Fig. 1.

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Distribution of members (blue), candidates (orange), and non-members (grey) for NGC 2527 in sky position (top left), proper motion (bottom left), parallax (top right), and the CMD (bottom right). The blue line in the CMD constitutes the isochrone that corresponds to the age of NGC 2527 as provided by Cantat-Gaudin et al. (2020). The dashed red lines indicate a ‘zero-uncertainty boundary’, outside of which sources with negligible errors are not selected as candidates. Candidates that lay outside these boundaries therefore have significant uncertainties.
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