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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 28.119.8+61.8$\[28.1_{-19.8}^{+61.8}\]$
TWA 28 2400 ± 100 2.90 ± 0.24 4.0 ± 0.5 32.022.2+67.0$\[32.0_{-22.2}^{+67.0}\]$
BT-Settl
TWA 27A 2605 ± 100 2.70 ± 0.20 4.0 ± 0.5 29.319.8+62.8$\[29.3_{-19.8}^{+62.8}\]$
TWA 28 2577 ± 100 2.55 ± 0.19 4.0 ± 0.5 26.016.9+53.5$\[26.0_{-16.9}^{+53.5}\]$

This work
0.97–5.27 μm
TWA 27A 2692 ± 3 3.08 ± 0.01 4.32 ± 0.03 80.55.6+6.6$\[80.5_{-5.6}^{+6.6}\]$
TWA 28 2594 ± 2 3.10 ± 0.01 4.44 ± 0.02 105.74.3+5.4$\[105.7_{-4.3}^{+5.4}\]$
1.63–5.27 μm
TWA 27A 3.11 ± 0.01 3.64 ± 0.04 16.91.2+1.4$\[16.9_{-1.2}^{+1.4}\]$
TWA 28 3.06 ± 0.01 3.88 ± 0.05 28.62.3+3.3$\[28.6_{-2.3}^{+3.3}\]$

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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