Fractional deviation from GR (Δσ∥ = σ∥ ,MG/σ∥ ,GR−1) of the relative radial velocity dispersion, Δσ∥, for the three f(R) models, binned by isolatedness (isolated vs. clustered) and mass (low and high halo mass) as described in Sect. 4.2. Pair separations r = 1 and 5 h-1 Mpc are presented with bold and pale shading, respectively. The isolated high-mass halo bin was excluded for r = 1h-1 Mpc because of the low number of halos within in.
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