Are stellar-mass black-hole binaries too quiet for LISA?

Are stellar-mass black-hole binaries too quiet for LISA?. Moore, C. J., Gerosa, D., & Klein, A. Monthly Notices of the Royal Astronomical Society, 488(1):L94-L98, September, 2019.
doi bibtex

@article{2019MNRAS.488L..94M,
	adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	adsurl = {https://ui.adsabs.harvard.edu/abs/2019MNRAS.488L..94M},
	archiveprefix = {arXiv},
	author = {{Moore}, Christopher J. and {Gerosa}, Davide and {Klein}, Antoine},
	doi = {10.1093/mnrasl/slz104},
	eprint = {1905.11998},
	journal = {Monthly Notices of the Royal Astronomical Society},
	keywords = {gravitational waves, stars: black holes, methods: data analysis, Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology},
	month = sep,
	number = {1},
	pages = {L94-L98},
	primaryclass = {astro-ph.HE},
	title = {{Are stellar-mass black-hole binaries too quiet for LISA?}},
	volume = {488},
	year = 2019,
	bdsk-url-1 = {https://doi.org/10.1093/mnrasl/slz104}}

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