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Gravitational waves (GWs) from the inspiral of binary compact objects offer a one-step measurement of the luminosity distance to the event, which is essential for the measurement of the Hubble constant, $H_0$, which characterizes the expansion rate of the Universe.
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Jeremy L. Tinker, Brant E. Robertson, Andrey V. Kravtsov, Anatoly Klypin, Michael S. Warren, Gustavo Yepes, and Stefan Gottlöber, “The large-scale bias of dark matter halos: Numerical calibration and model tests,” The Astrophysical Journal 724
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Surhud More, “How accurate is our knowledge of galaxy bias?” Astrophys. J. 741
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J. Aasi et al. (LIGO Scientific), “Advanced LIGO,” Class. Quant. Grav. 32
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