Fig. 5.
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Observed and modeled SED of J012026. The purple squares represent, respectively, the GALEX, DECam g, r, i, z, and W1 − W4 observed fluxes, while the red dots represent the model-predicted fluxes. The orange, gray, and blue lines represent the best-fit individual model components, which are respectively stellar, nebular, and dust emission. The black line is the total best-fit model.
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