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Astrophysically relevant transitions in the Mg-like ions Si III, S V and Fe XV have been studied. A J -dependent CIV3 calculation, more extensive than other, earlier ones, has led to improved accuracy in the calculated energy levels and oscillator strengths. Independent relativistic quantum defect orbital and multiconfigurational Dirac-Fock calculations have also been performed. An analysis of the results is given.
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Almaraz et al. (2000) studied this question.
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