Measurement for the KiDS-like set-up. The x-axis denotes the COSEBI order n, each panel shows the measurement for one combination of tomographic bins, whose numbers are given in the upper right corner of each panel. Upper right: COSEBI E-modes E_n measured for the original MICE galaxies (black points), the clustered catalogue (red plusses) and the unclustered catalogue (blue crosses) with the KiDS-1000 uncertainty (grey band). Lower left: Difference between E_n for the original and clustered sources (black points) and between the clustered and unclustered sources (blue crosses), divided by the KiDS-1000 uncertainty. The original sources have shear and position taken directly from the MICE galaxy catalogue, while the clustered sources have their position taken from the catalogue and the shear assigned from the shear maps. The unclustered sources have uniformly distributed positions and shear assigned from the shear maps.