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Fig. 22

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Left column: UV to mid-infrared SED fits. Black points: photometric observations, red line: best-fitting model, cyan line: stellar template, black line (where applicable): galaxy template of second photometric redshift solution. The inset shows the probability distribution function of the best-fit model. Right column: RGB cutouts made from Subaru RcIcz′ images, with a single VLA contour overlaid and the VLBA position indicated with red crosses. These images show regions 28.8 arcsec × 28.8 arcsec in size.

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