Evolution of the filamentary trend (dashed line) and the coplanar trend (solid line) for either the central galaxy’s minor axis aligned to the filament axis within a 37° cone (toppanels), or the central galaxy’s minor axis perpendicular to the filament axis within a 37° cone (bottom panels). From left to right panel, three different central galaxy stellar mass bins M_g are shown asindicated in each panel. Results are stacked for 0.3 < z < 0.8. In the top panels, the two trends are mutually exclusive. This reveals a transitional pattern: coplanar trend takes over for massive centrals while the filamentary trend is dominant for low mass centrals, consistently with the limited influence of the central torques in this case. In the bottom panels, the two trends reinforce each other. Expectedly, the trends are strengthened for the most massive centrals.