Posterior probability distributions of luminosity distances for each epoch sampled with MCMC runs. The distance estimate from the standard siren with and without very long baseline interferometry radio inclination angle data (Mooley et al. 2018; Hotokezaka et al. 2019) are shown as dashed and solid green lines, respectively. Cosmological redshift distances are also plotted for H₀ = 67.36 ± 0.54 (Planck Collaboration VI 2020) (dotted red) and H₀ = 73.03 ± 1.04 (Riess et al. 2022) (dotted purple).