Table 5
Summary of TBS results and published H.E.S.S. spectra.
| Object | Method | E min | E max | Φ0(1 TeV) | Γ | E cut | χ2/d.o.f. | |
| TeV | TeV | TeV-1 m-2 s-1 | TeV | |||||
|
|
||||||||
| Crab nebula | TBS | 0.63 | 20.0 | (3.82 ± 0.11) × 10-7 | 2.40 ± 0.06 |
|
7.24/12 | |
| Reflected regions(1) | 0.45 | 65 | (3.84 ± 0.09) × 10-7 | 2.41 ± 0.04 | 15.1 ± 2.8 | 12.6/9 | ||
|
|
||||||||
| Centaurus A | TBS | 0.32 | 10.0 | (2.10 ± 0.51) × 10-9 | 2.74 ± 0.37 | – | 11.81/12 | |
| Reflected regions(2) | 0.25 | ~6 | (2.45 ± 0.52) × 10-9 | 2.73 ± 0.45 | – | 2.76/4 | ||
|
|
||||||||
| HESS J1745–290 | TBS | 0.2 | 15.9 | (3.08 ± 0.15) × 10-8 | 2.10 ± 0.06 |
|
17.38/16 | |
| (Galactic centre) | Reflected regions(3) | 0.16 | 70 | (2.55 ± 0.06) × 10-8 | 2.10 ± 0.04 | 14.7 ± 3.4 | 23/26 | |
|
|
||||||||
| HESS J1507–622 | TBS | 0.5 | 6.3 | (1.91 ± 0.41) × 10-8 | 2.31 ± 0.30 | – | 6.69/9 | |
| Reflected regions(4) | ~0.5 | 40.0 | (1.8 ± 0.4) × 10-8 | 2.24 ± 0.16 | – | –/4 | ||
|
|
||||||||
| Vela X | TBS | 0.79 | 63.1 | (9.52 ± 1.59) × 10-8 | 1.32 ± 0.29 |
|
6.68/15 | |
| On/Off (5) | 0.75 | ~60 | (11.6 ± 0.6) × 10-8 | 1.36 ± 0.06 | 13.9 ± 1.6 | – | ||
|
|
||||||||
| Vela Junior | TBS | 0.3 | 20.0 | (2.23 ± 0.30) × 10-7 | 2.27 ± 0.13 | – | 11.23/16 | |
| On/Off (6) | 0.3 | 20.0 | (1.90 ± 0.08) × 10-7 | 2.24 ± 0.04 | – | – | ||
Notes. The TBS energy ranges were chosen to match the H.E.S.S. publication range. This was possible for Vela X and Vela Junior. For HESS J1507–622 and HESS J1745–290 the full energy range in TBS (though limited by statistics) were used. The standard choice of the first energy bin, as used for the spectra of Centaurus A and Crab nebula, is the bin with the peak in the differential rate (dN/ dE).
Reference. (1) Aharonian et al. (2006); (2) Aharonian et al. (2009b); (3) Aharonian et al. (2009a); (4) Acero et al. (2011); (5) Abramowski et al. (2012); (6) Aharonian et al. (2005).
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