The supernova remnant IC 443 is a very well studied source in the galactic plane. Many
observatories have observed this source with measurements ranging across the electromagnetic spectrum and with energies up to ∼2 TeV. Using data from the HAWC observatory, we further extended these measurements into the multi-TeV range, reaching energies higher than previous measurements. We study the emission region, study the source morphology, and model the energy spectrum, deriving the physical parameters of the corresponding acceleration mechanisms.
