Table C.1.
Stellar parameters of the targets selected from the LEGACY sample.
| M | R | Age |
 |
Y | Z | Teff | L | νmax | |
|---|---|---|---|---|---|---|---|---|---|
| (M⊙) | (R⊙) | (Myr) | (g/cm3) | (%) | (%) | (K) | (L⊙) | (μHz) | |
| 16 Cyg A | 1.08 ± 0.03 | 1.226 ± 0.011 | 7079 ± 109 | 0.824 ± 0.001 | 0.26 ± 0.02 | 0.019 ± 0.001 | 5827 ± 21 | 1.56 ± 0.01 | 2203.9 ± 22.6 |
| 16 Cyg B | 1.01 ± 0.02 | 1.105 ± 0.009 | 7057 ± 111 | 1.057 ± 0.001 | 0.27 ± 0.02 | 0.017 ± 0.001 | 5788 ± 27 | 1.23 ± 0.01 | 2555.2 ± 24.5 |
| Arthur | 1.21 ± 0.03 | 1.154 ± 0.011 | 1545 ± 90 | 1.115 ± 0.004 | 0.24 ± 0.01 | 0.018 ± 0.003 | 6065 ± 62 | 1.62 ± 0.04 | 2750.7 ± 29.7 |
| Barney | 1.27 ± 0.01 | 1.610 ± 0.007 | 4059 ± 176 | 0.429 ± 0.003 | 0.30 ± 0.02 | 0.027 ± 0.002 | 5985 ± 17 | 3.00 ± 0.04 | 1487.3 ± 7.7 |
| Carlsberg | 1.21 ± 0.03 | 1.170 ± 0.011 | 2076 ± 138 | 1.065 ± 0.003 | 0.24 ± 0.02 | 0.019 ± 0.002 | 6050 ± 47 | 1.65 ± 0.03 | 2668.1 ± 27.5 |
| Doris | 1.01 ± 0.01 | 0.936 ± 0.003 | 5617 ± 125 | 1.728 ± 0.011 | 0.26 ± 0.00 | 0.030 ± 0.002 | 5237 ± 31 | 0.59 ± 0.01 | 3726.0 ± 24.5 |
| Dushera | 1.21 ± 0.03 | 1.417 ± 0.012 | 3516 ± 192 | 0.600 ± 0.002 | 0.28 ± 0.02 | 0.019 ± 0.002 | 6170 ± 32 | 2.62 ± 0.05 | 1802.1 ± 14.6 |
| Nunny | 1.06 ± 0.01 | 1.240 ± 0.004 | 5847 ± 201 | 0.783 ± 0.001 | 0.26 ± 0.01 | 0.012 ± 0.001 | 6058 ± 17 | 1.87 ± 0.02 | 2079.3 ± 7.9 |
| Pinocha | 1.33 ± 0.03 | 1.299 ± 0.010 | 1599 ± 125 | 0.855 ± 0.004 | 0.24 ± 0.01 | 0.022 ± 0.003 | 6197 ± 47 | 2.24 ± 0.04 | 2349.1 ± 22.3 |
| Saxo2 | 1.25 ± 0.02 | 1.268 ± 0.008 | 2457 ± 80 | 0.864 ± 0.003 | 0.24 ± 0.01 | 0.018 ± 0.002 | 6174 ± 34 | 2.10 ± 0.03 | 2323.6 ± 14.3 |
Notes. These are the results of the fit of the frequency separation ratios, the classical constraints (metallicity and effective temperature for all the targets, and the luminosity except for Arthur, Doris, and Pinocha), and the inverted mean density treated as a classical constraint.
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