Same as Fig. 2 where samples are binned in distance, R_gs, from satellite to central. We restrict the sample to centrals with a minor axis aligned with the nearest filament (within a 37 degree cone).This is plotted for four different satellite-to-central stellar mass ratios M_g ∕M_s < 0.05 (top panels),0.05 < M_g∕M_s < 0.1 (upper intermediate panels), 0.1 < M_g∕M_s < 0.2 (lower intermediate panels) and M_g∕M_s > 0.2 (bottom panels). To help the eye, the maximal amplitude of the alignment signals across the four mass bins are represented as dotted blue lines in the plots obtained for stellar mass bins with weaker signal. The minimal amplitude of the orthogonality signal across the four mass bins is represented as a dotted pink line in the plots obtained for stellar mass bins with stronger signals. Results are stacked for 0.3 < z < 0.8.