Same as Fig. 2 where samples are binned in distance, R_gs, from satellite to central. This is plotted for three different central stellar mass bins: 10⁹ < M_g < 10¹⁰ M_⊙ (top panels),10¹⁰ < M_g < 10^10.5 M_⊙ (middle panels) and M_g > 10^10.5 M_⊙ (bottom panels). The amplitude of the signal for the lowest mass bin (10⁹ < M_g < 10¹⁰ M_⊙) is represented as a grey area in the plots obtained for higher stellar mass bins. Satellites close to the central galaxy tend to be distributed on the galactic plane with marginal alignment to the filament, while satellites in the outskirt of the host halo of the central are strongly aligned with the filament but the coplanarity with the central galaxy is weakened. Results are stacked for 0.3 < z < 0.8.