From a detailed comparison of Relativistic Hartree-Fock calculations with r
ecent laser lifetime measurements in Tm II, it is shown that Cowan's code,
which has been widely used in the past for atomic structure calculations in
light elements, is adequate also for providing accurate radiative data in
heavy ions and particularly in the astrophysically important singly ionized
lanthanides provided configuration interaction and core-polarization effec
ts are consistently taken into account in the adopted physical model. (C) 1
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