dc.contributorUniversidade de São Paulo (USP)
dc.contributorAalto Univ
dc.contributorAfrican Inst Math Sci
dc.contributorAgenzia Spaziale Italiana
dc.contributorAix Marseille Univ
dc.contributorUniv Cambridge
dc.contributorUniv KwaZulu Natal
dc.contributorALMA Santiago Cent Off
dc.contributorUniv Toronto
dc.contributorIRAP
dc.contributorTrinity Coll Dublin
dc.contributorCALTECH
dc.contributorCEFCA
dc.contributorLawrence Berkeley Natl Lab
dc.contributorCEA Saclay
dc.contributorTech Univ Denmark
dc.contributorUniv Geneva
dc.contributorUniv Oviedo
dc.contributorRadboud Univ Nijmegen
dc.contributorUniv British Columbia
dc.contributorUniv Southern Calif
dc.contributorUCL
dc.contributorFlorida State Univ
dc.contributorUniv Helsinki
dc.contributorPrinceton Univ
dc.contributorUniv Calif Santa Barbara
dc.contributorUniv Illinois
dc.contributorUniv Padua
dc.contributorUniv Ferrara
dc.contributorUniv Roma La Sapienza
dc.contributorUniv Milan
dc.contributorUniv Trieste
dc.contributorUniv Roma Tor Vergata
dc.contributorNiels Bohr Inst
dc.contributorUniv La Laguna
dc.contributorESO Vitacura
dc.contributorEuropean Space Agcy
dc.contributorUniv E Campus
dc.contributorIst Nazl Fis Nucl
dc.contributorHGSFP
dc.contributorHeidelberg Univ
dc.contributorUniversidade Estadual Paulista (Unesp)
dc.contributorINAF Osservatorio Astron Padova
dc.contributorINAF Osservatorio Astron Roma
dc.contributorINAF Osservatorio Astron Trieste
dc.contributorINAF IASF Bologna
dc.contributorINAF IASF Milano
dc.contributorUniv Roma Sapienza
dc.contributorUniv Grenoble Alpes
dc.contributorImperial Coll London
dc.contributorUniv Joseph Fourier Grenoble I
dc.contributorInst Univ France
dc.contributorUniv Paris Sud 11
dc.contributorInst Astrophys Paris
dc.contributorUniv Oslo
dc.contributorInst Astrofis Canarias
dc.contributorCSIC Univ Cantabria
dc.contributorUniv Manchester
dc.contributorKavli Inst Cosmol Cambridge
dc.contributorUniv Paris 11
dc.contributorUniv Savoie
dc.contributorObserv Paris
dc.contributorCNRS
dc.contributorTelecom ParisTech
dc.contributorRussian Acad Sci
dc.contributorMax Planck Inst Astrophys
dc.contributorNatl Univ Ireland
dc.contributorEcole Polytech Fed Lausanne
dc.contributorSISSA
dc.contributorCardiff Univ
dc.contributorUPMC
dc.contributorUniv Calif Berkeley
dc.contributorUniv Oxford
dc.contributorCERN
dc.contributorUPMC Univ Paris 06
dc.contributorUniv Toulouse
dc.contributorLudwig Maximilian Univ Munich
dc.contributorUniv Granada
dc.contributorUniv Warsaw Observ
dc.date.accessioned2018-11-26T17:06:47Z
dc.date.available2018-11-26T17:06:47Z
dc.date.created2018-11-26T17:06:47Z
dc.date.issued2016-10-01
dc.identifierAstronomy & Astrophysics. Les Ulis Cedex A: Edp Sciences S A, v. 594, 24 p., 2016.
dc.identifier1432-0746
dc.identifierhttp://hdl.handle.net/11449/162077
dc.identifier10.1051/0004-6361/201525826
dc.identifierWOS:000385832200011
dc.identifierWOS000385832200011.pdf
dc.description.abstractWe have constructed all-sky Compton parameters maps, y-maps, of the thermal Sunyaev-Zeldovich (tSZ) effect by applying specifically tailored component separation algorithms to the 30 to 857 GHz frequency channel maps from the Planck satellite. These reconstructed y-maps are delivered as part of the Planck 2015 release. The y-maps are characterized in terms of noise properties and residual foreground contamination, mainly thermal dust emission at large angular scales, and cosmic infrared background and extragalactic point sources at small angular scales. Specific masks are defined to minimize foreground residuals and systematics. Using these masks, we compute the y-map angular power spectrum and higher order statistics. From these we conclude that the y-map is dominated by tSZ signal in the multipole range, 20 < l < 600. We compare the measured tSZ power spectrum and higher order statistics to various physically motivated models and discuss the implications of our results in terms of cluster physics and cosmology.
dc.languageeng
dc.publisherEdp Sciences S A
dc.relationAstronomy & Astrophysics
dc.rightsAcesso aberto
dc.sourceWeb of Science
dc.subjectlarge-scale structure of Universe
dc.subjectcosmology: observations
dc.titlePlanck 2015 results XXII. A map of the thermal Sunyaev-Zeldovich effect
dc.typeArtículos de revistas


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