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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