Abstract
With a view to finding suitable transitions to be assigned to high-energy satellites of the L gamma spectra, the fine structure of each of the transitions (2p)-1 to (4d)-1 and (2s)-1 to (4p)-1 in presence of an additional M-shell vacancy has been studied. The transition energies have been calculated in the intermediate coupling limit using recent data on Auger transitions. It has been reported that excepting gamma '2, which arises from a single transition, each of the L gamma satellites arises from superposition of closely spaced lines corresponding to more than one transition. Two satellites reported in the L gamma spectrum of barium have been re-identified. It is suggested that the satellite gamma "2 should be renamed as gamma '3.

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