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Neutrinos from a Galactic core-collapse supernova will be measured byneutrino detectors minutes to days before an optical signal reaches Earth. Wepresent a novel calculation showing the ability of current and near-futureneutrino detectors to make fast predictions of the progenitor distance andplace constraints on the zero-age main sequence mass in order to inform theobserving strategy for electromagnetic follow-up. We show that for typicalGalactic supernovae, the distance can be constrained with an uncertainty of$\sim$5\% using IceCube or Hyper-K and, furthermore, the zero-age main sequencemass can be constrained for extremal values of compactness.

Measuring the distance and mass of galactic core-collapse supernovae using neutrinos