相关论文: The Simons Observatory: Large Diameter and Large L…

The Simons Observatory microwave SQUID multiplexing detector module design

Advances in cosmic microwave background (CMB) science depend on increasing the number of sensitive detectors observing the sky. New instruments deploy large arrays of superconducting transition-edge sensor (TES) bolometers tiled densely…

天体物理仪器与方法 · 物理学 2021-12-03 Heather McCarrick , Erin Healy , Zeeshan Ahmed , Kam Arnold , Zachary Atkins , Jason E. Austermann , Tanay Bhandarkar , Jim A. Beall , Sarah Marie Bruno , Steve K. Choi , Jake Connors , Nicholas F. Cothard , Kevin D. Crowley , Simon Dicker , Bradley Dober , Cody J. Duell , Shannon M. Duff , Daniel Dutcher , Josef C. Frisch , Nicholas Galitzki , Megan B. Gralla , Jon E. Gudmundsson , Shawn W. Henderson , Gene C. Hilton , Shuay-Pwu Patty Ho , Zachary B. Huber , Johannes Hubmayr , Jeffrey Iuliano , Bradley R. Johnson , Anna M. Kofman , Akito Kusaka , Jack Lashner , Adrian T. Lee , Yaqiong Li , Michael J. Link , Tammy J. Lucas , Marius Lungu , J. A. B. Mates , Jeffrey J. McMahon , Michael D. Niemack , John Orlowski-Scherer , Joseph Seibert , Maximiliano Silva-Feaver , Sara M. Simon , Suzanne Staggs , Aritoki Suzuki , Tomoki Terasaki , Joel N. Ullom , Eve M. Vavagiakis , Leila R. Vale , Jeff Van Lanen , Michael R. Vissers , Yuhan Wang , Edward J. Wollack , Zhilei Xu , Edward Young , Cyndia Yu , Kaiwen Zheng , Ningfeng Zhu

Optimal strategy for polarization modulation in the LSPE-SWIPE experiment

CMB B-mode experiments are required to control systematic effects with an unprecedented level of accuracy. Polarization modulation by a half wave plate (HWP) is a powerful technique able to mitigate a large number of the instrumental…

天体物理仪器与方法 · 物理学 2018-01-10 Alessandro Buzzelli , Paolo de Bernardis , Silvia Masi , Nicola Vittorio , Giancarlo de Gasperis

The Simons Observatory: Magnetic Sensitivity Measurements of Microwave SQUID Multiplexers

The Simons Observatory (SO) will be a cosmic microwave background (CMB) survey experiment with three small-aperture telescopes and one large-aperture telescope, which will observe from the Atacama Desert in Chile. In total, SO will field…

天体物理仪器与方法 · 物理学 2023-09-14 Eve M. Vavagiakis , Zeeshan Ahmed , Aamir Ali , Kam Arnold , Jason Austermann , Sarah Marie Bruno , Steve K. Choi , Jake Connors , Nicholas F. Cothard , Simon Dicker , Brad Dober , Shannon Duff , Valentina Fanfani , Erin Healy , Shawn Henderson , Shuay-Pwu Patty Ho , Duc-Thuong Hoang , Gene Hilton , Johannes Hubmayr , Nicoletta Krachmalnicoff , Yaqiong Li , John Mates , Heather McCarrick , Federico Nati , Michael Niemack , Maximiliano Silva-Feaver , Suzanne Staggs , Jason Stevens , Michael Vissers , Joel Ullom , Kasey Wagoner , Zhilei Xu , Ningfeng Zhu

The Simons Observatory: Design, Integration, and Current Status of Small Aperture Telescopes

The Simons Observatory (SO) is a cosmic microwave background (CMB) survey experiment located in the Atacama Desert in Chile at an elevation of 5200 meters, nominally consisting of an array of three 0.42-meter small aperture telescopes…

天体物理仪器与方法 · 物理学 2024-12-03 Aashrita Mangu , Lance Corbett , Sanah Bhimani , Fred Carl , Samuel Day-Weiss , Brooke DiGia , Josquin Errard , Nicholas Galitzki , Masashi Hazumi , Shawn W. Henderson , Varun Kabra , Amber Miller , Jenna Moore , Xue Song , Tran Tsan , Yuhan Wang , Andrea Zonca

The short wavelength instrument for the polarization explorer balloon-borne experiment: Polarization modulation issues

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…

天体物理仪器与方法 · 物理学 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

The Simons Observatory: Design, Optimization, and Performance of Low Frequency Detectors

The Simons Observatory (SO) is a cosmic microwave background (CMB) experiment located in the Atacama Desert in Chile that will make precise temperature and polarization measurements over six spectral bands ranging from 27 to 285 GHz. Three…

天体物理仪器与方法 · 物理学 2024-12-03 Aashrita Mangu , Benjamin Westbrook , Shawn Beckman , Lance Corbett , Kevin T. Crowley , Daniel Dutcher , Bradley R. Johnson , Adrian T. Lee , Varun Kabra , Bhoomija Prasad , Suzanne T. Staggs , Aritoki Suzuki , Yuhan Wang , Kaiwen Zheng

Calibration System with Cryogenically-Cooled Loads for CMB Polarization Detectors

We present a novel system to calibrate millimeter-wave polarimeters for CMB polarization measurements. This technique is an extension of the conventional metal mirror rotation approach, however it employs cryogenically-cooled blackbody…

天体物理仪器与方法 · 物理学 2012-05-01 M. Hasegawa , O. Tajima , Y. Chinone , M. Hazumi , K. Ishidoshiro , M. Nagai

The Simons Observatory: laboratory beam characterization for the first small aperture telescope

The Simons Observatory is a ground-based telescope array located at an elevation of 5200 meters, in the Atacama Desert in Chile, designed to measure the temperature and polarization of the cosmic microwave background. It comprises four…

天体物理仪器与方法 · 物理学 2024-11-13 Remington G. Gerras , Thomas Alford , Michael J. Randall , Joseph Seibert , Grace Chesmore , Kevin T. Crowley , Nicholas Galitzki , Jon Gudmundsson , Kathleen Harrington , Bradley R. Johnson , J. B. Lloyd , Amber D. Miller , Max Silva-Feaver

The Simons Observatory: forecasted constraints on primordial gravitational waves with the expanded array of Small Aperture Telescopes

We present updated forecasts for the scientific performance of the degree-scale (0.5 deg FWHM at 93 GHz), deep-field survey to be conducted by the Simons Observatory (SO). By 2027, the SO Small Aperture Telescope (SAT) complement will be…

宇宙学与河外天体物理 · 物理学 2025-12-19 The Simons Observatory Collaboration , I. Abril-Cabezas , S. Adachi , P. Ade , A. E. Adler , P. Agrawal , J. Aguirre , S. Aiola , T. Alford , A. Ali , D. Alonso , M. A. Alvarez , R. An , M. Aravena , K. Arnold , P. Ashton , F. Astori , Z. Atkins , J. Austermann , S. Azzoni , C. Baccigalupi , D. Baker , R. Balafendiev , A. Baleato Lizancos , D. Barron , P. Barry , J. Bartlett , A. Basyrov , N. Battaglia , E. S. Battistelli , R. Battye , A. Bayer , A. Bazarko , J. A. Beall , R. Bean , D. Beck , S. Beckman , J. Begin , A. Beheshti , B. Beringue , T. Bhandarkar , S. Bhimani , F. Bianchini , E. Biermann , M. Billi , S. Biquard , B. Bixler , L. Bizzarri , S. Boada , D. Boettger , B. Bolliet , J. R. Bond , J. Borrill , J. Borrow , C. Braithwaite , T. L. R. Brien , M. L. Brown , S. M. Bruno , S. Bryan , R. Bustos , H. Cai , E. Calabrese , V. Calafut , F. M. Carl , A. Carones , J. Carron , A. Challinor , E. Chamberlain , P. Chanial , N. Chen , K. Cheung , B. Chiang , Y. Chinone , J. Chluba , H. S. Cho , S. K. Choi , M. Chu , J. Clancy , S. E. Clark , P. Clarke , J. Cleary , D. L. Clements , J. Connors , C. Contaldi , G. Coppi , L. Corbett , N. F. Cothard , W. Coulton , D. Crichton , K. D. Crowley , K. T. Crowley , A. Cukierman , J. M. D'Ewart , K. Dachlythra , O. Darwish , R. Datta , S. Day-Weiss , T. de Haan , S. Desai , M. Devlin , L. Di Mascolo , S. Dicker , K. Ding , C. Doux , P. Dow , S. Doyle , C. J. Duell , S. M. Duff , A. J. Duivenvoorden , J. Dunkley , M. Duparc , D. Dutcher , R. Dünner , M. Edenton , H. El Bouhargani , C. Embil Villagra , J. Errard , G. Fabbian , V. Fanfani , F. Farhadi Khouzani , G. S. Farren , J. Fergusson , S. Ferraro , R. Flauger , M. Forconi , A. Foster , K. Freese , J. C. Frisch , A. Frolov , G. Fuller , N. Galitzki , P. A. Gallardo , G. Galloni , J. T. Galvez Ghersi , K. Ganga , X. Garrido , E. Gawiser , M. Gerbino , R. Gerras , S. Giardiello , A. Gill , V. Gilles , U. Giri , E. Gleave , V. Gluscevic , N. Goeckner-Wald , S. Goldstein , J. E. Golec , S. Gordon , M. Gralla , S. Gratton , D. Green , J. C. Groh , C. Groppi , S. Grubb , Y. Guan , N. Gupta , J. E. Guðmundsson , B. Hadzhiyska , S. Hagstotz , P. Hargrave , S. Haridas , K. Harrington , I. Harrison , M. Hasegawa , M. Hasselfield , V. Haynes , M. Hazumi , A. He , E. Healy , S. W. Henderson , B. S. Hensley , E. Hertig , C. Hervías-Caimapo , M. Higuchi , C. A. Hill , J. C. Hill , M. Hilton , A. D. Hincks , G. Hinshaw , R. Hložek , A. Y. Q. Ho , S. Ho , S. P. Ho , T. D. Hoang , J. Hoh , J. Holder , J. Hood , E. Hornecker , A. L. Hornsby , S. C. Hotinli , Z. Huang , Z. B. Huber , J. Hubmayr , K. Huffenberger , A. Hughes , J. P. Hughes , A. Idicherian Lonappan , M. Ikape , K. Inaba , K. Irwin , J. Iuliano , A. H. Jaffe , B. Jain , D. Jain , H. T. Jense , O. Jeong , A. Johnson , B. R. Johnson , M. Johnson , M. E. Jones , N. Joshi , B. Jost , W. Kabalan , V. Kabra , D. Kaneko , J. Kania , E. D. Karpel , Y. Kasai , N. Katayama , B. Keating , B. Keller , R. Keskitalo , A. A. Khatua , J. Kim , T. Kisner , K. Kiuchi , K. Knowles , A. M. Kofman , Y. Koizumi , B. J. Koopman , A. Kosowsky , R. Kou , N. Krachmalnicoff , D. Kramer , A. Krishak , A. Krolewski , A. Kusaka , A. Kusiak , Y. Kvasiuk , P. La Plante , A. La Posta , A. Laguë , A. Lai , J. Lashner , M. Lattanzi , A. Lee , E. Lee , J. Leech , L. Legrand , C. Lessler , J. S. Leung , A. Lewis , Y. Li , Z. Li , M. Limon , L. Lin , E. Linder , M. Link , J. Liu , Y. Liu , J. Lloyd , J. Lonergan , T. Louis , T. Lucas , M. Ludlam , M. Lungu , M. Lyons , N. MacCrann , A. MacInnis , M. Madhavacheril , D. Mak , F. Maldonado , M. Mallaby-Kay , A. Manduca , A. Mangu , H. Mani , A. S. Maniyar , G. A. Marques , P. Masson , J. Mates , J. Mathewson , T. Matsumura , P. Mauskopf , A. May , N. McCallum , H. McCarrick , F. McCarthy , M. McCulloch , J. McMahon , P. D. Meerburg , Y. Mehta , J. Melin , E. Meulbroek , J. Meyers , A. Middleton , Y. Miki , A. Miller , M. Mirmelstein , Y. Mizozoe , B. Mohammadian , G. Montefalcone , K. Moodley , J. Moore , T. Morris , M. Morshed , T. Morton , E. Moser , T. Mroczkowski , M. Murata , J. Myers , M. Münchmeyer , S. Naess , H. Nakata , T. Namikawa , M. Nashimoto , F. Nati , P. Natoli , M. Negrello , S. K. Nerval , L. Newburgh , D. V. Nguyen , A. Nicola , M. D. Niemack , H. Nishino , Y. Nishinomiya , A. Novelli , S. O'Neill , N. Okumoto , A. Orlando , J. Orlowski-Scherer , L. Pagano , L. A. Page , S. Pandey , A. Papageorgiou , I. Paraskevakos , B. Partridge , D. Patel , R. Patki , S. Paulino Korte , M. Peel , K. Perez Sarmiento , F. Perrotta , P. Phakathi , L. Piccirillo , E. Pierpaoli , T. Pinsonneault-Marotte , G. Pisano , J. Pitocco , D. Poletti , C. Popik , B. Prasad , R. Puddu , G. Puglisi , F. J. Qu , F. Rahman , M. J. Randall , C. Ranucci , C. Raum , R. Reeves , C. L. Reichardt , M. Remazeilles , X. Ren , Y. Rephaeli , D. Riechers , B. Reid Guachalla , A. Rizzieri , J. Robe , M. F. Robertson , N. Robertson , K. Rogers , F. Rojas , A. Romero , E. Rosenberg , A. Rotti , S. Rowe , A. Roy , S. Sadeh , N. Sailer , K. Sakaguri , T. Sakuma , Y. Sakurai , M. Salatino , G. H. Sanders , D. Sasaki , M. Sathyanarayana Rao , T. P. Satterthwaite , L. Saunders , L. Scalcinati , E. Schaan , B. Schmitt , M. Schmittfull , N. Sehgal , J. Seibert , Y. Seino , U. Seljak , S. Shaikh , E. Shaw , P. Shellard , B. Sherwin , M. Shimon , J. E. Shroyer , C. Sierra , J. Sievers , C. Sifón , P. Sikhosana , M. Silva-Feaver , S. M. Simon , A. Sinclair , K. Smith , W. Sohn , X. Song , R. F. Sonka , T. Souverin , J. Spisak , S. T. Staggs , G. Stein , J. R. Stevens , R. Stompor , E. Storer , R. Sudiwala , Y. Sueno , J. Sugiyama , P. Suman , K. M. Surrao , S. Sutariya , A. Suzuki , J. Suzuki , O. Tajima , R. Takaku , S. Takakura , A. Takeuchi , I. Tansieri , A. C. Taylor , G. Teply , T. Terasaki , A. Thomas , D. B. Thomas , R. Thornton , P. Timbie , H. Trac , T. Tsan , E. Tsang King Sang , C. Tucker , J. Ullom , L. Vacher , L. Vale , A. van Engelen , J. Van Lanen , J. van Marrewijk , D. D. Van Winkle , C. Vargas , E. M. Vavagiakis , I. Veenendaal , C. Vergès , A. Villarrubia Aguilar , M. Vissers , M. Viña , K. Wagoner , S. Walker , L. Walters , Y. Wang , B. Westbrook , J. Williams , P. Williams , J. Wilson , H. Winch , E. J. Wollack , K. Wolz , J. Wong , Z. Xu , K. Yamada , E. Young , B. Yu , C. Yu , G. Zagatti , M. Zannoni , W. Zhang , K. Zheng , N. Zhu , A. Zonca , I. Zubeldia

Impact of half-wave plate systematics on the measurement of CMB $B$-mode polarization

Polarization of the cosmic microwave background (CMB) can help probe the fundamental physics behind cosmic inflation via the measurement of primordial $B$ modes. As this requires exquisite control over instrumental systematics, some…

宇宙学与河外天体物理 · 物理学 2024-05-06 Marta Monelli , Eiichiro Komatsu , Tommaso Ghigna , Tomotake Matsumura , Giampaolo Pisano , Ryota Takaku

Calibration of detector time constant with a thermal source for the POLARBEAR-2A CMB polarization experiment

The Simons Array (SA) project is a ground-based Cosmic Microwave Background (CMB) polarization experiment. The SA observes the sky using three telescopes, and POLARBEAR-2A (PB-2A) is the receiver system on the first telescope. For the…

天体物理仪器与方法 · 物理学 2024-12-31 S. Takatori , M. Hasegawa , M. Hazumi , D. Kaneko , N. Katayama , A. T. Lee , S. Takakura , T. Tomaru , T. Adkins , D. Barron , Y. Chinone , K. T. Crowley , T. de Haan , T. Elleflot , N. Farias , C. Feng , T. Fujino , J. C. Groh , H. Hirose , F. Matsuda , H. Nishino , Y. Segawa , P. Siritanasak , A. Suzuki , K. Yamada

Optimization of the half wave plate configuration for the LSPE-SWIPE experiment

The search for the B-mode polarization of Cosmic Microwave Background (CMB) is the new frontier of observational Cosmology. A B-mode detection would give an ultimate confirmation to the existence of a primordial Gravitational Wave (GW)…

天体物理仪器与方法 · 物理学 2017-09-15 Alessandro Buzzelli , Giancarlo de Gasperis , Paolo de Bernardis , Silvia Masi , Nicola Vittorio

Testbed preparation of a small prototype polarization modulator for LiteBIRD low-frequency telescope

LiteBIRD is the Cosmic Microwave Background (CMB) radiation polarization satellite mission led by ISAS/JAXA. The main scientific goal is to search for primordial gravitational wave signals generated from the inflation epoch of the Universe.…

天体物理仪器与方法 · 物理学 2022-08-09 Thuong D. Hoang , Tomotake Matsumura , Ryota Takaku , Takashi Hasebe , Tommaso Ghigna , Nobuhiko Katayama , Yuki Sakurai , Kunimoto Komatsu , Teruhito Iida , Yurika Hoshino , Shinya Sugiyama , Hirokazu Ishino

The Simons Observatory: Magnetic Shielding Measurements for the Universal Multiplexing Module

The Simons Observatory (SO) includes four telescopes that will measure the temperature and polarization of the cosmic microwave background using over 60,000 highly sensitive transition-edge bolometers (TES). These multichroic TES bolometers…

天体物理仪器与方法 · 物理学 2023-03-03 Zachary B. Huber , Yaqiong Li , Eve M. Vavagiakis , Steve K. Choi , Jake Connors , Nicholas F. Cothard , Cody J. Duell , Nicholas Galitzki , Erin Healy , Johannes Hubmayr , Bradley R. Johnson , Benjamin Keller , Heather McCarrick , Michael D. Niemack , Yuhan Wang , Zhilei Xu , Kaiwen Zheng

The Simons Observatory: Combining delensing and foreground cleaning for improved constraints on inflation

The Simons Observatory (SO), a next-generation ground-based CMB experiment in its final stages of construction, will target primordial $B$-modes with unprecedented sensitivity to set tight bounds on the amplitude of inflationary…

宇宙学与河外天体物理 · 物理学 2024-05-24 Emilie Hertig , Kevin Wolz , Toshiya Namikawa , Antón Baleato Lizancos , Susanna Azzoni , Anthony Challinor

Vibration characteristics of a continuously rotating superconducting magnetic bearing and potential influence to TES and SQUID

We measured the vibration of a prototype superconducting magnetic bearing (SMB) operating at liquid nitrogen temperature. This prototype system was designed as a breadboard model for LiteBIRD low-frequency telescope (LFT) polarization…

仪器与探测器 · 物理学 2022-10-25 Shinya Sugiyama , Tommaso Ghigna , Yurika Hoshino , Nobuhiko Katayama , Satoru Katsuda , Kunimoto Komatsu , Tomotake Matsumura , Yuki Sakurai , Kosuke Sato , Ryota Takaku , Makoto Tashiro , Yukikatsu Terada

A Measurement of the Cosmic Microwave Background Gravitational Lensing Potential from 100 Square Degrees of SPTpol Data

We present a measurement of the cosmic microwave background (CMB) gravitational lensing potential using data from the first two seasons of observations with SPTpol, the polarization-sensitive receiver currently installed on the South Pole…

宇宙学与河外天体物理 · 物理学 2015-09-16 K. T. Story , D. Hanson , P. A. R. Ade , K. A. Aird , J. E. Austermann , J. A. Beall , A. N. Bender , B. A. Benson , L. E. Bleem , J. E. Carlstrom , C. L. Chang , H. C. Chiang , H-M. Cho , R. Citron , T. M. Crawford , A. T. Crites , T. de Haan , M. A. Dobbs , W. Everett , J. Gallicchio , J. Gao , E. M. George , A. Gilbert , N. W. Halverson , N. Harrington , J. W. Henning , G. C. Hilton , G. P. Holder , W. L. Holzapfel , S. Hoover , Z. Hou , J. D. Hrubes , N. Huang , J. Hubmayr , K. D. Irwin , R. Keisler , L. Knox , A. T. Lee , E. M. Leitch , D. Li , C. Liang , D. Luong-Van , J. J. McMahon , J. Mehl , S. S. Meyer , L. Mocanu , T. E. Montroy , T. Natoli , J. P. Nibarger , V. Novosad , S. Padin , C. Pryke , C. L. Reichardt , J. E. Ruhl , B. R. Saliwanchik , J. T. Sayre , K. K. Schaffer , G. Smecher , A. A. Stark , C. Tucker , K. Vanderlinde , J. D. Vieira , G. Wang , N. Whitehorn , V. Yefremenko , O. Zahn

Construction of a Large Diameter Reflective Half-Wave Plate Modulator for Millimeter Wave Applications

Polarization modulation is a powerful technique to increase the stability of measurements by enabling the distinction of a polarized signal from dominant slow system drifts and unpolarized foregrounds. Furthermore, when placed as close to…

天体物理仪器与方法 · 物理学 2022-08-12 Joseph R. Eimer , Michael K. Brewer , David T. Chuss , John Karakla , Rui Shi , John W. Appel , Charles L. Bennett , Joseph Cleary , Sumit Dahal , Rahul Datta , Thomas Essinger-Hileman , Tobias A. Marriage , Carolina Núñez , Matthew A. Petroff , Duncan J. Watts , Edward J. Wollack , Zhilei Xu

Testing magnetic interference between TES detectors and the telescope environment for future CMB satellite missions

The two most common components of several upcoming CMB experiments are large arrays of superconductive TES (Transition-Edge Sensor) detectors and polarization modulator units, e.g. continuously-rotating Half-Wave Plates (HWP). A high…

天体物理仪器与方法 · 物理学 2024-06-06 Tommaso Ghigna , Thuong Duc Hoang , Takashi Hasebe , Yurika Hoshino , Nobuhiko Katayama , Kunimoto Komatsu , Adrian Lee , Tomotake Matsumura , Yuki Sakurai , Shinya Sugiyama , Aritoki Suzuki , Christopher Raum , Ryota Takaku , Benjamin Westbrook

PROTOCALC, A W-band polarized calibrator for CMB Telescopes: application to Simons Observatory and CLASS

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…

天体物理仪器与方法 · 物理学 2025-06-02 Gabriele Coppi , Nadia Dachlythra , Federico Nati , Rolando Dünner-Planella , Alexandre E. Adler , Josquin Errard , Nicholas Galitzki , Yunyang Li , Matthew A. Petroff , Sara M. Simon , Ema Tsang King Sang , Amalia Villarrubia Aguilar , Edward J. Wollack , Mario Zannoni