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dc.contributor.authorAde, Peter Anthony Robert
dc.contributor.authorAghanim, Nabila
dc.contributor.authorArnaud, M.
dc.contributor.authorAshdown, Mark
dc.contributor.authorAumont, J.
dc.contributor.authorBaccigalupi, C.
dc.contributor.authorBalbi, A.
dc.contributor.authorBanday, A. J.
dc.contributor.authorBarreiro Vilas, Rita Belén 
dc.contributor.authorBartelmann, M.
dc.contributor.authorBartlett, J. G.
dc.contributor.authorBattaner, E.
dc.contributor.authorBenabed, K.
dc.contributor.authorBenoît, A.
dc.contributor.authorBernard, J.-P.
dc.contributor.authorDiego Rodríguez, José María 
dc.contributor.authorHerranz Muñoz, Diego 
dc.contributor.authorLópez-Caniego Alcarria, Marcos
dc.contributor.authorMartínez González, Enrique
dc.contributor.authorVielva Martínez, Patricio 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2023-04-05T11:18:24Z
dc.date.available2023-04-05T11:18:24Z
dc.date.issued2011-12
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.urihttps://hdl.handle.net/10902/28458
dc.description.abstractWe present precise Sunyaev-Zeldovich (SZ) effect measurements in the direction of 62 nearby galaxy clusters (z < 0.5) detected at high signal-tonoise in the first Planck all-sky data set. The sample spans approximately a decade in total mass, 2 × 1014 M < M500 < 2 × 1015 M, where M500 is the mass corresponding to a total density contrast of 500. Combining these high quality Planck measurements with deep XMM-Newton X-ray data, we investigate the relations between D2 A Y500, the integrated Compton parameter due to the SZ effect, and the X-ray-derived gas mass Mg,500, temperature TX, luminosity LX,500, SZ signal analogue YX,500 = Mg,500 × TX, and total mass M500. After correction for the effect of selection bias on the scaling relations, we find results that are in excellent agreement with both X-ray predictions and recently-published ground-based data derived from smaller samples. The present data yield an exceptionally robust, high-quality local reference, and illustrate Planck?s unique capabilities for all-sky statistical studies of galaxy clusters.es_ES
dc.description.sponsorshipThe Planck Collaboration acknowledges the support of: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN and JA (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and DEISA (EU). The present work is partly based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and the USA (NASA). This research has made use of the following databases: SIMBAD, operated at CDS, Strasbourg, France; the NED database, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration; BAX, which is operated by the Laboratoire d’Astrophysique de Tarbes-Toulouse (LATT), under contract with the Centre National d’Etudes Spatiales (CNES). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.rssd.esa.int/Planck.es_ES
dc.format.extent14 p.es_ES
dc.language.isoenges_ES
dc.publisherEDP Scienceses_ES
dc.rights© ESO 2011es_ES
dc.sourceAstronomy and Astrophysics, 2011, 536, A11es_ES
dc.subject.otherGalaxies: clusters: interacluster mediumes_ES
dc.subject.otherX-rays: galaxies: clusterses_ES
dc.subject.otherCosmology: observationses_ES
dc.titlePlanck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relationses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1051/0004-6361/201116458es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1051/0004-6361/201116458
dc.type.versionpublishedVersiones_ES


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