CO excitation of normal star-forming galaxies out to z = 1.5 as regulated by the properties of their interstellar medium

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Table 3

Far-IR SED fitting results and other physical properties.

Source	⟨ U ⟩	log L_IR/L_⊙	log M_dust/M_⊙	f_{1.3 mm} [mJy]^a	f_{2.2 mm} [mJy]^a	log M_stars/M_⊙	CO FWHM[′′]^b	C^c

4171	16.4 ± 4.2	12.00 ± 0.03	8.70 ± 0.10	0.35 ± 0.05	0.06 ± 0.01	10.60	1.34	0.12
16000	4.9 ± 1.3	11.85 ± 0.03	9.08 ± 0.10	0.52 ± 0.08	0.10 ± 0.02	10.63	1.28	0.07
17999	13.2 ± 2.9	12.06 ± 0.03	8.85 ± 0.09	0.48 ± 0.06	0.09 ± 0.02	10.59	0.75	0.11
21000	15.7 ± 3.3	12.32 ± 0.03	9.03 ± 0.09	0.66 ± 0.19	0.12 ± 0.04	10.89	0.72	0.18

Notes.

^(a)

Fluxes predicted from the SED fitting, computed at rest frequencies of CO[5–4] and CO[3–2].

^(b)

Reported from D10.

^(c)

Clumpiness measured in the HST-WFC3 F160W images (Sect. 6.6).

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