Table B.1.
List of high-z quasar candidates selected in this work. Here, we only show the first ten rows of the catalog as an example, while the entire catalog can be accessed at the CDS (see text).
| Source | RA | Dec | F444W | zphot | log Lbol | log M* | log SFR | log MBH | fAGN | Grade |
|---|---|---|---|---|---|---|---|---|---|---|
| [J2000] | [J2000] | [nJy] | [erg s−1] | [M⊙] | [M⊙ yr−1] | [M⊙] | ||||
| CWB-663 | 149.75099 | 2.15091 | 351.86 ± 10.87 | 6.05 ± 0.12 | 43.66 ± 0.90 | 9.13 ± 0.31 | 0.83 ± 0.35 | > 5.55 | 0.05 ± 0.35 | B |
| CWB-8286 | 149.76383 | 2.19782 | 203.96 ± 3.92 | 7.81 ± 0.30 | 43.58 ± 1.54 | 9.35 ± 0.25 | 1.03 ± 0.22 | > 5.46 | 0.05 ± 0.32 | B |
| CWB-19858 | 149.84033 | 2.24807 | 395.54 ± 3.92 | 6.70 ± 0.13 | 43.66 ± 1.31 | 9.38 ± 0.16 | 1.08 ± 0.15 | > 5.54 | 0.05 ± 0.19 | B |
| CWB-24983 | 149.85942 | 2.27450 | 234.01 ± 3.98 | 6.14 ± 0.17 | 44.01 ± 0.67 | 9.12 ± 0.26 | 0.53 ± 0.91 | > 5.89 | 0.20 ± 0.27 | A |
| CWB-26445 | 149.80063 | 2.30474 | 183.36 ± 3.92 | 6.93 ± 0.27 | 44.81 ± 0.82 | 9.19 ± 0.44 | 0.87 ± 0.45 | > 6.70 | 0.95 ± 0.33 | A |
| CWB-35877 | 149.95743 | 2.11303 | 129.15 ± 3.92 | 6.88 ± 0.22 | 44.76 ± 0.49 | 8.72 ± 0.46 | 0.44 ± 0.47 | > 6.65 | 0.95 ± 0.28 | A |
| CWB-40773 | 149.92404 | 2.15948 | 253.99 ± 6.37 | 7.30 ± 0.20 | 44.93 ± 0.32 | 8.88 ± 0.39 | 0.62 ± 0.42 | > 6.82 | 0.80 ± 0.29 | A |
| CWB-41512 | 149.93536 | 2.16019 | 836.82 ± 5.79 | 6.02 ± 0.12 | 45.22 ± 0.29 | 9.75 ± 0.15 | 1.46 ± 0.16 | > 7.11 | 0.20 ± 0.23 | A |
| CWB-42214 | 149.93324 | 2.16687 | 1760.68 ± 5.20 | 6.09 ± 0.12 | 44.88 ± 0.79 | 10.21 ± 0.38 | 1.67 ± 0.34 | > 6.77 | 0.50 ± 0.17 | A |
| CWB-43536 | 150.02278 | 2.14372 | 545.53 ± 11.98 | 8.10 ± 0.19 | 45.29 ± 0.59 | 9.83 ± 0.25 | 1.52 ± 0.25 | > 7.17 | 0.20 ± 0.27 | A |
Notes. Column (1): name of each candidate with specific prefixes indicating the originating dataset, that is, CWB (COSMOS-Web), JDS/GDS (JADES/GOODS-S), GDN (GOODS-N), UCV (UNCOVER), CRS (CEERS), PMC (PRIMER-COSMOS), and PMU (PRIMER-UDS). Column (2)–(3): right ascension (RA) and declination (Dec) in decimal degrees. Column (4): fluxes measured using the JWST/NIRCam images. Column (5): calculated photometric redshift of the target derived from the best-fitted SED template. Column (6): bolometric luminosity of the AGN SED component. Column (7): total stellar mass of the presumed host galaxy. Column (8): SFR averaged over 100 Myr. Column (9): lower limit of the black hole mass, assuming an accretion at the Eddington limit. Column (10): fraction of AGN component to the total spectral emission within the rest-frame wavelengths of 0.1–0.7 μm. Column (11): grade after employing the visual inspection, black hole mass limit, and AGN fraction threshold criteria.
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