Atmosphere-Interior Exchange Model for the TRAPPIST-1 Planets

This is an atmosphere-interior exchange model that includes the deep-water cycle and the carbon cycle. This was used to study the TRAPPIST-1 planets and specifically the effect of oxygen fugacity and initial volatile abundance on the abundances of different gas species in their atmospheres. This repository includes the input files, the model scripts, the output files and the jupyter notebook used to create the figures in Perez et al. after reviews for the manuscript submitted to JGR Planets.