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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 6.

The distance dependence on warning time for a 15 M⊙ star. Reference pre-SN light-curve models correspond to 15–25 M⊙ stars at 150 pc assuming the normal mass ordering, as listed in Table 1. The alarm threshold is FAR of 1 century–1.

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