Fig. A.2.
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Triaxiality of DM halos at z = 0 as function of the variable νNL(M, 0) = δc(z = 0)/σNL(M, 0) which takes into account the explicit dependence on the critical spherical overdensities δc, of each model. We note the universality for the cosmological models with the same δc(z = 0) parameter, but We observe no full cosmological invariance.
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