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Fig. 18.

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Quyllur compared to SEDs of single stellar populations at El Gordo’s redshift z = 0.87. Blue lines show the unreddened models as labeled, and green lines show the models reddened with E(B − V) = 3.5 mag. Black points with error bars show the Quyllur photometry. For a comparison with the SED of individual stars see Fig. 21.

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