Table 1.
continued.
| Objid | log[SFRLTIR (M⊙ yr−1)] | log[SFRCIGALE (M⊙ yr−1)] | log[SFRCIGALE(10 Myrs) (M⊙ yr−1)] | log[SFRCIGALE(100 Myrs) (M⊙ yr−1)] |
|---|---|---|---|---|
| (1) | (18) | (19) | (20) | (21) |
| 96 702 | 1.10 ± 0.12 | 0.87 ± 0.14 | 0.87 ± 0.14 | 0.83 ± 0.12 |
| 99 389 | 1.82 ± 0.05 | 1.59 ± 0.07 | 1.59 ± 0.07 | 1.58 ± 0.07 |
| 132 869 | 1.02 ± 0.03 | 0.74 ± 0.05 | 0.74 ± 0.05 | 0.73 ± 0.05 |
| 94 458 | 1.91 ± 0.02 | 1.61 ± 0.04 | 1.61 ± 0.04 | 1.59 ± 0.06 |
| 123 801 | 1.30 ± 0.06 | 0.95 ± 0.13 | 0.96 ± 0.13 | 0.94 ± 0.13 |
Notes. Column (1) is the unique identification number for each object in the Lockman-SpReSO catalogue. Column (2) is the spectroscopic redshift of the object. Column (3) is the stellar mass obtained from the SED fittings using CIGALE. Column (4) is the IR luminosity obtained from the SED fittings using CIGALE. Columns (5)–(8) are the colour excess calculated in this work (see Sect. 4). Columns (9)–(13) are the metallicities derived in this work following different calibrations (see Sect. 5). Columns (14)–(21) are the SFR derived in this work following different calibrations (see Sect. 6).
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