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Fig. 10.
F814W vs. F438W–F814W colour-magnitude diagram, showing the RGB for stars with ΔF336W−F343N > 0.047 (P1) and ΔF336W−F343N ≤ 0.047 (P2). The black curves are polynomial fits to the two sequences. Grey symbols indicate stars which are saturated in F814W.
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