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Fig. 6.

image

Prediction of the different models, ΛCDM, spline reconstruction, and coasting reconstruction with SNIa intrinsic luminosity evolution, for the growth of matter perturbations fσ8 observable. The predictions have been computed using the best-fit values for the parameters obtained from the fit of the combination SNIa+BAO+CMB computing rd explicitly. Therefore, it is not a fit to the fσ8 measurements. We follow the same color legend as in the previous figures: black for ΛCDM, red for the spline reconstruction, and green for the coasting reconstruction.

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