Top: Projected position–shape correlation function measurements as a function of galaxy pair separation for the red (red circles) and high n_s (orange triangles) galaxy sub-samples. The different luminosity sub-samples are indicated in the top left of each panel, with luminosity increasing from left to right. The best-fit NLA model is shown as solid lines of corresponding colour – with dotted lines where the model is no longer valid, at r_p<6 Mpc/h, which is also indicated with a vertical dotted black line. The grey area indicates the region where the covariance estimation is no longer accurate. Points are slightly offset for visual clarity. Bottom: Projected correlation measurements between galaxy positions and the cross ellipticity component.