HIGHLIGHTS
SUMMARY
In the last decades, the growing availability of an increasingly larger amount of astrophysical and cosmological data led the authors into a so-called "precision cosmology" era. From the bottom panels of Figs 1, 3, 4, 5 and 6, one can see that the estimates of con- centration parameter c200 show no significant differences between GR and the non -local model, being all consistent with each other at the 1σ level, although the non-local model tends to show higher concentrations than GR. The χ 2 function of the non -local model shows a low . . .
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