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Table 3
K-band magnitude estimates for some potential GRAVITY follow-up targets derived using different evolutionary models: ATMO (Phillips et al. 2020), AMES-DUSTY (Chabrier et al. 2000; Allard et al. 2001), and AMES-COND (Allard et al. 2001; Baraffe et al. 2003).
| Target name | ATMO | DUSTY | COND |
|---|---|---|---|
| γ Cephei A b | 23.93 | − | 26.80 |
| HD 128311 c | 23.81 | 21.92 | 26.14 |
| GJ 504 b | 20.35 | 22.11 | 21.16 |
| HD 89839 b | 26.39 | 21.92 | 29.85 |
| HD 154345 b | − | − | − |
| 2MASS J1315-2649 b | 15.43 | 15.71 | 15.42 |
| β Pic b | 12.57 | 11.68 | 12.05 |
| HD 114783 c | − | − | 53.62 |
| AF Lep b | 15.87 | 16.82 | 15.51 |
| HD 155555 (AB) b | 15.49 | 16.23 | 15.06 |
| HD 60584 b | 15.63 | 16.04 | 15.66 |
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