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Table A.2.
CO line luminositiesa computed for the ULIRGs in our sample.
| Source | CO(1−0) | CO(2−1) | CO(3−2) | CO(4−3) | CO(5−4) | CO(6−5) | CO(7−6) |
|---|---|---|---|---|---|---|---|
| IRAS F01572+0009 | 9.9 ± 1.5 | 11.8 ± 0.8 | 8.6 ± 0.7 | 5.2 ± 1.0 | 3.4 ± 0.8 | ||
| IRAS 03521+0028 | 14.5 ± 0.5 | 10.5 ± 0.8 | 7.9 ± 1.0 | ||||
| IRAS F05189-2524 | 3.9 ± 0.1 | 3.1 ± 0.1 | 2.0 ± 0.2 | 2.2 ± 0.3 | 0.7 ± 0.0 | ||
| IRAS 06035-7102 | 13.6 ± 0.6 | 13.2 ± 0.5 | 11.4 ± 0.6 | 4.0 ± 0.3 | |||
| IRAS 06206-6315 | 9.4 ± 0.6 | 6.2 ± 0.4 | 6.8 ± 0.7 | 3.3 ± 0.4 | |||
| IRAS 08311-2459 | 18.6 ± 0.7 | 14.5 ± 1.0 | 11.4 ± 0.8 | 6.3 ± 0.7 | |||
| IRAS 09022-3615 | 13.0 ± 0.4 | 9.1 ± 0.6 | 11.1 ± 0.8 | 3.4 ± 0.2 | |||
| IRAS 10378+1109 | 11.2 ± 0.9 | 8.9 ± 0.7 | 7.5 ± 1.3 | 9.4 ± 1.0 | |||
| IRAS F12112+0305 | 9.1 ± 0.3 | 12.7 ± 0.6 | 8.0 ± 0.4 | 5.8 ± 0.4 | 1.7 ± 0.2 | ||
| IRAS F13451+1232 | 9.5 ± 0.5 | 8.3 ± 1.0 | 5.4 ± 0.5 | 2.1 ± 0.5 | |||
| IRAS 16090-0139 | 16.0 ± 1.1 | 23.2 ± 0.9 | 18.0 ± 1.3 | 15.2 ± 1.5 | 14.7 ± 0.8 | ||
| IRAS 17208-0014 | 13.5 ± 0.2 | 13.3 ± 0.3 | 10.4 ± 0.4 | 4.8 ± 0.5 | 1.9 ± 0.1 | ||
| IRAS 19254-7245 | 8.3 ± 0.3 | 6.2 ± 0.7 | 0.9 ± 0.2 | ||||
| IRAS F20551-4250 | 6.2 ± 0.1 | 6.6 ± 0.2 | 4.2 ± 0.2 | 3.0 ± 0.3 | 0.7 ± 0.1 | ||
| IRAS F22491-1808 | 5.9 ± 0.4 | 4.4 ± 0.2 | 2.8 ± 0.3 | 1.6 ± 0.2 | |||
| IRAS F23060+0505 | 17.0 ± 0.6 | 21.6 ± 1.2 | 12.9 ± 0.7 | 12.4 ± 1.5 | 8.3 ± 1.5 | 4.0 ± 0.5 | |
| IRAS F23128-5919 | 5.0 ± 0.1 | 4.8 ± 0.1 | 3.6 ± 0.1 | 2.3 ± 0.3 | 0.6 ± 0.1 |
Notes. a Line luminosities (brightness temperatures) in units of 
K km s−1 pc2.
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