This is a repository for the reduction pipeline detailed in Wakeford, et al., 2016, ApJ. The method implements marginalization across a series of models to represent stochastic models for observatory and instrument systematics. This is primarily for HST WFC3, however, may be extended to STIS in the future.
I will be closing this pull request and removing this branch.
I will add back in this branch and the tutorials in a different way moving forward including additional instruction and transparency.
Tutorial on how to use the transit function and limb-darkening functions independent of the marginalisation framework.
This tutorial walks through the dependencies of the following functions and how to use them from the ExoTiC-ISM package
limb_dark_fit
phase_calc
impact_param
occultnl