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Table 4
Physical parameters associated with solar metallicity best fitting models explored in this article that are consistent with absolute flux and substellar evolution models constraints.
| Model type | Teff (K) | log g | log (Lbol/L⊙) | Extinction (AK) | M (MJup)1 | Compatible age (Myr)1 | Reduced χ2 |
|
|
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| ExoREM | 1200 | 4.2 | –4.4 | none | 10–13 | 50–100 | 1.58 |
| ExoREM | 1300 | 4.4 | –4.3 | none | 12–20 | 100–200 | 0.98 |
| ExoREM | 1400 | 5.0 | –4.5 | none | 35–40 | 600–700 | 1.27 |
|
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| Extincted BT-Settl | 1650 | 4.5 | –4.02 | 0.66 | 20–25 | ~100 | 0.41 |
| Extincted BT-Settl | 1700 | 5.0 | –4.12 | 0.59 | 35–40 | 300–400 | 0.51 |
Notes.
(1)
Mass and age are estimated using Baraffe et al. (2003) evolutionary models.
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