An ALMA survey of submillimetre galaxies in the COSMOS field: The extent of the radio-emitting region revealed by 3 GHz imaging with the Very Large Array

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Table E.1

Parameters of the T_dust profiles derived using different assumptions.

τ _ν ^a	^b	r ₀ ^b	m ^b	r = r(T_CMB) ^c
	[K]	[′′]		[′′]

0.48 (β = 1.5)	24.3	0.436 ± 0.002	2.378 ± 0.015	0.367
0.38 (β = 2)	25.6	0.397 ± 0.018	2.718 ± 0.158	0.358
0.66 (M_dust; β = 1.5)	22.9	0.449 ± 0.012	2.462 ± 0.080	0.357
1.51 (M_dust; β = 2)	20.7	0.497 ± 0.021	2.377 ± 0.104	0.344

Notes.

^(a)

The optical thickness at λ_rest = 163μm based on different assumptions of β and using either a simple frequency scaling or dust mass method (Eq. (E.2)).

^(b)

The Plummer profile parameters of Eq. (E.3).

^(c)

The radius at which the CMB temperature is reached.

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