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We examine the statistical properties of polarization maps from Planck 2018 within the patch of sky observed by the BICEP2/Keck experiment using the one point distribution function (1PDF), skewness, and kurtosis statistics. Our analysis is…

宇宙学与河外天体物理 · 物理学 2020-06-17 Hao Liu , James Creswell , Pavel Naselsky

We report on the status of an ongoing effort to develop arrays of horn-coupled, polarization-sensitive microwave kinetic inductance detectors (MKIDs) that are each sensitive to two spectral bands between 125 and 280 GHz. These multi-chroic…

Millimeter-wave refracting telescopes targeting the degree-scale structure of the cosmic microwave background (CMB) have recently grown to diffraction-limited apertures of over 0.5 meters. These instruments are entirely housed in vacuum…

In this work we describe upgrades to the Spider balloon-borne telescope in preparation for its second flight, currently planned for December 2021. The Spider instrument is optimized to search for a primordial B-mode polarization signature…

LiteBIRD is a space-borne experiment dedicated to detecting large-scale $B$-mode anisotropies in the linear polarization of the Cosmic Microwave Background (CMB) predicted by the theory of inflation. It is planned to be launched in the late…

天体物理仪器与方法 · 物理学 2022-09-27 Mayu Tominaga , Masahiro Tsujimoto , Graeme Smecher , Hirokazu Ishino

Measurements of cosmic microwave background (CMB) anisotropies constrain isocurvature fluctuations between photons and non-relativistic particles to be sub-dominant to adiabatic fluctuations. Perturbations in the relative number densities…

宇宙学与河外天体物理 · 物理学 2012-01-09 Daniel Grin , Olivier Doré , Marc Kamionkowski

LiteBIRD has been selected as JAXA's strategic large mission in the 2020s, to observe the cosmic microwave background (CMB) $B$-mode polarization over the full sky at large angular scales. The challenges of LiteBIRD are the wide…

天体物理仪器与方法 · 物理学 2021-01-19 Y. Sekimoto , P. A. R. Ade , A. Adler , E. Allys , K. Arnold , D. Auguste , J. Aumont , R. Aurlien , J. Austermann , C. Baccigalupi , A. J. Banday , R. Banerji , R. B. Barreiro , S. Basak , J. Beall , D. Beck , S. Beckman , J. Bermejo , P. de Bernardis , M. Bersanelli , J. Bonis , J. Borrill , F. Boulanger , S. Bounissou , M. Brilenkov , M. Brown , M. Bucher , E. Calabrese , P. Campeti , A. Carones , F. J. Casas , A. Challinor , V. Chan , K. Cheung , Y. Chinone , J. F. Cliche , L. Colombo , F. Columbro , J. Cubas , A. Cukierman , D. Curtis , G. D'Alessandro , N. Dachlythra , M. De Petris , C. Dickinson , P. Diego-Palazuelos , M. Dobbs , T. Dotani , L. Duband , S. Duff , J. M. Duval , K. Ebisawa , T. Elleflot , H. K. Eriksen , J. Errard , T. Essinger-Hileman , F. Finelli , R. Flauger , C. Franceschet , U. Fuskeland , M. Galloway , K. Ganga , J. R. Gao , R. Genova-Santos , M. Gerbino , M. Gervasi , T. Ghigna , E. Gjerløw , M. L. Gradziel , J. Grain , F. Grupp , A. Gruppuso , J. E. Gudmundsson , T. de Haan , N. W. Halverson , P. Hargrave , T. Hasebe , M. Hasegawa , M. Hattori , M. Hazumi , S. Henrot-Versillé , D. Herman , D. Herranz , C. A. Hill , G. Hilton , Y. Hirota , E. Hivon , R. A. Hlozek , Y. Hoshino , E. de la Hoz , J. Hubmayr , K. Ichiki , T. iida , H. Imada , K. Ishimura , H. Ishino , G. Jaehnig , T. Kaga , S. Kashima , N. Katayama , A. Kato , T. Kawasaki , R. Keskitalo , T. Kisner , Y. Kobayashi , N. Kogiso , A. Kogut , K. Kohri , E. Komatsu , K. Komatsu , K. Konishi , N. Krachmalnicoff , I. Kreykenbohm , C. L. Kuo , A. Kushino , L. Lamagna , J. V. Lanen , M. Lattanzi , A. T. Lee , C. Leloup , F. Levrier , E. Linder , T. Louis , G. Luzzi , T. Maciaszek , B. Maffei , D. Maino , M. Maki , S. Mandelli , E. Martinez-Gonzalez , S. Masi , T. Matsumura , A. Mennella , M. Migliaccio , Y. Minanmi , K. Mitsuda , J. Montgomery , L. Montier , G. Morgante , B. Mot , Y. Murata , J. A. Murphy , M. Nagai , Y. Nagano , T. Nagasaki , R. Nagata , S. Nakamura , T. Namikawa , P. Natoli , S. Nerval , T. Nishibori , H. Nishino , C. O'Sullivan , H. Ogawa , H. Ogawa , S. Oguri , H. Ohsaki , I. S. Ohta , N. Okada , N. Okada , L. Pagano , A. Paiella , D. Paoletti , G. Patanchon , J. Peloton , F. Piacentini , G. Pisano , G. Polenta , D. Poletti , T. Prouvé , G. Puglisi , D. Rambaud , C. Raum , S. Realini , M. Reinecke , M. Remazeilles , A. Ritacco , G. Roudil , J. A. Rubino-Martin , M. Russell , H. Sakurai , Y. Sakurai , M. Sandri , M. Sasaki , G. Savini , D. Scott , J. Seibert , B. Sherwin , K. Shinozaki , M. Shiraishi , P. Shirron , G. Signorelli , G. Smecher , S. Stever , R. Stompor , H. Sugai , S. Sugiyama , A. Suzuki , J. Suzuki , T. L. Svalheim , E. Switzer , R. Takaku , H. Takakura , S. Takakura , Y. Takase , Y. Takeda , A. Tartari , E. Taylor , Y. Terao , H. Thommesen , K. L. Thompson , B. Thorne , T. Toda , M. Tomasi , M. Tominaga , N. Trappe , M. Tristram , M. Tsuji , M. Tsujimoto , C. Tucker , J. Ullom , G. Vermeulen , P. Vielva , F. Villa , M. Vissers , N. Vittorio , I. Wehus , J. Weller , B. Westbrook , J. Wilms , B. Winter , E. J. Wollack , N. Y. Yamasaki , T. Yoshida , J. Yumoto , M. Zannoni , A. Zonca

QUBIC, the QU Bolometric Interferometer for Cosmology, is a novel forthcoming instrument to measure the B-mode polarization anisotropy of the Cosmic Microwave Background. The detection of the B-mode signal will be extremely challenging;…

天体物理仪器与方法 · 物理学 2018-11-07 A. J. May , C. Chapron , G. Coppi , G. D'Alessandro , P. de Bernardis , S. Masi , S. Melhuish , M. Piat , L. Piccirillo , A. Schillaci , J. -P. Thermeau , P. Ade , G. Amico , D. Auguste , J. Aumont , S. Banfi , G. Barbara , P. Battaglia , E. Battistelli , A. Bau , B. Belier , D. Bennett , L. Berge , J. -Ph. Bernard , M. Bersanelli , M. -A. Bigot-Sazy , N. Bleurvacq , J. Bonaparte , J. Bonis , G. Bordier , E. Breelle , E. Bunn , D. Burke , D. Buzi , A. Buzzelli , F. Cavaliere , P. Chanial , R. Charlassier , F. Columbro , A. Coppolecchia , F. Couchot , R. D'Agostino , G. De Gasperis , M. De Leo , M. De Petris , A. Di Donato , L. Dumoulin , A. Etchegoyen , A. Fasciszewski , C. Franceschet , M. M. Gamboa Lerena , B. Garcia , X. Garrido , M. Gaspard , A. Gault , D. Gayer , M. Gervasi , M. Giard , Y. Giraud-Heraud , M. Gomez Berisso , M. Gonzalez , M. Gradziel , L. Grandsire , E. Guerrard , J. -Ch. Hamilton , D. Harari , V. Haynes , S. Henrot-Versille , D. T. Hoang , F. Incardona , E. Jules , J. Kaplan , A. Korotkov , C. Kristukat , L. Lamagna , S. Loucatos , T. Louis , A. Lowitz , V. Lukovic , R. Luterstein , B. Maffei , S. Marnieros , A. Mattei , M. A. McCulloch , M. C. Medina , L. Mele , A. Mennella , L. Montier , L. M. Mundo , J. A. Murphy , J. D. Murphy , C. O'Sullivan , E. Olivieri , A. Paiella , F. Pajot , A. Passerini , H. Pastoriza , A. Pelosi , C. Perbost , O. Perdereau , F. Pezzotta , F. Piacentini , G. Pisano , G. Polenta , D. Prele , R. Puddu , D. Rambaud , P. Ringegni , G. E. Romero , M. Salatino , C. G. Scoccola , S. Scully , S. Spinelli , M. Stolpovskiy , F. Suarez , A. Tartari , P. Timbie , S. A. Torchinsky , M. Tristram , V. Truongcanh , C. Tucker , G. Tucker , S. Vanneste , D. Vigano , N. Vittorio , F. Voisin , B. Watson , F. Wicek , M. Zannoni , A. Zullo

The Cosmic Microwave Background Radiation (CMB) is an invaluable probe of the conditions of the early universe. Recent measurements of its spatial anisotropy have allowed accurate determinations of several fundamental cosmological…

天体物理学 · 物理学 2009-09-29 Christopher O'Dell

Multi-frequency, high resolution, full sky measurements of the anisotropy in both temperature and polarisation of the cosmic microwave background radiation are the goals of the satellite missions MAP (NASA) and Planck (ESA). The ultimate…

天体物理学 · 物理学 2007-05-23 K. M. Gorski , E. Hivon , B. D. Wandelt

The angular power spectrum of the cosmic microwave background temperature anisotropy observed by WMAP has an anomalous dip at l~20 and bump at l~40. One explanation for this structure is the presence of features in the primordial curvature…

宇宙学与河外天体物理 · 物理学 2009-05-19 Michael J. Mortonson , Cora Dvorkin , Hiranya V. Peiris , Wayne Hu

We present measurements of large-scale cosmic microwave background (CMB) E-mode polarization from the Cosmology Large Angular Scale Surveyor (CLASS) 90 GHz data. Using 115 det-yr of observations collected through 2024 with a variable-delay…

We present new measurements of the cosmic microwave background (CMB) polarization from the final season of the Cosmic Anisotropy Polarization MAPper (CAPMAP). The data set was obtained in winter 2004-2005 with the 7 m antenna in Crawford…

Polarized Galactic synchrotron emission is an undesirable foreground for cosmic microwave background (CMB) experiments observing at frequencies $< 150$ GHz. We perform a combined analysis of observational data at 1.4, 2.3, 23, 30 and 33 GHz…

宇宙学与河外天体物理 · 物理学 2022-09-07 Janet L. Weiland , Graeme E. Addison , Charles L. Bennett , Mark Halpern , Gary Hinshaw

We describe an off-axis microwave telescope for observations of the anisotropy in the cosmic microwave background (CMB) radiation on angular scales between 0.5 deg and 3 deg. The receiver utilizes cryogenic high-electron-mobility transistor…

天体物理学 · 物理学 2009-10-28 E. J. Wollack , M. J. Devlin , N. Jarosik , C. B. Netterfield , L. Page , D. Wilkinson

Current and future B-mode polarization data are the most powerful observables to constrain gravitational waves from the early Universe. We set conservative constraints on tensor modes when relaxing the inflationary consistency condition…

宇宙学与河外天体物理 · 物理学 2022-11-09 Daniela Paoletti , Fabio Finelli , Jussi Valiviita , Masashi Hazumi

We present details of the design, simulation, and initial test results of prototype detectors for the fourth-generation receiver of the South Pole Telescope (SPT). Optimized for the detection of key secondary anisotropies of the cosmic…

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