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Table A.3.

Spectral parameters for the MAGIC data from Mrk 501 in the energy range 0.1–10 TeV during the high activity in July 2014.

Date MJD Fit f0 Γ b χ2/d.o.f. p-value LP preference
[10−10 TeV−1 cm−2 s−1]
20140716 56854.91 PL 0.82 ± 0.10 −2.42 ± 0.11 11.6/8 0.2
PL 0.99 ± 0.12 −2.30 ± 0.12 9.8/8 0.3
20140717 56855.91 PL 1.24 ± 0.13 −2.39 ± 0.10 6.2/9 0.7
PL 1.48 ± 0.16 −2.27 ± 0.10 5.8/9 0.8
20140718 56856.91 PL 2.78 ± 0.15 −2.15 ± 0.05 10.7/11 0.5
PL 3.35 ± 0.18 −2.01 ± 0.05 9.1/11 0.6
20140720 56858.98 PL 2.94 ± 0.12 −2.19 ± 0.04 17.3/12 0.1
PL 3.53 ± 0.14 −2.04 ± 0.04 14.3/12 0.3
20140721 56859.97 LP 2.29 ± 0.10 −2.21 ± 0.04 0.15 ± 0.03 7.7/11 0.7 4.5σ
LP 2.66 ± 0.11 −2.05 ± 0.04 0.11 ± 0.03 6.6/11 0.8 3.4σ
20140723 56861.01 PL 1.42 ± 0.10 −2.22 ± 0.08 10.1/10 0.4
PL 1.69 ± 0.11 −2.06 ± 0.08 9.3/10 0.5
20140724 56862.02 PL 1.03 ± 0.05 −2.24 ± 0.06 11.8/11 0.4
PL 1.23 ± 0.06 −2.08 ± 0.06 9.1/11 0.6
20140725 56863.00 PL 1.16 ± 0.09 −2.12 ± 0.09 15.7/10 0.1
PL 1.38 ± 0.11 −1.97 ± 0.09 14.8/10 0.1
20140726 56864.02 PL 1.24 ± 0.05 −2.24 ± 0.04 15.2/13 0.3
PL 1.48 ± 0.06 −2.08 ± 0.04 12.5/13 0.5
20140727 56865.00 PL 1.75 ± 0.10 −2.14 ± 0.06 11.3/12 0.5
PL 2.09 ± 0.12 −1.97 ± 0.06 9.6/12 0.6
20140728 56866.00 LP 3.19 ± 0.08 −2.10 ± 0.02 0.09 ± 0.02 10.8/14 0.7 5.3 σ
PL 2.50 ± 0.07 −1.97 ± 0.02 17.6/15 0.3 2.7 σ
20140729 56867.00 PL 2.33 ± 0.11 −2.15 ± 0.05 10.2/12 0.6
PL 2.79 ± 0.13 −1.99 ± 0.05 9.8/12 0.6
20140730 56868.01 LP 3.17 ± 0.11 −2.09 ± 0.03 0.11 ± 0.03 22.8/12 0.03 4.5σ
LP 3.70 ± 0.12 −1.93 ± 0.03 0.09 ± 0.03 22.2/12 0.04 3.2σ
20140731 56869.92 PL 1.30 ± 0.08 −2.11 ± 0.07 8.2/10 0.6
PL 1.55 ± 0.10 −1.96 ± 0.07 9.0/10 0.5

Notes. Both a PL function and an LP function were used. For each night the observed spectral fits (first row) and EBL-corrected spectral fits using the EBL model from Domínguez et al. (2011) (second row) are provided. The parameters resulting from the fit with an LP (Eq. (4)) are provided when the LP function is preferred with respect to the PL function (Eq. (3)) with a significance higher than 3σ. The fit parameters for 2014 July 19 are reported in Table 3.

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