Fig. C.1.

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Effect of the DisPerSE persistence threshold (set by the value of the cut parameter) on the resulting small-scale skeleton around three random galaxies (from top to bottom). The black points in the background present a random sub-sample 1/1000) of the underlying DM distribution, and the central white star indicates the position of the galaxy. These boxes have a side length of 3 cMpc/h.
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