Fig. 12
Reducing brightness distributions to unidimensional parameters. Marginal PPDs (68%-confidence intervals) of the dayside barycenter brightness peak localization for the ΓSH,1 and Γ2 brightness models. A comparison with the marginal PPDs of the brightness peak localization (Fig. 9b) shows the reduced model-dependence of the dayside barycenter. In particular, it shows a less-extended PPD for the Γ2-model barycenter; because this extension for the brightness-peak-localization PPD emerges from the model wings, weighted by the dayside barycenter. In addition, it shows the shift and slight shrinking of the ΓSH,1 PPD that reflect the barycenter weighting based on to the geometrical configuration at superior conjunction; map cells closer to the substellar point have more weight.
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