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Cited article:

Evolution of the near-core rotation frequency of 2497 intermediate-mass stars from their dominant gravito-inertial mode

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Analysis of Newly Cataloged Open Star Cluster UPK 220 with Gaia DR3 and TESS: Discovering Member Variable Stars

İnci Akkaya Oralhan, Cenk Kayhan and Özgün Arslan
Publications of the Astronomical Society of the Pacific 137 (6) 064202 (2025)
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Age uncertainties of red giants due to cumulative rotational mixing of progenitors calibrated by asteroseismology

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Probability distributions of initial rotation velocities and core-boundary mixing efficiencies of γ Doradus stars

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Astronomy & Astrophysics 685 A21 (2024)
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Asteroseismology of the young open cluster NGC 2516

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Estimates of (convective core) masses, radii, and relative ages for ∼14 000 Gaia-discovered gravity-mode pulsators monitored by TESS

Joey S. G. Mombarg, Conny Aerts, Timothy Van Reeth and Daniel Hey
Astronomy & Astrophysics 691 A131 (2024)
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Ages of Stars and Planets in the Kepler Field Younger than Four Billion Years

Luke G. Bouma, Lynne A. Hillenbrand, Andrew W. Howard, Howard Isaacson, Kento Masuda and Elsa K. Palumbo
The Astrophysical Journal 976 (2) 234 (2024)
https://doi.org/10.3847/1538-4357/ad855f