  Fast radio bursts (FRBs) are bright, unresolved, millisecond-duration flashes
of radio emission originating from outside of the Milky Way. The source of
these mysterious outbursts is unknown, but their high luminosity, high
dispersion measure and short duration requires an extreme, high-energy,
astrophysical process. The majority of FRBs have been discovered as single
events which would require a chance coincidence for contemporaneous
multiwavelength observations. However, two have been observed to repeat: FRB
121102 and the recently detected FRB 180814.J0422+73. These repeating FRBs have
allowed for targeted observations by a number of different instruments,
including VERITAS. We present the VERITAS FRB observing program and the results
of these observations.

High Energy Astrophysical Phenomena;Instrumentation and Methods for Astrophysics