- Interpolate efficiently and easily in correlated-k and cross section tables
- Convert easily correlated-k and cross section tables from one format to another (pickle, hdf5, Exomol, LMDZ GCM format, etc.).
- Adapt precomputed correlated-k tables to your need:
- by changing the resolution
- by changing the pressure/temperature grid
- To create tables for a mix of gases using tables for individual gases.
- Test various assumptions in an integrated radiative transfer framework.
The new method used for the spectral binning of k-coefficients is described in Leconte (2021).
The whole documentation, including how to access and download the code, is available here.
Pytmosph3r computes transmission spectra
of exoplanets accounting for the 3D structure of their atmospheres (Caldas et al., 2019).
The input atmospheric structure can be parametrized or come from a 3D global climate model. The code produces the transmission spectrum along with the transmittance maps of the atmospheric limb at all wavelengths.
The whole documentation, including how to access and download the code, is available here.
Have fun!
