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Related papers: The Primordial Inflation Polarization Explorer (PI…

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The Polarized Instrument for Long-wavelength Observation of the Tenuous interstellar medium (PILOT) is a balloon-borne experiment aiming at measuring the polarized emission of thermal dust at a wavelength of 240 mm (1.2 THz). A first PILOT…

Measurements of Cosmic Microwave Background (CMB) anisotropy have served as the best experimental probe of the early universe to date. The inflationary paradigm, inspired in part by the extreme isotropy of the CMB, is now a cornerstone in…

The Stratospheric Kinetic Inductance Polarimeter (SKIP) is a proposed balloon-borne experiment designed to study the cosmic microwave background, the cosmic infrared background and Galactic dust emission by observing 1133 square degrees of…

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…

Astrophysics · Physics 2009-10-30 William H. Kinney

BICEP1 is a millimeter-wavelength telescope designed specifically to measure the inflationary B-mode polarization of the Cosmic Microwave Background (CMB) at degree angular scales. We present results from an analysis of the data acquired…

The curl-modes of Cosmic Microwave Background (CMB) polarization probe horizon-scale primordial gravitational waves related to inflation. A significant source of confusion is expected from a lensing conversion of polarization related to…

Astrophysics · Physics 2009-11-10 Asantha Cooray

We introduce the light-weight carbon fiber and aluminum gondola designed for the SPIDER balloon-borne telescope. SPIDER is designed to measure the polarization of the Cosmic Microwave Background radiation with unprecedented sensitivity and…

In this paper we discuss the latest developments of the STRIP instrument of the "Large Scale Polarization Explorer" (LSPE) experiment. LSPE is a novel project that combines ground-based (STRIP) and balloon-borne (SWIPE) polarization…

The BICEP3 Polarimeter is a small aperture, refracting telescope, dedicated to the observation of the Cosmic Microwave Background (CMB) at 95GHz. It is designed to target degree angular scale polarization patterns, in particular the…

Here we describe the design and performance of the Spider instrument. Spider is a balloon-borne cosmic microwave background polarization imager that will map part of the sky at 90, 145, and 280 GHz with sub-degree resolution and high…

The BICEP3 CMB Polarimeter is a small-aperture refracting telescope located at the South Pole and is specifically designed to search for the possible signature of inflationary gravitational waves in the Cosmic Microwave Background (CMB).…

Inflation predicts specific relations between the amplitudes and spectral indices of the primordial spectrum of density (scalar metric) perturbations and gravitational waves (tensor metric perturbations). Detection of a stochastic…

Astrophysics · Physics 2016-08-25 Marc Kamionkowski , Arthur Kosowsky

We quantify the limiting factors in optimizing current-technology cosmic microwave background (CMB) polarization experiments in order to learn about inflationary physics. We consider space-based, balloon-borne and ground-based experiments.…

Astrophysics · Physics 2011-05-12 Licia Verde , Hiranya Peiris , Raul Jimenez

The Probe of Inflation and Cosmic Origins (PICO) is a probe-class mission concept currently under study by NASA. PICO will probe the physics of the Big Bang and the energy scale of inflation, constrain the sum of neutrino masses, measure…

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

We evaluate the large scale polarization of the cosmic microwave background induced, via Thomson scattering prior to decoupling, by nearly scale-invariant spectra of scalar and tensor metric perturbations, such as those predicted by most…

Astrophysics · Physics 2016-08-30 Diego Harari , Matias Zaldarriaga

Interest in the study of magnetic fields and the properties of interstellar dust, explored through increasingly capable far-IR/submillimeter polarimetry, along with maturing detector technology, have set the stage for a transformative leap…

Instrumentation and Methods for Astrophysics · Physics 2025-09-03 C. Darren Dowell , Brandon S. Hensley , Marc Sauvage

The PRobe far-Infrared Mission for Astrophysics (PRIMA) is a cryogenically-cooled, far-infrared (far-IR) observatory expected to begin serving the astronomical community by early 2030. The mission features two advanced instruments: PRIMAger…