Excess surface mass density ΔΣ(ξ) for a few luminosity bins for an LSST-like survey. The blue dashed lines correspond to the measurements only for type-1 galaxies. The solid black lines correspond to the combination of both type-1 and type-2 galaxies. The range where we assume the measurement has a bias below 10% is highlighted (derived using our results for type-1 only profiles). The solid thick red line is the signal for the average cluster, shown for visual reference.