Magnetic storms on stars manifest as remarkable, randomly occurring changes of the
luminosity over durations that are tiny in comparison to the normal evolution of stars. These …

We outline the impact of a small two-band UV-photometry satellite mission on the field of
stellar physics, magnetospheres of stars, binaries, stellar clusters, interstellar matter, and …

Low-mass stars show evidence of vigorous magnetic activity in the form of large flares and
coronal mass ejections. Such space weather events may have important ramifications for the …

Recent work has demonstrated that high levels of X-ray and UV activity on young M dwarfs
may drive rapid atmospheric escape on temperate, terrestrial planets orbiting within the …

Superflares may provide the dominant source of biologically relevant UV radiation to rocky
habitable-zone M-dwarf planets (M-Earths), altering planetary atmospheres and conditions …

The ultraviolet (UV) emission of stellar flares may have a pivotal role in the habitability of
rocky exoplanets around low-mass stars. Previous studies have used white-light …

The upcoming deployment of the James Webb Space Telescope will dramatically advance
our ability to characterize exoplanet atmospheres, both in terms of precision and sensitivity …

Context. Magnetic fields are a key component in the main sequence evolution of low mass
stars. Flares, energetic eruptions on the surfaces of stars, are an unmistakable manifestation …

We present a multiwavelength study of stellar flares on primarily G-type stars using
overlapping time domain surveys in the near-ultraviolet (NUV) and optical regimes. The …

Extreme-ultraviolet and X-ray emission from stellar coronae drives mass loss from exoplanet
atmospheres, and ultraviolet emission from stellar chromospheres drives photochemistry in …