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	SEARCH FOR ASTROPHYSICAL NEUTRINO POINT SOURCES AT SUPER-KAMIOKANDE
	Thrane, E. ; Abe, K. ; Hayato, Y. ; Iida, T. ; Ikeda, M. ; Kameda, J. ; Kobayashi, K. ; Koshio, Y. ; Miura, M. ; Moriyama, S. ; Nakahata, M. ; Nakayama, S. ; Obayashi, Y. ; Ogawa, H. ; Sekiya, H. ; Shiozawa, M. ; Suzuki, Y. ; Takeda, A. ; Takenaga, Y. ; Takeuchi, Y. ; Ueno, K. ; Ueshima, K. ; Watanabe, H. ; Yamada, S. ; Vagins, M. R. ; Hazama, S. ; Higuchi, I. ; Ishihara, C. ; Kajita, T. ; Kaneyuki, K. ; Mitsuka, G. ; Nishino, H. ; Okumura, K. ; Tanimoto, N. ; Dufour, F. ; Kearns, E. ; Litos, M. ; Raaf, J. L. ; Stone, J. L. ; Sulak, L. R. ; Goldhaber, M. ; Bays, K. ; Casper, D. ; Cravens, J. P. ; Kropp, W. R. ; Mine, S. ; Regis, C. ; Smy, M. B. ; Sobel, H. W. ; Ganezer, K. S. ; Hill, J. ; Keig, W. E. ; Jang, J. S. ; Jeong, I. S. ; Kim, J. Y. ; Lim, I. T. ; Fechner, M. ; Scholberg, K. ; Walter, C. W. ; Wendell, R. ; Tasaka, S. ; Learned, J. G. ; Matsuno, S. ; Watanabe, Y. ; Hasegawa, T. ; Ishida, T. ; Ishii, T. ; Kobayashi, T. ; Nakadaira, T. ; Nakamura, K. ; Nishikawa, K. ; Oyama, Y. ; Sakashita, K. ; Sekiguchi, T. ; Tsukamoto, T. ; Suzuki, A. T. ; Ichikawa, A. K. ; Minamino, A. ; Nakaya, T. ; Yokoyama, M. ; Dazeley, S. ; Svoboda, R. ; Habig, A. ; Fukuda, Y. ; Itow, Y. ; Tanaka, T. ; Jung, C. K. ; Lopez, G. ; McGrew, C. ; Yanagisawa, C. ; Tamura, N. ; Idehara, Y. ; Ishino, H. ; Kibayashi, A. ; Sakuda, M. ; Kuno, Y. ; Yoshida, M. ; Kim, S. B. ; Yang, B. S. ; Ishizuka, T. ; Okazawa, H. ; Choi, Y. ; Seo, H. K. ; Furuse, Y. ; Nishijima, K. ; Yokosawa, Y. ; Koshiba, M. ; Totsuka, Y. ; Chen, S. ; Gong, G. ; Heng, Y. ; Xue, T. ; Yang, Z. ; Zhang, H. ; Kielczewska, D. ; Mijakowski, P. ; Connolly, K. ; Dziomba, M. ; Wilkes, R. J.
	2010-10-12 ; 2010-10-12
关键词	galaxies: active gamma rays: bursts neutrinos pulsars: general supernova remnants HIGH-ENERGY NEUTRINOS UPWARD-GOING MUONS GAMMA-RAY BURSTS COSMIC-RAYS GRB 080319B DISCOVERY TELESCOPE ASTRONOMY DETECTOR Astronomy & Astrophysics
中文摘要	It has been hypothesized that large fluxes of neutrinos may be created in astrophysical "cosmic accelerators." The primary background for a search for astrophysical neutrinos comes from atmospheric neutrinos, which do not exhibit the pointlike directional clustering that characterizes a distant astrophysical signal. We perform a search for neutrino point sources using the upward-going muon data from three phases of operation (SK-I, SK-II, and SK-III) spanning 2623 days of live time taken from 1996 April 1 to 2007 August 11. The search looks for signals from suspected galactic and extragalactic sources, transient sources, and uncataloged sources. While we find interesting signatures from two objects-RX J1713.7-3946 (97.5% CL) and GRB 991004D (95.3% CL)-these signatures lack compelling statistical significance given trial factors. We set limits on the flux and fluence of neutrino point sources above energies of 1.6 GeV.
语种	英语 ; 英语
出版者	IOP PUBLISHING LTD ; BRISTOL ; DIRAC HOUSE, TEMPLE BACK, BRISTOL BS1 6BE, ENGLAND
内容类型	期刊论文
源URL	[http://hdl.handle.net/123456789/78867]
专题	清华大学
推荐引用方式 GB/T 7714	Thrane, E.,Abe, K.,Hayato, Y.,et al. SEARCH FOR ASTROPHYSICAL NEUTRINO POINT SOURCES AT SUPER-KAMIOKANDE[J],2010, 2010.
APA	Thrane, E..,Abe, K..,Hayato, Y..,Iida, T..,Ikeda, M..,...&Wilkes, R. J..(2010).SEARCH FOR ASTROPHYSICAL NEUTRINO POINT SOURCES AT SUPER-KAMIOKANDE..
MLA	Thrane, E.,et al."SEARCH FOR ASTROPHYSICAL NEUTRINO POINT SOURCES AT SUPER-KAMIOKANDE".(2010).

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