<i>Planck</i>2015 results

Aghanim, N.; Arnaud, M.; Ashdown, M.; Aumont, J.; Baccigalupi, C.; J. Banday, A.; B. Barreiro, R.; G. Bartlett, J.; Bartolo, N.; Battaner, E.; Benabed, K.; Benoı̂t, A.; Benoit-Lévy, A.; Bernard, J.-P.; Bersanelli, M.; Bielewicz, P.; J. Bock, J.; Bonaldi, A.; Bonavera, L.; R. Bond, J.; Borrill, J.; R. Bouchet, F.; Boulanger, F.; Bucher, M.; Burigana, C.; C. Butler, R.; Calabrese, E.; Cardoso, J.-F.; Catalano, A.; Challinor, A.; C. Chiang, H.; R. Christensen, P.; L. Clements, D.; P. L. Colombo, L.; Combet, Céline; Coulais, A.; P. Crill, B.; Curto, A.; Cuttaia, F.; Danese, L.; D. Davies, R.; J. Davis, R.; de Bernardis, P.; de Rosa, A.; de Zotti, G.; de Zotti, G.; Désert, F.–X.; Di Valentino, Eleonora; L. Dickinson, C.; M. Diego, J.

doi:10.1051/0004-6361/201526926

Public

Planck2015 results

Published in Astronomy and Astrophysics • Jun 8, 2016

NobleIDark:/48914/w1/20260526/A5D8B506Record on NobleID

Authors:

N. Aghanim

,

M. Arnaud

,

M. Ashdown

Abstract

This paper presents the Planck 2015 likelihoods, statistical descriptions of the 2-point correlation functions of the cosmic microwave background (CMB) temperature and polarization fluctuations that account for relevant uncertainties, both instrumental and astrophysical in nature. They are based on ...

Subject

Physics

Planck

Astrophysics

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