activity
20042025
most citedKepler Asteroseismology Program: Introduction and First Results

480 citations · 2.2k across the 41 of their papers we have counts for

collaborators

41 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.EP2023★ 14 cited

Sub-Jovian desert of exoplanets at its boundaries. Parameter dependence along the main sequence

Gyula M. Szabó, Szilárd Kálmán, Luca Borsato +3

Context. The lack of sub-Jovian planets on orbits of days is a puzzling aspect of galaxy formation with regard to the distribution of exoplanets whose origins are…

astro-ph.SR2022★ 18 cited

Variable star classification with a Multiple-Input Neural Network

T. Szklenár, A. Bódi, D. Tarczay-Nehéz +3

In this experiment, we created a Multiple-Input Neural Network, consisting of Convolutional and Multi-layer Neural Networks. With this setup the selected highest-performing neural…

astro-ph.IM2022★ 8 cited

Rubin Observatory LSST Transients and Variable Stars Roadmap

Kelly M. Hambleton, Federica B. Bianco, Rachel Street +79

The Vera C. Rubin Legacy Survey of Space and Time holds the potential to revolutionize time domain astrophysics, reaching completely unexplored areas of the Universe and mapping va…

astro-ph.SR2021★ 42 cited

First results on RR Lyrae stars with the TESS space telescope: untangling the connections between mode content, colors and distances

László Molnár, Attila Bódi, András Pál +25

The TESS space telescope is collecting continuous, high-precision optical photometry of stars throughout the sky, including thousands of RR Lyrae stars. In this paper, we present r…

astro-ph.SR2021

Background Short Period Kepler Eclipsing Binaries

John Bienias, Attila Bódi, Adrienn Forró +2

During the primary Kepler mission, between 2009 and 2013, about 150,000 pre-selected targets were observed with a 29.42 minute-long cadence. However, a survey of background stars t…