text: VHE emission from 3C 66A was discovered by VER- 
  ITAS in September 2008 [17] during a ﬂaring episode 
  that was also observed by the Fermi-LAT [18]. The 
  observed ﬂux above 200 GeV was 6% of the Crab Neb- 
  ula ﬂux and the measured VHE spectrum was very 
  soft (ΓVHE ∼ 4.1). RGB J0710+591 was detected 