抄録
We present the results of searches for gamma-ray counterparts of the LIGO/Virgo gravitational wave events using CALorimetric Electron Telescope (CALET) observations. The main instrument of CALET, CALorimeter (CAL), observes gamma-rays from ∼1 GeV up to 10 TeV with a field of view (FOV) of nearly 2 sr. In addition, the CALET gamma-ray burst monitor views ∼3 sr and ∼2π sr of the sky in the 7 keV-1 MeV and the 40 keV-20 MeV bands, respectively, by using two different crystal scintillators. The CALET observations on the International Space Station started in 2015 October, and here we report analyses of events associated with the following gravitational wave events: GW151226, GW170104, GW170608, GW170814, and GW170817. Although only upper limits on gamma-ray emission are obtained, they correspond to a luminosity of 1049 ∼ 1053 erg s-1 in the GeV energy band depending on the distance and the assumed time duration of each event, which is approximately on the order of luminosity of typical short gamma-ray bursts. This implies that there will be a favorable opportunity to detect high-energy gamma-ray emission in further observations if additional gravitational wave events with favorable geometry will occur within our FOV. We also show the sensitivity of CALET for gamma-ray transient events, which is on the order of 10-7 erg cm-2 s-1 for an observation of 100 s in duration.
| 本文言語 | English |
|---|---|
| 論文番号 | 160 |
| ジャーナル | Astrophysical Journal |
| 巻 | 863 |
| 号 | 2 |
| DOI | |
| 出版ステータス | Published - 2018 8月 20 |
ASJC Scopus subject areas
- 天文学と天体物理学
- 宇宙惑星科学
フィンガープリント
「Search for GeV Gamma-Ray Counterparts of Gravitational Wave Events by CALET」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。引用スタイル
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In: Astrophysical Journal, Vol. 863, No. 2, 160, 20.08.2018.
研究成果: Article › 査読
}
TY - JOUR
T1 - Search for GeV Gamma-Ray Counterparts of Gravitational Wave Events by CALET
AU - Adriani, O.
AU - Akaike, Y.
AU - Asano, K.
AU - Asaoka, Y.
AU - Bagliesi, M. G.
AU - Berti, E.
AU - Bigongiari, G.
AU - Binns, W. R.
AU - Bonechi, S.
AU - Bongi, M.
AU - Brogi, P.
AU - Buckley, J. H.
AU - Cannady, N.
AU - Castellini, G.
AU - Checchia, C.
AU - Cherry, M. L.
AU - Collazuol, G.
AU - Felice, V. Di
AU - Ebisawa, K.
AU - Fuke, H.
AU - Guzik, T. G.
AU - Hams, T.
AU - Hareyama, M.
AU - Hasebe, N.
AU - Hibino, K.
AU - Ichimura, M.
AU - Ioka, K.
AU - Ishizaki, W.
AU - Israel, M. H.
AU - Kasahara, K.
AU - Kataoka, J.
AU - Kataoka, R.
AU - Katayose, Y.
AU - Kato, C.
AU - Kawanaka, N.
AU - Kawakubo, Y.
AU - Krawczynski, H. S.
AU - Krizmanic, J. F.
AU - Kohri, K.
AU - Lomtadze, T.
AU - Maestro, P.
AU - Marrocchesi, P. S.
AU - Messineo, A. M.
AU - Mitchell, J. W.
AU - Miyake, S.
AU - Moiseev, A. A.
AU - Mori, K.
AU - Mori, M.
AU - Mori, N.
AU - Motz, H. M.
AU - Munakata, K.
AU - Murakami, H.
AU - Nakahira, S.
AU - Nishimura, J.
AU - De Nolfo, G. A.
AU - Okuno, S.
AU - Ormes, J. F.
AU - Ozawa, S.
AU - Pacini, L.
AU - Palma, F.
AU - Papini, P.
AU - Penacchioni, A. V.
AU - Rauch, B. F.
AU - Ricciarini, S. B.
AU - Sakai, K.
AU - Sakamoto, T.
AU - Sasaki, M.
AU - Shimizu, Y.
AU - Shiomi, A.
AU - Sparvoli, R.
AU - Spillantini, P.
AU - Stolzi, F.
AU - Suh, J. E.
AU - Sulaj, A.
AU - Takahashi, I.
AU - Takayanagi, M.
AU - Takita, M.
AU - Tamura, T.
AU - Tateyama, N.
AU - Terasawa, T.
AU - Tomida, H.
AU - Torii, S.
AU - Tsunesada, Y.
AU - Uchihori, Y.
AU - Ueno, S.
AU - Vannuccini, E.
AU - Wefel, J. P.
AU - Yamaoka, K.
AU - Yanagita, S.
AU - Yoshida, A.
AU - Yoshida, K.
N1 - Funding Information: 1Department of Physics, University of Florence, Via Sansone, 1 I-50019 Sesto, Fiorentino, Italy 2INFN Sezione di Florence, Via Sansone, 1 I-50019 Sesto, Fiorentino, Italy 3Department of Physics, University of Maryland, Baltimore County, 1000 Hilltop Circle, Baltimore, MD 21250, USA 4Astroparticle Physics Laboratory, NASA/GSFC, Greenbelt, MD 20771, USA 5Institute for Cosmic Ray Research, The University of Tokyo, 5-1-5 Kashiwa-no-Ha, Kashiwa, Chiba 277-8582, Japan 6Waseda Research Institute for Science and Engineering, Waseda University, 3-4-1 Okubo, Shinjuku, Tokyo 169-8555, Japan; yoichi.asaoka@aoni.waseda.jp 7JEM Utilization Center, Human Spaceflight Technology Directorate, Japan Aerospace Exploration Agency, 2-1-1 Sengen, Tsukuba, Ibaraki 305-8505, Japan 8Department of Physical Sciences, Earth and Environment, University of Siena, via Roma 56, I-53100 Siena, Italy 9INFN Sezione di Pisa, Polo Fibonacci, Largo B. Pontecorvo, 3 I-56127 Pisa, Italy 10Department of Physics, Washington University, One Brookings Drive, St. Louis, MO 63130-4899, USA 11Department of Physics and Astronomy, Louisiana State University, 202 Nicholson Hall, Baton Rouge, LA 70803, USA 12Institute of Applied Physics (IFAC), National Research Council (CNR), Via Madonna del Piano, 10, I-50019 Sesto, Fiorentino, Italy 13Department of Physics and Astronomy, University of Padova, Via Marzolo, 8, I-35131 Padova, Italy 14INFN Sezione di Padova, Via Marzolo, 8, I-35131 Padova, Italy 15University of Rome “Tor Vergata,” Via della Ricerca Scientifica 1, I-00133 Rome, Italy 16INFN Sezione di Rome “Tor Vergata,” Via della Ricerca Scientifica 1, I-00133 Rome, Italy 17Space Science Data Center—Agenzia Spaziale Italiana, via del Politecnico, s.n.c., I-00133, Roma, Italy 18Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Chuo, Sagamihara, Kanagawa 252-5210, Japan 19CRESST and Astroparticle Physics Laboratory NASA/GSFC, Greenbelt, MD 20771, USA 20St. Marianna University School of Medicine, 2-16-1, Sugao, Miyamae-ku, Kawasaki, Kanagawa 216-8511, Japan 21Kanagawa University, 3-27-1 Rokkakubashi, Kanagawa, Yokohama, Kanagawa 221-8686, Japan 22Faculty of Science and Technology, Graduate School of Science and Technology, Hirosaki University, 3, Bunkyo, Hirosaki, Aomori 036-8561, Japan 23Yukawa Institute for Theoretical Physics, Kyoto University, Kitashirakawa Oiwakecho, Sakyo, Kyoto 606-8502, Japan 24National Institute of Polar Research, 10-3, Midori-cho, Tachikawa, Tokyo 190-8518, Japan 25Faculty of Engineering, Division of Intelligent Systems Engineering, Yokohama National University, 79-5 Tokiwadai, Hodogaya, Yokohama 240-8501, Japan 26Faculty of Science, Shinshu University, 3-1-1 Asahi, Matsumoto, Nagano 390-8621, Japan 27Hakubi Center, Kyoto University, Yoshida Honmachi, Sakyo-ku, Kyoto, 606-8501, Japan 28Department of Astronomy, Graduate School of Science, Kyoto University, Kitashirakawa Oiwake-cho, Sakyo-ku, Kyoto, 606-8502, Japan 29College of Science and Engineering, Department of Physics and Mathematics, Aoyama Gakuin University, 5-10-1 Fuchinobe, Chuo, Sagamihara, Kanagawa 252-5258, Japan 30Institute of Particle and Nuclear Studies, High Energy Accelerator Research Organization, 1-1 Oho, Tsukuba, Ibaraki, 305-0801, Japan 31University of Pisa, Polo Fibonacci, Largo B. Pontecorvo, 3 I-56127 Pisa, Italy 32Department of Electrical and Electronic Systems Engineering, National Institute of Technology, Ibaraki College, 866 Nakane, Hitachinaka, Ibaraki 312-8508 Japan 33Department of Astronomy, University of Maryland, College Park, MD 20742, USA 34Department of Physical Sciences, College of Science and Engineering, Ritsumeikan University, Shiga 525-8577, Japan; morim@fc.ritsumei.ac.jp 35Global Center for Science and Engineering Programs, Waseda University, 3-4-1 Okubo, Shinjuku, Tokyo 169-8555, Japan 36RIKEN, 2-1 Hirosawa, Wako, Saitama 351-0198, Japan 37Heliospheric Physics Laboratory, NASA/GSFC, Greenbelt, MD 20771, USA 38Department of Physics and Astronomy, University of Denver, Physics Building, Room 211, 2112 East Wesley Avenue, Denver, CO 80208-6900, USA 39ASI Science Data Center (ASDC), Via del Politecnico snc, I-00133 Rome, Italy 40College of Industrial Technology, Nihon University, 1-2-1 Izumi, Narashino, Chiba 275-8575, Japan 41Kavli Institute for the Physics and Mathematics of the Universe, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, 277-8583, Japan 42School of Advanced Science and Engineering, Waseda University, 3-4-1 Okubo, Shinjuku, Tokyo 169-8555, Japan 43Division of Mathematics and Physics, Graduate School of Science, Osaka City University, 3-3-138 Sugimoto, Sumiyoshi, Osaka 558-8585, Japan 44National Institutes for Quantum and Radiation Science and Technology, 4-9-1 Anagawa, Inage, Chiba 263-8555, Japan 45Nagoya University, Furo, Chikusa, Nagoya 464-8601, Japan 46College of Science, Ibaraki University, 2-1-1 Bunkyo, Mito, Ibaraki 310-8512, Japan 47Department of Electronic Information Systems, Shibaura Institute of Technology, 307 Fukasaku, Minuma, Saitama 337-8570, Japan Funding Information: We express our sincere thanks to ASI and NASA for their support to the CALET project. This work is partially supported by JSPS Grant-in-Aid for Scientific Research (S) Number 26220708, JSPS Grant-in- Aid for Scientific Research (B) Number 17H02901, JSPS Grant-in-Aid for Scientific Research (C) Number 16K05382, and MEXT-Supported Program for the Strategic Research Foundation at Private Universities (2011-2015) S1101021 in Waseda University. This work is also supported in part by MEXT Grant-in-Aid for Scientific Research on Innovative Areas Number 24103002. Publisher Copyright: © 2018. The American Astronomical Society. All rights reserved.
PY - 2018/8/20
Y1 - 2018/8/20
N2 - We present the results of searches for gamma-ray counterparts of the LIGO/Virgo gravitational wave events using CALorimetric Electron Telescope (CALET) observations. The main instrument of CALET, CALorimeter (CAL), observes gamma-rays from ∼1 GeV up to 10 TeV with a field of view (FOV) of nearly 2 sr. In addition, the CALET gamma-ray burst monitor views ∼3 sr and ∼2π sr of the sky in the 7 keV-1 MeV and the 40 keV-20 MeV bands, respectively, by using two different crystal scintillators. The CALET observations on the International Space Station started in 2015 October, and here we report analyses of events associated with the following gravitational wave events: GW151226, GW170104, GW170608, GW170814, and GW170817. Although only upper limits on gamma-ray emission are obtained, they correspond to a luminosity of 1049 ∼ 1053 erg s-1 in the GeV energy band depending on the distance and the assumed time duration of each event, which is approximately on the order of luminosity of typical short gamma-ray bursts. This implies that there will be a favorable opportunity to detect high-energy gamma-ray emission in further observations if additional gravitational wave events with favorable geometry will occur within our FOV. We also show the sensitivity of CALET for gamma-ray transient events, which is on the order of 10-7 erg cm-2 s-1 for an observation of 100 s in duration.
AB - We present the results of searches for gamma-ray counterparts of the LIGO/Virgo gravitational wave events using CALorimetric Electron Telescope (CALET) observations. The main instrument of CALET, CALorimeter (CAL), observes gamma-rays from ∼1 GeV up to 10 TeV with a field of view (FOV) of nearly 2 sr. In addition, the CALET gamma-ray burst monitor views ∼3 sr and ∼2π sr of the sky in the 7 keV-1 MeV and the 40 keV-20 MeV bands, respectively, by using two different crystal scintillators. The CALET observations on the International Space Station started in 2015 October, and here we report analyses of events associated with the following gravitational wave events: GW151226, GW170104, GW170608, GW170814, and GW170817. Although only upper limits on gamma-ray emission are obtained, they correspond to a luminosity of 1049 ∼ 1053 erg s-1 in the GeV energy band depending on the distance and the assumed time duration of each event, which is approximately on the order of luminosity of typical short gamma-ray bursts. This implies that there will be a favorable opportunity to detect high-energy gamma-ray emission in further observations if additional gravitational wave events with favorable geometry will occur within our FOV. We also show the sensitivity of CALET for gamma-ray transient events, which is on the order of 10-7 erg cm-2 s-1 for an observation of 100 s in duration.
KW - gamma rays: general
KW - gravitational waves
KW - methods: observational
UR - http://www.scopus.com/inward/record.url?scp=85052380958&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85052380958&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/aad18f
DO - 10.3847/1538-4357/aad18f
M3 - Article
AN - SCOPUS:85052380958
SN - 0004-637X
VL - 863
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 160
ER -