Table 1
Redshifts, masses, luminosities, and CO parameters.
| Parameter | SW022550 | SW022513 |
|
|
||
| z UV | 3.867 ± 0.009 | ... |
| z opt | 3.876 ± 0.001 | 3.427 ± 0.002 |
| F1.2 mm [mJy] | 4.70 ± 0.77 | 5.53 ± 0.72 |
| Mstellara [1010 M⊙] | 16–80 | 20–40 |
| Log(L(IR)a) [L⊙] | 12.5–13.3 | 12.5–13.2 |
| SFRa [ M⊙/yr] | 500–3000 | 500–3000 |
| z CO | 3.8719 ± 0.0008 | 3.4220 ± 0.0007 |
| z CO,1 | 3.8686 ± 0.0007 | 3.4208 ± 0.0013 |
| z CO,2 | 3.8761 ± 0.0012 | 3.4270 ± 0.0007 |
| νb [GHz] | 94.6330 | 104.2598 |
| ν1b [GHz] | 94.6978 | 104.2885 |
| ν2b [GHz] | 94.5504 | 104.1432 |
| FWHMb [km s-1] | 800 ± 120 | 1020 ± 110 |
| FWHM1b [km s-1] | 290 ± 90 | 950 ± 150 |
| FWHM2b [km s-1] | 420 ± 180 | 200 ± 150 |
| Δvc [km s-1] | 460 ± 90 | 420 ± 100 |
| ICO [Jy km s-1] | 1.46 ± 0.28 | 2.62 ± 0.36 |
| ICO,1 [Jy km s-1]d | 0.68 ± 0.11 | 2.25 ± 0.28 |
| ICO,2 [Jy km s-1]d | 0.70 ± 0.23 | 0.28 ± 0.21 |
| LCOe [108 L⊙] | 1.77 ± 0.32 | 2.61 ± 0.36 |
f [1010 K km s-1 pc2] |
5.7 ± 1.0 | 8.3 ± 1.2 |
| Mgasg [1010 M⊙] | 4.53 ± 0.82 | 6.66 ± 0.92 |
| Mgas/Mstellar | 0.06–0.29 | 0.17–0.33 |
[1010 M⊙] |
40 ± 20 | 2–34 |
[1010 M⊙] |
20 ± 10 | 9–35 |
| SFEh [L⊙/(K km s-1 pc2)] | 35–194 | 24–108 |
Notes. All CO parameters refer to the J=(4–3) transition;
L(IR) is the 8–1000μm luminosity in L⊙, Mstellar the stellar mass, and SFR the star-formation rate (see Sect. 2 and Polletta et al. 2008a);
ν is the observed frequency of the CO line fitted with a single Gaussian. ν1 and ν2 are the observed frequencies of the two CO peaks obtained with a double Gaussian fit, and FWHM, FWHM1, and FWHM2 are the corresponding full-widths-at-half maximum;
SFE is the star-formation efficiency defined as L(FIR)/
(see Sect. 5.3).
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