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Cited article:

HD 34736: an intensely magnetised double-lined spectroscopic binary with rapidly rotating chemically peculiar B-type components

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Monthly Notices of the Royal Astronomical Society 535 (3) 2812 (2024)
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Magnetic Doppler imaging considering atmospheric structure modifications due to local abundances: a luxury or a necessity?

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Monthly Notices of the Royal Astronomical Society 421 (4) 3004 (2012)
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Modelling of the ultraviolet and visual SED variability in the hot magnetic Ap star CU Virginis

J. Krtička, Z. Mikulášek, T. Lüftinger, et al.
Astronomy & Astrophysics 537 A14 (2012)
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Comprehensive study of the magnetic stars HD 5797 and HD 40711 with large chromium and iron overabundances

E. A. Semenko, I. A. Yakunin and E. Yu. Kuchaeva
Astronomy Letters 37 (1) 20 (2011)
https://doi.org/10.1134/S1063773710121023

Spot system and stratification of some chemical elements in the atmosphere of He-weak star HD 21699

Yu. V. Glagolevskij, A. V. Shavrina, J. Sylvestre, et al.
Astrophysical Bulletin 64 (2) 166 (2009)
https://doi.org/10.1134/S1990341309020059

A self-consistent empirical model atmosphere, abundance and stratification analysis of the benchmark roAp starα Circini

O. Kochukhov, D. Shulyak and T. Ryabchikova
Astronomy & Astrophysics 499 (3) 851 (2009)
https://doi.org/10.1051/0004-6361/200911653

Pushing the limit of instrument capabilities

Denis V. Shulyak, Werner W. Weiss, Gautier Mathys, et al.
Proceedings of the International Astronomical Union 5 (H15) 142 (2009)
https://doi.org/10.1017/S1743921310008549

Advanced model atmospheres with magnetic field effects included

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Proceedings of the International Astronomical Union 4 (S259) 407 (2008)
https://doi.org/10.1017/S1743921309030890