Three types of planets orbit red dwarfs

Density, not radius, separates rocky and water-rich small planets orbiting M dwarf stars

The Study of Atmosphere of Hot Jupiters and Their Host Stars

Constraining planetary mass-loss rates by simulating Parker wind profiles with Cloudy

Mass Production of 2021 KMTNet Microlensing Planets III: Analysis of Three Giant Planets

CHEOPS finds KELT-1b darker than expected in visible light: Discrepancy between the CHEOPS and TESS eclipse depths

A direct N-body integrator for modelling the chaotic, tidal dynamics of multi-body extrasolar systems: TIDYMESS

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