Average tangential shear for source samples in redshift bins (S1, S2, S3) = (0.95 < ɀ < 1.05,1.95 < ɀ < 2.05,2.9 < ɀ < 3), around the lens redshift slices (L1, L2, L3) = (0.45 < ɀ < 0.55,0.95 < ɀ < 1.05,1.45 < ɀ < 1.55. Panels show all possible combinations of cross-correlations between lens sample positions and source galaxy shear. Lens sample redshifts increase from top to bottom panels, whereas source redshift increases from left to right. Solid lines show a fiducial theory prediction for the nonlinear dark-matter power spectrum rescaled with a best-fit linear galaxy bias for the lens samples, b(L1) = 1.2, b(L2) = 1.45, b(L3) = 2.0.