Fig. C.1
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Top: F212N versus F162M-F212N CMD. The dashed purple line indicates that stars with F162M-F212N < 1.6 belong to the foreground population. Bottom: F405N versus F360M-F405N CMD. We cut the CMD at F405N = 12 mag because that is the saturation limit. The blue points are the foreground stars identified in the F212N versus F162M-F212N CMD.
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