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

Abstract: 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 C?EE and C?BB over the multipole range 40

Other publications of the same journal or congress with authors from the University of Cantabria

 Fuente: Astronomy & Astrophysics, 2016, 586, A133

Publisher: EDP Sciences

 Publication date: 01/02/2016

No. of pages: 25

Publication type: Article

 DOI: 10.1051/0004-6361/201425034

ISSN: 0004-6361,1432-0746

Publication Url: https://doi.org/10.1051/0004-6361/201425034

Authorship

LAURA BONAVERA

ANDRES CURTO MARTIN

JOAQUIN GONZALEZ-NUEVO GONZALEZ

ADAM, R.

MARCOS LOPEZ-CANIEGO ALCARRIA

LUIGI TOFFOLATTI