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Development of an Early-warning Method Incorporating Presupernova Neutrino Light Curves

  • Authors: K. Saito, M. Eizuka, Z. Hu, K. Ichimura, M. Ikeda, K. Ishidoshiro, N. Kawada, L. N. Machado, Ll. Marti, K. Mikami, K. Tachibana, R. A. Wendell

K. Saito et al 2026 The Astrophysical Journal 1008 .

  • Provider: AAS Journals

Caption: Figure 2.

Time evolution of pre-SN event rate in (a) KamLAND and (b) Super-Kamiokande for stars at 150 pc. The mass orderings are assumed to be normal. The pre-SN neutrino light-curve models are summarized in Table 1.

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