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}}

Downloads: 0