Abstract
Complete data sets of level energies, transition wavelengths, A-values, radiative and Auger widths and fluorescence yields for K-vacancy levels of the F, Na, P, Cl, K, Sc, Ti, V, Cr, Mn, Co, Cu and Zn isonuclear sequences have been computed by a Hartree-Fock method that includes relativistic corrections as implemented in Cowan's atomic structure computer suite. The atomic parameters for more than 3 million fine-structure K lines have been determined. Ions with electron number N > 9 are treated for the first time, and detailed comparisons with available measurements and theoretical data for ions with N ≤ 9 are carried out in order to estimate reliable accuracy ratings. © 2012 ESO.
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Palmeri, P., Quinet, P., Mendoza, C., Bautista, M. A., García, J., Witthoeft, M. C., & Kallman, T. R. (2012). Atomic decay data for modeling K lines of iron peak and light odd-Z elements. Astronomy and Astrophysics, 543. https://doi.org/10.1051/0004-6361/201219438
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