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Abstract
We present calculations of energy levels and transition probabilities in 3d and 3d9 configurations along the potassium and cobalt sequences for the ions Ti IV to Ag XXIX and Cu III to Dy XL, respectively. Similarly to previous investigations in 3pn and 4pn configurations, approximate relativistic Hartree-Fock wavefunctions were obtained from Cowan's code. The average energy and spin-orbit parameters for the 3d (3d9) configurations were adjusted so as to reproduce the observed splittings of the 2D terms or were deduced from the trends of these parameters along the sequences when experimental energy level values are missing.
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