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Cited article:

Improving the stellar age determination through joint modeling of binarity and asteroseismology

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Toward a Comprehensive Grid of Cepheid Models with MESA. I. Uncertainties of the Evolutionary Tracks of Intermediate-mass Stars

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Stellar model calibrations with the Ai Phe binary system

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Surface brightness-colour relations of dwarf stars from detached eclipsing binaries

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Tidally perturbed oblique pulsations in the hierarchical triple system V1031 Orionis

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Discovery of β Cep pulsations in the eclipsing binary V453 Cygni

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The mass discrepancy in intermediate- and high-mass eclipsing binaries: The need for higher convective core masses

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Astronomy & Astrophysics 637 A60 (2020)
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Examining the Relationship Between Convective Core Overshoot and Stellar Properties Using Asteroseismology

Lucas S. Viani and Sarbani Basu
The Astrophysical Journal 904 (1) 22 (2020)
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Asteroseismic age estimates of RGB stars in open clusters

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https://doi.org/10.1051/0004-6361/201833928