Three types of planets orbit red dwarfs
https://www.science.org/doi/10.1126/science.add7175
Density, not radius, separates rocky and water-rich small planets orbiting M dwarf stars
https://www.science.org/doi/10.1126/science.abl7164
The Study of Atmosphere of Hot Jupiters and Their Host Stars
https://arxiv.org/abs/2209.03669
Constraining planetary mass-loss rates by simulating Parker wind profiles with Cloudy
https://arxiv.org/abs/2209.03677
Mass Production of 2021 KMTNet Microlensing Planets III: Analysis of Three Giant Planets
https://arxiv.org/abs/2209.03886
CHEOPS finds KELT-1b darker than expected in visible light: Discrepancy between the CHEOPS and TESS eclipse depths
https://arxiv.org/abs/2209.03890
A direct N-body integrator for modelling the chaotic, tidal dynamics of multi-body extrasolar systems: TIDYMESS
https://arxiv.org/abs/2209.03955