Fig. 4.

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Examples of our best-fit SEDs. The left panel shows the best-fit SED for an LSB with only upper limits in the MIR and FIR wavelengths, whereas the SED in the right panel is of an HSB with extensive photometry at all wavelengths. The black solid line is the model SED. The blue open diamonds and the red circles are the observed fluxes and best-fit model fluxes, respectively. The green downward triangles are the observed flux upper limits used in the SED fitting.
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