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Fig. 2.

image

Left: cumulative distribution functions of fixing GN (red line) or imposing empirical lognormal priors (blue line) and flat priors (black line) on GN. The three cases show indistinguishable fit qualities. Right: histograms of the maximum-likelihood GN. The dark and light blue histograms correspond to lognormal and flat priors on GN, respectively. The inset (right panel) shows a zoom-in on the distribution for the Gaussian prior, switched to linear scale for a better view. The actual value of GN is indicated by red dashed lines. The Gaussian prior returns a tight distribution of GN without decreasing the fit quality; this confirms the constancy of GN as expected. The same argument has been applied for the constancy of g in Li et al. (2018).

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