Cascade-affected emission spectra of argon, krypton and xenon

Argon M-1-M-23, krypton N-1-N-23 and xenon O-1-O-23 emission spectra emitted during the cascading de-excitations of initial vacancies in the atomic inner subshells are calculated by straightforward construction of de-excitation trees in the configuration-averaged Hartree-Fock approximation. The spectra have complex spectator-vacancy satellite structures, reflecting the dynamics of the de-excitation processes.