text: 2009 Fermi Symposium, Washington, D.C., Nov. 2-5 
  
  (z = 0.341) detected in the VHE band. In addition, 
  VER J0521+211, likely associated with the radio-loud 
  AGN RGB J0521.8+2112, was detected by VERTAS 
  in ∼4 h of observations in October 2009 [23]. These 
  observations were motivated by its identiﬁcation as a 
  >30 GeV γ-ray source in the public Fermi-LAT data. 
  Its VHE ﬂux is 5% of the Crab Nebula ﬂux, placing it 
  among the brightest VHE blazars detected in recent 
  years. VERITAS later observed even brighter VHE 
  ﬂaring from VER J0521+211 in November 2009 [24], 
  leading to deeper VHE observations. 