Table 4.
Spatially integrated dust and line emission properties in the source plane.
| Line | Component | Spk | SR/SB | Iline | IR/IB | IG/Itotal | ΔVline | LLine/107 |  |
|---|---|---|---|---|---|---|---|---|---|
| (mJy) | (Jy km s−1) | (km s−1) | (L⊙) | (K km s−1 pc2) | |||||
| CO(6–5) | B | 1.3 ± 0.6 | 1.5 ± 0.7 | 0.3 ± 0.1 | 1.5 ± 0.5 | 0.2 ± 0.1 | 243 ± 65 | 5.7 ± 1.8 | 5.3 ± 1.7 |
| G | 0.9 ± 0.8 | 0.2 ± 0.1 | 197 ± 90 | 3.2 ± 2.3 | 3.0 ± 2.2 | ||||
| R(Rb+Rr) | 2.0 ± 0.4 | 0.5 ± 0.1 | 243 ± 28 | 8.5 ± 1.3 | 8.0 ± 1.3 | ||||
| H2O(211−202) | B | 0.4 ± 0.3 | 1.7 ± 1.2 | 0.1 ± 0.1 | 2.1 ± 1.2 | 0.2 ± 0.1 | 212 ± 67 | 1.8 ± 0.9 | 1.3 ± 0.7 |
| G | 0.4 ± 0.2 | 0.1 ± 0.1 | 197 (a) | 1.4 ± 0.7 | 1.1 ± 0.5 | ||||
| R(Rb+Rr) | 0.8 ± 0.3 | 0.2 ± 0.1 | 261 ± 40 | 3.8 ± 1.1 | 2.8 ± 0.8 | ||||
| LIR | B | log(LIR/L⊙) = 12.6 ± 0.3 | Td = 33−61 K | ||||||
| G | log(LIR/L⊙) = 11.6 ± 0.3 |
 K |
|||||||
| R(Rb+Rr) | log(LIR/L⊙) = 12.8 ± 0.3 | Td = 33−61 K | |||||||
Notes. The fitting errors are dominated by the uncertainties in lens modeling. The uncertainties of dust far-IR SED fitting is significant due to the limited constraints and the complexities of lens modeling. Therefore, we increase the uncertainties by 50% for the total IR luminosity and dust temperature. For separating the LIR for different component, we assume a similar ratio for LIR as found in LCO(6−5) for R and B, and the dust temperatures were derived based on a global dust SED fitting. (a)The linewidth has been fixed for G using those determined from fitting the CO line over the same emission region.
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