We present observations of the young supernova remnant (SNR) RX J1713.7-3946 with the Fermi Large Area Telescope (LAT). We clearly detect a source positionally coincident with the SNR. The source is extended with a best-fit extension of 0 degrees.55 +/- 0 degrees.04 matching the size of the non-thermal X-ray and TeV gamma-ray emission from the remnant. The positional coincidence and the matching extended emission allow us to identify the LAT source with SNR RX J1713.7-3946. The spectrum of the source can be described by a very hard power law with a photon index of Gamma = 1.5 +/- 0.1 that coincides in normalization with the steeper H. E. S. S.-detected gamma-ray spectrum at higher energies. The broadband gamma-ray emission is consistent wit...
We present observations of the young Supernova remnant (SNR) RX J1713.7-3946 with the Fermi Large Ar...
We present observations of the young supernova remnant (SNR) RX J1713.7-3946 with the Fermi Large Ar...
We report on gamma-ray observations of the supernova remnant (SNR) RX J0852.0-4622 with the Large Ar...
We present observations of the young supernova remnant (SNR) RX J1713.7-3946 with the Fermi Large Ar...
We present observations of the young Supernova remnant (SNR) RX J1713.7-3946 with the Fermi Large Ar...
We present observations of the young supernova remnant (SNR) RX J1713.7-3946 with the Fermi Large Ar...
We report on gamma-ray observations of the supernova remnant (SNR) RX J0852.0-4622 with the Large Ar...
We present observations of the young supernova remnant (SNR) RX J1713.7-3946 with the Fermi Large Ar...
We present observations of the young Supernova remnant (SNR) RX J1713.7-3946 with the Fermi Large Ar...
We present observations of the young supernova remnant (SNR) RX J1713.7-3946 with the Fermi Large Ar...
We report on gamma-ray observations of the supernova remnant (SNR) RX J0852.0-4622 with the Large Ar...