Passer à la navigation principale Passer à la recherche Passer au contenu principal

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
  • University of Tokyo
  • Universidad Autónoma de Madrid
  • British Columbia Institute of Technology
  • TRIUMF
  • Boston University
  • Long Beach VA and University of California
  • California State University, Dominguez Hills
  • Chonnam National University
  • Duke University
  • Ip Paris
  • Fukuoka Institute of Technology
  • Gifu University
  • Gwangju Institute of Science and Technology
  • University of Hawaii
  • Imperial College London
  • Politecnico di Bari
  • University of Naples Federico II
  • University of Padova
  • University of Rome
  • International Laboratory for Astrophysics
  • Keio University
  • High Energy Accelerator Research Organization (KEK)
  • Kobe University
  • University of Liverpool
  • Miyagi University of Education
  • Nagoya University
  • National Centre for Nuclear Research (NCBJ)
  • Stony Brook University
  • Okayama University
  • University of Oxford
  • CCLRC Rutherford Appleton Laboratory
  • King's College London
  • Seoul National University
  • The University of Sheffield
  • Shizuoka University of Welfare
  • Sungkyunkwan University
  • Tokai University
  • Tokyo Institute of Technology
  • 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 (IBS)

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

16 Citations (Scopus)

Résumé

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.

langue originaleAnglais
Numéro d'article35
journalAstrophysical Journal
Volume938
Numéro de publication1
Les DOIs
étatPublié - 1 oct. 2022

Empreinte digitale

Examiner les sujets de recherche de « Searching for Supernova Bursts in Super-Kamiokande IV ». Ensemble, ils forment une empreinte digitale unique.

Contient cette citation