Fig. 6.
SN Ia Hubble residuals, 
, calculated from a conventional linear standardization using SALT2.4 lightcurve parameters, as a function of the host-galaxy global stellar mass, log(M*/M⊙). The color code follows that of Fig. 4. The histograms on the right are 𝒫HM-weighted marginalizations of 
, and thus show the contribution of the low and high global stellar mass subsamples.
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