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Fig. 5
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Distributions of stars simulated by the Vasiliev et al. (2021) model and RRLs from the RRLS-SGR-MODEL, RRLS-SGR-R22, and RRLS-SGR-SELECTION samples on the µΛ versus Λ plane, color-coded by distance. The Sgr coordinates and proper motions are given in the system introduced by Vasiliev et al. (2021).
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