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Fig. 10.


Colour–magnitude diagram of the members of NGC 3201 created with the photometry taken from the HST UV globular cluster survey (Nardiello et al. 2018; Piotto et al. 2015). Colour-coded is the binary probability obtained by our statistical method. Large panel: full CMD of our sample using V and I equivalent filters. Small panel: detailed version of the MS turn-off CMD region using B and I equivalent filters. Additionally, the period P range is indicated by coloured circles where THE JOKER was able to fit a well constrained Keplerian orbit.

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