Fig. 2.

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Mass dependence of outflow channels. The panels indicate different redshift intervals. We compare SF-driven outflows (black error bars, Sect. 2.1), AGN-driven outflows (blue, Sect. 2.2), and AGN jet cavities preventing inflows (orange, Sect. 2.3). AGN outflows are only weakly dependent on stellar mass. The horizontal dashed line indicates the inverse Hubble time at that redshift. In the two right redshift panels, the AGN jet power is extrapolated (open orange points).
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