Kinetic power Ė_kin (left plot) and thrust (right) vs. bolometric luminosity for the C IVλ1549 emission line. The two outflow parameters were estimated by varying the outflow radius depending on λL_λ as defined in Kaspi et al. (2021). Magenta dashed lines indicate the least squares linear regression. Black dotted, continuous, and dashed lines show ${\dot{E}}_{\mathrm{kin}}=L_{\mathrm{bol}}$, ${\dot{E}}_{\mathrm{kin}}=0.05L_{\mathrm{bol}}$, and ${\dot{E}}_{\mathrm{kin}}=0.005L_{\mathrm{bol}}$ respectively. The dotted line in the right panel indicates ${\dot{M}}_{\mathrm{out}}{v}_{\mathrm{o}}=L_{\mathrm{bol}}/c$. Typical uncertainties are displayed in the bottom-right corner of the plots. The color scheme is the same as that in Fig. 4.