Fig. C.2.
Predicted 1- and 2-σ contours on the wCDM cosmological parameters, for Euclid, for different values of ns. All other parameter values are fixed to those shown in Table 1. Confidence regions and biases for ns = 0.86 (bottom left), and ns = 1.06 (top right) are shown. The additional IA-enhanced lensing bias is not included in these results. In general, varying the fiducial value of ns does not cause notable change to the significances of the biases.
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