Figure 8
The fraction of COLD GASS galaxies with CO line detections is plotted as a function of stellar mass, stellar mass surface density, concentration and sSFR (blue curve). Poisson errors are shown as the blue dashed lines. Results for the F10 models are shown as the black (KMT atomic-to-molecular gas prescription) and red (BR pressure prescription) curves.

The fraction of COLD GASS galaxies with CO line detections is plotted as a function of stellar mass, stellar mass surface density, concentration and sSFR (blue curve). Poisson errors are shown as the blue dashed lines. Results for the F10 models are shown as the black (KMT atomic-to-molecular gas prescription) and red (BR pressure prescription) curves.

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