Superluminal neutrino energy spectrum of OPERA and MINOS
  We analyze the velocity dependence on energy of superluminal neutrino
recorded by the OPERA and MINOS collaborations and manage to approximate the
energy spectrum by a power law E=p+Cp^a where parameters must be taken in the
range a=0.40--1.18 and C=1.5x10^{-5}--4.15x10^{-4} (momentum and energy are
expressed in GeV). This rough estimation is constrained by the errors of
measurements, and new experimental data are requested.
