Fig. B.1.
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RGB member candidates of WLM. Left: Color-magnitude diagram, V−I versus V. Blue lines enclose the RGB stars of WLM. Right: Space distribution of WLM member star candidates. The green dashed-line box indicates the field-of-view of the final stacked Subaru observations. The red cross and the gray ellipse indicate the optical center and the main body of WLM as in Fig. 1.
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