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Fig. B.2
Comparison of star formation rates computed with FUV+24 μm and Hα+24 μm. Residuals of the relations in dex for NGC 4501, NGC 4567/68, and NGC 4321. The continuous line corresponds to a linear relation between the two SFR indicators, while the dashed and dotted lines correspond to ± 1σ for each galaxy.
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