Table 5.
Results of [C II] emission line analysis.
| QSO | z[C II] | [C II] size | FWHM[CII] | Flux Density | S[C II] Δ v | L[C II] | Mmol | Mdynsin2i | Mdyn |
|---|---|---|---|---|---|---|---|---|---|
| [arcsec2] | [km s−1] | [mJy] | [Jy km s−1] | [109 L⊙] | [109 M⊙] | [109 M⊙] | [109 M⊙] | ||
| J0131-0321 | 5.193 ± 0.017 | 1.22 × 0.59 | 270 ± 51 | 0.89 ± 0.23 | 0.40 ± 0.11 | 0.32 ± 0.09 | 1.8 ± 0.4 | 41 ± 30 | 56 ± 45 |
| J0306+1853 | 5.3702 ± 0.0001 | 0.61 × 0.45 | 551 ± 22 | 9.10 ± 0.38 | 15.6 ± 1.5 | 13.0 ± 1.2 | 29 ± 2 | 111 ± 17 | 238 ± 38 |
| J2207-0416 | 5.5310 ± 0.0004 | 1.24 × 0.53 | 404 ± 31 | 3.7 ± 0.4 | 2.7 ± 0.3 | 2.4 ± 0.2 | 8.1 ± 0.6 | 123 ± 27 | 155 ± 31 |
| J1335-0328 | 5.699 ± 0.001 | 0.78 × 0.31 | 646 ± 60 | 0.48 ± 0.12 | 1.05 ± 0.12 | 0.96 ± 0.11 | 4.0 ± 0.4 | 184 ± 72 | 212 ± 87 |
Notes. Redshift is estimated from the line peak, [C II] size from 2D gaussian fit, [C II] FWHM from 1D gaussian fit, flux density integrated over the 2σ region, integrated flux density, [C II] luminosity, molecular and dynamical masses. Errors on masses account only for the statistic uncertainty. The systematic uncertainty on Mmol is of about 0.1 dex, and of 0.5 dex for Mdyn.
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