For the Fixed T0 , mt-m0 spectra has been fit by
(1/2*pi*mt)d2N/dmtdy = A*exp(- mt/(T0/cosh(y))) , where T0 is the global
temperature at which Mike Heffner obtained it from his proton, pion and
helion confidence contours, A is the amplitude or the normalization
factor.
For the Free T0 , mt-m0 spectra has been fit by
(1/2*pi*mt)d2N/dmtdy = A*exp(- mt/T) , then T0 = T*cosh(y), A is the
amplitude or the normalization
factor.