Tangential, and cross-components, (g₊ and g_×, respectively) of the raw shear estimates (without background selection and contamination correction) from the full-depth LensMC catalogue as a function of angular distance from the cluster centre. The signal is significant for r < 25′. The cross-shear, g_×, is largely consistent with zero (except the first bin, heavily contaminated by member galaxies), which demonstrates the good control of systematic errors in this raw catalogue.