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Fig. 9.

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Normalised number histogram of stars as a function of (GBPGRP) for each distance sub-sample. (a) All the Gaia stars in the region of the cluster, (b) Gaia stars which fall in the regions where there is less extinction (E(B − V) < 0.75 mag) (c) Gaia stars which fall in more extincted region (E(B − V) > 0.75 mag).

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