Table 6.
Derived properties for sources.
| Name | L[CII] | LIR | SFRIR | SFR[CII] | L[CII]/LIR | Ṁout | Mdyn, [CII] |
|---|---|---|---|---|---|---|---|
| [109 L⊙] | [1012 L⊙] | [M⊙ yr−1] | [M⊙ yr−1] | 10−3 | [M⊙ yr−1] | [1010 M⊙] | |
| BRI0952 | 2.46 ± 0.23 | 7.66 ± 2.49 | 770 | 247 | 0.37 | 98 ± 19 | 0.90 |
| Comp-N | 0.39 ± 0.04 | < 0.2 | < 21 | 34 | < 2.0 | – | 0.5 |
| Comp-SW | 0.19 ± 0.03 | < 0.2 | < 21 | 16 | < 1.0 | – | 0.4 |
| AzTEC-3 | 9.3 ± 0.80 | 73.4 ± 2 | 7340 | 809 | 0.12 ± 0.01 | 238 ± 30 | 6.5 |
| LBG-3 | 0.63 ± 0.05 | 0.40 ± 0.5 | 40 ± 46 | 55 | 1.6 ± 0.14 | – | 0.95 |
| Gal-S | 0.43 ± 0.04 | < 0.1 | < 12.0 | 37 | < 3 | – | 0.83 |
| Gal-SW | 0.12 ± 0.01 | 0.15 ± 0.2 | 15 ± 23 | 11 | 0.85 ± 0.13 | – | 1.6 |
Notes. LIR refers to the integrated IR luminosity from 8−1000 μm for BRI0952 (using LIRSF) and AzTEC-3 and to a modified blackbody approximation for the companion sources. SFRIR is the SFR derived from the LIR, SFR[CII] refers to the SFR derived from the relation given in De Looze et al. (2014) for starburst galaxies. Ṁout gives the mass outflow rate, and Mdyn is the dynamical mass. Upper limits are provided for inferred properties for Gal-S, Comp-N, and Comp-SW as we do not detect these sources in continuum emission. The luminosities reported for BRI0952 are corrected for magnification.
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