학술논문
Performance of SK-Gd's Upgraded Real-time Supernova Monitoring System
Document Type
Working Paper
Author
Kashiwagi, Y.; Abe, K.; Bronner, C.; Hayato, Y.; Hiraide, K.; Hosokawa, K.; Ieki, K.; Ikeda, M.; Kameda, J.; Kanemura, Y.; Kaneshima, R.; Kataoka, Y.; Miki, S.; Mine, S.; Miura, M.; Moriyama, S.; Nakano, Y.; Nakahata, M.; Nakayama, S.; Noguchi, Y.; Sato, K.; Sekiya, H.; Shiba, H.; Shimizu, K.; Shiozawa, M.; Sonoda, Y.; Suzuki, Y.; Takeda, A.; Takemoto, Y.; Tanaka, H.; Yano, T.; Han, S.; Kajita, T.; Okumura, K.; Tashiro, T.; Tomiya, T.; Wang, X.; Yoshida, S.; Fernandez, P.; Labarga, L.; Ospina, N.; Zaldivar, B.; Pointn, B. W.; Kearns, E.; Raaf, J. L.; Wan, L.; Wester, T.; Bian, J.; Griskevich, N. J.; Locke, S.; Smy, M. B.; Sobel, H. W.; Takhistov, V.; Yankelevich, A.; Hill, J.; Jang, M. C.; Lee, S. H.; Moon, D. H.; Park, R. G.; Bodur, B.; Scholberg, K.; Walter, C. W.; Beauchêne, A.; Drapier, O.; Giampaolo, A.; Mueller, Th. A.; Santos, A. D.; Paganini, P.; Quilain, B.; Rogly, R.; Nakamura, T.; Jang, J. S.; Machado, L. N.; Learned, J. G.; Choi, K.; Iovine, N.; Cao, S.; Anthony, L. H. V.; Martin, D.; Prouse, N. W.; Scott, M.; Sztuc, A. A.; Uchida, Y.; Berardi, V.; Catanesi, M. G.; Radicioni, E.; Calabria, N. F.; Langella, A.; De Rosa, G.; Collazuol, G.; Iacob, F.; Mattiazzi, M.; Ludovici, L.; Gonin, M.; Périssé, L.; Pronost, G.; Fujisawa, C.; Maekawa, Y.; Nishimura, Y.; Okazaki, R.; Akutsu, R.; Friend, M.; Hasegawa, T.; Ishida, T.; Kobayashi, T.; Jakkapu, M.; Matsubara, T.; Nakadaira, T.; Nakamura, K.; Oyama, Y.; Sakashita, K.; Sekiguchi, T.; Tsukamoto, T.; Bhuiyan, N.; Burton, G. T.; Di Lodovico, F.; Gao, J.; Goldsack, A.; Katori, T.; Migenda, J.; Ramsden, R. M.; Xie, Z.; Zsoldos, S.; Suzuki, A. T.; Takagi, Y.; Takeuchi, Y.; Zhong, H.; Feng, J.; Feng, L.; Hu, J. R.; Hu, Z.; Kawaue, M.; Kikawa, T.; Mori, M.; Nakaya, T.; Wendell, R. A.; Yasutome, K.; Jenkins, S. J.; McCauley, N.; Mehta, P.; Tarrant, A.; Fukuda, Y.; Itow, Y.; Menjo, H.; Ninomiya, K.; Yoshioka, Y.; Lagoda, J.; Lakshmi, S. M.; Mandal, M.; Mijakowski, P.; Prabhu, Y. S.; Zalipska, J.; Jia, M.; Jiang, J.; Jung, C. K.; Shi, W.; Wilking, M. J.; Yanagisawa, C.; Harada, M.; Hino, Y.; Ishino, H.; Koshio, Y.; Nakanishi, F.; Sakai, S.; Tada, T.; Tano, T.; Ishizuka, T.; Barr, G.; Barrow, D.; Cook, L.; Samani, S.; Wark, D.; Holin, A.; Nova, F.; Jung, S.; Yang, B. S.; Yang, J. Y.; Yoo, J.; Fannon, J. E. P.; Kneale, L.; Malek, M.; McElwee, J. M.; Thiesse, M. D.; Thompson, L. F.; Wilson, S. T.; Okazawa, H.; Kim, S. B.; Kwon, E.; Seo, J. W.; Yu, I.; Ichikawa, A. K.; Nakamura, K. D.; Tairafune, S.; Nishijima, K.; Eguchi, A.; Nakagiri, K.; Nakajima, Y.; Shima, S.; Taniuchi, N.; Watanabe, E.; Yokoyama, M.; de Perio, P.; Fujita, S.; Jesús-Valls, C.; Martens, K.; Tsui, K. M.; Vagins, M. R.; Xia, J.; Kuze, M.; Izumiyama, S.; Matsumoto, R.; Ishitsuka, M.; Ito, H.; Ommura, Y.; Shigeta, N.; Shinoki, M.; Yamauchi, K.; Yoshida, T.; Gaur, R.; Gousy-Leblanc, V.; Hartz, M.; Konaka, A.; Li, X.; Chen, S.; Xu, B. D.; Zhang, B.; Posiadala-Zezula, M.; Boyd, S. B.; Edwards, R.; Hadley, D.; Nicholson, M.; O'Flaherty, M.; Richards, B.; Ali, A.; Jamieson, B.; Amanai, S.; Marti, Ll.; Minamino, A.; Suzuki, S.
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Abstract
Among multi-messenger observations of the next galactic core-collapse supernova, Super-Kamiokande (SK) plays a critical role in detecting the emitted supernova neutrinos, determining the direction to the supernova (SN), and notifying the astronomical community of these observations in advance of the optical signal. On 2022, SK has increased the gadolinium dissolved in its water target (SK-Gd) and has achieved a Gd concentration of 0.033%, resulting in enhanced neutron detection capability, which in turn enables more accurate determination of the supernova direction. Accordingly, SK-Gd's real-time supernova monitoring system (Abe te al. 2016b) has been upgraded. SK_SN Notice, a warning system that works together with this monitoring system, was released on December 13, 2021, and is available through GCN Notices (Barthelmy et al. 2000). When the monitoring system detects an SN-like burst of events, SK_SN Notice will automatically distribute an alarm with the reconstructed direction to the supernova candidate within a few minutes. In this paper, we present a systematic study of SK-Gd's response to a simulated galactic SN. Assuming a supernova situated at 10 kpc, neutrino fluxes from six supernova models are used to characterize SK-Gd's pointing accuracy using the same tools as the online monitoring system. The pointing accuracy is found to vary from 3-7$^\circ$ depending on the models. However, if the supernova is closer than 10 kpc, SK_SN Notice can issue an alarm with three-degree accuracy, which will benefit follow-up observations by optical telescopes with large fields of view.
Comment: 38 pages, 29 figures, 6 tables
Comment: 38 pages, 29 figures, 6 tables