Table 1.
Contributions of each program used in this work to the final total sample.
| DATABASE | PROG ID | FIELD | GAL | SEL |
|---|---|---|---|---|
| CEERS | ERS 1345 | EGS | 109 | 77 |
| JADES | GTO 1180 | GOODS – North | 249 | 191 |
| GTO 1181 | ||||
| GTO 1210 | ||||
| GTO 1286 | ||||
| GTO 1287 | ||||
| GOODS – South | 373 | 222 | ||
| DJA | GO 1747 | BoRG-JWST | 14 | 12 |
| GO 1727 | COSMOS | 60 | 45 | |
| GO 2565 | COSMOS, EGS, UDS | 29 | 22 | |
| GTO 1211 | GOODS – North | 145 | 66 | |
| GTO 1181 | ||||
| GO 2198 | GOODS – South | 117 | 91 | |
| GO 3215 | ||||
| GTO 1210 | ||||
| GTO 1180 | ||||
| DD 6541 | ||||
| TOTAL | 1096 | 726 | ||
Notes. Programs used in our work and their contribution to the final sample. The column GAL includes all the sources in the spectroscopic databases residing in nonmagnified fields after the removal of the 26 identified AGN. The SEL column reports the number of sources remaining after implementing the additional criterion of S/N > 3 and discarding galaxies with spectral issues identified through visual inspection.
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