The Hubble parameter produces a frequency-independent angular enhancement in LISA timing residuals above 100 mHz, potentially enabling a percent-level H0 measurement without standard sirens.
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Impact of $H_0$ on gravitational wave propagation: prospects for the LISA mission
The Hubble parameter produces a frequency-independent angular enhancement in LISA timing residuals above 100 mHz, potentially enabling a percent-level H0 measurement without standard sirens.