Updated figure from Bonanomi et al. (2023), first presented in Marasco et al. (2020) and Tozzi et al. (2021), with the addition of 2M0918 (gray shaded area) and Mrk 509 (Zanchettin et al. 2021). This plot contains a compilation of sources for which UFO and galaxy-scale wind energetics are available, with the large-scale winds being either ionized, molecular or atomic. The ratio of the outflow momentum rates {\dot{P}_{\mathrm{OUT}}/\dot{P}_{\mathrm{UFO}}} /Ṗ_UFO is plotted for each source, together with values predicted from theory for momentum-driven or energy-driven scenarios. The predicted value can be estimated as the ratio V_OUT/V_UFO by imposing the conservation of energy, while the dashed line at Ṗ_OUT/Ṗ_UFO = 1 is the prediction of a momentum-driven scenario. For 2M0198, the average between the Ṗ_OUT derived from [OIII] and H_α was used. The compilation uses various reported values (Bischetti et al. 2019; Braito et al. 2018; Chartas et al. 2009; Cicone et al. 2014; Feruglio et al. 2015, 2017; García-Burillo et al. 2014; González-Alfonso et al. 2017; Longinotti et al. 2015, 2018; Lutz et al. 2020; Marasco et al. 2020; Mizumoto et al. 2019; Reeves & Braito 2019; Rupke et al. 2017; Sirressi et al. 2019; Smith et al. 2019; Tombesi et al. 2015; Tozzi et al. 2021; Veilleux et al. 2017; Zanchettin et al. 2021).