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<ri:Resource created="2015-02-24T14:28:33Z" 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>WMAP observations of Planck ESZ clusters</title><shortName>J/ApJ/771/137</shortName><identifier>ivo://CDS.VizieR/J/ApJ/771/137</identifier><altIdentifier>doi:10.26093/cds/vizier.17710137</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ma Y.-Z.</name></creator><creator><name>Hinshaw G.</name></creator><creator><name>Scott D.</name></creator><date role="Updated">2017-09-29T09:03:35Z</date><date role="Created">2015-02-24T14:28:33Z</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>radio-sources</subject><subject>surveys</subject><description>We examine the Sunyaev-Zeldovich (SZ) effect in the seven year Wilkinson Microwave Anisotropy Probe (WMAP) data by cross-correlating it with the Planck Early-release Sunyaev-Zeldovich catalog (Cat. VIII/88/esz). Our analysis proceeds in two parts. We first perform a stacking analysis in which the filtered WMAP data are averaged at the locations of the 175 Planck clusters. We then perform a regression analysis to compare the mean amplitude of the SZ signal, Y_500_, in the WMAP data to the corresponding amplitude in the Planck data. The aggregate Planck clusters are detected in the seven year WMAP data with a signal-to-noise ratio of 16.3. In the regression analysis, we find that the SZ amplitude measurements agree to better than 25%: a=1.23+/-0.18 for the fit Y_500_^wmap^=aY_500_^planck^.</description><source format="bibcode">2013ApJ...771..137M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/771/137</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/VIII/88">VIII/88 : Planck Early Release Compact Source Catalogue (Planck, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/772/25">J/ApJ/772/25 : Massive SZE clusters observations with ACT (Sifon+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/127">J/ApJ/763/127 : Galaxy clusters in the SPT survey (Reichardt+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/557/L1">J/A+A/557/L1 : WMAP cosmic microwave background data (Rassat+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/192/15">J/ApJS/192/15 : Seven-year WMAP catalog (Gold+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/170/288">J/ApJS/170/288 : WMAP 3 Year Temperature Analysis (Hinshaw+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/376/1073">J/MNRAS/376/1073 : Sunyaev-Zel'dovich effect in galaxy clusters (Zemcov+, 2007)</relatedResource><relatedResource>http://lambda.gsfc.nasa.gov/ : Legacy Archive for Microwave Background Data</relatedResource><relatedResource>http://www.cosmos.esa.int/web/planck : Planck home page</relatedResource><relatedResource>http://map.gsfc.nasa.gov/ : WMAP home 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