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Fig. 8.

image

Total gas masses from combined CO(1–0) and H I observations vs. the difference between observed total gas mass (CO+HI) and the dust-based total gas mass. Galaxies with detection in CO+HI are circled in green, while measurements with CO and/or H I upper limits are shown in red. The CO upper limits may be affected by beam dilution that works in the direction of the blue arrows.

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