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Fig. 6.

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Upper panel: Surface brightness profile of JADES-GS8-RL-1. One can see a deviation between the radial profiles of F356W (containing [OII]) and F335M (which does not) at 0.2 to 0.5 arcsec, which is consistent with the expelled weakly ionised gas scenario. Lower panel: Difference between the two radial profiles versus wavelength.

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