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Fig. 11.


Left panel: MBH vs. Mdyn for J2310+1855 (red star) and compilation of AGNs. Violet circles: IBISCO hard X-ray selected sample at z <  0.05 (Feruglio et al., in prep.). Cyan circle: Brusa et al. (2018). Green symbols: red QSOs at z ∼ 2.5, for these we plot the ranges given in Banerji et al. (2012, 2017). Blue squares: QSO at z >  4.7 from Willott et al. (2013, 2015, 2017), Kimball et al. (2015), Wang et al. (2016), De Rosa et al. (2014), Venemans et al. (2016, 2017a), Trakhtenbrot et al. (2017), Decarli et al. (2018). Black symbol: z = 7.54 QSO from Venemans et al. (2017), Bañados et al. (2018). For the QSO for which there is no estimate of the inclination available, we have assumed i = 50 deg (see e.g., Decarli et al. 2018). The solid line is the local MBH − Mbulge relationship (Kormendy & Ho 2013). Middle panel: BH accretion rate, acc vs. SFR. Same symbols as in the left panel, except purple squares = hyper-luminous QSO at z = 3 − 4 from the WISSH sample (Bischetti et al. 2017; Duras et al. 2017; Vietri et al. 2018). The line is the locus of η =outflow/SFR = 1, assuming the scaling relation of outflow with Lbol derived for molecular outflows (Fiore et al. 2017). Right panel: black hole growth timescale, MBH/acc vs. the galaxy growth time, Mdyn/SFR. The solid line is the 1:1 relation.

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