This folder includes grids of simulations computed with Exo-REM (https://gitlab.obspm.fr/Exoplanet-Atmospheres-LESIA/exorem).
The model is decribed in Baudino et al., 2015, Charnay et al. 2018 and Blain et al.,2021. The grids for young giant exoplanets correspond to the case with simple microphysics (iron and silicate clouds with supersaturation parameter S=0.003) and non-equilibirum chemmistry from Charnay et al. 2018. Please cite these papers if you use the Exo-REM grids.

The grids explore effective temperature (Teff), gravity (log(g)), metallicity (xsolar) and C/O. Parameter values are given in list_simulation.txt.

The folders cloud_R500.tar.gz and cloud_R20000.tar.gz includes: 
- spectra_YGP files with a spectral resolution of 20 cm-1 (equal to R=500 at 1 micron) or 0.5 cm-1 (equal to R=20000 at 1 micron): 1st column= wavenumber (cm-1), 2nd column = emission flux at top of the atmosphere (W/m2/cm-1)
- vmr_YGP files: 1st column = pressure (Pa), 2nd column = temperature (K), 3rd column = eddy diffusion coefficient (cm2/s), other columns =  gas volume mixing ratio (mol/mol)
- temperature_profile_YGP files: 1st column = pressure (Pa), 2nd column = temperature (K)

The medium resolution spectra (cloud_R20000) were computed from the vmr and temperature_profile files of cloud_R500 grid.

The high resolution spectra (cloud_R200000) do not have accurate line position and should be used with caution (ideally degraded to lower resolution).

cloud_R20000_isotopes includes variation of the C12/C13 ratio expressed in log(C12/C13)