dc.contributor.author | Ade, Peter Anthony Robert | |
dc.contributor.author | Aghanim, Nabila | |
dc.contributor.author | Argüeso, F. | |
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 | Barreiro Vilas, Rita Belén | |
dc.contributor.author | Bartlett, J. G. | |
dc.contributor.author | Battaner, E. | |
dc.contributor.author | Benabed, K. | |
dc.contributor.author | Bernard, J.-P. | |
dc.contributor.author | Bersanelli, M. | |
dc.contributor.author | Bhatia, R. | |
dc.contributor.author | Bonaldi, A. | |
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 | 2023-04-05T11:42:54Z | |
dc.date.available | 2023-04-05T11:42:54Z | |
dc.date.issued | 2011-12 | |
dc.identifier.issn | 0004-6361 | |
dc.identifier.issn | 1432-0746 | |
dc.identifier.uri | https://hdl.handle.net/10902/28461 | |
dc.description.abstract | The data reported in Planck?s Early Release Compact Source Catalogue (ERCSC) are exploited to measure the number counts (dN/dS) of extragalactic radio sources at 30, 44, 70, 100, 143 and 217 GHz. Due to the full-sky nature of the catalogue, this measurement extends to the rarest and brightest sources in the sky. At lower frequencies (30, 44, and 70 GHz) our counts are in very good agreement with estimates based on WMAP data, being somewhat deeper at 30 and 70 GHz, and somewhat shallower at 44 GHz. Planck?s source counts at 143 and 217 GHz join smoothly with the fainter ones provided by the SPT and ACT surveys over small fractions of the sky. An analysis of source spectra, exploiting Planck?s uniquely broad spectral coverage, finds clear evidence of a steepening of the mean spectral index above about 70 GHz. This implies that, at these frequencies, the contamination of the CMB power spectrum by radio sources below the detection limit is significantly lower than previously estimated. | es_ES |
dc.description.sponsorship | The Planck Collaboration thanks the referee, Ronald Ekers, for his insightful comments, which helped improve the paper. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France. The 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). A description of the Planck Collaboration and a list of its members can be found at http://www.rssd.esa.int/index.php?project=PLANCK&page=Planck_Collaboration | es_ES |
dc.format.extent | 10 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, A13 | es_ES |
dc.subject.other | Surveys | es_ES |
dc.subject.other | Radio continuum: general | es_ES |
dc.subject.other | Galaxies: active | es_ES |
dc.title | Planck early results. XIII. Statistical properties of extragalactic radio sources in the Planck Early Release Compact Source Catalogue | es_ES |
dc.type | info:eu-repo/semantics/article | es_ES |
dc.relation.publisherVersion | https://doi.org/10.1051/0004-6361/201116471 | es_ES |
dc.rights.accessRights | openAccess | es_ES |
dc.identifier.DOI | 10.1051/0004-6361/201116471 | |
dc.type.version | publishedVersion | es_ES |