Breaking degeneracies in exoplanetary parameters through self-consistent atmosphere–interior modelling
https://www.aanda.org/articles/aa/full_html/2024/12/aa48945-23/aa48945-23.html
Diversities and similarities exhibited by multi-planetary systems and their architectures – I. Orbital spacings
https://www.aanda.org/articles/aa/full_html/2024/12/aa51353-24/aa51353-24.html
The CHEOPS view of the climate of WASP-3 b
https://www.aanda.org/articles/aa/full_html/2024/12/aa51049-24/aa51049-24.html
An alternating minimization algorithm with trajectory for direct exoplanet detection – The AMAT algorithm
https://www.aanda.org/articles/aa/full_html/2024/12/aa51242-24/aa51242-24.html
Disequilibrium Chemistry, Diabatic Thermal Structure, and Clouds in the Atmosphere of COCONUTS-2b
https://iopscience.iop.org/article/10.3847/1538-3881/ad8b2d
Planet Mass Function around M Stars at 1–10 au: A Plethora of Sub-Earth Mass Objects
https://iopscience.iop.org/article/10.3847/1538-4357/ad8c44
Slow Rotation for the Super-puff Planet Kepler-51d
https://iopscience.iop.org/article/10.3847/2041-8213/ad91ae
High-temperature measurements of acetylene VUV absorption cross sections and application to warm exoplanet atmospheres
https://www.aanda.org/component/article?access=doi&doi=10.1051/0004-6361/202451638
Image-Constrained Modeling with Hubble and Keck Images Reveals that OGLE-2012-BLG-0563Lb is a Jupiter-Mass planet Orbiting a K Dwarf
https://arxiv.org/abs/2412.03651
JWST-TST DREAMS: A Precise Water Abundance for Hot Jupiter WASP-17b from the NIRISS SOSS Transmission Spectrum
https://arxiv.org/abs/2412.03675
A Global Perspective with Updated Constraints on the Ultra-hot Jupiter WASP-19b: Atmospheric Properties and Stellar Activity
https://arxiv.org/abs/2412.03739
The GAPS programme at TNG XLVI. A homogeneous search for Na i and its possible variability in ten gas giant exoplanets
https://arxiv.org/abs/2412.04330
DARWEN: Data-driven Algorithm for Reduction of Wide Exoplanetary Networks
https://arxiv.org/abs/2412.04359
From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest Mp/M∗ Systems Exhibit Low Obliquities, Even around Hot Stars
https://arxiv.org/abs/2412.04438