Fig. A.1
HST images, composite of F814W (blue), F125W (green), and F160W (red) from the CANDELS survey (left panels), and observed spectra (right panels) for the ten most massive and strongest star-forming galaxies (see text) in the VUDS-DR1. The CANDELS ID number is indicated in each of the left panels, while the ID, the spectroscopic redshift from VUDS-DR1, and the stellar mass M⋆ and SFR are indicated for each galaxy in the right panels.
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