Deep generative modeling of astronomical transient light curves
ParSNIP learns a generative model of transients from a large dataset of transient light curves. This code has many applications including classification of transients, cosmological distance estimation, and identifying novel transients. A full description of the algorithms in this code can be found in Boone 2021 (submitted to ApJ).
Instructions on how to install and use ParSNIP can be found on the ParSNIP readthedocs page.