Table C.1.
Fit parameters to the Fermi-LAT light curve for P1 and P3 as a function of energy.
| Range | P1 | P3 | ||||
|---|---|---|---|---|---|---|
| ΦP1 | σL | σT |
 |
ΦP3 | σP3 | |
| (GeV) | (Phase units) | (Phase units) | (Phase units) | (Phase units) | (Phase units) | (Phase units) |
| 1–3 | 0.12979 ± 0.00014 | 0.008354 ± 0.000094 | 0.01462 ± 0.00032 | 0.1328 ± 0.0001 | 0.27454 ± 0.00058 | 0.3126 ± 0.0026 |
| 3–10 | 0.12964 ± 0.00029 | 0.006194 ± 0.00019 | 0.02372 ± 0.00078 | 0.1342 ± 0.0002 | 0.29985 ± 0.00077 | 0.2229 ± 0.0031 |
| 10–20 | 0.1298 ± 0.0012 | 0.00364 ± 0.00080 | 0.0199 ± 0.0021 | 0.1355 ± 0.0006 | 0.3162 ± 0.0023 | 0.1567 ± 0.0065 |
| > 20 | 0.1578 ± 0.0026 | 0.0137 ± 0.0049 | 0.0001 ± 0.005 | 0.148 ± 0.004 | 0.4116 ± 0.0043 | 0.387 ± 0.098 |
Notes. An asymmetric Lorentzian and a log-normal function have been used, respectively. The results for the estimated position of P1 using a Gaussian KDE (
) are also shown. The errors on the latter estimates were evaluated using a bootstrapping method.
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