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Automated all-sky detection of γ Doradus/δ Scuti hybrids in TESS data from positive unlabelled (PU) learning

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The Period–Luminosity Relation of Long-period Variables in the Large Magellanic Cloud Observed with ATLAS

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Mode identification and ensemble asteroseismology of 119 β Cep stars detected by Gaia light curves and monitored by TESS

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Asteroseismic predictions for a massive main-sequence merger product

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A Be star that turned bright and blue during a major outburst

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

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The impact of radiative levitation on mode excitation of main-sequence B-type pulsators

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Asteroseismology of the young open cluster NGC 2516

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Age-dating the young open cluster UBC 1 with g-mode asteroseismology, gyrochronology, and isochrone fitting

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Automated eccentricity measurement from raw eclipsing binary light curves with intrinsic variability

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Unveiling the intricate symphony of nonlinear pulsation mode interactions in high-amplitude δ Scuti stars

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Non-linear three-mode coupling of gravity modes in rotating slowly pulsating B stars

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Astronomy & Astrophysics 687 A265 (2024)
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Estimates of (convective core) masses, radii, and relative ages for ∼14 000 Gaia-discovered gravity-mode pulsators monitored by TESS

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Identifying and characterising the population of hot sub-luminous stars with multi-colour MeerLICHT data

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Probing the physics in the core boundary layers of the double-lined B-type binary KIC 4930889 from its gravito-inertial modes

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A calibration point for stellar evolution from massive star asteroseismology

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Feasibility of structure inversions for gravity-mode pulsators

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V456 Cyg: An eclipsing binary with tidally perturbed g-mode pulsations

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Detection of period-spacing patterns due to the gravity modes of rotating dwarfs in the TESS southern continuous viewing zone

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K2 Photometry on Oscillation Mode Variability: The New Pulsating Hot B Subdwarf Star EPIC 220422705

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Analysis of high-resolution FEROS spectroscopy for a sample of variable B-type stars assembled from TESS photometry,

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Rossby numbers and stiffness values inferred from gravity-mode asteroseismology of rotating F- and B-type dwarfs

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Towards a systematic treatment of observational uncertainties in forward asteroseismic modelling of gravity-mode pulsators

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Astronomy & Astrophysics 656 A158 (2021)
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