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Table 2

Observation log.

Source IAU name RA Dec Observed lines H2O observation H2O ref
(J2000) (J2000)

G09v1.97 J083051.0+013224 08:30:51.156 +01:32:24.35 CO(3–2), (5–4) , (6–5) , (7–6) , [C I](2–1) 211–202, 321–312 1
G09v1.40 J085358.9+015537 08:53:58.862 +01:55:37.70 CO(2–1), CO(4–3) , (6–5) , (7–6) , [C I](2–1) 211–202 1
SDP17b J090302.9014127 09:03:03.031 01:41:27.11 CO(3–2), (4–3) , (7–6) , (8–7) , [C I](2–1) 202–111 2, 3
SDP81 J090311.6+003906 09:03:11.568 +00:39:06.43 CO(3–2), (5–4) , (6–5) , (109) 202–111 2
G12v2.43 J113526.3014605 11:35:26.273 01:46:06.55 CO(3–2), (4–3) , (5–4) , (6–5) , (8–7) , (109) 202–111, 321–312 1
G12v2.30 J114637.9001132 11:46:37.980 00:11:31.80 CO(4–3), (5–4) , (6–5) , (8–7) , (1110) 202–111 2
NCv1.143 J125632.7+233625 12:56:32.544 +23:36:27.63 CO(3–2), (5–4) , (6–5) , (7–6) , (109)a, [C I](2–1) 211–202, 321–312 1
NAv1.195 J132630.1+334410 13:26:30.216 +33:44:07.60 CO(5–4) 202–111, 321–312b 1
NAv1.177 J132859.3+292317 13:28:59.246 +29:23:26.13 CO(3–2), (5–4) , (7–6) , (8–7), [C I](2–1) 202–111, 321–312 1
NBv1.78 J133008.4+245900 13:30:08.520 +24:58:59.17 CO(5–4), (6–5) 202–111, 321–312 1
NAv1.144 J133649.9+291801 13:36:49.900 +29:18:01.00 CO(3–2), (4–3) , (7–6) , (8–7) , [C I](2–1) 211–202 2
NAv1.56 J134429.4+303036 13:44:29.518 +30:30:34.05 CO(5–4) 211–202 1
G15v2.235 J141351.9000026 14:13:51.900 00:00:26.00 CO(3–2), (4–3) , (5–4) , (7–6) , (9–8) , [C I](2–1)

G12v2.890 J113243.1005108 11:32:42.970 00:51:08.90 CO(3–2), (5–4) , (9–8)
G12v2.257 J115820.2013753 11:58:20.190 01:37:55.20 CO(3–2), (4–3) , (7–6) , (8–7) , [C I](2–1)

Notes. RA and Dec are the J2000 coordinates of the SMA 880 μm images from Bu13 (except for G12v2.890 and G12v2.257 which were not observed by SMA, Herschel SPIRE image coordinates in Valiante et al. 2016 are then used instead). These coordinates were used for observations. See Table B.1 for the observing frequencies. The H2O observations for each source are reported in (1) Yang et al. (2016); (2) Omont et al. (2013); (3) Omont et al. (2011). The sources have been divided into two groups as in the table, see Sect. 2.1 for more details.

(a)

This CO(109) data is taken from NOEMA/IRAM project S15CV (Yang et al., in prep.).

(b)

Except for this line, the rest H2O lines are detected.

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