Table 1
Projected distance and contrast values were obtained from the observations presented in the previous Table (Maire et al. 2016) (for systems with multiple observations, parameters were derived from datasets with asterisks).
| Name | Separation | Contrast | Age | Mass | Distance | Hill radius | Age references |
|---|---|---|---|---|---|---|---|
| (Myr) | (Mjup) | (pc) | (au) | ||||
| 51 Eri b | 0.45″ | 5.8 × 10−6 | 24 ± 5 |  |
29.8 | 1.2 | a |
| AB Pic B | 5.40″ | 6.4 × 10−4 |  |
 |
50.1 | 40.8 | b |
| β Pic b | 0.33″ | 1.0 × 10−4 | 24 ± 5 |  |
19.7 | 1.1 | a |
| CT Cha B | 2.68″ | 1.7 × 10−3 |  |
 |
191.8 | 78.5 | c |
| DH Tau B | 2.35″ | 4.1 × 10−3 | 1.4 ± 0.1 |  |
135.3 | 66.4 | c |
| η Tel B | 4.21″ | 1.5 × 10−3 | 24 ± 5 |  |
47.4 | 34.4 | a |
| GJ504 B | 2.49″ | 1.3 × 10−6 | 4000 ± 1800 |  |
17.5 | 7.6 | d |
| GQ Lup B | 0.70″ | 3.1 × 10−3 | 2–5 |  |
151.8 | 24.7 | e |
| HD 1160 B | 0.78″ | 8.9 × 10−4 |  |
 |
125.9 | 42.8 | f |
| HD 1160 C | 5.15″ | 4.4 × 10−3 |  |
 |
125.9 | 409.9 | f |
| HD 4747 B | 0.59″ | 6.5 × 10−4 | 2300 ± 1400 |  |
18.8 | 1.0 | g |
| HD 19467 B | 1.63″ | 2.4 × 10−5 |  |
 |
32.0 | 14.9 | h |
| HD 95086 b | 0.62″ | 9.1 × 10−6 |  |
 |
86.4 | 3.9 | i |
| HIP 64892B | 1.27″ | 1.3 × 10−3 |  |
 |
125.2 | 28.2 | j |
| HIP 65426 b | 0.83″ | 3.4 × 10−5 | 14 ± 4 |  |
109.2 | 12.1 | k |
| HIP 78530 B | 4.18″ | 7.1 × 10−4 |  |
 |
137.3 | 113.1 | l |
| HIP 107412 B | 0.27″ | 1.2 × 10−4 | 50–700 |  |
40.8 | 2.2 | m |
| HR 2562 B | 0.64″ | 2.3 × 10−5 | 200–750 |  |
34.0 | 4.3 | n |
| HR 3549 B | 0.85″ | 2.1 × 10−4 | 100–150 |  |
95.4 | 15.2 | o |
| HR 8799 b | 1.72″ | 2.8 × 10−5 |  |
 |
41.3 | 7.1 | p |
| HR 8799 c | 0.95″ | 6.9 × 10−5 |  |
 |
41.3 | 4.9 | p |
| HR 8799 d | 0.66″ | 7.2 × 10−5 |  |
 |
41.3 | 2.6 | p |
| HR 8799 e | 0.39″ | 7.6 × 10−5 |  |
 |
41.3 | 1.8 | p |
| PDS 70 b | 0.19″ | 5.5 × 10−4 | 5.4 ± 1.0 |  |
113.4 | 2.9 | q |
| PZ Tel B | 0.50″ | 3.0 × 10−3 | 24 ± 5 |  |
47.1 | 1.4 | a |
| TYC 7084-794-1 B | 2.99″ | 4.0 × 10−3 | 140 ± 40 |  |
22.4 | 19.8 | r |
| TYC 8047-232-1 B | 3.21″ | 8.0 × 10−4 |  |
 |
86.3 | 47.0 | p |
Notes. Masses were obtained using BT SETTL models and for 51 Eri b and HD 95086 b, the AMES COND models; distances were taken from the Gaia catalogue (Gaia Collaboration 2016, 2018); references for the ages are listed in the notes.
References. a: β Pic Moving Group; b: Carina Moving Group; c: Feiden (2016); d: Bonnefoy et al. (2018); e: Donati et al. (2012); f: Nielsen et al. (2012); g: Peretti et al. (2019); h: Maire et al. (in prep.); i: Desidera et al. (in prep.); j: Cheetham et al. (2018); k: Chauvin et al. (2017b); l: Upper ScoCen Moving Group; m: Delorme et al. (2017b); n: Mesa et al. (2018); o: Mesa et al. (2016); p: Columba Moving Group; q: Keppler et al. (2018); r: AB Doradus Moving Group.
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