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Table 1

Substellar companions detected around targets within the current sample.

Companion SpT M Semimajor axis Mass q Original Updated Statistical References
MpM 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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