  We test several phenomenological scenarios of faster-than-light neutrinos, by
fitting to the experimental data from OPERA, MINOS and Fermilab79. Our purpose
is to see, from the perspective of the current data, whether or not the speed
of the superluminal neutrino depends on its energy. We show that the
Coleman-Glashow scenario in which the velocity of the neutrino is free of the
energy fits the data best. However, the result of SN1987A cannot be explained
by this model. We find that a power-law model with the power close to zero can
simultaneously explain the results of SN1987A and OPERA+MINOS+Fermilab79.
