Each panel shows our estimate of ξ(s) measured for a particular wide area survey as labelled. We annotate each panel with the median magnitude in g for comparison to our survey. Errors are Poisson. We fit the data using the model from Section 6.1.2, where we assume Gaussian velocity dispersions in real space, γ = 1.8 with a velocity dispersion, |$\langle \omega ^{2}\rangle ^{\frac{1}{2}} = 750 \: \mathrm{km} \: s^{-1}$|⁠. In each panel we show the model where r₀ = 6.1 h⁻¹ Mpc (solid line) (see Section 6.1.2). For each survey we restrict the analysis to the redshift interval 0.3 < z < 2.9 as this range is well sampled by all surveys. The best-fitting models for the individual surveys are shown in Table 3.