Unified population inference
Project description
GWPopulation
A collection of parametric binary black hole mass/spin population models.
These are formatted to be consistent with the Bilby hyper-parameter inference package.
For an example using this code to analyse the first gravitational-wave transient catalog (GWTC-1) see here.
Automatically generated docs can be found here.
Attribution
Please cite Talbot et al (2019) if you find this package useful.
@ARTICLE{2019PhRvD.100d3030T,
author = {{Talbot}, Colm and {Smith}, Rory and {Thrane}, Eric and
{Poole}, Gregory B.},
title = "{Parallelized inference for gravitational-wave astronomy}",
journal = {\prd},
year = 2019,
month = aug,
volume = {100},
number = {4},
eid = {043030},
pages = {043030},
doi = {10.1103/PhysRevD.100.043030},
archivePrefix = {arXiv},
eprint = {1904.02863},
primaryClass = {astro-ph.IM},
}
Additionally, please consider citing the original references for the implemented models which should be include in docstrings.
Most of the models implemented are derived from models presented in one of:
As of v0.5.0 GWPopulation
supports only python >= 3.6
.
See the python 3 statement for more information.
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