Fig. 6.
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Correlation between the X-ray surface brightness in three energy bands (0.3–0.45, 0.45–0.7, 0.7–2.3 keV in yellow, cyan and red, respectively) during e0 vs. the column density of neutral material (left panel). Correlation between the X-ray surface brightness in three energy bands vs. the density of galaxies which are a proxy for the distribution of hot baryons in Cosmic filaments (right panel).
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