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.
The filenames of our result outputs and plots currently make no sense, we should change that.
Also, the final results from the marginalization should follow issue #12 and use pandas to be saved in a nicer human-readable table format.