Fig. 6
Parameter constraints in the σ8–Ωm plane from peaks as modelled by Camelus. The 1σ and 2σ contours represent the 68.3% and 95.4% most probable regions, respectively, after marginalizing over 
. The full Ωm prior range is shown, and the star marks the MICE input cosmology. The constraint is biased significantly toward high σ8 and low Ωm along the degeneracy direction.
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