activity
20112025
most citedThe DWARF project: Eclipsing binaries - precise clocks to discover exoplanets

58 citations · 256 across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.SR2025

The twin red giant branch system BD+20 5391 A case study of low-mass double-core evolution

M. Kurpas, M. Dorsch, S. Geier +12

Understanding interactions of binary systems on the red giant branch is crucial to understanding the formation of compact stellar remnants such as helium-core white dwarfs (He-WDs)…

astro-ph.SR2023★ 1 cited

Density asymmetry and wind velocities in the orbital plane of the symbiotic binary EG Andromedae

N. Shagatova, A. Skopal, E. Kundra +4

Context. Non-dusty late-type giants without a corona and large-scale pulsations represent objects that do not fulfil the conditions under which standard mass-loss mechanisms can be…

astro-ph.SR2022★ 4 cited

Variability of eclipse timing:the case of V471 Tauri

Emil Kundra, Ľubomír Hambálek, Siegfried Vanaverbeke +4

The post-common envelope binary V471 Tauri has been an object of interest for decades. V471 Tau shows various phenomena due to its evolutionary state and unique properties, e.g. it…

astro-ph.EP2022★ 12 cited

Revisiting the Transit Timing Variations in the TrES-3 and Qatar-1 systems with TESS data

Vineet Kumar Mannaday, Parijat Thakur, John Southworth +12

We present and analyze 58 transit light curves of TrES-3b and 98 transit light curves of Qatar-1b observed by Transiting Exoplanet Survey Satellite (TESS), plus two transit light c…

astro-ph.EP2022★ 7 cited

Rapidly rotating stars and their transiting planets: KELT-17b, KELT-19Ab, and KELT-21b in the CHEOPS and TESS era

Zoltán Garai, Theodor Pribulla, József Kovács +4

Rapidly rotating early-type main-sequence stars with transiting planets are interesting in many aspects. Unfortunately, several astrophysical effects in such systems are not well u…

astro-ph.SR2022

HD 183986: a high-contrast SB2 system with a pulsating component

Martin Vaňko, Theodor Pribulla, Pavol Gajdoš +7

There is a small group of peculiar early-type stars on the main sequence that show different rotation velocities from different spectral lines. This inconsistency might be due to t…