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Table 1.
Properties of three reference AXIS surveys simulated in this work.
| Survey | Area | Tile exposure | Total exposure | Flux limit (0.5–2 keV) | Number of detections |
|
|---|---|---|---|---|---|---|
| deg2 | ks | Ms | erg s−1 cm−2 | AGN | Galaxies | |
| Deep | 0.16 | 5000 | 5 | 5 × 10−19 | 3496 | 5387 |
| Intermediate | 2.5 | 300 | 5 | 3 × 10−18 | 32655 | 22071 |
| Wide | 50 | 15 | 5 | 4 × 10−17 | 190149 | 21840 |
Notes. The flux limit corresponds to 1% of the covered field (see Fig. 9), and is the flux at which 1% of the input sources is detected. The number of detections is computed in the 0.5–7 keV band.
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