ATLASGAL-selected massive clumps in the inner Galaxy - VII. Characterisation of mid-J CO emission

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Table C.1

Kolmogorov–Smirnov statistics of the mid-J CO line luminosity for the distance-limited sub-sample as a function of the evolutionary class of the clumps.

Transition	70w -IRw	70w -IRb	70w -H II	IRw-IRb	IRw-H II	IRb-H II
CO (6–5)	0.60, p < 0.001	0.80, p < 0.001	0.95, p < 0.001	0.31, p = 0.08	0.71, p <=0.001	0.51, p = 0.001
CO (7–6)	0.73, p < 0.001	0.80, p < 0.001	1.00, p < 0.001	0.34, p = 0.04	0.68, p <=0.001	0.52, p = 0.001

Notes. The rank KS and its corresponding probability (p) are shown for each comparison. A p-value of <0.001 indicate a correlation at 0.001 significance level. p-values of 0.05, 0.002 and <0.001 represent the ~ 2, 3 and > 3 σ confidence levels.

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