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As an example, the plot below shows some of the broad-brush comparisons available from just the core survey Phase I (from Geha et al. 2017). These aforementioned projects would expand from these "one point per galaxy" plots to more thoroughly characterize individual satellites and expand the scope of the observations from primarily-imaging to more thorough characterization and comparison with the wealth of data in the Local Group.
The work you imagine having the graduate student do:
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