Figure 9.
The fraction of the SF (fSF) (left-hand panels) and the passive (fpas) (right-hand panels) BGGs versus the stellar mass of BGGs for S-I+S-II, S-III+S-IV, and S-V. The solid black line, dotted red line, dashed green line illustrate the trends in observations and the G11 and DLB07 models, respectively.
