  Shell-type supernova remnants (SNRs) accelerate particles at the shock front
between the expanding remnant and the swept-up interstellar medium. If these
particles include protons and nuclei, very-high-energy gamma-ray emission may
result from the decay of pions produced in interactions between cosmic rays and
the local insterstellar medium. For SNRs that are interacting with a nearby
molecular cloud, such as IC 443, the enhanced matter density provides a target
medium that can amplify the gamma-ray emission. IC 443 also contains the pulsar
wind nebula (PWN) CXOU J061705.3+222127. PWNe are the most plentiful galactic
sources of very-high-energy gamma rays, which are produced in the shock formed
at the collision of the pulsar wind with the ambient medium.
  VERITAS is an array of four 12-m telescopes dedicated to gamma-ray astronomy
in the energy band above 100 GeV. Located on Mt. Hopkins in southern Arizona,
VERITAS operated during the 2006-2007 season in 2-, 3-, and 4-telescope
observation modes. In this talk, results from three-telescope observations of
the composite supernova remnant IC 443 during the 2006-2007 season are
discussed.
