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.
Sanduleak,A deep objective-prism survey for Large Magellanic Cloud members, Contribution from CTIO89(1970)
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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.