ivo://CDS.VizieR/J/ApJ/843/76</identifier><altIdentifier>doi:10.26093/cds/vizier.18430076</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Andrade-Santos F.</name></creator><creator><name>Jones C.</name></creator><creator><name>Forman W.R.</name></creator><creator><name>Lovisari L.</name></creator><creator><name>Vikhlinin A.,van Weeren R.J.</name></creator><creator><name>Murray S.S.</name></creator><creator><name>Arnaud M.</name></creator><creator><name>Pratt G.W.</name></creator><creator><name>Democles J.</name></creator><creator><name>Kraft R.,Mazzotta P.</name></creator><creator><name>Bohringer H.</name></creator><creator><name>Chon G.</name></creator><creator><name>Giacintucci S.</name></creator><creator><name>Clarke T.E.</name></creator><creator><name>Borgani S.,David L.</name></creator><creator><name>Douspis M.</name></creator><creator><name>Pointecouteau E.</name></creator><creator><name>Dahle H.</name></creator><creator><name>Brown S.</name></creator><creator><name>Aghanim N.,Rasia E.</name></creator><date role="Updated">2018-05-16T07:04:29Z</date><date role="Created">2018-04-03T09:08:35Z</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>x-ray-sources</subject><subject>redshifted</subject><description>We derive and compare the fractions of cool-core clusters in the Planck Early Sunyaev-Zel'dovich sample of 164 clusters with z&lt;=0.35 and in a flux- limited X-ray sample of 100 clusters with z&lt;=0.30, using Chandra observations. We use four metrics to identify cool-core clusters: (1) the concentration parameter, which is the ratio of the integrated emissivity profile within 0.15 r_500_ to that within r_500_; (2) the ratio of the integrated emissivity profile within 40kpc to that within 400kpc; (3) the cuspiness of the gas density profile, which is the negative of the logarithmic derivative of the gas density with respect to the radius, measured at 0.04 r_500_; and (4) the central gas density, measured at 0.01 r_500_. We find that the sample of X-ray-selected clusters, as characterized by each of these metrics, contains a significantly larger fraction of cool-core clusters compared to the sample of SZ-selected clusters (44%+/-7% versus 28%+/-4% using the concentration parameter in the 0.15-1.0 r_500_ range, 61%+/-8% versus 36%+/-5% using the concentration parameter in the 40-400 kpc range, 64%+/-8% versus 38%+/-5% using the cuspiness, and 53%+/-7% versus 39+/-5% using the central gas density). Qualitatively, cool-core clusters are more X-ray luminous at fixed mass. Hence, our X-ray, flux-limited sample, compared to the approximately mass-limited SZ sample, is overrepresented with cool-core clusters. We describe a simple quantitative model that uses the excess luminosity of cool-core clusters compared to non-cool-core clusters at fixed mass to successfully predict the observed fraction of cool-core clusters in X-ray-selected samples.</description><source format="bibcode">2017ApJ...843...76A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/843/76</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/B/chandra">B/chandra : The Chandra Archive Log (CXC, 1999-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/88">VIII/88 : Planck Early Release Compact Source Catalogue (Planck, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/98/64">J/AJ/98/64 : VLA survey of Abell clusters of galaxies I. (Zhao+ 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/511/65">J/ApJ/511/65 : Einstein images of galaxy clusters (Jones &amp; Forman, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/182/12">J/ApJS/182/12 : ICM entropy profiles (ACCEPT) (Cavagnolo+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/536/A8">J/A+A/536/A8 : Planck early results. VIII. ESZ sample. 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