Relative source-lens clustering bias of the weak lensing shear two-point correlation, (ξδγδγ∗ + ζδγγ∗) / | ξγγ∗ | (we neglect the four-point contribution), as a function of the second galaxy redshift z2, for a fixed first galaxy redshift z1 = 0.5,1, or 2. We consider the angular scales θ = 1, 10, and 100 arcmin, from the upper to the lower panels.
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