Table A.5
Evolutionary model predictions for the SINFONI Library.
| Name | Mass (MJup) | Teff (K) | log (ɡ) (dex) | Radius (RJup) | ||||
|---|---|---|---|---|---|---|---|---|
| cond | dusty | cond | dusty | cond | dusty | cond | dusty | |
| 2M 0103 AB b | 10.5 ± 1.1 | 12.6 ± 2.1 | 1731 ± 96 | 1801 ± 193 | 4.04 ± 0.03 | 4.07 ± 0.05 | 1.54 ± 0.03 | 1.63 ± 0.05 |
| AB Pic b | 9.4 ± 1.1 | 10.5 ± 2.1 | 1635 ± 99 | 1608 ± 72 | 4.01 ± 0.03 | 4.02 ± 0.04 | 1.51 ± 0.03 | 1.58 ± 0.10 |
| CAHA Tau 1 | 5.2 ± 1.1 | 12.6 ± 2.1 | 1901 ± 154 | 2036 ± 164 | 3.47 ± 0.03 | 3.96 ± 0.05 | 2.09 ± 0.15 | 1.85 ± 0.07 |
| CD-35 2722 b | 7.3 ± 1.1 | 7.3 ± 1.1 | 1668 ± 125 | 1668 ± 125 | 3.84 ± 0.04 | 3.84 ± 0.04 | 1.62 ± 0.05 | 1.62 ± 0.05 |
| DH Tau b | 8.4 ± 1.1 | 8.4 ± 1.1 | 2159 ± 61 | 2159 ± 61 | 3.52 ± 0.00 | 3.52 ± 0.01 | 2.51 ± 0.16 | 2.51 ± 0.16 |
| FU Tau b | 15.7 ± 3.1 | 21.0 ± 5.2 | 2400 ± 79 | 2544 ± 94 | 3.54 ± 0.00 | 3.79 ± 0.16 | 3.36 ± 0.37 | 2.89 ± 0.12 |
| HIP 78530 b | 31.4 ± 10.5 | 31.4 ± 10.5 | 2622 ± 180 | 2667 ± 180 | 3.97 ± 0.03 | 4.05 ± 0.08 | 2.88 ± 0.46 | 2.63 ± 0.26 |
| HR 7329 b | 21.0 ± 5.2 | 21.0 ± 5.2 | 2442 ± 254 | 2487 ± 319 | 3.94 ± 0.10 | 3.97 ± 0.08 | 2.42 ± 0.55 | 2.36 ± 0.50 |
| KPNO Tau 1 | 21.0 ± 5.2 | 21.0 ± 5.2 | 2452 ± 188 | 2504 ± 250 | 3.90 ± 0.06 | 3.93 ± 0.05 | 2.54 ± 0.48 | 2.48 ± 0.47 |
| KPNO Tau 4 | 31.4 ± 10.5 | 21.0 ± 5.2 | 2616 ± 164 | 2504 ± 250 | 3.80 ± 0.11 | 3.93 ± 0.05 | 3.53 ± 0.99 | 2.48 ± 0.47 |
| KPNO Tau 6 | 21.0 ± 5.2 | 21.0 ± 5.2 | 2452 ± 188 | 2504 ± 250 | 3.90 ± 0.06 | 3.93 ± 0.05 | 2.54 ± 0.48 | 2.48 ± 0.47 |
| USco 1606 2219 | 12.6 ± 2.1 | 15.7 ± 3.1 | 1915 ± 184 | 2168 ± 367 | 4.08 ± 0.04 | 4.05 ± 0.02 | 1.61 ± 0.07 | 1.87 ± 0.24 |
| USco 1606 2230 | 31.4 ± 10.5 | 31.4 ± 10.5 | 2622 ± 180 | 2667 ± 180 | 3.97 ± 0.03 | 4.05 ± 0.08 | 2.88 ± 0.46 | 2.63 ± 0.26 |
| USco 1606 2335 | 15.7 ± 3.1 | 15.7 ± 3.1 | 2188 ± 273 | 2168 ± 367 | 4.05 ± 0.04 | 4.05 ± 0.02 | 1.87 ± 0.26 | 1.87 ± 0.24 |
| USco 1607 2239 | 12.6 ± 2.1 | 12.6 ± 2.1 | 1915 ± 184 | 1801 ± 193 | 4.08 ± 0.04 | 4.07 ± 0.05 | 1.61 ± 0.07 | 1.63 ± 0.24 |
| USco 1608 2232 | 15.7 ± 3.1 | 15.7 ± 3.1 | 2188 ± 273 | 2168 ± 367 | 4.05 ± 0.04 | 4.05 ± 0.02 | 1.87 ± 0.26 | 1.87 ± 0.24 |
| USco 1608 2335 | 15.7 ± 3.1 | 15.7 ± 3.1 | 2188 ± 273 | 2168 ± 367 | 4.05 ± 0.04 | 4.05 ± 0.02 | 1.87 ± 0.26 | 1.87 ± 0.24 |
| USco 1610 2239 | 21.0 ± 5.2 | 21.0 ± 5.2 | 2442 ± 254 | 2487 ± 319 | 3.94 ± 0.10 | 3.97 ± 0.08 | 2.42 ± 0.55 | 2.36 ± 0.50 |
| USco 1612 2156 | 12.6 ± 2.1 | 12.6 ± 2.1 | 1915 ± 184 | 1801 ± 193 | 4.08 ± 0.04 | 4.07 ± 0.05 | 1.61 ± 0.07 | 1.63 ± 0.24 |
| USco 1613 2124 | 12.6 ± 2.1 | 12.6 ± 2.1 | 1915 ± 184 | 1801 ± 193 | 4.08 ± 0.04 | 4.07 ± 0.05 | 1.61 ± 0.07 | 1.63 ± 0.24 |
| USco CTIO 108 A | 12.6 ± 2.1 | 12.6 ± 2.1 | 1915 ± 184 | 1801 ± 193 | 4.08 ± 0.04 | 4.07 ± 0.05 | 1.61 ± 0.07 | 1.63 ± 0.24 |
Notes: We report the masses, effective temperatures, surface gravities, and radii for all our targets using the BHAC15 COND03 and DUSTY00 models (Baraffe et al. 2015). The predictions are based on the SPHERE IRDIS K12 2 filter. For these calculations we used the ages, which are taken from Table A.2, and the absolute magnitudes taken from Table A.3, which were derived using the distances from Table A.2 and the apparent magnitudes from Table A.3.
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