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Fig. 2


UVJ diagram of the Herschel-detected sources with z ≥ 1.2. The restframe magnitudes are obtained by photometric interpolation and originate from the work of Schreiber et al. (2015). The line separating the actively star-forming sources (bottom-right) from quiescent (top left) is the Williams et al. (2009) adopted definition for z ∈ [ 1,2 ].

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