Fig. 1.
Visualisation of the datasets in spherical sky-coordinates: kernel-smoothed 2-dimensional density from the distribution of photometric galaxies on the viewed region of the sphere (grey background density), filamentary spines (orange spines), and spectroscopic galaxies (red dots). Darker grey denotes a higher density of photometric galaxies. All the drawn objects are located in the distance range of 400 − 600 Mpc.
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