text: [10] report that, during its ﬂaring 
  epochs, 3C 454.3 transitions from its typical FSRQ 
  state to a more BL Lac-like state, where the syn- 
  chrotron component emits much more strongly com- 
  pared to the γ-ray component than during its “low 
  state”. 3C 454.3, which is the highest submillime- 
  ter luminosity FSRQ in our sample, would then shift 
  down and to the right in Figure 5 when it enters a 
  ﬂaring period. For the ﬁrst three months of the Fermi 
  mission, 3C 454.3 was not ﬂaring, which may explain 
  its present location in Figure 5. The three objects for 
  which there is a type discrepancy between CGRaBS 
  and LBAS are all FSRQs (in CGRaBS) and exhibit 
  
  Sikora et al. 
  
  eConf C091122 