Accurate modeling of exoplanet atmospheres can help inform and constrain observations. Current efforts to model exoplanet atmospheres primarily focus on minimal-complexity one-dimensional models, which miss some key atmospheric mechanisms, and high-complexity computationally expensive three-dimensional models. Therefore there is a natural gap for 2D shallow-water equations models. Many previous such models are built in Fortran, which makes them difficult to adapt to the needs of exoplanet science. Our model, SWAMP-E (Shallow-Water Atmospheric Model in Python for Exoplanets), can accurately and rapidly explore vast parameter space. The code is flexible, modular, built fully in Python, and could be easily adapted to model a variety of dissimi...
Atmospheric retrievals are commonly used to infer exoplanet properties (e.g., the chemical compositi...
The weather and climate of a planetary atmosphere is governed by its pressure-temperature (P-T) stru...
Context. Planetary mass and radius data suggest that low-mass exoplanets show a wide variety of dens...
A quarter-century of exoplanet science has delivered thousands of confirmed exoplanets, revealing a ...
It remains to be ascertained whether sub-Neptune exoplanets primarily possess hydrogen-rich atmosphe...
The grid is divided into two major condensation types, rainout condensation and local condensation. ...
We present the easy-to-use, publicly available, Python package petitRADTRANS, built for the spectral...
We present the easy-to-use, publicly available, Python package petitRADTRANS, built for the spectral...
We survey the basic principles of atmospheric dynamics relevant to explaining existing and future ob...
Many models are used to study the possible atmospheric conditions of extrasolar gas giants, in parti...
Liquid water is generally assumed to be the most important factor for the emergence of life, and so ...
Plain text outputs, associated input files, and comparison figures for hydrosphere properties for Pl...
Context. Despite swift progress in the characterisation of exoplanet atmospheres in composition and ...
This is the software archive for the initial v1.0 release of POSEIDON - as published in the Journal ...
Atmospheres act as windows into their host planets, containing measurable information on their plane...
Atmospheric retrievals are commonly used to infer exoplanet properties (e.g., the chemical compositi...
The weather and climate of a planetary atmosphere is governed by its pressure-temperature (P-T) stru...
Context. Planetary mass and radius data suggest that low-mass exoplanets show a wide variety of dens...
A quarter-century of exoplanet science has delivered thousands of confirmed exoplanets, revealing a ...
It remains to be ascertained whether sub-Neptune exoplanets primarily possess hydrogen-rich atmosphe...
The grid is divided into two major condensation types, rainout condensation and local condensation. ...
We present the easy-to-use, publicly available, Python package petitRADTRANS, built for the spectral...
We present the easy-to-use, publicly available, Python package petitRADTRANS, built for the spectral...
We survey the basic principles of atmospheric dynamics relevant to explaining existing and future ob...
Many models are used to study the possible atmospheric conditions of extrasolar gas giants, in parti...
Liquid water is generally assumed to be the most important factor for the emergence of life, and so ...
Plain text outputs, associated input files, and comparison figures for hydrosphere properties for Pl...
Context. Despite swift progress in the characterisation of exoplanet atmospheres in composition and ...
This is the software archive for the initial v1.0 release of POSEIDON - as published in the Journal ...
Atmospheres act as windows into their host planets, containing measurable information on their plane...
Atmospheric retrievals are commonly used to infer exoplanet properties (e.g., the chemical compositi...
The weather and climate of a planetary atmosphere is governed by its pressure-temperature (P-T) stru...
Context. Planetary mass and radius data suggest that low-mass exoplanets show a wide variety of dens...