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Table 3.
Best-fitting physical parameters of C1 and C6 obtained via SED fitting.
| C1 | C6 | |
|---|---|---|
| SFR100 Myr [M⊙ yr−1] | 228 ± 141 | 263 ± 77 |
| SFR10 Myr [M⊙ yr−1] | 1447 ± 677 | 1105 ± 198 |
| SFR0 Myr [M⊙ yr−1] | 2127 ± 1292 | 1232 ± 242 |
| M* [1010 M⊙] | 3.5 ± 2.8 | 3.5 ± 1.4 |
| Lbol, AGN [erg s−1] | (1.9 ± 0.7)×1047 | (3.3 ± 0.2)×1045 |
| Radio loudness | – | 98 ± 9 |
Notes. These rows report the best-fitting SFRs averaged over 100 Myr and 10 Myr, the instantaneous SFRs, the stellar masses, and the AGN bolometric luminosities.
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