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Table 2.

Absolute position of the reference maser feature.

(1) (2) (3) (4) (6) (7) (8) (9) (10) (11)
Epoch Reference Vlsr α2000 εrms Δα(a) δ2000 Δδ(a)
maser
(km s−1) (h :  m :  s) (mas) (mas) (mas) (s) (° :  ′: ″) (mas) (″)
2014.46 VLA1.1.15 10.45 20:38:36.43399 0.003 0.006 ±0.9 ±0.00008 +42:37:34.8710 0.04 ±0.0009
2016.45 VLA1.2.07 10.92 20:38:36.43403 0.029 0.05 ±1.2 ±0.00011 +42:37:34.8667 0.04 ±0.0010
2018.44 VLA1.3.04 8.63 20:38:36.43201 0.018 0.04 ±0.9 ±0.00008 +42:37:34.8588 0.03 ±0.0009
2020.82 VLA1.4.05 9.87 20:38:36.43111 0.029 0.06 ±1.0 ±0.00009 +42:37:34.8794 0.05 ±0.0009

Notes.

(a)

The uncertainties of the absolute positions (Δα and Δδ) are obtained by adding quadratically the systematic errors (εsys = 0.028 mas), the errors due to the thermal noise (εrms), the Gaussian fit errors (εgauss), the position errors of the phase-reference source J2040+4527 (ΔαJ2040 = 0.68 mas and ΔδJ2040 = 0.80 mas), and half of the restoring beam of W75N(B) to account for the maser spots scatter of each maser features (see Table 1 and Sect. 2).

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