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A population synthesis code for testing

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pyipn

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PyIPN is a tool for simulating GRB light curves observed by gamma-ray detectors dispersed throughout the Universe. Additionally, it provides fitting routines for fitting these light curves via random Fourier features to tringulate the location of the simulated GRB.

This work is a build 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 XXXXXX

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$> pip install pyipn

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pyipn-0.1.1.tar.gz (43.2 kB view hashes)

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