Table 5
Source fluxes, line ratios, luminosities, and gas masses of the sources using the redshifts listed in Table 4.
| Object | Line | FWZ I im | S rms | S peak value | Stot (r ≤ 10′′)1 |
|
|
|
M mol 4 |
| [km s-1] | [Jy beam-1 km s-1] | [Jy km s-1] | [108 K km s-1 pc2] | [109M⊙] | |||||
|
|
|||||||||
| HE 0433-1028 | 12CO(2–1) | 195 | 0.9 | 33.2 | 56.6 ± 3.3 | 8.19 | 0.632 | 1.0–6.2 | |
| 13CO(2–1) | 150 | 0.8 | 3.8 | 3.2 ± 1.2 | – | 5–20 | |||
| HE 1029-1831 | 12CO(3–2) | 205 | 1.9 | 81.4 | 110.3 ± 6.1 | 9.17 | 1.003 | 0.7–4.5 | |
| HCO+(4–3) | ~150 | 1.8 | – | ≤5.3 | ≥16 | ||||
| HE 1108-2813 | 12CO(2–1) | 260 | 0.8 | 78.3 | 104.5 ± 3.1 | 6.84 | 0.652 | 0.9–5.5 | |
| 13CO(2–1) | 150 | 0.5 | 3.5 | 3.0 ± 0.7 | 5–30 | ||||
Notes.
Flux errors do not include the flux calibration error of 20–30% and are based on image noise to demonstrate the data quality only;
based on single dish fluxes in Bertram et al. (2007) and corrected for source size and our cosmology;
based on line ratio map of PdBI data (Krips et al. 2007) and our data in Fig. 6;
total molecular mass in this observation (including Helium via a factor of 1.36), covering a mass range corresponding to αCO = 0.8–4.8 M⊙ (K km s-1 pc2)-1 for ULIRG and Galactic mass conversion (Downes & Solomon 1998; Solomon & Barrett 1991).
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