Fig. 6
Maximum velocity of the outflow versus the AGN LBol of the WISSH quasars compared with other samples from literature (i.e. Harrison et al. 2012, 2014; Genzel et al. 2014; Carniani et al. 2015; Perna et al. 2015a; Brusa et al. 2016; Nesvadba et al. 2006, 2008; Rupke & Veilleux 2013). The dashed line represents the relation 
(with arbitrary normalisation) expected for energy conserving winds (see Costa et al. 2014).
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