Table 1
Candidates with logarithmic odds ratio greater than zero under the parallax and proper motion model, sorted by decreasing log10 rcb(µ, ϖ) (Eq. (2)).
| Host Star | Host Star | Candidate ID | Ks-band | Nobs | ∆tobs | log10 rcb (µ) | log10 rcb(µ, ϖ) |
|---|---|---|---|---|---|---|---|
| (mag) | (yr) | ||||||
| HIP 71865 | bCen | b (1oh0dfaj) | 17.17 | 3 | 20.9 | 15.78 | ≥300 |
| HIP 61257 | HD 109195 | ‘B’ (58pwu3dv) | 12.81 | 3 | 2.8 | 1.81 | ≥300 |
| HIP 81208 | HD 149274 | B | 13.63 | 2 | 2.7 | -2.71 | 91.66 |
| HIP 82545 | µ2 Sco | b (snojiu5b) | 16.08 | 2 | 3.1 | 8.00 | 51.36 |
| HIP 81208 | HD 149274 | C | 12.56 | 2 | 2.7 | 2.29 | 42.58 |
| HIP 52742 | HD 93563 | x9ld1uh0 | 12.03 | 2 | 1.1 | 1.57 | 12.56 |
| HIP 76048 | HD 138221 | vslvj1zp | 14.50 | 2 | 0.2 | 1.42 | 2.00 |
| HIP 60009 | ζ Cru | rtolbhl8 | 20.49 | 2 | 1.0 | 0.07 | 0.32 |
| HIP 62327 | HD 110956 | n1ik1oif | 19.64 | 2 | 1.0 | 0.08 | 0.30 |
| HIP 69011 | HD 123247 | 962kt2vw | 18.16 | 2 | 0.2 | 0.81 | 0.26 |
| HIP 60009 | ζ Cru | ebmx222k | 19.97 | 2 | 1.0 | 0.05 | 0.18 |
| HIP 74100 | HD 133937 | ldj61i8l | 19.97 | 2 | 1.0 | 0.08 | 0.18 |
| HIP 52742 | HD 93563 | mm9uw3ha | 19.49 | 2 | 1.1 | 0.01 | 0.16 |
| HIP 60009 | ζ Cru | qhsttxkw | 20.14 | 2 | 1.0 | 0.03 | 0.15 |
| HIP 60009 | ζ Cru | n41zi1pt | 19.51 | 2 | 1.0 | 0.04 | 0.15 |
| HIP 60009 | ζ Cru | 4lh805ve | 18.85 | 2 | 1.0 | 0.06 | 0.14 |
| HIP 60009 | ζ Cru | a7214wz3 | 19.39 | 2 | 1.0 | 0.09 | 0.12 |
| HIP 60009 | ζ Cru | 5o2rkr75 | 20.11 | 2 | 1.0 | 0.05 | 0.10 |
| HIP 60009 | ζ Cru | d9oco7ww | 19.01 | 2 | 1.0 | 0.17 | 0.07 |
| HIP 60009 | ζ Cru | gtartoxk | 19.23 | 2 | 1.0 | 0.12 | 0.06 |
Notes. Those candidates with logarithmic odds ratio above 1.0 we identify as likely companions (in bold face). The column ‘Candidate ID’ contains unique identifier strings assigned to each candidate by Janson et al. (2021b) in most cases, and/or the commonly accepted companion name (‘B’ referring to a very probable stellar-mass companion). Here we show the first 20 candidates. The full table including results for 263 candidates (including six candidates published in Viswanath et al. 2023 that did not have follow-up when our list was compiled) is available at the CDS.
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