Literature DB >> 25815919

Joint analysis of BICEP2/keck array and Planck Data.

P A R Ade1, N Aghanim2, Z Ahmed3, R W Aikin4, K D Alexander5, M Arnaud6, J Aumont2, C Baccigalupi7, A J Banday8,9, D Barkats10, R B Barreiro11, J G Bartlett12,13, N Bartolo14,15, E Battaner16,17, K Benabed18,19, A Benoît20, A Benoit-Lévy18,19,21, S J Benton22, J-P Bernard8,9, M Bersanelli23,24, P Bielewicz7,8,9, C A Bischoff5, J J Bock4,13, A Bonaldi25, L Bonavera11, J R Bond26, J Borrill27,28, F R Bouchet18,29, F Boulanger2, J A Brevik4, M Bucher12, I Buder5, E Bullock30, C Burigana31,32,33, R C Butler31, V Buza5, E Calabrese34, J-F Cardoso12,18,35, A Catalano36,37, A Challinor38,39,40, R-R Chary41, H C Chiang42,43, P R Christensen44,45, L P L Colombo13,46, C Combet36, J Connors5, F Couchot47, A Coulais37, B P Crill4,13, A Curto11,48, F Cuttaia31, L Danese7, R D Davies25, R J Davis25, P de Bernardis49, A de Rosa31, G de Zotti7,50, J Delabrouille12, J-M Delouis18,19, F-X Désert51, C Dickinson25, J M Diego11, H Dole2,52, S Donzelli24, O Doré4,13, M Douspis2, C D Dowell13, L Duband53, A Ducout18,54, J Dunkley34, X Dupac55, C Dvorkin5, G Efstathiou38, F Elsner18,19,21, T A Enßlin56, H K Eriksen57, E Falgarone37, J P Filippini4,58, F Finelli31,33, S Fliescher59, O Forni8,9, M Frailis60, A A Fraisse42, E Franceschi31, A Frejsel44, S Galeotta60, S Galli18, K Ganga12, T Ghosh2, M Giard8,9, E Gjerløw57, S R Golwala4, J González-Nuevo7,11, K M Górski13,61, S Gratton38,39, A Gregorio60,62,63, A Gruppuso31, J E Gudmundsson42, M Halpern64, F K Hansen57, D Hanson13,26,65, D L Harrison38,39, M Hasselfield64, G Helou4, S Henrot-Versillé47, D Herranz11, S R Hildebrandt4,13, G C Hilton66, E Hivon18,19, M Hobson48, W A Holmes13, W Hovest56, V V Hristov4, K M Huffenberger67, H Hui4, G Hurier2, K D Irwin3,66,68, A H Jaffe54, T R Jaffe8,9, J Jewell13, W C Jones42, M Juvela69, A Karakci12, K S Karkare5, J P Kaufman70, B G Keating70, S Kefeli4, E Keihänen69, S A Kernasovskiy3, R Keskitalo27, T S Kisner71, R Kneissl72,73, J Knoche56, L Knox74, J M Kovac5, N Krachmalnicoff23, M Kunz2,75,76, C L Kuo3,68, H Kurki-Suonio69,77, G Lagache2,78, A Lähteenmäki77,79, J-M Lamarre37, A Lasenby39,48, M Lattanzi32, C R Lawrence13, E M Leitch80, R Leonardi55, F Levrier37, A Lewis81, M Liguori14,15, P B Lilje57, M Linden-Vørnle82, M López-Caniego11,55, P M Lubin83, M Lueker4, J F Macías-Pérez36, B Maffei25, D Maino23,24, N Mandolesi31,32, A Mangilli2,47, M Maris60, P G Martin26, E Martínez-González11, S Masi49, P Mason4, S Matarrese14,15,84, K G Megerian13, P R Meinhold83, A Melchiorri49,85, L Mendes55, A Mennella23,24, M Migliaccio38,39, S Mitra13,86, M-A Miville-Deschênes2,26, A Moneti18, L Montier8,9, G Morgante31, D Mortlock54, A Moss87, D Munshi1, J A Murphy88, P Naselsky44,45, F Nati42, P Natoli31,32,89, C B Netterfield90, H T Nguyen13, H U Nørgaard-Nielsen82, F Noviello25, D Novikov91, I Novikov44,91, R O'Brient13, R W Ogburn3,68, A Orlando70, L Pagano49,85, F Pajot2, R Paladini41, D Paoletti31,33, B Partridge92, F Pasian60, G Patanchon12, T J Pearson4,41, O Perdereau47, L Perotto36, V Pettorino93, F Piacentini49, M Piat12, D Pietrobon13, S Plaszczynski47, E Pointecouteau8,9, G Polenta89,94, N Ponthieu2,51, G W Pratt6, S Prunet18,19, C Pryke30,59, J-L Puget2, J P Rachen56,95, W T Reach96, R Rebolo97,98,99, M Reinecke56, M Remazeilles2,12,25, C Renault36, A Renzi100,101, S Richter5, I Ristorcelli8,9, G Rocha4,13, M Rossetti23,24, G Roudier12,13,37, M Rowan-Robinson54, J A Rubiño-Martín97,99, B Rusholme41, M Sandri31, D Santos36, M Savelainen69,77, G Savini102, R Schwarz59, D Scott64, M D Seiffert4,13, C D Sheehy59,103, L D Spencer1, Z K Staniszewski4,13, V Stolyarov39,48,104, R Sudiwala1, R Sunyaev56,105, D Sutton38,39, A-S Suur-Uski69,77, J-F Sygnet18, J A Tauber106, G P Teply4, L Terenzi31,107, K L Thompson3, L Toffolatti11,31,108, J E Tolan3, M Tomasi23,24, M Tristram47, M Tucci75, A D Turner13,80, L Valenziano31, J Valiviita69,77, B Van Tent109, L Vibert2, P Vielva11, A G Vieregg103,110, F Villa31, L A Wade13, B D Wandelt18,19,58, R Watson25, A C Weber13, I K Wehus13, M White111, S D M White56, J Willmert59, C L Wong5, K W Yoon3,68, D Yvon112, A Zacchei60, A Zonca83.   

Abstract

We report the results of a joint analysis of data from BICEP2/Keck Array and Planck. BICEP2 and Keck Array have observed the same approximately 400  deg^{2} patch of sky centered on RA 0 h, Dec. -57.5°. The combined maps reach a depth of 57 nK deg in Stokes Q and U in a band centered at 150 GHz. Planck has observed the full sky in polarization at seven frequencies from 30 to 353 GHz, but much less deeply in any given region (1.2  μK deg in Q and U at 143 GHz). We detect 150×353 cross-correlation in B modes at high significance. We fit the single- and cross-frequency power spectra at frequencies ≥150  GHz to a lensed-ΛCDM model that includes dust and a possible contribution from inflationary gravitational waves (as parametrized by the tensor-to-scalar ratio r), using a prior on the frequency spectral behavior of polarized dust emission from previous Planck analysis of other regions of the sky. We find strong evidence for dust and no statistically significant evidence for tensor modes. We probe various model variations and extensions, including adding a synchrotron component in combination with lower frequency data, and find that these make little difference to the r constraint. Finally, we present an alternative analysis which is similar to a map-based cleaning of the dust contribution, and show that this gives similar constraints. The final result is expressed as a likelihood curve for r, and yields an upper limit r_{0.05}<0.12 at 95% confidence. Marginalizing over dust and r, lensing B modes are detected at 7.0σ significance.

Entities:  

Year:  2015        PMID: 25815919     DOI: 10.1103/PhysRevLett.114.101301

Source DB:  PubMed          Journal:  Phys Rev Lett        ISSN: 0031-9007            Impact factor:   9.161


  9 in total

1.  Reproducibility: Don't cry wolf.

Authors:  Jan Conrad
Journal:  Nature       Date:  2015-07-02       Impact factor: 49.962

2.  Inner Workings: Probing cosmic mysteries in a remote desert.

Authors:  Amber Dance
Journal:  Proc Natl Acad Sci U S A       Date:  2015-07-14       Impact factor: 11.205

3.  Inner Workings: Search intensifies for primordial gravitational waves.

Authors:  Anil Ananthaswamy
Journal:  Proc Natl Acad Sci U S A       Date:  2019-05-14       Impact factor: 11.205

Review 4.  Cosmology and fundamental physics with the Euclid satellite.

Authors:  Luca Amendola; Stephen Appleby; Anastasios Avgoustidis; David Bacon; Tessa Baker; Marco Baldi; Nicola Bartolo; Alain Blanchard; Camille Bonvin; Stefano Borgani; Enzo Branchini; Clare Burrage; Stefano Camera; Carmelita Carbone; Luciano Casarini; Mark Cropper; Claudia de Rham; Jörg P Dietrich; Cinzia Di Porto; Ruth Durrer; Anne Ealet; Pedro G Ferreira; Fabio Finelli; Juan García-Bellido; Tommaso Giannantonio; Luigi Guzzo; Alan Heavens; Lavinia Heisenberg; Catherine Heymans; Henk Hoekstra; Lukas Hollenstein; Rory Holmes; Zhiqi Hwang; Knud Jahnke; Thomas D Kitching; Tomi Koivisto; Martin Kunz; Giuseppe La Vacca; Eric Linder; Marisa March; Valerio Marra; Carlos Martins; Elisabetta Majerotto; Dida Markovic; David Marsh; Federico Marulli; Richard Massey; Yannick Mellier; Francesco Montanari; David F Mota; Nelson J Nunes; Will Percival; Valeria Pettorino; Cristiano Porciani; Claudia Quercellini; Justin Read; Massimiliano Rinaldi; Domenico Sapone; Ignacy Sawicki; Roberto Scaramella; Constantinos Skordis; Fergus Simpson; Andy Taylor; Shaun Thomas; Roberto Trotta; Licia Verde; Filippo Vernizzi; Adrian Vollmer; Yun Wang; Jochen Weller; Tom Zlosnik
Journal:  Living Rev Relativ       Date:  2018-04-12       Impact factor: 40.429

Review 5.  Detection methods for stochastic gravitational-wave backgrounds: a unified treatment.

Authors:  Joseph D Romano; Neil J Cornish
Journal:  Living Rev Relativ       Date:  2017-04-04       Impact factor: 40.429

6.  Small field models with gravitational wave signature supported by CMB data.

Authors:  Ira Wolfson; Ramy Brustein
Journal:  PLoS One       Date:  2018-05-24       Impact factor: 3.240

7.  Likelihood analysis of small field polynomial models of inflation yielding a high Tensor-to-Scalar ratio.

Authors:  Ira Wolfson; Ramy Brustein
Journal:  PLoS One       Date:  2019-04-24       Impact factor: 3.240

8.  Record electron self-cooling in cold-electron bolometers with a hybrid superconductor-ferromagnetic nanoabsorber and traps.

Authors:  A V Gordeeva; A L Pankratov; N G Pugach; A S Vasenko; V O Zbrozhek; A V Blagodatkin; D A Pimanov; L S Kuzmin
Journal:  Sci Rep       Date:  2020-12-15       Impact factor: 4.379

9.  L2-CalSat: A Calibration Satellite for Ultra-Sensitive CMB Polarization Space Missions.

Authors:  Francisco J Casas; Enrique Martínez-González; Juan Bermejo-Ballesteros; Sergio García; Javier Cubas; Patricio Vielva; Rita B Barreiro; Angel Sanz
Journal:  Sensors (Basel)       Date:  2021-05-12       Impact factor: 3.576

  9 in total

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