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Table D.1
Same as Table 2, but for the spectral energy distribution fit of β Pic b.
| Model | Teff | log g | R |
|
MS.E. | RS.E. |
| (K) | (cm s-2) | (RJup) | (MJup) | (RJup) | ||
|
|
||||||
| Settl 10 | 1600 | 4.0 | 1.57 | 0.82 | 8 |
1.4 ± 0.1 |
| Settl 13-M/H = −0.5 | 1800 | 3.5 | 1.24 | 1.34 | 2 |
1.1 ± 0.1 |
| Settl 13-M/H = 0.0 | 1800 | 4.0 | 1.26 | 1.42 | 5 |
1.1 ± 0.1 |
| Settl 13-M/H = +0.5 | 1700 | 5.0 | 1.61 | 0.64 |
|
1.3 ± 0.1 |
| DP-M/H = −0.5 | 1700 | 4.0 | 1.43 | 0.38 | 6 |
1.3 ± 0.1 |
| DP-M/H = 0.0 | 1800 | 4.5 | 1.27 | 0.52 | 16 |
1.1 ± 0.1 |
| DP-M/H = +0.5 | 1800 | 4.5 | 1.34 | 0.66 | 16 |
1.1 ± 0.1 |
| LESIA − I | 1600 | 2.1 | 1.58 | 2.38 | 0.1 ± 0.1 | 1.4 ± 0.1 |
| LESIA - II | 1400 | 5.5 | 1.95 | 0.66 | 441 |
1.9 ± 0.1 |
| LESIA − III | 1500 | 3.8 | 1.76 | 0.50 | 7 |
1.6 ± 0.1 |
| LESIA − IV | 1500 | 3.2 | 1.78 | 0.60 | 1.7 |
1.6 ± 0.1 |
| LESIA − V | 1600 | 4.1 | 1.56 | 0.72 | 10  |
1.4 ± 0.1 |
Notes. The semi-empirical radius RS.E. derived from Teff and the bolometric luminosity can be compared with the radius inferred from the synthetic spectral fitting (R).
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