Detectability of four UDGs detected around NGC 5485 in Merritt et al. (2014) before and after 4 × 4 binning. Each quadrant presents one source with four panels arranged as follows: original data (upper left) with its corresponding segmentation map (upper right), and 4 × 4 binned data (lower left) with its corresponding segmentation map (lower right). The segmentation map shows the UDG segment in white and all other sources in red.