Submillimeter H2O and H2O+emission in lensed ultra- and hyper-luminous infrared galaxies at z ~ 2–4

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Volume 595 (November 2016)

A&A, 595 (2016) A80

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Table 1

Observation log.

IAU name	Source	RA	Dec	RA_pk	Dec_pk	H₂O line	ν_obs	Beam	t_on
		(J2000)	(J2000)	(J2000)	(J2000)		(GHz)	(″)	(h)

H-ATLAS J083051.0+013224	G09v1.97	08:30:51.02	+01:32:24.88	08:30:51.17	+01:32:24.39	2₁₁–2₀₂	162.286	5.6 × 3.3	3.5
				08:30:51.17	+01:32:24.09	3₂₁–3₁₂	250.952	2.6 × 1.1	3.1
H-ATLAS J113526.3−014605	G12v2.43	11:35:26.36	−01:46:05.56	11:35:26.27	−01:46:06.44	2₀₂–1₁₁	239.350	2.3 × 1.0	6.9
				11:35:26.28	−01:46:06.43	3₂₁–3₁₂	281.754	2.2 × 1.1	1.5
H-ATLAS J125632.7+233625	NCv1.143	12:56:32.70	+23:36:24.86	12:56:32.56	+23:36:27.92	2₁₁–2₀₂	164.739	3.1 × 2.9	1.5
				12:56:32.56	+23:36:27.69	3₂₁–3₁₂	254.745	2.1 × 1.0	1.5
H-ATLAS J132630.1+334410	NAv1.195	13:26:30.12	+33:44:09.90	13:26:30.14	+33:44:09.11	2₀₂–1₁₁	250.045	2.0 × 1.7	3.8
				13:26:30.14	+33:44:09.09	3₂₁–3₁₂	293.334	1.0 × 0.9	3.1
H-ATLAS J132859.3+292327	NAv1.177	13:28:59.29	+29:23:27.07	13:28:59.25	+29:23:26.18	2₀₂–1₁₁	261.495	1.9 × 1.7	2.3
				13:28:59.25	+29:23:26.34	3₂₁–3₁₂	307.812	1.6 × 0.9	2.3
H-ATLAS J133008.4+245900	NBv1.78	13:30:08.56	+24:58:58.30	13:30:08.56	+24:58:58.55	3₂₁–3₁₂	282.878	1.7 × 1.1	4.2
H-ATLAS J084933.4+021443	G09v1.124-W	08:49:33.36	+02:14:42.30	08:49:33.59	+02:14:44.68	2₁₁–2₀₂	220.537	1.8 × 1.2	8.4
H-ATLAS J084933.4+021443	G09v1.124-T	08:49:33.36	+02:14:42.30	08:49:32.95	+02:14:39.70	2₁₁–2₀₂	220.537	1.8 × 1.2	8.4
H-ATLAS J085358.9+015537	G09v1.40	08:53:58.90	+01:55:37.00	08:53:58.84	+01:55:37.75	2₁₁–2₀₂	243.425	1.8 × 1.0	1.9
H-ATLAS J091043.1−000321	SDP11	09:10:43.09	−00:03:22.51	09:10:43.06	−00:03:22.10	2₀₂–1₁₁	354.860	1.9 × 1.5	3.8
H-ATLAS J125135.4+261457	NCv1.268	12:51:35.46	+26:14:57.52	12:51:35.38	+26:14:58.12	2₁₁–2₀₂	160.864	2.9 × 2.6	7.7
H-ATLAS J134429.4+303036	NAv1.56	13:44:29.52	+30:30:34.05	13:44:29.46	+30:30:34.01	2₁₁–2₀₂	227.828	1.7 × 1.7	2.3

Notes. RA and Dec are the J2000 Herschel coordinates which were taken as the centres of the NOEMA images displayed in Fig. A.1; RA_pk and Dec_pk are the J2000 coordinates of the NOEMA dust continuum image peaks; ν_obs is the central observed frequency. The rest-frame frequencies of para-H₂O 2₀₂–1₁₁, 2₁₁–2₀₂and ortho-H₂O 3₂₁–3₁₂ lines are: 987.927 GHz, 752.033 GHz and 1162.912 GHz, respectively (the rest-frame frequencies are taken from the JPL catalogue: http://spec.jpl.nasa.gov); t_on is the on-source integration time. The source G09v1.124, which is not resolved by SPIRE, is a cluster that consists of two main components: eastern component W (G09v1.124-W) and western component T (G09v1.124-T) as described in Ivison et al. (2013) (see also Fig. A.3).

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