Data Products and Models for "JWST Transmission Spectroscopy of TOI-3235 b: Constraints on Giant Planet Formation around M Dwarfs amid Stellar Contamination"

This archive contains the data products and model outputs needed to reproduce the main results and figures in "JWST Transmission Spectroscopy of TOI-3235 b: Constraints on Giant Planet Formation around M Dwarfs amid Stellar Contamination". The figure-generation notebooks are available separately on GitHub at:https://github.com/zoekko/TOI3235b-JWST-transmission The archive contains three main folders. `TOI3235b_transmission` contains the TOI-3235 b transmission spectrum (`toi3235b_trans_spec.txt`) and the dynesty retrieval outputs for the transmission spectrum analyses, including the atmosphere-only model (`atm`), atmosphere + stellar contamination model (`atm_SC`), atmosphere + stellar contamination + Gaussian Process model (`atm_SC_GP`), and corresponding retrievals performed on the truncated spectrum (`atm_SC_on_truncated_spectrum` and `atm_SC_GP_on_truncated_spectrum`). `TOI3235b_synthetic_emission` contains synthetic emission spectra corresponding to different atmospheric metallicities and cloud-top pressures, the wavelength grid used for these spectra, and the retrieval results for each synthetic emission spectrum. `TOI3235b_VULCAN_outputs` contains VULCAN chemical-equilibrium model outputs for five different atmospheric metallicities. To reproduce the figures, download this Zenodo archive and clone the GitHub repository. The notebooks require numpy, matplotlib, pandas, corner, and exocomp. The original JWST observations are available from MAST at:https://doi.org/10.17909/02a7-ck05 This Zenodo record is associated with AAS manuscript #AAS73388.