Fig. 10
Credible parameter contours from ξ± (calibrated) with CosmoPMC for the three combinations of 
. The width ΔΣ8 of the σ8–Ωm contour is comparable to, but in fact larger than the value from peaks, despite the distributions seen in Fig. 8. As with peaks, 
cannot be constrained without a tomographic analysis. The star indicates the MICE cosmology.
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