We present a direct calculation of the cross section for the reaction He-3(
e,e'p) including the radiation tail originating from bremsstrahlung process
es. This calculation is compared to measured cross sections. The calculatio
n is carried out from within a Monte Carlo simulation program so that accep
tance-averaging effects, along with a subset of possible energy losses, are
taken into account. Excellent agreement is obtained between our calculatio
n and measured data, after a correction factor fur higher-order bremsstrahl
ung is devised and applied to the tail. Industry-standard radiative correct
ions fail fur these data, and we use the results of our calculation to diss
ect the failure. Implications for design and analysis of experiments in the
Jefferson-Laboratory energy domain are discussed.