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A program for computing on-the-fly non-LTE atomic and molecular spectra and opacities for solving self-consistent radiative transfer problems in exoplanet atmospheres.
First release. Note the code here is a test version used to compute the models presented in the first TIRAMISU release
paper.
A full release is forthcoming.
About
A program for computing on-the-fly non-LTE atomic and molecular spectra and opacities for solving self-consistent radiative transfer problems in exoplanet atmospheres.