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Fig. A.1.

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SED fitting of ALESS073.1 in rest wavelengths (Circosta et al. in prep.). The black circles are all the available photometric points, while the white-filled circles represent the 3σ upper limits. The black solid line is the best-fit result. The yellow, red, and green solid lines are the best models for the attenuated stellar emission, dust emission, and AGN emission, respectively.

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