Table 6.
Population properties according to the probed models.
| Model | N | L [ph s−1] | F [ph cm−2 s−1] |
|---|---|---|---|
| Mean/Std | Median/QD | ||
| mSNR |  |
(1.73/0.16) × 1036 | (4.89/1.41) × 10−10 |
| mPWN |  |
(2.47/0.18) × 1036 | (7.74/1.86) × 10−10 |
| mFE |  |
(6.32/0.26) × 1036 | (1.54/0.16) × 10−9 |
| mSp4 |  |
(1.59/0.17) × 1036 | (3.38/0.70) × 10−10 |
| mSp2B |  |
(1.44/0.14) × 1036 | (1.96/0.20) × 10−10 |
Notes. The distribution of the total number of Galactic VHE γ-ray sources N and their combined luminosity L and flux F. The luminosities are characterised by the mean and standard deviation as this quantity is almost symmetrically distributed over the different realisations. In contrast, the median and quartile deviation are used as a more robust description of the total flux F, whose distribution is strongly affected by outliers that stem from (rare) nearby sources.
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