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Table 1

List of BeSSeL sources observed with the JVLA.

Source Position V LSR Dist. L bol
RA (J2000) Dec (J2000)
(hms) (°′′) (km s-1) (kpc) (L)

G000.670.04 17 47 20.1 28 23 03 65.0 7.75 ± 0.72 7.3 × 105
G000.680.03 17 47 19.9 28 22 19 55.0 7.75 ± 0.72 3.2 × 105
G005.88 0.39 18 00 30.3 24 04 04 9 2.99 ± 0.18 5.8 × 104
G009.990.03 18 07 50.1 20 18 56 50 5.0 a 1.2 × 10 4
G011.92 0.61 18 13 58.1 18 54 20 30 3.37 ± 0.35 1.2 × 104
G012.431.12 18 16 52.1 18 41 43 30 3.7 a 4.2 b × 10 4
G012.68 0.18 18 13 54.7 18 01 47 59 2.40 ± 0.18 5.7 × 103
G012.900.24 18 14 34.4 17 51 52 36 2.45 ± 0.15 8.6 × 102
G012.910.26 18 14 39.4 17 52 06 41 2.53 ± 0.20 2.7 × 104
G014.640.58 18 19 15.5 16 29 45 19 1.83 ± 0.07 1.1 × 103
G016.58 0.05 18 21 09.0 14 31 49 64 3.58 ± 0.30 1.3 × 104
G024.490.04 18 36 05.7 07 31 19 110 7.25c± 1.42 3.8 × 104
G026.42+1.69 18 33 30.5 05 01 02 55 3.1 a 9.0 b × 10 3
G031.58+0.08 18 48 41.7 01 09 59 96 4.90 ± 0.72 2.0 × 104
G035.02+0.35 18 54 00.7 +02 01 19 52 2.33 ± 0.22 1.0 × 104
G045.07+0.13 19 13 22.0 +10 50 53 59 8.00 ± 0.32 3.5 × 105
G048.61+0.02 19 20 31.2 +13 55 25 25 10.75 ± 0.58 2.8 × 105
G049.190.34 19 22 57.8 +14 16 10 67 5.29 ± 0.20 6.0 × 103
G074.04 1.71 20 25 07.1 +34 49 58 5 1.59 ± 0.05 3.7 b × 10 2
G075.76 + 0.34 20 21 41.1 +37 25 29 10 3.51 ± 0.28 1.4 × 104
G076.380.62 20 27 25.5 +37 22 48 2 1.30 ± 0.09 1.4 b × 10 4
G079.88+1.18 20 30 29.1 +41 15 54 5 1.61 ± 0.07 8.6 × 102
G090.21+2.32 21 02 22.7 +50 03 08 3 0.67 ± 0.02 2.7 × 101
G092.69 + 3.08 21 09 21.7 +52 22 37 10 1.63 ± 0.05 (4.7b× 103)
G097.53 + 3.18 21 32 12.4 +55 53 50 77 7.52 ± 0.96 (8.8b× 104)
G100.38 3.58 22 16 10.4 +52 21 34 30 3.44 ± 0.10 8.5 b × 10 3
G105.42+9.88 21 43 06.5 +66 06 55 10 0.89 ± 0.05 (5.8b× 102)
G108.20+0.59 22 49 31.5 +59 55 42 49 4.37 ± 0.53 2.1 × 103
G108.59+0.49 22 52 38.3 +60 00 52 52 2.51 ± 0.20 2.8 × 103
G111.241.24 23 17 20.8 +59 28 47 53 3.47 ± 0.53 1.0 b × 10 4
G111.25 0.77 23 16 10.4 +59 55 29 47 3.40 ± 0.18 5.0 b × 10 3
G160.14+3.16 05 01 40.2 +47 07 19 18 4.10 ± 0.10 8.4 b × 10 3
G168.06+0.82 05 17 13.7 +39 22 20 27 7.69 ± 2.37 1.6 × 104
G176.52+0.20 05 37 52.1 +32 00 04 17 0.96 ± 0.02 1.5 × 102
G182.683.27 05 39 28.4 +24 56 32 7 6.71 ± 0.50 8.6 b × 10 2
G183.723.66 05 40 24.2 +23 50 55 3 1.75 ± 0.04 9.7 b × 10 2
G229.57+0.15 07 23 01.8 14 41 36 47 4.52 ± 0.29 2.2 × 103
G236.82+1.98 07 44 28.2 20 08 30 43 3.36 ± 0.20 2.3 b × 10 3
G240.32+0.07 07 44 51.9 24 07 43 67 4.72 ± 0.47 8.3 × 103
G359.970.46 17 47 20.2 29 11 59 4 4.0 a 5.7 b × 10 4

Notes. Column 1 reports the source name: the sources with underlined name have been observed with the JVLA A-Array between October 2012 and January 2013, and those in boldface characters are the ones reported in this paper; Cols. 2–4 list the water maser position (RA and Dec, rounded to 0 1 and 1′′, respectively) and VLSR; Cols. 5 and 6 show the trigonometric parallax distance from BeSSeL (available for all but four sources, for which the kinematic distance is reported) and the evaluated bolometric luminosity, respectively. Kinematic distances and more uncertain luminosities are given in italic characters.

(a)

Since it was not possible to derive a reliable parallax measurement from the BeSSeL observations, the kinematic distance is adopted for this source.

(b)

For this source no Herschel Hi-GAL data are available, and the source luminosity has been estimated on the basis of archival mid-infrared (WISE and MSX) and far-infrared (IRAS) fluxes. Values which might be severe upper limits are enclosed within brackets.

(c)

This source is thought to belong to the Hii region complex W42, whose distance has been recently determined by us using 6.7 GHz methanol maser, BeSSeL data (not yet published).

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