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

Adam, R ; Ade, P A R ; Aghanim, N ; Arnaud, M ; Aumont, J ; Baccigalupi, C ; Banday, A J ; Barreiro, R B ; Bartlett, J G

Astronomy and astrophysics (Berlin), 2016-02, Vol.586, p.A133 [Periódico revisado por pares]

United States: EDP Sciences

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Título:
Planck intermediate results: XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes
Autor: Adam, R ; Ade, P A R ; Aghanim, N ; Arnaud, M ; Aumont, J ; Baccigalupi, C ; Banday, A J ; Barreiro, R B ; Bartlett, J G
Assuntos: Assessments ; ASTRONOMY AND ASTROPHYSICS ; Astrophysics ; cosmic background radiation ; Cosmic dust ; Cosmic microwave background ; Cosmology and Extra-Galactic Astrophysics ; cosmology observations ; Dust ; Emission ; ISM magnetic fields ; ISM structure ; Physics ; Polarization ; Power spectra ; Sky
É parte de: Astronomy and astrophysics (Berlin), 2016-02, Vol.586, p.A133
Notas: ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
AC02-05CH11231
USDOE Office of Science (SC)
Descrição: 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
Editor: United States: EDP Sciences
Idioma: Inglês

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