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2019ApJS..245....9S - Astrophys. J., Suppl. Ser., 245, 9-9 (2019/November-0)

Relativistic MR-MP energy levels for L-shell ions of iron.

SANTANA J.A., PENA-COTTO E.L., MORALES BUTLER E.J., BEIERSDORFER P. and BROWN G.V.

Abstract (from CDS):

A comprehensive set of level energies is provided for the valence and K-vacancy states of the ions Fe XVII, Fe XVIII, Fe XIX, Fe XX, Fe XXI, Fe XXII, Fe XXIII, and Fe XXIV. Level energies were calculated with the relativistic Multi-Reference Moller-Plesset Perturbation Theory method (MR-MP). The data set includes level energies coming from the configurations 1s22(s,p)q, 1s22(s,p)q–1nl, 1s12(s,p)q+1, 1s12(s,p)qnl, 2(s,p)q+2, and 2(s,p)q+1nl, where 1 <= q <= 8, n <= 5, and l <= 3. The results have been compared with data from the National Institute of Standards and Technology (NIST) online database and with previous calculations. In general, the deviation from the NIST-recommended values is below 0.6 and 1.0 eV for valence and K-vacancy level energies, respectively. However, we identify numerous outliers among the NIST-recommended values. The extensive data set presented here greatly augments the amount of available reference level energies in the NIST database for L-shell ions of Fe, and we expect our data set to ease line identification and confirm level designations.

Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.

Journal keyword(s): Atomic data benchmarking - Atomic spectroscopy - Atomic physics - Line positions - Spectroscopy

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