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Table 4.

Brown dwarfs expected to have a full astrometric solution in future Gaia data releases.

Name Parallax Spectral
(mas) type
Luhman 16 A 501.6 ± 0.1 L7.5
Luhman 16 B 501.6 ± 0.1 T0.5
ϵ Ind C 270.7 ± 0.7 T6.0
SCR J1845–6357 B 249.7 ± 0.1 T6.0
Scholz’s Star B 147.1 ± 1.2 T5.0
SCR J1546–5534 B 119.1 ± 0.7 T6.0
2MASS J16471580+5632057 116.0 ± 29.0 L9 pec
WISE J223617.59+510551.9 102.8 ± 1.9 T5.5
CFBDS J213926+022023 A 101.5 ± 2.0 L8.5
CFBDS J213926+022023 B 101.5 ± 2.0 T3.5
2MASS J07584037+3247245 101.3 ± 3.3 T2.5
BD+16 2708 B 100.5 ± 0.1 M9

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