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DETECTION OF THE PULSAR WIND NEBULA HESS J1825โ€“137 WITH THE<i>FERMI</i>LARGE AREA TELESCOPE

DETECTION OF THE PULSAR WIND NEBULA HESS J1825โ€“137 WITH THE<i>FERMI</i>LARGE AREA TELESCOPE

We announce the discovery of 1 - 100 GeV gamma-ray emission from the archetypal TeV pulsar wind nebula HESS J1825-137 using 20 months of survey data from the Fermi Large Area Telescope (LAT). The gamma-ray emission detected by the LAT is significantly spatially extended, with a best-fit rms extension of โ€ฆ