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Table 1.

Observational details.

Source Observation Calibrator Polarization Beam size Position rms σs.−n.d Estimated absolute position using FRMAP
date angle Angle α2000 δ2000 Δαe Δδe
(°) (mas × mas) (°) () () (h :  m :  s) (° :  ′: ″) (mas) (mas)
G23.44−0.18 01 March 2014 J2202+4216a −33 ± 4 9.6 × 4.2 −26.47 3 31 +18:34:39.187 −08:31:25.441 0.8 5.4
G25.83−0.18 02 March 2014 J2202+4216b −33 ± 5 8.7 × 5.5 −8.76 4 43 +18:39:03.630 −06:24:11.163 0.8 6.0
G25.71−0.04 03 March 2014 J2202+4216c −33 ± 4 16.5 × 6.5 +4.98 3 9 +18:38:03.140 −06:24:15.453 1.7 12.3
G28.31−0.39 12 June 2014 J2202+4216c −33 ± 4 12.9 × 3.0 −44.20 3 13 +18:44:22.030 −04:17:38.304 0.6 6.3
G28.83−0.25 13 June 2014 J2202+4216c −33 ± 4 10.5 × 3.5 −36.32 4 10 +18:44:51.080 −03:45:48.494 0.4 6.4
G29.96−0.02 14 June 2014 J2202+4216c −33 ± 4 10.1 × 3.2 −39.10 4 55 +18:46:03.740 −02:39:22.299 0.3 7.8
G43.80−0.13 15 June 2014 J2202+4216c −33 ± 4 9.9 × 3.4 −30.83 7 16 +19:11:53.990 +09:35:50.300 0.3 1.0

Notes.

(a)

Calibrated using 3C286 (I = 0.39 Jy beam−1, Pl = 4.3%).

(b)

Calibrated using 3C286 (I = 0.49 Jy beam−1, Pl = 4.8%).

(c)

Calibrated using results from G23.44-0.18.

(d)

Self-noise in the maser emission channels (e.g., Sault 2012). When no circularly polarized emission is detected we consider the self-noise of the brightest maser feature.

(e)

Formal errors of the fringe rate mapping.

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