Kavli Affiliate: Sara Seager | Summary:TRAPPIST-1 is an ultra-cool dwarf that flares frequently. These flares shape the surrounding planets’ high-energy irradiation environments, with consequences for atmospheric chemistry and escape, and they can contaminate transmission spectroscopy of those planets. A quantitative flare-frequency distribution (FFD) spanning the full energy range is therefore essential for both interpreting JWST […]
Continue.. A single power law for the TRAPPIST-1 flare distribution across four orders of magnitude in energy