Figure 4.
Same as Fig. 3, but with coloured lines representing different metallicity bins for the BH host galaxy. At z < 10 observable BHs are preferentially hosted by galaxies with Log(Z/Z⊙) ≥ −2, whereas at higher redshifts an increasing fraction of observable systems resides in galaxies with −3 ≤ Log(Z/Z⊙) < −2.

Same as Fig. 3, but with coloured lines representing different metallicity bins for the BH host galaxy. At z < 10 observable BHs are preferentially hosted by galaxies with Log(Z/Z) ≥ −2, whereas at higher redshifts an increasing fraction of observable systems resides in galaxies with −3 ≤ Log(Z/Z) < −2.

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