Joshua Wood (University of Maryland, College Park)
Geminga is a radio-quiet pulsar ~250 parsecs from Earth that was first discovered as a GeV gamma-ray source and then identified as a pulsar. Milagro observed an extended TeV source spatially consistent with Geminga. HAWC observes a similarly extended source. Observations of Geminga’s flux and extension will be presented.
|Registration number following "ICRC2015-I/"||1160|
Brian Baughman (University of Maryland, College Park)