Table 1. Open in new tab Observed CO...

Source	z_CO ^a	S_CO ^b	v_FWHM ^b	I_CO 1-0 ^c	\|$L_\mathrm{CO}^{\prime }\ ^d$\|	S_31 GHz ^e	S_35 GHz ^e
SPT 2332−53†	2.7256(2)	4.66 ± 0.51	342 ± 42	1.70 ± 0.25	3.94 ± 0.58	<120	<120
SPT 0538−50blue‡	2.7854(1)	3.81 ± 0.36	210 ± 34	0.85 ± 0.08	1.49 ± 0.14	–	–
SPT 0538−50red‡	2.7897(6)	1.18 ± 0.27	281 ± 80	0.35 ± 0.18	0.61 ± 0.31	–	–
SPT 0538−50	2.7855(1)	-	–	1.20 ± 0.20	2.16 ± 0.36	171 ± 35	130 ± 20

Source	z_CO ^a	S_CO ^b	v_FWHM ^b	I_CO 1-0 ^c	\|$L_\mathrm{CO}^{\prime }\ ^d$\|	S_31 GHz ^e	S_35 GHz ^e
SPT 2332−53†	2.7256(2)	4.66 ± 0.51	342 ± 42	1.70 ± 0.25	3.94 ± 0.58	<120	<120
SPT 0538−50blue‡	2.7854(1)	3.81 ± 0.36	210 ± 34	0.85 ± 0.08	1.49 ± 0.14	–	–
SPT 0538−50red‡	2.7897(6)	1.18 ± 0.27	281 ± 80	0.35 ± 0.18	0.61 ± 0.31	–	–
SPT 0538−50	2.7855(1)	-	–	1.20 ± 0.20	2.16 ± 0.36	171 ± 35	130 ± 20

Table 1.

Observed CO properties.

Source	z_CO ^a	S_CO ^b	v_FWHM ^b	I_CO 1-0 ^c	\|$L_\mathrm{CO}^{\prime }\ ^d$\|	S_31 GHz ^e	S_35 GHz ^e
		(mJy)	(km s⁻¹)	(Jy km s⁻¹)	(×10¹⁰ (μ/μ₀)⁻¹ K km s⁻¹ pc²)	(μJy)	(μJy)
SPT 2332−53†	2.7256(2)	4.66 ± 0.51	342 ± 42	1.70 ± 0.25	3.94 ± 0.58	<120	<120
SPT 0538−50blue‡	2.7854(1)	3.81 ± 0.36	210 ± 34	0.85 ± 0.08	1.49 ± 0.14	–	–
SPT 0538−50red‡	2.7897(6)	1.18 ± 0.27	281 ± 80	0.35 ± 0.18	0.61 ± 0.31	–	–
SPT 0538−50	2.7855(1)	-	–	1.20 ± 0.20	2.16 ± 0.36	171 ± 35	130 ± 20

Source	z_CO ^a	S_CO ^b	v_FWHM ^b	I_CO 1-0 ^c	\|$L_\mathrm{CO}^{\prime }\ ^d$\|	S_31 GHz ^e	S_35 GHz ^e
		(mJy)	(km s⁻¹)	(Jy km s⁻¹)	(×10¹⁰ (μ/μ₀)⁻¹ K km s⁻¹ pc²)	(μJy)	(μJy)
SPT 2332−53†	2.7256(2)	4.66 ± 0.51	342 ± 42	1.70 ± 0.25	3.94 ± 0.58	<120	<120
SPT 0538−50blue‡	2.7854(1)	3.81 ± 0.36	210 ± 34	0.85 ± 0.08	1.49 ± 0.14	–	–
SPT 0538−50red‡	2.7897(6)	1.18 ± 0.27	281 ± 80	0.35 ± 0.18	0.61 ± 0.31	–	–
SPT 0538−50	2.7855(1)	-	–	1.20 ± 0.20	2.16 ± 0.36	171 ± 35	130 ± 20

†Integrated values over all CO components are listed.

‡Here, SPT 0538−50blue and SPT 0538−50red are the brighter and fainter CO peaks, respectively.

^aCO redshift. For SPT 0538−50, the redshift is computed as the weighted average between the redshifts of SPT 0538−50blue and red.

^bCO line peak flux and line full-width half-maximum (FWHM) velocity.

^cIntegrated CO line intensity (I_CO = ∫S_COdv).

^dCO line luminosity. The magnification factor μ₀ is assumed to be 15 and 20 for SPT 2332−53 and SPT 0538−50, respectively.

^eContinuum fluxes at ∼31 and 35 GHz.