Table C.3.
Results of the correlation analysis between the spectral index and flux in the HE γ-ray band.
| Lightcurve | Period | r | p-value | Significance | p0 | p1 | χ2/ndof |
|---|---|---|---|---|---|---|---|
| 30-day bins | Pre-flare | 0.41 | 0.033 | 2.1σ | 7±2 | 0.7±0.2 | 4.1/20 |
| Daily bins | Flare | 0.32 | 0.10 | 1.7σ | 7±2 | 0.8±0.3 | 6.4/16 |
| 30-day bins | Post-flare | 0.25 | 0.32 | 1.0σ | 8±5 | 0.9±0.7 | 0.3/4 |
Notes. Columns: (1) Fermi-LAT lightcurve. (2) Period. (3) Pearson coefficient between Γγ and log10Fγ, estimated as described in Appendix A. (4), (5) p-value and significance for the null hypothesis of no-correlation. (6), (7) Best-fit parameters of the Γγ−log10Fγ trend with Eq. 6. (8) Goodness of fit, expressed as χ2 per number of degrees of freedom (ndof).
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