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Mg line formation in late-type stellar atmospheres

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Inelastic aluminium-hydrogen collision data for non-LTE applications in stellar atmospheres

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Stellar spectroscopy in the infrared at high spectral resolution

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Physica Scripta T134 014001 (2009)
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Systematic trend of water vapour absorption in red giant atmospheres revealed by high resolution TEXES 12 μm spectra

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NLTE line formation

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The44Ti-powered spectrum of SN 1987A

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Infrared transitions and oscillator strengths of Ca and Mg

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A grid of non-local thermodynamic equilibrium corrections for magnesium and calcium in late-type giant and supergiant stars: application to Gaia

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Modelling the spectrum of Mg in cool stars

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Non-LTE aluminium abundances in late-type stars

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Microwave spectroscopy of singlet Mg I inL= 0–4 Rydberg states

K B MacAdam, S F Dyubko, V A Efremov, A S Kutsenko and N L Pogrebnyak
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Mg line formation in late-type stellar atmospheres

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Are “realistic” model atmospheres realistic enough?

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Line broadening in the Si I, Si II, Si III, and Si IV spectra in the helium plasma

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NLTE Line Formation for Mg i and Mg ii in the Atmospheres of B–A–F–G–K Stars

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The Astrophysical Journal 866 (2) 153 (2018)
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The NLTE Analyses of Carbon Emission Lines in the Atmospheres of O- and B-type Stars

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NLTE analysis of Co i /Co ii lines in spectra of cool stars with new laboratory hyperfine splitting constants

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