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Table 3.
Bona fide sample as selected by means of SED fitting with BC03 models: number and mass densities in different redshift bins.
| Δz | Number | z | log(M*/M⊙) | log(ρN) | log(ρ*) |
|---|---|---|---|---|---|
| bona fide | median | median | (Mpc−3) | (M⊙ Mpc−3) | |
| 3.0 ≤ z < 3.5 | 5 | 3.17 | 10.81 |
 |
 |
| 3.5 ≤ z < 4.0 | 4 | 3.72 | 10.70 |
 |
 |
Notes. Errors include Poissonian errors, cosmic variance, and photometric redshift errors. No objects in the bona fide sample are located at z ≥ 4.
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