A population synthesis code for testing
Project description
pyipn
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
Install
$> pip install pyipn
Release history Release notifications | RSS feed
Download files
Download the file for your platform. If you're not sure which to choose, learn more about installing packages.
Source Distribution
pyipn-0.1.1.tar.gz
(43.2 kB
view details)
File details
Details for the file pyipn-0.1.1.tar.gz.
File metadata
- Download URL: pyipn-0.1.1.tar.gz
- Upload date:
- Size: 43.2 kB
- Tags: Source
- Uploaded using Trusted Publishing? No
- Uploaded via: twine/3.2.0 pkginfo/1.5.0.1 requests/2.24.0 setuptools/49.1.0 requests-toolbelt/0.9.1 tqdm/4.47.0 CPython/3.8.5
File hashes
| Algorithm | Hash digest | |
|---|---|---|
| SHA256 | 7165affdd2ee509937f6ffc2654e462ebbfc9140c1031da8ebfb4878e9eb13e6 |
|
| MD5 | 9470f9f059794c4ab375182f74cfa1c6 |
|
| BLAKE2b-256 | 1a6c91c790978e6f317f76d97034627ada07ee76a1e217f6ed5904162ca7ab41 |
