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Fig. 5.

image

Top row, left: age-relative error adopting δν as observational constraints (with observational error of 5%) versus the true stellar mass. Data were sampled from grid at different ΔYZ = 1.0, 2.0, and 3.0 and reconstructed over the grid with ΔYZ = 2.0. Right: same as in the left panel but as a function of the stellar relative age. Bottom row: as in the top row, but using the constraint on δν with an observational error of 2%.

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