{"paper":{"title":"Search for GeV Gamma-ray Counterparts of Gravitational Wave Events by CALET","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.A. Moiseev, A.M. Messineo, A. Shiomi, A. Sulaj, A.V. Penacchioni, A. Yoshida, B.F. Rauch, C. Checchia, C. Kato, E. Berti, E. Vannuccini, F. Palma, F. Stolzi, G.A. de Nolfo, G. Bigongiari, G. Castellini, G. Collazuol, H. Fuke, H.M. Motz, H. Murakami, H.S. Krawczynski, H. Tomida, I. Takahashi, J.E. Suh, J.F. Krizmanic, J.F. Ormes, J.H. Buckley, J. Kataoka, J. Nishimura, J.P. Wefel, J.W. Mitchell, K. Asano, K. Ebisawa, K. Hibino, K. Ioka, K. Kasahara, K. Kohri, K. Mori, K. Munakata, K. Sakai, K. Yamaoka, K. Yoshida (CALET Collaboration), L. Pacini, M. Bongi, M.G. Bagliesi, M. Hareyama, M.H. Israel, M. Ichimura, M.L. Cherry, M. Mori, M. Sasaki, M. Takayanagi, M. Takita, N. Cannady, N. Hasebe, N. Kawanaka, N. Mori, N. Tateyama, O. Adriani, P. Brogi, P. Maestro, P. Papini, P.S. Marrocchesi, P. Spillantini, R. Kataoka, R. Sparvoli, S. Bonechi, S.B. Ricciarini, S. Miyake, S. Nakahira, S. Okuno, S. Ozawa, S. Torii, S. Ueno, S. Yanagita, T.G. Guzik, T. Hams, T. Lomtadze, T. Sakamoto, T. Tamura, T. Terasawa, V. Di Felice, W. Ishizaki, W.R. Binns, Y. Akaike, Y. Asaoka, Y. Katayose, Y. Kawakubo, Y. Shimizu, Y. Tsunesada, Y. Uchihori","submitted_at":"2018-07-04T03:06:48Z","abstract_excerpt":"We present results on searches for gamma-ray counterparts of the LIGO/Virgo gravitational-wave events using CALorimetric Electron Telescope ({\\sl CALET}) observations. The main instrument of {\\sl CALET}, CALorimeter (CAL), observes gamma-rays from $\\sim1$ GeV up to 10 TeV with a field of view of nearly 2 sr. In addition, the {\\sl CALET} gamma-ray burst monitor (CGBM) views $\\sim$3 sr and $\\sim2\\pi$ 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 {\\sl CALET} observations on the International Space Station starte"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1807.01435","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}