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Fig. 5

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Increase in the cumulative halo mass function from simulations for the two f(R) scenarios, f¯,R0=105${\bar f_{,R0}} = {10^{ - 5}}$ (F5, top row) and f¯,R0=106${\bar f_{,R0}} = {10^{ - 6}}$ (F6, bottom row), relative to the reference ACDM cosmology. The enhancement factor Bn = n/nACDM is measured for different codes (different line styles) at two different redshifts, z = 1 (left panels) and z = 0.667 (right panels). The bottom panel of each plot shows the relative agreement of the individual measurements, using MG–Arepo as a common reference.

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