Table 3.
Number of detectable halos in the CTA survey, NHALOs, depending on how their typical size is defined (lepton energy 
at which the extent of pair halo overdensity on top of interstellar background is evaluated, reference gamma-ray energy 
at which the flux profile is taken, and containment fraction fc of the latter).
| fc |  (TeV) |
 (TeV) |
NHALOs |
|---|---|---|---|
| 0.68 | 1 | 1 | 70 |
| 0.95 | 1 | 1 | 56 |
| 0.68 | 10 | 1 | 69 |
| 0.95 | 10 | 1 | 58 |
| 0.68 | 10 | 3 | 74 |
| 0.95 | 10 | 3 | 63 |
| 0.68 | 10 | 10 | 82 |
| 0.95 | 10 | 10 | 70 |
| 0.68 | 100 | 10 | 83 |
| 0.95 | 100 | 10 | 71 |
Notes. The numbers correspond to a population of halos with suppressed diffusion region of size 50 pc and diffusion suppression by a factor 500.
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