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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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New Fe i Level Energies and Line Identifications from Stellar Spectra. III. Initial Results from UV, Optical, and Infrared Spectra

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The Astrophysical Journal Supplement Series 260 (2) 28 (2022)
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Population kinetics of many-electron atoms in ionizing plasmas studied using a continuous collisional radiative model

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Physical Review E 102 (5) (2020)
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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)
https://doi.org/10.1051/0004-6361/201629854

Comprehensive atomic wavelengths, energy levels, and hyperfine structure for singly ionized iron-group elements

Gillian Nave, Craig J. Sansonetti, Keeley Townley-Smith, Juliet C. Pickering, Anne P. Thorne, Florence Liggins and Christian Clear
Canadian Journal of Physics 95 (9) 811 (2017)
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Atomic and molecular data: data organization in A+M databases and their use for stellar spectroscopy

Tatiana Ryabchikova
The European Physical Journal D 71 (6) (2017)
https://doi.org/10.1140/epjd/e2017-80059-0

New Fe i Level Energies and Line Identifications from Stellar Spectra. II. Initial Results from New Ultraviolet Spectra of Metal-poor Stars

Ruth C. Peterson, Robert L. Kurucz and Thomas R. Ayres
The Astrophysical Journal Supplement Series 229 (2) 23 (2017)
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STELLAR ATMOSPHERES, ATMOSPHERIC EXTENSION, AND FUNDAMENTAL PARAMETERS: WEIGHING STARS USING THE STELLAR MASS INDEX

Hilding R. Neilson, Fabien Baron, Ryan Norris, Brian Kloppenborg and John B. Lester
The Astrophysical Journal 830 (2) 103 (2016)
https://doi.org/10.3847/0004-637X/830/2/103

NEW Fe I LEVEL ENERGIES AND LINE IDENTIFICATIONS FROM STELLAR SPECTRA

Ruth C. Peterson and Robert L. Kurucz
The Astrophysical Journal Supplement Series 216 (1) 1 (2014)
https://doi.org/10.1088/0067-0049/216/1/1

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

Abundance analysis, spectral variability, and search for the presence of a magnetic field in the typical PGa star HD 19400

S. Hubrig, F. Castelli, J. F. González, et al.
Monthly Notices of the Royal Astronomical Society 442 (4) 3604 (2014)
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M dwarf stars in the light of (future) exoplanet searches

B. Rojas‐Ayala, E.J. Hilton, A.W. Mann, S. Lépine, E. Gaidos, X. Bonfils, Ch. Helling, T.J. Henry, L. A. Rogers, K. von Braun and A. Youdin
Astronomische Nachrichten 334 (1-2) 155 (2013)
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Oscillator strengths for selected Fe II lines in the range λλ 300–400 nm

N. G. Shchukina and I. E. Vasil’eva
Kinematics and Physics of Celestial Bodies 29 (2) 53 (2013)
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Discovery of the longest period rapidly oscillating Ap star HD 177765

D. Alentiev, O. Kochukhov, T. Ryabchikova, M. Cunha, V. Tsymbal and W. Weiss
Monthly Notices of the Royal Astronomical Society: Letters 421 (1) L82 (2012)
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Elemental abundance analyses with DAO spectrograms. XXVIII. Comparisons with two series of automated elemental abundance analyses

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New Astronomy 16 (3) 191 (2011)
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ATOMIC DATA: DIVISION XII / COMMISSION 14 / WORKING GROUP ATOMIC DATA

Gillian Nave, Glenn M. Wahlgren and Jeffrey R. Fuhr
Proceedings of the International Astronomical Union 7 (T28A) 341 (2011)
https://doi.org/10.1017/S1743921312003080

Atomic data for stellar astrophysics: from the UV to the IR1This article is part of a Special Issue on the 10th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas.

Glenn M. Wahlgren
Canadian Journal of Physics 89 (4) 345 (2011)
https://doi.org/10.1139/p10-125