Lensing signal multiplied with the projected separation in arcmin as a function of angular distance from the lens, for the “all” lens sample (left-hand panels), the “red” lens sample (middle panels) and the “blue” lens sample (right-hand panels). In the top panels, the green squares (blue triangles) show the average rΔΣ along the major (minor) axis (quadrants B (A) in Fig. 3). The dashed lines indicate the best fit NFW profile times the projected separation, fitted to the azimuthally averaged lensing signal on scales between 50 and 500 kpc using the mean lens redshift. In the middle panel, the green squares (blue triangles) show the cross shear signal averaged in quadrant D (C) of Fig. 3. In the bottom panels, 1 / f_mm and are shown by the red squares and black triangles, respectively. The dotted lines indicate the virial radius from the best-fit NFW profiles. The shear ratio does not provide clear signs for the alignment between galaxies and their dark matter haloes.