Top-left: Same as Fig. 3, but the cross-correlations are between the most quenched or the 10% of the most star-forming central galaxies and the respective parent sample of primary galaxies. Top-right: Cross-correlations between the oldest or youngest central galaxies and the respective parent sample of primary galaxies. Bottom: Same as Fig. 2, but the primary samples are separated between the 10% of the most quenched and the 10% of the most star-forming central galaxies (left) and between the 10% of the oldest and 10% of the youngest central galaxies (right).