Fig. 5.
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Mass function of the nodes connected to the filaments at different redshifts (thick curves). The vertical marks show the mean masses, which are 
, 13.30, 12.90, 12.47, and 12.06, respectively, from z = 0 to 4. For comparison, the thin curves give the mass functions of all the FoF haloes of the MTNG simulation with a stellar mass content of at least 108 M⊙.
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