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A clue to finding the long-sought sources of cosmic rays is the recentobservation of an astrophysical flux of high-energy neutrinos by the IceCubedetector, since these possibly originate in hadronic interactions at cosmic-rayaccelerators. While the neutrino sky map shows no significant indication ofpoint sources so far, it is possible to utilize the sensitivity of Imaging AirCherenkov Telescope (IACT) arrays, such as VERITAS, to search for hadronicgamma-ray emission from the neutrino directions.  Over the last 2 years, the positions of neutrino events detected by IceCubehave been observed using the VERITAS array. Observations have been limited tomuon neutrino events, since their typical angular reconstruction uncertainty isbelow 1 degree, smaller than the 3.5-degree diameter of the VERITAS field ofview. The location of VERITAS further constrains the neutrino event positionsthat can be observed to those located in the northern sky, or at moderatesouthern declinations. The list of observed positions was selected frompublished results and a set of high-energy muon tracks provided by IceCube. Wepresent the current status and some preliminary results from this program.

Searching for TeV gamma-ray emission associated with IceCube high-energy neutrinos using VERITAS