Fig. 6
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Histograms across samples (full CALIFA, cyan bars; galaxies in the full iEDGE sample, black empty bars; CO detected galaxies in the iEDGE, red bars) related (from left to right) to M*, SFR, specific SFR (sSFR=SFR/M*), and logarithmic distance from the SF main sequence (ΔSFMS). Similarly to CALIFA, iEDGE spans a representative range of SFR, M*, and related values. However, CO detections decrease at low sSFR and ΔSFMS values.
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