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The effects of local inhomogeneities on low redshift $H_0$ determinations are studied by estimating the redshift-distance relation of mock sources in N-body simulations.
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Wendy L. Freedman et al.: Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble Constant, 2012, ApJ, 758, 24
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George Efstathiou: H 0 H_{0} Revisited, MNRAS 440, 1138–1152 (2014), arXiv:1311.3461v2 [astro-ph.CO]
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