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Fig. 7

image

Spectral energy distribution from MAGPHYS (black curve) with the observed photometry (blue filled circles) and the 3D-HST spectrum (red line). The 3D-HST spectrum is corrected for the flux loss outside the slit, as described in the text. The plot also reports the MUSIC ID of the source and its redshift, measured from the near-IR spectrum. The inset shows a zoom on the 3D-HST spectrum, close to the Hα emission line.

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