文献

J-GLOBAL ID：201902265391353281   整理番号：19A0863800

望遠鏡アレイ実験の表面検出器を用いた10~18eV以上のエネルギーによる拡散光子フラックスに関する制約【JST・京大機械翻訳】

Constraints on the diffuse photon flux with energies above 10¹⁸ eV using the surface detector of the Telescope Array experiment

著者 (120件)： Abbasi R.U. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Abe M. (The Graduate School of Science and Engineering, Saitama University, Saitama, Saitama, Japan) ,  Abu-Zayyad T. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Allen M. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Azuma R. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Barcikowski E. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Belz J.W. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Bergman D.R. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Blake S.A. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Cady R. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Cheon B.G. (Department of Physics and The Research Institute of Natural Science, Hanyang University, Seongdong-gu, Seoul, South Korea) ,  Chiba J. (Department of Physics, Tokyo University of Science, Noda, Chiba, Japan) ,  Chikawa M. (Department of Physics, Kindai University, Higashi Osaka, Osaka, Japan) ,  di Matteo A. (Service de Physique Theorique, Universite Libre de Bruxelles, Brussels, Belgium) ,  Fujii T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Fujita K. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Fukushima M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Fukushima M. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan) ,  Furlich G. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Goto T. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Hanlon W. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Hayashi M. (Information Engineering Graduate School of Science and Technology, Shinshu University, Nagano, Nagano, Japan) ,  Hayashi Y. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Hayashida N. (Faculty of Engineering, Kanagawa University, Yokohama, Kanagawa, Japan) ,  Hibino K. (Faculty of Engineering, Kanagawa University, Yokohama, Kanagawa, Japan) ,  Honda K. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan) ,  Ikeda D. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Inoue N. (The Graduate School of Science and Engineering, Saitama University, Saitama, Saitama, Japan) ,  Ishii T. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan) ,  Ishimori R. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Ito H. (Astrophysical Big Bang Laboratory, RIKEN, Wako, Saitama, Japan) ,  Ivanov D. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Jeong H.M. (Department of Physics, Sungkyunkwan University, Jang-an-gu, Suwon, Korea) ,  Jeong S. (Department of Physics, Sungkyunkwan University, Jang-an-gu, Suwon, Korea) ,  Jui C.C.H. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Kadota K. (Department of Physics, Tokyo City University, Setagaya-ku, Tokyo, Japan) ,  Kakimoto F. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Kalashev O. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Kasahara K. (Advanced Research Institute for Science and Engineering, Waseda University, Shinjuku-ku, Tokyo, Japan) ,  Kawai H. (Department of Physics, Chiba University, Chiba, Chiba, Japan) ,  Kawakami S. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Kawana S. (The Graduate School of Science and Engineering, Saitama University, Saitama, Saitama, Japan) ,  Kawata K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Kido E. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Kim H.B. (Department of Physics and The Research Institute of Natural Science, Hanyang University, Seongdong-gu, Seoul, South Korea) ,  Kim J.H. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Kim J.H. (Department of Physics, School of Natural Sciences, Ulsan National Institute of Science and Technology, UNIST-gil, Ulsan, South Korea) ,  Kishigami S. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Kitamura S. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Kitamura Y. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Kuzmin V. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Kuznetsov M. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Kwon Y.J. (Department of Physics, Yonsei University, Seodaemun-gu, Seoul, South Korea) ,  Lee K.H. (Department of Physics, Sungkyunkwan University, Jang-an-gu, Suwon, Korea) ,  Lubsandorzhiev B. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Lundquist J.P. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Machida K. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan) ,  Martens K. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba, Japan) ,  Matsuyama T. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Matthews J.N. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Mayta R. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Minamino M. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Mukai K. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan) ,  Myers I. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Nagasawa K. (The Graduate School of Science and Engineering, Saitama University, Saitama, Saitama, Japan) ,  Nagataki S. (Astrophysical Big Bang Laboratory, RIKEN, Wako, Saitama, Japan) ,  Nakamura R. (Academic Assembly School of Science and Technology Institute of Engineering, Shinshu University, Nagano, Nagano, Japan) ,  Nakamura T. (Faculty of Science, Kochi University, Kochi, Kochi, Japan) ,  Nonaka T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Oda H. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Ogio S. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Ogura J. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Ohnishi M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Ohoka H. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Okuda T. (Department of Physical Sciences, Ritsumeikan University, Kusatsu, Shiga, Japan) ,  Omura Y. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Ono M. (Astrophysical Big Bang Laboratory, RIKEN, Wako, Saitama, Japan) ,  Onogi R. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Oshima A. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Ozawa S. (Advanced Research Institute for Science and Engineering, Waseda University, Shinjuku-ku, Tokyo, Japan) ,  Park I.H. (Department of Physics, Sungkyunkwan University, Jang-an-gu, Suwon, Korea) ,  Piskunov M.S. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Pshirkov M.S. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Pshirkov M.S. (Sternberg Astronomical Institute, Moscow M.V. Lomonosov State University, Moscow, Russia) ,  Remington J. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Rodriguez D.C. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Rubtsov G.I. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Ryu D. (Department of Physics, School of Natural Sciences, Ulsan National Institute of Science and Technology, UNIST-gil, Ulsan, South Korea) ,  Sagawa H. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Sahara R. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Saito K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Saito Y. (Academic Assembly School of Science and Technology Institute of Engineering, Shinshu University, Nagano, Nagano, Japan) ,  Sakaki N. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Sakurai N. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Scott L.M. (Department of Physics and Astronomy, Rutgers University - The State University of New Jersey, Piscataway, NJ, USA) ,  Seki T. (Academic Assembly School of Science and Technology Institute of Engineering, Shinshu University, Nagano, Nagano, Japan) ,  Sekino K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Shah P.D. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Shibata F. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan) ,  Shibata T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Shimodaira H. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Shin B.K. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Shin H.S. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Smith J.D. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Sokolsky P. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Stokes B.T. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Stratton S.R. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Stratton S.R. (Department of Physics and Astronomy, Rutgers University - The State University of New Jersey, Piscataway, NJ, USA) ,  Stroman T.A. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Suzawa T. (The Graduate School of Science and Engineering, Saitama University, Saitama, Saitama, Japan) ,  Takagi Y. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Takahashi Y. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Takamura M. (Department of Physics, Tokyo University of Science, Noda, Chiba, Japan) ,  Takeda M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Takeishi R. (Department of Physics, Sungkyunkwan University, Jang-an-gu, Suwon, Korea) ,  Taketa A. (Earthquake Research Institute, University of Tokyo, Bunkyo-ku, Tokyo, Japan) ,  Takita M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Tameda Y. (Department of Engineering Science, Faculty of Engineering, Osaka Electro-Communication University, Neyagawa-shi, Osaka, Japan) ,  Tanaka H. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Tanaka K. (Graduate School of Information Sciences, Hiroshima City University, Hiroshima, Hiroshima, Japan)
資料名： Astroparticle Physics  (Astroparticle Physics)
巻： 110  ページ： 8-14  発行年： 2019年 
JST資料番号： W0658A  ISSN： 0927-6505  資料種別： 逐次刊行物 (A)
記事区分： 原著論文  発行国： オランダ (NLD)  言語： 英語 (EN)

抄録/ポイント： 望遠鏡アレイ表面検出器からの9年間のデータをもつ超高エネルギー光子の探索結果を示した。大規模空気シャワーの16の再構成パラメータについて多変量分類器を構築した。これらのパラメータは,シャワーフロントの曲率と幅,横方向分布関数の急峻さ,およびシャワーのミュオン含有量に敏感な波形のタイミングパラメータに関連している。探索において見出された2つの光子候補の総数は,期待されるバックグラウンドと完全に互換性がある。10~18.0,10~18.5,10~19.0,10~19.5および10~20.0eVのエネルギーをもつ光子の拡散流束に対する95%CL限界は,対応して0.067,0.012,0.0036,0.0013,0.0013km-2yr-1sr-1のレベルに設定された。Copyright 2019 Elsevier B.V., Amsterdam. All rights reserved. Translated from English into Japanese by JST.【JST・京大機械翻訳】

シソーラス用語： 分布関数 ,  *望遠鏡 ,  空気シャワー ,  *光子 ,  再構成 ,  *検出器 ,  互換性 ,  曲率 ,  シャワー
準シソーラス用語： 多変量 ,  高エネルギー , 【Automatic Indexing@JST】

著者キーワード (3件)： 超高エネルギー光子 ,  望遠鏡アレイ実験 ,  広範囲空気シャワー

分類 (3件)： 人体の汚染及び防止  (MB02020Z) ,  モジュレーションと地球物理学的効果  (DB02030B) ,  環境の汚染及び防止  (MB02030K)

タイトルに関連する用語 (9件)： 望遠鏡 ,  アレイ ,  実験 ,  検出器 ,  エネルギー ,  拡散 ,  光子 ,  フラックス ,  制約