Random Forest quenching classification for bulge and disk structures in CANDELS for the full redshift range (0.5 < z < 2.0), based on UVJ colours. Results for galaxies treated as a whole are shown in black; results for bulge structures and disk structures treated separately are shown in red and blue, respectively. For both bulge and disk structures, bulge mass is clearly found to be the most important parameter governing quenching at high redshifts. Note also that all other parameters are consistently found to be of very little predictive power, even disk mass in disk structures. Compare to Fig. 9 for the low redshift results, which show a very similar trend.