The time behavior of delayed neutrons from the photofission of 238U and 235U was measured for bremsstrahlung endpoint energies of 8- and 10-MeV. The data were analyzed to determine the relative abundances (βi) of the delayed-neutron groups assuming the observed time distribution can be adequately described by six groups. A comparison of the 238U results at 8- and 10-MeV, and other results at 15-MeV show no strong dependence of the βi on endpoint energy. In the case of 235U, no large differences were observed between the βi at 8- and 10-MeV, however there are marked variations for several groups at 15 MeV. Possible causes for the observed differences in the βi with endpoint energy are discussed. No evidence was found for the existence of a delayed-neutron group with a half-life in the 10 to 100 msec region