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Table 1

Positions and brightnesses.

Source RA (J2000) Dec (J2000) S p θ sep PA V LSR Beam
(h m s) (° ′ ′′) (Jy/beam) (°) (°) (km s-1) (mas mas °)
(1) (2) (3) (4) (5) (6) (7) (8)

22 GHz
NML Cyg....... 20 46 25.5444 40 06 59.383 16−77 ... ... 5.22 0.6 ×  0.3 @ −08
J2052 + 3635.... 20 52 52.0550 36 35 35.300 0.050 3.7 −19 ... 2.7 ×  1.4 @ +31
J2044 + 4005.... 20 44 11.0877 40 05 36.360 0.005 0.4  +87 ... 2.7 ×  1.3 @ +25
J2046 + 4106.... 20 46 21.8414 41 06 01.107 0.014 1.0 −01 ... 2.7 ×  1.2 @ +24
J2049 + 4118.... 20 49 43.9548 41 18 14.583 0.011 1.3  +28 ... 2.7 ×  1.2 @ +26
43 GHz
NML Cyg....... 20 46 25.5378 40 06 59.413 3.4 ... ... −5.70 0.3 ×  0.1 @ −07
J2046 + 4106.... 20 46 21.8414 41 06 01.107 0.017 1.0 −01 ... 0.7 ×  0.4 @ −25

Notes. The fourth and seventh columns give the peak brightnesses (Sp) and VLSR of reference maser spot. The fifth and sixth columns give the separations (θsep) and position angles (PA) east of north of the background sources relative to the maser. The last column gives the FWHM size and PA of the Gaussian restoring beam. Calibrator J2052 + 3635 is from the VLBA Calibrator Survey (VCS) by Kovalev et al. (2007). The other calibrators are from the VLA program BZ035.

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