activity
20182022
most citedSix New Compact Triply Eclipsing Triples Found With TESS

46 citations · 94 across the 8 of their papers we have counts for

collaborators

11 papers

astro-ph.EP20227 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…

astro-ph.SR202246 cited

Six New Compact Triply Eclipsing Triples Found With TESS

S. A. Rappaport, T. Borkovits, R. Gagliano +21

In this work we report the discovery and analysis of six new compact triply eclipsing triple star systems found with the TESS mission: TICs 37743815, 42565581, 54060695, 178010808,…

astro-ph.EP20211 cited

Exploiting timing capabilities of the CHEOPS mission with warm-Jupiter planets

Borsato L, Piotto G, Gandolfi D +75

We present 17 transit light curves of seven known warm-Jupiters observed with the CHaracterising ExOPlanet Satellite (CHEOPS). The light curves have been collected as part of the C…

astro-ph.IM202127 cited

Ariel: Enabling planetary science across light-years

Giovanna Tinetti, Paul Eccleston, Carole Haswell +313

Ariel, the Atmospheric Remote-sensing Infrared Exoplanet Large-survey, was adopted as the fourth medium-class mission in ESA's Cosmic Vision programme to be launched in 2029. Durin…

astro-ph.SR2020

Secular changes in the orbits of the quadruple system VW LMi

T. Pribulla, E. Puha, T. Borkovits +8

VW~LMi is the tightest known quadruple system with 2+2 hierarchy. It consists of a W UMa-type eclipsing binary (P12 = 0.47755 days) and another detached non-eclipsing binary (P34 =…