Table B.1.
Results from the forward-folding fits with an LP up to 1.5 TeV to the single-night MAGIC VHE spectra that contains at least three spectral points beyond 1.5 TeV.
| MJD | f0 | Γ | b | χ2/d.o.f. | χ2/d.o.f. |
|---|---|---|---|---|---|
| [10−10 TeV−1 cm−2 s−1] | up to 1.5 TeV | above 1.5 TeV | |||
| 56857.98 | 2.54 ± 0.10 | −2.26 ± 0.06 | 0.15 ± 0.06 | 10.3/7 | 54.5/7 (6.0σ) |
| 2.92 ± 0.12 | −2.08 ± 0.06 | 0.10 ± 0.06 | 10.6/7 | 41.4/7 (5.0σ) | |
| 56858.98 | 3.26 ± 0.19 | −2.32 ± 0.06 | 0.18 ± 0.06 | 7.4/8 | 18.5/3 (3.6 σ) |
| 3.75 ± 0.21 | −2.15 ± 0.06 | 0.13 ± 0.06 | 8.0/8 | 14.8/3 (3.1 σ) | |
| 56859.97 | 2.33 ± 0.10 | −2.26 ± 0.05 | 0.21 ± 0.05 | 4.0/8 | 8.9/3 (2.2 σ) |
| 2.69 ± 0.12 | −2.10 ± 0.05 | 0.16 ± 0.05 | 3.9/8 | 5.7/3 (1.5 σ) | |
| 56864.02 | 1.35 ± 0.08 | −2.26 ± 0.06 | 0.12 ± 0.07 | 11.0/8 | 4.7/4 (1.0σ) |
| 1.56 ± 0.09 | −2.09 ± 0.06 | 0.08 ± 0.07 | 10.8/8 | 2.9/4 (0.6σ) | |
| 56865.00 | 2.06 ± 0.17 | −2.11 ± 0.09 | 0.22 ± 0.12 | 5.3/8 | 2.7/3 (0.8σ) |
| 2.38 ± 0.20 | −1.94 ± 0.09 | 0.17 ± 0.12 | 5.6/8 | 1.7/3 (0.5σ) | |
| 56866.00 | 3.14 ± 0.09 | −2.09 ± 0.03 | 0.07 ± 0.03 | 5.9/8 | 6.2/6 (0.8σ) |
| 3.63 ± 0.11 | −1.93 ± 0.03 | 0.02 ± 0.03 | 5.3/8 | 9.8/6 (1.5σ) | |
| 56867.0 | 2.35 ± 0.16 | −2.13 ± 0.07 | −6.6 × 10−3 ± 0.07 | 8.9/8 | 1.6/3 (0.4σ) |
| 2.71 ± 0.19 | −1.96 ± 0.07 | 0.05 ± 0.07 | 8.5/8 | 1.2/3(0.3σ) | |
| 56868.01 | 3.11 ± 0.12 | −2.08 ± 0.04 | 0.08 ± 0.05 | 14.8/8 | 10.1/4 (2.1σ) |
| 3.59 ± 0.14 | −1.91 ± 0.04 | 0.03 ± 0.05 | 14.0/8 | 16.6/4 (3.0σ) |
Notes. For each night the fit to the observed (first line) and the EBL-corrected (second line) using the model from Domínguez et al. (2011) are given. The table reports the data-model agreement, quantified with a χ2, for the spectral data below 1.5 TeV (goodness of fit) and above 1.5 TeV. The reported significances in the last column refer the confidence level at which the data-model agreement above 1.5 TeV can be rejected.
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