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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 .

Caption: Figure 4.

Time evolution of expected FAR in SK. The pre-SN neutrino models and lines used in these plots are described in the caption of Figure 3.