{"paper":{"title":"Search for Neutrinos in Super-Kamiokande associated with Gravitational Wave Events GW150914 and GW151226","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"astro-ph.HE","authors_text":"A. Himmel, A. Kibayashi, A. Konaka, A. Minamino, A. Orii, A. Takeda, A. T. Suzuki, B. L. Hartfiel, C. Bronner, C. Kachulis, C. K. Jung, C. M. Nantais, C. W. Walter, C. Xu, C. Yanagisawa, D. Fukuda, E. Kearns, E. O'Sullivan, E. Richard, F. d. M. Blaszczyk, G. Santucci, H. A. Tanaka, H. Ishino, H. Okazawa, H. Sekiya, H. Tanaka, H. W. Sobel, I. T. Lim, J. F. Martin, J. G. Learned, J. Gustafson, J. Hignight, J. Hil, J. Imber, J. Kameda, J. L. Palomino, J. L. Raaf, J. L. Stone, J. S. Jang, J. Y. Kim, K. Abe, K. Choi, K. Frankiewicz, K. Haga, K. Huang, K. Iyogi, K. Kaneyuki, K. Martens, K. Nakamura, K. Nishijima, K. Okumura, K. Sakashita, K. Scholberg, K. S. Ganezer, K. Suzuki, L. Labarga, Ll. Marti, L. R. Sulak, L. Wan, M. B. Smy, M. Friend, M. Goldhaber, M. Hartz, M. Ikeda, M. Jiang, M. J. Wilking, M. Koshiba, M. Miura, M. Nakahata, M. R. Vagins, M. Sakuda, M. Shiozawa, M. Yokoyama, N. D. Patel, N. Hong, P. Fernandez, P. Mijakowski, P. Weatherly, R. Akutsu, R. A. Wendell, R. G. Calland, R. G. Park, R. J. Wilkes, R. Tacik, S. Berkman, S. B. Kim, S. Chen, S. Hirota, S. Matsuno, S. Mine, S. Moriyama, S. Nakayama, S. N. Smith, S. Tasaka, S. Tobayama, S. V. Cao, T. Hasegawa, T. Hiraki, T. Ishida, T. Ishii, T. Ishizuka, T. Kajita, T. Kayano, T. Kobayashi, T. Mori, T. Nakadaira, T. Nakajima, T. Nakamura, T. Nakaya, T. Sekiguchi, T. Suzuki, T. Tomura, T. Tsukamoto, T. Yano, V. Takhistov, W. R. Kropp, X. Li, Y. Choi, Y. Fukuda, Y. Hayato, Y. Itow, Y. Kishimoto, Y. Koshio, Y. Kuno, Y. Nakano, Y. Nishimura, Y. Oyama, Y. Suda, Y. Suzuki, Y. Takeuchi, Y. Totsuka, Y. Zhang, Z. Li","submitted_at":"2016-08-31T07:00:50Z","abstract_excerpt":"We report the results from a search in Super-Kamiokande for neutrino signals coincident with the first detected gravitational wave events, GW150914 and GW151226, using a neutrino energy range from 3.5 MeV to 100 PeV. We searched for coincident neutrino events within a time window of $\\pm$500 seconds around the gravitational wave detection time. Four neutrino candidates are found for GW150914 and no candidates are found for GW151226. The remaining neutrino candidates are consistent with the expected background events. We calculated the 90\\% confidence level upper limits on the combined neutrino"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1608.08745","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"}