Fig. B.2.
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Measured data and model 
vector for all combinations of aperture filter radii θap ∈ {4′,8′,16′,32′}. The data vector results from one full-sky convergence realisation without shape noise. The grey band shows the expected uncertainty of KiDS-1000 estimated with the convergence maps. The 
is scaled by the third root of the product of the corresponding filter radii.
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