Molecular mass outflow rate as a function of AGN luminosity. Circles correspond to the QSO2s. Horizontal dotted lines indicate the position that they would occupy if we use the more conservative L_bol values derived from SED fitting from Jarvis et al. (2019). Blue squares are the CO outflows of Seyferts and ULIRGs compiled by Fiore et al. (2017), but dividing the outflow rates by a factor of 3 to match our outflow geometry (see Eq. (1)). Blue dashed line is the linear fit of the blue squares. Pink diamonds are the galaxies included in Table 7 that are not in Fiore et al. (2017) except NGC 1068 and IC 5063, for which they report different AGN luminosities and outflow rates.