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In the field of astrophysics, the faint signal from distant galaxies and other dim cosmological sources at millimeter and submillimeter wavelengths require the use of high-sensitivity experiments. Cryogenics and the use of low-temperature…

Instrumentation and Methods for Astrophysics · Physics 2020-09-22 Lionel Duband , Thomas Prouve , James Bock , Lorenzo Moncelsi , Alessandro Schillaci

We present an improved search for axion-like polarization oscillations in the cosmic microwave background (CMB) with observations from the Keck Array. An all-sky, temporally sinusoidal rotation of CMB polarization, equivalent to a…

We present a measurement of the $B$-mode polarization power spectrum of the cosmic microwave background anisotropies at 32 $\le$ $\ell$ $<$ 502 for three bands centered at 95, 150, and 220 GHz using data from the SPT-3G receiver on the…

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

We report on the development of commercially fabricated multi-chroic antenna coupled Transition Edge Sensor (TES) bolometer arrays for Cosmic Microwave Background (CMB) polarimetry experiments. The orders of magnitude increase in detector…

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…

ASTEP South is the first phase of the ASTEP project (Antarctic Search for Transiting ExoPlanets). The instrument is a fixed 10 cm refractor with a 4kx4k CCD camera in a thermalized box, pointing continuously a 3.88 degree x 3.88 degree…

We present the design and the preliminary on sky performance with respect to beams and pass-bands of a multichroic polarimeter array covering the 90 and 146 GHz Cosmic Microwave Background (CMB) bands and its enabling broadband optical…

The South Pole Telescope (SPT) is a high-resolution microwave-frequency telescope designed to observe the Cosmic Microwave Background (CMB). To date, two cameras have been installed on the SPT to conduct two surveys of the CMB, the first in…

Instrumentation and Methods for Astrophysics · Physics 2016-01-22 Benjamin Saliwanchik

The Kepler mission has provided a treasure trove of eclipsing binaries (EBs), observed at extremely high photometric precision, nearly continuously for several years. We are carrying out a survey of ~100 of these EBs to derive dynamical…

The Cosmology Large Angular Scale Surveyor (CLASS) is a polarization-sensitive telescope array located at an altitude of 5,200 m in the Chilean Atacama Desert and designed to measure the polarized Cosmic Microwave Background (CMB) over…

Here we describe the Compact Array Broadband Backend (CABB) and present first results obtained with the upgraded Australia Telescope Compact Array (ATCA). The 16-fold increase in observing bandwidth, from 2 x 128 MHz to 2 x 2048 MHz, high…

The Princeton IQU Experiment (PIQUE) and the Cosmic Anisotropy Polarization MAPper (CAPMAP) are experiments designed to measure the polarization of the Cosmic Microwave Background (CMB) on sub-degree scales in an area within 1 degree of the…

Development of the Silicon photomultiplier Elementary Cell Add-on camera (SiECA) has provided extensive information regarding the use of SiPMs for future cosmic ray detection systems. We present the technical aspects of sensor readout…

Instrumentation and Methods for Astrophysics · Physics 2019-08-27 W. Painter , A. Haungs , T. Huber , M. Karus , A. Menshikov , M. Oehler , M. Renschler , JEM-EUSO Collaboration

The Cosmology Large Angular Scale Surveyor (CLASS) is a polarization-sensitive telescope array located at an altitude of 5,200 m in the Chilean Atacama Desert. CLASS is designed to measure "E-mode" (even parity) and "B-mode" (odd parity)…

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