Dust and gas in star-forming galaxies at z ~ 3 - Extending galaxy uniformity to 11.5 billion years

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Table 2

Physical properties.

Name	log L_IR	I_{CO [3−2]}	^a	log M_dust^b	log M_H₂^c	log M_∗	⟨ U ⟩	T_d ^d
	[L_⊙]	[Jy km s^-1]	[K km s^-1 pc²]	[M_⊙]	[M_⊙]	[M_⊙]	–	[K]

D49	12.78 ± 0.03	1.10 ± 0.18	10.93 ± 0.11	9.12 ± 0.12	11.32 ± 0.15	11.28 ± 0.12	35.7 ± 7.0	40.6 ± 2.0
M28	12.51 ± 0.04	–	–	8.90 ± 0.15	11.01 ± 0.12	11.38 ± 0.10	32.2 ± 8.0	41.8 ± 3.0

Notes.

^(a)

CO[1–0] luminosity assuming an excitation correction of r₃₁ = 0.5. The quoted uncertainty includes the observed uncertainty in the flux measurement and the uncertainty in r₃₁, in quadrature.

^(b)

Derived based on DL07 models.

^(c)

Average value, between CO, δ_GD and R-J approach.

^(d)

Based on a MBB model with fixed β = 1.8.

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