Fig. 2.

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Model fitted by FADO to a galaxy in our sample with Xneb = 10%. Upper panel: observed spectrum (black line) and total, stellar and nebular continuum fitted by FADO (blue, green and red lines, respectively). The shaded regions represent the uncertainty in the estimated models. Bottom panel: ratio between the nebular and total continuum fitted by FADO as a function of wavelength.
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