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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.authorBattye, R.
dc.contributor.authorBenabed, K.
dc.contributor.authorBenoît, A.
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.accessioned2023-04-05T10:58:54Z
dc.date.available2023-04-05T10:58:54Z
dc.date.issued2011-12
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.urihttps://hdl.handle.net/10902/28456
dc.description.abstractWe present the first all-sky sample of galaxy clusters detected blindly by the Planck satellite through the Sunyaev-Zeldovich (SZ) effect from its six highest frequencies. This early SZ (ESZ) sample is comprised of 189 candidates, which have a high signal-to-noise ratio ranging from 6 to 29. Its high reliability (purity above 95%) is further ensured by an extensive validation process based on Planck internal quality assessments and by external cross-identification and follow-up observations. Planck provides the first measured SZ signal for about 80% of the 169 previously-known ESZ clusters. Planck furthermore releases 30 new cluster candidates, amongst which 20 meet the ESZ signal-to-noise selection criterion. At the submission date, twelve of the 20 ESZ candidates were confirmed as new clusters, with eleven confirmed using XMM-Newton snapshot observations, most of them with disturbed morphologies and low luminosities. The ESZ clusters are mostly at moderate redshifts (86% with z below 0.3) and span more than a decade in mass, up to the rarest and most massive clusters with masses above 1 × 1015 M?.es_ES
dc.description.sponsorshipThe authors thank N. Schartel, ESA XMM-Newton project scientist, for granting the Director Discretionary Time used for confirmation of SZ Planck candidates. 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, operated by the Laboratoire d’Astrophysique de Tarbes-Toulouse (LATT), under contract with the Centre National d’Études Spatiales (CNES), SZ repository operated by IAS Data and Operation Center (IDOC) under contract with CNES. The authors acknowledge the use of software provided by the US National Virtual Observatory. A description of the Planck Collaboration and a list of its members, indicating which technical or scientific activities they have been involved in, can be found at http://www.rssd.esa.int/Planck.es_ES
dc.format.extent28 p.es_ES
dc.language.isoenges_ES
dc.publisherEDP Scienceses_ES
dc.rights© ESO 2011es_ES
dc.sourceAstronomy and Astrophysics, 2011, 536, A8es_ES
dc.subject.otherCosmology: observationses_ES
dc.subject.otherGalaxies: clusters: generales_ES
dc.subject.otherCatalogses_ES
dc.titlePlanck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster samplees_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1051/0004-6361/201116459es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1051/0004-6361/201116459
dc.type.versionpublishedVersiones_ES


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