text: Prior to the launch of Fermi VERITAS had discov- 
  ered VHE emission from 2 blazars. These included 
  the ﬁrst VHE-detected IBL, W Comae [14, 15], and 
  the HBL 1ES 0806+524 [16]. VERITAS has discov- 
  ered 6 VHE blazars since the launch of Fermi. Three 
  of these were initially observed by VERITAS prior to 
  the release of Fermi-LAT results, due to the X-ray 
  brightness of the synchrotron peaks of their SEDs. 
  
  **4. Blazar Discovery Program**
  
  The blazars observed in the discovery program are 
  largely high-frequency-peaked BL Lac objects. How- 
  ever, the program also includes IBLs (intermediate- 
  peaked) and LBLs (low-peaked), as well as ﬂat spec- 
  trum radio quasars (FSRQs), in an attempt to in- 
  crease the types of blazars known to emit VHE γ-rays. 
  The observed targets are drawn from a target list con- 
  taining objects visible to the telescopes at reasonable 
  zenith angles (−8◦ < δ < 72◦), without a previously 
  published VHE limit below 1.5% Crab, and with a 
  measured redshift z < 0.3. To further the study of the 