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dc.contributor.authorAghanim, N.
dc.contributor.authorBattaner López, Eduardo 
dc.contributor.authorPlanck Collaboration
dc.identifier.citationAghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., ... & Battye, R. (2016). Planck 2015 results-XXII. A map of the thermal Sunyaev-Zeldovich effect. Astronomy & Astrophysics, 594, A22. []es_ES
dc.descriptionThe 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, MINECO, J.A., and RES (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); ERC and PRACE (EU). 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
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.es_ES
dc.description.sponsorshipCentre National D'etudes Spatialeses_ES
dc.description.sponsorshipCNRS/INSU-IN2P3-INP (France)es_ES
dc.description.sponsorshipEuropean Space Agencyes_ES
dc.description.sponsorshipItalian Space Agency (ASI)es_ES
dc.description.sponsorshipItalian National Research Counciles_ES
dc.description.sponsorshipIstituto Nazionale Astrofisica (INAF)es_ES
dc.description.sponsorshipNational Aeronautics & Space Administration (NASA)es_ES
dc.description.sponsorshipUnited States Department of Energy (DOE)es_ES
dc.description.sponsorshipUKSA (UK)es_ES
dc.description.sponsorshipConsejo Superior de Investigaciones Cientificas (CSIC)es_ES
dc.description.sponsorshipMINECO (Spain)es_ES
dc.description.sponsorshipRES (Spain)es_ES
dc.description.sponsorshipFinnish Funding Agency for Technology & Innovation (TEKES)es_ES
dc.description.sponsorshipAoF (Finland)es_ES
dc.description.sponsorshipCSC (Finland)es_ES
dc.description.sponsorshipHelmholtz Associationes_ES
dc.description.sponsorshipGerman Aerospace Centre (DLR)es_ES
dc.description.sponsorshipMax Planck Societyes_ES
dc.description.sponsorshipCSA (Canada)es_ES
dc.description.sponsorshipDTU Space (Denmark)es_ES
dc.description.sponsorshipSER/SSO (Switzerland)es_ES
dc.description.sponsorshipRCN (Norway)es_ES
dc.description.sponsorshipScience Foundation Irelandes_ES
dc.description.sponsorshipPortuguese Foundation for Science and Technologyes_ES
dc.description.sponsorshipERC (EU)es_ES
dc.description.sponsorshipEuropean Union (EU)es_ES
dc.description.sponsorshipJ.A. (Spain)es_ES
dc.description.sponsorshipScience & Technology Facilities Council (STFC) ST/L000768/1es_ES
dc.publisherEDP Scienceses_ES
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 España*
dc.subjectLarge-scale structure of Universees_ES
dc.subjectCosmology: observationses_ES
dc.titlePlanck 2015 results XXII. A map of the thermal Sunyaev-Zeldovich effectes_ES

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Atribución-NoComercial-SinDerivadas 3.0 España
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