- Eötvös Loránd UniversityHU4 papers
- Konkoly ObservatoryHU3 papers
- NASA Exoplanet Science InstituteUS3 papers
- National Institute for AstrophysicsIT3 papers
- Astronomical Institute of the Slovak Academy of SciencesSK2 papers
- Astronomical Observatory of RomeIT2 papers
- Institute of Astrophysics and Space SciencesPT2 papers
- Keele UniversityGB2 papers
- Leiden UniversityNL2 papers
- Observatoire astronomique de StrasbourgFR2 papers
- University of BernCH2 papers
- University of LiègeBE2 papers
5 papers
Radio Jet Properties of the Flaring Gamma-Ray Blazar PKS 0346-27
Máté Krezinger, Sándor Frey, Krisztina Ã. Gabányi
The blazar PKS 0346-27 at redshift z=0.991 is among the most distant extragalactic sources detected in very high energy gamma-rays. It underwent a major flare reaching TeV energies…
Spin-Orbit Geometry of AU Mic b and c from Back-to-Back Transits Observed Contemporaneously with Magellan PFS, LCOGT, and CHEOPS
Zitao Lin, Gyula M. Szabó, Krzysztof Sz. ZieliÅski +37
Young planets offer a unique window into the early stages of planetary evolution. AU Mic is one of the nearest (9.8 pc) pre-main sequence stars (~20 Myr), hosting two transiting Ne…
Gaia21bja: pre-main sequence star with quasi-periodic bursts
Ãdám Mátéfy, Zsófia Nagy, Ãgnes Kóspál +12
Gaia21bja is a Gaia alerted young stellar object (YSO) that exhibits at least seven quasi-peridoic brightenings over a 20 year-long light curve with durations of 1.5-2 years and am…
The multi-planet system TOI-5624: Four transiting sub-Neptunes with an outer companion revealed by transit-timing variations
A. Bonfanti, D. Gandolfi, P. Leonardi +96
Following the 2022 alert of a TESS object of interest transiting TOI-5624 (a G7 V star 100 pc away), a CHEOPS campaign in 2023 detected four planetary signals at $P_b\approx3…
Discovery of the First Octupole Pulsation Mode in a delta Scuti Star: A Stationary l = 3 Sectoral Mode
S. A. Rappaport, R. Jayaraman, G. Handler +8
Aims. We are attempting to better understand how stellar pulsations in close binary systems are affected, and possibly induced, by tidal, Coriolis, and centrifugal forces. Methods.…