Table 1
Assumptions made by exoplanet atmosphere studies.
| Paper | Planet | Code | Use case | Approach | Cloud species |
|---|---|---|---|---|---|
| Dyrek et al. (2023) | WASP-107b | ARCiS | Transm. | Brg. | MgSiO3, SiO2, SiO |
| pRT | Transm. | par. | − | ||
| pRT | Transm. | hom. | MgSiO3, SiO2, KCl | ||
| Grant et al. (2023) | WASP-17b | ATMO | Transm. | grey | − |
| VIRGA | Transm. | hom. | SiO2, Al2O3 | ||
| POSEIDON | Transm. | grey | − | ||
| POSEIDON | Transm. | hom. | SiO2 | ||
| pRT | Transm. | hom. | SiO2 | ||
| Alderson et al. (2023) | WASP-39b | VIRGA | Transm. | hom. | MnS, Na2S, MgSiO3 |
| ATMO | Transm. | grey | − | ||
| PHOENIX | Transm. | grey | − | ||
| Rustamkulov et al. (2023) | WASP-39b | PICASO 3.0 | Transm. | grey | − |
| ScCHIMERA | Transm. | grey | − | ||
| ATMO | Transm. | grey | − | ||
| PHOENIX | Transm. | grey | − | ||
| Ahrer et al. (2023) | WASP-39b | VIRGA | Transm. | hom. | MnS, Na2S, MgSiO3 |
| Feinstein et al. (2023) | WASP-39b | ATMO | Transm. | par. | − |
| PHOENIX | Transm. | par. | − | ||
| VIRGA | Transm. | hom. | MnS, Na2S, MgSiO3 | ||
| ScCHIMERA | Transm. | grey | − | ||
| ScCHIMERA | Transm. | hom. | MgSiO3 | ||
| Arfaux & Lavvas (2024) | WASP-39b | “unnamed” | Transm. | hom. | Na2S, MgSiO3 |
| Lustig-Yaeger et al. (2023) | LHS 457 b | CHIMERA | Transm. | grey | − |
| Min et al. (2020) | Multiple | ARCiS | Transm. | Brg. | SiO2, Fe, FeS, Al2O3, C, SiC, TiO2, VO, MgSiO3 |
| Wong et al. (2020) | HAT-P-12b | CARMA | Transm. | cs. | TiO2, Al2O3, Mg2SiO4, MnS, Na2S, KCl, ZnS |
| Powell et al. (2019) | Test case | CARMA | Transm. | hom. | TiO2, Fe, Mg2SiO4, Al2O3 |
| Kempton et al. (2023) | GJ 1214b | HyDRo | Therm. | hom. | KCl |
| Chubb & Min (2022) | WASP-43b | ARCiS | Therm. | par. | − |
| Gao & Powell (2021) | Grid | CARMA | Therm. | cs. | TiO2, Fe, Cr, KCl, Mg2SiO4, MnS, Al2O3, Na2S |
| Webber et al. (2015) | Kepler-7b | ‘unnamed’ | Therm. | hom. | MgSiO3, Mg2SiO4, Fe |
| Demory et al. (2013) | Kepler-7b | ‘unnamed’ | Therm. | hom. | Mg2SiO4 |
| Lee (2023) | HAT-P-1b | Mini-Cloud | GCM | LLL | TiO2, Al2O3, Fe, Mg2SiO4 |
| Christie et al. (2022) | GJ 1214b | UM | GCM | hom. | KCl, ZnS |
| Komacek et al. (2022) | Grid | MITgcm | GCM | cs. | TiO2, Fe, Cr, KCl, Mg2SiO4, Cr, MnS, Al2O3, Na2S |
| Roman et al. (2021) | Grid | RM-GCM | GCM | hom. | KCl, ZnS, Na2S, MnS, SiO2, Mg2SiO4, VO, Ca2SiO4, CaTiO2, Al2O3, Fe, Cr2O3, Ni |
| Tan & Showman (2021) | Test case | MITgcm | GCM | hom. | MgSiO3 |
| Lines et al. (2018b) | HD 209458b | UM | GCM | Brg./LLL | TiO2, SiO, SiO2, MgSiO3, Mg2SiO4 |
| Lee et al. (2016) | HD 189733b | ‘unnamed’ | GCM | Brg./LLL | TiO2, SiO, SiO2, Mg2SiO4, MgSiO3 |
Notes. Studies that consider absorption features within transmission spectra are labelled ‘Transm.’. Studies that consider absorption features within the thermal emission of the planet are labelled ‘Therm.’. Studies that consider radiative feedback of clouds within global circulation models are labelled ‘GCM’. All cloud species are in the solid phase ([s]). Abbreviations used in this table: Bruggeman (Brg.), core-shell (cs.), homogeneous cloud particles (hom.), grey cloud deck (grey), and parameterised cloud description (par.).
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