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Table 4.
60 MeV–10 GeV spectral properties of the Crab Nebula measured in different flux states.
Component | State (b) | PL Γ | PLEC Γ | PLEC Ec | TSPLEC − TSPL(c) | Integrated flux (d) |
---|---|---|---|---|---|---|
(GeV) | (10−9 cm−2 s−1) | |||||
IC (a) | Average | 1.415 ± 0.023 | … | … | … | 107 ± 5 |
High | 2.830 ± 0.015 | 2.497 ± 0.041 | 0.77 ± 0.10 | 114.1 | 8432 ± 92 | |
Synchrotron | Average | 3.278 ± 0.011 | 3.250, ± 0.026 | 6.6 ± 5.7 | 1.7 | 2534 ± 15 |
Low | … | … | … | … | 370 ± 130 | |
Syn+IC | Low | 1.653 ± 0.048 | … | … | … | 221 ± 22 |
Notes.
(a)
The parameters of the IC component are determined from the complete ten-year data set, and are assumed to remain constant.
(b)
The high and low states are defined based on the 60 MeV–600 MeV light curve of the Crab Nebula (Fig. 2).
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