Table 11.
Known substellar companions with a confirmed mass in the planetary and brown dwarf regime, respectively.
| Gaia DR3 | Name | ℳc sin i | ℳc | i | Plit | PGaia | elit | eGaia | a0 | Refs. |
|---|---|---|---|---|---|---|---|---|---|---|
| (ℳJup) | (ℳJup) | (deg) | (days) | (days) | (mas) | |||||
| 6421118739093252224 | HD 175167 b | 7.8 ± 3.5 | 9.5 ± 0.9 | 28 ± 19 | 1290 ± 22 | 898 ± 198 | 0.54 ± 0.09 | 0.19 ± 0.12 | 0.22 ± 0.02 | 1 |
| 4062446910648807168 | HD 164604 b | 2.7 ± 1.3 | 14.3 ± 5.5 | 29 ± 19 | 606 ± 9 | 615 ± 12 | 0.24 ± 0.14 | 0.61 ± 0.34 | 0.56 ± 0.22 | 1, 2 |
| 1594127865540229888 | HD 132406 b | 5.6 | 6.7 ± 2.1 | 122 ± 14 | 974 ± 39 | 893 ± 251 | 0.34 ± 0.09 | 0.31 ± 0.29 | 0.16 ± 0.04 | 3 |
| 4745373133284418816 | HR 810 b | 2.26 ± 0.18 | 6.2 ± 0.5 | 87 ± 6 | 312 ± 5 | 332 ± 6 | 0.15 ± 0.05 | 0.04 ± 0.2 | 0.30 ± 0.02 | 4, 5 |
| 2367734656180397952 | BD −17 0063 b | 5.1 ± 0.12 | 4.3 ± 0.5 | 80 ± 6 | 656 ± 0.6 | 649 ± 36 | 0.54 ± 0.005 | 0.28 ± 0.22 | 0.22 ± 0.02 | 6 |
| 5855730584310531200 | HD 111232 b | 6.8 | 8.3 ± 0.6 | 97 ± 4 | 1143 ± 14 | 882 ± 34 | 0.20 ± 0.01 | 0.50 ± 0.10 | 0.51 ± 0.03 | 7 |
| 637329067477530368 | HD 81040 b | 6.8 ± 0.7 | 7.9 ± 0.9 | 108 ± 6 | 1002 ± 7 | 851 ± 113 | 0.53 ± 0.04 | 0.37 ± 0.15 | 0.39 ± 0.03 | 8 |
| 4976894960284258048 | HD 142 b | 1.3 ± 0.2 | 7.1 ± 1.0 | 59 ± 7 | 350 ± 4 | 319 ± 7 | 0.26 ± 0.18 | 0.26 ± 0.23 | 0.21 ± 0.03 | 5, 9, 10 |
| 2603090003484152064 | GJ 876 b | 2.1 ± 0.2 | 3.6 ± 0.4 | 101 ± 8 | 61.08 ± 0.01 | 61.4 ± 0.2 | 0.027 ± 0.002 | 0.16 ± 0.15 | 0.43 ± 0.05 | 11–18 |
| 2651390587219807744 | BD −00 4475 b | 25 ± 2 | 48.4 ± 7.6 | 129 ± 7 | 723.2 ± 0.7 | 780 ± 84 | 0.39 ± 0.01 | 0.48 ± 0.11 | 1.91 ± 0.28 | 19 |
| 2778298280881817984 | HD 5433 b | 49 ± 3 | 53.8 ± 1.7 | 12 ± 39 | 576.6 ± 1.6 | 576.7 ± 10.6 | 0.81 ± 0.02 | 0.46 ± 0.12 | 1.04 ± 0.03 | 19 |
| 3309006602007842048 | HD 30246 b |  |
40.6 ± 8.3 | 78 ± 2 | 990 ± 6 | 814 ± 141 | 0.84 ± 0.08 | 0.59 ± 0.10 | 1.34 ± 0.24 | 19 |
| 3750881083756656128 | HD 91669 b | 30.6 ± 2.1 | 43.2 ± 2.2 | 58 ± 3 | 497.5 ± 0.6 | 500.4 ± 6.9 | 0.448 ± 0.002 | 0.32 ± 0.06 | 0.73 ± 0.04 | 19 |
| 3751763647996317056 | HD 89707 b |  |
82.5 ± 12.7 | 54 ± 10 | 298.5 ± 0.1 | 297 ± 2 | 0.90 ± 0.04 | 0.68 ± 0.20 | 1.82 ± 0.30 | 19 |
| 685029558383335168 | HD 77065 b | 41 ± 2 | 64.2 ± 5.1 | 42 ± 3 | 119.113 ± 0.003 | 119.1 ± 0.2 | 0.694 ± 0.0004 | 0.70 ± 0.04 | 1.04 ± 0.07 | 20 |
| 855523714036230016 | HD 92320 b | 59.4 ± 4.0 | 70 ± 3.1 | 111 ± 2 | 145.4 ± 0.01 | 145.1 ± 0.3 | 0.323 ± 0.001 | 0.26 ± 0.05 | 0.82 ± 0.01 | 20 |
| 824461960796102528 | HD 82460 b | 73.2 ± 3.0 | 62.5 ± 6.4 | 66 ± 1 | 590.9 ± 0.2 | 579 ± 6 | 0.84 ± 0.01 | 0.73 ± 0.04 | 1.63 ± 0.09 | 21 |
| 873616860770228352 | BD +29 1539 b | 59.7 ± 2.0 | 60.7 ± 23.5 | 120 ± 9 | 175.87 ± 0.01 | 173 ± 3 | 0.275 ± 0.001 | 0.43 ± 0.12 | 0.61 ± 0.14 | 21 |
| 5563001178343925376 | HD 52756 b | 59.3 ± 2.0 | 61.2 ± 8.6 | 73 ± 4 | 52.8657 ± 0.0001 | 52.9 ± 0.1 | 0.678 ± 0.0003 | 0.54 ± 0.16 | 0.54 ± 0.08 | 22 |
References. (1) Arriagada et al. (2010); (2) Feng et al. (2019); (3) da Silva et al. (2007); (4) Kürster et al. (2000); (5) Butler et al. (2006); (6) Moutou et al. (2009); (7) Mayor et al. (2004); (8) Sozzetti et al. (2006); (9) Tinney et al. (2002); (10) Wittenmyer et al. (2012); (11) Trifonov et al. (2018); (12) Rivera et al. (2005); (13) Rivera et al. (2010); (14) Benedict et al. (2002); (15) Marcy et al. (1998); (16) Marcy et al. (2001); (17) Correia et al. (2010); (18) Nelson et al. (2016); (19) Dalal et al. (2021); (20) Wilson et al. (2016); (21) Kiefer et al. (2019); (22) Sahlmann et al. (2011).
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