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Showing papers by "K. Ishihara published in 2007"


Journal ArticleDOI
G. Guillian1, J. Hosaka2, K. Ishihara2, J. Kameda2, Yusuke Koshio2, A. Minamino2, C. Mitsuda2, M. Miura2, Shigetaka Moriyama2, Masayuki Nakahata2, Toshio Namba2, Y. Obayashi2, H. Ogawa2, Masato Shiozawa2, Yasunari Suzuki2, Atsushi Takeda2, Y. Takeuchi2, Shinya Yamada2, I. Higuchi2, M. Ishitsuka2, Takaaki Kajita2, K. Kaneyuki2, G. Mitsuka2, Shoei Nakayama2, H. Nishino2, A. Okada2, Ko Okumura2, C. Saji2, Y. Takenaga2, Shantanu Desai3, Shantanu Desai4, E. Kearns3, J. L. Stone3, L. R. Sulak3, W. Wang3, M. Goldhaber5, David William Casper6, W. Gajewski6, J. Griskevich6, W. R. Kropp6, D. W. Liu6, S. Mine6, Michael B. Smy6, H. W. Sobel6, Mark R. Vagins6, K. S. Ganezer7, John Hill7, W. E. Keig7, Kate Scholberg8, C. W. Walter8, R. W. Ellsworth9, Shigeki Tasaka10, A. Kibayashi, J. G. Learned, S. Matsuno, M. D. Messier11, Y. Hayato, A. K. Ichikawa, T. Ishida, T. Ishii, T. Iwashita, T. Kobayashi, T. Nakadaira, K. Nakamura, K. Nitta, Yuichi Oyama, Y. Totsuka, Atsumu Suzuki12, Masaya Hasegawa13, I. Kato13, H. Maesaka13, Tsuyoshi Nakaya13, K. Nishikawa13, Hiroshi Sato13, Shoji Yamamoto13, Masashi Yokoyama13, Todd Haines14, S. Dazeley15, S. Hatakeyama15, R. Svoboda15, E. Blaufuss16, J. A. Goodman16, G. W. Sullivan16, D. Turcan16, Alec Habig17, Y. Fukuda18, Yoshitaka Itow19, Makoto Sakuda20, Minoru Yoshida21, S. B. Kim22, J. Yoo22, H. Okazawa, T. Ishizuka23, C. K. Jung24, T. Kato24, Katsuhiro Kobayashi24, M. Malek24, C. Mauger24, C. McGrew24, E. Sharkey24, C. Yanagisawa24, Y. Gando25, Takehisa Hasegawa25, Kunio Inoue25, J. Shirai25, A. Suzuki25, Kyoshi Nishijima26, Hirokazu Ishino27, Y. Watanabe27, Masatoshi Koshiba2, D. Kielczewska6, D. Kielczewska28, H. G. Berns29, R. Gran29, R. Gran17, K. K. Shiraishi29, A. L. Stachyra29, K. Washburn29, R. J. Wilkes29, Kazuoki Munakata30 
TL;DR: In this article, the first 2D celestial map of primary cosmic-ray flux was obtained from 2.10 10 8 8 cosmic ray muons accumulated in 1662.0 days of Super-Kamiokande, which indicated an (0:104 0:020)% excess region in the constellation of Taurus and a ( 0:094 0:014)% deficit region toward Virgo.
Abstract: A first-ever 2-dimensional celestial map of primary cosmic-ray flux was obtained from 2:10 10 8 cosmic-ray muons accumulated in 1662.0 days of Super-Kamiokande. The celestial map indicates an (0:104 0:020)% excess region in the constellation of Taurus and a (0:094 0:014)% deficit region toward Virgo. Interpretations of this anisotropy are discussed.

179 citations


Journal ArticleDOI
M. Ikeda1, Atsushi Takeda2, Y. Fukuda3, Mark R. Vagins4, K. Abe2, T. Iida2, K. Ishihara2, J. Kameda2, Yusuke Koshio2, A. Minamino2, C. Mitsuda2, M. Miura2, Shigetaka Moriyama2, Masayuki Nakahata2, Y. Obayashi2, H. Ogawa2, Hiroyuki Sekiya2, Masato Shiozawa2, Yasunari Suzuki2, Y. Takeuchi2, K. Ueshima2, Haruki Watanabe2, S. Yamada2, I. Higuchi2, C. Ishihara2, M. Ishitsuka2, Takaaki Kajita2, K. Kaneyuki2, G. Mitsuka2, Shoei Nakayama2, H. Nishino2, Ko Okumura2, C. Saji2, Y. Takenaga2, S. Clark5, Shantanu Desai6, Shantanu Desai5, Frédéric Dufour5, E. Kearns5, S. Likhoded5, Michael Litos5, J. L. Raaf5, J. L. Stone5, Lawrence Sulak5, W. Wang5, M. Goldhaber7, David William Casper4, J. P. Cravens4, J. Dunmore4, W. R. Kropp4, D. W. Liu4, S. Mine4, C. Regis4, Michael B. Smy4, Henry W. Sobel4, K. S. Ganezer8, John Hill8, W. E. Keig8, J. S. Jang9, J. Y. Kim9, I. T. Lim9, Kate Scholberg10, N. Tanimoto10, C. W. Walter10, R. A. Wendell10, R. W. Ellsworth11, Shigeki Tasaka12, G. Guillian13, John G. Learned13, S. Matsuno13, M. D. Messier14, Y. Hayato2, Y. Hayato15, A. K. Ichikawa15, T. Ishida15, T. Ishii15, T. Iwashita15, T. Kobayashi15, T. Nakadaira15, Koji Nakamura15, K. Nitta15, Yuichi Oyama15, Y. Totsuka15, Y. Totsuka2, Atsumu Suzuki16, Masaya Hasegawa17, Katsuki Hiraide17, H. Maesaka17, Tsuyoshi Nakaya17, K. Nishikawa15, Takanori Sasaki17, Shoji Yamamoto17, Masashi Yokoyama17, T. J. Haines18, T. J. Haines4, S. Dazeley19, S. Hatakeyama19, R. Svoboda19, G. W. Sullivan20, D. Turcan20, Alec Habig21, T. Sato3, Yoshitaka Itow22, T. Koike22, Tetsuya S. Tanaka22, C. K. Jung23, T. Kato23, Katsuhiro Kobayashi23, Magdalena Malek23, C. McGrew23, A. Sarrat23, R. Terri23, C. Yanagisawa23, N. Tamura24, Y. Idehara1, Makoto Sakuda1, M. Sugihara1, Y. Kuno25, Minoru Yoshida25, S. B. Kim26, B. S. Yang26, J. Yoo26, T. Ishizuka27, H. Okazawa27, Y. Choi28, H. Seo28, Y. Gando29, Takehisa Hasegawa29, Kunio Inoue29, Y. Furuse30, H. Ishii30, Kyoshi Nishijima30, Hirokazu Ishino31, Y. Watanabe31, Masatoshi Koshiba2, Shaomin Chen32, Zhi Deng32, Yueh-Feng Liu32, D. Kielczewska4, D. Kielczewska33, J. Zalipska33, H. G. Berns34, R. Gran34, R. Gran21, K. K. Shiraishi34, A. L. Stachyra34, E. Thrane34, K. Washburn34, R. J. Wilkes34 
TL;DR: In this article, the results of a search for neutrino bursts from supernova explosions using the Super-Kamiokande detector were reported, showing that the expected number of events comprising such a burst is 104, and the average energy of the neutrinos is in the range of a few tens of MeV for a core-collapse supernova explosion at a typical distance in our galaxy (10 kpc); this strong signal means that the detection efficiency anywhere within our galaxy and well past the Magellanic Clouds should be 100%.
Abstract: We report the results of a search for neutrino bursts from supernova explosions using the Super-Kamiokande detector. Super-Kamiokande is sensitive to core-collapse supernova explosions via observation of their neutrino emissions. The expected number of events comprising such a burst is ~104, and the average energy of the neutrinos is in the range of a few tens of MeV for a core-collapse supernova explosion at a typical distance in our galaxy (10 kpc); this strong signal means that the detection efficiency anywhere within our galaxy and well past the Magellanic Clouds should be 100%. We examined a data set taken from 1996 May to 2001 July, and from 2002 December to 2005 October, corresponding to 2589.2 live days. However, there is no evidence of such a supernova explosion during the data-taking period. The 90% C.L. upper limit on the rate of core-collapse supernova explosions out to distances of 100 kpc is found to be 0.32 SN yr-1.

167 citations


Journal ArticleDOI
Y. Takenaga, Ke. Abe, Y. Hayato, T. Iida, K. Ishihara, J. Kameda, Yusuke Koshio, A. Minamino, C. Mitsuda, M. Miura, S. Moriyama, Masayuki Nakahata, Y. Obayashi, H. Ogawa, Masato Shiozawa, Yasunari Suzuki, Atsushi Takeda, Y. Takeuchi, K. Ueshima, Hiroshi Watanabe, S. Yamada, I. Higuchi, C. Ishihara, Masaki Ishitsuka, T. Kajita, K. Kaneyuki, G. Mitsuka, S. Nakayama, H. Nishino, Ko Okumura, C. Saji, Y. Totsuka, S. Clark, Shantanu Desai, F. Dufour, A. Herfurth, E. Kearns, S. Likhoded, Michael Litos, J. L. Raaf, J. L. Stone, Lawrence Sulak, W. Wang, M. Goldhaber, David William Casper, J. P. Cravens, J. Dunmore, J. Griskevich, W. R. Kropp, D. W. Liu, S. Mine, C. Regis, M. B. Smy, H. W. Sobel, M. R. Vagins, K. S. Ganezer, J. Hill, W. E. Keig, J. S. Jang, J. Y. Kim, I. T. Lim, Kate Scholberg, N. Tanimoto, C. W. Walter, R. A. Wendell, R. W. Ellsworth, Shigeki Tasaka, E. Guillian, John G. Learned, S. Matsuno, M. D. Messier, A. K. Ichikawa, T. Ishida, T. Ishii, T. Iwashita, T. Kobayashi, T. Nakadaira, K. Nakamura, K. Nishikawa, K. Nitta, Yuichi Oyama, A. T. Suzuki, Makoto Hasegawa, H. Maesaka, Tsuyoshi Nakaya, Takuya Sasaki, Hiroshi Sato, Shoji Yamamoto, Masashi Yokoyama, T. J. Haines, Steven Dazeley, S. Hatakeyama, R. Svoboda, G. W. Sullivan, R. Gran, Alec Habig, Y. Fukuda, T. Sato, Y. Itow1, Y. Itow2, T. Koike2, T. Koike1, C. K. Jung, T. Kato, Ken-ichiro Kobayashi, C. McGrew, A. Sarrat, R. Terri, C. Yanagisawa, N. Tamura, Makoto Sakuda, M. Sugihara, Y. Kuno, Michitoshi Yoshida, S. B. Kim, B. S. Yang, T. Ishizuka, H. Okazawa, Y. Choi, H. Seo, Y. Gando, Takehisa Hasegawa, Kunio Inoue, H. Ishii, K. Nishijima, Hirokazu Ishino, Y. Watanabe, M. Koshiba, Song Chen, Zhi Deng, Yueh-Feng Liu, D. Kielczewska, H. G. Berns, K. K. Shiraishi, Eric Thrane, K. Washburn, R. J. Wilkes 
TL;DR: A search for Q-balls has been carried out in Super-Kamiokande II with 541.7 days of live time as mentioned in this paper, but no candidate for successive contained event groups has been found.

34 citations