Phase-space of gas in filaments, including the contribution of galactic haloes (i.e. haloes of mass M_tot > 10¹² M_⊙ hosting at least one galaxy of mass 10⁹ ≤ M_∗[M_⊙] ≤ 10¹²). The 68% and 99% contours correspond to results of short (orange) and long filaments (blue), to galactic haloes (dotted green lines), and gas around the maximum density critical points of the field (CPmax, in dash-dotted red contours).