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Fig. 2.

image

Select SED fits. Each panel shows the inferred SED PDF, in yellow intensity scale, normalized by the MCMC-averaged TIR. The color violin plots represent the synthetic photometry PDF, for each waveband. The black error bars are the observations. Panels a–c: arbitrary chosen galaxies, representative of their classes (early-type, late-type, and irregulars, respectively). Panel d: case, where most constraints are only upper limits.

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