Table 1
Substellar companions detected around targets within the current sample.
Companion | SpT | M⋆ | Semimajor axis | Mass | q | Original | Updated | Statistical | References |
---|---|---|---|---|---|---|---|---|---|
Mp∕M⋆ | priority | priority | weight | ||||||
[M⊙] | [au] | [MJup] | [%] | ||||||
New SHINE detections | |||||||||
HIP 64892 B | B9 | 2.09 | 147–171 | 29–37 | 1.3–1.7% | P1 | 1.00 | 1 | |
HIP 65426 b | A2 | 1.96 | 80–210 | 7–9 | 0.3–0.4% | P1 | 1.00 | 2, 3 | |
Previously known detections – no priority update | |||||||||
η Tel B | A0 | 2.00 | 125–432 | 20–50 | 1.0–2.4% | P1 | 1.00 | 4, 5 | |
CD -35 2722 B | M1 | 0.56 | 74–216 | 23–39 | 3.9–6.6% | P1 | 1.00 | 6, 5 | |
Previously known detections – updated priority | |||||||||
HIP 78530 B(a) | B9 | 1.99 | ~620 | 19–26 | 0.9–1.2% | P1 | P0 | 0.60 | 7 |
β Pic b | A3 | 1.61 | 8.5–9.2 | 9–16 | 0.5–0.9% | P1 | P0 | 0.60 | 8, 9 |
HR 8799 b | A5 | 1.42 | 62–72 | 5.3–6.3 | 0.3–0.4% | P1 | P0 | 0.60 | 10 |
HR 8799 c | A5 | 1.42 | 39–45 | 6.5–7.8 | 0.4–0.5% | P1 | P0 | 0.60 | 10 |
HR 8799 d | A5 | 1.42 | 24–27 | 6.5–7.8 | 0.4–0.5% | P1 | P0 | 0.60 | 10 |
HR 8799 e | A5 | 1.42 | 14–17 | 6.5–7.8 | 0.4–0.5% | P1 | P0 | 0.60 | 10 |
HD 95086 b | A8 | 1.55 | 28–64 | 2–9 | 0.1–0.6% | P1 | P0 | 0.60 | 11, 12 |
51 Eri b | F0 | 1.45 | 10–16 | 6–14 | 0.4–0.9% | P1 | P0 | 0.60 | 13, 14 |
HIP 107412 B | F5 | 1.32 | 6.2–7.1 | 15–30 | 1.1–2.2% | P4 | P0 | 0.01 | 15, 16 |
PZ Tel B | G9 | 1.07 | 19–30 | 38–54 | 3.4–4.8% | P1 | P0 | 0.60 | 17, 18 |
AB Pic B | K1 | 0.97 | ~250 | 13–30 | 1.3–3.0% | P1 | P0 | 0.60 | 19, 20 |
GSC 8047-0232 B | K2 | 0.89 | 190–880 | 15–35 | 1.6–3.8% | P2 | P0 | 0.35 | 21, 22 |
Notes. (a)With a semimajor axis of ~620 au and no additional published constraints, HIP 78530 is not taken into account into most of our simulations, which use a cutoff at 300 au.
References. (1) Cheetham et al. (2018); (2) Chauvin et al. (2017); (3) Cheetham et al. (2019); (4) Neuhäuser et al. 2011; (5) Blunt et al. (2017); (6) Wahhaj et al. (2011); (7) Lafrenière et al. (2011); (8) Dupuy et al. (2019); (9) Lagrange et al. (2019); (10) Wang et al. (2018); (11) De Rosa et al. (2016); (12) Chauvin et al. (2018); (13) Samland et al. (2017); (14) Maire et al. (2019); (15) Delorme et al. (2017b); (16) Grandjean et al. (2019); (17) Maire et al. (2016); (18) Bowler et al. (2020); (19) Chauvin et al. (2005b); (20) Bonnefoy et al. (2010); (21) Chauvin et al. (2005a); (22) Ginski et al. (2014).
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