Table 3
VHE AGN spectra used in this study.
| Source | Redshift | Experiment | Energy range | VHE slope | Fermi slope | Variability index | Reference | Comments |
| (TeV) | Γ ± σstat ± σsys | Γ ± σstat | ||||||
|
|
||||||||
| Mkn 421 | 0.031 | HESS | 1.75–23.1 | 2.05 ± 0.22 | 1.77 ± 0.01 | 112.8 | (1) | hardest index |
| Mkn 501 | 0.034 | MAGIC | 0.17–4.43 | 2.79 ± 0.12 | 1.64 ± 0.09 | 72.33 | (2) | hardest index |
| Mkn 501 | 0.034 | HEGRA | 0.56–21.45 | 1.92 ± 0.03 ± 0.20 | 1.64 ± 0.09 | 72.33 | (3) | hardest index |
| 1ES 2344+514 | 0.044 | MAGIC | 0.19–4.00 | 2.95 ± 0.12 ± 0.20 | 1.72 ± 0.08 | 28.13 | (4) | steady |
| Mkn 180 | 0.045 | MAGIC | 0.18–1.31 | 3.25 ± 0.66 | 1.74 ± 0.08 | 19.67 | (5) | steady |
| 1ES 1959+650 | 0.048 | HEGRA | 1.52–10.94 | 2.83 ± 0.14 ± 0.08 | 1.94 ± 0.03 | 52.30 | (6) | hardest index |
| 1ES 1959+650 | 0.048 | MAGIC | 0.19–2.40 | 2.58 ± 0.18 | 1.94 ± 0.03 | 52.30 | (7) | hardest index |
| BL Lacertae | 0.069 | MAGIC | 0.16–0.70 | 3.6 ± 0.5 | 2.11 ± 0.04 | 267.0 | (8) | hardest index |
| PKS 2005-489 | 0.071 | HESS | 0.34–4.57 | 3.20 ± 0.16 ± 0.10 | 1.90 ± 0.06 | 68.86 | (9) | hardest index |
| RGB J0152+017 | 0.080 | HESS | 0.31–2.95 | 2.95 ± 0.36 ± 0.20 | 1.79 ± 0.14 | 27.73 | (10) | steady |
| PKS 2155-304 | 0.116 | HESS | 0.25–3.20 | 3.34 ± 0.05 ± 0.1 | 1.81 ± 0.11 | 262.9 | (11) | simul |
| RGB J0710+591 | 0.125 | VERITAS | 0.42–3.65 | 2.69 ± 0.26 ± 0.20 | 1.53 ± 0.12 | 29.86 | (12) | steady |
| H 1426+428 | 0.129 | HEGRA | 0.78–5.37 | – | 1.32 ± 0.12 | 22.16 | (13) | steady |
| 1ES 0806+524 | 0.138 | MAGIC | 0.31–0.63 | 3.6 ± 1.0 ± 0.3 | 1.94 ± 0.06 | 37.80 | (14) | steady |
| H 2356-309 | 0.165 | HESS | 0.23–1.71 | 3.06 ± 0.15 ± 0.10 | 1.89 ± 0.17 | 20.19 | (15) | steady |
| 1ES 1218+304 | 0.182 | MAGIC | 0.09–0.63 | 3.0 ± 0.4 | 1.71 ± 0.07 | 40.00 | (16) | steady |
| 1ES 1218+304 | 0.182 | VERITAS | 0.19–1.48 | 3.08 ± 0.34 ± 0.2 | 1.71 ± 0.07 | 40.00 | (17) | steady |
| 1ES 1101-232 | 0.186 | HESS | 0.18–2.92 | 2.88 ± 0.17 | 1.80 ± 0.21 | 25.74 | (18) | steady |
| 1ES 1011+496 | 0.212 | MAGIC | 0.15–0.59 | 4.0 ± 0.5 | 1.72 ± 0.04 | 48.05 | (19) | hardest index |
| 1ES 0414+009 | 0.287 | HESS | 0.17–1.13 | 3.44 ± 0.27 ± 0.2 | 1.98 ± 0.16 | 15.56 | (20) | steady |
| PKS 1222+21 a | 0.432 | MAGIC | 0.08–0.35 | 3.75 ± 0.27 ± 0.2 | 1.95 ± 0.21 | 13030 | (21) | simul |
| 3C 279 | 0.536 | MAGIC | 0.08–0.48 | 4.1 ± 0.7 ± 0.2 | 2.22 ± 0.02 | 2935 | (22) | hardest index |
|
|
||||||||
| 1ES 0229+200 b | 0.140 | HESS | 0.60–11.45 | 2.5 ± 0.19 ± 0.10 | – | – | (23) | – |
Notes. If not stated otherwise in the text, the Fermi slope and variability index are taken from the 2FGL. See the text for details on the Comments column.
There was no simultaneous measurement during the 0.5 h in which MAGIC detected the source. However, the index used in high energies was extracted from Fermi data in the 2.5 h before and after the MAGIC observation (Aleksić et al. 2011).
The spectrum is only tested against the IntVHELumi criterion as it is not detected with the Fermi-LAT.
References. (1) Tluczykont (2011); (2) Abdo et al. (2011a); (3) Aharonian et al. (1999); (4) Albert et al. (2007a); (5) Albert et al. (2006b); (6) Aharonian et al. (2003b); (7) Tagliaferri et al. (2008); (8) Albert et al. (2007b); (9) HESS Collaboration et al. (2010b); (10) Aharonian et al. (2008a); (11) Aharonian et al. (2009); (12) Acciari et al. (2010); (13) Aharonian et al. (2003a); (14) Acciari et al. (2009a); (15) HESS Collaboration et al. (2010a); (16) Albert et al. (2006a); (17) Acciari et al. (2009b); (18) Aharonian et al. (2006); (19) Albert et al. (2007c); (20) HESS Collaboration et al. (2012); (21) Aleksić et al. (2011); (22) Albert et al. (2008); (23) Aharonian et al. (2007a).
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