Past and ongoing IFU surveys targeting the [O III] λ5007 emission line to study the properties of outflows in AGN host galaxies in the L_bol versus redshift plane. The grey data points represent surveys at z <  1 (Husemann et al. 2013, 2014, 2017; Liu et al. 2013; Harrison et al. 2014; Karouzos et al. 2016; Bae et al. 2017; Rupke et al. 2017), while the solid black symbols are collected from z >  1 studies (Nesvadba et al. 2006, 2017; Alexander et al. 2010; Harrison et al. 2012; Cresci et al. 2015; Carniani et al. 2015; Brusa et al. 2016; Kakkad et al. 2016; Vayner et al. 2017; Vietri et al. 2018). The blue shaded area covers the parameter space of the KASHz survey (Harrison et al. 2016) and the red shaded area that of the overall SUPER survey (Circosta et al. 2018). This paper presents an analysis on the Type 1 sub-sample of the SUPER survey, the data points of which are shown as cyan star symbols. Adapted from Circosta et al. (2018), to which we refer the reader for further details.