Table 2
Bayesian mass and age estimates for stars in detached eclipsing binary star systems (⟨ M⋆ ⟩) compared to the mass of the stars directly measured from observations (Mobs).
| Star | P orb | T eff | [ Fe/H ] s | ρ ⋆ | M obs | ⟨ M⋆ ⟩ | |
| [d] | [K] | [ρ⊙] | [M⊙] | [M⊙] | Ref. | ||
|
|
|||||||
| WOCS 40007 A | 3.18 | 6240 ± 90 | 0.09 ± 0.03 | 0.451 ± 0.010 | 1.236 ± 0.020 | 1.243 ± 0.038 | 1 |
| WOCS 40007 B | 5960 ± 150 | 0.820 ± 0.016 | 1.086 ± 0.018 | 1.102 ± 0.056 | 1 | ||
| CD Tau A | 3.43 | 6190 ± 60 | 0.08 ± 0.15 | 0.248 ± 0.008 | 1.442 ± 0.016 | 1.326 ± 0.079 | 2 |
| CD Tau B | 6190 ± 60 | 0.344 ± 0.014 | 1.368 ± 0.016 | 1.266 ± 0.072 | 2 | ||
| CO And A | 3.65 | 6140 ± 130 | 0.01 ± 0.15 | 0.250 ± 0.009 | 1.289 ± 0.007 | 1.281 ± 0.090 | 3 |
| CO And B | 6160 ± 130 | 0.260 ± 0.008 | 1.264 ± 0.007 | 1.263 ± 0.092 | 3 | ||
| CoRoT 105906206 B | 3.69 | 6150 ± 160 | 0.0 ± 0.1 | 0.536 ± 0.017 | 1.29 ± 0.03 | 1.145 ± 0.071 | 4 |
| GX Gem B | 4.04 | 6160 ± 100 | −0.12 ± 0.10 | 0.131 ± 0.002 | 1.467 ± 0.010 | 1.283 ± 0.041 | 5 |
| UX Men A | 4.18 | 6190 ± 100 | 0.04 ± 0.10 | 0.500 ± 0.015 | 1.223 ± 0.001 | 1.191 ± 0.056 | 6, 7 |
| UX Men B | 6150 ± 100 | 0.574 ± 0.018 | 1.188 ± 0.001 | 1.165 ± 0.057 | 6, 7 | ||
| WZ Oph A | 4.18 | 6160 ± 100 | −0.27 ± 0.07 | 0.446 ± 0.012 | 1.227 ± 0.007 | 1.054 ± 0.052 | 8, 9 |
| WZ Oph B | 6110 ± 100 | 0.427 ± 0.011 | 1.22 ± 0.006 | 1.043 ± 0.053 | 8, 9 | ||
| V636 Cen A | 4.28 | 5900 ± 80 | −0.20 ± 0.08 | 0.997 ± 0.013 | 1.052 ± 0.005 | 0.960 ± 0.045 | 10, 11 |
| V636 Cen B | 5000 ± 100 | 1.493 ± 0.022 | 0.854 ± 0.003 | 0.762 ± 0.024 | 10, 11 | ||
| CoRoT 102918586 B | 4.39 | 7100 ± 120 | 0.11 ± 0.05 | 0.460 ± 0.013 | 1.49 ± 0.03 | 1.492 ± 0.043 | 12 |
| EK Cep B | 4.43 | 5700 ± 200 | 0.07 ± 0.05 | 0.494 ± 0.009 | 1.124 ± 0.012 | 1.017 ± 0.069 | 13 |
| YZ Cas B | 4.47 | 6890 ± 240 | 0.10 ± 0.06 | 0.562 ± 0.008 | 1.325 ± 0.007 | 1.342 ± 0.040 | 14 |
| BK Peg A | 5.49 | 6270 ± 90 | −0.12 ± 0.07 | 0.180 ± 0.002 | 1.414 ± 0.007 | 1.244 ± 0.033 | 15 |
| BK Peg B | 6320 ± 90 | 0.392 ± 0.013 | 1.257 ± 0.005 | 1.205 ± 0.047 | 15 | ||
| V785 Cep A | 6.50 | 5900 ± 100 | −0.06 ± 0.06 | 0.382 ± 0.015 | 1.103 ± 0.007 | 1.081 ± 0.059 | 16 |
| V785 Cep B | 5870 ± 100 | 0.418 ± 0.017 | 1.081 ± 0.007 | 1.053 ± 0.057 | 16 | ||
| BW Aqr B | 6.72 | 6220 ± 100 | −0.07 ± 0.11 | 0.242 ± 0.018 | 1.386 ± 0.021 | 1.262 ± 0.086 | 17 |
| EW Ori A | 6.94 | 6070 ± 100 | 0.05 ± 0.09 | 0.736 ± 0.012 | 1.173 ± 0.011 | 1.126 ± 0.051 | 18 |
| EW Ori B | 5900 ± 100 | 0.851 ± 0.014 | 1.123 ± 0.009 | 1.066 ± 0.051 | 18 | ||
| V568 Lyr A | 14.47 | 5650 ± 90 | 0.28 ± 0.05 | 0.399 ± 0.011 | 1.087 ± 0.004 | 1.138 ± 0.058 | 19 |
| V568 Lyr B | 4820 ± 150 | 1.735 ± 0.034 | 0.828 ± 0.002 | 0.832 ± 0.038 | 19 | ||
| KIC 6131659 A | 17.53 | 5790 ± 50 | −0.23 ± 0.20 | 1.353 ± 0.016 | 0.922 ± 0.007 | 0.915 ± 0.053 | 20 |
| LV Her A | 18.44 | 6210 ± 160 | 0.08 ± 0.21 | 0.476 ± 0.013 | 1.193 ± 0.010 | 1.197 ± 0.104 | 21 |
| LV Her B | 6020 ± 160 | 0.517 ± 0.013 | 1.170 ± 0.008 | 1.142 ± 0.092 | 21 | ||
| V565 Lyr A | 18.80 | 5600 ± 90 | 0.28 ± 0.05 | 0.746 ± 0.014 | 0.995 ± 0.003 | 1.045 ± 0.042 | 22 |
| V565 Lyr B | 5430 ± 130 | 1.016 ± 0.017 | 0.929 ± 0.003 | 0.991 ± 0.051 | 22 | ||
| Kepler-35 A | 20.73 | 5610 ± 140 | −0.34 ± 0.20 | 0.816 ± 0.007 | 0.888 ± 0.005 | 0.835 ± 0.041 | 23 |
| Kepler-35 B | 5200 ± 100 | 1.666 ± 0.016 | 0.809 ± 0.005 | 0.775 ± 0.043 | 23 | ||
| AI Phe B | 24.59 | 6310 ± 150 | −0.14 ± 0.10 | 0.200 ± 0.008 | 1.195 ± 0.004 | 1.303 ± 0.096 | 24 |
| Kepler-34 A | 27.80 | 5920 ± 120 | −0.07 ± 0.15 | 0.668 ± 0.006 | 1.048 ± 0.003 | 1.033 ± 0.074 | 25 |
| Kepler-34 B | 5860 ± 140 | 0.782 ± 0.007 | 1.021 ± 0.002 | 1.004 ± 0.061 | 25 | ||
| KX Cnc A | 31.22 | 5900 ± 100 | 0.07 ± 0.10 | 0.945 ± 0.006 | 1.138 ± 0.003 | 1.067 ± 0.057 | 26 |
| KX Cnc B | 5850 ± 100 | 0.980 ± 0.006 | 1.131 ± 0.003 | 1.061 ± 0.048 | 26 | ||
| KIC 8410637 B | 408.3 | 6490 ± 170 | 0.20 ± 0.11 | 0.341 ± 0.021 | 1.322 ± 0.017 | 1.407 ± 0.067 | 27 |
Reference. (1) Jeffries et al. (2013); (2) Ribas et al. (1999); (3) Sandberg Lacy et al. (2010); (4) da Silva et al. (2014); (5) Lacy et al. (2008); (6) Andersen et al. (1989); (7) Hełminiak et al. (2009); (8) Clausen et al. (2008b); (9) Clausen et al. (2008a); (10) Clausen et al. (2008b); (11) Clausen et al. (2009); (12) Maceroni et al. (2013); (13) Martin & Rebolo (1993); (14) Pavlovski et al. (2014); (15) Clausen et al. (2010b); (16) Meibom et al. (2009); (17) Clausen et al. (2010b); (18) Clausen et al. (2010a); (19) Brogaard et al. (2011); (20) Bass et al. (2012); (21) Torres et al. (2009); (22) Brogaard et al. (2011); (23) Welsh et al. (2012); (24) Andersen et al. (1988); (25) Welsh et al. (2012); (26) Sowell et al. (2012); (27) Frandsen et al. (2013).
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