Top panel: distribution of the non-parametric velocity, w₈₀ measured for [O III] λ5007 line, for AGN and star forming samples from different surveys. The AGN sample consists of targets from the SUPER survey in red (this paper) and targets from KASHz survey matched in redshift in hatched black (Harrison et al. 2016). The Type 1 sample used in this paper has a median hard X-ray luminosity of 10^44.8 erg s⁻¹ and the redshift-matched KASHz targets have a median X-ray luminosity of 10^43.9 erg s⁻¹. The blue histogram shows the w₈₀ distribution of mass-matched low redshift star forming sample from Wylezalek et al. (2020), while the ocean-blue vertical bar shows the w₈₀ value from the redshift and mass-matched star forming sample from the KLEVER survey (334 ± 35 km s⁻¹, Curti et al. 2020). The dashed black-line at 600 km s⁻¹ corresponds to the w₈₀ value used in this work to define if a target hosts an AGN-driven outflow. Lower panel: inverse cumulative w₈₀ distribution with the same colour coding as in the top panel. It is clear from both the panels that targets from the SUPER survey occupy the higher end of the w₈₀ distribution. Based on the w₈₀ criteria, all the targets in the SUPER survey show the presence of outflows, and ∼52% of the redshift matched targets in the KASHz survey show outflows.