A generalized precession parameter \ensuremathχ$_{p}$ to interpret gravitational-wave data. Gerosa, D., Mould, M., Gangardt, D., Schmidt, P., Pratten, G., & Thomas, L. M. Physical Review D, 103(6):064067, March, 2021. doi bibtex @article{2021PhRvD.103f4067G,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021PhRvD.103f4067G},
archiveprefix = {arXiv},
author = {{Gerosa}, Davide and {Mould}, Matthew and {Gangardt}, Daria and {Schmidt}, Patricia and {Pratten}, Geraint and {Thomas}, Lucy M.},
doi = {10.1103/PhysRevD.103.064067},
eid = {064067},
eprint = {2011.11948},
journal = {Physical Review D},
keywords = {General Relativity and Quantum Cosmology, Astrophysics - High Energy Astrophysical Phenomena},
month = mar,
number = {6},
pages = {064067},
primaryclass = {gr-qc},
title = {{A generalized precession parameter {\ensuremath{\chi}}$_{p}$ to interpret gravitational-wave data}},
volume = {103},
year = 2021,
bdsk-url-1 = {https://doi.org/10.1103/PhysRevD.103.064067}}
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