  We compare models of supernova (SN) neutrino emission with the Kamiokande II
data on SN 1987A using the Bayesian approach. These models are taken from
simulations and are representative of current 1D SN models. We find that models
with a brief accretion phase of neutrino emission are the most favored. This
result is not affected by varying the overall flux normalization or considering
neutrino oscillations. We also check the compatibility of the best-fit models
with the data.
