Fig. E.1.
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Comparison between the total IR LF in SPRITZ (solid black lines) and the total IR LF observed by Herschel (red circles). We also report the best fits (dashed red lines) for each redshift bin, as derived by Gruppioni et al. (2013). Grey shaded areas indicate the 1σ uncertainties associated with the SPRITZ IR LF. In each panel we also report the reduced χ2 associated with each redshift bin.
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