{"paper":{"title":"Development of a data overflow protection system for Super-Kamiokande to maximize data from nearby supernovae","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE","astro-ph.SR","hep-ex"],"primary_cat":"astro-ph.IM","authors_text":"A. Ali, A. A. Sztuc, A. Beauchene, A. D. Santos, A. Eguchi, A. Giampaolo, A. Goldsack, A. Holin, A. K. Ichikawa, A. Konaka, A. Langella, A. Minamino, A. Takeda, A. Takenaka, A. Tarant, A. T. Suzuki, A. Yankelevich, B. Bodur, B. D. Xu, B. Jamieson, B. Quilain, B. Richards, B. S. Yang, B. W. Pointon, B. Zaldivar, B. Zhang, C. Bronner, C. Fujisawa, C. J. Valls, C. K. Jung, C. W. Walter, C. Yanagisawa, D. Barrow, D. Hadley, D. H. Moon, D. Martin, D. Wark, E. Kearns, E. Kwon, E. Radicioni, E. Watanabe, F. Di Lodovico, F. Iacob, F. LiCheng, F. Nakanishi, F. Nova, G. Barr, G. Collazuol, G. De Rosa, G. D. Megias, G. Pintaudi, G. Pronost, G. T. Burton, H. A. Tanaka, H. Ishino, H. Ito, H. Kitagawa, H. Menjo, H. Okazawa, H. Ozaki, H. Sekiya, H. Shiba, H. Tanaka, H. W. Sobel, H. Zhong, I. Yu, J. Bian, J. E. P. Fannon, J. Feng, J. F. Martin, J. Gao, J. G. Learned, J. Hill, J. Jiang, J. Kameda, J. Lagoda, J. L. Raaf, J. Migenda, J. M. McElwee, J. R. Hu, J. S. Jang, J. W. Seo, J. Xia, J. Yoo, J. Y. Yang, J. Zalipska, K. Abe, K. Choi, K. D. Nakamura, K. Hiraide, K. Hosokawa, K. Ieki, K. Martens, K. M. Tsui, K. Nakagiri, K. Nakamura, K. Ninomiya, K. Nishijima, K. Okamoto, K. Okumura, K. Sakashita, K. Sato, K. Scholberg, K. Shimizu, K. Wada (The Super-Kamiokande Collaboration), K. Yamauchi, K. Yasutome, L. Cook, L. F. Thompson, L. H. V. Anthony, L. Kneale, L. Labarga, Ll. Marti, L. Ludovici, L. N. Machado, L. Perisse, L. Wan, M. B. Smy, M. C. Jang, M. D. Thiesse, M. Friend, M. G. Catanesi, M. Gonin, M. Harada, M. Hartz, M. Ikeda, M. Ishitsuka, M. Jakkapu, M. Jia, M. J. Wilking, M. Kawaune, M. Kuze, M. Lamoureux, M. Malek, M. Mandal, M. Mattiazzi, M. Miura, M. Mori, M. Nakahata, M. Nicholson, M. O' Flaherty, M. Posiadala-Zezula, M. R. Vagins, M. Scott, M. Shinoki, M. Shiozawa, M. Yokoyama, N. Bhuiyan, N. F. Calabria, N. Iovine, N. J. Griskevich, N. McCauley, N. Ospina, N. Shigeta, N. Taniuchi, N. W. Prouse, O. Drapier, P. de Perio, P. Fernandez, P. Mehta, P. Mijakowski, P. Paganini, R. Akutsu, R. A. Wendell, R. Edwards, R. Gaur, R. G. Park, R. Kaneshima, R. Matsumoto, R. M. Ramsden, R. Okazaki, R. Rogly, S. Amanai, S. B. Boyd, S. B. Kim, S. Cao, S. Chen, S. Fujita, S. Han, S. H. Lee, S. Izumiyama, S. J. Jenkins, S. Jung, S. Locke, S. Miki, S. Mine, S. M. Lakshmi, S. Moriyama, S. Nakayama, S. Sakai, S. Samani, S. Sano, S. Shima, S. Suzuki, S. Tairafune, S. Watanabe, S. Wilson, S. Yoshida, S. Zsoldos, Th. A. Mueller, T. Hasegawa, T. Ishida, T. Ishizuka, T. Kajita, T. Katori, T. Kikawa, T. Kinoshita, T. Kobayashi, T. Matsubara, T. Nakadaira, T. Nakamura, T. Nakaya, T. Sekiguchi, T. Suganuma, T. Tada, T. Tano, T. Tashiro, T. Tomiya, T. Towstego, T. Tsukamoto, T. Wester, T. Yano, T. Yoshida, V. Berardi, V. Gousy-Leblanc, V. Takhistov, W. Shi, X. Li, X. Wang, Y. Fukuda, Y. Hayato, Y. Hino, Y. Itow, Y. Kanemura, Y. Kashiwagi, Y. Kataoka, Y. Koshio, Y. Kotsar, Y. Maekawa, Y. Nakajima, Y. Nakano, Y. Nishimura, Y. Noguchi, Y. Ommura, Y. Oyama, Y. Sonoda, Y. S. Prabhu, Y. Suzuki, Y. Takagi, Y. Takemoto, Y. Takeuchi, Y. Uchida, Y. Yoshioka, Z. Hu, Z. Xie","submitted_at":"2024-04-12T15:01:28Z","abstract_excerpt":"Neutrinos from very nearby supernovae, such as Betelgeuse, are expected to generate more than ten million events over 10\\,s in Super-Kamokande (SK). At such large event rates, the buffers of the SK analog-to-digital conversion board (QBEE) will overflow, causing random loss of data that is critical for understanding the dynamics of the supernova explosion mechanism. In order to solve this problem, two new DAQ modules were developed to aid in the observation of very nearby supernovae. The first of these, the SN module, is designed to save only the number of hit PMTs during a supernova burst and"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2404.08725","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2404.08725/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}