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Fig. 9
Fractions of gas mass, oxygen mass, and O vi mass in each phase of the CGM: cool, warm and hot (in blue, yellow and orange, respectively), as a function of stellar mass, at redshifts, z = 2,1 and 0 (from left to right) for S230D. The O vi masses are estimated by adopting the UVB of Faucher-Giguère et al. (2009).
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