Measurements of a series of galaxy-galaxy lensing and clustering statistics (rows) for each different lens redshift slice (columns) of the MICE mocks. The first row displays the projected mass density ΔΣ(R), where measurements corresponding to the different source tomographic samples have been optimally combined following the procedure described in Appendix C. The second row shows the corresponding measurements of Υ_gm(R), derived from ΔΣ(R) using Eq. (40) and assuming R₀ = 2 h⁻¹ Mpc. The third and fourth rows display the galaxy clustering statistics w_p(R) and Υ_gg(R) for each lens redshift slice, where w_p(R) is the projected correlation function measurement, and Υ_gg(R) is the associated quantity suppressing contributions from small scales, derived using Eq. (41) and again assuming R₀ = 2 h⁻¹ Mpc. The fifth row shows the combined-probe statistic E_G(R), derived from the Υ_gm(R) and Υ_gg(R) measurements using Eq. (44). Errors are displayed using the diagonal elements of the analytical covariance matrix, propagating errors where appropriate. The overplotted models are determined using the galaxy bias factors fitted to the Υ_gg measurements for each lens redshift slice, and χ² statistics between the mock mean data and model are displayed in each panel.