Spectral energy distributions of the galaxies in our target sample, sorted by increasing observer-frame z − K color (rest-frame NUV − g at z = 3.5). The observed photometry is shown with open black squares and gray error bars, and the best-fitting stellar continuum template from FAST++ obtained assuming z = zphot is shown in gray in the background. For galaxies with a measured spectroscopic redshift (see Sect. 3.3), we display the best-fitting template at z = zspec in orange, and the photometry corrected for emission line contamination with red squares.
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