Fig. 2
Typical best-fit SED by CIGALE from the FUV to the SPIRE 350 μm bands. This SED corresponds to one pixel in NGC 4254. The observed fluxes are represented by the red crosses with green 3-σ error bars. The value of χ2 is 0.76. The parameters are derived by taking the probability distribution function yielded by a set of reasonably good fits into account.
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