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Fig. 18.


Same as Fig. 3, but for the “young-quiescent” galaxies, namely galaxies in ZFOURGE that lie outside of the UVJ-quiescent region but are probably still quiescent. Beside the name of each galaxy, we show the probability that its sSFR is lower than sSFRQ, our adopted threshold for quiescence, and we also indicate which galaxies have X-ray detections (“X-ray”) and those which are covered by ALMA but not detected (“no ALMA”).

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