Fig. 2.

Stellar radial density profile for M 67 members (black filled circles). The different templates are plotted in different colours (see text for details). Vertical grey lines mark the derived rc and rt for the King (short dashed lines) and Nuker (long dashed lines) templates and rc for the EFF template (dot-dashed line). Small arrows in the bottom show previous cluster size determinations by Bonatto & Bica (2003), Davenport & Sandquist (2010), and Gao (2018) from left to right.
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