Gamma-ray emission from the shell of supernova remnant W44 revealed by the Fermi LAT
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Pelassa, V
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Pesce Rollins, M
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Although the analysis was performed by using events above 200 MeV, the quoted flux was obtained by extrapolating the best-fit function down to 100 MeV to make it easier to compare the value with past publications on GeV gamma-ray observations.
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Although the analysis was performed by using events above 200 MeV, the quoted flux was obtained by extrapolating the best-fit function down to 100 MeV to make it easier to compare the value with past publications on GeV gamma-ray observations.
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The Fermi LAT Collaboration acknowledges support from a number of agencies and institutes for both development and the operation of the LAT as well as scientific data analysis. These include NASA and Department of Energy in the United States; CEA/lrfu, IN2P3/CNRS, and Centre National d'Études Spatiales in France; ASI, INFN, and INAF in Italy; Ministry of Education, Culture, Sports, Science, and Technology, High Energy Accelerator Research Organization (KEK) and JAXA in Japan; and the K. A. Wallenberg Foundation, the Swedish Research Council, and the National Space Board in Sweden.
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The Fermi LAT Collaboration acknowledges support from a number of agencies and institutes for both development and the operation of the LAT as well as scientific data analysis. These include NASA and Department of Energy in the United States; CEA/lrfu, IN2P3/CNRS, and Centre National d'Études Spatiales in France; ASI, INFN, and INAF in Italy; Ministry of Education, Culture, Sports, Science, and Technology, High Energy Accelerator Research Organization (KEK) and JAXA in Japan; and the K. A. Wallenberg Foundation, the Swedish Research Council, and the National Space Board in Sweden.
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