Extended Data Fig. 1: Optical/NIR images and full SEDs of the UV-luminous targets REBELS-29 and REBELS-12.
From: Normal, dust-obscured galaxies in the epoch of reionization
The cutouts show images from which photometry was extracted. SED fits (bottom-right panels) are performed using the BAGPIPES33. In b and d, blue solid lines and bands represent the median posterior SEDs together with their 68% confidence contours for REBELS-29 and REBELS-12, respectively. Error bars corresponds to 1σ uncertainties, and downward arrows show 2σ upper limits. a and c show that the [C ii] 158 μm emission line redshifts (red) are in perfect agreement with the photometric redshift probability distributions (blue), that had been previously estimated from the optical/NIR photometry for both sources. This confirms their high-redshift nature.