Calibrating signal-to-noise ratio detection thresholds using gravitational-wave catalogs. Mould, M., Moore, C. J., & Gerosa, D. Physical Review D, 109(6):063013, March, 2024.
doi  bibtex   
@article{2024PhRvD.109f3013M,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2024PhRvD.109f3013M},
	archiveprefix = {arXiv},
	author = {{Mould}, Matthew and {Moore}, Christopher J. and {Gerosa}, Davide},
	doi = {10.1103/PhysRevD.109.063013},
	eid = {063013},
	eprint = {2311.12117},
	journal = {Physical Review D},
	keywords = {General Relativity and Quantum Cosmology, Astrophysics - High Energy Astrophysical Phenomena},
	month = mar,
	number = {6},
	pages = {063013},
	primaryclass = {gr-qc},
	title = {{Calibrating signal-to-noise ratio detection thresholds using gravitational-wave catalogs}},
	volume = {109},
	year = 2024,
	bdsk-url-1 = {https://doi.org/10.1103/PhysRevD.109.063013}}

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