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arXiv · 1508.03497

TeV Gamma-Ray Emission Observed from Geminga with HAWC

B. M. Baughman·J. Wood
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Abstract

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.

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B. M. Baughman, J. Wood. 2015-08-14. TeV Gamma-Ray Emission Observed from Geminga with HAWC. https://arxiv.org/abs/1508.03497

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