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Fig. 9.

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Scatter plot of temperature for baryonic gas as a function of dark matter density. Panels (a)–(f) are for z = 4–0, respectively. Gas with T < 105 K is the warm gas, gas with T > 107 K is the hot gas, and gas with temperatures between these two ranges is the WHIM. Note that regions of temperature below 104 K in the TNG data are not well resolved, particularly for the cells of star-forming gas (see Springel & Hernquist 2003), and should be interpreted with caution.

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