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Table F.1.

Astrometric parameters of the identified runaway candidates.

Star α [h m s] δ [d m s] π [mas] μ α Mathematical equation: $ \mu_{\alpha}^{*} $ [mas/yr] μδ [mas/yr] vrad [km/s] Ref. vrad
λ CMa 06 28 10.1906 -32 34 47.8387 7.41±0.11 -13.78±0.10 25.46±0.11 41.00±4.10 (2)
HD 160093 17 39 28.7275 -32 12 26.3260 2.16±0.02 -1.00±0.02 -5.88±0.02 39.23±2.58 (3)
66 Eri 05 06 45.6628 -04 39 18.6093 10.73±0.11 9.31±0.11 -0.52±0.08 32.60±2.80 (2)
γ Gru 21 53 55.6541 -37 21 53.3624 15.45±0.67 98.07±0.60 -13.22±0.40 0.10±0.40 (2)
γ Crv 12 15 48.4679 -17 32 31.1413 19.78±0.81 -159.58±0.66 22.31±0.54 -4.20±2.60 (2)
α2 CVn 12 56 01.8409 +38 19 05.6862 29.60±1.04 -233.43±1.01 54.98±0.78 -4.10±0.20 (2)
β Lib 15 17 00.4718 -09 22 58.3210 17.62±0.16 -98.10±0.18 -19.65±0.15 -35.60±1.80 (2)
ζ Oph 16 37 09.5300 -10 34 01.7465 8.91±0.20 15.26±0.26 24.79±0.22 12.20±3.30 (5)

Notes. For the first three stars in this table, coordinates α and δ, parallaxes π as well as proper motions μ α Mathematical equation: $ \mu_{\alpha}^{*} $ and μδ were taken from Gaia DR3; for γ Crv and α2 CVn, the corresponding data was taken from the HIPPARCOS catalog and in the cases of γ Gru, β Lib and ζ Oph, this data was taken from van Leeuwen (2007). References for the presented radial velocities vrad are indicated by the following indices: (2): XHIP; (3): Frinchaboy & Majewski (2008); (5): Zehe et al. (2018).

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