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Table 6.

Mean values, marginalised 68% errors, and bias.

CH18
ST15
HD15
θ max θ σ B θ σ B θ σ B
ωb, 0 1500 0.2246 0.00011 0.09 0.2245 0.00012 0.00 0.02249 0.00012 0.34
5000 0.02251 0.00012 0.51 0.02252 0.00012 0.64 0.02252 0.00012 0.56

ωc, 0 1500 0.12061 0.00035 0.15 0.12059 0.00036 0.08 0.12044 0.00040 0.30
5000 0.12109 0.00036 1.49 0.12110 0.00037 1.46 0.12083 0.00036 0.76

h 1500 0.6833 0.0069 1.92 0.6799 0.0065 1.52 0.6819 0.0069 1.73
5000 0.6990 0.0041 7.15 0.7069 0.0041 9.11 0.6835 0.0045 2.99

ln(1010As) 1500 3.0571 0.0087 0.14 3.0590 0.0083 0.07 3.0578 0.0084 0.07
5000 3.0644 0.0083 0.73 3.0679 0.0087 1.10 3.0592 0.0083 0.10

ns 1500 0.9583 0.0024 0.68 0.9589 0.0025 0.42 0.9572 0.0025 1.11
5000 0.9489 0.0020 5.49 0.9488 0.0021 5.44 0.9503 0.0021 4.69

w0 1500 −1.040 0.078 1.79 −0.990 0.078 1.16 −1.063 0.092 1.77
5000 −1.220 0.039 8.22 −1.240 0.040 8.43 −1.142 0.053 4.55

wa 1500 0.43 0.19 1.68 0.30 0.20 0.98 0.51 0.23 1.78
5000 0.84 0.09 8.27 0.84 0.10 7.70 0.73 0.13 5.04

Δχ2 1500 6.35 3.94 11.54
5000 63.61 107.32 45.05

Notes. The values are obtained by fitting mock Planck and Euclid cosmic shear data with Halofit without baryonic corrections, to non-linear corrections with either CH18, ST15 or HD15 methods non-linear corrections. The number of degrees of freedom in this case is 11 (the number of free parameters), which enables one to compare Δχ2 to the corresponding confidence interval.

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