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Planck 2015 results I. Overview of products and scientific results




TekijätAdam R, Ade PAR, Aghanim N, Akrami Y, Alves MIR, Argueso F, Arnaud M, Arroja F, Ashdown M, Aumont J, Baccigalupi C, Ballardini M, Banday AJ, Barreiro RB, Bartlett JG, Bartolo N, Basak S, Battaglia P, Battaner E, Battye R, Benabed K, Benoit A, Benoit-Levy A, Bernard JP, Bersanelli M, Bertincourt B, Bielewicz P, Bikmaev I, Bock JJ, Bohringer H, Bonaldi A, Bonavera L, Bond JR, Borrill J, Bouchet FR, Boulanger F, Bucher M, Burenin R, Burigana C, Butler RC, Calabrese E, Cardoso JF, Carvalho P, Casaponsa B, Castex G, Catalano A, Challinor A, Chamballu A, Chary RR, Chiang HC, Chluba J, Chon G, Christensen PR, Church S, Clemens M, Clements DL, Colombi S, Colombo LPL, Combet C, Comis B, Contreras D, Couchot F, Coulais A, Crill BP, Cruz M, Curto A, Cuttaia F, Danese L, Davies RD, Davis RJ, de Bernardis P, de Rosa A, de Zotti G, Delabrouille J, Delouis JM, Desert FX, Di Valentino E, Dickinson C, Diego JM, Dolag K, Dole H, Donzelli S, Dore O, Douspis M, Ducout A, Dunkley J, Dupac X, Efstathiou G, Eisenhardt PRM, Elsner F, Ensslin TA, Eriksen HK, Falgarone E, Fantaye Y, Farhang M, Feeney S, Fergusson J, Fernandez-Cobos R, Feroz F, Finelli F, Florido E, Forni O, Frailis M, Fraisse AA, Franceschet C, Franceschi E, Frejsel A, Frolov A, Galeotta S, Galli S, Ganga K, Gauthier C, Genova-Santos RT, Gerbino M, Ghosh T, Giard M, Giraud-Heraud Y, Giusarma E, Gjerlow E, Gonzalez-Nuevo J, Gorski KM, Grainge KJB, Gratton S, Gregorio A, Gruppuso A, Gudmundsson JE, Hamann J, Handley W, Hansen FK, Hanson D, Harrison DL, Heavens A, Helou G, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huang Z, Huffenberger KM, Hurier G, Ilic S, Jaffe AH, Jaffe TR, Jin T, Jones WC, Juvela M, Karakci A, Keihanen E, Keskitalo R, Khamitov I, Kiiveri K, Kim J, Kisner TS, Kneissl R, Knoche J, Knox L, Krachmalnicoff N, Kunz M, Kurki-Suonio H, Lacasa F, Lagache G, Lahteenmaki A, Lamarre JM, Langer M, Lasenby A, Lattanzi M, Lawrence CR, Jeune M, Leahy JP, Lellouch E, Leonardi R, Leon-Tavares J, Lesgourgues J, Levrier F, Lewis A, Liguori M, Lilje PB, Lilley M, Linden-Vornle M, Lindholm V, Liu H, Lopez-Caniego M, Lubin PM, Ma YZ, Macias-Perez JF, Maggio G, Maino D, Mak DSY, Mandolesi N, Mangilli A, Marchini A, Marcos-Caballero A, Marinucci D, Maris M, Marshall DJ, Martin PG, Martinelli M, Martinez-Gonzalez E, Masi S, Matarrese S, Mazzotta P, McEwen JD, McGehee P, Mei S, Meinhold PR, Melchiorri A, Melin JB, Mendes L, Mennella A, Migliaccio M, Mikkelsen K, Millea M, Mitra S, Miville-Deschenes MA, Molinari D, Moneti A, Montier L, Moreno R, Morgante G, Mortlock D, Moss A, Mottet S, Munchmeyer M, Munshi D, Murphy JA, Narimani A, Naselsky P, Nastasi A, Nati F, Natoli P, Negrello M, Netterfield CB, Norgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Olamaie M, Oppermann N, Orlando E, Oxborrow CA, Paci F, Pagano L, Pajot F, Paladini R, Pandolfi S, Paoletti D, Partridge B, Pasian F, Patanchon G, Pearson TJ, Peel M, Peiris HV, Pelkonen VM, Perdereau O, Perotto L, Perrott YC, Perrotta F, Pettorino V, Piacentini F, Piat M, Pierpaoli E, Pietrobon D, Plaszczynski S, Pogosyan D, Pointecouteau E, Polenta G, Popa L, Pratt GW, Prezeau G, Prunet S, Puget JL, Rachen JP, Racine B, Reach WT, Rebolo R, Reinecke M, Remazeilles M, Renault C, Renzi A, Ristorcelli I, Rocha G, Roman M, Romelli E, Rosset C, Rossetti M, Rotti A, Roudier G, d'Orfeuil BR, Rowan-Robinson M, Rubino-Martin JA, Ruiz-Granados B, Rumsey C, Rusholme B, Said N, Salvatelli V, Salvati L, Sandri M, Sanghera HS, Santos D, Saunders RDE, Sauve A, Savelainen M, Savini G, Schaefer BM, Schammel MP, Scott D, Seiffert MD, Serra P, Shellard EPS, Shimwell TW, Shiraishi M, Smith K, Souradeep T, Spencer LD, Spinelli M, Stanford SA, Stern D, Stolyarov V, Stompor R, Strong AW, Sudiwala R, Sunyaev R, Sutter P, Sutton D, Suur-Uski AS, Sygnet JF, Tauber JA, Tavagnacco D, Terenzi L, Texier D, Toffolatti L, Tomasi M, Tornikoski M, Tramonte D, Tristram M, Troja A, Trombetti T, Tucci M, Tuovinen J, Turler M, Umana G, Valenziano L, Valiviita J, Van Tent F, Vassallo T, Vibert L, Vidal M, Viel M, Vielva P, Villa F, Wade LA, Walter B, Wandelt BD, Watson R, Wehus IK, Welikala N, Weller J, White M, White SDM, Wilkinson A, Yvon D, Zacchei A, Zibin JP, Zonca A, Zonca A, Zibin JP, White SDM, Wilkinson A, Yvon D, Zacchei A

KustantajaEDP SCIENCES S A

Julkaisuvuosi2016

Lehti: Astronomy and Astrophysics

Tietokannassa oleva lehden nimiASTRONOMY & ASTROPHYSICS

Lehden akronyymiASTRON ASTROPHYS

Artikkelin numeroARTN A1

Vuosikerta594

Sivujen määrä38

ISSN1432-0746

DOIhttps://doi.org/10.1051/0004-6361/201527101


Tiivistelmä
The European Space Agency's Planck satellite, which is dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013. In February 2015, ESA and the Planck Collaboration released the second set of cosmology products based on data from the entire Planck mission, including both temperature and polarization, along with a set of scientific and technical papers and a web-based explanatory supplement. This paper gives an overview of the main characteristics of the data and the data products in the release, as well as the associated cosmological and astrophysical science results and papers. The data products include maps of the cosmic microwave background (CMB), the thermal Sunyaev-Zeldovich effect, diffuse foregrounds in temperature and polarization, catalogues of compact Galactic and extragalactic sources (including separate catalogues of Sunyaev-Zeldovich clusters and Galactic cold clumps), and extensive simulations of signals and noise used in assessing uncertainties and the performance of the analysis methods. The likelihood code used to assess cosmological models against the Planck data is described, along with a CMB lensing likelihood. Scientific results include cosmological parameters derived from CMB power spectra, gravitational lensing, and cluster counts, as well as constraints on inflation, non-Gaussianity, primordial magnetic fields, dark energy, and modified gravity, and new results on low-frequency Galactic foregrounds.

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