Galactic bars and active galactic nucleus fuelling in the second half of cosmic history

Open Access

Fig. D.1.

Bar fraction, f_bar, as a function of f_AGN(3–30 μm) (top) and L_disc (bottom) revised after including major mergers in the analysis. Markers and lines follow the same style as Figures 13 and 15. Empty symbols show the results presented in Figures 13 and 15.

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