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Table 4

Compilation of astrometric measurements for the HD 160934 system.

Relative positions of HD 160934 A HD 160934 c
Epoch Instrument Δα (mas) Δδ (mas) Reference

1998.496 HST/NICMOS (IR) 154.3 ± 0.9 14.8 ± 0.5 (1)
2005.296 Gemini (IR) 212.9 ± 2.0 5.6 ± 2.6 (2)
2006.518 AstraLux (IR) 214.9 ± 1.0 3.4 ± 1.0 (1)
2006.712 Gemini (IR) 217.9 ± 2.0 4.9 ± 2.6 (2)
2008.477 Palomar (IR) 169.1 ± 0.3 9.7 ± 0.3 (3)
2010.318 Keck (IR) 64.6 ± 0.3 18.9 ± 0.3 (3)
2011.310 Keck (IR) 6.3 ± 0.3 18.9 ± 0.3 (3)
2012.830 EVN (radio) 22.3 ± 0.1 6.2 ± 0.2 (4)
2014.175 EVN (radio) 149.3 ± 0.1 12.9 ± 0.2 (4)
2015.887 AstraLux (IR) 225.7 ± 3.0 11.8 ± 3.0 (4)

Absolute positions of HD 160934 (EVN)
Epoch Component RA (h m s) Dec (°′′)

2012.830 A 17 38 39.59830 ± 0.00014 61 14 16.6077 ± 0.0005 (4)
c 17 38 39.60138 ± 0.00014 61 14 16.6015 ± 0.0005 (4)
2013.392 A 17 38 39.60667 ± 0.00016 61 14 16.6865 ± 0.0007 (4)
2014.175 A 17 38 39.61159 ± 0.00013 61 14 16.6882 ± 0.0005 (4)
c 17 38 39.59090 ± 0.00013 61 14 16.6753 ± 0.0005 (4)

Notes. (1) Hormuth et al. (2007); (2) Lafrenière et al. (2007); (3) Evans et al. (2012); (4) this work. The standard deviation of the relative position corresponds to the S/N-based uncertainty of the peaks of brightness of HD 160934 A and c. The absolute positions were obtained with reference to the IERS coordinate of the external quasar J1746+6226 (). The standard deviation of the absolute position includes, in addition to the uncertainty of the peak of brightness, the contribution of the propagation media and the reference source structure.

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