Posterior contours of the main constrained cosmological parameters from the KiDS-SBI analysis of the KiDS-1000 cosmic shear data assuming the anisotropic systematics model (in blue) compared against posterior contours from other analyses. In orange, we show the posterior from the same data while assuming the standard isotropic systematics model. In black and pink, we show the posteriors from the equivalent analyses done assuming a Gaussian likelihood for a given model. For clarity purposes, the δ_z parameters are marginalised out, while ω_b and ω_c are folded into Ω_m. The green contour shows the posterior from the cosmic microwave background constraints from the TT,TE,EE+lowE modes (Planck Collaboration VI 2020). We note that the Planck TT,TE,EE+lowE contours do not have any marginals in A_IA or A_bary as the CMB is not sensitive to the IAs of galaxies or baryonic feedback.