Planetary system LHS 1140 revisited with ESPRESSO and TESS

The cloudy shape of hot Jupiter thermal phase curves

Clouds in Three-Dimensional Models of Hot Jupiters Over a Wide Range of Temperatures I: Thermal Structures and Broadband Phase Curve Predictions

Statistics of the Chemical Composition of Solar Analog Stars and Links to Planet Formation

Impossible moons — Transit timing effects that cannot be due to an exomoon

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