  CCD images of three newly discovered dwarf spheroidal companions to M31, And
V, VI, and VII, are used to extract surface brightness profiles and total
magnitudes. Using distance modulii provided by Armandroff et al. (1998 & 1999)
and Grebel & Guhathakurta (1999), these galaxies are shown to have similar
luminosities to other Local Group dwarf spheroidals; And V in particular is
similar to Draco & UMi in luminosity, i.e., among the faintest known. In the
luminosity-metallicity relation, And V is shown to have a significantly higher
metallicity than expected.
