Fig. 7.
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Hubble residuals Δμ for the DES SNe Ia as a function of the stellar mass for the respective host galaxies, plotted in gray. The optimal step locations, as recorded in Table 5 are shown in dashed blue. The blue dots show the mean values of log(M⋆/M⊙) and Δμ in each bin, with the error in the x-axis given by the standard deviation.
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