TeV Gamma-Ray Emission Observed from Geminga with HAWC

Geminga is a radio- quiet pulsar~250 parsecsfrom Earth that was first discovered as a GeV gamma-ray source and then identified as a pulsar. Milagroobserved an extended TeV source spatially consistent with Geminga. HAWC observes a similarly extended source. Observations of Geminga's flux and extension will be presented.