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Table 5.
[C II] luminosities, emission line equivalent widths, [C II] -based star formation rates, and the dynamical and [C II] -based molecular gas masses values for the RL quasars in our sample.
| Name | L[CII] | EW[CII] | SFR[CII] | Mdyn | MH2, [C II] |
|---|---|---|---|---|---|
| [108 L⊙] | [km s−1] | [M⊙ yr−1] | [1010 M⊙] | [109 M⊙] | |
| J0131-0321 | 3.8 ± 0.8 | 225 ± 45 | 40 ± 9 | 4.8 ± 4.0 | 11 ± 2.0 |
| PSO055-00 (⋆) | 3.1 ± 0.3 | 578 ± 78 | 32 ± 3 | 2.8 ± 2.2 | 9.3 ± 0.8 |
| PSO135+16 | 27.7 ± 1.0 | 683 ± 35 | 416 ± 18 | 15.0 ± 1.8 | 83 ± 3.0 |
| J1034+2033 | 3.1 ± 0.3 | 2476 ± 505 | 32 ± 4 | 5.8 ± 4.9 | 9.3 ± 0.9 |
| PSO352–15 | 7.9 ± 1.1 | 2790 ± 472 | 95 ± 15 | 23.3 ± 10.7 | 24 ± 3.0 |
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