Same as Fig. 2 but binning the sample in distance, R_gs, from satellite to central, and restricting it to satellites hosted by halos whose central galaxy’s minor axis is aligned to the nearest filament within a 37° double cone, for which the coplanar and filamentary trends compete. Results are stacked for 0.3 < z < 0.8 for different radius R_gs bins. Satellites close to their central tend to be distributed on the galactic plane, hence orthogonally to the filament, while satellites in the outskirts of the halo are strongly aligned with the filament and the coplanarity with the central is lost.