Theoretical Transmission Spectra of Exoplanet Atmospheres with Hydrocarbon Haze. II. Dependence on UV Irradiation Intensity, Metallicity, C/O Ratio, Eddy Diffusion Coefficient, and Temperature

First radial velocity results from the MINiature Exoplanet Radial Velocity Array (MINERVA)

The Heavy-element Content Trend of Planets: A Tracer of their Formation Sites

WASP-169, WASP-171, WASP-175 and WASP-182: One bloated sub-Saturn and three hot Jupiters discovered by WASP-south

Leave a Reply