Fig. 18

One- and two-dimensional posterior likelihood distribution of the derived parameters fσ8, bσ8 and σ12 for the 0.5 <z< 0.7 redshift bin. This corresponds to the result of the analysis of VIPERS data using the dispersion model, the Scoccimarro model, the Taruya model, and smin = 5h-1 Mpc. The dark- and light-shaded areas correspond to the 68% and 95% joint two-parameter confidence levels, respectively. The lower redshift sample shows comparable contours and shapes.
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