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Table 1

Target fields of the POETS survey.

Phase center
Field RA (J2000) Dec (J2000)
(h m s) (°′″) (10−5 L)
G009.99−0.03 18:07:50.100 −20:18:56.00 0.75
G012.43−1.12 18:16:52.100 −18:41:43.00 4.98
G012.90−0.24 18:14:34.400 −17:51:52.00 0.36
G012.91−0.26 18:14:39.400 −17:52:06.00 0.05
G014.64−0.58 18:19:15.500 −16:29:45.00 0.10
G026.42+1.69 18:33:30.500 −05:01:02.00 0.31
G031.58+0.08 18:48:41.700 −01:09:59.00 0.77
G035.02+0.35 18:54:00.700 +02:01:19.00 0.63
G049.19−0.34 19:22:57.800 +14:16:10.00 9.87
G076.38−0.62 20:27:25.500 +37:22:48.00 0.24
G079.88+1.18 20:30:29.100 +41:15:54.00 0.08
G090.21+2.32 21:02:22.700 +50:03:08.00 0.03
G105.42+9.88 21:43:06.500 +66:06:55.00 0.16
G108.20+0.59 22:49:31.500 +59:55:42.00 3.61
G108.59+0.49 22:52:38.300 +60:00:52.00 0.15
G111.24−1.24 23:17:20.800 +59:28:47.00 1.06
G160.14+3.16 05:01:40.200 +47:07:19.00 0.41
G168.06+0.82 05:17:13.700 +39:22:20.00 14.32
G176.52+0.20 05:37:52.100 +32:00:04.00 0.14
G182.68−3.27 05:39:28.400 +24:56:32.00 0.41
G183.72−3.66 05:40:24.200 +23:50:55.00 1.51
G229.57+0.15 07:23:01.800 −14:41:36.00 0.71
G236.82+1.98 07:44:28.200 −20:08:30.00 0.51
G240.32+0.07 07:44:51.900 −24:07:43.00 1.24
G359.97−0.46 17:47:20.200 −29:11:59.00 1.57
Targets presented in Moscadelli et al. (2016)
G005.88−0.39 18:00:30.306 −24:04:04.48 1.86
G011.92−0.61 18:13:58.120 −18:54:20.28 3.27
G012.68−0.18 18:13:54.744 −18:01:47.57 8.83
G016.58−0.05 18:21:09.084 −14:31:49.56 4.36a
G074.04−1.71 20:25:07.104 +34:49:58.58 0.25
G075.76+0.34 20:21:41.086 +37:25:29.28 0.75
G075.78+0.34 20:21:41.086 +37:25:29.28 7.98
G092.69+3.08 21:09:21.724 +52:22:37.10 2.98
G097.53+3.18 21:32:12.441 +55:53:50.61 69.72
G100.38−3.58 22:16:10.368 +52:21:34.11 1.40
G111.25−0.77 23:16:10.360 +59:55:29.53 1.36

Notes. Column 1: field name. Columns 2 and 3: phase center of the observations. Column 4: isotropic H2O maser luminosity. For each source, this luminosity refers to the averaged luminosity measured with the VLBA in the period from March 2011 to April 2012 (from the BeSSeL Survey data). The isotropic maser luminosity was estimated with the following formula: (L) = 2.3 ⋅ 10−8 × (SH2O Jy km s−1) × (D∕kpc)2, where SH2O and D are the integrated H2O maser flux and the heliocentric distance to the H2O maser site, respectively. (a)Luminosity estimated from data in Sanna et al. (2010a).

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