Fig. 5.
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Mean scaling relations between halo number density and selected non-local halo properties across different f(R) cosmologies at redshift z = 0.5. The properties plotted are Vmax, ℰh, ℳ5, Δ5, 𝒟5, and 𝒯A. The lower panels show the ratio of each property in f(R) with respect to ΛCDM. The error bars represent the uncertainty in the mean for each mass bin.
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