Fig. 10.
Projected distances of UCDs to their assumed host galaxies versus their magnitudes. We show the UCDs from several sources including Rejkuba et al. (2007), Mieske et al. (2008), Brodie et al. (2011), Norris & Kannappan (2011), Liu et al. (2015), Misgeld et al. (2011) and (Galleti et al. 2004). We show the sources with absolute magnitudes between −9.5 > MV > −14.0 mag, the magnitude range for typical UCDs. Details on how the data were compiled can be found in Appendix B.
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