The prospects for the habitability of M-dwarf planets have long been debated, due to key
differences between the unique stellar and planetary environments around these low-mass …

Abstract The Very Large Array Sky Survey (VLASS) is a synoptic, all-sky radio sky survey
with a unique combination of high angular resolution (≈ 2 farcs 5), sensitivity (a 1σ goal of …

We perform a study of stellar flares for the 24,809 stars observed with 2 minute cadence
during the first two months of the TESS mission. Flares may erode exoplanets' atmospheres …

Coherent low-frequency (≲ 200 MHz) radio emission from stars encodes the conditions of
the outer corona, mass-ejection events and space weather,,,–. Previous low-frequency …

Understanding the impact of active M dwarf stars on the atmospheric equilibrium and
surface conditions of a habitable zone Earth-like planet is key to assessing M dwarf planet …

Recently, many Earth-sized planets have been discovered around stars other than the Sun
that might possess appropriate conditions for life. The development of theoretical methods …

The habitability of the surface of any planet is determined by a complex evolution of its
interior, surface, and atmosphere. The electromagnetic and particle radiation of stars drive …

We present the discovery and validation of a three-planet system orbiting the nearby (31.1
pc) M2 dwarf star TOI-700 (TIC 150428135). TOI-700 lies in the TESS continuous viewing …

Evidence of star–planet interactions in the form of planet-modulated chromospheric
emission has been noted for a number of hot Jupiters. Magnetic star–planet interactions …

One of the primary goals of exoplanetary science is to detect small, temperate planets
passing (transiting) in front of bright and quiet host stars. This enables the characterization of …