Outflow mass (left panel) and a proxy for the kinetic energy (right panel) versus the jet radio power. Circles are galaxies from Venturi et al. (2021), while the star corresponds to NGC 2110 (see Sect. 5.5). For this galaxy, the outflowing ionized gas mass corresponds only to that observed in the outflow region. The horizontal error bars for NGC 2110 take the errors in Eq. (16) of Bîrzan et al. (2008) into account, while vertical error bars include the uncertainties related to the extinction correction and the relative flux calibration between the two MEGARA gratings, as well as the uncertainty from the absolute flux calibration.