A sensitive APEX and ALMA CO(1–0), CO(2–1), CO(3–2), and [CI](1–0) spectral survey of 40 local (ultra-)luminous infrared galaxies

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Volume 673 (May 2023)

A&A, 673 (2023) A13

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Table B.2.

Description of the observations

Galaxy name	CO(1–0)			CO(2–1)			CO(3–2)			[CI](1–0)
	d_aperture [”]	t_obs [h]	rms [mJy]	d_aperture [”]	t_obs [h]	rms [mJy]	d_aperture [”]	t_obs [h]	rms [mJy]	d_aperture [”]	t_obs [h]	rms [mJy]
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)
IRAS 00188−0856	30	0.65	3	28	1.4	32	15	0.34	5

IRAS 01003−2238	5	0.03	5	28	3.3	35	20	0.84	45
							20	0.49	93

IRAS F01572+0009^†	7	0.03	10	34	1.3	12	20	1.6	30
							8	0.54	5

IRAS 03521+0028				34	2.0	10	20	0.95	28

IRAS F05024−1941				34	2.3	10	20	1.24	22

IRAS F05189−2524	30	1.5	4	27	0.21	25	20	0.75	120	13	0.82	148
							12	1.86	13

IRAS 06035−7102	41	0.24	11	27	0.19	32	20	3.3	486	13	0.6	158

IRAS 06206−6315				27	0.6	26	20	0.44	59
							20	0.8	45

IRAS 07251−0248				5	0.69	3.3	20	1.11	110
				28	1.22	24

IRAS 08311−2459				27	0.43	41	20	0.74	98

IRAS 09022−3615				27	0.46	39	20	0.63	152	13	0.17	139
										8	0.08	46

IRAS 10378+1109				27	1.66	22	20	1.43	42

IRAS 11095−0238				27	0.76	26	20	0.37	144

IRAS F12072−0444^†	5	0.03	7	27	0.33	29	20	0.86	65

IRAS F12112+0305	10	0.09	5	27	0.4	37	20	1.47	113	13	0.23	148
							15	2.72	42	10	0.08	36

IRAS 13120−5453	17	0.22	12	28	0.35	81	20	0.5	130	13	0.17	185
				30			20

IRAS F13305−1739				34	0.71	12

IRAS F13451+1232	12	0.4	4	27	0.24	26	20	1.26	37
							6	0.08	6

IRAS F14348−1447				27	0.21	32				13	0.24	292

IRAS F14378−3651	30	0.15	8	28	0.21	107				9	0.08	15
				20	0.08	9				13	0.08	191

IRAS F15462−0450	17	0.3	17	28	1.9	20

IRAS 16090−0139	30	0.15	6	27	0.68	21	20	0.53	77	13	1.8	131
							15	0.17	13

IRAS 17208−0014	16	0.53	1.35	27	0.11	39	20	0.34	239	13	0.18	232
							11	0.27	81.5

IRAS 19254−7245				28	1.2	27				13	0.41	79

IRAS F19297−0406				27	0.42	19	30	0.17	19

IRAS 19542+1110	9	0.35	5	27	0.64	34				13	0.08	138

IRAS 20087−0308	30	0.08	9	27	0.59	22	20	0.17	14

IRAS 20100−4156	25	3.5	1	27	1.09	17	20	1.58	59
							7	0.94	6

IRAS 20414−1651				27	0.98	19	20	1.24	70
				4	0.78	122	20	0.76	90

IRAS F20551−4250	35	0.4	11	27	0.4	42	20	0.42	150	9	0.08	44
							20	0.2	132

IRAS F22491−1808				27	0.32	30	20	2	69	13	0.53	135
										9	0.08	29

IRAS F23060+0505	10	3	1	34	1.32	16	20	2.7	28

IRAS F23128−5919	23	2.27	2	27	0.68	26	15	2.7	20	13	0.16	414
							20	0.35	102	11	0.08	43

IRAS 23230−6926	30	1.29	4	27	0.73	21	20	0.58	8
							15	0.6	116

IRAS 23253−5415				27	0.83	21	20	1.28	75

IRAS F23389+0300				34	2.4	11	20	1.8	25

IRAS F00509+1225	23	0.07	26	27	0.29	42				13	0.72	650

PG1126−041				32	2.5	2
				27	0.59	25

IRAS F12243−0036	12	0.5	4	29	1.3	18	20	0.06	562	13	0.11	327
										9	0.45	23

PG2130+099				30	2.06	3				13	1.8	70
				27	2	17

Notes. For each transition, we report single-dish beam or spectral extraction aperture (d_aperture), the observing time (t_obs) (corresponding to the effective value after excluding the discarded sub-scans), and the spectral rms computed using Δv = 50 km s⁻¹velocity channels. ^† Sources for which uv-tapering was applied for the ALMA CO(1–0) archival data.

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