Table 6
ExoDNN closest-candidates prediction.
| Name | Alt. name | Gaia designation | Parallax[mas] | Sp Type | ruwe | ε [mas] | p̂ |
|---|---|---|---|---|---|---|---|
| G 158-27 | GJ 1002 | Gaia DR3 2441630500517079808 | 206.35 | M 5.5 V7 | 1.34 | 0.36 | 0.29 |
| CD Cet | GJ 1057 | Gaia DR3 3179036008830848 | 116.28 | M4.5V8 | 1.45 | 0.35 | 0.27 |
| Wolf 1069 | GJ 1253 | Gaia DR3 2188318517720321664 | 104.44 | dM5.06 | 1.42 | 0.31 | 0.33 |
| LP 732−35 | GJ 3668 | Gaia DR3 3560746351897773952 | 86.90 | M4.5 V1 | 1.90 | 0.36 | 0.52 |
| CC Eri | GJ 103 | Gaia DR3 4946938113149426944 | 86.61 | K7.V C10 | 2.26 | 0.38 | 0.33 |
| G 41−8 | − | Gaia DR3 605079910398496640 | 85.80 | M6.0V2 | 1.12 | 0.20 | 0.35 |
| VV Lyn A | GJ 277A | Gaia DR3 898506093171335424 | 83.38 | M 4.5 V1 | 2.51 | 0.41 | 0.37 |
| HD 304043 | GJ 442 | Gaia DR3 5339892367684811520 | 78.89 | M 3.5 V1 | 1.01 | 0.34 | 0.31 |
| RX J1935.4+3746 | − | Gaia DR3 2051984436005124480 | 69.12 | M3.0V3 | 2.20 | 0.42 | 0.50 |
| θ Boo B | GJ 549 B | Gaia DR3 1604859408265509632 | 68.81 | M 2.5 V4 | 1.15 | 0.35 | 0.36 |
| G 268-38 | GJ 3053 | Gaia DR3 2371032916186181760 | 66.83 | M 4.5 V1 | 1.53 | 0.28 | 0.29 |
| HD 52698 | GJ 259 | Gaia DR3 2920772722738017920 | 67.80 | K 1. V B5 | 13.03 | 2.16 | 0.99 |
| LP 491-51 | - | Gaia DR3 3968118399284369280 | 65.84 | M3.0V3 | 3.17 | 0.54 | 0.43 |
Notes. ruwe and astrometric_excess_noise ε values are from Gaia DR3 main source table. The column p̂, is the probability computed by ExoDNN that the given source hosts a detectable companion. (1) Reid et al. (1995); (2) Newton et al. (2014); (3) Shkolnik et al. (2009); (4) Alonso-Floriano et al. (2015); (5) Torres et al. (2006); (6) Schweitzer et al. (2019); (7) Shan et al. (2024); (8) Lépine et al. (2013); (9) Keenan & McNeil (1989); (10) Torres et al. (2006).
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