Fig. 4

GOODS–Herschel detection limits (from Table 1) and total IR luminosities of the
Herschel sources as a function of redshift (filled dots:
spectroscopic, open dots: photometric). The right axis is the SFR derived from
SFR[M⊙ yr-1] = 1.72 × 10-10 × [L⊙]
(Kennicutt 1998a). These limits were
computed assuming the local library of template SEDs of CE01. For comparison, the
Spitzer MIPS-24 μm detection limit is
represented as well as the knee of the total IR luminosity function, as derived by
Magnelli et al. (2009, 2010).
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