Authors
PAR Ade, N Aghanim, M Arnaud, M Ashdown, J Aumont, C Baccigalupi, AJ Banday, RB Barreiro, JG Bartlett, N Bartolo, Suman Basak, E Battaner, 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, HC Chiang, PR Christensen, S Church, DL Clements, S Colombi, LPL Colombo, C Combet, F Couchot, 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, JM Diego, H Dole, S Donzelli, O Doré, M Douspis, A Ducout, J Dunkley, X Dupac, G Efstathiou, F Elsner, TA Enßlin, HK Eriksen, J Fergusson, F Finelli, O Forni, M Frailis, AA Fraisse, E Franceschi, A Frejsel, S Galeotta, S Galli, K Ganga, M Giard, Y Giraud-Héraud, E Gjerløw, J González-Nuevo, KM Górski, S Gratton, A Gregorio, A Gruppuso, Jón E Gudmundsson, FK Hansen, D Hanson, DL Harrison, S Henrot-Versillé, C Hernández-Monteagudo, D Herranz, SR Hildebrandt, E Hivon, M Hobson, WA Holmes, Allan Hornstrup, W Hovest, KM Huffenberger, G Hurier, AH Jaffe, TR Jaffe, WC Jones, M Juvela, E Keihänen, R Keskitalo, TS Kisner, R Kneissl, J Knoche, M Kunz, H Kurki-Suonio, G Lagache, A Lähteenmäki, J-M Lamarre, A Lasenby, M Lattanzi, CR Lawrence, R Leonardi, J Lesgourgues, F Levrier, A Lewis, M Liguori, PB Lilje, Michael Linden-Vørnle, M López-Caniego, PM Lubin, JF Macías-Pérez, G Maggio, D Maino, N Mandolesi, A Mangilli, M Maris, PG Martin, E Martínez-González, S Masi, S Matarrese, P McGehee, PR Meinhold, A Melchiorri, L Mendes, A Mennella, M Migliaccio, Susanta Mitra, M-A Miville-Deschênes, A Moneti, L Montier, G Morgante, D Mortlock, Adam Moss, D Munshi, JA Murphy, P Naselsky
Publication date
2016/10/1
Journal
Astronomy & Astrophysics
Volume
594
Pages
A15
Publisher
EDP Sciences
Description
We present the most significant measurement of the cosmic microwave background (CMB) lensing potential to date (at a level of 40σ), using temperature and polarization data from the Planck 2015 full-mission release. Using a polarization-only estimator, we detect lensing at a significance of 5σ. We cross-check the accuracy of our measurement using the wide frequency coverage and complementarity of the temperature and polarization measurements. Public products based on this measurement include an estimate of the lensing potential over approximately 70% of the sky, an estimate of the lensing potential power spectrum in bandpowers for the multipole range 40≤ L≤ 400, and an associated likelihood for cosmological parameter constraints. We find good agreement between our measurement of the lensing potential power spectrum and that found in the ΛCDM model that best fits the Planck temperature and polarization power spectra. Using the lensing likelihood alone we obtain a percent-level measurement of the parameter combination σ 8 ω 0.25 m= 0: 591±0: 021. We combine our determination of the lensing potential with the E-mode polarization, also measured by Planck, to generate an estimate of the lensing B-mode. We show that this lensing B-mode estimate is correlated with the B-modes observed directly by Planck at the expected level and with a statistical significance of 10σ, confirming Planck's sensitivity to this known sky signal. We also correlate our lensing potential estimate with the large-scale temperature anisotropies, detecting a cross-correlation at the 3σ level, as expected because of dark energy in the concordance …
Total citations
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Scholar articles
PAR Ade, N Aghanim, M Arnaud, F Arroja, M Ashdown… - Astronomy & Astrophysics, 2016
Planck Collaboration - Astronomy and Astrophysics, 2016
PAR Ade, N Aghanim, M Arnaud, M Ashdown… - Astronomy & Astrophysics, 2016
P Collaboration, PAR Ade, N Aghanim, M Arnaud… - Astron. Astrophys, 2016
JG Bartlett, M Bucher, JF Cardoso, J Delabrouille… - Astronomy and Astrophysics, 2016
PAR Ade, N Aghanim, M Arnaud, M Ashdown… - Astronomy & Astrophysics/Astronomie et Astrophysique, 2016