Table F.1.
Results from Gaussian fits of CO(3-2) emission lines.
| Quasar | zCO | FWHM | FCO(3 − 2) | M(H2) |
|---|---|---|---|---|
| (km s−1) | (Jy km s−1) | (1010 M⊙) | ||
| J0015+1842 | 2.6285 | 1010 ± 120 | 1.1 ± 0.2 | 3.4 - 17 |
| J0059+1124 | 3.0378 | 500 ± 110 | 0.24 ± 0.07 | 0.9 - 4.6 |
| J0125–0129 | 2.6618 | 460 ± 80 | 0.5 ± 0.1 | 1.5 - 7.4 |
| J1259+0309 | 3.2405 | 450 ± 180 | 0.2 ± 0.1 | 0.8 - 3.9 |
| J1331+0206 | 2.9168 | 350 ± 100 | 0.22 ± 0.08 | 0.8 - 4.0 |
| J2228-0221. | 2.7780 | 330 ± 60 | 0.27 ± 0.07 | 0.9 - 4.5 |
Notes. Molecular masses are calculated from the CO(3-2) luminosities assuming r31 = 0.97 (Carilli & Walter 2013). The range corresponds to assumed CO-to-H2 conversion factors either typical for quasars αCO = 0.8 M⊙(km s−1 pc2)−1 (see e.g. Bolatto et al. 2013) or using the standard value αCO = 4 M⊙(km s−1 pc2)−1.
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