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The Primordial Inflation Explorer (PIXIE) is an Explorer-class mission to measure the gravity-wave signature of primordial inflation through its distinctive imprint on the linear polarization of the cosmic microwave background. The…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 A. Kogut , D. J. Fixsen , D. T. Chuss , J. Dotson , E. Dwek , M. Halpern , G. F. Hinshaw , S. M. Meyer , S. H. Moseley , M. D. Seiffert , D. N. Spergel , E. J. Wollack

The Primordial Inflation Explorer (PIXIE) is an Explorer-class mission concept to measure the energy spectrum and linear polarization of the cosmic microwave background (CMB). A single cryogenic Fourier transform spectrometer compares the…

The Primordial Inflation Explorer (PIXIE) is an Explorer-class mission concept to measure cosmological signals from both linear polarization of the cosmic microwave background and spectral distortions from a perfect blackbody. The targeted…

Instrumentation and Methods for Astrophysics · Physics 2021-03-08 A. Kogut , D. J. Fixsen

The Primordial Inflation Explorer (PIXIE) is an Explorer-class mission concept to measure the gravitational-wave signature of primordial inflation through its distinctive imprint on the linear polarization of the cosmic microwave background…

Instrumentation and Methods for Astrophysics · Physics 2019-08-05 A. Kogut , D. J. Fixsen

The Primordial Inflation Explorer (PIXIE) is an Explorer-class mission concept to measure the spectrum and polarization of the cosmic microwave background. Cosmological signals are small compared to the instantaneous instrument noise,…

The Primordial Inflation Polarization Explorer (PIPER) is a balloon-borne cosmic microwave background (CMB) polarimeter designed to search for evidence of inflation by measuring the large-angular scale CMB polarization signal. BICEP2…

The balloon-borne LSPE mission is optimized to measure the linear polarization of the Cosmic Microwave Background at large angular scales. The Short Wavelength Instrument for the Polarization Explorer (SWIPE) is composed of 3 arrays of…

The Primordial Inflation Polarization ExploreR (PIPER) is a balloon-borne telescope designed to measure the polarization of the Cosmic Microwave Background on large angular scales. PIPER will map 85% of the sky at 200, 270, 350, and 600 GHz…

In this paper we explore the possibility of using transition edge sensor (TES) detectors in multi-mode configuration in the focal plane of the Short Wavelength Instrument for the Polarization Explorer (SWIPE) of the balloon-borne…

Instrumentation and Methods for Astrophysics · Physics 2016-02-26 R. Gualtieri , E. S. Battistelli , A. Cruciani , P. de Bernardis , M. Biasotti , D. Corsini , F. Gatti , L. Lamagna , S. Masi

In this paper we investigate the impact of using a polarization modulator in the Short Wavelenght Instrument for the Polarization Explorer (SWIPE) of the Large Scale Polarization Explorer (LSPE). The experiment is optimized to measure the…

Instrumentation and Methods for Astrophysics · Physics 2019-04-04 F. Columbro , E. S. Battistelli , A. Coppolecchia , G. D'Alessandro , P. de Bernardis , L. Lamagna , S. Masi , L. Pagano , A. Paiella , F. Piacentini , G. Presta

Inflation is the leading theory of the first instant of the universe. Inflation, which postulates that the universe underwent a period of rapid expansion an instant after its birth, provides convincing explanation for cosmological…

Instrumentation and Methods for Astrophysics · Physics 2018-06-13 A. Suzuki , P. A. R. Ade , Y. Akiba , D. Alonso , K. Arnold , J. Aumont , C. Baccigalupi , D. Barron , S. Basak , S. Beckman , J. Borrill , F. Boulanger , M. Bucher , E. Calabrese , Y. Chinone , H-M. Cho , A. Cukierman , D. W. Curtis , T. de Haan , M. Dobbs , A. Dominjon , T. Dotani , L. Duband , A. Ducout , J. Dunkley , J. M. Duval , T. Elleflot , H. K. Eriksen , J. Errard , J. Fischer , T. Fujino , T. Funaki , U. Fuskeland , K. Ganga , N. Goeckner-Wald , J. Grain , N. W. Halverson , T. Hamada , T. Hasebe , M. Hasegawa , K. Hattori , M. Hattori , L. Hayes , M. Hazumi , N. Hidehira , C. A. Hill , G. Hilton , J. Hubmayr , K. Ichiki , T. Iida , H. Imada , M. Inoue , Y. Inoue , K. D. , H. Ishino , O. Jeong , H. Kanai , D. Kaneko , S. Kashima , N. Katayama , T. Kawasaki , S. A. Kernasovskiy , R. Keskitalo , A. Kibayashi , Y. Kida , K. Kimura , T. Kisner , K. Kohri , E. Komatsu , K. Komatsu , C. L. Kuo , N. A. Kurinsky , A. Kusaka , A. Lazarian , A. T. Lee , D. Li , E. Linder , B. Maffei , A. Mangilli , M. Maki , T. Matsumura , S. Matsuura , D. Meilhan , S. Mima , Y. Minami , K. Mitsuda , L. Montier , M. Nagai , T. Nagasaki , R. Nagata , M. Nakajima , S. Nakamura , T. Namikawa , M. Naruse , H. Nishino , T. Nitta , T. Noguchi , H. Ogawa , S. Oguri , N. Okada , A. Okamoto , T. Okamura , C. Otani , G. Patanchon , G. Pisano , G. Rebeiz , M. Remazeilles , P. L. Richards , S. Sakai , Y. Sakurai , Y. Sato , N. Sato , M. Sawada , Y. Segawa , Y. Sekimoto , U. Seljak , B. D. Sherwin , T. Shimizu , K. Shinozaki , R. Stompor , H. Sugai , H. Sugita , J. Suzuki , O. Tajima , S. Takada , R. Takaku , S. Takakura , S. Takatori , D. Tanabe , E. Taylor , K. L. Thompson , B. Thorne , T. Tomaru , T. Tomida , N. Tomita , M. Tristram , C. Tucker , P. Turin , M. Tsujimoto , S. Uozumi , S. Utsunomiya , Y. Uzawa , F. Vansyngel , I. K. Wehus , B. Westbrook , M. Willer , N. Whitehorn , Y. Yamada , R. Yamamoto , N. Yamasaki , T. Yamashita , M. Yoshida

Measurements of cosmic microwave background spectral distortions have profound implications for our understanding of physical processes taking place over a vast window in cosmological history. Foreground contamination is unavoidable in such…

Cosmology and Nongalactic Astrophysics · Physics 2017-08-03 Maximilian H. Abitbol , Jens Chluba , J. Colin Hill , Bradley R. Johnson

EBEX is a balloon-borne polarimeter designed to measure the intensity and polarization of the cosmic microwave background radiation. The measurements would probe the inflationary epoch that took place shortly after the big bang and would…

[Abridged] The measurement of the polarization of the Cosmic Microwave Background radiation is one of the current frontiers in cosmology. In particular, the detection of the primordial B-modes, could reveal the presence of gravitational…

Instrumentation and Methods for Astrophysics · Physics 2021-08-10 The LSPE collaboration , G. Addamo , P. A. R. Ade , C. Baccigalupi , A. M. Baldini , P. M. Battaglia , E. S. Battistelli , A. Baù , P. de Bernardis , M. Bersanelli , M. Biasotti , A. Boscaleri , B. Caccianiga , S. Caprioli , F. Cavaliere , F. Cei , K. A. Cleary , F. Columbro , G. Coppi , A. Coppolecchia , F. Cuttaia , G. D'Alessandro , G. De Gasperis , M. De Petris , V. Fafone , F. Farsian , L. Ferrari Barusso , F. Fontanelli , C. Franceschet , T. C. Gaier , L. Galli , F. Gatti , R. Genova-Santos , M. Gerbino , M. Gervasi , T. Ghigna , D. Grosso , A. Gruppuso , R. Gualtieri , F. Incardona , M. E. Jones , P. Kangaslahti , N. Krachmalnicoff , L. Lamagna , M. Lattanzi , C. H. López-Caraballo , M. Lumia , R. Mainini , D. Maino , S. Mandelli , M. Maris , S. Masi , S. Matarrese , A. May , L. Mele , P. Mena , A. Mennella , R. Molina , D. Molinari , G. Morgante , U. Natale , F. Nati , P. Natoli , L. Pagano , A. Paiella , F. Panico , F. Paonessa , S. Paradiso , A. Passerini , M. Perez-de-Taoro , O. A. Peverini , F. Piacentini , L. Piccirillo , G. Pisano , D. Poletti , G. Presta , S. Realini , N. Reyes , J. A. Rubino-Martin , M. Sandri , S. Sartor , F. Pezzotta , G. Polenta , A. Rocchi , A. Schillaci , G. Signorelli , B. Siri , M. Soria , F. Spinella , V. Tapia , A. Tartari , A. C. Taylor , L. Terenzi , M. Tomasi , E. Tommasi , C. Tucker , D. Vaccaro , D. M. Vigano , F. Villa , G. Virone , N. Vittorio , A. Volpe , R. E. J. Watkins , A. Zacchei , M. Zannoni

The Large Scale Polarization Explorer (LSPE) is a cosmology program for the measurement of large scale curl-like features (B-modes) in the polarization of the Cosmic Microwave Background. Its goal is to constrain the background of…

The Primordial Inflation Polarization Explorer (PIPER) is a stratospheric balloon payload to measure polarization of the cosmic microwave background. Twin telescopes mounted within an open-aperture bucket dewar couple the sky to bolometric…

Instrumentation and Methods for Astrophysics · Physics 2024-06-19 A. Kogut , T. Essinger-Hileman , D. Fixsen , L. Lowe , P. Mirel , E. Switzer , E. Wollack

Bolometric Interferometry (BI) is one of the most promising techniques for precise measurements of the Cosmic Microwave Background polarization. In this paper, we present the results of DIBO (Demonstrateur d'Interferometrie Bolometrique), a…

Instrumentation and Methods for Astrophysics · Physics 2009-02-04 Adnan Ghribi , Andrea Tartari , Silvia Galli , Michel Piat , Eric Breelle , Jean-Christophe Hamilton , Sebastiano Spinelli , Massimo Gervasi , Mario Zannoni

We have developed a bolometric detector that is intrinsically sensitive to linear polarization which is optimized for making measurements of the polarization of the cosmic microwave background radiation. The receiver consists of a pair of…

Astrophysics · Physics 2020-12-22 W. C. Jones , R. S. Bhatia , J. J. Bock , A. E. Lange

The BICEP experiment was designed specifically to search for the signature of inflationary gravitational waves in the polarization of the cosmic microwave background (CMB). Using a novel small-aperture refractor and 49 pairs of…

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