CALET UPPER LIMITS ON X-RAY AND GAMMA-RAY COUNTERPARTS OF GW151226

被引：25

作者：

Adriani, O. ^{[1
,2
,3
]}

Akaike, Y. ^{[4
,5
,6
]}

Asano, K. ^{[7
]}

Asaoka, Y. ^{[8
,9
]}

Bagliesi, M. G. ^{[2
,10
]}

Bigongiari, G. ^{[2
,10
]}

Binns, W. R. ^{[11
]}

Bonechi, S. ^{[2
,10
]}

Bongi, M. ^{[1
,2
,3
]}

Brogi, P. ^{[2
,10
]}

Buckley, J. H. ^{[11
]}

Cannady, N. ^{[12
]}

Castellini, G. ^{[1
,2
,3
]}

Checchia, C. ^{[13
]}

Cherry, M. L. ^{[12
]}

Collazuol, G. ^{[13
]}

Di Felice, V. ^{[2
,14
]}

Ebisawa, K. ^{[15
]}

Fuke, H. ^{[15
]}

Guzik, T. G. ^{[12
]}

Hams, T. ^{[5
,6
,16
]}

Hareyama, M. ^{[17
]}

Hasebe, N. ^{[9
]}

Hibino, K. ^{[18
]}

Ichimura, M. ^{[19
]}

Ioka, K. ^{[20
]}

Ishizaki, W. ^{[7
]}

Israel, M. H. ^{[11
]}

Javaid, A. ^{[12
]}

Kasahara, K. ^{[9
]}

Kataoka, J. ^{[9
]}

Kataoka, R. ^{[21
]}

Katayose, Y. ^{[22
]}

Kato, C. ^{[23
]}

Kawanaka, N. ^{[24
]}

Kawakubo, Y. ^{[25
]}

Kitamura, H. ^{[26
]}

Krawczynski, H. S. ^{[11
]}

Krizmanic, J. F. ^{[4
,5
,6
]}

Kuramata, S. ^{[19
]}

Lomtadze, T. ^{[27
,28
]}

Maestro, P. ^{[2
,10
]}

Marrocchesi, P. S. ^{[2
,10
]}

Messineo, A. M. ^{[27
,28
]}

Mitchell, J. W. ^{[29
]}

Miyake, S. ^{[30
]}

Mizutani, K. ^{[31
]}

Moiseev, A. A. ^{[5
,6
,32
]}

Mori, K. ^{[9
,15
]}

Mori, M. ^{[33
]}

机构：

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

[2] Ist Nazl Fis Nucl, Natl Inst Nucl Phys, Piazza Caprettari 70, I-00186 Rome, Italy

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

[4] Univ Space Res Assoc, 7178 Columbia Gateway Dr, Columbia, MD 21046 USA

[5] CRESST, Greenbelt, MD 20771 USA

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

[7] Univ Tokyo, Inst Cosm Ray Res, 5-1-5 Kashiwa No Ha, Kashiwa, Chiba 2778582, Japan

[8] Japan Aerosp Explorat Agcy, Human Spaceflight Technol Directorate, JEM Miss Operat & Integrat Ctr, 2-1-1 Sengen, Tsukuba, Ibaraki 3058505, Japan

[9] Waseda Univ, Res Inst Sci & Engn, Shinjuku Ku, 3-4-1 Okubo, Tokyo 1698555, Japan

[10] Univ Siena, Via Banchi Sotto 55, I-53100 Siena, Italy

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

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

[13] Univ Padua, Dept Phys & Astron, Via Marzolo 8, I-35131 Padua, Italy

[14] Univ Roma Tor Vergata, Via Ric Sci 1, I-00133 Rome, Italy

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

[16] Univ Maryland Baltimore Cty, Dept Phys, 1000 Hilltop Circle, Baltimore, MD 21250 USA

[17] St Marianna Univ, Sch Med, Miyamae Ku, 2-16-1 Sugao, Kawasaki, Kanagawa 2168511, Japan

[18] Kanagawa Univ, 3-27-1 Rokkakubashi, Yokohama, Kanagawa 2218686, Japan

[19] Hirosaki Univ, Grad Sch Sci & Technol, Fac Sci & Technol, Bunkyo Ku, Hirosaki, Aomori 0368561, Japan

[20] Kyoto Univ, Yukawa Inst Theoret Phys, Sakyo Ku, Kyoto 6068502, Japan

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

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

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

[24] Univ Tokyo, Sch Sci, Bunkyo Ku, 7-3-1 Hongo, Tokyo 113003, Japan

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

[26] Natl Inst Radiol Sci, Inage Ku, 4-9-1 Anagawa, Chiba 2638555, Japan

[27] Univ Pisa, Pisa, Italy

[28] Ist Nazl Fis Nucl, Pisa, Italy

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

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

[31] Saitama Univ, Shimo Okubo 255, Saitama 3388570, Japan

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

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

[34] Waseda Univ, Int Ctr Sci & Engn Programs, Shinjuku Ku, 3-4-1 Okubo, Tokyo 1698555, Japan

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

[36] ASDC, Via Politecn Snc, I-00133 Rome, Italy

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

[38] Univ Tokyo, Kavli Inst Phys & Math Universe, 5-1-5 Kashiwanoha, Kashiwa, Chiba 2778583, Japan

[39] RIKEN, 2-1 Hirosawa, Wako, Saitama 3510198, Japan

[40] Osaka City Univ, Grad Sch Sci, Div Math & Phys, 3-3-138 Sugimoto, Sumiyoshi, Osaka 5588585, Japan

[41] Nagoya Univ, Chikusa Ku, Nagoya, Aichi 4648601, Japan

[42] Ibaraki Univ, Grad Sch Sci & Engn, 2-1-1 Bunkyo, Mito, Ibaraki 3108512, Japan

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

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2016年 / 829卷 / 01期

关键词：

gamma-ray burst; general - gravitational waves;

D O I：

10.3847/2041-8205/829/1/L20

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present upper limits in the hard X-ray and gamma-ray bands at the time of the Laser Interferometer Gravitational-wave Observatory (LIGO) gravitational-wave event GW151226 derived from the CALorimetric Electron Telescope (CALET) observation. The main instrument of CALET, CALorimeter (CAL), observes gammarays from similar to 1 GeV up to 10 TeV with a field of view of similar to 2 sr. The CALET gamma-ray burst monitor (CGBM) views similar to 3 sr and similar to 2 pi sr of the sky in the 7 keV-1 MeV and the 40 keV-20 MeV bands, respectively, by using two different scintillator-based instruments. The CGBM covered 32.5% and 49.1% of the GW151226 sky localization probability in the 7 keV-1 MeV and 40 keV-20 MeV bands respectively. We place a 90% upper limit of 2 x 10(-7) erg cm(-2) s(-1) in the 1-100 GeV band where CAL reaches 15% of the integrated LIGO probability (similar to 1.1 sr). The CGBM 7 sigma upper limits are 1.0 x 10(-6) erg cm(-2) s(-1) (7-500 keV) and 1.8. x. 10(-6) erg cm(-2) s(-1) (50-1000 keV) for a 1 s exposure. Those upper limits correspond to the luminosity of 3-5. x. 10(49) erg s(-1), which is significantly lower than typical short GRBs.

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