Fig. D.1
Comparison of two derivations of the 68 and 95% confidence contours in the Ωm and w parameters for a flat w-CDM cosmology. In one case, constraints are derived from the exploration of the full Planck+WP+JLA likelihood (blue). In the other case CMB constraints are summarized by the geometric distance prior described in Sect. 7.1 (dashed red).
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