“…As shown in [7], for electron energies greater than 10 GeV, and a beam divergence less than πΎ β1 , the scatter in the energies of reflected photons relative to the Bragg energy π B does not exceed fractions of a percent. Therefore, from here forward, rather than discussing the spectral-angular distribution, we will instead discuss the DTR angular distribution π½ DTR (π B , π β² π₯ , π β² π¦ ).…”