FERMI-LAT-SCIENTIFIC PLOTS
a7
Phase-resolved spectral energy distributions of the Crab Pulsar. The labels indicate the phase intervals. Spectral results are presented in Table 2. The black dotted curve is the best-fit power-law with an exponential cut-off. The LAT spectral points (cf. Figure 5 for the description of the conventions) are obtained using the model-independent maximum likelihood method described in Section 4.2. 90% C.L. upper limits are computed when the statistical significance is lower than 3σ.
a7
Phase-resolved spectral energy distributions of the Crab Pulsar. The labels indicate the phase intervals. Spectral results are presented in Table 2. The black dotted curve is the best-fit power-law with an exponential cut-off. The LAT spectral points (cf. Figure 5 for the description of the conventions) are obtained using the model-independent maximum likelihood method described in Section 4.2. 90% C.L. upper limits are computed when the statistical significance is lower than 3σ.