Figure 11
A fit of the satellite XES (Eem) using the ab initio shake-off values as the relative intensities, At in equation (2). The background spectrum has been subtracted so we only have the Kα3,4 profile with no diagram spectrum. The incident energy is Einc = 9100 eV. The 2s spectrum has quite the wrong structure and would require a significant energy offset and correction. The 2p theoretical spectrum predicts the two main peaks with accurate energies, but predicts a different peak shape from experiment and omits the shoulder. Including both components and using the theoretical ab initio shake probabilities for their relative amplitudes represents the experimental data well, . |