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Fig. 13

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Models SFR functions at various redshifts compared to observations of Bell et al. (2007) and to the infrared luminosity functions observed by Le Floc’h et al. (2005), and Rodighiero et al. (2010) converted into SFR functions assuming log (SFR) = log (L/L) − 9.97 (Buat et al. 2008).

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