E. Thrane et al. 2009 ApJ 697 730 doi:10.1088/0004-637X/697/1/730
E. Thrane1, K. Abe2, Y. Hayato2,3, T. Iida2, M. Ikeda2, J. Kameda2, K. Kobayashi2, Y. Koshio2,3, M. Miura2, S. Moriyama2,3, M. Nakahata2,3, S. Nakayama2, Y. Obayashi2, H. Ogawa2, H. Sekiya2,3, M. Shiozawa2,3, Y. Suzuki2,3, A. Takeda2, Y. Takenaga2, Y. Takeuchi2,3, K. Ueno2, K. Ueshima2, H. Watanabe2, S. Yamada2, M. R. Vagins3,7, S. Hazama4, I. Higuchi4, C. Ishihara4, T. Kajita4,3, K. Kaneyuki4,3, G. Mitsuka4, H. Nishino4, K. Okumura4, N. Tanimoto4, F. Dufour5, E. Kearns5,3, M. Litos5, J. L. Raaf5, J. L. Stone5,3, L. R. Sulak5, M. Goldhaber6, K. Bays7, D. Casper7, J. P. Cravens7, W. R. Kropp7, S. Mine7, C. Regis7, M. B. Smy7,3, H. W. Sobel7,3, K. S. Ganezer8, J. Hill8, W. E. Keig8, J. S. Jang9, I. S. Jeong9, J. Y. Kim9, I. T. Lim9, M. Fechner10, K. Scholberg10,3, C. W. Walter10,3, R. Wendell10, S. Tasaka11, J. G. Learned12, S. Matsuno12, Y. Watanabe13, T. Hasegawa14, T. Ishida14, T. Ishii14, T. Kobayashi14, T. Nakadaira14, K. Nakamura14,3, K. Nishikawa14, Y. Oyama14, K. Sakashita14, T. Sekiguchi14, T. Tsukamoto14, A. T. Suzuki15, A. K. Ichikawa16, A. Minamino16, T. Nakaya16,3, M. Yokoyama16, S. Dazeley17, R. Svoboda18, A. Habig19, Y. Fukuda20, Y. Itow21, T. Tanaka21, C. K. Jung22, G. Lopez22, C. McGrew22, C. Yanagisawa22, N. Tamura23, Y. Idehara24, H. Ishino24, A. Kibayashi24, M. Sakuda24, Y. Kuno25, M. Yoshida25, S. B. Kim26, B. S. Yang26, T. Ishizuka27, H. Okazawa28, Y. Choi29, H. K. Seo1,31, Y. Furuse30, K. Nishijima30, Y. Yokosawa30, M. Koshiba31, Y. Totsuka31, S. Chen32, G. Gong32, Y. Heng32, T. Xue32, Z. Yang32, H. Zhang32, D. Kielczewska33, P. Mijakowski33, H. G. Berns34, K. Connolly34, M. Dziomba34 (The Super-Kamiokande Collaboration), R. J. Wilkes34
Show affiliationsWe perform a search for neutrinos coincident with GRB 080319B—the brightest GRB observed to date—in a ±1000 s window. No statistically significant coincidences were observed and we thereby obtain an upper limit on the fluence of neutrino-induced muons from this source. From this we apply reasonable assumptions to derive a limit on neutrino fluence from the GRB.
Issue 1 (2009 May 20)
Received 2008 November 19, accepted for publication 2009 February 26
Published 2009 May 5
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