CALET UPPER LIMITS on X-RAY and GAMMA-RAY COUNTERPARTS of GW151226

O. Adriani; Y. Akaike; K. Asano; Y. Asaoka; M. G. Bagliesi; G. Bigongiari; W. R. Binns; S. Bonechi; M. Bongi; P. Brogi; J. H. Buckley; N. Cannady; G. Castellini; C. Checchia; M. L. Cherry; G. Collazuol; V. Di Felice; K. Ebisawa; H. Fuke; T. G. Guzik; T. Hams; M. Hareyama; N. Hasebe; K. Hibino; M. Ichimura; K. Ioka; W. Ishizaki; M. H. Israel; A. Javaid; K. Kasahara; J. Kataoka; R. Kataoka; Y. Katayose; C. Kato; N. Kawanaka; Y. Kawakubo; H. Kitamura; H. S. Krawczynski; J. F. Krizmanic; S. Kuramata; T. Lomtadze; P. Maestro; P. S. Marrocchesi; A. M. Messineo; J. W. Mitchell; S. Miyake; K. Mizutani; A. A. Moiseev; K. Mori; M. Mori; N. Mori; H. M. Motz; K. Munakata; H. Murakami; Y. E. Nakagawa; S. Nakahira; J. Nishimura; S. Okuno; J. F. Ormes; S. Ozawa; L. Pacini; F. Palma; P. Papini; A. V. Penacchioni; B. F. Rauch; S. Ricciarini; K. Sakai; T. Sakamoto; M. Sasaki; Y. Shimizu; A. Shiomi; R. Sparvoli; P. Spillantini; F. Stolzi; I. Takahashi; M. Takayanagi; M. Takita; T. Tamura; N. Tateyama; T. Terasawa; H. Tomida; S. Torii; Y. Tsunesada; Y. Uchihori; S. Ueno; E. Vannuccini; J. P. Wefel; K. Yamaoka; S. Yanagita; A. Yoshida; K. Yoshida; T. Yuda

doi:10.3847/2041-8205/829/1/L20

CALET UPPER LIMITS on X-RAY and GAMMA-RAY COUNTERPARTS of GW151226

O. Adriani, Y. Akaike, K. Asano, Y. Asaoka, M. G. Bagliesi, G. Bigongiari, W. R. Binns, S. Bonechi, M. Bongi, P. Brogi, J. H. Buckley, N. Cannady, G. Castellini, C. Checchia, M. L. Cherry, G. Collazuol, V. Di Felice, K. Ebisawa, H. Fuke, T. G. GuzikT. Hams, M. Hareyama, N. Hasebe, K. Hibino, M. Ichimura, K. Ioka, W. Ishizaki, M. H. Israel, A. Javaid, K. Kasahara, J. Kataoka, R. Kataoka, Y. Katayose, C. Kato, N. Kawanaka, Y. Kawakubo, H. Kitamura, H. S. Krawczynski, J. F. Krizmanic, S. Kuramata, T. Lomtadze, P. Maestro, P. S. Marrocchesi, A. M. Messineo, J. W. Mitchell, S. Miyake, K. Mizutani, A. A. Moiseev, K. Mori, M. Mori, N. Mori, H. M. Motz, K. Munakata, H. Murakami, Y. E. Nakagawa, S. Nakahira, J. Nishimura, S. Okuno, J. F. Ormes, S. Ozawa, L. Pacini, F. Palma, P. Papini, A. V. Penacchioni, B. F. Rauch, S. Ricciarini, K. Sakai, T. Sakamoto, M. Sasaki, Y. Shimizu, A. Shiomi, R. Sparvoli, P. Spillantini, F. Stolzi, I. Takahashi, M. Takayanagi, M. Takita, T. Tamura, N. Tateyama, T. Terasawa, H. Tomida, S. Torii, Y. Tsunesada, Y. Uchihori, S. Ueno, E. Vannuccini, J. P. Wefel, K. Yamaoka, S. Yanagita, A. Yoshida, K. Yoshida, T. Yuda

研究成果: Article › 査読

36 被引用数 (Scopus)

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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 gamma-rays from ∼1 GeV up to 10 TeV with a field of view of ∼2 sr. The CALET gamma-ray burst monitor (CGBM) 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 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 ×10^-7 erg cm^-2 s^-1 in the 1-100 GeV band where CAL reaches 15% of the integrated LIGO probability (∼1.1 sr). The CGBM 7σ upper limits are 1.0 ×10^-6 erg cm^-2 s^-1 (7-500 keV) and 1.8 ×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 ×10⁴⁹ erg s^-1, which is significantly lower than typical short GRBs.

本文言語	English
論文番号	L20
ジャーナル	Astrophysical Journal Letters
巻	829
号	1
DOI	https://doi.org/10.3847/2041-8205/829/1/L20
出版ステータス	Published - 2016 9月 20

ASJC Scopus subject areas

天文学と天体物理学
宇宙惑星科学

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10.3847/2041-8205/829/1/L20

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Adriani, O., Akaike, Y., Asano, K., Asaoka, Y., Bagliesi, M. G., Bigongiari, G., Binns, W. R., Bonechi, S., Bongi, M., Brogi, P., Buckley, J. H., Cannady, N., Castellini, G., Checchia, C., Cherry, M. L., Collazuol, G., Felice, V. D., Ebisawa, K., Fuke, H., ... Yuda, T. (2016). CALET UPPER LIMITS on X-RAY and GAMMA-RAY COUNTERPARTS of GW151226. Astrophysical Journal Letters, 829(1), Article L20. https://doi.org/10.3847/2041-8205/829/1/L20

Adriani, O, Akaike, Y, Asano, K, Asaoka, Y, Bagliesi, MG, Bigongiari, G, Binns, WR, Bonechi, S, Bongi, M, Brogi, P, Buckley, JH, Cannady, N, Castellini, G, Checchia, C, Cherry, ML, Collazuol, G, Felice, VD, Ebisawa, K, Fuke, H, Guzik, TG, Hams, T, Hareyama, M, Hasebe, N, Hibino, K, Ichimura, M, Ioka, K, Ishizaki, W, Israel, MH, Javaid, A, Kasahara, K, Kataoka, J, Kataoka, R, Katayose, Y, Kato, C, Kawanaka, N, Kawakubo, Y, Kitamura, H, Krawczynski, HS, Krizmanic, JF, Kuramata, S, Lomtadze, T, Maestro, P, Marrocchesi, PS, Messineo, AM, Mitchell, JW, Miyake, S, Mizutani, K, Moiseev, AA, Mori, K, Mori, M, Mori, N, Motz, HM, Munakata, K, Murakami, H, Nakagawa, YE, Nakahira, S, Nishimura, J, Okuno, S, Ormes, JF, Ozawa, S, Pacini, L, Palma, F, Papini, P, Penacchioni, AV, Rauch, BF, Ricciarini, S, Sakai, K, Sakamoto, T, Sasaki, M, Shimizu, Y, Shiomi, A, Sparvoli, R, Spillantini, P, Stolzi, F, Takahashi, I, Takayanagi, M, Takita, M, Tamura, T, Tateyama, N, Terasawa, T, Tomida, H, Torii, S, Tsunesada, Y, Uchihori, Y, Ueno, S, Vannuccini, E, Wefel, JP, Yamaoka, K, Yanagita, S, Yoshida, A, Yoshida, K & Yuda, T 2016, 'CALET UPPER LIMITS on X-RAY and GAMMA-RAY COUNTERPARTS of GW151226', Astrophysical Journal Letters, vol. 829, no. 1, L20. https://doi.org/10.3847/2041-8205/829/1/L20

@article{df123e20aad14fc488422444ec96da06,

title = "CALET UPPER LIMITS on X-RAY and GAMMA-RAY COUNTERPARTS of GW151226",

abstract = "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 gamma-rays from ∼1 GeV up to 10 TeV with a field of view of ∼2 sr. The CALET gamma-ray burst monitor (CGBM) 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 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 ×10-7 erg cm-2 s-1 in the 1-100 GeV band where CAL reaches 15% of the integrated LIGO probability (∼1.1 sr). The CGBM 7σ upper limits are 1.0 ×10-6 erg cm-2 s-1 (7-500 keV) and 1.8 ×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 ×1049 erg s-1, which is significantly lower than typical short GRBs.",

keywords = "gamma-ray burst: general, gravitational waves",

author = "O. Adriani and Y. Akaike and K. Asano and Y. Asaoka and Bagliesi, {M. G.} and G. Bigongiari and Binns, {W. R.} and S. Bonechi and M. Bongi and P. Brogi and Buckley, {J. H.} and N. Cannady and G. Castellini and C. Checchia and Cherry, {M. L.} and G. Collazuol and Felice, {V. Di} and K. Ebisawa and H. Fuke and Guzik, {T. G.} and T. Hams and M. Hareyama and N. Hasebe and K. Hibino and M. Ichimura and K. Ioka and W. Ishizaki and Israel, {M. H.} and A. Javaid and K. Kasahara and J. Kataoka and R. Kataoka and Y. Katayose and C. Kato and N. Kawanaka and Y. Kawakubo and H. Kitamura and Krawczynski, {H. S.} and Krizmanic, {J. F.} and S. Kuramata and T. Lomtadze and P. Maestro and Marrocchesi, {P. S.} and Messineo, {A. M.} and Mitchell, {J. W.} and S. Miyake and K. Mizutani and Moiseev, {A. A.} and K. Mori and M. Mori and N. Mori and Motz, {H. M.} and K. Munakata and H. Murakami and Nakagawa, {Y. E.} and S. Nakahira and J. Nishimura and S. Okuno and Ormes, {J. F.} and S. Ozawa and L. Pacini and F. Palma and P. Papini and Penacchioni, {A. V.} and Rauch, {B. F.} and S. Ricciarini and K. Sakai and T. Sakamoto and M. Sasaki and Y. Shimizu and A. Shiomi and R. Sparvoli and P. Spillantini and F. Stolzi and I. Takahashi and M. Takayanagi and M. Takita and T. Tamura and N. Tateyama and T. Terasawa and H. Tomida and S. Torii and Y. Tsunesada and Y. Uchihori and S. Ueno and E. Vannuccini and Wefel, {J. P.} and K. Yamaoka and S. Yanagita and A. Yoshida and K. Yoshida and T. Yuda",

note = "Funding Information: This work is partially supported by JSPS Grant-in-Aid for Scientific Research (S) number 26220708 and MEXTSupported Program for the Strategic Research Foundation at Private Universities (20112015) S1101021 in Waseda University. This work is also supported in part by MEXT Grant-in- Aid for Scientific Research on Innovative Areas number 24103002. US CALET work is supported by NASA under RTOP 14-APRA14-0075 (GSFC) and grants NNX16AC02G (WUSL), NNX16AB99G (LSU), and NNX11AE06G (Denver). Publisher Copyright: {\textcopyright} 2016. The American Astronomical Society. All rights reserved..",

year = "2016",

month = sep,

day = "20",

doi = "10.3847/2041-8205/829/1/L20",

language = "English",

volume = "829",

journal = "Astrophysical Journal Letters",

issn = "2041-8205",

publisher = "IOP Publishing Ltd.",

number = "1",

}

TY - JOUR

T1 - CALET UPPER LIMITS on X-RAY and GAMMA-RAY COUNTERPARTS of GW151226

AU - Adriani, O.

AU - Akaike, Y.

AU - Asano, K.

AU - Asaoka, Y.

AU - Bagliesi, M. G.

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 - Javaid, A.

AU - Kasahara, K.

AU - Kataoka, J.

AU - Kataoka, R.

AU - Katayose, Y.

AU - Kato, C.

AU - Kawanaka, N.

AU - Kawakubo, Y.

AU - Kitamura, H.

AU - Krawczynski, H. S.

AU - Krizmanic, J. F.

AU - Kuramata, S.

AU - Lomtadze, T.

AU - Maestro, P.

AU - Marrocchesi, P. S.

AU - Messineo, A. M.

AU - Mitchell, J. W.

AU - Miyake, S.

AU - Mizutani, K.

AU - Moiseev, A. A.

AU - Mori, K.

AU - Mori, M.

AU - Mori, N.

AU - Motz, H. M.

AU - Munakata, K.

AU - Murakami, H.

AU - Nakagawa, Y. E.

AU - Nakahira, S.

AU - Nishimura, J.

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.

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 - 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.

AU - Yuda, T.

N1 - Funding Information: This work is partially supported by JSPS Grant-in-Aid for Scientific Research (S) number 26220708 and MEXTSupported Program for the Strategic Research Foundation at Private Universities (20112015) S1101021 in Waseda University. This work is also supported in part by MEXT Grant-in- Aid for Scientific Research on Innovative Areas number 24103002. US CALET work is supported by NASA under RTOP 14-APRA14-0075 (GSFC) and grants NNX16AC02G (WUSL), NNX16AB99G (LSU), and NNX11AE06G (Denver). Publisher Copyright: © 2016. The American Astronomical Society. All rights reserved..

PY - 2016/9/20

Y1 - 2016/9/20

N2 - 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 gamma-rays from ∼1 GeV up to 10 TeV with a field of view of ∼2 sr. The CALET gamma-ray burst monitor (CGBM) 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 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 ×10-7 erg cm-2 s-1 in the 1-100 GeV band where CAL reaches 15% of the integrated LIGO probability (∼1.1 sr). The CGBM 7σ upper limits are 1.0 ×10-6 erg cm-2 s-1 (7-500 keV) and 1.8 ×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 ×1049 erg s-1, which is significantly lower than typical short GRBs.

AB - 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 gamma-rays from ∼1 GeV up to 10 TeV with a field of view of ∼2 sr. The CALET gamma-ray burst monitor (CGBM) 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 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 ×10-7 erg cm-2 s-1 in the 1-100 GeV band where CAL reaches 15% of the integrated LIGO probability (∼1.1 sr). The CGBM 7σ upper limits are 1.0 ×10-6 erg cm-2 s-1 (7-500 keV) and 1.8 ×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 ×1049 erg s-1, which is significantly lower than typical short GRBs.

KW - gamma-ray burst: general

KW - gravitational waves

UR - http://www.scopus.com/inward/record.url?scp=84989160261&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84989160261&partnerID=8YFLogxK

U2 - 10.3847/2041-8205/829/1/L20

DO - 10.3847/2041-8205/829/1/L20

M3 - Article

AN - SCOPUS:84989160261

SN - 2041-8205

VL - 829

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

IS - 1

M1 - L20

ER -

CALET UPPER LIMITS on X-RAY and GAMMA-RAY COUNTERPARTS of GW151226

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