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Table 1

Detected substellar companions to stars in the sample.

Name Subsample Date S/N sep PA H H H2 – H3 Mass SMA Source
arcsec deg mag mag mag MJup au
HD 206893 b FGK 2016-09-22 7.2 0.268 ± 0.002 61.5 ± 0.4 11.1 13.7 ± 0.1 0.5 ± 0.1 28 9.6 1,1

HR 8799 c BA 2016-09-19 37.1 0.953 ± 0.002 330.8 ± 0.2 12.5 14.8 ± 0.2 0.4 ± 0.2 8.5 41 2,2

HR 8799 d BA 2016-09-19 19.4 0.666 ± 0.002 223.5 ± 0.2 12.5 14.7 ± 0.2 0.3 ± 0.2 8.5 27 2,2

HR 8799 e BA 2016-09-19 9.2 0.393 ± 0.003 284.1 ± 0.4 12.2 14.4 ± 0.2 0.3 ± 0.2 9.6 16 3,2

2014-12-18 14.7 0.439 ± 0.002 171.3 ± 0.3 14.3 16.7 ± 0.2 −1.2 ± 0.1
2015-01-31 5.0 0.456 ± 0.007 170.4 ± 0.8 15.1
51 Eri b BA 2015-09-01 10.9 0.442 ± 0.003 166.8 ± 0.4 14.7 17.1 ± 0.2 −1.0 ± 0.2 4.1 11.1 4,5
2015-12-20 7.5 0.443 ± 0.005 166.5 ± 0.7 14.4 16.8 ± 0.2 −0.6 ± 0.2
2016-09-18 12.7 0.442 ± 0.003 162.0 ± 0.4 14.4 16.8 ± 0.1 −0.8 ± 0.1

2015-11-06 8.3 0.421 ± 0.004 359.1 ± 0.6 9.8 11.9 ± 0.2 0.4 ± 0.1
β Pic b BA 2015-12-22 7.7 0.241 ± 0.002 213.2 ± 0.4 9.6 11.7 ± 0.2 0.4 ± 0.1 11.9 9.93 6,6
2016-01-21 7.5 0.226 ± 0.002 212.3 ± 0.6 10.4 12.5 ± 0.3 0.4 ± 0.3

2013-12-11 8.9 0.635 ± 0.003 150.6 ± 0.3 13.8 15.9 ± 0.2 0.2 ± 0.2
HD 95086 b BA 2016-02-29 9.3 0.627 ± 0.003 148.1 ± 0.4 13.6 15.8 ± 0.2 0.2 ± 0.1 2.6 61.7 7,8
2016-03-06 8.1 0.626 ± 0.004 148.1 ± 0.4 14.0 16.1 ± 0.2 0.7 ± 0.2
2016-03-28 4.9 0.629 ± 0.006 147.5 ± 0.6 14.2 16.4 ± 0.2 0.0 ± 0.3

2016-01-25 17.0 0.605 ± 0.002 294.7 ± 0.3 12.8 15.3 ± 0.2 0.6 ± 0.3
HR 2562 b FGK 2017-02-13 21.4 0.635 ± 0.002 298.3 ± 0.2 11.3 13.8 ± 0.1 0.3 ± 0.1 10.28 21.2 9,9
2017-11-29 12.5 0.654 ± 0.002 297.8 ± 0.3 12.8 15.2 ± 0.2 0.4 ± 0.1
2018-11-19 28.1 0.677 ± 0.002 297.3 ± 0.2 11.3 13.7 ± 0.3 0.3 ± 0.3

HD 984 B(a) FGK 2015-08-30 0.219 ± 0.002 84.0 ± 0.4 7.7 61 28 10,10

PZ Tel B(a) FGK 2015-07-30 0.501 ± 0.002 59.5 ± 0.2 5.9 27 27 11,11

Notes. (a)Reduction through the custom cADI. (mass, sma) sources for planet properties: (1) Hinkley et al. (2023); (2) Zurlo et al. (2022); (3) Brandt et al. (2021); (4) Elliott et al. (2024); (5) De Rosa et al. (2020b); (6) Lacour et al. (2021); (7) Nielsen et al. (2019); (8) Rameau et al. (2016); (9) Zhang et al. (2023); (10) Franson et al. (2022); (11) Franson & Bowler (2023). The column named “subsample” indicates whether the parent star belongs to the FGK or the BA subsample (see Sect. 3.4).

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