activity
20242026
collaborators

6 papers

astro-ph.SR2026

Variability classification of TESS targets in LOPS2, the first long-term pointing field of PLATO. Version 1 of the public variability catalogue

Mykyta Kliapets, Pablo Huijse, Jeroen Audenaert +28

The PLAnetary Transits and Oscillations of stars (PLATO) mission is expected to launch in January 2027. A total of 8\% of its data rate will be dedicated to complementary science t…

astro-ph.IM2025

Exploiting tidal asteroseismology in binary populations from combined space photometry and time-resolved high-resolution spectroscopy

Ema Šipková, Alex Kemp, Dario Fritzewski +4

Space-based photometry has substantially increased the number of pulsating stars found in binary systems by more than four orders of magnitude. Combined with high-resolution spectr…

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

Populations of tidal and pulsating variables in eclipsing binaries

Alex Kemp, Jasmine Vrancken, Joey S. G. Mombarg +4

In this work, we seek to characterise a large sample of 14377 main sequence eclipsing binaries in terms of their stellar, asteroseismic, and orbital properties. We conduct manual v…

astro-ph.SR2025

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

Mykyta Kliapets, Pablo Huijse, Andrew Tkachenko +4

The Transiting Exoplanet Survey Satellite (TESS) mission has observed hundreds of millions of stars, substantially contributing to the available pool of high-precision photometric…

astro-ph.SR2024

KIC 4150611: A quadruply eclipsing heptuple star system with a g-mode period-spacing pattern Asteroseismic modelling of the g-mode period-spacing pattern

Alex Kemp, Dario J Fritzewski, Timothy Van Reeth +7

In this work, we aim to estimate the stellar parameters of the primary (Aa) by performing asteroseismic analysis on its period-spacing pattern. We use the C-3PO neural network to p…