Observed ratio statistics with jackknife errors for the CFHTLenS lens samples in the low-z bin (panels A and C) and the high-z bin (panels B and D). The source samples are BACK low-z and BACK high-z, respectively. The data points are slightly shifted along the x-axis for better visibility. The dashed lines are predictions for unbiased galaxies (the galaxy-bias normalisation) with SM3 p_d(z). The shaded regions bracket the prediction variations using the p_d(z) of the other lens samples. Top panels: relative clustering of galaxies and matter. Bottom panels: correlation between the (projected) galaxy and matter distribution. This plot uses seven evenly spaced aperture sizes instead of the eight used in the analysis.