Same panels as in Fig. 8, showing SUPER type-2 (filled red circles) and type-1 (filled blue circles) measurements along with IFS-based results from the literature of other type-2 (empty red star; XID5395, Brusa et al. 2016) and type-1 AGN (empty blue symbols; Cano-Díaz et al. 2012; Carniani et al. 2015; Vayner et al. 2021a) at z ∼ 1 − 3. The orange symbols represent red obscured systems that were nevertheless optically classified as type-1 AGN (Perrotta et al. 2019; Vayner et al. 2021b; Cresci et al. 2023; Veilleux et al. 2023). Outflow velocities from Brusa et al. (2016) and Perrotta et al. (2019) have been corrected to account for discrepancies with the v_out and v_max definitions we adopted (see Sect. 6). While the ‘standard’ blue type-1 and red type-2 from the literature agree with values found in SUPER, the orange points, almost all at L_bol ≳ 10⁴⁷ erg s⁻¹, clearly show that higher outflow velocities are recovered when we select optical type-1 but dusty obscured objects.