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Table 3

List of stars with ΔQ> 30 in HTPM case A, with assumed radial velocities set to zero.

HIP ΔQ Hp ϖ v r μ r Δθpersp Remark
[mas ] [mas yr-1] [km s-1] [mas yr-1] [mas]

87937 8 044.46 9.490 548.31 10 358.94 − 110.51 − 12 782.22 361.87 Barnard’s star
24186 5 053.12 8.932 255.66 8 669.40 245.19 13 223.43 312.01 Kapteyn’s star
57939 686.11 6.564 109.99 7 059.03 − 98.35 − 2 281.95 43.72 Groombridge 1830
104217 618.09 6.147 285.88 5 172.58 − 64.07 − 3 863.82 54.70 61 Cyg Ba
54035 572.73 7.506 392.64 4 801.04 − 84.69 − 7 014.64 92.31
70890 229.59 10.761 771.64 3 852.57 − 22.40 − 3 646.21 38.32 Proxima Centauri
74235 76.86 9.200 34.65 3 681.26 310.12 2 266.79 24.80
439 62.69 8.618 230.42 6 100.36 25.38 1 233.65 20.64
74234 34.62 9.568 35.14 3 680.96 310.77 2 303.67 21.63
54211 30.13 8.803 206.27 4 510.10 68.89 2 997.58 36.97

Notes. The threshold 30 was set for a probability of false alarm ~ 10-5, assuming that ΔQ follows the χ2 distribution with 5 degrees of freedom. The columns contain the Hipparcos identifier, Hipparcos magnitude, parallax, and total proper motion (all from the Hipparcos Catalogue), the radial velocity from XHIP, and the calculated radial motion and positional offset over Δt = 23.75 yr due to perspective acceleration.

(a)

61 Cyg A (HIP 104214) was not included in the simulations since it is brighter than the nominal Gaia bright star limit.

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