Table 3.
Observations needed for best chances of detectability of the sources according to the modelled broadband SED.
| CTAO detectability | |||
|---|---|---|---|
| Source | log parabola model | Broken power-law model | Array visibility |
| 5BZBJ0333−3619 | No | No | CTAO-S |
| 5BZBJ1253+3826 | ≥100 h | No | CTAO-N |
| 5BZBJ1636−1248 | 50h | ≥100 h | CTAO-N |
| 5BZBJ1251−2958 | 50 h | ≥100 h | Both |
| 5BZBJ0040−2719 | 50 h | No | both |
| 5BZBJ1302+5056 | No | No | CTAO-N |
| 5BZBJ1057+2303 | 50 h | ≥100 h | Both |
| 5BZBJ2217−3106 | No | No | CTAO-S |
| 5BZBJ0124+0918 | No | No | Both |
| 5BZBJ1258+0134 | ≥100 h | No | Both |
Notes. The detectability was assessed visually by comparing the fluxes reached by the model with the CTAO-N or CTAO-S sensitivity. We assumed that a target is visible by an array if during the year it reaches an altitude higher than 30° above the horizon at its site declination.
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