Fig. 11

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mF322W2 vs. mF606W − mF322W2 CMD of proper-motion-selected members of NGC 6397, constructed using NIRCam data. The inset displays the ΔF606W–F322W2 vs. ΔF814W–F150W2 ChM, where black points represent NGC 6397 stars, and the orange points correspond to a simulated ChM for a single-population cluster. Red error bars indicate the typical color and magnitude uncertainties for stars in different magnitude bins.
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