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Table 1.
Overview of the employed selection that we used to detect the high-z quasars.
| Step | Selection | COSMOS-Web | JADES/ | GOODS-N | UNCOVER | CEERS | PRIMER- | PRIMER- |
|---|---|---|---|---|---|---|---|---|
| GOODS-S | COSMOS | UDS | ||||||
| 1 | All sources | 342 435 | 70 899 | 37 890 | 61 648 | 76 300 | 118 794 | 143 552 |
| 2 | SED modeling | 247 | 383 | 61 | 105 | 237 | 172 | 185 |
| 3 | Visual inspection | 30 | 58 | 16 | 32 | 54 | 69 | 91 |
| 4 | MBH > 105 M⊙ | 18 | 11 | 6 | 3 | 6 | 13 | 7 |
| and fAGN ≥ 0.2 | ||||||||
| • | Sky coverage (arcmin2) | 1008 | 57 | 55 | 49 | 91 | 164 | 212 |
| • | Faintest magnitude | 26.1 | 29.4 | 27.4 | 28.1 | 27.7 | 28.0 | 27.8 |
Notes. At the end of our search, we found 350 compact sources, including 64 showing attributes consistent with low-luminosity AGNs. We also report the sky area covered by each dataset and the faintest F444W magnitude of the candidates.
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