![]() Since these two pulsars are close to the Galactic plane we run our analysis with ten different interstellar emission models (IEMs) to study the systematics due to the modeling of this component. We analyze, for the first time, almost 10 years of γ-ray data obtained with the Fermi Large Area Telescope at E γ > 8 GeV in the direction of Geminga and Monogem. ![]() The HAWC Collaboration has discovered a γ-ray emission extended about 2 degrees around the Geminga and Monogem pulsar wind nebulae (PWNe) at γ-ray energies E γ > 5 TeV.
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