Fig. 5.

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Residuals in distance modulus as a function of redshift for objects in the Hubble flow in the Baseline solution. Error bars reflect the individual source scatter, without the common calibration uncertainty. The shaded region in each plot indicates the effect of a velocity uncertainty of 250 km s−1. The bars at the right show the mean and dispersion for each group of sources and the calibration uncertainty, which is a common error mode for all points in each panel.
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