Table 3
Phase-folded stacking analysis of all available data for dedicated time intervals identified with a Bayesian Block approach (see Sect. 4.4 for details).
| Interval | Days from tp /[d] | tL /[h] | ΓVHE | Signif. |  |
|
|---|---|---|---|---|---|---|
| Int. 1 | [−108.085, −46.677] | 34.8 | 2.7 ± 0.1 | 11.0σ | 1.7 ± 0.2 | |
| Int. 2 | [−46.677, −31.944] | 31.2 | 2.91 ± 0.09 | 20.7σ | 4.0 ± 0.3 | |
| Int. 3 | [−31.944, −26.339] | 2.6 | 2.7 ± 0.2 | 12.1σ | 9.7 ± 1.2 | |
| Int. 4 | [−26.339, −12.334] | 29.4 | 2.4 ± 0.1 | 11.2 σ | 2.2 ± 0.2 | |
| Int. 5 | [−12.334, −6.052] | 11.9 | 2.8 ± 0.1 | 16.5σ | 5.7 ± 0.5 | |
| Int. 6 | [−6.052, 16.208] | 29.0 | 2.9 ± 0.2 | 8.7σ | 1.9 ± 0.3 | |
| Int. 7 | [16.208, 57.470] | 42.6 | 2.70 ± 0.04 | 39.8σ | 7.5 ± 0.3 | |
| Int. 8 | [57.470, 71.057] | 12.6 | 2.5 ± 0.1 | 11.8σ | 3.0 ± 0.3 | |
| Int. 9 | [71.057, 100.526] | 29.3 | 2.5 ± 0.1 | 9.4σ | 1.3 ± 0.2 |
Notes. Columns indicate the time range with respect to periastron passage tp, the total acceptance corrected observation time of the observations, the significance level of the stacked data set analysis, the photon index Γ, and integralflux above 1 TeV with statistical errors only (systematic uncertainties at the level of ~20% and ~ 0.1 are to be considered for the flux and photon index values, respectively).
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