Fig. 11

Templates from this work compared to the most popular IR SED templates normalized to L8 − 1000. Left panel: low-z templates. In black: all of the templates computed in this work (Fig. 10). For better comparison, we plot only the templates of the different libraries whose properties (LIR, α) match those of the HRS. In turquoise: templates of Dale & Helou (2002) with α ranging from 1.5 to 4. In orange: library of Chary & Elbaz (2001) with log (LIR/L⊙) < 10.9, in magenta: median templates of Smith et al. (2012a) binned in dust luminosity for log (LIR/L⊙) < 11, and in green: templates of Rieke et al. (2009) with log (LIR/L⊙) < 11. Right panel: high-z templates. In black: mean SED from HRS (Fig. 9) as a reference for z = 0 galaxies. In purple: MS templates and in red the starburst template from Magdis et al. (2012). In blue: main MS template from Elbaz et al. (2011); and in cyan: starburst template from Elbaz et al. (2011). In green: selected templates from Berta et al. (2013). At low-z, there is a large discrepency between the templates between 20 and 100 μm.
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