Fig. B.3.
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Individual CO spectral line distributions of AGN hosts and star-forming galaxies and individual SLEDs for AGN hosts and star-forming galaxies normalized to the average CO (2 − 1) flux of main-sequence galaxies at z ∼ 1.2 from V20a. Yellow and red lines indicate galaxies in our sample with fAGN ≤ 20% and > 20%, respectively. Open blue circles show Chandra detections at 2−10 keV.
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