Unresolved massive black hole binaries will create a stochastic foreground in LISA that can raise the minimum detectable amplitude of a cosmological gravitational wave background by up to a factor of about 40 near a spectral index of one.
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A Fog Over the Cosmological SGWB: Unresolved Massive Black Hole Binaries in the LISA Band
Unresolved massive black hole binaries will create a stochastic foreground in LISA that can raise the minimum detectable amplitude of a cosmological gravitational wave background by up to a factor of about 40 near a spectral index of one.