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

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Table C.6

Parameters of the fits of L_CO as a function of the clump properties for the Gaussian fluxes.

Transition	Property	α	β	ϵ
	L_bol	−0.80	0.54 ± 0.04	0.33
CO (4–3)	M_clump	−1.36	0.92 ± 0.06	0.32
	L∕M	1.06	0.36 ± 0.09	0.56

	L_bol	−0.95	0.62 ± 0.04	0.24
CO (6–5)	M_clump	−1.16	0.92 ± 0.07	0.33
	L∕M	1.08	0.49 ± 0.07	0.52

	L_bol	−1.26	0.65 ± 0.03	0.22
CO (7–6)	M_clump	−1.62	1.01 ± 0.07	0.31
	L∕M	0.79	0.59 ± 0.09	0.51

Notes. The fits were performed by adjusting a model with three free parameters in the form of log (y) = α + βlog(x) ± ϵ, where α, β and ϵ correspond to the intercept, the slope and the intrinsic scatter, respectively.

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