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Table 4.
Number of expected high-redshift detections in the deep and wide tier of the ATHENA–WFI survey simulation, and logarithm of the 0.5–2 keV luminosity limit (computed using the flux limit at 20% of the survey area).
Gilli et al. (2007) mock |
Vito et al. (2014) mock |
|||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
ATHENA survey | z > 3 |
z > 4 |
z > 5 |
z > 6 |
z > 7 |
z > 3 | z > 4 | z > 5 | z > 6 | z > 7 | ||||||
nsrc | Llim | nsrc | Llim | nsrc | Llim | nsrc | Llim | nsrc | Llim | nsrc | nsrc | nsrc | nsrc | nsrc | ||
Deep | 1744 | 42.1 | 326 | 42.4 | 68 | 42.6 | 15 | 42.8 | 6 | 42.9 | 2667 | 534 | 147 | 38 | 15 | |
Wide | 7344 | 42.5 | 1350 | 42.8 | 259 | 43.0 | 54 | 43.2 | 22 | 43.3 | 8878 | 1831 | 416 | 85 | 23 |
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