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Table 3.
Comparison of the current data set with previous MAGIC observations of the pulsed emission from the Crab Nebula.
| Reference | Emission component | Nexcess | FWHM | σ | Duration | Erange |
|---|---|---|---|---|---|---|
| [h] | [GeV] | |||||
| Aleksić et al. (2012) | P1+P2 | 1175 ± 116 | – | 10.4 | 73 | 46–416 |
| Aleksić et al. (2014) | P1 | 930 ± 120 | 0.025 ± 0.007 | 8 | 135 | 50–400 |
| P2 | 1510 ± 120 | 0.026 ± 0.004 | 12 | 135 | 50–400 | |
| Ansoldi et al. (2016) | P1 | 1252 ± 442 | 0.010 ± 0.003 | 2.86 | 320 | 100–400 |
| P2 | 2537 ± 454 | 0.040 ± 0.009 | 5.66 | 320 | 100–400 | |
| P1+P2 | 433 ± 73 | – | 6.06 | 16 | 43–368 | |
| This work | P1 | 144 ± 41 | 0.015 ± 0.005 | 3.5 | 16 | 43–368 |
| P2 | 289 ± 58 | 0.036 ± 0.009 | 4.9 | 16 | 43–368 | |
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