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Fig. E.1

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Relation between the molecular gas fraction and the attenuation. There is a clear trend, with increasing molecular fraction the attenuation increases, with the exception of NGC 2403 which shows no trend. This is consistent with the trends observed in Fig. 3. The number of elements and the Spearman correlation coefficient are indicated at the bottom of each panel whereas the uncertainty on AFUV is shown in the bottom-right corner.

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