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Milky Way Dwarf Galaxies: A Search for Stellar Substructure

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Figure

Table 2.1: Fundamental Parameters of Hercules
Figure 2.2: Example of the star/galaxy separation method used, where objects are distinguishedmby their light profile
Table 2.2: Significance values for the 1σt detected Hercules over-densities, where segment labellingcorresponds to the grey outlines in Figure 2.8.
Table 2.4: Significance values for ‘nuggets’ depicted bysegmentation. The segments are shown in Figure Sand et al
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