Distinguishing black-hole spin-orbit resonances by their gravitational wave signatures. II. Full parameter estimation. Trifirò, D., O'Shaughnessy, R., Gerosa, D., Berti, E., Kesden, M., Littenberg, T., & Sperhake, U. Physical Review D, 93(4):044071, February, 2016. doi bibtex @article{2016PhRvD..93d4071T,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {https://ui.adsabs.harvard.edu/abs/2016PhRvD..93d4071T},
archiveprefix = {arXiv},
author = {{Trifir{\`o}}, Daniele and {O'Shaughnessy}, Richard and {Gerosa}, Davide and {Berti}, Emanuele and {Kesden}, Michael and {Littenberg}, Tyson and {Sperhake}, Ulrich},
doi = {10.1103/PhysRevD.93.044071},
eid = {044071},
eprint = {1507.05587},
journal = {Physical Review D},
keywords = {General Relativity and Quantum Cosmology, Astrophysics - High Energy Astrophysical Phenomena},
month = feb,
number = {4},
pages = {044071},
primaryclass = {gr-qc},
title = {{Distinguishing black-hole spin-orbit resonances by their gravitational wave signatures. II. Full parameter estimation}},
volume = {93},
year = 2016,
bdsk-url-1 = {https://doi.org/10.1103/PhysRevD.93.044071}}
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