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Fig. 8

Left: relative-age bias due to adopting a low initial helium abundance as a function of the masses of the binary system. Artificial stars are sampled from the grid with ΔY/ ΔZ = 1, and their age is estimated on the standard grid (ΔY/ ΔZ = 2). Right: same as the left panel, but sampling from a grid with ΔY/ ΔZ = 3.
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