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Fig. 9


Distributions of the SFR ratios (SFRNRK/SFRSED) in different bins of NRKssfr. The distribution are renormalized to unity. The top panel refers to the 24  μm sample while the bottom panel includes all galaxies with K ≤ 23.5 and more massive than M ~ 2 × 109 M. For each interval of NRKssfr, we report the fraction of objects (fTot), catastrophic failures (fCat), the median (Δ) and dispersion (σ).

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