We discuss detailed Ms of the BATSE and PYO gamma-ray burst peak-flux
distributions with Friedmann models taking into account possible densi
ty evolution and standard candle or power-law luminosity functions. A
chi(2) analysis is used to estimate the goodness of the fits, and we d
erive the significance level of limits on the density evolution and lu
minosity function parameters. Cosmological models provide a good st ov
er a range of parameter space that is physically reasonable.