Table 1.
Percentiles of the relative error in the age estimates from different binary systems.
| S1 | S2 | ||||||
|---|---|---|---|---|---|---|---|
| Masses (M⊙) | q16 | q50 | q84 | q16 | q50 | q84 | |
| 0.85/0.85 | −9.7 | −0.2 | 11.1 | −6.8 | 0.3 | 6.0 | |
| 0.90/0.85 | −9.6 | 0.3 | 11.3 | −6.5 | 0.6 | 6.3 | |
| 0.90/0.90 | −9.7 | −0.4 | 11.4 | −8.0 | 0.5 | 7.2 | |
| 0.95/0.85 | −9.0 | 0.8 | 11.3 | −6.0 | 0.8 | 6.6 | |
| 0.95/0.90 | −9.9 | −0.3 | 9.8 | −6.8 | 0.3 | 6.5 | |
| 0.95/0.95 | −9.4 | −1.2 | 10.4 | −7.8 | 0.0 | 7.4 | |
| 1.00/0.85 | −9.7 | −0.2 | 9.1 | −6.5 | 0.2 | 6.2 | |
| 1.00/0.90 | −9.0 | −0.2 | 8.5 | −6.7 | 0.2 | 6.3 | |
| 1.00/0.95 | −8.2 | 0.4 | 9.5 | −7.0 | 0.4 | 7.3 | |
| 1.00/1.00 | −9.8 | −1.7 | 8.4 | −7.9 | −0.2 | 7.3 | |
Notes. In the first column, the masses of the primary and secondary stars are provided. Columns 2–4 contain the percentiles of the relative error in the estimated ages under uncertainty set S1. Columns 5–8 present the corresponding percentiles for uncertainty set S2.
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