Table 2.
Number of detectable sources in past or forthcoming surveys, obtained for one single realization of the population model.
| Survey | SNRs | PWNe | Halos (30 pc) | Halos (50 pc) | Halos (80 pc) | Total |
|---|---|---|---|---|---|---|
| Total in population | 266 | 945 | 2613 | 2613 | 2613 | 3824 |
| HESS (HGPS) | 8 | 54 | 17 | 23 | 23 | 79, 85, or 85 |
| HAWC (3HWC) | 2 | 19 | 10 | 15 | 16 | 31, 36, or 37 |
| CTA (GPS) | 30 | 171 | 43 | 74 | 103 | 244, 275, or 304 |
| CTA (GPS+) | 44 | 261 | 103 | 166 | 217 | 408, 471, or 522 |
Notes. The prospects for halos are given for three alternative modeling, with different radii for the suppressed diffusion regions of 30, 50, or 80 pc, and diffusion suppression by factor 500 (see Table 1). Prospects for CTA are also given for a variant of the survey, GPS+, with sensitivity improvement by a factor of 2 with respect to the values published in Cherenkov Telescope Array Consortium (2019).
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