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Table A.1
Flux corrections to a common beam size.
| Galaxy | rs | Transition | Original beam | Common beam | Aperture | Tmb | ICO |
| (arcsec) | (arcsec) | (arcsec) | correction | correction | corrected | ||
| A Pcor | (K km s-1) | ||||||
|
|
|||||||
| Mrk 0996 | 3.6 | 12CO(1–0) | 21.4 | 22.0 | 1.014 | 0.964 | 0.235 |
| Mrk 0996 | 3.6 | 12CO(2–1) (IRAM) | 10.7 | 22.0 | 1.843 | 0.438 | 0.128 |
| Mrk 0996 | 3.6 | 12CO(2–1) (APEX) | 27.2 | 22.0 | 0.908 | 1.389 | 0.938 |
| Mrk 0996 | 3.6 | 12CO(3–2) | 18.1 | 22.0 | 1.13 | 0.77 | <0.161 |
| NGC 1140 | 6.4 | 12CO(1–0) | 21.4 | 22.0 | 1.027 | 0.976 | 0.564 |
| NGC 1140 | 6.4 | 12CO(2–1) | 10.7 | 22.0 | 2.502 | 0.595 | 1.180 |
| NGC 1140 | 6.4 | 12CO(3–2) | 18.1 | 22.0 | 1.238 | 0.841 | 0.972 |
| NGC 1140 | 6.4 | 12CO(4–3) | 13.6 | 22.0 | 1.784 | 0.682 | 0.582 |
| NGC 1140 | 6.4 | 13CO(1–0) | 22.4 | 22.0 | 0.980 | 1.019 | 0.053 |
| NGC 1140 | 6.4 | 13CO(2–1) | 11.2 | 22.0 | 2.342 | 0.609 | 0.105 |
| NGC 1140 | 6.4 | [Ci](1–0) | 12.7 | 22.0 | 1.952 | 0.655 | 0.369 |
| NGC 1156 | 44.9 | 12CO(1–0) | 21.4 | 22.0 | 1.055 | 0.995 | 1.841 |
| NGC 1156 | 44.9 | 12CO(2–1) | 10.7 | 22.0 | 3.903 | 0.921 | 0.668 |
| NGC 3353 | 5.4 | 12CO(1–0) | 21.4 | 22.0 | 1.025 | 0.971 | 2.100 |
| NGC 3353 | 5.4 | 12CO(2–1) | 10.7 | 22.0 | 2.314 | 0.548 | 1.876 |
| NGC 7077 | 4.8 | 12CO(1–0) | 21.4 | 22.0 | 1.022 | 0.969 | 0.474 |
| NGC 7077 | 4.8 | 12CO(2–1) | 10.7 | 22.0 | 2.175 | 0.516 | 0.548 |
| NGC 7077 | 4.8 | 12CO(3–2) | 18.1 | 22.0 | 1.186 | 0.804 | 0.431 |
| UM 448 | 4.4 | 12CO(1–0) | 21.4 | 22.0 | 1.009 | 0.985 | 1.035 |
| UM 448 | 4.4 | 12CO(2–1) (IRAM) | 10.7 | 22.0 | 2.036 | 0.497 | 1.237 |
| UM 448 | 4.4 | 12CO(2–1) (APEX) | 27.6 | 22.0 | 0.869 | 1.365 | 2.106 |
| UM 448 | 4.4 | 12CO(3–2) | 18.1 | 22.0 | 1.154 | 0.806 | 0.705 |
Notes. Assuming that the CO is distributed in an exponential disk like the dust.
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