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Fig. 9

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Gaia EDR3 colour-magnitude diagram for the hot subluminous star region showing the initial parallax selection (grey dots), Final Parallax Selection (yellow circles), known hot subdwarfs in wide binary systems displaying an excess in flux error (blue circles), and known hot subdwarfs in close binary systems that display an excess in flux error (magenta squares). The red lines show the variability cutoffs used.

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