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Fig. 2.
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SEDs obtained with this new version of the code HR-PYPOPSTAR. We show a comparison among SEDs with a) different ages (τ) for the same metallicity, Z = 0.02, and CHA IMF; b) different metallicities for a given age, log τ = 8.00, and CHA IMF; and c) different IMFs for a given age, log τ = 8.00, and metallicity, Z = 0.02.
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