JWST-Jupiter MIRI Exogenous molecules (HCN, CO2 and H2O)

In these files you will find the dataset used for the refered article. You will find three main directories noted 'obsX', where X is the JWST observation 1, 2 or 3, each of them for a specific longitude (335W, 70W and 135W). Within these files you will find the directories to HCN, CO2 and H2O. We remind that for CO2 you will find the retrieved profiles in the .inv files for each spaxel of the MRS FOV. For HCN and H2O you will find the mean latitude spectra. The comparison between the observed and synthetic spectrum is found in the .res files. For more information regarding this dataset, please contact pablo.ovalle@obspm.fr or thierry.fouchet@obspm.fr