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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. CMB polarimetry experiments have deployed…

Instrumentation and Methods for Astrophysics · Physics 2018-05-09 Aritoki Suzuki , Chris Bebek , Maurice Garcia-Sciveres , Stephen Holland , Akito Kusaka , Adrian T. Lee , Nicholas Palaio , Natalie Roe , Leo Steinmetz

Current and future Cosmic Microwave Background (CMB) Radiation experiments are targeting the polarized $B$-mode signal. The small amplitude of this signal makes a successful measurement challenging for current technologies. Therefore, very…

Instrumentation and Methods for Astrophysics · Physics 2020-11-18 Tommaso Ghigna , Tomotake Matsumura , Guillaume Patanchon , Hirokazu Ishino , Masashi Hazumi

In this work, we present the design and manufacturing of the two multi-mode antenna arrays of the COSMO experiment and the preliminary beam pattern measurements of their fundamental mode compared with simulations. COSMO is a cryogenic…

Despite several decades of multi-wavelength and multi-messenger spectral observations, Gamma-Ray Bursts (GRBs) remain one of the big mysteries of modern astrophysics. Polarization measurements are essential to gain a more clear and complete…

Instrumentation and Methods for Astrophysics · Physics 2021-09-08 N. De Angelis , J. M. Burgess , F. Cadoux , J. Greiner , J. Hulsman , M. Kole , H. C. Li , S. Mianowski , A. Pollo , N. Produit , D. Rybka , J. Stauffer , J. C. Sun , B. B. Wu , X. Wu , A. Zadrozny , S. N. Zhang

Cosmic microwave background (CMB) polarimetry has the potential to provide revolutionary advances in cosmology. Future experiments to detect the very weak B mode signal in CMB polarization maps will require unprecedented sensitivity and…

Astrophysics · Physics 2009-11-13 Peter Hyland , Brent Follin , Emory F. Bunn

We developed a waveguide-type dual-polarization sideband-separating SIS receiver system of the 100-GHz band for the 45-m radio telescope at the Nobeyama Radio Observatory, Japan. This receiver is composed of an ortho-mode transducer and two…

The Q & U Bolometric Interferometer for Cosmology, QUBIC, is an innovative experiment designed to measure the polarization of the Cosmic Microwave Background and in particular the signature left therein by the inflationary expansion of the…

Instrumentation and Methods for Astrophysics · Physics 2020-03-18 E. S. Battistelli , P. Ade , J. G. Alberro , A. Almela , G. Amico , L. H. Arnaldi , D. Auguste , J. Aumont , S. Azzoni , S. Banfi , P. Battaglia , A. Baù , B. Bèlier , D. Bennett , L. Bergè , J. -Ph. Bernard , M. Bersanelli , M. -A. Bigot-Sazy , N. Bleurvacq , J. Bonaparte , J. Bonis , A. Bottani , E. Bunn , D. Burke , D. Buzi , A. Buzzelli , F. Cavaliere , P. Chanial , C. Chapron , R. Charlassier , F. Columbro , G. Coppi , A. Coppolecchia , G. D'Alessandro , P. de Bernardis , G. De Gasperis , M. De Leo , M. De Petris , S. Dheilly , A. Di Donato , L. Dumoulin , A. Etchegoyen , A. Fasciszewski , L. P. Ferreyro , D. Fracchia , C. Franceschet , M. M. Gamboa Lerena , K. Ganga , B. Garcìa , M. E. Garcìa Redondo , M. Gaspard , A. Gault , D. Gayer , M. Gervasi , M. Giard , V. Gilles , Y. Giraud-Heraud , M. Gòmez Berisso , M. Gonzàlez , M. Gradziel , L. Grandsire , J. -Ch. Hamilton , D. Harari , V. Haynes , S. Henrot-Versillè , D. T. Hoang , F. Incardona , E. Jules , J. Kaplan , A. Korotkov , C. Kristukat , L. Lamagna , S. Loucatos , T. Louis , R. Luterstein , B. Maffei , S. Marnieros , W. Marty , S. Masi , A. Mattei , A. May , M. McCulloch , M. C. Medina , L. Mele , S. Melhuish , A. Mennella , L. Montier , L. Mousset , L. M. Mundo , J. A. Murphy , J. D. Murphy , F. Nati , E. Olivieri , C. Oriol , C. O'Sullivan , A. Paiella , F. Pajot , A. Passerini , H. Pastoriza , A. Pelosi , C. Perbost , M. Perciballi , F. Pezzotta , F. Piacentini , M. Piat , L. Piccirillo , G. Pisano , M. Platino , G. Polenta , D. Prèle , R. Puddu , D. Rambaud , P. Ringegni , G. E. Romero , M. Salatino , J. M. Salum , A. Schillaci , C. Scòccola , S. Scully , S. Spinelli , G. Stankowiak , M. Stolpovskiy , F. Suarez , A. Tartari , J. -P. Thermeau , P. Timbie , M. Tomasi , S. Torchinsky , M. Tristram , C. Tucker , G. Tucker , S. Vanneste , D. Viganò , N. Vittorio , F. Voisin , B. Watson , F. Wicek , M. Zannoni , A. Zullo

POLAR is a dedicated Gamma-Ray Burst polarimeter making use of Compton-scattering which took data from the second Chinese spacelab, the Tiangong-2 from September 2016 to April 2017. It has a wide Field of View of $\sim6$ steradians and an…

High Energy Astrophysical Phenomena · Physics 2022-09-21 Hancheng Li , POLAR Collaboration

We describe an on-sky demonstration of a microwave-multiplexing readout system in one of the receivers of the Keck Array, a polarimetry experiment observing the cosmic microwave background at the South Pole. During the austral summer of…

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;…

Instrumentation and Methods for Astrophysics · Physics 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

Current large-aperture cosmic microwave background (CMB) telescopes have nearly maximized the number of detectors that can be illuminated while maintaining diffraction-limited image quality. The polarization-sensitive detector arrays being…

Instrumentation and Methods for Astrophysics · Physics 2016-04-20 Michael D. Niemack

The Simons Observatory (SO) is a ground-based cosmic microwave background instrument to be sited in the Atacama Desert in Chile. SO will deploy 60,000 transition-edge sensor bolometers in 49 separate focal-plane modules across a suite of…

Fulfilling the science goals of the Simons Observatory, a state-of-the-art cosmic microwave background (CMB) experiment, has required deploying tens of thousands of superconducting bolometers. Reading out data from the observatory's more…

Instrumentation and Methods for Astrophysics · Physics 2026-02-12 Thomas P. Satterthwaite , Zeeshan Ahmed , Cody J. Duell , Shawn W. Henderson , Tristan Pinsonneault-Marotte , Max Silva-Feaver , Yuhan Wang

Taurus is a balloon-borne cosmic microwave background (CMB) experiment optimized to map the E-mode polarization and Galactic foregrounds at the largest angular scales ($\ell$ $\lt$ 30) and improve measurements of the optical depth to…

The Atacama Cosmology Telescope Polarimeter (ACTPol) is a polarization sensitive upgrade to the Atacama Cosmology Telescope. Located at an elevation of 5190 m, ACTPol measures the Cosmic Microwave Background (CMB) temperature and…

Advanced ACTPol (AdvACT) is a third generation polarization upgrade to the Atacama Cosmology Telescope, designed to observe the cosmic microwave background (CMB). AdvACT expands on the 90 and 150 GHz transition edge sensor (TES) bolometer…