K
K. Ebisawa
Researcher at Japan Aerospace Exploration Agency
Publications - 65
Citations - 1292
K. Ebisawa is an academic researcher from Japan Aerospace Exploration Agency. The author has contributed to research in topics: Gamma ray & Cosmic ray. The author has an hindex of 16, co-authored 65 publications receiving 969 citations.
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Journal ArticleDOI
Extended Measurement of the Cosmic-Ray Electron and Positron Spectrum from 11 GeV to 4.8 TeV with the Calorimetric Electron Telescope on the International Space Station.
O. Adriani,Y. Akaike,Katsuaki Asano,Yoichi Asaoka,Maria Grazia Bagliesi,Eugenio Berti,Gabriele Bigongiari,W. R. Binns,S. Bonechi,M. Bongi,Paolo Brogi,J. H. Buckley,N. Cannady,G. Castellini,C. Checchia,Michael Cherry,G. Collazuol,V. Di Felice,K. Ebisawa,H. Fuke,T. G. Guzik,T. Hams,M. Hareyama,N. Hasebe,K. Hibino,M. Ichimura,Kunihito Ioka,W. Ishizaki,M. H. Israel,K. Kasahara,J. Kataoka,Ryuho Kataoka,Y. Katayose,Chihiro Kato,Norita Kawanaka,Y. Kawakubo,Kazunori Kohri,Henric Krawczynski,J. F. Krizmanic,T. Lomtadze,Paolo Maestro,P. S. Marrocchesi,A. M. Messineo,John Mitchell,S. Miyake,A. A. Moiseev,K. Mori,Masaki Mori,N. Mori,Holger Motz,Kazuoki Munakata,H. Murakami,Satoshi Nakahira,J. Nishimura,G. A. de Nolfo,S. Okuno,J. F. Ormes,S. Ozawa,L. Pacini,F. Palma,P. Papini,A. V. Penacchioni,Brian Rauch,S. B. Ricciarini,K. Sakai,T. Sakamoto,M. Sasaki,Y. Shimizu,A. Shiomi,R. Sparvoli,P. Spillantini,F. Stolzi,J. E. Suh,A. Sulaj,I. Takahashi,M. Takayanagi,Masato Takita,T. Tamura,N. Tateyama,Toshio Terasawa,H. Tomida,Shoji Torii,Y. Tsunesada,Y. Uchihori,Seiya Ueno,E. Vannuccini,J. P. Wefel,Kazutaka Yamaoka,S. Yanagita,A. Yoshida,Kenji Yoshida +90 more
TL;DR: The measured all-electron flux, including statistical errors and a detailed breakdown of the systematic errors, is tabulated in the Supplemental Material in order to allow more refined spectral analyses based on the data.
Journal ArticleDOI
Energy Spectrum of Cosmic-Ray Electron and Positron from 10 GeV to 3 TeV Observed with the Calorimetric Electron Telescope on the International Space Station
O. Adriani,Y. Akaike,Katsuaki Asano,Yoichi Asaoka,Maria Grazia Bagliesi,Gabriele Bigongiari,W. R. Binns,S. Bonechi,M. Bongi,Paolo Brogi,J. H. Buckley,N. Cannady,G. Castellini,C. Checchia,Michael Cherry,G. Collazuol,V. Di Felice,K. Ebisawa,H. Fuke,T. G. Guzik,T. Hams,M. Hareyama,N. Hasebe,K. Hibino,M. Ichimura,Kunihito Ioka,W. Ishizaki,M. H. Israel,A. Javaid,K. Kasahara,J. Kataoka,Ryuho Kataoka,Y. Katayose,Chihiro Kato,Norita Kawanaka,Y. Kawakubo,Henric Krawczynski,J. F. Krizmanic,Shuichi Kuramata,T. Lomtadze,Paolo Maestro,P. S. Marrocchesi,A. M. Messineo,John Mitchell,S. Miyake,K. Mizutani,A. A. Moiseev,K. Mori,Masaki Mori,N. Mori,Holger Motz,Kazuoki Munakata,H. Murakami,Satoshi Nakahira,J. Nishimura,G. A. de Nolfo,S. Okuno,J. F. Ormes,S. Ozawa,L. Pacini,F. Palma,P. Papini,A. V. Penacchioni,Brian Rauch,S. B. Ricciarini,K. Sakai,T. Sakamoto,M. Sasaki,Y. Shimizu,A. Shiomi,R. Sparvoli,P. Spillantini,F. Stolzi,I. Takahashi,M. Takayanagi,Masato Takita,T. Tamura,N. Tateyama,Toshio Terasawa,H. Tomida,Shoji Torii,Y. Tsunesada,Y. Uchihori,Seiya Ueno,E. Vannuccini,J. P. Wefel,Kazutaka Yamaoka,S. Yanagita,A. Yoshida,Kenji Yoshida,T. Yuda +90 more
TL;DR: First results of a cosmic-ray electron and positron spectrum from 10 GeV to 3 TeV is presented based upon observations with the CALET instrument on the International Space Station starting in October, 2015.
Journal ArticleDOI
Direct Measurement of the Cosmic-Ray Proton Spectrum from 50 GeV to 10 TeV with the Calorimetric Electron Telescope on the International Space Station
O. Adriani,Y. Akaike,Y. Akaike,Katsuaki Asano,Yoichi Asaoka,Yoichi Asaoka,Maria Grazia Bagliesi,Eugenio Berti,Gabriele Bigongiari,W. R. Binns,S. Bonechi,M. Bongi,Paolo Brogi,A. Bruno,J. H. Buckley,N. Cannady,G. Castellini,C. Checchia,Michael Cherry,G. Collazuol,V. Di Felice,K. Ebisawa,H. Fuke,T. G. Guzik,T. Hams,T. Hams,N. Hasebe,K. Hibino,M. Ichimura,Kunihito Ioka,W. Ishizaki,M. H. Israel,K. Kasahara,Jun Kataoka,Ryuho Kataoka,Y. Katayose,Chihiro Kato,Norita Kawanaka,Y. Kawakubo,Y. Kawakubo,Kazunori Kohri,Henric Krawczynski,John F. Krizmanic,John F. Krizmanic,Teimuraz Lomtadze,Paolo Maestro,P. S. Marrocchesi,Alberto Messineo,John Mitchell,S. Miyake,A. A. Moiseev,A. A. Moiseev,K. Mori,K. Mori,Masaki Mori,N. Mori,Holger Motz,Kazuoki Munakata,H. Murakami,Satoshi Nakahira,Jun Nishimura,G. A. de Nolfo,S. Okuno,J. F. Ormes,S. Ozawa,L. Pacini,L. Pacini,F. Palma,P. Papini,A. V. Penacchioni,A. V. Penacchioni,Brian Rauch,S. B. Ricciarini,K. Sakai,K. Sakai,T. Sakamoto,Manami Sasaki,Manami Sasaki,Y. Shimizu,A. Shiomi,R. Sparvoli,P. Spillantini,F. Stolzi,J. E. Suh,A. Sulaj,I. Takahashi,Masahiro Takayanagi,Masato Takita,T. Tamura,Toshio Terasawa,H. Tomida,Shoji Torii,Y. Tsunesada,Y. Uchihori,Shinji Ueno,E. Vannuccini,J. P. Wefel,Kazutaka Yamaoka,Shohei Yanagita,A. Yoshida,Kenji Yoshida +100 more
TL;DR: The observed spectrum is consistent with AMS-02 but extends to nearly an order of magnitude higher energy, showing a very smooth transition of the power-law spectral index, thereby confirming the existence of spectral hardening and providing evidence of a deviation from a single power law by more than 3σ.
Proceedings ArticleDOI
LiteBIRD satellite: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization
Masashi Hazumi,P. A. R. Ade,Alexandre E. Adler,E. Allys,Kam Arnold,D. Auguste,J. Aumont,R. Aurlien,J. Austermann,Carlo Baccigalupi,A. J. Banday,R. Banjeri,R. B. Barreiro,Soumen Basak,J. A. Beall,Douglas H Beck,S. Beckman,J. Bermejo,P. de Bernardis,Marco Bersanelli,J. Bonis,Julian Borrill,Julian Borrill,F. Boulanger,S. Bounissou,M. Brilenkov,Michael L. Brown,M. Bucher,Erminia Calabrese,P. Campeti,A. Carones,F. J. Casas,Anthony Challinor,V. Chan,Karen C. Cheung,Yuji Chinone,J. F. Cliche,L. P. L. Colombo,F. Columbro,Javier Cubas,A. Cukierman,A. Cukierman,D. W. Curtis,Giuseppe D'Alessandro,Nadia Dachlythra,M. De Petris,Clive Dickinson,P. Diego-Palazuelos,M. A. Dobbs,Tadayasu Dotani,L. Duband,Shannon M. Duff,J. M. Duval,K. Ebisawa,Tucker Elleflot,H. K. Eriksen,Josquin Errard,Thomas Essinger-Hileman,Fabio Finelli,Raphael Flauger,Cristian Franceschet,U. Fuskeland,M. Galloway,K. Ganga,J. R. Gao,Ricardo Génova-Santos,Martina Gerbino,Massimo Gervasi,T. Ghigna,T. Ghigna,E. Gjerløw,Marcin Gradziel,J. Grain,Frank Grupp,A. Gruppuso,Jon E. Gudmundsson,T. de Haan,N. W. Halverson,Peter Charles Hargrave,T. Hasebe,Masaya Hasegawa,Makoto Hattori,Sophie Henrot-Versille,D. Herman,D. Herranz,Charles A. Hill,Charles A. Hill,Gene C. Hilton,Y. Hirota,E. Hivon,Renée Hlozek,Y. Hoshino,E. de la Hoz,Johannes Hubmayr,Kiyotomo Ichiki,Toshiaki Iida,H. Imada,Kosei Ishimura,Hirokazu Ishino,G. Jaehnig,T. Kaga,Shingo Kashima,N. Katayama,A. Kato,T. Kawasaki,Reijo Keskitalo,Reijo Keskitalo,Theodore Kisner,Theodore Kisner,Y. Kobayashi,Nozomu Kogiso,A. Kogut,K. Kohri,Eiichiro Komatsu,K. Komatsu,Kuniaki Konishi,Nicoletta Krachmalnicoff,I. Kreykenbohm,C. L. Kuo,A. Kushino,Luca Lamagna,Jeff Van Lanen,Massimiliano Lattanzi,Adrian T. Lee,Adrian T. Lee,C. Leloup,François Levrier,Eric V. Linder,Eric V. Linder,Thibaut Louis,Gemma Luzzi,Thierry Maciaszek,Bruno Maffei,Davide Maino,M. Maki,S. Mandelli,Enrique Martinez-Gonzalez,Silvia Masi,Tomotake Matsumura,A. Mennella,M. Migliaccio,Yuto Minami,K. Mitsuda,Joshua Montgomery,L. Montier,Gianluca Morgante,B. Mot,Yasuhiro Murata,J. A. Murphy,M. Nagai,Y. Nagano,T. Nagasaki,R. Nagata,Shogo Nakamura,Toshiya Namikawa,P. Natoli,S. Nerval,Toshiyuki Nishibori,H. Nishino,F. Noviello,Créidhe O'Sullivan,Hideo Ogawa,Shugo Oguri,Hiroyuki Ohsaki,I. S. Ohta,Norio Okada,L. Pagano,Alessandro Paiella,D. Paoletti,G. Patanchon,J. Peloton,F. Piacentini,Giampaolo Pisano,Giampaolo Pisano,G. Polenta,Davide Poletti,T. Prouvé,Giuseppe Puglisi,D. Rambaud,Christopher Raum,S. Realini,Martin Reinecke,Mathieu Remazeilles,A. Ritacco,A. Ritacco,G. Roudil,Jose Alberto Rubino-Martin,M. Russell,Haruyuki Sakurai,Yuki Sakurai,M. Sandri,Misao Sasaki,Giorgio Savini,Douglas Scott,Joseph Seibert,Yutaro Sekimoto,Blake D. Sherwin,Blake D. Sherwin,Keisuke Shinozaki,Maresuke Shiraishi,Peter Shirron,Giovanni Signorelli,Graeme Smecher,S. Stever,S. Stever,Radek Stompor,Hajime Sugai,S. Sugiyama,A. Suzuki,Jun-ichi Suzuki,T. L. Svalheim,Eric R. Switzer,Ryota Takaku,H. Takakura,S. Takakura,Y. Takase,Yasuhiro Takeda,A. Tartari,E. Taylor,Yasunori Terao,H. Thommesen,K. L. Thompson,B. Thorne,T. Toda,M. Tomasi,Mayu Tominaga,N. Trappe,M. Tristram,M. Tsuji,Masahiro Tsujimoto,Carole Tucker,Joel N. Ullom,G. Vermeulen,P. Vielva,F. Villa,Michael R. Vissers,Nicola Vittorio,Ingunn Kathrine Wehus,Jochen Weller,Jochen Weller,Benjamin Westbrook,Jörn Wilms,Berend Winter,E. J. Wollack,Noriko Y. Yamasaki,T. Yoshida,Junji Yumoto,Mario Zannoni,Andrea Zonca +248 more
TL;DR: LiteBIRD as mentioned in this paper, the Lite (Light) satellite for the study of B-mode polarization and inflation from cosmic background radiation detection, is a space mission for primordial cosmology and fundamental physics.
Journal ArticleDOI
Updated design of the CMB polarization experiment satellite LiteBIRD
Hajime Sugai,Peter A. R. Ade,Y. Akiba,David Alonso,Kam Arnold,Jonathan Aumont,J. E. Austermann,C. Baccigalupi,A. J. Banday,R. Banerji,R. B. Barreiro,Soumen Basak,J. A. Beall,S. Beckman,Marco Bersanelli,Julian Borrill,F. Boulanger,Michael L. Brown,M. Bucher,Alessandro Buzzelli,Erminia Calabrese,F. J. Casas,Anthony Challinor,V. Chan,Yuji Chinone,J. F. Cliche,F. Columbro,A. Cukierman,D. W. Curtis,P. Danto,P. de Bernardis,T. de Haan,M. De Petris,Clive Dickinson,M. A. Dobbs,Tadayasu Dotani,L. Duband,A. Ducout,Shannon M. Duff,Adriaan J. Duivenvoorden,J. M. Duval,K. Ebisawa,Tucker Elleflot,H. Enokida,H. K. Eriksen,Josquin Errard,Thomas Essinger-Hileman,Fabio Finelli,Raphael Flauger,Cristian Franceschet,U. Fuskeland,K. Ganga,Jiansong Gao,Ricardo Génova-Santos,T. Ghigna,Ana Gómez,Marcin Gradziel,J. Grain,Frank Grupp,A. Gruppuso,Jon E. Gudmundsson,N. W. Halverson,Peter Charles Hargrave,T. Hasebe,Masaya Hasegawa,Makoto Hattori,Masashi Hazumi,Sophie Henrot-Versille,D. Herranz,C. Hill,Gene C. Hilton,Y. Hirota,E. Hivon,Renée Hlozek,D. T. Hoang,J. Hubmayr,Kiyotomo Ichiki,Toshiaki Iida,H. Imada,Kosei Ishimura,Hirokazu Ishino,G. Jaehnig,M. Jones,T. Kaga,Shingo Kashima,Yousuke Kataoka,Nobuhiko Katayama,T. Kawasaki,R. Keskitalo,A. Kibayashi,T. Kikuchi,Kimihiro Kimura,Theodore Kisner,Yohei Kobayashi,Nozomu Kogiso,A. Kogut,K. Kohri,Eiichiro Komatsu,K. Komatsu,Kuniaki Konishi,N. Krachmalnicoff,C. L. Kuo,Noah Kurinsky,A. Kushino,Makoto Kuwata-Gonokami,Luca Lamagna,Massimiliano Lattanzi,Adrian T. Lee,Eric V. Linder,Bruno Maffei,Davide Maino,M. Maki,Anna Mangilli,Enrique Martinez-Gonzalez,Silvia Masi,R. Mathon,Tomotake Matsumura,A. Mennella,M. Migliaccio,Yuto Minami,K. Mistuda,D. Molinari,L. Montier,Gianluca Morgante,B. Mot,Yasuhiro Murata,J. A. Murphy,Masaaki Nagai,R. Nagata,Shogo Nakamura,T. Namikawa,P. Natoli,S. Nerva,Toshiyuki Nishibori,H. Nishino,Yasunori Nomura,F. Noviello,Créidhe O'Sullivan,H. Ochi,Hideo Ogawa,Hiroyuki Ohsaki,Izumi S. Ohta,Norio Okada,L. Pagano,Alessandro Paiella,D. Paoletti,G. Patanchon,F. Piacentini,Giampaolo Pisano,G. Polenta,D. Poletti,T. Prouvé,Giuseppe Puglisi,Damien Rambaud,Christopher Raum,S. Realini,Mathieu Remazeilles,G. Roudil,Jose Alberto Rubino-Martin,M. Russell,Haruyuki Sakurai,Yuki Sakurai,M. Sandri,Giorgio Savini,Douglas Scott,Yutaro Sekimoto,Blake D. Sherwin,Keisuke Shinozaki,Maresuke Shiraishi,Peter Shirron,G. Signorelli,Graeme Smecher,P. Spizzi,S. L. Stever,R. Stompor,S. Sugiyama,A. Suzuki,Jun-ichi Suzuki,Eric R. Switzer,Ryota Takaku,H. Takakura,S. Takakura,Yasuhiro Takeda,Angela C. Taylor,E. Taylor,Yasunori Terao,K. L. Thompson,B. Thorne,M. Tomasi,H. Tomida,Neil Trappe,M. Tristram,M. Tsuji,Masahiro Tsujimoto,Carole Tucker,J. N. Ullom,S. Uozumi,Shin Utsunomiya,J. Van Lanen,Gerard Vermeulen,P. Vielva,F. Villa,Michael R. Vissers,Nicola Vittorio,F. Voisin,Ian J. Walker,N. Watanabe,Ingunn Kathrine Wehus,Jochen Weller,Benjamin Westbrook,Benedict Tobias Winter,Edward J. Wollack,Ryo Yamamoto,Noriko Y. Yamasaki,Masato Yanagisawa,T. Yoshida,Junji Yumoto,Mario Zannoni,A. Zonca +218 more
TL;DR: LiteBIRD as discussed by the authors is a large-scale transition-edge sensors (TES) mission with a total wide frequency coverage between 34GHz and 448GHz, targeting its launch in Japanese Fiscal Year 2027 (2027FY) with JAXA's H3 rocket, which will accommodate more than 4000 TESs in focal planes of reflective low-frequency and refractive medium-and high-frequency telescopes.