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@article{Ade:2016:0004-6361/201525830,
author = {Ade, PAR and Aghanim, N and Arnaud, M and Ashdown, M and Aumont, J and Baccigalupi, C and Banday, AJ and Barreiro, RB and Bartlett, JG and Bartolo, N and Battaner, E and Battye, R and Benabed, K and Benoît, A and Benoit-Lévy, A and Bernard, J-P and Bersanelli, M and Bielewicz, P and Bock, JJ and Bonaldi, A and Bonavera, L and Bond, JR and Borrill, J and Bouchet, FR and Boulanger, F and Bucher, M and Burigana, C and Butler, RC and Calabrese, E and Cardoso, J-F and Catalano, A and Challinor, A and Chamballu, A and Chary, R-R and Chiang, HC and Chluba, J and Christensen, PR and Church, S and Clements, DL and Colombi, S and Colombo, LPL and Combet, C and Coulais, A and Crill, BP and Curto, A and Cuttaia, F and Danese, L and Davies, RD and Davis, RJ and de, Bernardis P and de, Rosa A and de, Zotti G and Delabrouille, J and Désert, F-X and Di, Valentino E and Dickinson, C and Diego, JM and Dolag, K and Dole, H and Donzelli, S and Doré, O and Douspis, M and Ducout, A and Dunkley, J and Dupac,},
doi = {0004-6361/201525830},
journal = {Astronomy & Astrophysics},
title = {Planck 2015 results. XIII. Cosmological parameters},
url = {http://dx.doi.org/10.1051/0004-6361/201525830},
volume = {594},
year = {2016}
}

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TY  - JOUR
AB  - 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% upper limits on other parameters. We present the first results of polarization measurements with the Low Frequency Instrument at large angular scales. Combined with the Planck temperature and lensing data, these measurements give a reionization optical depth of τ = 0.066 ± 0.016, corresponding to a reionization redshift of . These results are consistent with those from WMAP polarization measurements cleaned for dust emission using 353-GHz polarization maps from the High Frequency Instrument. We find no evidence for any departure from base ΛCDM in the neutrino sector of the theory; for example, combining Planck observations with other astrophysical data we find Neff = 3.15 ± 0.23 for the effective number of relativistic degrees of freedom, consistent with the value Neff = 3.046 of the Standard Model of particle physics. The sum of neutrino masses is constrained to ∑ mν < 0.23 eV. The spatial curvature of our Universe is found to be very close to zero, with | ΩK | < 0.005. Adding
AU  - Ade,PAR
AU  - Aghanim,N
AU  - Arnaud,M
AU  - Ashdown,M
AU  - Aumont,J
AU  - Baccigalupi,C
AU  - Banday,AJ
AU  - Barreiro,RB
AU  - Bartlett,JG
AU  - Bartolo,N
AU  - Battaner,E
AU  - Battye,R
AU  - Benabed,K
AU  - Benoît,A
AU  - Benoit-Lévy,A
AU  - Bernard,J-P
AU  - Bersanelli,M
AU  - Bielewicz,P
AU  - Bock,JJ
AU  - Bonaldi,A
AU  - Bonavera,L
AU  - Bond,JR
AU  - Borrill,J
AU  - Bouchet,FR
AU  - Boulanger,F
AU  - Bucher,M
AU  - Burigana,C
AU  - Butler,RC
AU  - Calabrese,E
AU  - Cardoso,J-F
AU  - Catalano,A
AU  - Challinor,A
AU  - Chamballu,A
AU  - Chary,R-R
AU  - Chiang,HC
AU  - Chluba,J
AU  - Christensen,PR
AU  - Church,S
AU  - Clements,DL
AU  - Colombi,S
AU  - Colombo,LPL
AU  - Combet,C
AU  - Coulais,A
AU  - Crill,BP
AU  - Curto,A
AU  - Cuttaia,F
AU  - Danese,L
AU  - Davies,RD
AU  - Davis,RJ
AU  - de,Bernardis P
AU  - de,Rosa A
AU  - de,Zotti G
AU  - Delabrouille,J
AU  - Désert,F-X
AU  - Di,Valentino E
AU  - Dickinson,C
AU  - Diego,JM
AU  - Dolag,K
AU  - Dole,H
AU  - Donzelli,S
AU  - Doré,O
AU  - Douspis,M
AU  - Ducout,A
AU  - Dunkley,J
AU  - Dupac,X
AU  - Efstathiou,G
AU  - Elsner,F
AU  - Enßlin,TA
AU  - Eriksen,HK
AU  - Farhang,M
AU  - Fergusson,J
AU  - Finelli,F
AU  - Forni,O
AU  - Frailis,M
AU  - Fraisse,AA
AU  - Franceschi,E
AU  - Frejsel,A
AU  - Galeotta,S
AU  - Galli,S
AU  - Ganga,K
AU  - Gauthier,C
AU  - Gerbino,M
AU  - Ghosh,T
AU  - Giard,M
AU  - Giraud-Héraud,Y
AU  - Giusarma,E
AU  - Gjerløw,E
AU  - González-Nuevo,J
AU  - Górski,KM
AU  - Gratton,S
AU  - Gregorio,A
AU  - Gruppuso,A
AU  - Gudmundsson,JE
AU  - Hamann,J
AU  - Hansen,FK
AU  - Hanson,D
AU  - Harrison,DL
AU  - Helou,G
AU  - Henrot-Versillé,S
AU  - Hernández-Monteagudo,C
AU  - Herranz,D
AU  - Hildebrandt,SR
AU  - Hivon,E
AU  - Hobson,M
AU  - Holmes,WA
AU  - Hornstrup,A
AU  - Hovest,W
AU  - Huang,Z
AU  - Huffenberger,KM
AU  - Hurier,G
AU  - Jaffe,AH
AU  - Jaffe,TR
AU  - Jones,WC
AU  - Juvela,M
AU  - Keihänen,E
AU  - Keskitalo,R
AU  - Kisner,TS
AU  - Kneissl,R
AU  - Knoche,J
AU  - Knox,L
AU  - Kunz,M
AU  - Kurki-Suonio,H
AU  - Lagache,G
AU  - Lähteenmäki,A
AU  - Lamarre,J-M
AU  - Lasenby,A
AU  - Lattanzi,M
AU  - Lawrence,CR
AU  - Leahy,JP
AU  - Leonardi,R
AU  - Lesgourgues,J
AU  - Levrier,F
AU  - Lewis,A
AU  - Liguori,M
AU  - Lilje,PB
AU  - Linden-Vørnle,M
AU  - López-Caniego,M
AU  - Lubin,PM
AU  - Macías-Pérez,JF
AU  - Maggio,G
AU  - Maino,D
AU  - Mandolesi,N
AU  - Mangilli,A
AU  - Marchini,A
AU  - Maris,M
AU  - Martin,PG
AU  - Martinelli,M
AU  - Martínez-González,E
AU  - Masi,S
AU  - Matarrese,S
AU  - McGehee,P
AU  - Meinhold,PR
AU  - Melchiorri,A
AU  - Melin,J-B
AU  - Mendes,L
AU  - Mennella,A
AU  - Migliaccio,M
AU  - Millea,M
AU  - Mitra,S
AU  - Miville-Deschênes,M-A
AU  - Moneti,A
AU  - Montier,L
AU  - Morgante,G
AU  - Mortlock,D
AU  - Moss,A
AU  - Munshi,D
AU  - Murphy,JA
AU  - Naselsky,P
AU  - Nati,F
AU  - Natoli,P
AU  - Nette
DO  - 0004-6361/201525830
PY  - 2016///
SN  - 1432-0746
TI  - Planck 2015 results. XIII. Cosmological parameters
T2  - Astronomy & Astrophysics
UR  - http://dx.doi.org/10.1051/0004-6361/201525830
UR  - http://hdl.handle.net/10044/1/43993
VL  - 594
ER  -

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