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Cited article:

Laboratory confirmation and improved accuracy of 4f and 5d energy levels of Fe ii previously identified from stellar spectra

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An abundance analysis from the STIS-HST UV spectrum of the non-magnetic Bp star HR 6000

F. Castelli, C. R. Cowley, T. R. Ayres, G. Catanzaro and F. Leone
Astronomy & Astrophysics 601 A119 (2017)
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Comprehensive atomic wavelengths, energy levels, and hyperfine structure for singly ionized iron-group elements

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Elemental Abundance Analyses with DAO Spectrograms. XXXIV. A Three-Dimensional Graphical Examination of the Elemental Abundances of the Mercury-Manganese and Metallic-Line Stars

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Publications of the Astronomical Society of the Pacific 126 (938) 345 (2014)
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Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars

Robert L. Kurucz
GeoPlanet: Earth and Planetary Sciences, Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars 63 (2014)
https://doi.org/10.1007/978-3-319-06956-2_6

ATOMIC DATA: DIVISION XII / COMMISSION 14 / WORKING GROUP ATOMIC DATA

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Proceedings of the International Astronomical Union 7 (T28A) 341 (2011)
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Including all the lines1This article is part of a Special Issue on the 10th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas.

Robert L. Kurucz
Canadian Journal of Physics 89 (4) 417 (2011)
https://doi.org/10.1139/p10-104