Critical AGN luminosity for radiatively driven quasar winds in the model of Murray et al. (2005) as a function of stellar mass. Large filled red dots and filled black dots show galaxies from our sample with measurements and upper limit of stellar mass, respectively. Small empty blue boxes and small empty black dots show the HeRGE galaxies without SINFONI observations and with measurements and upper limits on stellar mass, respectively. Quasar luminosities were taken from Drouart et al. (2014) and correspond to their AGN component of the FIR luminosity, which was scaled by a factor of 6 to approximate the bolometric QSO luminosity. The dashed red line shows the critical luminosity at which the momentum carried by the quasar radiation may balance gravity (see Murray et al. 2005, for details).