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Table 2.
Observed VHE gamma-ray integral flux of the sample.
| (1) | (2) | (3) | (4) | (5) |
|---|---|---|---|---|
| Source name | Epoch | Ethr | F> Ethr | Prob (a) |
| (MJD) | (GeV) | (×10−11 cm−2 s−1) | % | |
| VER J0521+211 | 56580-56627 | 200 | 5.8 ± 0.6 | 1.1 |
| PKS 1424+240{ | 56740-56826 | 150 | 1.1 ± 0.2 | 69.5 |
| 57045-57187 | 150 | 0.6 ± 0.2 | 62.4 | |
| 1ES 1727+502 | 57307-57327 | 300 | 1.8 ± 0.3 | 0.08 |
| 1ES 1959+650{ | 57547 | 300 | 18.9 ± 1.1 | 12.8 |
| 57553 | 300 | 32.8 ± 1.3 | 12.7 | |
| 57711 | 300 | 3.8 ± 0.3 | 55.8 | |
| 1ES 2344+514{ | 57611-57612 | 300 | 3.8 ± 0.4 | 8.3 × 10−7 |
| 57611 | 300 | 6.9 ± 0.9 | 4.0 | |
| 57612 | 300 | 2.2 ± 0.5 | 82.0 |
Notes. Columns: (1) source name. (2) Observation epoch. (3) Energy threshold. (4) Observed integral flux above energy threshold. (5) Probability for a fit of the flux with a constant.
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