text: 2009 Fermi Symposium, Washington, D.C., Nov. 2-5 
  
  **3. VERITAS Blazar KSP**
  
  • All nearby (z < 0.3) HBL and IBL recom- 
  mended as potential VHE emitters in [5, 6, 7]. 
  
  • The X-ray brightest HBL (z < 0.3) in the recent 
  Sedentary [8] and ROXA [9] surveys. 
  
  • Several FSRQ recommended as potential VHE 
  emitters in [6, 11]. 
  
  • All nearby (z < 0.3) blazars detected by 
  
  • All nearby (z < 0.3) blazars contained in the 
  Fermi-LAT Bright AGN Sample [13]. 
  
  • All sources (|b| > 10◦) detected by Fermi-LAT 
  where extrapolations of their MeV-GeV γ-ray 
  spectrum (including EBL absorption; assuming 
  z = 0.3 if the redshift is unknown) indicates a 
  possible VERITAS detection in less than 20 h. 
  This criteria is the focus of the 2009-10 VERI- 
  TAS blazar discovery program. 