Relative effect of nodes and filaments of the cosmic web on the quenching of galaxies and the orientation of their spin

Open Access

Fig. A.1.

Density contrast distribution for all the critical points in the simulation box (blue) and those identified as closest to at least a subhalo (only maxima and bifurcations considered, in red) when performing the measurement of d_CP. The vertical black line shows the threshold in critical point density contrast we adopted.

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