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Fig. 3

image

Redshift distribution of the AKARI NEP deep field MIR selected galaxies derived by CIGALE code (solid line) together with those published in the literature (dashed: Magliocchetti et al. 2008; dash-dot-dashed and dash-triple-dotted: Desai et al. (2008), for objects with and without spectroscopic redshifts; large-dashed: Gilli & Daddi 2007; and dotted: Starikova et al. 2012).

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