Gaseous Planets

Knobs and dials of retrieving JWST transmission spectra. II. Impacts of pipeline-level differences on retrieval posteriors
The study investigates the impacts of pipeline-level differences on retrieval posteriors using three different Eureka! data reductions of the WASP-39b PRISM observations.
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Knobs and dials of retrieving JWST transmission spectra. II. Impacts of pipeline-level differences on retrieval posteriors
Radiative Flux from a High-resolution Atmospheric Dynamics Simulation of a Hot Jupiter for JWST and Ariel
The study presents estimates of spectroscopic variability of hot Jupiters, using radiative transfer post-processing of high-resolution atmospheric dynamics calculations.
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Radiative Flux from a High-resolution Atmospheric Dynamics Simulation of a Hot Jupiter for JWST and Ariel
Cloud and haze parameterization in atmospheric retrievals: Insights from Titan's Cassini data and JWST observations of hot Jupiters
The study investigates the properties of four hot Jupiters observed with JWST (NIRISS, NIRSpec, NIRCam, and MIRI) to infer their atmospheric composition. A strong emphasize is done on the parameterization of clouds and hazes, which are shown to be important for properly interpreting these complex atmospheres.
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Cloud and haze parameterization in atmospheric retrievals: Insights from Titan's Cassini data and JWST observations of hot Jupiters
Is the atmosphere of the ultra-hot Jupiter WASP-121b variable?
The study investigates the phase-curve of WASP-121b by HST. We find temporal variability in the data, i.e., storms and weather patterns.
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Is the atmosphere of the ultra-hot Jupiter WASP-121b variable?