dc.contributor.author | Ade, Peter Anthony Robert | |
dc.contributor.author | Aghanim, Nabila | |
dc.contributor.author | Arnaud, M. | |
dc.contributor.author | Ashdown, Mark | |
dc.contributor.author | Aumont, J. | |
dc.contributor.author | Baccigalupi, C. | |
dc.contributor.author | Balbi, A. | |
dc.contributor.author | Banday, A. J. | |
dc.contributor.author | Barreiro Vilas, Rita Belén | |
dc.contributor.author | Bartelmann, M. | |
dc.contributor.author | Bartlett, J. G. | |
dc.contributor.author | Battaner, E. | |
dc.contributor.author | Battye, R. | |
dc.contributor.author | Benabed, K. | |
dc.contributor.author | Benoît, A. | |
dc.contributor.author | Diego Rodríguez, José María | |
dc.contributor.author | Herranz Muñoz, Diego | |
dc.contributor.author | López-Caniego Alcarria, Marcos | |
dc.contributor.author | Martínez González, Enrique | |
dc.contributor.author | Vielva Martínez, Patricio | |
dc.contributor.other | Universidad de Cantabria | es_ES |
dc.date.accessioned | 2023-04-05T10:58:54Z | |
dc.date.available | 2023-04-05T10:58:54Z | |
dc.date.issued | 2011-12 | |
dc.identifier.issn | 0004-6361 | |
dc.identifier.issn | 1432-0746 | |
dc.identifier.uri | https://hdl.handle.net/10902/28456 | |
dc.description.abstract | We 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.sponsorship | The 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.extent | 28 p. | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | EDP Sciences | es_ES |
dc.rights | © ESO 2011 | es_ES |
dc.source | Astronomy and Astrophysics, 2011, 536, A8 | es_ES |
dc.subject.other | Cosmology: observations | es_ES |
dc.subject.other | Galaxies: clusters: general | es_ES |
dc.subject.other | Catalogs | es_ES |
dc.title | Planck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample | es_ES |
dc.type | info:eu-repo/semantics/article | es_ES |
dc.relation.publisherVersion | https://doi.org/10.1051/0004-6361/201116459 | es_ES |
dc.rights.accessRights | openAccess | es_ES |
dc.identifier.DOI | 10.1051/0004-6361/201116459 | |
dc.type.version | publishedVersion | es_ES |