Top panel: same as in Fig. 10 but now using the volume-limited samples in fully VIPERS-like mocks. Filled points result from using the Scoccimarro model while the empty markers show the growth rate estimates adopting the dispersion model. Both models adopt a second Gaussian damping factor to mimic the effect of spectroscopic redshift errors in the galaxy redshifts (see Sect. 7.3). The shaded regions are the 5% and 1% intervals around the unbiased case. Bottom panel: relative statistical uncertainties expected for a single VIPERS-like realisation. For clarity, only the Scoccimarro model case is shown.