Ratio of the 2PCCF between star-forming galaxies and the total control galaxies as a function of the projected distance (r_p) in different stellar mass bins. Error bars are the standard deviation of the 2PCCF ratio among 100 bootstrap samples. The horizontal dashed line in each panel indicates the theoretical ratio from a halo bias model (Tinker et al. 2010) that uses the halo mass measured from weak lensing as the input. For clarity, we only show the results for the four highest-mass bins, where the uncertainties in lensing mass measurements are relatively small.