Distributions of ⟨θ⟩ as a function of the distances from the features of the cosmic web d_fil (dashed red line in every panel), d_CP (dotted blue line in every panel), and d_skel (solid orange line in every panel). The first panel shows the distributions obtained when all subhalo components are considered (same as the top middle panel of Figure 6), the subsequent panels refer to the distributions obtained when only the gas component is considered (second panel), only the stellar component (third panel), and when both gas and stars (but not dark matter) are considered (bottom panel). The dashed black line in every panel is the average of the considered quantity in the full simulation box. In the top middle panel, the grey line is , computed given equation (3) for the total subhalo sample. In every panel, the first distance bin considered extends all the way to zero for all distances, but it is cut because the x-axis is in logarithmic scale.