Supernova classification Pipeline Leveraging Attributes of Supernova Hosts (SPLASH)

SPLASH classifies supernovae by using photometry to infer their host properties, and then using those properties (along with host-supernova angular separation) to predict supernova classes.

Here we are classifying supernova detections from ZTF in real time!

Here is the SPLASH methods paper!

Installation

The pacakge can be installed from the python package index with

pip install astro_SPLASH