text: tion of correlated VHE and X-ray ﬂux variability, as 
  well as correlated spectral hardening in both the VHE 
  and X-ray bands. The VHE MWL observations were 
  performed in both ”quiescent” and ﬂaring states for 
  some of the observed blazars. For the observed HBL 
  objects, the SEDs can be well described by a simple 
  SSC model in both high and low states. However, an 
  additional external Compton component is necessary 
  to adequately ﬁt the SEDs of the IBL objects. 
  
  orating institutions in the construction and operation 
  of the instrument. 
  
  **References**
  
  The Fermi-LAT is already having a signiﬁcant im- 
  pact on the blazar KSP. In future seasons, the VER- 
  ITAS blazar discovery program will focus its dis- 
  covery program on hard-spectrum blazars detected 
  by Fermi-LAT, and will likely have a greater focus 
  on high-risk/high-reward objects at larger redshifts 
  (0.3 < z < 0.7). 
  In addition, the number of VHE 
  blazars studied in pre-planned MWL campaigns will 
  increase as data from the Fermi-LAT will be publicly 
  available. 
  In particular, the extensive pre-planned 
  MWL campaigns will focus on objects that are note- 
  worthy for the impact their data may have on under- 
  standing the EBL. The simultaneous observations of 
  blazars by VERITAS and Fermi-LAT will completely 
  resolve the higher-energy SED peak, often for the ﬁrst 
  time, enabling unprecedented constraints on the un- 
  derlying blazar phenomena to be derived. 