activity
20082026
most citedStarspots Modelling and Flare Analysis on Selected MV Stars

20 citations · 137 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2026

New Approach to Superflare Energy Determination

Petr Heinzel, Robert Falewicz, Kamil Bicz +1

We present a new method for estimating the total energy radiated by stellar flares in broad-band continua, which assumes a constant emitting area but incorporates a time-dependent…

astro-ph.SR2025

Observational signs of limited flare area variation and peak flare temperatures estimations in main-sequence flaring stars

K. Bicz, R. Falewicz, P. Heinzel +8

In the study of stellar flares, traditional method of calculating total energy emitted in the continuum assumes the emission originating from a narrow chromospheric condensation re…

astro-ph.SR2024

Analysis of the Stellar Occultations During the Unprecedented Long-Duration Flare

Kamil Bicz, Robert Falewicz, Petr Heinzel +2

In strong stellar and solar flares flare loops typically appear during the decay phase, providing an additional contribution to the flare emission and, possibly, obscuring the flar…

astro-ph.SR2023

Unveiling the spectacular over 24-hour flare of star CD-36 3202

Kamil Bicz, Robert Falewicz, Małgorzata Pietras

We studied the light curve of the star CD-36 3202, observed by TESS for the presence of stellar spots and to analyze the rotationally modulated flare. We mainly wanted to model the…

astro-ph.SR2023★ 6 cited

Analysis of Solar-like X-Class Flare on Wolf 359 Observed Simultaneously with TESS and XMM-Newton

Małgorzata Pietras, Robert Falewicz, Marek Siarkowski +3

We present an analysis of a flare on the Wolf 359 star based on simultaneous observations of TESS and XMM-Newton. A stellar flare with energy comparable to an X-class solar flare i…

astro-ph.SR2022★ 20 cited

Starspots Modelling and Flare Analysis on Selected MV Stars

Kamil Bicz, Robert Falewicz, Małgorzata Pietras +2

We studied light curves of GJ 1243, YZ CMi, and V374 Peg, observed by TESS for the presence of stellar spots and stellar flares. One of the main goals was to model light curves of…