Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond. Baibhav, V., Berti, E., Gerosa, D., Mapelli, M., Giacobbo, N., Bouffanais, Y., & Di Carlo, U. N. Physical Review D, 100(6):064060, September, 2019.
doi  bibtex   
@article{2019PhRvD.100f4060B,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2019PhRvD.100f4060B},
	archiveprefix = {arXiv},
	author = {{Baibhav}, Vishal and {Berti}, Emanuele and {Gerosa}, Davide and {Mapelli}, Michela and {Giacobbo}, Nicola and {Bouffanais}, Yann and {Di Carlo}, Ugo N.},
	doi = {10.1103/PhysRevD.100.064060},
	eid = {064060},
	eprint = {1906.04197},
	journal = {Physical Review D},
	keywords = {General Relativity and Quantum Cosmology, Astrophysics - High Energy Astrophysical Phenomena},
	month = sep,
	number = {6},
	pages = {064060},
	primaryclass = {gr-qc},
	title = {{Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond}},
	volume = {100},
	year = 2019,
	Bdsk-Url-1 = {https://doi.org/10.1103/PhysRevD.100.064060}}

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