Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures. Gerosa, D., O'Shaughnessy, R., Kesden, M., Berti, E., & Sperhake, U. Physical Review D, 89(12):124025, June, 2014.
doi  bibtex   
@article{2014PhRvD..89l4025G,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2014PhRvD..89l4025G},
	archiveprefix = {arXiv},
	author = {{Gerosa}, Davide and {O'Shaughnessy}, Richard and {Kesden}, Michael and {Berti}, Emanuele and {Sperhake}, Ulrich},
	doi = {10.1103/PhysRevD.89.124025},
	eid = {124025},
	eprint = {1403.7147},
	journal = {Physical Review D},
	keywords = {04.25.dg, 04.70.Bw, 04.30.-w, Numerical studies of black holes and black-hole binaries, Classical black holes, Gravitational waves: theory, General Relativity and Quantum Cosmology, Astrophysics - High Energy Astrophysical Phenomena},
	month = jun,
	number = {12},
	pages = {124025},
	primaryclass = {gr-qc},
	title = {{Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures}},
	volume = {89},
	year = 2014,
	Bdsk-Url-1 = {https://doi.org/10.1103/PhysRevD.89.124025}}

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