Table 4.
SED model fitting results.
| zbin | T | NBB | NAGN | αAGN | Nradio | α | LIR | LSF | LAGN |
|---|---|---|---|---|---|---|---|---|---|
| RDQs | [K ] | [mJy] | [mJy] | [mJy] | |||||
| 0.0 ≤ z ≤ 1.0 | 21.57 ± 1.90 | 4.97 ± 0.62 | 1.47 ± 0.48 | 2.17 ± 0.21 | 1.47 ± 0.48 | 0.58 ± 0.15 |  |
 |
 |
| 1.0 < z ≤ 1.8 | 32.04 ± 2.90 | 2.57 ± 0.56 | 0.37 ± 0.16 | 1.64 ± 0.27 | 0.37 ± 0.16 | 0.64 ± 0.17 |  |
 |
 |
| 1.8 < z ≤ 2.7 | 26.69 ± 1.72 | 1.92 ± 0.19 | 0.21 ± 0.06 | 1.40 ± 0.19 | 0.21 ± 0.06 | 0.74 ± 0.12 |  |
 |
 |
| 2.7 < z ≤ 6.15 | 47.77 ± 6.73 | 1.85 ± 0.44 | 0.14 ± 0.02 | 1.16 ± 0.06 | 0.14 ± 0.02 | 0.65 ± 0.19 |  |
 |
 |
| RUQs | |||||||||
| 0.0 ≤ z ≤ 1.0 | 22.07 ± 1.15 | 16.95 ± 2.14 | 5.02 ± 0.56 | 2.29 ± 0.07 | 5.02 ± 0.56 | 0.47 ± 0.15 |  |
 |
 |
| 1.0 < z ≤ 1.8 | 23.14 ± 1.58 | 11.39 ± 1.88 | 2.22 ± 0.55 | 2.17 ± 0.16 | 2.22 ± 0.55 | 0.63 ± 0.06 |  |
 |
 |
| 1.8 < z ≤ 2.7 | 28.36 ± 4.03 | 6.12 ± 1.49 | 0.89 ± 0.23 | 1.69 ± 0.16 | 0.89 ± 0.23 | 0.59 ± 0.06 |  |
 |
 |
| 2.7 < z ≤ 6.15 | 27.17 ± 3.78 | 2.53 ± 0.63 | 0.36 ± 0.02 | 1.46 ± 0.04 | 0.36 ± 0.02 | 0.63 ± 0.06 |  |
 |
 |
Notes.
The best-fit models are showed in Figs. 8 and 9. See Sect. 4.3 for more details about the models used. LIR is the total infrared luminosity over the rest-frame wavelengths 8.0 μm and λc = 1000 μm. LSF and LAGN are the integrated SF and AGN luminosities, respectively. All the luminosities are in units of log(L⊙).
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