Real-time supernova neutrino burst monitor at Super-Kamiokande

K. Abe; Y. Haga; Y. Hayato; M. Ikeda; K. Iyogi; J. Kameda; Y. Kishimoto; M. Miura; S. Moriyama; M. Nakahata; Y. Nakano; S. Nakayama; H. Sekiya; M. Shiozawa; Y. Suzuki; A. Takeda; H. Tanaka; T. Tomura; K. Ueno; R. A. Wendell; T. Yokozawa; T. Irvine; T. Kajita; I. Kametani; K. Kaneyuki; K. P. Lee; T. McLachlan; Y. Nishimura; E. Richard; K. Okumura; L. Labarga; P. Fernandez; S. Berkman; H. A. Tanaka; S. Tobayama; J. Gustafson; E. Kearns; J. L. Raaf; J. L. Stone; L. R. Sulak; M. Goldhaber; G. Carminati; W. R. Kropp; S. Mine; P. Weatherly; A. Renshaw; M. B. Smy; H. W. Sobel; V. Takhistov; K. S. Ganezer; B. L. Hartfiel; J. Hill; W. E. Keig; N. Hong; J. Y. Kim; I. T. Lim; T. Akiri; A. Himmel; K. Scholberg; C. W. Walter; T. Wongjirad; T. Ishizuka; S. Tasaka; J. S. Jang; J. G. Learned; S. Matsuno; S. N. Smith; T. Hasegawa; T. Ishida; T. Ishii; T. Kobayashi; T. Nakadaira; K. Nakamura; Y. Oyama; K. Sakashita; T. Sekiguchi; T. Tsukamoto; A. T. Suzuki; Y. Takeuchi; C. Bronner; S. Hirota; K. Huang; K. Ieki; T. Kikawa; A. Minamino; A. Murakami; T. Nakaya; K. Suzuki; S. Takahashi; K. Tateishi; Y. Fukuda; K. Choi; Y. Itow; G. Mitsuka; P. Mijakowski; J. Hignight; J. Imber; C. K. Jung; C. Yanagisawa; M. J. Wilking; H. Ishino; A. Kibayashi; Y. Koshio; T. Mori; Makoto Sakuda; R. Yamaguchi; T. Yano; Y. Kuno; R. Tacik; S. B. Kim; H. Okazawa; Y. Choi; K. Nishijima; M. Koshiba; Y. Suda; Y. Totsuka; M. Yokoyama; K. Martens; Ll Marti; M. R. Vagins; J. F. Martin; P. De Perio; A. Konaka; S. Chen; Y. Zhang; K. Connolly; R. J. Wilkes

doi:10.1016/j.astropartphys.2016.04.003

Real-time supernova neutrino burst monitor at Super-Kamiokande

K. Abe, Y. Haga, Y. Hayato, M. Ikeda, K. Iyogi, J. Kameda, Y. Kishimoto, M. Miura, S. Moriyama, M. Nakahata, Y. Nakano, S. Nakayama, H. Sekiya, M. Shiozawa, Y. Suzuki, A. Takeda, H. Tanaka, T. Tomura, K. Ueno, R. A. WendellT. Yokozawa, T. Irvine, T. Kajita, I. Kametani, K. Kaneyuki, K. P. Lee, T. McLachlan, Y. Nishimura, E. Richard, K. Okumura, L. Labarga, P. Fernandez, S. Berkman, H. A. Tanaka, S. Tobayama, J. Gustafson, E. Kearns, J. L. Raaf, J. L. Stone, L. R. Sulak, M. Goldhaber, G. Carminati, W. R. Kropp, S. Mine, P. Weatherly, A. Renshaw, M. B. Smy, H. W. Sobel, V. Takhistov, K. S. Ganezer, B. L. Hartfiel, J. Hill, W. E. Keig, N. Hong, J. Y. Kim, I. T. Lim, T. Akiri, A. Himmel, K. Scholberg, C. W. Walter, T. Wongjirad, T. Ishizuka, S. Tasaka, J. S. Jang, J. G. Learned, S. Matsuno, S. N. Smith, T. Hasegawa, T. Ishida, T. Ishii, T. Kobayashi, T. Nakadaira, K. Nakamura, Y. Oyama, K. Sakashita, T. Sekiguchi, T. Tsukamoto, A. T. Suzuki, Y. Takeuchi, C. Bronner, S. Hirota, K. Huang, K. Ieki, T. Kikawa, A. Minamino, A. Murakami, T. Nakaya, K. Suzuki, S. Takahashi, K. Tateishi, Y. Fukuda, K. Choi, Y. Itow, G. Mitsuka, P. Mijakowski, J. Hignight, J. Imber, C. K. Jung, C. Yanagisawa, M. J. Wilking, H. Ishino, A. Kibayashi, Y. Koshio, T. Mori, Makoto Sakuda, R. Yamaguchi, T. Yano, Y. Kuno, R. Tacik, S. B. Kim, H. Okazawa, Y. Choi, K. Nishijima, M. Koshiba, Y. Suda, Y. Totsuka, M. Yokoyama, K. Martens, Ll Marti, M. R. Vagins, J. F. Martin, P. De Perio, A. Konaka, S. Chen, Y. Zhang, K. Connolly, R. J. Wilkes

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Abstract

We present a real-time supernova neutrino burst monitor at Super-Kamiokande (SK). Detecting supernova explosions by neutrinos in real time is crucial for giving a clear picture of the explosion mechanism. Since the neutrinos are expected to come earlier than light, a fast broadcasting of the detection may give astronomers a chance to make electromagnetic radiation observations of the explosions right at the onset. The role of the monitor includes a fast announcement of the neutrino burst detection to the world and a determination of the supernova direction. We present the online neutrino burst detection system and studies of the direction determination accuracy based on simulations at SK.

Original language	English
Pages (from-to)	39-48
Number of pages	10
Journal	Astroparticle Physics
Volume	81
DOIs	https://doi.org/10.1016/j.astropartphys.2016.04.003
Publication status	Published - Aug 1 2016

Keywords

Neutrinos
Super-Kamiokande
Supernova

ASJC Scopus subject areas

Astronomy and Astrophysics

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10.1016/j.astropartphys.2016.04.003

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Abe, K., Haga, Y., Hayato, Y., Ikeda, M., Iyogi, K., Kameda, J., Kishimoto, Y., Miura, M., Moriyama, S., Nakahata, M., Nakano, Y., Nakayama, S., Sekiya, H., Shiozawa, M., Suzuki, Y., Takeda, A., Tanaka, H., Tomura, T., Ueno, K., ... Wilkes, R. J. (2016). Real-time supernova neutrino burst monitor at Super-Kamiokande. Astroparticle Physics, 81, 39-48. https://doi.org/10.1016/j.astropartphys.2016.04.003

Abe, K, Haga, Y, Hayato, Y, Ikeda, M, Iyogi, K, Kameda, J, Kishimoto, Y, Miura, M, Moriyama, S, Nakahata, M, Nakano, Y, Nakayama, S, Sekiya, H, Shiozawa, M, Suzuki, Y, Takeda, A, Tanaka, H, Tomura, T, Ueno, K, Wendell, RA, Yokozawa, T, Irvine, T, Kajita, T, Kametani, I, Kaneyuki, K, Lee, KP, McLachlan, T, Nishimura, Y, Richard, E, Okumura, K, Labarga, L, Fernandez, P, Berkman, S, Tanaka, HA, Tobayama, S, Gustafson, J, Kearns, E, Raaf, JL, Stone, JL, Sulak, LR, Goldhaber, M, Carminati, G, Kropp, WR, Mine, S, Weatherly, P, Renshaw, A, Smy, MB, Sobel, HW, Takhistov, V, Ganezer, KS, Hartfiel, BL, Hill, J, Keig, WE, Hong, N, Kim, JY, Lim, IT, Akiri, T, Himmel, A, Scholberg, K, Walter, CW, Wongjirad, T, Ishizuka, T, Tasaka, S, Jang, JS, Learned, JG, Matsuno, S, Smith, SN, Hasegawa, T, Ishida, T, Ishii, T, Kobayashi, T, Nakadaira, T, Nakamura, K, Oyama, Y, Sakashita, K, Sekiguchi, T, Tsukamoto, T, Suzuki, AT, Takeuchi, Y, Bronner, C, Hirota, S, Huang, K, Ieki, K, Kikawa, T, Minamino, A, Murakami, A, Nakaya, T, Suzuki, K, Takahashi, S, Tateishi, K, Fukuda, Y, Choi, K, Itow, Y, Mitsuka, G, Mijakowski, P, Hignight, J, Imber, J, Jung, CK, Yanagisawa, C, Wilking, MJ, Ishino, H, Kibayashi, A, Koshio, Y, Mori, T, Sakuda, M, Yamaguchi, R, Yano, T, Kuno, Y, Tacik, R, Kim, SB, Okazawa, H, Choi, Y, Nishijima, K, Koshiba, M, Suda, Y, Totsuka, Y, Yokoyama, M, Martens, K, Marti, L, Vagins, MR, Martin, JF, De Perio, P, Konaka, A, Chen, S, Zhang, Y, Connolly, K & Wilkes, RJ 2016, 'Real-time supernova neutrino burst monitor at Super-Kamiokande', Astroparticle Physics, vol. 81, pp. 39-48. https://doi.org/10.1016/j.astropartphys.2016.04.003

@article{9469072634a64f208d9a46cebac5fd72,

title = "Real-time supernova neutrino burst monitor at Super-Kamiokande",

abstract = "We present a real-time supernova neutrino burst monitor at Super-Kamiokande (SK). Detecting supernova explosions by neutrinos in real time is crucial for giving a clear picture of the explosion mechanism. Since the neutrinos are expected to come earlier than light, a fast broadcasting of the detection may give astronomers a chance to make electromagnetic radiation observations of the explosions right at the onset. The role of the monitor includes a fast announcement of the neutrino burst detection to the world and a determination of the supernova direction. We present the online neutrino burst detection system and studies of the direction determination accuracy based on simulations at SK.",

keywords = "Neutrinos, Super-Kamiokande, Supernova",

author = "K. Abe and Y. Haga and Y. Hayato and M. Ikeda and K. Iyogi and J. Kameda and Y. Kishimoto and M. Miura and S. Moriyama and M. Nakahata and Y. Nakano and S. Nakayama and H. Sekiya and M. Shiozawa and Y. Suzuki and A. Takeda and H. Tanaka and T. Tomura and K. Ueno and Wendell, {R. A.} and T. Yokozawa and T. Irvine and T. Kajita and I. Kametani and K. Kaneyuki and Lee, {K. P.} and T. McLachlan and Y. Nishimura and E. Richard and K. Okumura and L. Labarga and P. Fernandez and S. Berkman and Tanaka, {H. A.} and S. Tobayama and J. Gustafson and E. Kearns and Raaf, {J. L.} and Stone, {J. L.} and Sulak, {L. R.} and M. Goldhaber and G. Carminati and Kropp, {W. R.} and S. Mine and P. Weatherly and A. Renshaw and Smy, {M. B.} and Sobel, {H. W.} and V. Takhistov and Ganezer, {K. S.} and Hartfiel, {B. L.} and J. Hill and Keig, {W. E.} and N. Hong and Kim, {J. Y.} and Lim, {I. T.} and T. Akiri and A. Himmel and K. Scholberg and Walter, {C. W.} and T. Wongjirad and T. Ishizuka and S. Tasaka and Jang, {J. S.} and Learned, {J. G.} and S. Matsuno and Smith, {S. N.} and T. Hasegawa and T. Ishida and T. Ishii and T. Kobayashi and T. Nakadaira and K. Nakamura and Y. Oyama and K. Sakashita and T. Sekiguchi and T. Tsukamoto and Suzuki, {A. T.} and Y. Takeuchi and C. Bronner and S. Hirota and K. Huang and K. Ieki and T. Kikawa and A. Minamino and A. Murakami and T. Nakaya and K. Suzuki and S. Takahashi and K. Tateishi and Y. Fukuda and K. Choi and Y. Itow and G. Mitsuka and P. Mijakowski and J. Hignight and J. Imber and Jung, {C. K.} and C. Yanagisawa and Wilking, {M. J.} and H. Ishino and A. Kibayashi and Y. Koshio and T. Mori and Makoto Sakuda and R. Yamaguchi and T. Yano and Y. Kuno and R. Tacik and Kim, {S. B.} and H. Okazawa and Y. Choi and K. Nishijima and M. Koshiba and Y. Suda and Y. Totsuka and M. Yokoyama and K. Martens and Ll Marti and Vagins, {M. R.} and Martin, {J. F.} and {De Perio}, P. and A. Konaka and S. Chen and Y. Zhang and K. Connolly and Wilkes, {R. J.}",

note = "Funding Information: We gratefully acknowledge the cooperation of the Kamioka Mining and Smelting Company. The Super-Kamiokande experiment has been built and operated from funding by the Japanese Ministry of Education, Culture, Sports, Science and Technology, the U.S. Department of Energy , and the U.S. National Science Foundation . Some of us have been supported by funds from the Research Foundation of Korea ( BK21 and KNRC), the Korean Ministry of Science and Technology , the National Research Foundation of Korea (NRF- 20110024009 ), the European Union (H2020 RISE-GA641540-SKPLUS), the Japan Society for the Promotion of Science , the National Natural Science Foundation of China under Grant no. 11235006 , the Natural Sciences and Engineering Research Council (NSERC) of Canada, and the Scinet and Westgrid consortia of Compute Canada. This work was partly supported by the Grant-in-Aid for Scientific Research on Innovative Areas [JSPS No. 26104006]. Publisher Copyright: {\textcopyright} 2016 Published by Elsevier B.V.",

year = "2016",

month = aug,

day = "1",

doi = "10.1016/j.astropartphys.2016.04.003",

language = "English",

volume = "81",

pages = "39--48",

journal = "Astroparticle Physics",

issn = "0927-6505",

publisher = "Elsevier",

}

TY - JOUR

T1 - Real-time supernova neutrino burst monitor at Super-Kamiokande

AU - Abe, K.

AU - Haga, Y.

AU - Hayato, Y.

AU - Ikeda, M.

AU - Iyogi, K.

AU - Kameda, J.

AU - Kishimoto, Y.

AU - Miura, M.

AU - Moriyama, S.

AU - Nakahata, M.

AU - Nakano, Y.

AU - Nakayama, S.

AU - Sekiya, H.

AU - Shiozawa, M.

AU - Suzuki, Y.

AU - Takeda, A.

AU - Tanaka, H.

AU - Tomura, T.

AU - Ueno, K.

AU - Wendell, R. A.

AU - Yokozawa, T.

AU - Irvine, T.

AU - Kajita, T.

AU - Kametani, I.

AU - Kaneyuki, K.

AU - Lee, K. P.

AU - McLachlan, T.

AU - Nishimura, Y.

AU - Richard, E.

AU - Okumura, K.

AU - Labarga, L.

AU - Fernandez, P.

AU - Berkman, S.

AU - Tanaka, H. A.

AU - Tobayama, S.

AU - Gustafson, J.

AU - Kearns, E.

AU - Raaf, J. L.

AU - Stone, J. L.

AU - Sulak, L. R.

AU - Goldhaber, M.

AU - Carminati, G.

AU - Kropp, W. R.

AU - Mine, S.

AU - Weatherly, P.

AU - Renshaw, A.

AU - Smy, M. B.

AU - Sobel, H. W.

AU - Takhistov, V.

AU - Ganezer, K. S.

AU - Hartfiel, B. L.

AU - Hill, J.

AU - Keig, W. E.

AU - Hong, N.

AU - Kim, J. Y.

AU - Lim, I. T.

AU - Akiri, T.

AU - Himmel, A.

AU - Scholberg, K.

AU - Walter, C. W.

AU - Wongjirad, T.

AU - Ishizuka, T.

AU - Tasaka, S.

AU - Jang, J. S.

AU - Learned, J. G.

AU - Matsuno, S.

AU - Smith, S. N.

AU - Hasegawa, T.

AU - Ishida, T.

AU - Ishii, T.

AU - Kobayashi, T.

AU - Nakadaira, T.

AU - Nakamura, K.

AU - Oyama, Y.

AU - Sakashita, K.

AU - Sekiguchi, T.

AU - Tsukamoto, T.

AU - Suzuki, A. T.

AU - Takeuchi, Y.

AU - Bronner, C.

AU - Hirota, S.

AU - Huang, K.

AU - Ieki, K.

AU - Kikawa, T.

AU - Minamino, A.

AU - Murakami, A.

AU - Nakaya, T.

AU - Suzuki, K.

AU - Takahashi, S.

AU - Tateishi, K.

AU - Fukuda, Y.

AU - Choi, K.

AU - Itow, Y.

AU - Mitsuka, G.

AU - Mijakowski, P.

AU - Hignight, J.

AU - Imber, J.

AU - Jung, C. K.

AU - Yanagisawa, C.

AU - Wilking, M. J.

AU - Ishino, H.

AU - Kibayashi, A.

AU - Koshio, Y.

AU - Mori, T.

AU - Sakuda, Makoto

AU - Yamaguchi, R.

AU - Yano, T.

AU - Kuno, Y.

AU - Tacik, R.

AU - Kim, S. B.

AU - Okazawa, H.

AU - Choi, Y.

AU - Nishijima, K.

AU - Koshiba, M.

AU - Suda, Y.

AU - Totsuka, Y.

AU - Yokoyama, M.

AU - Martens, K.

AU - Marti, Ll

AU - Vagins, M. R.

AU - Martin, J. F.

AU - De Perio, P.

AU - Konaka, A.

AU - Chen, S.

AU - Zhang, Y.

AU - Connolly, K.

AU - Wilkes, R. J.

N1 - Funding Information: We gratefully acknowledge the cooperation of the Kamioka Mining and Smelting Company. The Super-Kamiokande experiment has been built and operated from funding by the Japanese Ministry of Education, Culture, Sports, Science and Technology, the U.S. Department of Energy , and the U.S. National Science Foundation . Some of us have been supported by funds from the Research Foundation of Korea ( BK21 and KNRC), the Korean Ministry of Science and Technology , the National Research Foundation of Korea (NRF- 20110024009 ), the European Union (H2020 RISE-GA641540-SKPLUS), the Japan Society for the Promotion of Science , the National Natural Science Foundation of China under Grant no. 11235006 , the Natural Sciences and Engineering Research Council (NSERC) of Canada, and the Scinet and Westgrid consortia of Compute Canada. This work was partly supported by the Grant-in-Aid for Scientific Research on Innovative Areas [JSPS No. 26104006]. Publisher Copyright: © 2016 Published by Elsevier B.V.

PY - 2016/8/1

Y1 - 2016/8/1

N2 - We present a real-time supernova neutrino burst monitor at Super-Kamiokande (SK). Detecting supernova explosions by neutrinos in real time is crucial for giving a clear picture of the explosion mechanism. Since the neutrinos are expected to come earlier than light, a fast broadcasting of the detection may give astronomers a chance to make electromagnetic radiation observations of the explosions right at the onset. The role of the monitor includes a fast announcement of the neutrino burst detection to the world and a determination of the supernova direction. We present the online neutrino burst detection system and studies of the direction determination accuracy based on simulations at SK.

AB - We present a real-time supernova neutrino burst monitor at Super-Kamiokande (SK). Detecting supernova explosions by neutrinos in real time is crucial for giving a clear picture of the explosion mechanism. Since the neutrinos are expected to come earlier than light, a fast broadcasting of the detection may give astronomers a chance to make electromagnetic radiation observations of the explosions right at the onset. The role of the monitor includes a fast announcement of the neutrino burst detection to the world and a determination of the supernova direction. We present the online neutrino burst detection system and studies of the direction determination accuracy based on simulations at SK.

KW - Neutrinos

KW - Super-Kamiokande

KW - Supernova

UR - http://www.scopus.com/inward/record.url?scp=84968902005&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84968902005&partnerID=8YFLogxK

U2 - 10.1016/j.astropartphys.2016.04.003

DO - 10.1016/j.astropartphys.2016.04.003

M3 - Article

AN - SCOPUS:84968902005

SN - 0927-6505

VL - 81

SP - 39

EP - 48

JO - Astroparticle Physics

JF - Astroparticle Physics

ER -

Real-time supernova neutrino burst monitor at Super-Kamiokande

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