Table 2
List of the sources located in the southern hemisphere potentially detectable with a detector similar to the IceCube detector located in the north pole (see Fig. 11).
| Gal. longitude (l) | Name | E thr | A 100 | Γ |
| 19° | HESS J1825-137 | 2.5 × 104 | 3.0 × 10-12 | 2.30 |
| 267° | Vela Jr. | 3.2 × 104 | 1.1 × 10-12 | 2.12 |
| 337–338° | HESS cluster | 2.0 × 104 | ~3.2 × 10-12 | 2.33 |
Notes. The three last columns show the expected neutrino flux (see Eq. (1)) and the optimal energy threshold for a considered region of 2 degrees around the Galactic longitude listed in the Col. 1. Units for Ethr and A100 are the same as in Table 1. The so-called HESS cluster is a generic term for the sources detected by H.E.S.S. in the region around l = 337 − 338°.
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