Two-point correlation functions of primary galaxies hosted by dark matter halos with masses of 10^11.6 ≤ M_h/h⁻¹ M_⊙ < 10^11.8. The autocorrelation function for the case with all the central galaxies in the primary sample (PrimAll) is shown as a solid black line, whereas the dark red solid line and navy blue circles correspond to the cross-correlation functions of quenched and star-forming primary galaxies, respectively. On the other hand, the dashed gray line corresponds to the autocorrelation function after removing the central galaxies in the vicinity of halos more massive than 10¹³ h⁻¹ M_⊙ from the primary sample (PrimB case). The red dashed line and open blue circles correspond to the cross-correlation functions of quenched and star-forming primary galaxies in the PrimB case, respectively. The dashed lines and open circles are then the results after removing the galaxies that mostly contribute to the two-halo galactic conformity. The sub-panel shows the ratio between the correlation function of each sub-sample and the respective parent sample. The solid and dashed lines are for the cases Q PrimAll and Q PrimB, respectively. The solid and open circles are for the cases SF PrimAll and SF PrimB, respectively. There is an overlap in the circles because both ratios are close to unity.