Fig. 3
WHIM density distribution at δLD ~ 65 (where the WHIM density peaks at δb ~ 26) using all the simulation data within the filamentary environments are shown with blue crosses and dashed lines. Red crosses indicate the distribution when using only volume elements with galaxies fainter than Mr = −20.5 (left panel), or with gas hotter than T = 5 × 106 K (right panel).
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