Publications [#248162] of Kate Scholberg

Papers Published
  1. Gando, Y; Fukuda, S; Fukuda, Y; Ishitsuka, M; Itow, Y; Kajita, T; Kameda, J; Kaneyuki, K; Kobayashi, K; Koshio, Y; Miura, M; Moriyama, S; Nakahata, M; Nakayama, S; Namba, T; Obayashi, Y; Okada, A; Ooyabu, T; Saji, C; Sakurai, N; Shiozawa, M; Suzuki, Y; Takeuchi, H; Takeuchi, Y; Totsuka, Y; Yamada, S; Desai, S; Earl, M; Kearns, E; Messier, MD; Stone, JL; Sulak, LR; Walter, CW; Goldhaber, M; Barszczak, T; Casper, D; Gajewski, W; Kropp, WR; Mine, S; Liu, DW; Smy, MB; Sobel, HW; Vagins, MR; Gago, A; Ganezer, KS; Hill, J; Keig, WE; Ellsworth, RW; Tasaka, S; Kibayashi, A; Learned, JG; Matsuno, S; Takemori, D; Hayato, Y; Ichikawa, AK; Ishii, T; Kobayashi, T; Maruyama, T; Nakamura, K; Oyama, Y; Sakuda, M; Yoshida, M; Kohama, M; Iwashita, T; Suzuki, AT; Inagaki, T; Kato, I; Nakaya, T; Nishikawa, K; Haines, TJ; Dazeley, S; Hatakeyama, S; Svoboda, R; Blaufuss, E; Chen, ML; Goodman, JA; Guillian, G; Sullivan, GW; Turcan, D; Scholberg, K; Habig, A; Ackermann, M; Jung, CK; Martens, K; Malek, M; Mauger, C; McGrew, C; Sharkey, E; Viren, B; Yanagisawa, C; Toshito, T; Mitsuda, C; Miyano, K; Shibata, T; Kajiyama, Y; Nagashima, Y; Nitta, K; Takita, M; Kim, HI; Kim, SB; Yoo, J; Okazawa, H; Ishizuka, T; Etoh, M; Hasegawa, T; Inoue, K; Ishihara, K; Shirai, J; Suzuki, A; Koshiba, M; Hatakeyama, Y; Ichikawa, Y; Koike, M; Nishijima, K; Ishino, H; Morii, M; Nishimura, R; Watanabe, Y; Kielczewska, D; Berns, HG; Boyd, SC; Stachyra, AL; Wilkes, RJ; Super-Kamiokande Collaboration,, Search for nu(e) from the sun at Super-Kamiokande-I., Physical Review Letters, vol. 90 no. 17 (May, 2003), pp. 171302 [12786067], [doi] .

    Abstract:
    We present the results of a search for low energy nu(e) from the Sun using 1496 days of data from Super-Kamiokande-I. We observe no significant excess of events and set an upper limit for the conversion probability to nu(e) of the 8B solar neutrino. This conversion limit is 0.8% (90% C.L.) of the standard solar model's neutrino flux for total energy=8-20 MeV. We also set a flux limit for monochromatic nu(e) for E(nu(e))=10-17 MeV.