Abstract
The configuration-interaction method as implemented in the computer code CIV3 is used to determine energy levels, electric dipole radiative transition wavelengths, oscillator strengths and transition probabilities for inner-shell excitation of transitions in Fe xv and Fe XVI. Specifically, transitions are considered of the type 1s22s22p63s 2-1s22s22p53l3l′3lPrime; (l, l′ and l″ = s, p or d) in Fe xv and 1s22s 22p63s-1s22s22p 53l3l′ (l and l′ = s,p or d) in Fe XVI, using the relativistic Breit-Pauli approach. An assessment of the accuracy of the derived atomic data is performed.
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Kisielius, R., Hibbert, A., Ferland, G. J., Foord, M. E., Rose, S. J., Van Hoof, P. A. M., & Keenan, F. P. (2003). Inner-shell photoexcitation of Fe XV and Fe XVI. Monthly Notices of the Royal Astronomical Society, 344(3), 696–706. https://doi.org/10.1046/j.1365-8711.2003.06801.x
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