Table 4
CARLA J1103 + 3449 cluster confirmed member 
, attenuation, metallicity, SFR, sSFR, depletion time, and SFE.
| id |  |
AHα | 12 + log(O/H) | SFRHα | sSFR | τdep | SFE |
|---|---|---|---|---|---|---|---|
| (M⊙ yr−1) | (M⊙ yr−1) | (Gyr−1) | (Gyr) | (Gyr−1) | |||
| AGN/491 100% | <140 | 1.4 | 8.6 | 140 ± 50 | 3 ± 2 | <0.2 | >5 |
| AGN/491 80% | ... | 1.4 | 8.6 | 110 ± 40 | 2 ± 1 | <0.3 | >4 |
| AGN/491 60% | ... | 1.4 | 8.6 | 80 ± 30 | 2 ± 1 | <0.4 | >3 |
| AGN/491 40% | ... | 1.5 | 8.6 | 50 ± 20 | 1.1 ± 0.7 | <0.6 | >2 |
| AGN/491 20% | ... | 1.5 | 8.7 | 30 ± 8 | 0.5 ± 0.3 | <1 | >0.8 |
| 490(+) | 25 ± 5 | ... | ... | ... | ... | <1 | > 0.8 |
| 320 | 10 ± 5 | 0.8 | 8.6 | 6 ± 3 | 1 ± 1 | <7 | >0.1 |
| 283(+) | 16 ± 7 | ... | ... | ... | ... | <3 | >0.3 |
| 279(+) | 11 ± 6 | ... | .... | ... | ... | <5 | >0.2 |
| 199 | 11 ± 4 | 1.4 | 8.7 | 9 ± 4 | 0.2 ± 0.1 | <8 | >0.1 |
| 183 | 13 ± 5 | 0.5 | 8.4 | 6 ± 4 | 2 ± 3 | <12 | >0.1 |
| 93 | 10 ± 2 | ... | ... | ... | ... | ... | ... |
Notes. The identification numbers in the column “id” are the same as in the catalog published by Noirot et al. (2018). The column
shows the SFR calculated in Noirot et al. (2018). The other columns show our measurements of attenuation, metallicity, SFR, sSFR, depletion time, and SFE for the confirmed members of the CARLA J1103 + 3449 cluster. In the case of the AGN (id 491), since we cannot separate the AGN and stellar contributions, we vary the stellar contribution to the total Hα+[NII] emission flux in the range 20−100%. The plus symbol (+) shows the cluster members for which we use the values of SFR reported in Noirot et al. (2018) to estimate depletion time and SFE.
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