Fig. A.1.
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Gaussian fitting of the normalized initial distance distribution of the CF4 supernovae sample (top panel), ungrouped CF4 catalog (middle panel), and grouped CF4 catalog (bottom panel). The priors were fit according to the precision of the distance moduli: less than 0.5 mag errors were modeled as class 0, and ≥0.5mag errors are in class 1.
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