VERITAS observations of Geminga

The Geminga x-ray source was first detected by SAS-2 and COS-B, and has been identified as a radio quiet pulsar associated with a 300,000 year old supernova remnant. During 2007 VERITAS performed observations to search for potential TeV gamma ray emission from the Geminga pulsar and the region near Geminga. In this presentation, we describe these measurements and the analysis of these observations.