The study of planetary atmospheres is crucial for understanding the origin, evolution, and
processes that shape celestial bodies like planets, moons and comets. The interpretation of …

Context. Retrieving the physical parameters from spectroscopic observations of exoplanets
is key to understanding their atmospheric properties. Exoplanetary atmospheric retrievals …

Aims. Characterizing the interior structure of exoplanets is essential for understanding their
diversity, formation, and evolution. As the interior of exoplanets is inaccessible to …

Exoplanet atmospheric retrieval is a computational technique widely used to infer properties
of planetary atmospheres from remote spectroscopic observations. Retrieval codes typically …

Photoacoustic imaging potentially allows for the real-time visualization of functional human
tissue parameters such as oxygenation but is subject to a challenging underlying …

Detecting H 2 O in exoplanet atmospheres is the first step on the path to determining planet
habitability. Coronagraphic design currently limits the observing strategy used to detect H 2 …

We present the open-source Bayesian Atmospheric Radiative Transfer (BART) retrieval
package, which produces estimates and uncertainties for an atmosphere's thermal profile …

This is an exciting era for exo-planetary exploration. The recently launched JWST, and other
upcoming space missions such as Ariel, Twinkle, and ELTs are set to bring fresh insights to …

Conventional atmospheric retrieval codes are designed to extract information, such as
chemical abundances, thermal structures, and cloud properties, from fully" reduced" spectra …

Atmospheric mass-loss is known to play a leading role in sculpting the demographics of
small, close-in exoplanets. Knowledge of how such planets evolve allows one to 'rewind the …