Fig. 7.
The y-axis is the quotient D dependent on the distance r, which is described by the x-axis. See Sect. 3.4 for a detailed description of D. The dark green line draws the quotient of distances from filamentary spines to photometric galaxy lines of sight and to lines of sight that are distributed randomly. The red line draws the quotient of distances from the filamentary spines to spectroscopic galaxy lines of sight and to lines of sight that are distributed randomly. The shaded areas surrounding the lines denote the calculated 0.95 confidence intervals.
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