Fig. 7
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Upper panels: distributions of RRLs from the RRLS-SGR-SELECTION sample in the Cartesian Z versus X plane, the heliocentric distance versus the Sgr Λ coordinate plane, and the proper motion μΛ versus Λ plane, color-coded by metallicity. Lower panels: same distributions but for the sample of simulated stars from Vasiliev et al. (2021), color-coded by time of stripping from the Sgr progenitor.
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