3D simulations of the exoplanet TRAPPIST-1e using WACCM6

The data is associated with the article titled ‘Degenerate interpretations of O3 spectral features in exoplanet atmosphere observations due to stellar UV uncertainties: a 3D case study with TRAPPIST-1e’. There are ten simulations of the atmosphere of the exoplanet TRAPPIST-1e. These are split into two sets of five. Each set has a different stellar input spectrum. One is with the P19 spectrum, and the other is the W21 spectrum. Then each set has oxygen concentrations of 100%, 10%, 1%, and 0.1% the present atmospheric level of oxygen (which has a mixing ratio of 21% by volume). Finally, there is a case which is not tidally locked. This dataset provides the data from the WACCM6 simulations which is needed to produce all of the figures and results in the article.