Percentage deviations of the XSB profiles of halos located in filaments (green), compared to those in the filament-void transition region (left panel: red lines) and in voids and walls (right: purple lines). We also show the effect of varying the halo-mass bins, where the dotted lines represent the M_200 m ∈ 10^{12 − 12.5}  M_⊙ halos, whereas the dashed and solid lines represent the M_200 m ∈ 10^{12.5 − 13}  M_⊙ and M_200 m ∈ 10^{13 − 13.5}  M_⊙ bins, respectively. We find that the XSB profiles of fil_gal are X-ray brighter in ∼(0.3 − 0.5)×R_200 m by 20 − 45% with respect to the fil-voids transit_gal and voids+wall_gal populations.