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Fig. 9.

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Fig. 8 continued. Models of the soft X-ray surface brightness profiles for the stellar mass-selected sample with mass M* > 1.7 × 1010 M (top left, 10.25), M* > 3.1 × 1010 M (top right, 10.5), M* > 5.6 × 1010 M (bottom left, 10.75), M* > 1011 M (bottom right, 11.0). The model accounts well for the measurements. The point source, satellite and two-halo terms show little evolution. The hot gas model brightness increases significantly with the stellar mass threshold.

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