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Surface brightness-colour relations of dwarf stars from detached eclipsing binaries
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Characterisation of magnetic activity of M dwarfs
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Surface brightness–colour relations of Cepheids calibrated by optical interferometry
M. C. Bailleul, N. Nardetto, V. Hocdé, P. Kervella, W. Gieren, J. Storm, G. Pietrzyński, A. Gallenne, A. Mérand, G. Bras, A. Recio Blanco, P. de Laverny, P. A. Palicio, A. Afanasiev and W. Kiviaho Astronomy & Astrophysics 698 A46 (2025) https://doi.org/10.1051/0004-6361/202553740
Asteroseismology of the Nearby K Dwarf σ Draconis Using the Keck Planet Finder and TESS
Marc Hon, Daniel Huber, Yaguang Li, Travis S. Metcalfe, Timothy R. Bedding, Joel Ong, Ashley Chontos, Ryan Rubenzahl, Samuel Halverson, Rafael A. García, Hans Kjeldsen, Dennis Stello, Daniel R. Hey, Tiago Campante, Andrew W. Howard, Steven R. Gibson, Kodi Rider, Arpita Roy, Ashley D. Baker, Jerry Edelstein, Chris Smith, Benjamin J. Fulton, Josh Walawender, Max Brodheim, Matt Brown, et al. The Astrophysical Journal 975(1) 147 (2024) https://doi.org/10.3847/1538-4357/ad76a9
Optimised use of interferometry, spectroscopy, and stellar atmosphere models for determining the fundamental parameters of stars
N. Ebrahimkutty, M. R. Gent, D. Mourard, A. Domiciano de Souza, M. Bergemann, T. Morel, G. Morello, N. Nardetto and B. Plez Astronomy & Astrophysics 691 A207 (2024) https://doi.org/10.1051/0004-6361/202450105
Gaia FGK benchmark stars: Fundamental Teff and log g of the third version
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Accurate and Model-independent Radius Determination of Single FGK and M Dwarfs Using Gaia DR3 Data
A Distance Determination to the Small Magellanic Cloud with an Accuracy of Better than Two Percent Based on Late-type Eclipsing Binary Stars
Dariusz Graczyk, Grzegorz Pietrzyński, Ian B. Thompson, Wolfgang Gieren, Bartłomiej Zgirski, Sandro Villanova, Marek Górski, Piotr Wielgórski, Paulina Karczmarek, Weronika Narloch, Bogumił Pilecki, Monica Taormina, Radosław Smolec, Ksenia Suchomska, Alexandre Gallenne, Nicolas Nardetto, Jesper Storm, Rolf-Peter Kudritzki, Mikołaj Kałuszyński and Wojciech Pych The Astrophysical Journal 904(1) 13 (2020) https://doi.org/10.3847/1538-4357/abbb2b