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Supernova neutrinos are invaluable signals that offer information about theinterior of supernovae. Because a nearby supernova can occur at any time,preparing for future supernova neutrino observation is an urgent task. For theprompt analysis of supernova neutrinos, we have developed a new analysis code,``Supernova Parameter Estimation Code based on Insight on Analytic Late-timeBurst Light curve at Earth Neutrino Detector (SPECIAL BLEND)''. This codeestimates the parameters of supernova based on an analytic model of supernovaneutrinos from the proto-neutron star cooling phase. For easy availability tothe community, this code is public and easily runs on web environments. SPECIALBLEND can estimate the parameters better than the analysis pipeline wedeveloped in the previous paper. By using SPECIAL BLEND, we can estimate thesupernova parameters within $10\%$ precision up to $\sim 20\,{\rm kpc}$ and$\sim 60\,{\rm kpc}$ (Large Magellanic Cloud contained) with Super Kamiokandeand Hyper Kamiokande, respectively.

Observing Supernova Neutrino Light Curves with Super-Kamiokande. IV.  Development of SPECIAL BLEND: a New Public Analysis Code for Supernova  Neutrinos