The widest broadband transmission spectrum (0.38–1.71 μm) of HD 189733b from ground-based chromatic Rossiter–McLaughlin observations
https://www.aanda.org/articles/aa/abs/2020/11/aa39213-20/aa39213-20.html
The eccentricity distribution of giant planets and their relation to super-Earths in the pebble accretion scenario
https://www.aanda.org/articles/aa/full_html/2020/11/aa38856-20/aa38856-20.html
Reflected Light Observations of the Galilean Satellites from Cassini: A Test Bed for Cold Terrestrial Exoplanets
https://iopscience.iop.org/article/10.3847/1538-3881/abb8df
Dynamical Mass Estimates of the β Pictoris Planetary System through Gaussian Process Stellar Activity Modeling
https://iopscience.iop.org/article/10.3847/1538-3881/abba30
Identifying Exoplanets with Deep Learning. IV. Removing Stellar Activity Signals from Radial Velocity Measurements Using Neural Networks
https://arxiv.org/abs/2011.00003
Separating planetary reflex Doppler shifts from stellar variability in the wavelength domain
https://arxiv.org/abs/2011.00018
The Three Dimensional Flow Field Around Planets on Eccentric Orbits
https://arxiv.org/abs/2011.00022
A new perspective on interiors of ice-rich planets: Ice-rock mixture rather than a layered structure
https://arxiv.org/abs/2011.00602
Evaluating the Effect of Four Unknown Parameters Included in a Latitudinal Energy Balance Model on the Habitability of Exoplanets
https://arxiv.org/abs/1809.06907