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Please use this identifier to cite or link to this item: http://hdl.handle.net/10651/42929

Title: Planck intermediate results: L. Evidence of spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB B-mode analysis
Author(s): Aghanim, N.
Ashdown, Mark
Aumont, J.
González-Nuevo González, Joaquín
Toffolatti, Luigi
Planck Collaboration
Issue date: 2017
Publisher version: http://dx.doi.org/10.1051/0004-6361/201629164
Citation: Astronomy & Astrophysics, 599, A51 (2017); doi:10.1051/0004-6361/201629164
Format extent: p. A51-
URI: http://hdl.handle.net/10651/42929
ISSN: 0004-6361
Sponsored: The 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, JA, 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). 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.
Project id.: info:eu-repo/grantAgreement/EC/FP7/267934
Appears in Collections:Física
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