collaborators

10 papers

astro-ph.SR2026

Hidden massive eclipsing binaries in red supergiant systems: The hierarchical triple system KQ Puppis and other candidates

D. Jadlovský, L. Molnár, A. Ercolino +26

The majority of massive stars are part of binary systems that may interact during their evolution. However, not many RSGs are known binaries, and only a few have constrained orbita…

astro-ph.SR2026

Rotational characteristics of five photometrically variable stars

Pavlína Rutová, Marek Skarka, Jiří Žák +1

This study explores photometric variability in a sample of hot stars in order to test whether variability arises from rotational modulation due to surface temperature spots. Freque…

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.IM2026

ASTRAFier: A Novel and Scalable Transformer-based Stellar Variability Classifier

Paul F. X. Gregory, Jeroen Audenaert, Mykyta Kliapets +5

Photometric missions such as Kepler and TESS have generated millions of light curves covering almost the entire sky, offering unprecedented opportunities to study stellar variabili…

astro-ph.EP2026

Aligned, Misaligned and Polar Orbits of Hot Jupiters: Measuring Spin-Orbit Angles via Doppler Tomography with HARPS-N

Z. Balkóová, J. Žák, M. Skarka +4

Although the migration of hot Jupiters is not yet fully understood, measurements of the projected spin-orbit angle λ help shed light on the processes involved. Here we present Dop…

astro-ph.SR2025

On the origin of sinusoidal brightness variations in F to O-type stars through radial velocities

E. Šipková, M. Skarka, M. Vaňko +3

Stellar variability may originate from various phenomena such as binarity, pulsations, or rotation. These mechanisms can induce flux variations of similar magnitudes, shapes, and p…