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arXiv · 1607.00233

CALET Upper Limits on X-ray and Gamma-ray Counterparts of GW 151226

O. Adriani·Y. Akaike·K. Asano·Y. Asaoka·M. G. Bagliesi·G. Bigongiari·W. R. Binns·S. Bonechi·M. Bongi·P. Brog·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
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Abstract

We present upper limits in the hard X-ray and gamma-ray bands at the time of the LIGO gravitational-wave event GW 151226 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 ~2pi 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 GW 151226 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 (~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 one second 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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O. Adriani, Y. Akaike, K. Asano, Y. Asaoka, M. G. Bagliesi, G. Bigongiari, W. R. Binns, S. Bonechi, M. Bongi, P. Brog, 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. 2016-07-01. CALET Upper Limits on X-ray and Gamma-ray Counterparts of GW 151226. https://doi.org/10.3847/2041-8205/829/1/l20

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