Notes. We employ a flat ΛCDM model with parameters fitted to the KiDS-1000 cosmic shear data (Asgari et al. 2021). The structure growth parameter, S₈ = σ₈(Ω_m/0.3)^0.5, and the amplitude of the intrinsic alignments of galaxies, A_IA, are the only two parameters that KiDS-1000 cosmic shear data constrain. Ω_m is the total matter density parameter, and Ω_b represents the density parameter for baryonic matter. The spectral index of the primordial power spectrum is denoted as n_s, while h represents the dimensionless Hubble parameter. We allow for baryonic feedback through A_bary, which is equal to 3.13 for a dark-matter-only scenario. Additionally, the sum of the neutrino masses is fixed to 0.06 eV.