<i>Planck</i>2013 results. XVI. Cosmological parameters

A. R. Ade, P.; Aghanim, N.; Armitage-Caplan, C.; Arnaud, M.; Ashdown, M.; Atrio‐Barandela, F.; Aumont, J.; Baccigalupi, C.; J. Banday, A.; B. Barreiro, R.; G. Bartlett, J.; Battaner, E.; Benabed, K.; Benoı̂t, A.; Benoit-Lévy, A.; P. Bernard, J.; Bersanelli, M.; Bielewicz, P.; Bobin, J.; J. Bock, J.; Bonaldi, A.; R. Bond, J.; Borrill, J.; R. Bouchet, F.; Bridges, M.; Bucher, M.; Burigana, C.; C. Butler, R.; Calabrese, E.; Cappellini, B.; Cardoso, J.-F.; Catalano, A.; Challinor, A.; Chamballu, A.; Chary, Ranga‐Ram; Chen, X.; C. Chiang, H.; Chiang, L.-Y; R. Christensen, P.; Church, S.; L. Clements, D.; Colombi, S.; P. L. Colombo, L.; Couchot, F.; Coulais, A.; P. Crill, B.; Curto, A.; Cuttaia, F.; Danese, L.; D. Davies, R.

doi:10.1051/0004-6361/201321591

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Planck2013 results. XVI. Cosmological parameters

Shared by NobleBlocks on Feb 25, 2014 • 12:00 AM UTC

Authors:

P. A. R. Ade

N. Aghanim

C. Armitage-Caplan

Abstract

This paper presents the first cosmological results based on Planck measurements of the cosmic microwave background (CMB) temperature and lensing-potential power spectra. We find that the Planck spectra at high multipoles ( > 40) are extremely well described by the standard spatiallyflat six-paramete...

Subject

Physics

Planck

Cosmic microwave background

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