Abstract
Using a combined configuration interaction and many-body perturbation theory method, we compute the wavelengths of n → 2 (3 ≤ n ≤ 7) transitions of Fe and Ni L-shell ions. The uncertainties of the results are determined to be a few mA through extensive comparisons with existing laboratory measurements. We provide a complete line list of these X-ray transitions of Fe and Ni and incorporate them in the emissivity tables of the Astrophysical Plasma Emission Database (APED).
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