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.
Krivoruchenko,A statistival analysis of angular distribution of neutrino events observed in Kamiokande-II and IMB detectors from supernova SN1987A,Z
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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.