“…The features between 8.5 and 10.5 eV (band A) are attributed to the 10e and 3e molecular orbitals, which are principally Fe 3d in character. 3,5 The photolines above 14 eV are typically attributed to the ligands. 5,2, 3 Baerends et al 2 and Fukuda et al 3 assigned the photolines between 13 and 17 eV (band B) to the CO(5σ ) and CO(1π ) orbitals, and those from 17 and 20 eV (band C) to the CO(4σ ) orbital.…”