Table A.1.
Eclipsing binaries + α Cen + Sun: the obtained age and errors of the solution.
| Binary | Star | log M/M⊙ | Error | log R/R⊙ | Error | log L/L⊙ | Error | [M/H] | Error | Ref. | Age/Age⊙ | Error |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| AD Boo | A | 0.1504 | 0.0028 | 0.2074 | 0.0038 | 0.640 | 0.030 | 0.10 | 0.15 | (1) | 0.3729 | 0.1351 |
| AD Boo | B | 0.0824 | 0.0022 | 0.0849 | 0.0036 | 0.280 | 0.040 | |||||
| AL Dor | A | 0.0425 | 0.0002 | 0.0496 | 0.0039 | 0.159 | 0.033 | 0.10 | 0.10 | (2) | 0.6511 | 0.2179 |
| AL Dor | B | 0.0421 | 0.0002 | 0.0484 | 0.0039 | 0.145 | 0.033 | |||||
| α Cen | A | 0.0434 | 0.0028 | 0.0878 | 0.0011 | 0.190 | 0.008 | 0.24 | 0.04 | (3) | 0.9495 | 0.1532 |
| α Cen | B | −0.0297 | 0.0028 | −0.0640 | 0.0025 | −0.303 | 0.021 | |||||
| BG Ind | A | 0.1547 | 0.0024 | 0.3598 | 0.0032 | 0.870 | 0.070 | −0.20 | 0.10 | (4) | 0.5938 | 0.1248 |
| BG Ind | B | 0.1116 | 0.0027 | 0.2253 | 0.0098 | 0.680 | 0.080 | |||||
| BK Peg | A | 0.1504 | 0.0021 | 0.2984 | 0.0017 | 0.740 | 0.020 | −0.12 | 0.07 | (5) | 0.6135 | 0.0694 |
| BK Peg | B | 0.0993 | 0.0017 | 0.1685 | 0.0050 | 0.490 | 0.030 | |||||
| BW Aqr | A | 0.1377 | 0.0057 | 0.2388 | 0.0022 | 0.669 | 0.027 | −0.07 | 0.11 | (6) | 0.4939 | 0.0577 |
| BW Aqr | B | 0.1670 | 0.0053 | 0.3161 | 0.0008 | 0.796 | 0.028 | |||||
| CO And | A | 0.1103 | 0.0025 | 0.2373 | 0.0053 | 0.580 | 0.038 | 0.01 | 0.15 | (7) | 0.7117 | 0.1334 |
| CO And | B | 0.1019 | 0.0025 | 0.2289 | 0.0044 | 0.572 | 0.038 | |||||
| EPIC 210822691 | A | 0.0374 | 0.0040 | 0.0969 | 0.0035 | 0.245 | 0.028 | 0.00 | 0.05 | (8) | 1.3228 | 0.5111 |
| EPIC 210822691 | B | −0.0177 | 0.0090 | −0.0269 | 0.0046 | −0.118 | 0.038 | |||||
| EPIC 219394517 | A | 0.0327 | 0.0008 | 0.0233 | 0.0045 | 0.091 | 0.031 | 0.07 | 0.03 | (9) | 0.4999 | 0.2257 |
| EPIC 219394517 | B | 0.0278 | 0.0010 | 0.0179 | 0.0050 | 0.066 | 0.031 | |||||
| EW Ori | A | 0.0693 | 0.0041 | 0.0674 | 0.0019 | 0.220 | 0.030 | 0.05 | 0.09 | (10) | 0.5105 | 0.1806 |
| EW Ori | B | 0.0504 | 0.0035 | 0.0402 | 0.0020 | 0.120 | 0.030 | |||||
| FL Lyr | A | 0.0829 | 0.0027 | 0.0948 | 0.0080 | 0.330 | 0.095 | −0.07 | 0.09 | (11) | 0.9479 | 0.5833 |
| FL Lyr | B | −0.0217 | 0.0018 | −0.0458 | 0.0116 | −0.180 | 0.080 | |||||
| GX Gem | A | 0.1726 | 0.0032 | 0.3668 | 0.0022 | 0.860 | 0.030 | −0.12 | 0.10 | (12) | 0.7018 | 0.0788 |
| GX Gem | B | 0.1664 | 0.0030 | 0.3499 | 0.0023 | 0.820 | 0.030 | |||||
| IM Vir | A | −0.0083 | 0.0053 | 0.0257 | 0.0065 | −0.012 | 0.034 | −0.10 | 0.25 | (13) | 2.5543 | 0.4300 |
| IM Vir | B | −0.1776 | 0.0031 | −0.1669 | 0.0083 | −0.867 | 0.056 | |||||
| Kepler-34 | A | 0.0203 | 0.0013 | 0.0651 | 0.0011 | 0.173 | 0.033 | −0.07 | 0.15 | (14) | 1.3305 | 0.2720 |
| Kepler-34 | B | 0.0089 | 0.0009 | 0.0385 | 0.0012 | 0.107 | 0.036 | |||||
| Kepler-35 | A | −0.0517 | 0.0025 | 0.0122 | 0.0008 | −0.027 | 0.043 | −0.34 | 0.20 | (15) | 2.5429 | 0.3827 |
| Kepler-35 | B | −0.0918 | 0.0024 | −0.1045 | 0.0012 | −0.387 | 0.020 | |||||
| KIC 10031808 | A | 0.2408 | 0.0022 | 0.4133 | 0.0034 | 1.185 | 0.027 | −0.11 | 0.08 | (16) | 0.2593 | 0.0157 |
| KIC 10031808 | B | 0.2548 | 0.0031 | 0.4810 | 0.0020 | 1.254 | 0.027 | |||||
| KIC 2557430 | A | 0.2279 | 0.0077 | 0.2742 | 0.0046 | 0.899 | 0.038 | −0.11 | 0.03 | (17) | 0.3651 | 0.2134 |
| KIC 2557430 | B | 0.1303 | 0.0064 | 0.0899 | 0.0106 | 0.249 | 0.075 | |||||
| KIC 3439031 | A | 0.0890 | 0.0010 | 0.1471 | 0.0008 | 0.450 | 0.060 | 0.10 | 0.13 | (18) | 0.4972 | 0.1591 |
| KIC 3439031 | B | 0.0884 | 0.0009 | 0.1484 | 0.0007 | 0.450 | 0.060 | |||||
| KIC 7177553 | A | 0.0183 | 0.0058 | −0.0269 | 0.0023 | −0.055 | 0.040 | −0.05 | 0.09 | (19) | 0.3702 | 0.2341 |
| KIC 7177553 | B | −0.0061 | 0.0066 | −0.0264 | 0.0023 | −0.071 | 0.041 | |||||
| KIC 7821010 | A | 0.1062 | 0.0058 | 0.1059 | 0.0037 | 0.470 | 0.040 | 0.10 | 0.08 | (20) | 0.0712 | 0.0652 |
| KIC 7821010 | B | 0.0867 | 0.0057 | 0.0828 | 0.0050 | 0.390 | 0.050 | |||||
| KX Cnc | A | 0.0561 | 0.0011 | 0.0269 | 0.0008 | 0.091 | 0.002 | 0.07 | 0.10 | (21) | 0.2186 | 0.0946 |
| KX Cnc | B | 0.0535 | 0.0012 | 0.0208 | 0.0008 | 0.061 | 0.002 | |||||
| LL Aqr | A | 0.0777 | 0.0003 | 0.1209 | 0.0020 | 0.332 | 0.014 | 0.02 | 0.04 | (22) | 0.8486 | 0.1033 |
| LL Aqr | B | 0.0144 | 0.0003 | 0.0009 | 0.0022 | −0.019 | 0.016 | |||||
| LV Her | A | 0.0766 | 0.0036 | 0.1329 | 0.0038 | 0.349 | 0.044 | 0.08 | 0.21 | (23) | 0.8695 | 0.2541 |
| LV Her | B | 0.0681 | 0.0030 | 0.1183 | 0.0036 | 0.311 | 0.044 | |||||
| UX Men | A | 0.0874 | 0.0005 | 0.1294 | 0.0042 | 0.380 | 0.030 | 0.04 | 0.10 | (24) | 0.5995 | 0.1356 |
| V1130 Tau | A | 0.1159 | 0.0027 | 0.1729 | 0.0029 | 0.590 | 0.020 | −0.25 | 0.10 | (25) | 0.4551 | 0.0493 |
| V1130 Tau | B | 0.1436 | 0.0025 | 0.2509 | 0.0027 | 0.740 | 0.020 | |||||
| V785 Cep | A | 0.0426 | 0.0028 | 0.1535 | 0.0058 | 0.340 | 0.030 | −0.06 | 0.06 | (26) | 1.6414 | 0.2150 |
| V785 Cep | B | 0.0338 | 0.0028 | 0.1377 | 0.0060 | 0.300 | 0.030 | |||||
| VZ Hya | A | 0.1041 | 0.0021 | 0.1186 | 0.0017 | 0.480 | 0.040 | −0.20 | 0.12 | (27) | 0.2798 | 0.1483 |
| VZ Hya | B | 0.0592 | 0.0027 | 0.0461 | 0.0027 | 0.240 | 0.040 | |||||
| WZ Oph | A | 0.0888 | 0.0025 | 0.1464 | 0.0037 | 0.410 | 0.030 | −0.27 | 0.07 | (28) | 1.0450 | 0.1542 |
| WZ Oph | B | 0.0864 | 0.0021 | 0.1520 | 0.0037 | 0.400 | 0.030 | |||||
| Sun | 0 | 4.4E−05 | 0 | 8.7E−05 | 0 | 0.00062 | 0 | 0.005 | See text | 0.9327 | 0.0621 |
References. (1), (27) and (28) Clausen et al. (2008a,b); (2) Gallenne et al. (2019), Graczyk et al. (2019); (3) Kervella et al. (2017); (4) Rozyczka et al. (2011); (5) Clausen et al. (2010a); (6) Maxted (2018), Clausen et al. (2010a); (7) Sandberg Lacy et al. (2010); (8) Hoyman & Çakırlı (2020); (9) Torres et al. (2018); (10) Clausen et al. (2010b), Popper et al. (1986); (11) Hełminiak et al. (2019b), Popper et al. (1986); (12) Lacy et al. (2008); (13) Morales et al. (2009); (14) and (15) Welsh et al. (2012); (16), (18) and (20) Hełminiak et al. (2019b); (17) Hoyman et al. (2020); (19) Lehmann et al. (2016); (21) Southworth (2020), Sowell et al. (2012); (22) Graczyk et al. (2016), Southworth (2013); (23) Torres et al. (2009); (24) Andersen et al. (1989), Hełminiak et al. (2009); (25) Clausen et al. (2010c); (26) Meibom et al. (2009).
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