Fig. 11.

Upper panel: effect of magnification bias on GGL for several high-z fiducial lens samples showing an increase in excess density ΔΣ (or tangential shear) for R ≳ 1 Mpc. Solid curves ignore the magnification, whereas dotted lines account for it. Lower panel: dependence of this effect on the source redshift. In both panels, cuts in stellar mass are expressed in units of 1011 M⊙.
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