Fig. 10.

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Heliocentric distance as a function of δ. The gray dots represent the stream particles. The blue points represent the four BHB stars in our samples, whose distances come from Xue et al. (2011). The red dots and error bars represent distances and corresponding errors for all member stars estimated using the method of Carlin et al. (2015). The dashed red line corresponds to their median value, 33 kpc. The solid green line marks the adopted distance, 30 kpc. Two black error bars represent 26 ± 4 kpc (Bonaca et al. 2012) and 35 ± 3 kpc (Martin et al. 2013).
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