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A Direct Comparison between the Use of Double Gray and Multiwavelength Radiative Transfer in a General Circulation Model with and without Radiatively Active Clouds
Isaac Malsky, Emily Rauscher, Michael T. Roman, Elspeth K. H. Lee, Hayley Beltz, Arjun Savel, Eliza M.-R. Kempton and L. Cinque The Astrophysical Journal 961(1) 66 (2024) https://doi.org/10.3847/1538-4357/ad0b70
Implementation of Aerosol Mie Scattering in POSEIDON with Application to the Hot Jupiter HD 189733 b’s Transmission, Emission, and Reflected Light Spectrum
Modelling reflected polarized light from close-in giant exoplanet WASP-96b using PolHEx (Polarization of hot exoplanets)
Katy L Chubb, Daphne M Stam, Christiane Helling, Dominic Samra and Ludmila Carone Monthly Notices of the Royal Astronomical Society 527(3) 4955 (2023) https://doi.org/10.1093/mnras/stad3413
A New Sedimentation Model for Greater Cloud Diversity in Giant Exoplanets and Brown Dwarfs
How does thermal scattering shape the infrared spectra of cloudy exoplanets? A theoretical framework and consequences for atmospheric retrievals in the JWST era
Jake Taylor, Vivien Parmentier, Michael R Line, et al. Monthly Notices of the Royal Astronomical Society 506(1) 1309 (2021) https://doi.org/10.1093/mnras/stab1854
How Does the Shape of the Stellar Spectrum Affect the Raman Scattering Features in the Albedo of Exoplanets?