We show the results from table 4 with the Low-z cluster sample and the different absolute-magnitude cuts for galaxy selections after marginalizing over the off-centering effects. The left-hand panel shows the projected cross-correlation measurements and the 16th and 84th percentiles of the model predictions from the MCMC chains for each selection. The right-hand panel presents constraints on the three-dimensional galaxy density profile ρ_g(r) = 〈Σ_g〉ξ_3D(r)/(2R_max) (see subsection 3.1 for more details) from the MCMC chains for each selection. (Color online)