2 papers
astro-ph.SR2026
Extending TESS flare frequency distributions with CHEOPS: Power-law versus lognormal
Julien Poyatos, Octavi Fors, José Maria Gómez Cama
Stellar flares are intense bursts of radiation caused by magnetic reconnection on active stars. They are especially frequent on M dwarfs, where they can significantly influence the…
astro-ph.SR2025
Enhancing the detection of low-energy M dwarf flares: Wavelet-based denoising of CHEOPS data
J. Poyatos, O. Fors, J. M. Gómez Cama +1
Stellar flares are powerful bursts of electromagnetic radiation triggered by magnetic reconnection in the chromosphere of stars, occurring frequently and intensely on active M dwar…