A comparison between the properties of the dwarf galaxy candidates studied in this work and the known dwarf galaxies of the LG (McConnachie 2012). Top: effective radius in pc vs. V band luminosity in L_⊙. Middle: V band surface brightness in mag arcsec^-2 vs. effective radius in pc. Bottom: V band surface brightness in mag arcsec^-2 vs. absolute V band magnitude. In the latter, the outliers are emphasized by name. The V band quantities were obtained by transforming r band magnitudes to V magnitudes using Fukugita et al. (1996).