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Multi-messenger observations of binary neutron star mergers offer a promising path towards resolution of the Hubble constant ($H_0$) tension, provided their constraints are shown to be free from systematics such as the Malmquist bias.
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K. G. Malmquist, On some relations in stellar statistics, Meddelanden fran Lunds Astronomiska Observatorium Serie I 100
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T. J. Loredo, Accounting for source uncertainties in analyses of astronomical survey data, AIP Conf. Proc. 735
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M. Visser, Jerk and the cosmological equation of state, Class. Quant. Grav. 21
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T. Hastie, R. Tibshirani, and J. Friedman, The elements of statistical learning: data mining, inference,and prediction (2009)
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S. R. Taylor, J. R. Gair, and I. Mandel, Cosmology using advanced gravitational-wave detectors alone, Phys. Rev. D 85
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C. Messenger and J. Read, Measuring a cosmological distance-redshift relationship using only gravitational wave observations of binary neutron star coalescences, Phys. Rev. Lett. 108
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Planck Collaboration, Planck 2018 results. VI. Cosmological parameters, A&A 641
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A. G. Kim, Characterizing the sample selection for supernova cosmology, The Open Journal of Astrophysics 4
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