Projected position-position, w_gg (left), and position-shape, w_g+ (right), correlation functions for all galaxies with more than 300 stellar particles in the 2.8 Gpc box, as a function of the projected separation, r_p. The sample contains 4 941 492 galaxies with stellar masses ranging from 10^11.28 to 10^13.68 M_⊙ and halo masses (M_200mean) ranging from 10^12.2 to 10^15.78 M_⊙. Overplotted is the best-fitting joint clustering and NLA or TATT model with the residuals in the lower panel. The gray regions show the scales excluded from the fitting. Considering scales between 5 and 100 Mpc/h, TATT achieves residuals within 4 per cent.