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The most metal-poor tail of the Galactic halo: Hypothesis for its origin from precise spectral analysis
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HR-GO
T. M. Sitnova, Z. Yuan, T. Matsuno, L. I. Mashonkina, S. A. Alexeeva, E. Holmbeck, F. Sestito, L. Lombardo, P. Banerjee, N. F. Martin and F. Jiang Astronomy & Astrophysics 690 A331 (2024) https://doi.org/10.1051/0004-6361/202450981
Discovery of an Extremely r-process-enhanced Thin-disk Star with [Eu/H] = +0.78
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1D non-LTE corrections for chemical abundance analyses of very metal-poor stars
L Mashonkina, Yu Pakhomov, T Sitnova, A Smogorzhevskii, P Jablonka and V Hill Monthly Notices of the Royal Astronomical Society 524(3) 3526 (2023) https://doi.org/10.1093/mnras/stad2114
The Pristine Inner Galaxy Survey (PIGS) VII: a discovery of the first inner Galaxy CEMP-r/s star
L Mashonkina, A Arentsen, D S Aguado, et al. Monthly Notices of the Royal Astronomical Society 523(2) 2111 (2023) https://doi.org/10.1093/mnras/stad1536
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
TITANS metal-poor reference stars
R. E. Giribaldi, S. Van Eck, T. Merle, A. Jorissen, P. Krynski, L. Planquart, M. Valentini, C. Chiappini and H. Van Winckel Astronomy & Astrophysics 679 A110 (2023) https://doi.org/10.1051/0004-6361/202347208
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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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Chemical composition of a palomar 12 blue straggler
L Pasquini, P Bonifacio, L Pulone, et al. Monthly Notices of the Royal Astronomical Society 512(4) 5701 (2022) https://doi.org/10.1093/mnras/stac842
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
The formation of the milky way halo and its dwarf satellites: a NLTE-1D abundance analysis. IV. Segue 1, Triangulum ii, and Coma Berenices UFDs
T M Sitnova, L I Mashonkina, A M Tatarnikov, et al. Monthly Notices of the Royal Astronomical Society 504(1) 1183 (2021) https://doi.org/10.1093/mnras/stab786
The Pristine survey – XIV. Chemical analysis of two ultra-metal-poor stars
The formation of the Milky Way halo and its dwarf satellites: A NLTE–1D abundance analysis. V. The Sextans galaxy
L Mashonkina, Yu V Pakhomov, T Sitnova, et al. Monthly Notices of the Royal Astronomical Society 509(3) 3626 (2021) https://doi.org/10.1093/mnras/stab3189
Chemical Abundance Signature of J0023+0307: A Second-generation Main-sequence Star with [Fe/H] < −6*
Anna Frebel, Alexander P. Ji, Rana Ezzeddine, Terese T. Hansen, Anirudh Chiti, Ian B. Thompson and Thibault Merle The Astrophysical Journal 871(2) 146 (2019) https://doi.org/10.3847/1538-4357/aae848
Abundances of α-Process Elements in Thin-Disk, Thick-Disk, and Halo Stars of the Galaxy: Non-LTE Analysis
Ultra metal-poor stars: improved atmospheric parameters and NLTE abundances of magnesium and calcium
A Frebel, R Ezzeddine, L I Mashonkina and T M Sitnova Monthly Notices of the Royal Astronomical Society 485(3) 3527 (2019) https://doi.org/10.1093/mnras/stz626
NLTE Line Formation for Mg i and Mg ii in the Atmospheres of B–A–F–G–K Stars
Non-local Thermodynamic Equilibrium Stellar Spectroscopy with 1D and 〈3D〉 Models. II. Chemical Properties of the Galactic Metal-poor Disk and the Halo
Maria Bergemann, Remo Collet, Ralph Schönrich, Rene Andrae, Mikhail Kovalev, Greg Ruchti, Camilla Juul Hansen and Zazralt Magic The Astrophysical Journal 847(1) 16 (2017) https://doi.org/10.3847/1538-4357/aa88b5
Mega (metal-poor) not so much : Non-LTE spectroscopic stellar parameters and abundance determination of Ultra metal-poor stars
Rana Ezzeddine, Tatyana Sitnova, Anna Frebel, Lyudmilla Mashonkina and Bertrand Plez Proceedings of the International Astronomical Union 13(S334) 259 (2017) https://doi.org/10.1017/S1743921317007177
Non-local Thermodynamic Equilibrium Stellar Spectroscopy with 1D and
Models. I. Methods and Application to Magnesium Abundances in Standard Stars
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Experimental and theoretical oscillator strengths of Mg i for accurate abundance analysis
SYSTEMATIC NON-LTE STUDY OF THE −2.6 ≤ [Fe/H] ≤ 0.2 F AND G DWARFS IN THE SOLAR NEIGHBORHOOD. II. ABUNDANCE PATTERNS FROM Li TO Eu*
G. Zhao, L. Mashonkina, H. L. Yan, S. Alexeeva, C. Kobayashi, Yu. Pakhomov, J. R. Shi, T. Sitnova, K. F. Tan, H. W. Zhang, J. B. Zhang, Z. M. Zhou, M. Bolte, Y. Q. Chen, X. Li, F. Liu and M. Zhai The Astrophysical Journal 833(2) 225 (2016) https://doi.org/10.3847/1538-4357/833/2/225
Model estimates of inelastic calcium-hydrogen collision data for non-LTE stellar atmospheres modeling
Laimons Začs, Julius Sperauskas, Aija Grankina, Viktoras Deveikis, Bogdan Kaminskyi, Yakiv Pavlenko and Faig A. Musaev The Astrophysical Journal 803(1) 17 (2015) https://doi.org/10.1088/0004-637X/803/1/17
Mg line formation in late-type stellar atmospheres
Theoretical Stark broadening parameters for spectral lines arising from the 2p5ns, 2p5np and 2p5nd electronic configurations of Mg iii
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Inelastic aluminium-hydrogen collision data for non-LTE applications in stellar atmospheres