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We present a harmonic model for the data analysis of an all-sky cosmic microwave background survey, such as Planck, where the survey is obtained through ring-scans of the sky. In this model, resampling and pixelisation of the data are…

We combine observational data on a dozen independent cosmic properties at high-$z$ with the information on reionization drawn from the spectra of distant luminous sources and the cosmic microwave background (CMB) to constrain the…

We present constraints on primordial B modes from large angular scale cosmic microwave background polarisation anisotropies measured with the Planck satellite. To remove Galactic polarised foregrounds, we use a Bayesian parametric component…

宇宙学与河外天体物理 · 物理学 2022-11-30 Roger de Belsunce , Steven Gratton , George Efstathiou

Cosmic microwave background (CMB) anisotropy is our richest source of cosmological information; the standard cosmological model was largely established thanks to study of the temperature anisotropies. By the end of the decade, the Planck…

天体物理学 · 物理学 2009-11-11 James G. Bartlett

We derive a constraint on patchy screening of the cosmic microwave background from inhomogeneous reionization, using off-diagonal TB and TT correlations in WMAP-7 temperature/polarization data. We interpret this as a constraint on the rms…

宇宙学与河外天体物理 · 物理学 2013-10-08 Vera Gluscevic , Marc Kamionkowski , Duncan Hanson

We study the reionization history of the Universe in cosmological models with non-Gaussian density fluctuations, taking them to have a renormalized $\chi^2$ probability distribution function parametrized by the number of degrees of freedom,…

天体物理学 · 物理学 2009-11-11 Pedro P. Avelino , Andrew R. Liddle

We present a simple way of coding and compressing the data on board the Planck instruments (HFI and LFI) to address the problem of the on board data reduction. This is a critical issue in the Planck mission. The total information that can…

天体物理学 · 物理学 2009-10-31 E. Gaztanaga , A. Romeo , J. Barriga , E. Elizalde

It has been long recognised that, besides being a formidable experiment to observe the primordial CMB anisotropies, Planck will also have the capability to detect galaxy clusters via their SZ imprint. In this paper constraints on…

天体物理学 · 物理学 2009-11-11 Joern Geisbuesch , Michael Hobson

The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14~May 2009 and scanned the microwave and submillimetre sky continuously between 12~August 2009 and 23~October…

宇宙学与河外天体物理 · 物理学 2016-09-28 Planck Collaboration , R. Adam , P. A. R. Ade , N. Aghanim , Y. Akrami , M. I. R. Alves , M. Arnaud , F. Arroja , J. Aumont , C. Baccigalupi , M. Ballardini , A. J. Banday , R. B. Barreiro , J. G. Bartlett , N. Bartolo , S. Basak , P. Battaglia , E. Battaner , R. Battye , K. Benabed , A. Benoît , A. Benoit-Lévy , J. -P. Bernard , M. Bersanelli , B. Bertincourt , P. Bielewicz , A. Bonaldi , L. Bonavera , J. R. Bond , J. Borrill , F. R. Bouchet , F. Boulanger , M. Bucher , C. Burigana , R. C. Butler , E. Calabrese , J. -F. Cardoso , P. Carvalho , B. Casaponsa , G. Castex , A. Catalano , A. Challinor , A. Chamballu , R. -R. Chary , H. C. Chiang , J. Chluba , P. R. Christensen , S. Church , M. Clemens , D. L. Clements , S. Colombi , L. P. L. Colombo , C. Combet , B. Comis , D. Contreras , F. Couchot , A. Coulais , B. P. Crill , M. Cruz , A. Curto , F. Cuttaia , L. Danese , R. D. Davies , R. J. Davis , P. de Bernardis , A. de Rosa , G. de Zotti , J. Delabrouille , J. -M. Delouis , F. -X. Désert , E. Di Valentino , C. Dickinson , J. M. Diego , K. Dolag , H. Dole , S. Donzelli , O. Doré , M. Douspis , A. Ducout , J. Dunkley , X. Dupac , G. Efstathiou , P. R. M. Eisenhardt , F. Elsner , T. A. Enßlin , H. K. Eriksen , E. Falgarone , Y. Fantaye , M. Farhang , S. Feeney , J. Fergusson , R. Fernandez-Cobos , F. Feroz , F. Finelli , E. Florido , O. Forni , M. Frailis , A. A. Fraisse , C. Franceschet , E. Franceschi , A. Frejsel , A. Frolov , S. Galeotta , S. Galli , K. Ganga , C. Gauthier , R. T. Génova-Santos , M. Gerbino , T. Ghosh , M. Giard , Y. Giraud-Héraud , E. Giusarma , E. Gjerløw , J. González-Nuevo , K. M. Górski , K. J. B. Grainge , S. Gratton , A. Gregorio , A. Gruppuso , J. E. Gudmundsson , J. Hamann , W. Handley , F. K. Hansen , D. Hanson , D. L. Harrison , A. Heavens , G. Helou , S. Henrot-Versillé , C. Hernández-Monteagudo , D. Herranz , S. R. Hildebrandt , E. Hivon , M. Hobson , W. A. Holmes , A. Hornstrup , W. Hovest , Z. Huang , K. M. Huffenberger , G. Hurier , S. Ilić , A. H. Jaffe , T. R. Jaffe , T. Jin , W. C. Jones , M. Juvela , A. Karakci , E. Keihänen , R. Keskitalo , K. Kiiveri , J. Kim , T. S. Kisner , R. Kneissl , J. Knoche , N. Krachmalnicoff , M. Kunz , H. Kurki-Suonio , F. Lacasa , G. Lagache , A. Lähteenmäki , J. -M. Lamarre , M. Langer , A. Lasenby , M. Lattanzi , C. R. Lawrence , M. Le Jeune , J. P. Leahy , E. Lellouch , R. Leonardi , J. León-Tavares , J. Lesgourgues , F. Levrier , A. Lewis , M. Liguori , P. B. Lilje , M. Linden-Vørnle , V. Lindholm , H. Liu , M. López-Caniego , P. M. Lubin , Y. -Z. Ma , J. F. Macías-Pérez , G. Maggio , D. S. Y. Mak , N. Mandolesi , A. Mangilli , A. Marchini , A. Marcos-Caballero , D. Marinucci , D. J. Marshall , P. G. Martin , M. Martinelli , E. Martínez-González , S. Masi , S. Matarrese , P. Mazzotta , J. D. McEwen , P. McGehee , S. Mei , P. R. Meinhold , A. Melchiorri , J. -B. Melin , L. Mendes , A. Mennella , M. Migliaccio , K. Mikkelsen , S. Mitra , M. -A. Miville-Deschênes , D. Molinari , A. Moneti , L. Montier , R. Moreno , G. Morgante , D. Mortlock , A. Moss , S. Mottet , M. Müenchmeyer , D. Munshi , J. A. Murphy , A. Narimani , P. Naselsky , A. Nastasi , F. Nati , P. Natoli , M. Negrello , C. B. Netterfield , H. U. Nørgaard-Nielsen , F. Noviello , D. Novikov , I. Novikov , M. Olamaie , N. Oppermann , E. Orlando , C. A. Oxborrow , F. Paci , L. Pagano , F. Pajot , R. Paladini , S. Pandolfi , D. Paoletti , B. Partridge , F. Pasian , G. Patanchon , T. J. Pearson , M. Peel , H. V. Peiris , V. -M. Pelkonen , O. Perdereau , L. Perotto , Y. C. Perrott , F. Perrotta , V. Pettorino , F. Piacentini , M. Piat , E. Pierpaoli , D. Pietrobon , S. Plaszczynski , D. Pogosyan , E. Pointecouteau , G. Polenta , L. Popa , G. W. Pratt , G. Prézeau , S. Prunet , J. -L. Puget , J. P. Rachen , B. Racine , W. T. Reach , R. Rebolo , M. Reinecke , M. Remazeilles , C. Renault , A. Renzi , I. Ristorcelli , G. Rocha , M. Roman , E. Romelli , C. Rosset , M. Rossetti , A. Rotti , G. Roudier , B. Rouillé d'Orfeuil , M. Rowan-Robinson , J. A. Rubiño-Martín , B. Ruiz-Granados , C. Rumsey , B. Rusholme , N. Said , V. Salvatelli , L. Salvati , M. Sandri , H. S. Sanghera , D. Santos , R. D. E. Saunders , A. Sauvé , M. Savelainen , G. Savini , B. M. Schaefer , M. P. Schammel , D. Scott , M. D. Seiffert , P. Serra , E. P. S. Shellard , T. W. Shimwell , M. Shiraishi , K. Smith , T. Souradeep , L. D. Spencer , M. Spinelli , S. A. Stanford , D. Stern , V. Stolyarov , R. Stompor , A. W. Strong , R. Sudiwala , R. Sunyaev , P. Sutter , D. Sutton , A. -S. Suur-Uski , J. -F. Sygnet , J. A. Tauber , D. Tavagnacco , L. Terenzi , D. Texier , L. Toffolatti , M. Tomasi , M. Tornikoski , M. Tristram , A. Troja , T. Trombetti , M. Tucci , J. Tuovinen , M. Türler , G. Umana , L. Valenziano , J. Valiviita , B. Van Tent , T. Vassallo , M. Vidal , M. Viel , P. Vielva , F. Villa , L. A. Wade , B. Walter , B. D. Wandelt , R. Watson , I. K. Wehus , N. Welikala , J. Weller , M. White , S. D. M. White , A. Wilkinson , D. Yvon , A. Zacchei , J. P. Zibin , A. Zonca

We explore the ability of observations of the global brightness temperature of the 21-cm signal to constrain the reionization history and the properties of the ionizing sources. In order to describe the reionization signal, we employ either…

宇宙学与河外天体物理 · 物理学 2015-05-27 Andrea Morandi , Rennan Barkana

We compare the detection abilities for the relic gravitational waves by two kinds of forthcoming cosmic microwave background radiation (CMB) experiments, space-based Planck satellite and the various ground-based experiments. Comparing with…

宇宙学与河外天体物理 · 物理学 2009-07-17 W. Zhao , W. Zhang

The Microwave Anisotropy Probe and Planck missions will provide low noise maps of the temperature of the cosmic microwave background (CMB). These maps will allow measurement of the power spectrum of the CMB with measurement noise below…

We study Minkowski Functionals as probes of primordial non-Gaussianity in the Cosmic Microwave Background, specifically for the estimate of the primordial `local' bi-spectrum parameter f_NL, with instrumental parameters which should be…

宇宙学与河外天体物理 · 物理学 2015-06-11 Anne Ducout , François Bouchet , Stéphane Colombi , Dmitri Pogosyan , Simon Prunet

Modern cosmological data demand modern data analysis techniques. We introduce BayOp, a new likelihood sampling and maximisation method which is based on the Bayesian Optimisation algorithm and learns a function instead of randomly sampling…

宇宙学与河外天体物理 · 物理学 2022-04-15 Jan Hamann , Julius Wons

Observations of cosmic microwave background polarisation, essential for probing a potential phase of inflation in the early universe, suffer from contamination by polarised emission from the Galactic interstellar medium. This work combines…

宇宙学与河外天体物理 · 物理学 2024-09-25 Jacques Delabrouille

Observations of the polarization of the cosmic microwave backround (CMB) have the potential to place much tighter constraints on cosmological parameters than observations of the fluctuations in temperature alone. We discuss using CMB…

天体物理学 · 物理学 2009-10-30 William H. Kinney

[Abridged] We use our most recent training set for the RICO code to estimate the impact of recombination uncertainties on the posterior probability distributions which will be obtained from future CMB experiments, and in particular the…

宇宙学与河外天体物理 · 物理学 2015-05-14 J. A. Rubino-Martin , J. Chluba , W. A. Fendt , B. D. Wandelt

We show that results from the Planck satellite reported in 2013 are consistent with the simplest cyclic models for natural parameter ranges i.e., order unity dimensionless coefficients, assuming the standard entropic mechanism for…

宇宙学与河外天体物理 · 物理学 2015-06-15 Jean-Luc Lehners , Paul J. Steinhardt

We describe the BeyondPlanck project in terms of motivation, methodology and main products, and provide a guide to a set of companion papers that describe each result in fuller detail. We implement a complete end-to-end Bayesian analysis…

We revisit the anisotropic universe model previously developed by Ackerman, Carroll and Wise (ACW), and generalize both the theoretical and computational framework to include polarization and various forms of systematic effects. We apply…

宇宙学与河外天体物理 · 物理学 2014-11-20 Nicolaas E. Groeneboom , Lotty Ackerman , Ingunn Kathrine Wehus , Hans Kristian Eriksen