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

@article{Moore2019AreSB,
  title={Are stellar-mass black-hole binaries too quiet for LISA?},
  author={Christopher J. Moore and Davide Gerosa and Antoine Klein},
  journal={Monthly Notices of the Royal Astronomical Society: Letters},
  year={2019}
}
The progenitors of the high-mass black-hole mergers observed by LIGO and Virgo are potential LISA sources and promising candidates for multiband GW observations. In this letter, we consider the minimum signal-to-noise ratio these sources must have to be detected by LISA bearing in mind the long duration and complexity of the signals. Our revised threshold of ρthr ∼ 15 is higher than previous estimates, which significantly reduces the expected number of events. We also point out the importance… 

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