Fig. 10.

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Correlation between the CO emission line intensities. Left: ICO(2 − 1) and ICO(1 − 0) emission line comparison for CO-VGS and xCOLD GASS galaxies. Right: emission line ratio (R21 = ICO(2 − 1)/ICO(1 − 0)) as a function of the aperture-correction factor (fap) for CO-VGS and xCOLD GASS galaxies.
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