Table 1
Data sets on VHE blazars detected by H.E.S.S. that are used for this study of the EBL.
| Data set | Nγ | σ | Emin − Emax |
| [TeV] | |||
|
|
|||
| Mrk 421 (1) | 3381 | 96.7 | 0.95−41 |
| Mrk 421 (2) | 5548 | 135 | 0.95−37 |
| Mrk 421 (3) | 5156 | 134 | 0.95−45 |
| PKS 2005-489 (1) | 1540 | 25.3 | 0.16−37 |
| PKS 2005-489 (2) | 910 | 28.9 | 0.18−25 |
| PKS 2155-304 (2008) | 5279 | 99.2 | 0.13−19 |
| PKS 2155-304 (1) | 3499 | 93.0 | 0.13−5.7 |
| PKS 2155-304 (2) | 3470 | 116 | 0.13−9.3 |
| PKS 2155-304 (3) | 9555 | 186 | 0.13−14 |
| PKS 2155-304 (4) | 4606 | 132 | 0.18−4.6 |
| PKS 2155-304 (5) | 11 901 | 219 | 0.13−5.7 |
| PKS 2155-304 (6) | 6494 | 166 | 0.15−5.7 |
| PKS 2155-304 (7) | 8253 | 191 | 0.20−7.6 |
| 1ES 0229+200 | 670 | 12.6 | 0.29−25 |
| H 2356-309 | 1642 | 21.2 | 0.11−34 |
| 1ES 1101-232 | 1268 | 17.8 | 0.12−23 |
| 1ES 0347-121 | 604 | 13.5 | 0.13−11 |
Notes. For highly variable sources, the data are divided into smaller subsets that are indexed in Col. 1 and correspond to restricted flux ranges. The photon excess, detection significance, and energy range of the spectra (in TeV) are given in Cols. 2 − 4, respectively.
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