Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes

Cosmology (including clusters of galaxies).-- et al.

Detalles Bibliográficos
Autores: Aumont, Jonathan, Barreiro, R. Belén, Bonavera, Laura, Curto, Andrés, Diego, José María, González-Nuevo, J., Herranz, Diego, López-Caniego, M., Martínez-González, Enrique, Toffolatti, Luigi, Vielva, Patricio, Rebolo López, Rafael, Planck Collaboration
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2016
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/140626
Acceso en línea:http://hdl.handle.net/10261/140626
Access Level:acceso abierto
Palabra clave:Cosmic background radiation
Cosmology: observations
ISM: structure
ISM: magnetic fields
Polarization
id ES_bb7b11bfc624f0a7d40b4e963520e9a7
oai_identifier_str oai:digital.csic.es:10261/140626
network_acronym_str ES
network_name_str España
repository_id_str
dc.title.none.fl_str_mv Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes
title Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes
spellingShingle Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes
Aumont, Jonathan
Cosmic background radiation
Cosmology: observations
ISM: structure
ISM: magnetic fields
Polarization
title_short Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes
title_full Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes
title_fullStr Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes
title_full_unstemmed Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes
title_sort Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes
dc.creator.none.fl_str_mv Aumont, Jonathan
Barreiro, R. Belén
Bonavera, Laura
Curto, Andrés
Diego, José María
González-Nuevo, J.
Herranz, Diego
López-Caniego, M.
Martínez-González, Enrique
Toffolatti, Luigi
Vielva, Patricio
Rebolo López, Rafael
Planck Collaboration
author Aumont, Jonathan
author_facet Aumont, Jonathan
Barreiro, R. Belén
Bonavera, Laura
Curto, Andrés
Diego, José María
González-Nuevo, J.
Herranz, Diego
López-Caniego, M.
Martínez-González, Enrique
Toffolatti, Luigi
Vielva, Patricio
Rebolo López, Rafael
Planck Collaboration
author_role author
author2 Barreiro, R. Belén
Bonavera, Laura
Curto, Andrés
Diego, José María
González-Nuevo, J.
Herranz, Diego
López-Caniego, M.
Martínez-González, Enrique
Toffolatti, Luigi
Vielva, Patricio
Rebolo López, Rafael
Planck Collaboration
author2_role author
author
author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Science and Technology Facilities Council (UK)
NASA
Istituto Nazionale di Astrofisica
Centre National de la Recherche Scientifique (France)
European Space Agency
Junta de Andalucía
Consejo Superior de Investigaciones Científicas (España)
Ministerio de Economía y Competitividad (España)
European Commission
European Research Council
Academy of Finland
Center for Science (Finland)
Agenzia Spaziale Italiana
Department of Energy (US)
UK Space Agency
Fundação para a Ciência e a Tecnologia (Portugal)
Science Foundation Ireland
German Centre for Air and Space Travel
DTU Space (Denmark)
Swiss Space Office
Max Planck Society
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Cosmic background radiation
Cosmology: observations
ISM: structure
ISM: magnetic fields
Polarization
topic Cosmic background radiation
Cosmology: observations
ISM: structure
ISM: magnetic fields
Polarization
description Cosmology (including clusters of galaxies).-- et al.
publishDate 2016
dc.date.none.fl_str_mv 2016
2016
2016
2016
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/10261/140626
url http://hdl.handle.net/10261/140626
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv #PLACEHOLDER_PARENT_METADATA_VALUE#
info:eu-repo/grantAgreement/EC/FP7/267934
http://dx.doi.org/10.1051/0004-6361/201425034
Sí
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
repository.name.fl_str_mv
repository.mail.fl_str_mv
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spelling Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudesAumont, JonathanBarreiro, R. BelénBonavera, LauraCurto, AndrésDiego, José MaríaGonzález-Nuevo, J.Herranz, DiegoLópez-Caniego, M.Martínez-González, EnriqueToffolatti, LuigiVielva, PatricioRebolo López, RafaelPlanck CollaborationCosmic background radiationCosmology: observationsISM: structureISM: magnetic fieldsPolarizationCosmology (including clusters of galaxies).-- et al.The polarized thermal emission from diffuse Galactic dust is the main foreground present in measurements of the polarization of the cosmic microwave background (CMB) at frequencies above 100 GHz. In this paper we exploit the uniqueness of the Planck HFI polarization data from 100 to 353 GHz to measure the polarized dust angular power spectra CℓEE and CℓBB over the multipole range 40 <ℓ< 600 well away from the Galactic plane. These measurements will bring new insights into interstellar dust physics and allow a precise determination of the level of contamination for CMB polarization experiments. Despite the non-Gaussian and anisotropic nature of Galactic dust, we show that general statistical properties of the emission can be characterized accurately over large fractions of the sky using angular power spectra. The polarization power spectra of the dust are well described by power laws in multipole, Cℓ ∝ ℓα, with exponents αEE,BB = −2.42 ± 0.02. The amplitudes of the polarization power spectra vary with the average brightness in a way similar to the intensity power spectra. The frequency dependence of the dust polarization spectra is consistent with modified blackbody emission with βd = 1.59 and Td = 19.6 K down to the lowest Planck HFI frequencies. We find a systematic difference between the amplitudes of the Galactic B- and E-modes, CℓBB/CℓEE = 0.5. We verify that these general properties are preserved towards high Galactic latitudes with low dust column densities. We show that even in the faintest dust-emitting regions there are no “clean” windows in the sky where primordial CMB B-mode polarization measurements could be made without subtraction of foreground emission. Finally, we investigate the level of dust polarization in the specific field recently targeted by the BICEP2 experiment. Extrapolation of the Planck 353 GHz data to 150 GHz gives a dust power ℓBB ≡ ℓ(ℓ+1)CℓBB/(2π) of 1.32 × 10-2 μKCMB2 over the multipole range of the primordial recombination bump (40 <ℓ< 120); the statistical uncertainty is ± 0.29 × 10-2 μKCMB2 and there is an additional uncertainty (+0.28, −0.24) × 10-2 μKCMB2 from the extrapolation. This level is the same magnitude as reported by BICEP2 over this ℓ range, which highlights the need for assessment of the polarized dust signal even in the cleanest windows of the sky.The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, 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); and PRACE (EU).The research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Programme (FP7/2007-2013) / ERC grant agreement No. 267934.Peer ReviewedEDP SciencesScience and Technology Facilities Council (UK)NASAIstituto Nazionale di AstrofisicaCentre National de la Recherche Scientifique (France)European Space AgencyJunta de AndalucíaConsejo Superior de Investigaciones Científicas (España)Ministerio de Economía y Competitividad (España)European CommissionEuropean Research CouncilAcademy of FinlandCenter for Science (Finland)Agenzia Spaziale ItalianaDepartment of Energy (US)UK Space AgencyFundação para a Ciência e a Tecnologia (Portugal)Science Foundation IrelandGerman Centre for Air and Space TravelDTU Space (Denmark)Swiss Space OfficeMax Planck SocietyConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2016201620162016info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/140626reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/EC/FP7/267934http://dx.doi.org/10.1051/0004-6361/201425034Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/1406262026-05-22T06:33:51Z
score 15.811543

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