Ratio between stellar and halo mass as a function of halo mass from z = 0 to z = 2.25. Solid lines: our results based on abundance matching technique. Triangles: measurements from galaxy-galaxy lensing (Mandelbaum et al. 2006). Squares: measurements from satellite galaxies (Conroy et al. 2007) at z ~ 0 (black) and z ~ 1 (green). Diamonds: measurements from combined kinematics and galaxy-galaxy lensing (Reyes et al. 2011). Typical uncertainties on the results of abundance matching are 0.2 dex.