Measurements of the average tangential shear, γ_t(θ), for the KiDS-LRG dataset (black points) and representative MICE mocks (red points), between all pairs of lens spectroscopic redshift slices (rows) and source tomographic samples split by photometric redshift (columns). The errors are derived from the diagonal elements of the full analytical covariance matrix (where we note that measurements are correlated across scales and samples). The overplotted model is not a fit to this dataset, but rather a prediction based on the galaxy bias parameter fits to the Υ_gg statistic of each lens redshift slice, which is inaccurate on small scales. The y-values are scaled by a factor of θ (in degrees) for clarity.