Fig. 9
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Euclid images (log scale) of proto-brown dwarf candidates from Palau et al. (2012) and Morata et al. (2015). J041847 is clearly resolved as a spiral galaxy, possibly a galaxy merger. J041913 shows some extended emission that suggests that it is a galaxy. J042016, J042019, and J042118 have a neighbor within 3″ that might cause the radio emission. J042123 is resolved as an elliptical galaxy.
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