Table 3.
Best-fit power-law model parameters of observed Fermi-LAT spectrum.
| Name | TS | PL Index | Flux |
|---|---|---|---|
| 1 | 2 | 3 | 4 |
| 1ES 0120+340 | |||
| 2015/01-2021/01 [L1] | 53.32 | 1.35 ± 0.25 | 0.11 ± 0.04 |
| RGB J0710+591 | |||
| 2008/09-2009/08 [L1] | 92.99 | 1.45 ± 0.14 | 2.06 ± 0.83 |
| 2013/01-2016/12 [L2] | 102.20 | 1.67 ± 0.11 | 0.32 ± 0.06 |
| 2017/01-2021/01 [L3] | 139.87 | 1.76 ± 0.12 | 0.54 ± 0.07 |
| 1ES 1101–232 | |||
| 2009/01-2015/01 [L1] | 52.05 | 1.63 ± 0.19 | 0.31 ± 0.09 |
| 2015/01-2019/01 [L2] | 63.3 | 1.65 ± 0.15 | 0.35 ± 0.08 |
| 1ES 1741+196 | |||
| 2010/01-2011/01 [L1] | 45.72 | 1.84 ± 0.15 | 5.45 ± 2.32 |
| 2017/01-2021/01 [L2] | 161.25 | 1.86 ± 0.08 | 4.97 ± 1.21 |
| 1ES 2322–409 | |||
| 2019/01-2021/01 [L1] | 787 | 1.79 ± 0.05 | 7.17 ± 0.97 |
Notes. Column 1: Source name with LAT integration time and abbreviation for different spectra. Column 2: Test-statistic values. Column 3: Photon index 1σ error. Column 4: Integrated flux in the energy range 0.3–300 GeV with 1σ error in units of 10−9 cm−2 s−1.
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