Authors
Peter AR Ade, N Aghanim, M Arnaud, M Ashdown, J Aumont, C Baccigalupi, AJ Banday, RB Barreiro, JG Bartlett, N Bartolo, E Battaner, R Battye, K Benabed, A Benoît, A Benoit-Lévy, J-P Bernard, M Bersanelli, P Bielewicz, JJ Bock, A Bonaldi, L Bonavera, JR Bond, J Borrill, FR Bouchet, F Boulanger, M Bucher, C Burigana, RC Butler, E Calabrese, J-F Cardoso, A Catalano, A Challinor, A Chamballu, R-R Chary, HC Chiang, J Chluba, PR Christensen, S Church, DL Clements, S Colombi, LPL Colombo, C Combet, A Coulais, BP Crill, A Curto, F Cuttaia, L Danese, RD Davies, RJ Davis, P De Bernardis, A De Rosa, Giulia De Zotti, J Delabrouille, F-X Désert, E Di Valentino, C Dickinson, JM Diego, K Dolag, H Dole, Simona Donzelli, O Doré, M Douspis, A Ducout, Joanna Dunkley, X Dupac, G Efstathiou, F Elsner, TA Enßlin, HK Eriksen, M Farhang, J Fergusson, F Finelli, O Forni, M Frailis, AA Fraisse, E Franceschi, A Frejsel, S Galeotta
Publication date
2016/10/1
Journal
Astronomy & Astrophysics
Volume
594
Pages
A13
Publisher
EDP sciences
Description
This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. Our results are in very good agreement with the 2013 analysis of the Planck nominal-mission temperature data, but with increased precision. The temperature and polarization power spectra are consistent with the standard spatially-flat 6-parameter ΛCDM cosmology with a power-law spectrum of adiabatic scalar perturbations (denoted “base ΛCDM” in this paper). From the Planck temperature data combined with Planck lensing, for this cosmology we find a Hubble constant, H0 = (67.8 ± 0.9) km s-1Mpc-1, a matter density parameter Ωm = 0.308 ± 0.012, and a tilted scalar spectral index with ns = 0.968 ± 0.006, consistent with the 2013 analysis. Note that in this abstract we quote 68% confidence limits on measured parameters and 95 …
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PAR Ade, N Aghanim, M Arnaud, M Ashdown… - Astronomy & Astrophysics, 2016