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Fig. 6
Best-fit model SED fits to the redshift- and extinction-corrected observed spectra of Haro 11B, Haro 11C, and ESO 338-IG 004. The contributions from the stellar and ionised gas components are shown by the green and blue lines, respectively. The sum of stellar and ionised gas emission is shown by the red line.
This figure is made of several images, please see below:
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