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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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