## Introduction
This directory contains files and resources for our study on using a variable fsed and including a cloud base falloff in the eddysed cloud profile. For more details on the purpose and significance of these tests please refer to Section 3.2 and 3.3 in the paper. In this case, all profiles have solar metallicity.

## Directory Structure
- `egp_profiles/`: Contains the atmospheric profiles.
  - Models follow this naming convention: T[teff]K_g[log(g)]_H2O_0.0metal.atm
  - These profiles are the same pressure-temperature profiles used to generate the CARMA clouds.
  - The columns are labeled in the first row of each file.

- `egp_clouds/`: Contains the H2O cloud optical properties.
  - The naming convention for these files is the same as the egp_profile .atm files but with _picaso.cld at the end
  - All cloud profiles are generated using a variable fsed with the recommended parameters in Figure 8 of the paper.
  - These files follow the format used to generate spectra with PICASO.
  - The columns are atmospheric layer index, wavenumber grid index (196 grid), optical depth, asymmetry parameter, single scattering albedo.
  - Follow this step when using PICASO to include these cloud files: https://natashabatalha.github.io/picaso/notebooks/5_AddingTransitSpectrum.html#Adding-Cloud-From-Model-Output
  
- `carma_clouds/`: Contains the post-processed microphysical CARMA cloud.
  - These files follow the same format described above for the egp_clouds

- `README.txt`: This file.
