Fig. 2.
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Subsample of the light curves (normalized with respect to their mean magnitudes) of the gold sample BL Her stars in the LMC (in red) with their best-matched models (in blue). The full image is displayed in Fig. B.3. The input stellar parameters of the corresponding models are included in the format (Z, M/M⊙, L/L⊙, Teff, convection set) in each subplot.
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