E
Erminia Calabrese
Researcher at Cardiff University
Publications - 313
Citations - 96285
Erminia Calabrese is an academic researcher from Cardiff University. The author has contributed to research in topics: Cosmic microwave background & Planck. The author has an hindex of 105, co-authored 287 publications receiving 82143 citations. Previous affiliations of Erminia Calabrese include Sapienza University of Rome & University of Oxford.
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In-flight polarization angle calibration for LiteBIRD: blind challenge and cosmological implications
Nicoletta Krachmalnicoff,Tomotake Matsumura,Elena de la Hoz,Soumen Basak,Alessandro Gruppuso,Yuto Minami,Carlo Baccigalupi,Eiichiro Komatsu,Enrique Martínez-González,P. Vielva,Jonathan Aumont,R. Aurlien,S. Azzoni,A. J. Banday,R. B. Barreiro,Nicola Bartolo,Marco Bersanelli,Erminia Calabrese,Alessandro Carones,F. J. Casas,K. Cheung,Yuji Chinone,F. Columbro,Paolo de Bernardis,Patricia Diego-Palazuelos,Josquin Errard,Fabio Finelli,U. Fuskeland,M. Galloway,Ricardo Genova-Santos,Martina Gerbino,T. Ghigna,Serena Giardiello,Eirik Gjerløw,Masashi Hazumi,Sophie Henrot-Versille,Theodore Kisner,Luca Lamagna,Massimiliano Lattanzi,François Levrier,Gemma Luzzi,Davide Maino,Silvia Masi,M. Migliaccio,L. Montier,Gianluca Morgante,Baptiste Mot,Ryo Nagata,Federico Nati,Paolo Natoli,Luca Pagano,Alessandro Paiella,Daniela Paoletti,Guillaume Patanchon,F. Piacentini,Gianluca Polenta,Davide Poletti,Mathieu Remazeilles,Jose Alberto Rubino-Martin,Manami Sasaki,Maresuke Shiraishi,Giovanni Signorelli,Samantha Stever,Andrea Tartari,Matthieu Tristram,Masatoshi Tsuji,Léo Vacher,Ingunn Kathrine Wehus,Mario Zannoni +68 more
TL;DR: In this paper, the in-flight angle calibration for the JAXA/ISAS second strategic large class mission, LiteBIRD, and estimate its impact on the measurement of the tensor-to-scalar ratio parameter, r, using simulated data.
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The Atacama Cosmology Telescope: Microwave Intensity and Polarization Maps of the Galactic Center
Yilun Guan,Susan E. Clark,Brandon S. Hensley,Patricio A. Gallardo,Sigurd Naess,Cody J. Duell,Simone Aiola,Zachary Atkins,Erminia Calabrese,Steve K. Choi,Nicholas F. Cothard,Mark J. Devlin,Adriaan J. Duivenvoorden,Jo Dunkley,Rolando Dünner,Simone Ferraro,Simone Ferraro,Matthew Hasselfield,John P. Hughes,Brian J. Koopman,Arthur Kosowsky,Mathew S. Madhavacheril,Jeff McMahon,Federico Nati,Michael D. Niemack,Lyman A. Page,Maria Salatino,Emmanuel Schaan,Emmanuel Schaan,Neelima Sehgal,Cristóbal Sifón,Suzanne T. Staggs,Eve M. Vavagiakis,Edward J. Wollack,Zhilei Xu,Zhilei Xu +35 more
TL;DR: In this article, the Atacama Cosmology Telescope (ACT) was used to obtain arcminute-resolution intensity and polarization maps of the Galactic center made with the ACT at 98, 150, and 224 GHz.
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Concept Study of Optical Configurations for High-Frequency Telescope for LiteBIRD
T. Hasebe,Shingo Kashima,Peter A. R. Ade,Y. Akiba,David Alonso,Kam Arnold,Jonathan Aumont,Carlo Baccigalupi,Darcy Barron,Soumen Basak,Soumen Basak,S. Beckman,Julian Borrill,Julian Borrill,F. Boulanger,M. Bucher,Erminia Calabrese,Yuji Chinone,Yuji Chinone,H. M. Cho,A. Cukierman,D. W. Curtis,T. de Haan,M. A. Dobbs,A. Dominjon,Tadayasu Dotani,L. Duband,A. Ducout,Jo Dunkley,Jo Dunkley,J. M. Duval,Tucker Elleflot,H. K. Eriksen,Josquin Errard,J. Fischer,T. Fujino,T. Funaki,U. Fuskeland,K. Ganga,Neil Goeckner-Wald,J. Grain,N. W. Halverson,T. Hamada,Masaya Hasegawa,Kaori Hattori,Makoto Hattori,L. Hayes,Masashi Hazumi,N. Hidehira,Charles A. Hill,Charles A. Hill,Gene C. Hilton,Johannes Hubmayr,Kiyotomo Ichiki,Toshiaki Iida,H. Imada,M. Inoue,Yuki Inoue,Kent D. Irwin,Hirokazu Ishino,Oliver Jeong,H. Kanai,D. Kaneko,N. Katayama,T. Kawasaki,S. A. Kernasovskiy,Reijo Keskitalo,Reijo Keskitalo,A. Kibayashi,Y. Kida,Kimihiro Kimura,Theodore Kisner,Theodore Kisner,Kazunori Kohri,Eiichiro Komatsu,K. Komatsu,C. L. Kuo,Noah Kurinsky,Akito Kusaka,Akito Kusaka,Alex Lazarian,Aaron Lee,Aaron Lee,Dale Li,Eric V. Linder,Eric V. Linder,Bruno Maffei,Anna Mangilli,M. Maki,Tomotake Matsumura,Shuji Matsuura,D. Meilhan,Satoru Mima,Yuto Minami,Kazuhisa Mitsuda,L. Montier,M. Nagai,T. Nagasaki,R. Nagata,M. Nakajima,Shogo Nakamura,Toshiya Namikawa,Masato Naruse,H. Nishino,Tom Nitta,Takashi Noguchi,Hideo Ogawa,Shugo Oguri,Norio Okada,Atsushi Okamoto,Takahiro Okamura,Chiko Otani,G. Patanchon,Giampaolo Pisano,Gabriel M. Rebeiz,Mathieu Remazeilles,Paul L. Richards,Shin-ichiro Sakai,Yuki Sakurai,Y. Sato,N. Sato,Makoto Sawada,Y. Segawa,Yutaro Sekimoto,Yutaro Sekimoto,Uroš Seljak,Blake D. Sherwin,Blake D. Sherwin,Toshifumi Shimizu,Keisuke Shinozaki,R. Stompor,Hajime Sugai,Hiroyuki Sugita,Aritoki Suzuki,Jun-ichi Suzuki,Osamu Tajima,Suguru Takada,R. Takaku,S. Takakura,S. Takatori,D. Tanabe,E. Taylor,K. L. Thompson,B. Thorne,B. Thorne,Takayuki Tomaru,T. Tomida,N. Tomita,M. Tristram,Carole Tucker,Paul Turin,Masahiro Tsujimoto,S. Uozumi,Shin Utsunomiya,Yoshinori Uzawa,F. Vansyngel,Ingunn Kathrine Wehus,Benjamin Westbrook,M. Willer,Nathan Whitehorn,Yasuhiro Yamada,Ryo Yamamoto,Noriko Y. Yamasaki,T. Yamashita,Mitsuhiro Yoshida +164 more
TL;DR: In this paper, the anti-reflection (AR) coating on the lens for the refractive option is derived and the simulation result of a sub-wavelength AR structure on both surfaces of silicon, which shows a band-averaged reflection of 1.1-3.2% at 101-448 GHz.
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The Simons Observatory: gain, bandpass and polarization-angle calibration requirements for B-mode searches
Maximilian H. Abitbol,David Alonso,Sara M. Simon,Jack Lashner,Kevin T. Crowley,Aamir Ali,S. Azzoni,Carlo Baccigalupi,Darcy Barron,Michael L. Brown,Erminia Calabrese,Julien Carron,Yuji Chinone,Yuji Chinone,Jens Chluba,Gabriele Coppi,Kevin D. Crowley,Mark J. Devlin,Jo Dunkley,Josquin Errard,Valentina Fanfani,Nicholas Galitzki,Martina Gerbino,J. Colin Hill,J. Colin Hill,Bradley R. Johnson,Baptiste Jost,Brian Keating,Nicoletta Krachmalnicoff,Akito Kusaka,Adrian T. Lee,Thibaut Louis,Mathew S. Madhavacheril,Heather McCarrick,Jeff McMahon,P. Daniel Meerburg,Federico Nati,Haruki Nishino,Lyman A. Page,Davide Poletti,Giuseppe Puglisi,Giuseppe Puglisi,Michael J. Randall,Aditya Rotti,Jacob Spisak,Aritoki Suzuki,Grant Teply,Clara Vergès,Edward J. Wollack,Zhilei Xu,Zhilei Xu,Mario Zannoni +51 more
TL;DR: In this paper, the authors quantify the calibration requirements for systematic uncertainties for next-generation ground-based observatories targeting the large-angle B-mode polarization of the Cosmic Microwave Background, with a focus on the Simons Observatory (SO).
Journal ArticleDOI
Polarization angle requirements for CMB B-mode experiments. Application to the LiteBIRD satellite
P. Vielva,E. Mart'inez-Gonz'alez,F. J. Casas,Tomotake Matsumura,Sophie Henrot-Versille,Eiichiro Komatsu,J. Aumont,R. Aurlien,Carlo Baccigalupi,A. J. Banday,R. B. Barreiro,N. Bartolo,Erminia Calabrese,K. Cheung,F. Columbro,Alessandro Coppolecchia,P. de Bernardis,T. de Haan,Enrique De La Hoz,Marco De Petris,S. Della Torre,P. Diego-Palazuelos,H. K. Eriksen,Josquin Errard,Fabio Finelli,Cristian Franceschet,Unni Irene Fuskeland,Matt Galloway,K. Ganga,Massimo Gervasi,Ricardo Genova-Santos,T. Ghigna,E. Gjerløw,Alessandro Gruppuso,Masashi Hazumi,D. Herranz,E. Hivon,Kumiko Kohri,Luca Lamagna,Christophe Leloup,J. F. Macías-Pérez,Silvia Masi,Frederick Matsuda,Gianluca Morgante,Ryo Nakano,Federico Nati,Paolo Natoli,S. Nerval,Kiyoyuki Odagiri,Shugo Oguri,L. Pagano,Alessandro Paiella,Daniela Paoletti,F. Piacentini,G. Polenta,Giuseppina Emma Puglisi,Mathieu Remazeilles,A. Ritacco,Jose Alberto Rubino-Martin,Douglas Scott,Yusuke Sekimoto,Mitsuaki Shiraishi,Giovanni Signorelli,S. Takakura,Andrea Tartari,K. L. Thompson,M. Tristram,Luc Vacher,Nicola Vittorio,Ingunn Kathrine Wehus,Mario Zannoni +70 more
TL;DR: In this article , the uncertainties in the polarization angle of each detector set are related to a given bias on the tensor-to-scalar ratio r parameter, and a methodology to provide the requirements for different sets of detectors, at a given frequency of a CMB polarization experiment is presented.