CALET Search for Electromagnetic Counterparts of Gravitational Waves during the LIGO/Virgo O3 Run

被引：1

作者：

Adriani, O. ^{[1
,2
]}

Akaike, Y. ^{[3
,4
]}

Asano, K. ^{[5
]}

Asaoka, Y. ^{[5
]}

Berti, E. ^{[1
,2
]}

Bigongiari, G. ^{[6
,7
]}

Binns, W. R. ^{[8
,9
]}

Bongi, M. ^{[1
,2
]}

Brogi, P. ^{[6
,7
]}

Bruno, A. ^{[10
]}

Buckley, J. H. ^{[8
,9
]}

Cannady, N. ^{[11
,12
,13
]}

Castellini, G. ^{[14
]}

Checchia, C. ^{[6
,7
]}

Cherry, M. L. ^{[15
,41
]}

Collazuol, G. ^{[16
,17
]}

Ebisawa, K. ^{[18
]}

Ficklin, A. W. ^{[15
]}

Fuke, H. ^{[18
]}

Gonzi, S. ^{[1
,2
]}

Guzik, T. G. ^{[15
]}

Hams, T. ^{[11
]}

Hibino, K. ^{[19
]}

Ichimura, M. ^{[20
]}

Ioka, K. ^{[21
]}

Ishizaki, W. ^{[5
]}

Israel, M. H. ^{[8
,9
]}

Kasahara, K. ^{[22
]}

Kataoka, J. ^{[23
]}

Kataoka, R. ^{[24
]}

Katayose, Y. ^{[25
]}

Kato, C. ^{[26
]}

Kawanaka, N.

Kawakubo, Y. ^{[15
,41
]}

Kobayashi, K. ^{[3
,4
]}

Kohri, K. ^{[27
]}

Krawczynski, H. S. ^{[8
,9
]}

Krizmanic, J. F. ^{[12
]}

Maestro, P. ^{[6
,7
]}

Marrocchesi, P. S. ^{[6
,7
]}

Messineo, A. M. ^{[28
]}

Mitchell, J. W. ^{[12
]}

Miyake, S. ^{[29
]}

Moiseev, A. A. ^{[12
,13
,30
]}

Mori, M. ^{[31
]}

Mori, N. ^{[2
]}

Motz, H. M. ^{[32
]}

Munakata, K. ^{[26
]}

Nakahira, S. ^{[18
]}

Nishimura, J. ^{[18
]}

机构：

[1] Univ Florence, Dept Phys, Via Sansone 1, I-50019 Sesto Fiorentino, Italy

[2] INFN Sez Florence, Via Sansone 1, I-50019 Sesto Fiorentino, Italy

[3] Waseda Univ, Waseda Res Inst Sci & Engn, 17 Kikuicho,Shinjuku, Tokyo 1620044, Japan

[4] Japan Aerosp Explorat Agcy, Human Spaceflight Technol Directorate, JEM Utilizat Ctr, 2-1-1 Sengen, Tsukuba, Ibaraki 3058505, Japan

[5] Univ Tokyo, Inst Cosm Ray Res, 5-1-5 Kashiwano Ha, Kashiwa, Chiba 2778582, Japan

[6] Univ Siena, Dept Phys Sci Earth & Environm, Via Roma 56, I-53100 Siena, Italy

[7] INFN Sezione Pisa, Polo Fibonacci,Largo B Pontecorvo,3, I-56127 Pisa, Italy

[8] Washington Univ, Dept Phys, One Brookings Dr, St Louis, MO 63130 USA

[9] Washington Univ, McDonnell Ctr Space Sci, One Brookings Dr, St Louis, MO 63130 USA

[10] NASA GSFC, Heliospher Phys Lab, Greenbelt, MD 20771 USA

[11] Univ Maryland, Ctr Space Sci & Technol, 1000 Hilltop Circle, Baltimore, MD 21250 USA

[12] NASA GSFC, Astroparticle Phys Lab, Greenbelt, MD 20771 USA

[13] NASA GSFC, Ctr Res & Explorat Space Sci & Technol, Greenbelt, MD 20771 USA

[14] Natl Res Council CNR, Inst Appl Phys IFAC, Via Madonna Piano,10, I-50019 Sesto Fiorentino, Italy

[15] Louisiana State Univ, Dept Phys & Astron, 202 Nicholson Hall, Baton Rouge, LA 70803 USA

[16] Univ Padua, Dept Phys & Astron, Via Marzolo, I-35131 Padua, Italy

[17] INFN Sez Padova, Via Marzolo, I-35131 Padua, Italy

[18] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan

[19] Kanagawa Univ, 3-27-1 Rokkakubashi, Rokkakubashi, Kanagawa 3271, Japan

[20] Hirosaki Univ, Grad Sch Sci & Technol, Fac Sci & Technol, 3,Bunkyo, Hirosaki, Aomori 0368561, Japan

[21] Kyoto Univ, Yukawa Inst Theoret Phys, Kitashirakawa Oiwake Cho,Sakyo Ku, Kyoto 6068502, Japan

[22] Shibaura Inst Technol, Dept Elect Informat Syst, 307 Fukasaku, Saitama 3378570, Japan

[23] Waseda Univ, Sch Adv Sci & Engn, 3-4-1 Okubo,Shinjuku, Tokyo 1698555, Japan

[24] Natl Inst Polar Res, 10-3,Midori Cho, Tachikawa, Tokyo 1908518, Japan

[25] Yokohama Natl Univ, Div Intelligent Syst Engn, Fac Engn, 79-5 Tokiwadai, Yokohama, Kanagawa 2408501, Japan

[26] Shinshu Univ, Fac Sci, 3-1-1 Asahi, Matsumoto, Nagano 3908621, Japan

[27] Inst Particle & Nucl Studies, High Energy Accelerator Res Org, 1-1 Oho, Tsukuba, Ibaraki 3050801, Japan

[28] Univ Pisa, Polo Fibonacci,Largo B Pontecorvo,3, I-56127 Pisa, Italy

[29] Natl Inst Technol KOSEN, Dept Elect & Elect Syst Engn, Ibaraki Coll, 866 Nakane, Hitachinaka, Ibaraki 3128508, Japan

[30] Univ Maryland, Dept Astron, College Pk, MD 20742 USA

[31] Ritsumeikan Univ, Dept Phys Sci, Coll Sci & Engn, Shiga 5258577, Japan

[32] Waseda Univ, Global Ctr Sci & Engn, Fac Sci & Engn, 3-4-1 Okubo,Shinjuku, Tokyo 1698555, Japan

[33] Univ Denver, Dept Phys & Astron, Phys Bldg,Room 211,2112 East Wesley Ave, Denver, CO 80208 USA

[34] Natl Inst Informat & Commun Technol, Quantum ICT Adv Dev Ctr, 4-2-1 Nukui Kitamachi, Koganei, Tokyo 1848795, Japan

[35] Aoyama Gakuin Univ, Dept Math & Phys, Coll Sci & Engn, 5-10-1 Fuchinobe, Sagamihara, Kanagawa 2525258, Japan

[36] Nihon Univ, Coll Ind Technol, I-2-1 Izumi, Narashino, Chiba 2758575, Japan

[37] Osaka Metropolitan Univ, Grad Sch Sci, Sumiyoshi, Osaka 5588585, Japan

[38] Osaka Metropolitan Univ, Nambu Yoichiro Inst Theoret & Expt Phys, Sumiyoshi, Osaka 5588585, Japan

[39] Natl Inst Quantum & Radiat Sci & Technol, 4-9-1 Anagawa, Chiba 2638555, Japan

[40] Nagoya Univ, Nagoya, Aichi 4648601, Japan

[41] Ibaraki Univ, Coll Sci, 2-1-1 Bunkyo, Mito, Ibaraki 3108512, Japan

来源：

ASTROPHYSICAL JOURNAL | 2022年 / 933卷 / 01期

关键词：

GAMMA-RAY-BURSTS; NEUTRINO BURST; FERMI-LAT; SWIFT; MERGERS; MODELS; 1987A;

D O I：

10.3847/1538-4357/ac6f53

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The CALorimetric Electron Telescope (CALET) on the International Space Station consists of a high-energy cosmic-ray CALorimeter (CAL) and a lower-energy CALET Gamma-ray Burst Monitor (CGBM). CAL is sensitive to electrons up to 20 TeV, cosmic-ray nuclei from Z = 1 through Z similar to 40, and gamma rays over the range 1 GeV-10 TeV. CGBM observes gamma rays from 7 keV to 20 MeV. The combined CAL-CGBM instrument has conducted a search for gamma-ray bursts (GRBs) since 2015 October. We report here on the results of a search for X-ray/gamma-ray counterparts to gravitational-wave events reported during the LIGO/Virgo observing run O3. No events have been detected that pass all acceptance criteria. We describe the components, performance, and triggering algorithms of the CGBM-the two Hard X-ray Monitors consisting of LaBr3(Ce) scintillators sensitive to 7 keV-1 MeV gamma rays and a Soft Gamma-ray Monitor BGO scintillator sensitive to 40 keV-20 MeV-and the high-energy CAL consisting of a charge detection module, imaging calorimeter, and the fully active total absorption calorimeter. The analysis procedure is described and upper limits to the time-averaged fluxes are presented.

引用

页数：16

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