Fig. 2.

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Example SED fitting in the disk of NGC 628. The black crosses and red circles correspond to the observed and modeled fluxes, respectively. The purple dashed line represents a black body emission to account for the old stellar population, while the blue, green, and red dashed lines show the emission of the PAHs, VSGs, and BGs, respectively. The blue continuous line is the total emission. The panel below presents the residuals of the fit.
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