activity
20062025
most citedHAT-P-11b: A Super-Neptune Planet Transiting a Bright K Star in the Kepler Field

420 citations · 4k across the 64 of their papers we have counts for

collaborators

66 papers

astro-ph.EP2025

Three fast-rotating Jovian Trojans identified by TESS set new population density limits

Csaba Kiss, Nóra Takács, Csilla E. Kalup +8

Here we report on the identification of the three fastest rotating Jovian Trojans with reliable population assignment, using light curve data from the Transiting Exoplanet Satellit…

astro-ph.SR2023★ 6 cited

To Grow Old and Peculiar: A Survey of Anomalous Variable Stars in M80 and Age Determination using K2 and Gaia

László Molnár, Emese Plachy, Attila Bódi +11

The globular cluster Messier 80 was monitored by the Kepler space telescope for 80 days during the K2 mission. Continuous, high-precision photometry of such an old, compact cluster…

astro-ph.EP2022★ 5 cited

The multichord stellar occultation by the centaur Bienor on January 11, 2019

E. Fernández-Valenzuela, N. Morales, M. Vara-Lubiano +42

Within our program of physical characterization of trans-Neptunian objects and centaurs, we predicted a stellar occultation by the centaur (54598) Bienor to occur on January 11, 20…

astro-ph.SR2022★ 6 cited

Mid-infrared time-domain study of recent dust production events in the extreme debris disc of TYC 4209-1322-1

A. Moór, P. Ábrahám, Á. Kóspál +23

Extreme debris discs are characterized by unusually strong mid-infrared excess emission, which often proves to be variable. The warm dust in these discs is of transient nature and…

astro-ph.SR2022★ 9 cited

Accretion and extinction variations in the low-mass pre-main sequence binary system WX Cha

Eleonora Fiorellino, Gabriella Zsidi, Agnes Kospal +5

Light curves of young star systems show photometric variability due to different kinematic, and physical processes. One of the main contributors to the photometric variability is t…

astro-ph.SR2022★ 1 cited

A gap at 1 au in the disk of DI Cha A revealed by infrared interferometry

Tímea Juhász, Péter Ábrahám, Attila Moór +6

DI Cha A is K0-type pre-main sequence star, the brightest component of a quadruple stellar system. Here we report on a detailed study of this star based on archival VLTI/MIDI and V…