Fractional change of the shear profile by magnification, where the magnification is only turned on for the source galaxies at z_s = 0.99 (Table 1a). At a local slope of α_s ≈ 1 the impact of magnification flips its sign. The relation between α_s and δ_γ is almost linear. Different redshifts of the lenses z_d = 0.41 (plus) and 0.62 (cross) affect the impact of the sources’ magnification; the r-band limiting magnitude of lenses is fixed to 22 mag.