$\star$ Residuals according to the factor of stretching

Figure 10.22 in top on the right presents the value of the residuals at the diagram of Hubble according to the factor of stretching. Once again, we note that there does not remain residual correlation after the adjustment of the relation of standardization. In the same way, the remote supernovæ follow the distributions of the close supernovæ indicating that our relations of standardization are also correct for the factor of stretching.

Figure 10.22: Residuals of the diagram of Hubble out of U according to the parameters of the lightcurves: in top on the left, the redshift, in top on the right, the factor of stretching, bellow on the left, it $\Delta m_{15}$, bellow on the right the color.