The ALMA Frontier Fields Survey - III. 1.1 mm emission line identifications in Abell 2744, MACSJ 0416.1-2403, MACSJ 1149.5+2223, Abell 370, and Abell S1063

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Volume 608 (December 2017)

A&A, 608 (2017) A138

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Table 2

Emission line candidates in five ALMA-FF galaxy clusters.

ID^a	RA	Dec	S/N	P _S/N	Sep.	P _sep	P	Line identification
					[′′]

A2744-EL01†	00:14:18.43	–30:24:47.50	6.0	0.777	0.5	0.120	0.093	CO(8–7) at z = 2.62, tentative
A2744-EL02	00:14:16.29	–30:24:22.44	5.9	0.925	0.5	0.120	0.111	...
A2744-EL03	00:14:18.88	–30:23:45.60	5.9	0.925	1.1	0.464	0.429	...
MACSJ 0416-EL01*	04:16:10.17	–24:04:37.82	6.4	0.026	1.6	0.783	0.020	No identification
MACSJ 0416-EL02	04:16:09.24	–24:05:21.67	6.1	0.342	1.3	0.635	0.217	...
MACSJ 0416-EL03*^,†	04:16:10.50	–24:05:05.47	6.0	0.500	0.4	0.091	0.045	CO(7–6) at z = 1.96, tentative
MACSJ 0416-EL04	04:16:10.56	–24:04:02.67	5.9	0.605	0.8	0.317	0.051	...
MACSJ 0416-EL05	04:16:12.32	–24:05:02.47	5.9	0.605	1.2	0.576	0.348	...
MACSJ 0416-EL06	04:16:08.68	–24:03:42.37	5.7	0.973	1.0	0.449	0.437	...
MACSJ 1149-EL01*	11:49:36.09	+22:23:47.90	6.0	0.368	0.1	0.006	0.002	No identification
MACSJ 1149-EL02	11:49:34.67	+22:23:44.40	5.9	0.500	1.9	0.892	0.446	...
MACSJ 1149-EL03*	11:49:38.37	+22:24:30.60	5.9	0.500	0.4	0.094	0.047	No identification
A370-EL01*	02:39:51.02	–01:33:45.39	7.6	0.000	0.0^b	0.000	0.000	CO(3–2) at z = 0.36, secure
A370-EL02	02:39:50.42	–01:34:40.86	5.8	0.667	1.7	0.613	0.409	...
A370-EL03	02:39:52.46	–01:35:35.33	5.8	0.667	3.6	0.986	0.658	...
A370-EL04*	02:39:53.25	–01:33:49.13	5.6	0.985	0.2	0.013	0.013	CO(3–2) at z = 0.28, tentative
A370-EL05	02:39:55.26	–01:34:43.13	5.6	0.985	1.7	0.613	0.604	...
AS1063-EL01*	22:48:40.14	–44:30:50.56	5.9	0.561	0.0^b	0.000	0.000	CO(3–2) at z = 0.35, secure
AS1063-EL02	22:48:48.03	–44:31:11.55	5.8	0.788	1.5	0.599	0.472	...
AS1063-EL03*	22:48:47.45	–44:32:59.00	5.8	0.788	0.1	0.004	0.003	CO(9–8) at z = 3.07, tentative
AS1063-EL04	22:48:40.37	–44:31:58.00	5.7	0.924	0.9	0.281	0.260	...
AS1063-EL05	22:48:43.65	–44:31:35.60	5.7	0.924	2.0	0.803	0.742	...
AS1063-EL06	22:48:47.26	–44:31:49.20	5.7	0.924	1.0	0.334	0.309	...
AS1063-EL07	22:48:48.42	–44:31:50.05	5.7	0.924	2.4	0.904	0.835	...
AS1063-EL08*	22:48:42.98	–44:31:55.70	5.6	0.985	0.2	0.016	0.016	No identification
AS1063-EL09	22:48:43.35	–44:32:31.40	5.6	0.985	0.9	0.281	0.277	...

Notes.

^(a)

Sources with P< 0.05 are denoted by “*”. Sources which are spatially coincident with significant 1.1 mm continuum detections are denoted by “†”; given the low source density of 1.1 mm continuum detections (GL17) and high likelihood of a physical connection, this implies P< 0.05.

^(b)

Sources that lie within the extents of large star-forming galaxies, and thus are considered to have separations of 0.̋0.

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