Encoding of the infrared excess in the NUVrK color diagram for star-forming galaxies

S. Arnouts; E. Le Floc’h; J. Chevallard; B. D. Johnson; O. Ilbert; M. Treyer; H. Aussel; P. Capak; D. B. Sanders; N. Scoville; H. J. McCracken; B. Milliard; L. Pozzetti; M. Salvato

doi:doi:10.1051/0004-6361/201321768

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Fig. 9

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Distributions of the SFR ratios (SFR^NRK/SFR^SED) in different bins of NRK_ssfr. 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 NRK_ssfr, we report the fraction of objects (f_Tot), catastrophic failures (f_Cat), the median (Δ) and dispersion (σ).

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