Fig. 11.
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Ionized mass outflow rates versus bolometric luminosities compiled from the literature by Fiore et al. (2017) for a sample of AGN with z < 0.5 (black points), and by Musiimenta et al. (in prep.) for AGN at z > 0.5 (grey points). The red and blue stars correspond to J0945 using the electron density calculated in Sect. 3.2 (ne = 662 cm−3) and the value of 200 cm−3 assumed by Fiore et al. (2017).
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