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Fig. 10.

image

Contour plots at the 68 and 95 percent confidence levels for the Gaussian likelihood evaluated with: a cosmology-dependent covariance matrix (black), a covariance matrix fixed at the input cosmology (blue) and covariance matrices computed at two wrong cosmologies, one with lower parameter values (Ωm = 0.295, log10As = −8.685 and σ8 = 0.776, red) and one with higher parameter values (Ωm = 0.320, log10As = −8.625 and σ8 = 0.884, orange). The gray dotted lines represent the input values of parameters.

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