TeV Gamma-Ray Emission Observed from Geminga with HAWC
arXiv:1508.03497
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.
Presented at the 34th International Cosmic Ray Conference (ICRC2015), The Hague, The Netherlands. See arXiv:1508.03327 for all HAWC contributions
References in corpus (5)
- Observation of an anomalous positron abundance in the cosmic radiation
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- Milagro Observations of Multi-TeV Emission from Galactic Sources in the Fermi Bright Source List
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- A Search for Pulsations from Geminga Above 100 GeV with VERITAS