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We present the BOOMERanG-03 experiment and maps of the Stokes parameters I, Q, U of the microwave sky obtained during a 14 day balloon flight in 2003. Three regions of the southern sky were surveyed: a deep survey (~ 90 square degrees) and…

Recent developments of transition-edge sensors (TESs), based on extensive experience in ground-based experiments, have been making the sensor techniques mature enough for their application on future satellite CMB polarization experiments.…

Instrumentation and Methods for Astrophysics · Physics 2021-04-06 H. Sugai , P. A. R. Ade , Y. Akiba , D. Alonso , K. Arnold , J. Aumont , J. Austermann , C. Baccigalupi , A. J. Banday , R. Banerji , R. B. Barreiro , S. Basak , J. Beall , S. Beckman , M. Bersanelli , J. Borrill , F. Boulanger , M. L. Brown , M. Bucher , A. Buzzelli , E. Calabrese , F. J. Casas , A. Challinor , V. Chan , Y. Chinone , J. -F. Cliche , F. Columbro , A. Cukierman , D. Curtis , P. Danto , P. de Bernardis , T. de Haan , M. De Petris , C. Dickinson , M. Dobbs , T. Dotani , L. Duband , A. Ducout , S. Duff , A. Duivenvoorden , J. -M. Duval , K. Ebisawa , T. Elleflot , H. Enokida , H. K. Eriksen , J. Errard , T. Essinger-Hileman , F. Finelli , R. Flauger , C. Franceschet , U. Fuskeland , K. Ganga , J. -R. Gao , R. Génova-Santos , T. Ghigna , A. Gomez , M. L. Gradziel , J. Grain , F. Grupp , A. Gruppuso , J. E. Gudmundsson , N. W. Halverson , P. Hargrave , T. Hasebe , M. Hasegawa , M. Hattori , M. Hazumi , S. Henrot-Versille , D. Herranz , C. Hill , G. Hilton , Y. Hirota , E. Hivon , R. Hlozek , D. -T. Hoang , J. Hubmayr , K. Ichiki , T. Iida , H. Imada , K. Ishimura , H. Ishino , G. C. Jaehnig , M. Jones , T. Kaga , S. Kashima , Y. Kataoka , N. Katayama , T. Kawasaki , R. Keskitalo , A. Kibayashi , T. Kikuchi , K. Kimura , T. Kisner , Y. Kobayashi , N. Kogiso , A. Kogut , K. Kohri , E. Komatsu , K. Komatsu , K. Konishi , N. Krachmalnicoff , C. L. Kuo , N. Kurinsky , A. Kushino , M. Kuwata-Gonokami , L. Lamagna , M. Lattanzi , A. T. Lee , E. Linder , B. Maffei , D. Maino , M. Maki , A. Mangilli , E. Martínez-González , S. Masi , R. Mathon , T. Matsumura , A. Mennella , M. Migliaccio , Y. Minami , K. Mistuda , D. Molinari , L. Montier , G. Morgante , B. Mot , Y. Murata , J. A. Murphy , M. Nagai , R. Nagata , S. Nakamura , T. Namikawa , P. Natoli , S. Nerva , T. Nishibori , H. Nishino , Y. Nomura , F. Noviello , C. O'Sullivan , H. Ochi , H. Ogawa , H. Ogawa , H. Ohsaki , I. Ohta , N. Okada , N. Okada , L. Pagano , A. Paiella , D. Paoletti , G. Patanchon , F. Piacentini , G. Pisano , G. Polenta , D. Poletti , T. Prouvé , G. Puglisi , D. Rambaud , C. Raum , S. Realini , M. Remazeilles , G. Roudil , J. A. Rubiño-Martín , M. Russell , H. Sakurai , Y. Sakurai , M. Sandri , G. Savini , D. Scott , Y. Sekimoto , B. D. Sherwin , K. Shinozaki , M. Shiraishi , P. Shirron , G. Signorelli , G. Smecher , P. Spizzi , S. L. Stever , R. Stompor , S. Sugiyama , A. Suzuki , J. Suzuki , E. Switzer , R. Takaku , H. Takakura , S. Takakura , Y. Takeda , A. Taylor , E. Taylor , Y. Terao , K. L. Thompson , B. Thorne , M. Tomasi , H. Tomida , N. Trappe , M. Tristram , M. Tsuji , M. Tsujimoto , C. Tucker , J. Ullom , S. Uozumi , S. Utsunomiya , J. Van Lanen , G. Vermeulen , P. Vielva , F. Villa , M. Vissers , N. Vittorio , F. Voisin , I. Walker , N. Watanabe , I. Wehus , J. Weller , B. Westbrook , B. Winter , E. Wollack , R. Yamamoto , N. Y. Yamasaki , M. Yanagisawa , T. Yoshida , J. Yumoto , M. Zannoni , A. Zonca

QUBIC, the Q & U Bolometric Interferometer for Cosmology, is a telescope that observes the polarisation of the sky in the millimetre-wavelength range. Its goal is to detect the primordial B-modes of polarisation in the cosmic microwave…

Cosmology and Nongalactic Astrophysics · Physics 2026-04-21 Alexandre Huchet , Tom Laclavère , Leonora Kardum

The Atacama B-mode Search (ABS) experiment is a 145 GHz polarimeter designed to measure the B-mode polarization of the Cosmic Microwave Background (CMB) at large angular scales. The ABS instrument will ship to the Atacama Desert of Chile…

Current- and next-generation Cosmic Microwave Background (CMB) experiments will measure polarization anisotropies with unprecedented sensitivities. The need for high precision in these measurements underscores the importance of gaining a…

The PLANCK satellite mission has been launched the 14th of May 2009 and is dedicated to the measurement of the Cosmic Microwave Background (CMB) in temperature and polarization. The presence of diffuse galactic polarized emission…

Cosmology and Nongalactic Astrophysics · Physics 2010-07-20 L. Fauvet , J. F. Macias-Perez , F. X. Desert

We describe the design and expected performance of Clover, a new instrument designed to measure the B-mode polarization of the cosmic microwave background. The proposed instrument will comprise three independent telescopes operating at 90,…

We describe the MAXIMA experiment, a balloon-borne measurement designed to map temperature anisotropy in the Cosmic Microwave Background (CMB) over a wide range of angular scales (multipole range 80 < l < 800). The experiment consists of a…

The cosmic microwave background radiation (CMB) is now firmly established as a fundamental and essential probe of the geometry, constituents, and birth of the Universe. The CMB is a potent observable because it can be measured with…

Instrumentation and Methods for Astrophysics · Physics 2015-06-05 S. Hanany , M. Niemack , L. Page

Precise measurement of the foreground synchrotron emission, which contaminates the faint polarized cosmic microwave background radiation (CMB), is a major challenge for the next-generation of CMB experiments. To address this, dedicated…

The POLARBEAR-2/Simons Array Cosmic Microwave Background (CMB) polarization experiment is an upgrade and expansion of the existing POLARBEAR-1 (PB-1) experiment, located in the Atacama desert in Chile. Along with the CMB temperature and…

Instrumentation and Methods for Astrophysics · Physics 2018-06-15 Logan Howe , Calvin Tsai , Lindsay Lowry , Kam Arnold , Gabriele Coppi , John Groh , Xiaoyu Guo , Brian Keating , Adrian Lee , Andrew J. May , Lucio Piccirillo , Nathan Stebor , Grant Teply

We present results from the QMAP balloon experiment, which maps the Cosmic Microwave Background (CMB) and probes its angular power spectrum on degree scales. In two separate flights, data were taken in six channels at two frequency bands…

As the sensitivity of CMB telescopes increases, the need for precise calibration becomes critical. Started in 2022, the COSMOCal project aims to place an artificial polarized source in geostationary orbit, which will serve as a reference…

We report measurements of the CMB polarization power spectra from the January 2003 Antarctic flight of BOOMERANG. The primary results come from six days of observation of a patch covering 0.22% of the sky centered near R.A. = 82.5 deg.,…

The Simons Observatory (SO) will make precise temperature and polarization measurements of the cosmic microwave background (CMB) using a set of telescopes which will cover angular scales between 1 arcminute and tens of degrees, contain over…

The White Mountain Polarimeter (WMPol) is a dedicated ground-based microwave telescope and receiver system for observing polarization of the Cosmic Microwave Background. WMPol is located at an altitude of 3880 meters on a plateau in the…

Scattering of cosmic microwave background (CMB) radiation in galaxy clusters induces a polarization signal proportional to the CMB quadrupole anisotropy at the cluster's location and look-back time. A survey of such remote quadrupole…

Astrophysics · Physics 2007-05-23 Emory F. Bunn
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