International audienceTo uniformly determine the properties of supernova remnants (SNRs) at high energies, we have developed the first systematic survey at energies from 1 to 100 GeV using data from the Fermi Large Area Telescope (LAT). Based on the spatial overlap of sources detected at GeV energies with SNRs known from radio surveys, we classify 30 sources as likely GeV SNRs. We also report 14 marginal associations and 245 flux upper limits. A mock catalog in which the positions of known remnants are scrambled in Galactic longitude allows us to determine an upper limit of 22% on the number of GeV candidates falsely identified as SNRs. We have also developed a method to estimate spectral and spatial systematic errors arising from the diffu...
International audienceTo uniformly determine the properties of supernova remnants (SNRs) at high ene...
The Astrophysical Journal Supplement Series 209.2 (2013): 34 reproduced by permission of the AASWe p...
We present the second catalog of high-energy gamma-ray sources detected by the Large Area Telescope ...
To uniformly determine the properties of supernova remnants (SNRs) at high energies, we have develop...
We present a detailed analysis of the GeV gamma-ray emission toward the supernova remnant (SNR) G8.7...
The supernova remnant (SNR) W49B originated from a core-collapse supernova that occurred between one...
While supernova remnants (SNRs) are widely thought to be powerful cosmicray accelerators, indirect e...
We report on the first detection of GeV high-energy gamma-ray emission from a young supernova remnan...
International audienceTo uniformly determine the properties of supernova remnants (SNRs) at high ene...
The Astrophysical Journal Supplement Series 209.2 (2013): 34 reproduced by permission of the AASWe p...
We present the second catalog of high-energy gamma-ray sources detected by the Large Area Telescope ...
To uniformly determine the properties of supernova remnants (SNRs) at high energies, we have develop...
We present a detailed analysis of the GeV gamma-ray emission toward the supernova remnant (SNR) G8.7...
The supernova remnant (SNR) W49B originated from a core-collapse supernova that occurred between one...
While supernova remnants (SNRs) are widely thought to be powerful cosmicray accelerators, indirect e...
We report on the first detection of GeV high-energy gamma-ray emission from a young supernova remnan...
International audienceTo uniformly determine the properties of supernova remnants (SNRs) at high ene...
The Astrophysical Journal Supplement Series 209.2 (2013): 34 reproduced by permission of the AASWe p...
We present the second catalog of high-energy gamma-ray sources detected by the Large Area Telescope ...