Fig. 4.

Phase portraits of gas, presenting the normalised 2D histograms of the gas cells in the corresponding structures. First panel: gas in filaments (within 1 Mpc from the core). Second panel: gas within the R200 radius of galactic haloes (defined as haloes of mass Mtot > 1012 M⊙ hosting at least one galaxy of mass 109 ≤ M∗[M⊙] ≤ 1012). Third panel: gas within the R200 radius of the DisPerSE maximum density critical points (CPmax), tracers of nodes. The 68% and 99% contours correspond to results of short (orange) and long filaments (blue), to galactic haloes (dotted green lines), and CPmax (dash-dotted red contours).
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