Table 2
Physical properties of TWA 27A and TWA 28 from different studies.
| Target | Teff (K) | Radius (RJup) | log g (cgs) | Mass (MJup) |
|---|---|---|---|---|
| Venuti et al. (2019) |
||||
| TWA 27A | 2640 ± 20 | 3.41 | 3.75 ± 0.14 | 19.9 ± 6.3 |
| TWA 28 | 2660 ± 70 | 2.82 | 4.10 ± 0.30 | 21.0 ± 5.2 |
Manjavacas et al. (2024) |
||||
| ATMO | ||||
| TWA 27A | 2600 ± 100 | 2.70 ± 0.21 | 4.0 ± 0.5 | ![]() |
| TWA 28 | 2400 ± 100 | 2.90 ± 0.24 | 4.0 ± 0.5 | ![]() |
| BT-Settl | ||||
| TWA 27A | 2605 ± 100 | 2.70 ± 0.20 | 4.0 ± 0.5 | ![]() |
| TWA 28 | 2577 ± 100 | 2.55 ± 0.19 | 4.0 ± 0.5 | ![]() |
This work |
||||
| 0.97–5.27 μm | ||||
| TWA 27A | 2692 ± 3 | 3.08 ± 0.01 | 4.32 ± 0.03 | ![]() |
| TWA 28 | 2594 ± 2 | 3.10 ± 0.01 | 4.44 ± 0.02 | ![]() |
| 1.63–5.27 μm | ||||
| TWA 27A | − | 3.11 ± 0.01 | 3.64 ± 0.04 | ![]() |
| TWA 28 | − | 3.06 ± 0.01 | 3.88 ± 0.05 | ![]() |
Notes. Effective temperature (Teff) and mass are inferred from the models, while radius and surface gravity are directly retrieved as free parameters. ATMO and BT-Settl refer to different atmospheric model grids from M24. Wavelength ranges indicate the spectral coverage: 0.97–5.27 μm includes all three NIRSpec gratings (G140H, G235H, G395H), while 1.63–5.27 μm uses only G235H and G395H.
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