Table 5
50th, 15.9th, and 84.1th percentiles of the count predictions of 5.7 < z < 6.4 and log (L2−10 keV∕(erg s−1)) > 45.5 AGNs that will be detected with eROSITA in eRASS:8 (restricted to the extragalactic sky, 34 100 deg2).
| Mod. |  |
 |
 |
|---|---|---|---|
| G15 | 99 | 38 | 245 |
| U14 | 73 | 38 | 136 |
| M15 | 92 | 41 | 204 |
| sAREA | 244 | 42 | 439 |
Notes. The counts are obtained by sampling from the XLF models of G15, U14, and M15. The distributions are weighted bythe probability of the sampled XLFs of supporting at least one detection in eFEDS. The results for sAREA are obtained from naive area-scaling.The edges of the 1σ confidence interval are estimated from the percentile method.
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