Table 5
Comparison between parameters from ForMoSA and parameters in using evolutionary models (Chabrier et al. 2000) (BT-SETTL15/ForMoSA independent).
| ForMoSA | Bolometric correction + Evolutionary models | ||||||||
|---|---|---|---|---|---|---|---|---|---|
| Object | log (L∕L⊙) | R | log (g) | Teff | log (L∕L⊙) | R | log (g) | Teff | M |
| (RJup) | (dex) | (K) | (RJup) | (dex) | (K) | (MJup) | |||
| USco 1610-1913 B (1) |  |
 |
≤ 4.17 |  |
− 2.13 ± 0.17 | 3.6 ± 0.7 | 4.03 ± 0.20 | 2827 ± 169 | 57 ± 28 |
| HIP 77900 B (1) |  |
 |
≤ 4.36 |  |
− 2.59 ± 0.16 | 2.8 ± 0.4 | 4.02 ± 0.17 | 2611 ± 185 | 34 ± 14 |
| HIP 78530 B (1) |  |
 |
≤ 4.34 |  |
− 2.68 ± 0.17 | 2.6 ± 0.4 | 4.00 ± 0.13 | 2544 ± 179 | 28 ± 10 |
| USco 1607-2242 |  |
 |
≤ 4.10 |  |
− 3.23 ± 0.20 | 1.9 ± 0.2 | 3.99 ± 0.09 | 2044 ± 203 | 14 ± 4 |
| USco 1608-2232 |  |
 |
≤ 4.09 |  |
− 2.96 ± 0.20 | 2.1 ± 0.3 | 4.01 ± 0.06 | 2262 ± 182 | 17 ± 4 |
| USco 1606-2335 |  |
 |
≤ 4.36 |  |
− 3.05 ± 0.20 | 2.1 ± 0.2 | 4.01 ± 0.06 | 2215 ± 179 | 16 ± 4 |
| USco 1610-2239 |  |
 |
≤ 4.01 |  |
− 2.75 ± 0.20 | 2.5 ± 0.3 | 3.97 ± 0.08 | 2467 ± 173 | 24 ± 7 |
| USco 1608-2315 |  |
 |
≤ 4.16 |  |
− 2.71 ± 0.20 | 2.5 ± 0.4 | 3.98 ± 0.08 | 2474 ± 179 | 24 ± 8 |
| USco 1607-2211 |  |
 |
≤ 4.05 |  |
− 2.76 ± 0.24 | 2.5 ± 0.4 | 3.98 ± 0.09 | 2461 ± 204 | 24 ± 8 |
Notes. The luminosity has been determined using the bollometric corrections at J and K bands from Filippazzo et al. (2015). For the luminosity of our reference objects we directly use the Filippazzo et al. (2015) values. We also provide the mass values. (1) With the hypothesis that companions are at the same distance as the primary star.
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