HOD best-fit model parameters obtained by adjusting the model from Sect. 4 on the w_p(r_p) measurements obtained in Sect. 3 and shown in Fig. 2. Differently colored lines represent different samples, identified here by the logarithm of their minimum stellar mass, in solar masses. The color scheme follows that of Fig. 1. We show the corner plot of the parameters and their 1,2,3σ contours in the top panel. The trends of the parameters obtained and their correlation with the stellar mass threshold of the different galaxy samples is sensible: M_min is correlated with the minimum stellar mass, while σ_log(M) is anti-correlated. Model w_p(r_p) obtained and their 1,2,3σ contours (bottom left). Posterior HOD with 1,2,3 σ contours (bottom right). The ordering of the HOD curves follows the stellar mass selection and follows expectations. An individual comparison of the models and the measurements are shown in Fig. C.5.