Top: this is an RGB image (using F444W, F356W, and F277W) of galaxy ID_DR3 = 14207, which is likely to have undergone tidal disruptions due to interactions with ID_DR3 = 14206, distinctly visible in the LW filters. Bottom: this is an RGB image (using F200W, F150W, and F115W) of galaxy ID_DR3 = 18351, which is likely to be a merger candidate. We can see nearby objects to its left with very similar redshifts. Both the cutouts are of 8″. Surrounding galaxies with similar redshifts (obtained using BAGPIPES, within the error bars of their photometric redshifts) are marked in the cutouts.