Model predictions vs. observations for the best luminosity evolution model, ΛCDM B2 and NALPL B2 (together with the standard ΛCDM prediction, for illustrative purposes) for all the cosmological probes considered. In each prediction, we used the best-fit values obtained from the global fit. Top left: residuals of SNIa data with respect to the corresponding model. Top right: residuals of BAO data with respect to the corresponding model. The isotropic measurements of the BAO are represented with a circle and their observable is D_V(z) /r_d, while the stars stand for the radial measurements with observable r(z) /r_d and the squares stand for the transverse measurements with observable c/ (H(z)r_d). Bottom left: measurements of H(z)/(1 + z) together with the model predictions. Bottom right: measurements of fσ₈(z) and the different model predictions.