Fig. 1.
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Results of the NUVrJ color-color selection results, defined in Eq. (2) shown for redshift bins adopted in this work. The NUVrJ colors (Ilbert et al. 2013) are used in order to distinguish between sources reddened due to the lack of star formation (quiescent galaxies – upper left section of the plots) from those where red colors are caused by dust extinction (SFGs – main locus in the plots).
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