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20242026
most citedVariability in hot sub-luminous stars and binaries: Machine-learning analysis of Gaia DR3 multi-epoch photometry

7 citations · 13 across the 4 of their papers we have counts for

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astro-ph.SR2025

Probing stellar rotation in the Pleiades with gravity-mode pulsators

D. J. Fritzewski, A. Kemp, G. Li +1

Due to their proximity, the Pleiades are an important benchmark open cluster. Despite its status, asteroseismic analyses of its members are rare. In particular, the gravity-mode (g…

astro-ph.SR2025

Asteroseismic predictions for a massive main-sequence merger product

J. Henneco, F. R. N. Schneider, M. Heller +2

The products of stellar mergers between two massive main-sequence (MS) stars appear as seemingly normal MS stars after a phase of thermal relaxation, if not for certain peculiariti…

astro-ph.SR20245 cited

MOCKA -- A PLATO mock asteroseismic catalogue: Simulations for gravity-mode oscillators

N. Jannsen, A. Tkachenko, P. Royer +14

With ESA's PLATO space mission set for launch in December 2026, a new photometric legacy and a future of new scientific discoveries await. In this work we investigate PLATO's poten…

astro-ph.SR20247 cited

Variability in hot sub-luminous stars and binaries: Machine-learning analysis of Gaia DR3 multi-epoch photometry

P. Ranaivomanana, M. Uzundag, C. Johnston +3

Hot sub-luminous stars represent a population of stripped and evolved red giants that is located on the extreme horizontal branch. Since they exhibit a wide range of variability du…

astro-ph.SR2024

Gaia/GSP-spec spectroscopic properties of gamma Doradus pulsators

P. de Laverny, A. Recio-Blanco, C. Aerts +1

Gaia/DR3 has provided a large sample of new g-mode pulsators, among which~11,600 are Gam Dor stars. This work present the spectroscopic parameters of these Gam Dor pulsators estima…