Planck 2013 results. I. Overview of products and scientific results

The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sky continuously since 12 August 2009. In March 2013, ESA and the Planck Collaboration released the...

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Autores: Tauber, J. A., Barreiro, R. Belén, Bonavera, Laura, Curto, Andrés, Diego, José María, Fosalba, Pablo, González-Nuevo, J., Herranz, Diego, López-Caniego, M., Marcos-Caballero, A., Martínez-González, Enrique, Rebolo López, Rafael, Toffolatti, Luigi, Vielva, Patricio, Planck Collaboration
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2014
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:dnet:digitalcsic_::1be56542ca063d4006e053583d2b7b62
Acceso en línea:http://hdl.handle.net/10261/110552
Access Level:acceso abierto
Palabra clave:Cosmic background radiation
Space vehicles: instruments
Instrumentation: detectors
Cosmology: observations
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spelling Planck 2013 results. I. Overview of products and scientific resultsTauber, J. A.Barreiro, R. BelénBonavera, LauraCurto, AndrésDiego, José MaríaFosalba, PabloGonzález-Nuevo, J.Herranz, DiegoLópez-Caniego, M.Marcos-Caballero, A.Martínez-González, EnriqueRebolo López, RafaelToffolatti, LuigiVielva, PatricioPlanck CollaborationCosmic background radiationSpace vehicles: instrumentsInstrumentation: detectorsCosmology: observationsThe European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sky continuously since 12 August 2009. In March 2013, ESA and the Planck Collaboration released the initial cosmology products based on the first 15.5 months of Planck data, along with a set of scientific and technical papers and a web-based explanatory supplement. This paper gives an overview of the mission and its performance, the processing, analysis, and characteristics of the data, the scientific results, and the science data products and papers in the release. The science products include maps of the cosmic microwave background (CMB) and diffuse extragalactic foregrounds, a catalogue of compact Galactic and extragalactic sources, and a list of sources detected through the Sunyaev-Zeldovich effect. The likelihood code used to assess cosmological models against the Planck data and a lensing likelihood are described. Scientific results include robust support for the standard six-parameter ΛCDM model of cosmology and improved measurements of its parameters, including a highly significant deviation from scale invariance of the primordial power spectrum. The Planck values for these parameters and others derived from them are significantly different from those previously determined. Several large-scale anomalies in the temperature distribution of the CMB, first detected by WMAP, are confirmed with higher confidence. Planck sets new limits on the number and mass of neutrinos, and has measured gravitational lensing of CMB anisotropies at greater than 25σ. Planck finds no evidence for non-Gaussianity in the CMB. Planck's results agree well with results from the measurements of baryon acoustic oscillations. Planck finds a lower Hubble constant than found in some more local measures. Some tension is also present between the amplitude of matter fluctuations (σ8) derived from CMB data and that derived from Sunyaev-Zeldovich data. The Planck and WMAP power spectra are offset from each other by an average level of about 2% around the first acoustic peak. Analysis of Planck polarization data is not yet mature, therefore polarization results are not released, although the robust detection of E-mode polarization around CMB hot and cold spots is shown graphically.The Planck Collaboration acknowledge 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 PRACE (EU).Peer ReviewedEDP Sciences2015201520142015info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/110552reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Ingléshttp://dx.doi.org/10.1051/0004-6361/201321529info:eu-repo/semantics/openAccessoai:dnet:digitalcsic_::1be56542ca063d4006e053583d2b7b622026-05-22T06:33:51Z
dc.title.none.fl_str_mv Planck 2013 results. I. Overview of products and scientific results
title Planck 2013 results. I. Overview of products and scientific results
spellingShingle Planck 2013 results. I. Overview of products and scientific results
Tauber, J. A.
Cosmic background radiation
Space vehicles: instruments
Instrumentation: detectors
Cosmology: observations
title_short Planck 2013 results. I. Overview of products and scientific results
title_full Planck 2013 results. I. Overview of products and scientific results
title_fullStr Planck 2013 results. I. Overview of products and scientific results
title_full_unstemmed Planck 2013 results. I. Overview of products and scientific results
title_sort Planck 2013 results. I. Overview of products and scientific results
dc.creator.none.fl_str_mv Tauber, J. A.
Barreiro, R. Belén
Bonavera, Laura
Curto, Andrés
Diego, José María
Fosalba, Pablo
González-Nuevo, J.
Herranz, Diego
López-Caniego, M.
Marcos-Caballero, A.
Martínez-González, Enrique
Rebolo López, Rafael
Toffolatti, Luigi
Vielva, Patricio
Planck Collaboration
author Tauber, J. A.
author_facet Tauber, J. A.
Barreiro, R. Belén
Bonavera, Laura
Curto, Andrés
Diego, José María
Fosalba, Pablo
González-Nuevo, J.
Herranz, Diego
López-Caniego, M.
Marcos-Caballero, A.
Martínez-González, Enrique
Rebolo López, Rafael
Toffolatti, Luigi
Vielva, Patricio
Planck Collaboration
author_role author
author2 Barreiro, R. Belén
Bonavera, Laura
Curto, Andrés
Diego, José María
Fosalba, Pablo
González-Nuevo, J.
Herranz, Diego
López-Caniego, M.
Marcos-Caballero, A.
Martínez-González, Enrique
Rebolo López, Rafael
Toffolatti, Luigi
Vielva, Patricio
Planck Collaboration
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Cosmic background radiation
Space vehicles: instruments
Instrumentation: detectors
Cosmology: observations
topic Cosmic background radiation
Space vehicles: instruments
Instrumentation: detectors
Cosmology: observations
description The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sky continuously since 12 August 2009. In March 2013, ESA and the Planck Collaboration released the initial cosmology products based on the first 15.5 months of Planck data, along with a set of scientific and technical papers and a web-based explanatory supplement. This paper gives an overview of the mission and its performance, the processing, analysis, and characteristics of the data, the scientific results, and the science data products and papers in the release. The science products include maps of the cosmic microwave background (CMB) and diffuse extragalactic foregrounds, a catalogue of compact Galactic and extragalactic sources, and a list of sources detected through the Sunyaev-Zeldovich effect. The likelihood code used to assess cosmological models against the Planck data and a lensing likelihood are described. Scientific results include robust support for the standard six-parameter ΛCDM model of cosmology and improved measurements of its parameters, including a highly significant deviation from scale invariance of the primordial power spectrum. The Planck values for these parameters and others derived from them are significantly different from those previously determined. Several large-scale anomalies in the temperature distribution of the CMB, first detected by WMAP, are confirmed with higher confidence. Planck sets new limits on the number and mass of neutrinos, and has measured gravitational lensing of CMB anisotropies at greater than 25σ. Planck finds no evidence for non-Gaussianity in the CMB. Planck's results agree well with results from the measurements of baryon acoustic oscillations. Planck finds a lower Hubble constant than found in some more local measures. Some tension is also present between the amplitude of matter fluctuations (σ8) derived from CMB data and that derived from Sunyaev-Zeldovich data. The Planck and WMAP power spectra are offset from each other by an average level of about 2% around the first acoustic peak. Analysis of Planck polarization data is not yet mature, therefore polarization results are not released, although the robust detection of E-mode polarization around CMB hot and cold spots is shown graphically.
publishDate 2014
dc.date.none.fl_str_mv 2014
2015
2015
2015
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
Publisher's version
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/110552
url http://hdl.handle.net/10261/110552
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv http://dx.doi.org/10.1051/0004-6361/201321529
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
dc.source.none.fl_str_mv reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC
instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str DIGITAL.CSIC. Repositorio Institucional del CSIC
collection DIGITAL.CSIC. Repositorio Institucional del CSIC
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