Photometric classification of supernovae
Project description
Superphot
Superphot is an open-source Python package for photometric classification of supernovae, based on the method of Villar et al. (2019). To apply this method, you must have the full griz light curve and redshift (e.g., from the host galaxy) for each transient. As such, Superphot is designed for use by time-domain surveys to retrospectively classify transients that were not observed spectroscopically, not for real-time classification.
In Villar et al. (2019) and Dauphin et al. (2020), we trained the classifier on a sample of ~500 spectroscopically classified supernovae from the Pan-STARRS1 Medium Deep Survey, and then applied it to an additional ~3000 transients with host galaxy redshifts. This trained classifier is included in the package, but users will most likely want to train on their own survey data for better performance.
Project details
Download files
Download the file for your platform. If you're not sure which to choose, learn more about installing packages.
Source Distribution
Built Distribution
Hashes for superphot-0.1.0-py3-none-any.whl
Algorithm | Hash digest | |
---|---|---|
SHA256 | ac96a51ead6658545d69ca81d3bb138f4297aba74d8fdaa9bddaf6cc7f572348 |
|
MD5 | 7c793b0a0a92ecf774b920c56f5f411b |
|
BLAKE2b-256 | f90c5c51c01d0ff75c8cd3bb8e979b0e2d32e487d763785bad577febe989a568 |