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Fig. 11.

image

Distance moduli of the SNe Ia belonging to the two local samples (SBF and SH0ES) estimated using the Cepheid (y-axis) or the SBF (x-axis) as calibrators. The two calibrations used here do not include the cosmological sample in the analysis. It does not include the host galaxy mass correction. For a visual comparison, the line x = y is plotted. Bottom panel: residual difference among the distances calibrated by Cepheid and SBF, Δμ = μCeph − μSBF.

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