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 current environment.yml file is just an environment dump, we need to just have actual packages in it since Conda installs all dependencies automatically.
This is easiest done by collecting all imports that happen in all scripts, which we don't have many of. The only dependency so far that we need and does not get explicitly imported is pango.
The current environment.yml file is just an environment dump, we need to just have actual packages in it since Conda installs all dependencies automatically.