Best-fit template obtained from a SED-fitting decomposition (green lines), as a function of M_⋆ (left to right, expressed in log M_⊙) and redshift (top to bottom). Red circles indicate the IR/sub-mm photometry (MIPS 24 μm, PACS 100−160 μm, SPIRE 250−350−500 μm, SCUBA 850 μm, and AzTEC 1.1 mm), while downward arrows mark the corresponding 3σ upper limits. The red dotted line is the best-fit AGN template, shown in the only bin where its significance is above 3σ. Green dashed lines represent SEDs without FIR measurements and at z ≳ 1.5, for which the integrated L_IR is interpreted as 3σ upper limit (5/42 bins). MIPS 24 μm flux densities are not used in the fitting.