Open Access

Table A.1.

MAGIC analysis results.

MJD start MJD end F0.2−1 TeV F>1 TeV f0 α β χ2/dof
[10−10cm−2s−1] [10−11cm−2s−1] [10−10cm−2s−1TeV−1]
57727.248 57727.269 1.11 ± 0.15 0.17 ± 0.12 3.08 ± 0.31 2.77 ± 0.11 12.6/8
57729.244 57729.269 0.83 ± 0.13 0.00 ± 0.10 2.65 ± 0.28 2.42 ± 0.15 13.7/6
57749.217 57749.273 1.50 ± 0.14 0.46 ± 0.14 5.54 ± 0.41 2.53 ± 0.09 0.97 ± 0.24 7.2/9
57751.236 57751.278 1.62 ± 0.18 0.44 ± 0.17 5.63 ± 0.45 2.42 ± 0.08 0.64 ± 0.22 12.3/8
57753.184 57753.226 1.55 ± 0.14 0.89 ± 0.19 4.79 ± 0.23 2.39 ± 0.06 8.8/9
57756.183 57756.258 2.38 ± 0.14 1.37 ± 0.20 7.99 ± 0.34 2.20 ± 0.05 0.53 ± 0.10 7.5/11
57757.019 57757.281 3.82 ± 0.10 3.17 ± 0.14 12.10 ± 0.20 2.15 ± 0.02 0.28 ± 0.03 10.9/13
57762.157 57762.185 2.75 ± 0.21 2.26 ± 0.36 7.79 ± 0.35 2.20 ± 0.05 20.1/11
57763.154 57763.196 1.81 ± 0.14 1.02 ± 0.19 5.29 ± 0.25 2.29 ± 0.06 27.2/10
57771.127 57771.279 1.49 ± 0.07 0.72 ± 0.08 5.19 ± 0.19 2.38 ± 0.05 0.47 ± 0.11 15.6/12
57772.038 57772.059 2.41 ± 0.21 1.95 ± 0.29 9.78 ± 0.20 2.09 ± 0.03 0.25 ± 0.04 14.7/14
57776.190 57776.228 1.86 ± 0.15 0.76 ± 0.18 6.55 ± 0.40 2.30 ± 0.06 0.47 ± 0.15 19.6/9
57778.189 57778.276 2.16 ± 0.11 1.81 ± 0.18 6.70 ± 0.37 2.07 ± 0.08 0.47 ± 0.14 7.9/10
57780.185 57780.234 2.09 ± 0.14 1.44 ± 0.21 7.22 ± 0.35 2.21 ± 0.06 0.44 ± 0.12 9.3/11
57782.177 57782.203 0.87 ± 0.13 0.36 ± 0.16 2.95 ± 0.26 2.60 ± 0.11 5.8/9
57785.002 57785.140 3.38 ± 0.14 3.01 ± 0.22 10.60 ± 0.30 2.09 ± 0.03 0.36 ± 0.06 34.5/12
57788.039 57788.067 5.85 ± 0.29 7.39 ± 0.59 17.60 ± 0.55 1.95 ± 0.04 0.19 ± 0.05 10.7/14
57789.025 57789.099 3.01 ± 0.13 3.44 ± 0.26 9.68 ± 0.28 2.00 ± 0.04 0.29 ± 0.06 28.1/14
57789.969 57790.146 1.63 ± 0.08 1.07 ± 0.09 5.35 ± 0.20 2.18 ± 0.05 0.39 ± 0.09 8.8/11
57791.026 57791.145 1.08 ± 0.07 0.45 ± 0.08 3.78 ± 0.20 2.45 ± 0.07 0.50 ± 0.16 4.3/11
57792.160 57792.230 0.99 ± 0.08 0.48 ± 0.10 3.09 ± 0.18 2.53 ± 0.07 14.7/13
57800.065 57800.257 1.97 ± 0.07 1.01 ± 0.08 6.69 ± 0.20 2.29 ± 0.04 0.50 ± 0.09 16.7/11
57802.178 57802.199 1.56 ± 0.16 0.46 ± 0.17 4.54 ± 0.33 2.57 ± 0.10 12.7/10
57803.086 57803.166 1.93 ± 0.11 1.21 ± 0.16 6.36 ± 0.26 2.24 ± 0.04 0.37 ± 0.09 9.3/12
57806.091 57806.155 1.13 ± 0.08 0.63 ± 0.12 3.75 ± 0.17 2.44 ± 0.06 8.6/10
57807.108 57807.136 1.30 ± 0.14 0.66 ± 0.19 3.86 ± 0.24 2.38 ± 0.08 18.0/9
57809.082 57809.092 1.46 ± 0.26 1.37 ± 0.50 4.47 ± 0.45 2.23 ± 0.12 10.6/9
57811.103 57811.124 1.30 ± 0.15 0.93 ± 0.27 3.81 ± 0.28 2.20 ± 0.08 9.6/10
57812.931 57813.264 1.39 ± 0.06 0.98 ± 0.08 4.75 ± 0.16 2.09 ± 0.04 0.47 ± 0.09 14.0/10
57815.088 57815.103 1.50 ± 0.21 2.51 ± 0.55 4.80 ± 0.40 2.01 ± 0.09 7.7/11
57816.863 57816.956 1.12 ± 0.19 0.59 ± 0.08 3.46 ± 0.48 2.14 ± 0.18 2.8/7
57820.029 57820.196 1.07 ± 0.07 0.41 ± 0.08 3.66 ± 0.22 2.16 ± 0.10 0.95 ± 0.24 10.8/9
57833.101 57833.122 2.43 ± 0.21 1.42 ± 0.27 8.42 ± 0.57 2.11 ± 0.09 0.63 ± 0.19 3.8/9
57835.142 57835.162 1.18 ± 0.16 0.82 ± 0.20 3.63 ± 0.33 2.39 ± 0.11 7.1/10
57838.027 57838.048 0.83 ± 0.13 0.39 ± 0.16 2.44 ± 0.24 2.51 ± 0.11 24.5/10
57839.907 57840.233 0.83 ± 0.04 0.29 ± 0.05 2.87 ± 0.13 2.49 ± 0.05 0.50 ± 0.13 10.3/8
57841.020 57841.039 1.25 ± 0.17 0.79 ± 0.26 3.48 ± 0.30 2.19 ± 0.10 6.0/10
57841.866 57841.887 1.09 ± 0.16 0.35 ± 0.15 2.99 ± 0.36 2.80 ± 0.16 8.9/9
57843.951 57843.972 1.15 ± 0.16 0.76 ± 0.25 3.10 ± 0.27 2.20 ± 0.10 10.4/10
57846.038 57846.080 0.59 ± 0.08 0.21 ± 0.09 1.88 ± 0.16 2.59 ± 0.10 20.6/11
57846.945 57847.029 0.52 ± 0.07 0.45 ± 0.12 1.83 ± 0.15 2.37 ± 0.10 7.3/9
57847.958 57848.037 0.82 ± 0.07 0.26 ± 0.08 2.93 ± 0.22 2.45 ± 0.11 0.69 ± 0.26 8.1/9
57861.964 57862.009 1.88 ± 0.13 1.52 ± 0.22 5.51 ± 0.22 2.22 ± 0.04 15.8/12
57864.954 57865.003 1.75 ± 0.13 1.01 ± 0.18 5.73 ± 0.34 2.24 ± 0.06 0.43 ± 0.14 6.5/9
57866.952 57867.005 1.08 ± 0.10 0.83 ± 0.15 3.10 ± 0.17 2.21 ± 0.06 14.9/10
57889.925 57889.956 1.15 ± 0.12 0.89 ± 0.20 3.25 ± 0.23 2.18 ± 0.08 10.7/10
57890.930 57890.968 1.32 ± 0.11 1.10 ± 0.18 4.05 ± 0.22 2.21 ± 0.06 19.8/13
57891.939 57891.967 1.08 ± 0.12 0.75 ± 0.18 3.64 ± 0.26 2.37 ± 0.08 11.7/11

Notes. The start and end of each observation are listed in the first two columns. The 0.2-1 keV and > 1 TeV fluxes are given in the third and fourth column. The parameters of the log-parabolic (normalisation energy is 300 GeV) or power-law fits above 100 GeV with their corresponding χ2/dof are also listed. All fits were performed after correcting for the EBL absorption.

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