Fig. 3
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Left: CMD of NGC 5824 with Clay photometry. Black dots correspond to the full sharp-cleaned data. Light blue dots are BHB candidates. Red dots are RGB candidates. Blue and yellow dots correspond to the isochrone. Right: NGC 5824 proper motion (PM) diagrams. Gray dots correspond to the full data with PM measurements. Light blue dots (upper panel) are BHB candidates. Red dots (lower panel) are RGB candidates.
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