Fig. 8
Top: Hubble diagram of the combined sample. The distance modulus redshift relation of the best-fit ΛCDM cosmology for a fixed H0 = 70 km s-1 Mpc-1 is shown as the black line. Bottom: residuals from the best-fit ΛCDM cosmology as a function of redshift. The weighted average of the residuals in logarithmic redshift bins of width Δz/z ~ 0.24 are shown as black dots.
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