Open Access
Table D.1.
Total CO fluxes and luminosities.
| Galaxy name | CO(1–0) | CO(2–1) | CO(3–2) | [CI](1–0) | ||||
|---|---|---|---|---|---|---|---|---|
| SCOdv |
 |
SCOdv |
 |
SCOdv |
 |
S[CI]dv |
 |
|
| [Jy km s−1] | [K km s−1 pc2] | [Jy km s−1] | [K km s−1 pc2] | [Jy km s−1] | [K km s−1 pc2] | [Jy km s−1] | [K km s−1 pc2] | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| IRAS 00188-0856 | 6.4 ± 0.5 | 5.4 ± 0.4 | 46.6 ± 4.4 | 9.8 ± 0.9 | 45.4 ± 1.2 | 4.2 ± 0.1 | ||
| IRAS 01003-2238 | 3.5 ± 0.5 | 2.5 ± 0.4 | 9.6 ± 2.5 | 1.7 ± 0.4 | 21.2 ± 3.8 | 1.7 ± 0.3 | ||
| IRAS F01572+0009 | 5.9 ± 0.8 | 8.1 ± 1.2 | 32.7 ± 2.2 | 11.2 ± 0.8 | 49.7 ± 3.9 | 7.5 ± 0.6 | ||
| IRAS 03521+0028 | 47.8 ± 1.8 | 14.1 ± 0.5 | 73.1 ± 5.6 | 9.6 ± 0.7 | ||||
| IRAS F05024-1941 | 22.0 ± 1.6 | 10.7 ± 0.8 | 35.5 ± 2.6 | 7.7 ± 0.6 | ||||
| IRAS F05189-2524 | 42.0 ± 1.3 | 3.7 ± 0.1 | 133.6 ± 5.8 | 3.0 ± 0.1 | 167.0 ± 15.5 | 1.6 ± 0.2 | 134.4 ± 17.1 | 0.7 ± 0.1 |
| IRAS 06035-7102 | 40.3 ± 1.9 | 12.7 ± 0.6 | 154.4 ± 6.7 | 12.1 ± 0.5 | 326.5 ± 14.8 | 11.4 ± 0.5 | 224.9 ± 17.4 | 3.9 ± 0.3 |
| IRAS 06206-6315 | 81.6 ± 4.9 | 8.7 ± 0.5 | 115.0 ± 7.0 | 5.5 ± 0.3 | ||||
| IRAS 07251-0248 | 71.3 ± 1.0 | 6.8 ± 0.1 | 145.5 ± 12.4 | 6.2 ± 0.5 | ||||
| IRAS 08311-2459 | 136.7 ± 5.3 | 17.3 ± 0.7 | 247.4 ± 16.5 | 13.9 ± 0.9 | ||||
| IRAS 09022-3615 | 284.4 ± 7.9 | 12.5 ± 0.3 | 368.2 ± 40.3 | 7.2 ± 0.8 | 168.0 ± 16.3 | 1.6 ± 0.2 | ||
| IRAS 10378+1109 | 46.7 ± 3.1 | 11.1 ± 0.7 | 89.0 ± 6.8 | 9.4 ± 0.7 | ||||
| IRAS 11095-0238 | 43.4 ± 2.9 | 6.2 ± 0.4 | 761.5* | 48.4* | ||||
| IRAS F12072-0444 | 6.6 ± 0.8 | 5.6 ± 0.7 | 49.3 ± 3.4 | 10.3 ± 0.7 | 45.2 ± 7.8 | 4.2 ± 0.7 | ||
| IRAS F12112+0305 | 34.6 ± 1.1 | 9.2 ± 0.3 | 183.8 ± 9.0 | 12.2 ± 0.6 | 306.7 ± 19.6 | 9.0 ± 0.6 | 88.0 ± 12.2 | 1.3 ± 0.2 |
| IRAS 13120-5453 | 263.8 ± 4.6 | 12.2 ± 0.2 | 838.3 ± 28.6 | 9.7 ± 0.3 | 1477.2 ± 55.2 | 7.6 ± 0.3 | 794.2 ± 42.8 | 2.0 ± 0.1 |
| IRAS F13305-1739 | 11.4 ± 1.3 | 3.2 ± 0.4 | ||||||
| IRAS F13451+1232 | 11.8 ± 0.6 | 8.8 ± 0.5 | 29.2 ± 4.2 | 5.5 ± 0.8 | 80.1 ± 0.2 | 6.7 ± 0.02 | ||
| IRAS F14348-1447 | 201.0 ± 6.4 | 17.3 ± 0.5 | 115.4 ± 16.7 | 2.2 ± 0.3 | ||||
| IRAS F14378-3651 | 19.4 ± 1.0 | 4.4 ± 0.2 | 78.0 ± 1.6 | 4.5 ± 0.1 | 68.5 ± 3.1 | 0.9 ± 0.01 | ||
| IRAS F15462-0450 | 47.0 ± 2.8 | 23.8 ± 1.4 | ||||||
| IRAS 16090-0139 | 17.0 ± 0.9 | 15.5 ± 0.8 | 97.5 ± 3.9 | 22.1 ± 0.9 | 148.3 ± 12.9 | 15.0 ± 1.3 | 123.8 ± 13.6 | 6.2 ± 0.7 |
| IRAS 17208-0014 | 150.9 ± 2.0 | 13.5 ± 0.2 | 583.0 ± 14.6 | 13.1 ± 0.3 | 1041.2 ± 36.6 | 10.4 ± 0.4 | 339.1 ± 26.0 | 1.7 ± 0.1 |
| IRAS 19254-7245 | 170.0 ± 6.4 | 7.9 ± 0.3 | 98.7 ± 13.5 | 1.0 ± 0.1 | ||||
| IRAS F19297-0406 | 57.5 ± 3.0 | 5.3 ± 0.3 | 214.7 ± 4.6 | 8.7 ± 0.2 | ||||
| IRAS 19542+1110 | 16.5 ± 0.8 | 3.2 ± 0.15 | 48.8 ± 3.6 | 2.3 ± 0.2 | 93.9 ± 14.0 | 1.0 ± 0.1 | ||
| IRAS 20087-0308 | 30.3 ± 1.6 | 17.0 ± 0.9 | 141.8 ± 4.6 | 19.9 ± 0.6 | 202.1 ± 4.2 | 12.6 ± 0.3 | ||
| IRAS 20100-4156 | 11.3 ± 0.2 | 9.7 ± 0.2 | 54.7 ± 3.0 | 11.7 ± 0.6 | 133.5 ± 8.4 | 12.7 ± 0.8 | ||
| IRAS 20414-1651 | 63.7 ± 3.1 | 6.0 ± 0.3 | 163.0 ± 11.1 | 6.9 ± 0.5 | ||||
| IRAS F20551-4250 | 67.1 ± 1.5 | 6.1 ± 0.13 | 292.1 ± 6.5 | 6.6 ± 0.15 | 389.0 ± 19.2 | 3.9 ± 0.2 | 90.8 ± 5.2 | 0.5 ± 0.03 |
| IRAS F22491-1808 | 77.9 ± 4.6 | 5.9 ± 0.3 | 133.8 ± 7.4 | 4.5 ± 0.2 | 106.2 ± 16.0 | 1.8 ± 0.3 | ||
| IRAS F23060+0505 | 10.7 ± 0.3 | 16.5 ± 0.5 | 54.2 ± 3.1 | 20.9 ± 1.2 | 70.3 ± 3.6 | 12.1 ± 0.6 | ||
| IRAS F23128-5919 | 51.2 ± 0.7 | 5.0 ± 0.1 | 191.9 ± 4.4 | 4.7 ± 0.1 | 329.5 ± 5.4 | 3.6 ± 0.1 | 233.3 ± 43.0 | 1.2 ± 0.2 |
| IRAS 23230-6926 | 8.3 ± 0.7 | 4.8 ± 0.4 | 44.1 ± 3.3 | 6.3 ± 0.5 | 83.5 ± 2.4 | 5.3 ± 0.2 | ||
| IRAS 23253-5415 | 119.6 ± 3.9 | 25.7 ± 0.8 | 160.1 ± 10.5 | 15.3 ± 1.0 | ||||
| IRAS F23389+0300 | 24.1 ± 1.3 | 6.5 ± 0.4 | 52.4 ± 3.1 | 6.3 ± 0.4 | ||||
| IRAS F00509+1225 | 47.4 ± 4.7 | 8.7 ± 0.9 | 80.6 ± 6.1 | 3.7 ± 0.3 | 67.7 ± 16.4 | 0.7 ± 0.2 | ||
| PG1126-041 | 16.7 ± 0.4 | 0.7 ± 0.02 | ||||||
| IRAS F12243-0036 | 101.6 ± 1.0 | 0.2 ± 0.003 | 428.2 ± 5.6 | 0.3 ± 0.003 | 862.5 ± 56.3 | 0.2 ± 0.02 | 520.4 ± 61.5 | 0.1 ± 0.001 |
| PG2130+099 | 22.5 ± 1.8 | 1.1 ± 0.1 | 72.4* | 0.78* | ||||
Notes. We compute the 3σ upper limit on the total integrated line flux, following 
, where σrms, channel is the rms noise per spectral channel, δvchannel is the channel width, and Δvline is the expected line width (assumed to be equal to the CO(2–1) line width).
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