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Table 4

Average CO SLED of the (U)LIRGs from P12 that we used here.

J I CO a ΔICO b N bands c

1 1.00 0.00 14
2 3.59 0.22 13
3 7.11 0.53 14
4 12.4 1.40 6
5 12.2 1.90 0
6 10.6 2.40 14

Notes.

(a)

Fluxes of individual galaxies have been normalised to CO[1–0].

(b)

The error is the rms dispersion of individual measurements divided by the square root of the number of galaxies in the sample.

(c)

Total number of measurements available for the transition from P12. Lacking a direct measurement, we have used an estimate based on LVG modeling of the other available transitions.

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