Table 1
Derived companion parameters and stellar association membership from the literature.
| Object | Member | Age [Myr] | log L/L⊙ [dex] | log LG/L⊙ [dex] | Δ [σG] | Mdyn [MJup] | Mevo [MJup] | Refs. |
|---|---|---|---|---|---|---|---|---|
| BD+70 260 b | FIELD | – | – | ![]() |
– | – | – | 1 |
| 51 Eri b | BPMG | ![]() |
![]() |
![]() |
1.0 | – | ![]() |
1,2,3 |
| AF Lep b | BPMG | ![]() |
![]() |
![]() |
0.3 | ![]() |
![]() |
1,3,4 |
| β Pic b | BPMG | ![]() |
![]() |
![]() |
0.4 | ![]() |
![]() |
1,3,5,6 |
| β Pic c | BPMG | ![]() |
![]() |
![]() |
0.6 | ![]() |
![]() |
1,3,5,6 |
| CD-35 2722 b | ABDMG | ![]() |
– | ![]() |
– | – | ![]() |
1,3 |
| GQ Lup b | UCL | ![]() |
−2.16 | ![]() |
2.6 | – | ![]() |
1,7,8 |
| HD 984 b | FIELD | ![]() |
![]() |
![]() |
0.7 | ![]() |
![]() |
1,5 |
| HD 1160 b | FIELD | ![]() |
![]() |
![]() |
2.2 | – | ![]() |
1,9,10 |
| HD 4113 c | FIELD | ![]() |
– | ![]() |
– | ![]() |
![]() |
1,11 |
| HD 4747 b | FIELD | ![]() |
![]() |
![]() |
0.4 | ![]() |
![]() |
1,12 |
| HD 13724 b | FIELD | ![]() |
![]() |
![]() |
0.6 | ![]() |
![]() |
1,13 |
| HD 17155 b | FIELD | – | – | ![]() |
– | ![]() |
– | 1,14 |
| HD 72946 b | FIELD | ![]() |
![]() |
![]() |
1.1 | ![]() |
![]() |
1,15 |
| HD 95086 b | LCC | ![]() |
![]() |
![]() |
0.5 | – | ![]() |
1,16 |
| HD 112863 b | FIELD | ![]() |
![]() |
![]() |
0.0 | ![]() |
– | 1,17,18 |
| HD 167665 b | FIELD | ![]() |
![]() |
![]() |
0.0 | ![]() |
![]() |
1,19 |
| HD 206505 b | FIELD | ![]() |
![]() |
![]() |
1.2 | ![]() |
– | 1,17,18 |
| HD 206893 b | ARG | ![]() |
![]() |
![]() |
0.1 | ![]() |
– | 1,20 |
| HD 206893 c | ARG | ![]() |
![]() |
![]() |
0.0 | ![]() |
– | 1,20 |
| HIP 64892 b | LCC | ![]() |
![]() |
![]() |
0.8 | – | ![]() |
1,21,22 |
| HIP 65426 b | LCC | ![]() |
![]() |
![]() |
1.0 | – | ![]() |
1,21,23 |
| HIP 75056 b | UCL | ![]() |
![]() |
![]() |
0.7 | ![]() |
![]() |
1,21,24 |
| HIP 79098 b | USCO | ![]() |
– | ![]() |
– | – | ![]() |
1,21 |
| HIP 99770 b | ARG | ![]() |
![]() |
![]() |
1.5 | ![]() |
![]() |
1,25,26 |
| HR 2562 b | FIELD | ![]() |
– | ![]() |
– | – | ![]() |
1,27 |
| HR 3549 b | FIELD | ![]() |
– | ![]() |
– | – | ![]() |
1,28 |
| HR 7672 b | FIELD | ![]() |
![]() |
![]() |
2.8 | ![]() |
![]() |
1,12 |
| HR 8799 b | COL | ![]() |
![]() |
![]() |
1.0 | – | ![]() |
1,13,29 |
| HR 8799 c | COL | ![]() |
![]() |
![]() |
1.4 | – | ![]() |
1,13,29 |
| HR 8799 d | COL | ![]() |
![]() |
![]() |
0.4 | – | ![]() |
1,13,29 |
| HR 8799 e | COL | ![]() |
![]() |
![]() |
2.2 | ![]() |
![]() |
1,13,29 |
| μ2 Sco b | UCL | ![]() |
– | ![]() |
– | – | ![]() |
1,21 |
| PDS 70 b | UCL | ![]() |
![]() |
![]() |
0.3 | – | ![]() |
1,30,31 |
| PDS 70 c | UCL | ![]() |
![]() |
![]() |
1.7 | – | ![]() |
1,30,31 |
| PZ Tel b | BPMG | ![]() |
– | ![]() |
– | – | ![]() |
1,3 |
| HD 135344 Ab | UCL | ![]() |
![]() |
![]() |
0.2 | – | ![]() |
1,21,32 |
| WT 766 b | FIELD | ![]() |
– | ![]() |
– | ![]() |
– | 1,33 |
| YSES 1 b | LCC | ![]() |
![]() |
![]() |
0.3 | – | ![]() |
1,21,34 |
Notes. L is the luminosity from the literature and LG is the luminosity derived from the GRAVITY spectra. ∆ is their difference in units of standard deviations of the GRAVITY-derived luminosity σG. An additional systematic uncertainty of 10% (~0.05 dex) has been added in quadrature to the GRAVITY-derived luminosity to account for flux calibration errors. Mdyn is the dynamical mass from the literature and Mevo is the mass derived from evolutionary models based on the GRAVITY luminosity. (1) Gagné et al. 2018, (2) Brown-Sevilla et al. 2023, (3) Bell et al. 2015, (4) Balmer et al. 2025, (5) Franson et al. 2022, (6) Lacour et al. 2021, (7) Donati et al. 2012, (8) Stolker et al. 2021, (9) Maire et al. 2016, (10) Sutlieff et al. 2024, (11) Cheetham et al. 2018b, (12) Brandt et al. 2019, (13) Brandt et al. 2021, (14) Unger et al. 2023, (15) Balmer et al. 2023, (16) Mâlin et al. 2024, (17) Rickman et al. 2024, (18) Ceva et al. 2025, (19) Maire et al. 2024, (20) Hinkley et al. 2023, (21) Pecaut & Mamajek 2016, (22) Cheetham et al. 2018a, (23) Carter et al. 2023, (24) Balmer et al. 2024, (25) Currie et al. 2023b, (26) Winterhalder et al. (2025), (27) Mesa et al. 2018, (28) Mesa et al. 2016, (29) Nasedkin et al. 2024, (30) Müller et al. 2018, (31) Wang et al. 2021, (32) Stolker et al. 2025, (33) Winterhalder et al. 2024, (34) Bohn et al. 2020.
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