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Table 1

VLBI observations used in the paper.

Epoch Exp. code Telescope(a) Vel. res. (km s−1) 1σ noise (mJy beam−1) Beam (mas × mas, °) Ref.

No. Date MJD
1 2004 Nov. 06 53 315 EL032 EVN(8) 0.09 7 13.8×5.3, −57 1
2 2006 Sep. 09 53 987 JVN(4) 0.18 60 9.4×4.3, −70 2
3 2007 Jul. 28 54 309 JVN(5) 0.18 90 9.2×4.3, −43 2
4 2008 Oct. 25 54 764 JVN(5) 0.18 120 7.0×3.9, −79 2
5 2013 Mar. 01 56 352 ES071A EVN(8) 0.04 4–6 4.3×3.1, −58 3
6 2014 Feb. 28 56 716 ES071B EVN(8) 0.04 4–6 4.0×3.4, −67 3
7 2015 Mar. 13 57 094 ES071C EVN(9) 0.04 4–6 3.9×3.0, −53 3
8 2020 Jun. 02 59 002 RD002 EVN(4) 0.04 5 7.5×3.5, +86 4
9 2020 Oct. 18 59 140 ED048B EVN(8) 0.09 4 4.5×3.8,+12 4

Notes. (a) Telescopes are the EVN and the Japan VLBI Network (JVN). The number of antennas is given in parentheses.

References. (1) (Torstensson et al. 2011); (2) (Sugiyama et al. 2014); (3) (Sanna et al. 2017); (4) this work.

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