activity
20112025
most citedSpin-orbit resonance, transit duration variation and possible secular perturbations in KOI-13

70 citations · 370 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.EP2025★ 1 cited

Detection of a peculiar noise type in the TESS "fast" light curves

Sz. Kálmán, Sz. Csizmadia, A. Pál +1

We present the detection of a peculiar high-frequency noise component in the 20 second cadence SAP (Simple Aperture Photometry) light curve of TESS (Transiting Exoplanets Survey Sa…

astro-ph.EP2023★ 23 cited

A large topographic feature on the surface of the trans-Neptunian object (307261) 2002 MS measured from stellar occultations

F. L. Rommel, F. Braga-Ribas, J. L. Ortiz +201

This work aims at constraining the size, shape, and geometric albedo of the dwarf planet candidate 2002 MS4 through the analysis of nine stellar occultation events. Using multichor…

astro-ph.EP2023★ 6 cited

Converting the sub-Jovian desert of exoplanets to a savanna with TESS, PLATO and Ariel

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

There is a lack of exoplanets with sizes similar to Neptune orbiting their host stars with periods days -- hence the name ``sub-Jovian/Neptune desert''. Recently, seve…

astro-ph.SR2023★ 10 cited

TIC 219006972: A Compact, Coplanar Quadruple Star System Consisting of Two Eclipsing Binaries with an Outer Period of 168 days

Veselin B. Kostov, Tamas Borkovits, Saul A. Rappaport +12

We present the discovery of a new highly compact quadruple star system, TIC 219006972, consisting of two eclipsing binary stars with orbital periods of 8.3 days and 13.7 days, and…

astro-ph.HE2023★ 23 cited

The peak-flux of GRB 221009A measured with GRBAlpha

Jakub Ripa, Hiromitsu Takahashi, Yasushi Fukazawa +42

The brightest gamma-ray burst ever observed, long-duration GRB 221009A, was detected by GRBAlpha nano-satellite without saturation. We present light curves of the prompt emission i…

astro-ph.SR2022★ 5 cited

Photometric and spectroscopic study of the burst-like brightening of two Gaia-alerted young stellar objects

Zsófia Nagy, Péter Ábrahám, Ágnes Kóspál +18

Young stars show variability on different time-scales from hours to decades, with a range of amplitudes. We studied two young stars, which triggered the Gaia Science Alerts system…