Table 3
Values for the SFR and the stellar mass obtained from direct measurement on the observed spectra and photometry of each galaxy.
| ID | z spec | SFR |
|
sSFR(Hα) | A(Hα) | SF R corr |
| [ M⊙ yr-1 ] | [ M⊙ ] | [ yr-1 ] | mag. | [ M⊙ yr-1 ] | ||
|
|
||||||
| A1 | 1.6777 | 13.0 ± 1.0 | 1.7 × 1011 | 7.6 × 10-11 | 2.0 | 82 ± 6 |
| A2 | 1.6839 | 7.8 ± 1.0 | 1.8 × 1011 | 4.3 × 10-11 | 2.0 | 49 ± 6 |
| B2a | 1.6819 | 4.6 ± 1.0 | 0.5 × 1011 | 9.2 × 10-11 | 1.4 | 17 ± 4 |
|
|
||||||
| A4a | 2.0383 | 4.8 ± 2.2 | 3.0 × 1011 | 1.6 × 10-11 | 2.3 | 40 ± 18 |
| C1b | 2.0387 | 30.1 ± 1.9 | ||||
| D1 | 2.0186 | 7.2 ± 2.2 | 1.1 × 1011 | 6.5 × 10-11 | 1.8 | 38 ± 11 |
Notes. The specific star formation rate (sSFR) is defined as the ratio between these two quantities. The corrected SFR is deduced by applying the extinction factor A(Hα) line, with the relation measured in Kashino et al. (2013). C1a has been removed from the table because, if is identified with a extremely red QSO, then these values do not make sense. C1b is blended with C1a and Ks photometry is not reliable.
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