Fig. A.2
Best-fit panchromatic (UV-radio) rest-frame SEDs of our SMGs that are likely to host an AGN. All these sources except AzTEC/C24b and C77a are detected in X-rays. However, AzTEC/C24b and C77a are detected with the VLBA at 1.4 GHz with flux densities of about 0.13 mJy and 0.33 mJy, respectively, and hence both of them are likely to host a radio-emitting AGN.
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