Fig. 2
Example of SED fitting for a representative sample of the FIR cluster galaxies: one spectroscopic cluster member, one Herschel-only detected, one MIPS-only detected and one detected in both MIPS and Herschel. Black filled circles show the observed photometry of each source, open triangles show upper limits. Blue curves represent the BC03 template that best fit the stellar part of the spectrum from the optical to IRAC 8 μm. Red curves are the CE01 templates that best fit the fluxes from IRAC 8 μm to SPIRE 500 μm.
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