MUSE-ALMA Haloes - XII. Molecular gas in z ∼ 0.5 H I – selected galaxies

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Table A.1.

Detections. Measured properties of the new nine detected sources from the MUSE-ALMA Haloes ALMA Large Program.

Galaxy	z_gal	log N(H I)	b	12 + log(O/H)	[M/H]	CO line	F_peak	F_CO	FWHM	log $L'_{CO (1 - - 0)}$ $Mathematical equation: $ L\prime_{\mathrm{CO(1--0)}} $$	log M_H₂
		cm⁻²	kpc				mJy	mJy km s⁻¹	km s⁻¹	K km s⁻¹pc²	M_⊙
Q0152m2001_12	0.78018	18.87	55.0	8.73 ± 0.10	−1.9 ± 0.1	CO(2-1)	0.61	122 ± 40	241 ± 71	8.53 ± 0.17	9.11 ± 0.15
Q0152p0023_13	0.48206	19.78	140.0	8.68 ± 0.10	−0.1 ± 0.01	CO(2-1)	-	< 90	-	< 8.44	< 9.06
Q0152p0023_20	0.48143	19.78	122.9	8.43 ± 0.06	−0.1 ± 0.01	CO(2-1)	-	< 90	-	< 8.44	< 9.28
Q0152p0023_23	0.48068	19.78	187.8	8.59 ± 0.12	−0.1 ± 0.01	CO(2-1)	-	< 90	-	< 8.43	< 9.13
Q0152p0023_44	0.48320	19.78	170.7	-	−0.1 ± 0.01	CO(2-1)	-	< 90	-	< 8.44	< 9.63
Q0454m220_4	0.48377	18.65	107.6	8.66 ± 0.05	$- 0 . 7_{- 0.7}^{+ 0.1}$ $Mathematical equation: $ -0.7^{+0.1}_{-0.7} $$	CO(2-1)	1.10	256 ± 31	198 ± 37	8.50 ± 0.05	9.14 ± 0.05
Q0454m220_69	0.47450	19.45	8.4	8.33 ± 0.12	−0.48 ± 0.1	CO(2-1)	-	< 106	-	< 8.50	< 9.44
Q0454p039_15	1.15497	18.59	58.0	-	−0.19 ± 0.22	CO(3-2)	-	< 88	-	< 8.84	< 10.02
Q0454p039_57	0.85877	20.69	18.3	-	−1.57 ± 0.17	CO(4-3)	-	< 271	-	< 8.83	< 10.00
Q0454p039_65	1.15470	18.59	127.1	-	−0.19 ± 0.22	CO(3-2)	-	< 88	-	< 8.84	< 9.66
Q1110p0048_15	0.56035	20.20	129.7	8.26 ± 0.09	-	CO(2-1)	-	< 73	-	< 8.48	< 9.50
Q1110p0048_44	0.56118	20.20	5.7	8.46 ± 0.10	-	CO(2-1)	-	< 73	-	< 8.49	< 9.30
Q1110p0048_6	0.56006	20.20	59.6	8.490.05	-	CO(2-1)	-	< 73	-	< 8.48	< 9.27
Q1211p1030_13	0.89909	18.50	175.3	-	< − 1.2	CO(4-3)	-	< 159	-	< 8.63	< 9.85
Q1211p1030_16	0.89940	18.50	77.4	-	< − 1.2	CO(4-3)	0.90	90 ± 40	112 ± 46	7.87 ± 0.24	8.70 ± 0.24
Q1211p1030_38	0.63031	20.30	138.4	8.44 ± 0.10	−2.82 ± 0.89	CO(2-1)	-	< 89	-	< 8.67	< 9.51
Q1211p1030_57	0.62957	20.30	16.9	8.63 ± 0.20	−2.82 ± 0.89	CO(2-1)	-	< 89	-	< 8.67	< 9.34
Q1211p1030_58	0.89894	18.50	268.6	-	< − 1.2	CO(4-3)	-	< 159	-	< 8.63	< 9.58
Q1229m021_10	0.83190	18.84	173.6	8.63 ± 0.16	< − 2.6	CO(2-1)	-	< 86	-	< 8.90	< 9.56
Q1229m021_41	0.83199	18.84	186.8	8.34 ± 0.19	< − 2.6	CO(2-1)	-	< 86	-	< 8.90	< 9.83
Q1229m021_6	0.83170	18.84	182.2	-	< − 2.6	CO(2-1)	0.39	197 ± 43	419 ± 191	8.93 ± 0.08	9.74 ± 0.08
Q1229m021_8	0.83060	18.84	125.5	-	< − 2.6	CO(2-1)	0.36	172 ± 16	464 ± 204	8.76 ± 0.04	9.59 ± 0.04
Q1342m0035_4	0.53773	19.78	43.6	8.67 ± 0.06	−1.2 ± 0.1	CO(2-1)	1.44	273 ± 40	169 ± 34	8.63 ± 0.06	9.26 ± 0.06
Q1342m0035_9	0.53877	19.78	24.3	8.60 ± 0.18	−1.2 ± 0.1	CO(2-1)	-	< 92	-	< 8.55	< 9.24
Q1345m0023_13	0.60697	18.85	55.6	8.64 ± 0.07	−0.9 ± 0.2	CO(2-1)	0.94	201 ± 43	224 ± 75	8.49 ± 0.12	9.15 ± 0.13
Q1345m0023_40	0.60540	18.85	162.4	8.31 ± 0.14	−0.9 ± 0.2	CO(2-1)	-	< 112	-	< 8.74	< 9.70
Q1431m0050_10	0.60843	19.18	45.4	8.62 ± 0.05	−0.8 ± 0.1	CO(2-1)	4.13	116 ± 47	77 ± 13	8.46 ± 0.13	9.13 ± 0.15
Q1431m0050_26	0.68710	18.40	23.3	-	$- 1 . 2_{- 0.01}^{+ 0.03}$ $Mathematical equation: $ -1.2^{+0.03}_{-0.01} $$	CO(2-1)	-	< 100	-	< 8.80	< 9.41
Q1431m0050_68	0.60742	19.18	73.0	-	−0.8 ± 0.1	CO(2-1)	-	< 95	-	< 8.67	< 9.34
Q1431m0050_73	0.68687	18.40	188.7	-	$- 1 . 2_{- 0.01}^{+ 0.03}$ $Mathematical equation: $ -1.2^{+0.03}_{-0.01} $$	CO(2-1)	-	< 100	-	< 8.80	< 9.84
Q1515p0410_13	0.55860	20.20	194.1	8.75 ± 0.08	0.2 ± 0.24	CO(2-1)	-	< 78	-	< 8.51	< 9.07
Q1515p0410_4	0.55859	20.20	10.1	-	0.2 ± 0.24	CO(2-1)	-	< 78	-	< 8.51	< 9.16
Q1515p0410_54	0.55892	20.20	168.8	8.53 ± 0.15	0.2 ± 0.24	CO(2-1)	-	< 78	-	< 8.51	< 9.26
Q1515p0410_9	0.55866	20.20	221.0	8.61 ± 0.11	0.2 ± 0.24	CO(2-1)	-	< 78	-	< 8.51	< 9.19
Q1554m203_51	0.78558	19.00	23.0	-	< − 1.6	CO(2-1)	-	< 79	-	< 8.82	< 9.69
Q2131m1207_26	0.42971	19.50	172.1	8.43 ± 0.12	−1.47 ± 0.22	CO(2-1)	-	< 91	-	< 8.34	< 9.18
Q2131m1207_34	0.43080	19.50	59.2	8.12 ± 0.11	−1.47 ± 0.22	CO(2-1)	-	< 91	-	< 8.34	< 9.52
Q2131m1207_43	0.43003	19.50	145.9	-	−1.47 ± 0.22	CO(2-1)	-	< 91	-	< 8.34	< 8.99
Q2131m1207_5	0.42999	19.50	48.5	8.68 ± 0.05	−1.47 ± 0.22	CO(2-1)	0.85	210 ± 26	225 ± 41	8.26 ± 0.06	8.88 ± 0.06

b is the impact parameter, and F_peak is the measured peak flux

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