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Fig. 6.
Same as Fig. 5 but for (J − Ks)0 color. The bluer and redder stars, divided by (u − g)0, overlap in (J − Ks)0 color. Thus, the distinct double RC observed in the (Ks, J − Ks)0 CMD may be due to the synergy of the faint clump of the bluer stars and the bright and faint clumps of the redder stars.
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