PyIPN is a tool for simulating GRB light curves observed by gamma-ray detectors dispersed throughout the Universe (theorectically, but mostly in the Sol system).
The sister fitting code that recovers the time-delays and localizations of the simulated GRBs is Nazgul.
This work is built upon the classical InterPlanetary Network (IPN) developed to do source tringulation via cross-corelation of the observed light curves.
This work is a joint effort by:
- J. Michael Burgess
- Ewan Cameron
- Dmitry Svinkin
If you find this work useful, please cite our paper here
$> pip install pyipn