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.
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
eConf C091122