text: • 1ES 0806+524: The observed SED of this new 
  VHE HBL can be explained by an SSC model 
  [16]. 
  
  • W Comae: This IBL, the ﬁrst discovered at 
  VHE, ﬂared twice in 2008 [14, 15]. Modeling of 
  the SED is improved by including an external- 
  Compton (EC) component in an SSC interpre- 
  tation. 
  
  • 3C 66A: This IBL ﬂared at VHE and MeV-GeV 
  energies in 2008[17, 18]. Similar to W Comae 
  and PKS 1424+240, modeling of observed SED 
  suggests a strong EC component in addition to 
  an SSC component. 
  
  • Mkn 421: This HBL exhibited major ﬂaring be- 
  havior for several months in 2008. Correlations 
  of the VHE and X-ray ﬂux were observed, along 
  with spectral hardening with increased ﬂux in 
  both bands [29].  The MWL aspect of the VERITAS blazar KSP has 
  also been highly successful. Every VERITAS obser- 
  vation of a known, or newly discovered, VHE blazar 
  has been accompanied by contemporaneous MWL ob- 
  servations. These data have resulted in the identiﬁca- 