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Fig. 4.

image

Corner plot showing posterior distributions for the parameters P0, P1, R, and H0 along with the intrinsic scatter obtained using the SBF sample (24 SNe Ia) with the redshift-cut cosmological sample (96 SNe Ia). The title on each histogram shows the median value of the respective posterior distribution. The luminosity correction does not include any dependence on host galaxy stellar mass.

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