Projected separations in physical units versus the distance to the potential host galaxy for each UDG candidate in the sample. We note that the data has been truncated at separations < 0.8 Mpc and distances ≲50 Mpc. The potential hosts have been separated into four mass bins, which is reflected by the size of the data points. The galaxy we have assumed is the host in this work is plotted in pink, while the distances at which the dwarf would be considered a UDG are shaded in gray. The dashed red vertical lines indicate the measured distances, when an estimate is available.