Figure 10.
Fractional impact of baryonic physics for the different AGN models as a function of the relative mass within haloes with respect to the NoAGN simulation. Different symbols represent this quantity for the stellar mass (star symbols), gas mass (square symbols), and total baryonic mass (including SMBH mass; circle symbols). Different fable runs are displayed with different symbol colours (see the legend below panels). We also include separate power-law best fits (see text) to the stars, gas, and total baryons symbols, as yellow, green, and blue bands, respectively. Relative baryonic mass within haloes provides the best tracer for the relative suppression of power, both at $k_\text{scale} = 10\, \,\,\text{h}\,\,\text{cMpc}^{-1}$ and $k_\text{scale} = 1\, \,\,\text{h}\,\,\text{cMpc}^{-1}$.

Fractional impact of baryonic physics for the different AGN models as a function of the relative mass within haloes with respect to the NoAGN simulation. Different symbols represent this quantity for the stellar mass (star symbols), gas mass (square symbols), and total baryonic mass (including SMBH mass; circle symbols). Different fable runs are displayed with different symbol colours (see the legend below panels). We also include separate power-law best fits (see text) to the stars, gas, and total baryons symbols, as yellow, green, and blue bands, respectively. Relative baryonic mass within haloes provides the best tracer for the relative suppression of power, both at |$k_\text{scale} = 10\, \,\,\text{h}\,\,\text{cMpc}^{-1}$| and |$k_\text{scale} = 1\, \,\,\text{h}\,\,\text{cMpc}^{-1}$|⁠.

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