Notes. The first column shows the parameter and the second and third show the prior range adopted by KiDS and DES, respectively. Flat priors are indicated in square brackets, showing the edges of the prior and the Gaussian priors are shown as the mean ± the standard deviation on the parameter. The first 10 are cosmological parameters: A_s is the amplitude (defined at k₀ = 0.05 Mpc⁻¹) and n_s is the spectral index of the primordial power spectrum. Ω_b, Ω_m, and Ω_CDM are the density parameters for baryonic, total and cold dark matter, respectively, while Ω_ν is the neutrino density parameter. Finally h is the dimensionless Hubble parameter. The next three parameters are the amplitude, A_IA and redshift evolution, η_IA, parameters for the intrinsic alignment of galaxies and the baryon feedback parameter A_bar (called B in H20). The final set of parameters capture the systematic effects, where m_i is the multiplicative shear bias, σ_m is the dispersion of m_i and Δz_i is the additive shifts in redshift distributions for each bin. In the H20 setup the effect of m is applied to the data and its error is added to the covariance matrix (see Eq. (A.11)). A_c is the amplitude of the 2D additive bias explained in H20. The model used to evolve the non-linear matter power spectrum is shown in the last row.