Fig. 1.
Number of galaxies (top panel) and the normalized density distribution (bottom panel) as a function of the host galaxy stellar mass for the SBF and the SH0ES calibration samples. We also plot the host stellar mass distribution for the cosmological sample. The KS-test P value for the two calibration samples gives 6.03 × 10−6, indicating that the stellar mass distributions of the host galaxies of SNe Ia are different for the two samples.
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