Fig. 11.
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Relation between the NUV−r color and the sSFR inferred by SED model-fitting for EFIGI ∩ GALEX galaxies with Incl-Elong ≤ 2, showing the correlation between these two parameters, with the bluest galaxies being the most star forming, while red sequence galaxies mostly show no star formation. Intermediate colors are prone to larger uncertainties.
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