activity
20132025
most citedK2 Observations of SN 2018oh Reveal a Two-Component Rising Light Curve for a Type Ia Supernova

106 citations · 569 across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.EP2025

A Compact Multi-Planet System of Three Transiting Giant Planets Around TIC118798035

Rafael Brahm, Trifon Trifonov, Andrés Jordán +20

We report the discovery and characterization of three transiting giant planets in the TIC118798035 system. The three planets were identified as transiting candidates from data of t…

astro-ph.HE2025

SN 2023ixf in M101: physical parameters from bolometric light curve modeling

J. Vinko, Zs. R. Bodola, A. Godeny +25

We present new photometric observations of the core-collapse supernova SN 2023ixf occurred in M101, taken with the RC80 and BRC80 robotic telescopes in Hungary. The initial nickel…

astro-ph.HE2023★ 3 cited

SN 2022oqm: A Bright and Multi-peaked Calcium-rich Transient

S. Karthik Yadavalli, V. Ashley Villar, Luca Izzo +60

We present the photometric and spectroscopic evolution of SN 2022oqm, a nearby multi-peaked hydrogen- and helium-weak calcium-rich transient (CaRT). SN 2022oqm was detected 13.1 kp…

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.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…