Overshooting calibration and age determination from evolved binary systems - A statistical investigation on biases and random variability

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Table 4

Estimated individual overshooting efficiency for primary and secondary stars in different scenarios and their differences.

Scenario	β₁			β₂			β₁ − β₂
	q₁₆	q₅₀	q₈₄	q₁₆	q₅₀	q₈₄	q₁₆	q₅₀	q₈₄
A	0.20	0.30	0.30	0.12	0.14	0.18	0.04	0.14	0.17
B	0.10	0.14	0.16	0.08	0.12	0.19	–0.04	0.01	0.03
C	0.09	0.11	0.13	0.08	0.10	0.14	–0.03	0.01	0.03

Notes. The table shows the 16th, 50th and 84th quantiles of the fitted overshooting efficiency β₁ (columns 1–3), of the fitted overshooting efficiency β₂ (columns 4–6), and of their difference (columns 7–9).

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