Fig. 9
The enclosed dark mass within 300 pc as a function of dSph luminosity. The purple dots are from Strigari et al. (2008) and the red squares are our cleaned samples presented in Fig. 8. The empty circles correspond to the fits of Angus (2010) to the uncleaned Walker et al. (2007) data, using the same cored dark halos as we implement here. The points referring to the same dSph are slightly shifted along the L axis for clarity.
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