A new relative-time-offset alignment of SN1987A detector clocks favors an accretion-phase electron anti-neutrino origin for the first Kamiokande-II event over a neutronization-burst origin by a likelihood ratio of 3-6.
Krauss,Neutrino Spectroscopy of the Supernova Sn1987a,Nature329(1987) 689
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The temporal distribution of SN1987A neutrino events
A new relative-time-offset alignment of SN1987A detector clocks favors an accretion-phase electron anti-neutrino origin for the first Kamiokande-II event over a neutronization-burst origin by a likelihood ratio of 3-6.