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Searching for Supernova Bursts in Super-Kamiokande IV

  • M. Mori
  • , K. Abe
  • , Y. Hayato
  • , K. Hiraide
  • , K. Ieki
  • , M. Ikeda
  • , S. Imaizumi
  • , J. Kameda
  • , Y. Kanemura
  • , R. Kaneshima
  • , Y. Kashiwagi
  • , Y. Kataoka
  • , S. Miki
  • , S. Mine
  • , M. Miura
  • , S. Moriyama
  • , Y. Nagao
  • , M. Nakahata
  • , Y. Nakano
  • , S. Nakayama
  • Y. Noguchi, T. Okada, K. Okamoto, A. Orii, K. Sato, H. Sekiya, H. Shiba, K. Shimizu, M. Shiozawa, Y. Sonoda, Y. Suzuki, A. Takeda, Y. Takemoto, A. Takenaka, H. Tanaka, T. Tomiya, S. Watanabe, T. Yano, S. Yoshida, S. Han, T. Kajita, K. Okumura, T. Tashiro, X. Wang, J. Xia, G. D. Megias, D. Bravo-Berguño, P. Fernandez, L. Labarga, N. Ospina, B. Zaldivar, S. Zsoldos, B. W. Pointon, F. D.M. Blaszczyk, E. Kearns, J. L. Raaf, J. L. Stone, L. Wan, T. Wester, J. Bian, N. J. Griskevich, W. R. Kropp, S. Locke, M. B. Smy, H. W. Sobel, V. Takhistov, A. Yankelevich, J. Hill, J. Y. Kim, I. T. Lim, R. G. Park, B. Bodur, K. Scholberg, C. W. Walter, L. Bernard, A. Coffani, O. Drapier, S. El Hedri, A. Giampaolo, Th A. Mueller, P. Paganini, B. Quilain, A. D. Santos, T. Ishizuka, T. Nakamura, J. S. Jang, J. G. Learned, L. H.V. Anthony, D. Martin, M. Scott, A. A. Sztuc, Y. Uchida, V. Berardi, M. G. Catanesi, E. Radicioni, N. F. Calabria, L. N. Machado, G. De Rosa, G. Collazuol, F. Iacob, M. Lamoureux, M. Mattiazzi, L. Ludovici, M. Gonin, G. Pronost, Y. Maekawa, Y. Nishimura, C. Fujisawa, M. Friend, T. Hasegawa, T. Ishida, T. Kobayashi, M. Jakkapu, T. Matsubara, T. Nakadaira, K. Nakamura, Y. Oyama, K. Sakashita, T. Sekiguchi, T. Tsukamoto, H. Ozaki, T. Shiozawa, A. T. Suzuki, Y. Takeuchi, S. Yamamoto, Y. Kotsar, Y. Ashida, C. Bronner, J. Feng, S. Hirota, T. Kikawa, T. Nakaya, R. A. Wendell, K. Yasutome, N. McCauley, P. Mehta, K. M. Tsui, Y. Fukuda, Y. Itow, H. Menjo, K. Ninomiya, T. Niwa, M. Tsukada, J. Lagoda, S. M. Lakshmi, P. Mijakowski, J. Zalipska, M. Mandal, Y. S. Prabhu, J. Jiang, C. K. Jung, C. Vilela, M. J. Wilking, C. Yanagisawa, M. Jia, K. Hagiwara, M. Harada, T. Horai, H. Ishino, S. Ito, H. Kitagawa, Y. Koshio, W. Ma, F. Nakanishi, N. Piplani, S. Sakai, G. Barr, D. Barrow, L. Cook, S. Samani, D. Wark, F. Nova, T. Boschi, J. Gao, A. Goldsack, T. Katori, F. Di Lodovico, J. Migenda, M. Taani, S. Zsoldos, J. Y. Yang, S. J. Jenkins, M. Malek, J. M. McElwee, O. Stone, M. D. Thiesse, L. F. Thompson, H. Okazawa, S. B. Kim, J. W. Seo, I. Yu, K. Nishijima, M. Koshiba, K. Nakagiri, Y. Nakajima, K. Iwamoto, N. Taniuchi, M. Yokoyama, K. Martens, P. De Perio, M. R. Vagins, M. Kuze, S. Izumiyama, T. Yoshida, M. Inomoto, M. Ishitsuka, H. Ito, T. Kinoshita, R. Matsumoto, K. Ohta, Y. Ommura, N. Shigeta, M. Shinoki, T. Suganuma, K. Yamauchi, J. F. Martin, H. A. Tanaka, T. Towstego, R. Akutsu, V. Gousy-Leblanc, M. Hartz, A. Konaka, N. W. Prouse, S. Chen, B. D. Xu, B. Zhang, M. Posiadala-Zezula, D. Hadley, M. Nicholson, M. O'Flaherty, B. Richards, A. Ali, B. Jamieson, J. Walker, Ll Marti, A. Minamino, K. Okamoto, G. Pintaudi, R. Sasaki, S. Sano, S. Suzuki, K. Wada, S. Cao, A. Ichikawa, K. D. Nakamura, S. Tairafune, K. Choi
  • Kyoto University
  • The University of Tokyo
  • Universidad Autónoma de Madrid
  • British Columbia Institute of Technology
  • TRIUMF
  • Boston University
  • University of California at Irvine
  • California State University Dominguez Hills
  • Chonnam National University
  • Duke University
  • Laboratoire Leprince-Ringuet
  • Fukuoka Institute of Technology
  • Gifu University
  • Gwangju Institute of Science and Technology
  • University of Hawai'i at Mānoa
  • Imperial College London
  • Polytechnic University of Bari
  • University of Naples Federico II
  • University of Padua
  • University of Rome La Sapienza
  • International Laboratory for Astrophysics
  • Keio University
  • High Energy Accelerator Research Organization, Tsukuba
  • Kobe University
  • University of Liverpool
  • Miyagi University of Education
  • Nagoya University
  • National Centre for Nuclear Research
  • Stony Brook University
  • Okayama University
  • University of Oxford
  • Rutherford Appleton Laboratory
  • King's College London
  • Seoul National University
  • University of Sheffield
  • Shizuoka University of Welfare
  • Sungkyunkwan University
  • Tokai University
  • Institute of Science Tokyo
  • Tokyo University of Science
  • University of Toronto
  • Tsinghua University
  • University of Warsaw
  • University of Warwick
  • University of Winnipeg
  • Yokohama National University
  • ICISE
  • Tohoku University
  • Institute for Basic Science

Research output: Contribution to journalArticlepeer-review

Abstract

Super-Kamiokande has been searching for neutrino bursts characteristic of core-collapse supernovae continuously, in real time, since the start of operations in 1996. The present work focuses on detecting more distant supernovae whose event rate may be too small to trigger in real time, but may be identified using an offline approach. The analysis of data collected from 2008 to 2018 found no evidence of distant supernovae bursts. This establishes an upper limit of 0.29 yr-1 on the rate of core-collapse supernovae out to 100 kpc at 90% C.L. For supernovae that fail to explode and collapse directly to black holes the limit reaches to 300 kpc.

Original languageEnglish
Article number35
JournalAstrophysical Journal
Volume938
Issue number1
DOIs
StatePublished - 1 Oct 2022

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