Fig. 10.
Comparison between the 2AGL (black spectra; 30 MeV–10 GeV) and 3FGL (red spectra; 100 MeV–10 GeV) spectra for some of the most highly exposed AGILE–GRID sources. Error bars are 1σ statistical error; upper limits are 2σ. Different values in flux at the highest energy bands depend on the evaluation of the cut-off energies due to the statistics. Panel a: Vela pulsar. Panel b: 2AGL J2021+4029 (Gamma Cygni and LAT PSR J2021+4026). Panel c: 2AGL J1710−4429. Panel d: 2AGL J1836+5924 (PSR J1836+5925).
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