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Table 1

Observational details.

Source Observation Calibrator Polarization Beam size Position rms σs.−n. (b) Estimated absolute position using FRMAP
name (a) date angle angle α2000 δ2000 Δα (c) Δδ (c)
(°) (mas × mas) (°) () () (h :  m :  s) (° : ′ : ″) (mas) (mas)
G30.70-0.07 16 October 2014 J2202+4216 (d) + 1 ± 1 8.5 × 4.2 −40.93 2 25 +18:47:36.900 −02:01:05.025 0.4 13.1
G30.76-0.05 17 October 2014 J2202+4216 (e) + 1 ± 1 8.5 × 3.9 −36.28 5 29 +18:47:39.732 −01:57:21.975 0.3 10.2
G31.28+0.06 20 October 2015 J2202+4216 (f) − 15 ± 3 5.3 × 4.4 −66.03 3 60 +18:48:12.390 −01:26:22.629 0.8 37.4
G32.03+0.06 21 October 2015 J2202+4216 (g) − 16 ± 5 5.1 × 4.4 −76.73 3 40 +18:49:36.580 −00:45:46.891 0.2 17.5
G69.52-0.97 22 October 2015 J2202+4216 (h) − 27 ± 4 5.9 × 3.1 −67.04 2 28 +20:10:09.0699 +31:31:34.399 0.7 1.8

Notes. (a)Source name provided in Galactic coordinates. (b)Self-noise in the maseremission channels (e.g., Sault 2012). When more than one maser feature shows circularly polarized emission, we present the self-noise of the weakest feature. When no circularly polarized emission is detected, we consider the self-noise of the brightest maser feature. (c)Formal errors of the fringe-rate mapping. (d)Calibrated using results from G30.76-0.05.(e)Calibrated using 3C286 (I = 1.26 Jy beam−1, Pl = 6.5%). (f) Calibrated using 3C286 (I = 0.60 Jy beam−1, Pl = 7.7%). (g) Calibrated using 3C286 (I = 0.73 Jy beam−1, Pl = 9.0%). (h) Calibrated using 3C286 (I = 0.65 Jy beam−1, Pl = 9.2%).

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