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Fig. 17.

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Spectral energy distribution of Xp9. The radio data points are from Rodriguez-Rico et al. (2004). The mid-IR data points are upper limits obtained from the Subaru-COMICS images (Gandhi et al. 2011). The luminosity range at 12 μm, expected from the low-luminosity AGN hypothesis, is indicated by the dotted-line, which could be within the reach of the upcoming JWST observations.

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