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1D non-LTE corrections for chemical abundance analyses of very metal-poor stars
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NLTE Analysis of Y i and Y ii in the Atmospheres of FGK Stars
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Metal Mixing in the r-process Enhanced Ultrafaint Dwarf Galaxy Reticulum II*
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The Pristine survey – XXII. A serendipitous discovery of an extremely Li-rich very metal-poor giant and a new method of 6Li/7Li isotope measurement
T M Sitnova, T Matsuno, Z Yuan, N F Martin, P Banerjee, F Sestito, K A Venn and J I González Hernández Monthly Notices of the Royal Astronomical Society 526(4) 5976 (2023) https://doi.org/10.1093/mnras/stad3141
Influence of departures from LTE on determinations of the scandium abundances in A–B-type stars
A blue depression in the optical spectra of M dwarfs
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Detailed abundances of the wide pairs of stars with and without planets: the binary systems 16 Cyg and HD 219542
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Accurate Metallicities for Very Metal-poor Stars from the Ca ii Infrared Triplet
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The R-process Alliance: A Nearly Complete R-process Abundance Template Derived from Ultraviolet Spectroscopy of the R-process-enhanced Metal-poor Star HD 222925*
Ian U. Roederer, James E. Lawler, Elizabeth A. Den Hartog, Vinicius M. Placco, Rebecca Surman, Timothy C. Beers, Rana Ezzeddine, Anna Frebel, Terese T. Hansen, Kohei Hattori, Erika M. Holmbeck and Charli M. Sakari The Astrophysical Journal Supplement Series 260(2) 27 (2022) https://doi.org/10.3847/1538-4365/ac5cbc
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The Pristine survey – XVII. The C-19 stream is dynamically hot and more extended than previously thought
Zhen Yuan, Nicolas F Martin, Rodrigo A Ibata, et al. Monthly Notices of the Royal Astronomical Society 514(2) 1664 (2022) https://doi.org/10.1093/mnras/stac1399
Observational constraints on the origin of the elements
The Pristine survey – IX. CFHT ESPaDOnS spectroscopic analysis of 115 bright metal-poor candidate stars
Kim A Venn, Collin L Kielty, Federico Sestito, et al. Monthly Notices of the Royal Astronomical Society 492(3) 3241 (2020) https://doi.org/10.1093/mnras/stz3546
The Gaia-ESO survey: 3D NLTE abundances in the open cluster NGC 2420 suggest atomic diffusion and turbulent mixing are at the origin of chemical abundance variations
Quantum study of inelastic processes in low-energy calcium–hydrogen collisions
A K Belyaev, D V Vlasov, A Mitrushchenkov and N Feautrier Monthly Notices of the Royal Astronomical Society 490(3) 3384 (2019) https://doi.org/10.1093/mnras/stz2763
Ca line formation in late-type stellar atmospheres
Ultra metal-poor stars: improved atmospheric parameters and NLTE abundances of magnesium and calcium
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Data on inelastic processes in low-energy potassium-hydrogen and rubidium-hydrogen collisions
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High-precision stellar abundances of the elements: methods and applications
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High-precision abundances of elements inKeplerLEGACY stars
Mega (metal-poor) not so much : Non-LTE spectroscopic stellar parameters and abundance determination of Ultra metal-poor stars
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