Table 1
Optimal positions and energy thresholds of the source signal regions for the search of neutrino emission from extended regions.
| Ψ | RA | Dec | l | b | E thr | A 100 | Γ |
|
|
|||||||
| 2° | 306.6° | 40.7° | 79.0° | 1.5° | 4.0 × 104 | 1.05 × 10-12 | 2.40 |
| 4° | 308.3° | 41.7° | 80.5° | 1.0° | 3.2 × 104 | 1.65 × 10-12 | 2.42 |
Notes. Column 1 shows the radius of the source region circle; positions in equatorial and galactic coordinates are given in Cols. 2–4. Column 6 shows the optimal energy threshold (in GeV), while the two last columns show the expected muonic neutrino signal deduced from the observed γ-ray signal (represented in Fig. 4): normalization at 100 GeV in units 1/GeV cm2 s and spectral index, respectively (see Eq. (1)).
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