Table A.3
Calculated HE luminosities and number of events above 100 GeV detected by Fermi-LAT from five HBLs.
| Source | z a | Indexb | L 60 GeV c | N d | N s e |
| [1043 erg s-1] | |||||
|
|
|||||
| Mrk 421 | 0.030 | 1.77 ± 0.01 | 19.2 ± 1.1 | 35 | 18 |
| Mrk 501 | 0.034 | 1.74 ± 0.03 | 6.95 ± 0.75 | 16 | 10 |
| 1ES 2344+514 | 0.044 | 1.72 ± 0.08 | 2.30 ± 0.56 | 9 | 9 |
| Mrk 180 | 0.046 | 1.74 ± 0.08 | 2.01 ± 0.51 | 1 | 1 |
| 1ES 1959+650 | 0.048 | 1.94 ± 0.03 | 6.00 ± 0.80 | 3 | 4 |
Notes.
Simple power law spectral index measured by Fermi-LAT (Nolan et al. 2012). Note that for all sources the simple power law is clearly preferred over a curved description of the spectrum.
Luminosity at 60 GeV, determined on the basis of the 10−100 GeV photon counts reported in Nolan et al. (2012).
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