Mean quenched fractions of neighboring galaxies (f_Q) as functions of the real-space distance from primary galaxies hosted by low-mass halos of 10^11.6 ≤ M_h/h⁻¹ M_⊙ < 10^11.8 (main panel). The primary samples are separated by their sSFR. The f_Q is shown around quenched and star-forming PrimAll galaxies as a dark red solid line and navy blue solid circles, respectively. The red dashed line and blue open circles correspond, respectively, to the mean fractions after removing the quenched and star-forming primary galaxies in the vicinity of halos more massive than 10¹³ h⁻¹ M_⊙, i.e, the PrimB case. The lower sub-panel shows the difference in the mean quenched fractions of neighboring galaxies around quenched and star-forming primary galaxies at fixed halo mass. The solid line shows the PrimAll case, whereas the dashed line is the result obtained for PrimB. The dotted line denotes the case of zero difference, namely, where there is no conformity.