Abstract
Resonant photoemission of Fe(100) in the vicinity of the 3p-electron excitation threshold (53 eV) has been studied as a function of emission angle and photon energy. The resonant part in the energy distributions resembles closely convolutions of the spin-split valence-band density of states of Fe, centered at constant kinetic energy. This demonstrates that Auger decay dominates the resonant feature. At the binding energy of ${\ensuremath{\Gamma}}_{25}^{\mathcal{'}\ensuremath{\uparrow}}$ the photocurrent is virtually independent of photon energy.
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