Figure 8.
Uncertainties ΔCκ(ℓ) (shaded area) in the prediction of the non-linear weak lensing spectra Cκ(ℓ) from drawing samples for Ωm, σ8, h, ns and w from a Gaussian parameter likelihood, for which we use a prior on the wCDM model combining BAO, lensing and the CMB (Euclid 10-bin BAO spectra, Euclid 10-bin weak lensing spectra and Planck CMB temperature and polarization spectra). The uncertainty is compared to the ellipticity spectra $C_E^\epsilon (\ell )$ (green line) and $C_B^\epsilon (\ell )$ (red line) determined with the CNPT model.

Uncertainties ΔCκ(ℓ) (shaded area) in the prediction of the non-linear weak lensing spectra Cκ(ℓ) from drawing samples for Ωm, σ8, h, ns and w from a Gaussian parameter likelihood, for which we use a prior on the wCDM model combining BAO, lensing and the CMB (Euclid 10-bin BAO spectra, Euclid 10-bin weak lensing spectra and Planck CMB temperature and polarization spectra). The uncertainty is compared to the ellipticity spectra |$C_E^\epsilon (\ell )$| (green line) and |$C_B^\epsilon (\ell )$| (red line) determined with the CNPT model.

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