Figure 7.
Top: examples of the method used to determine the colour and magnitude for RC and turn-off for solar metallicity parsec isochrones of age $\log [t({\rm yr})]=8.3$ (left), 9.1 (middle), and 9.5 (right). Bottom-left panel: CMD of all isochrones used, where the red region corresponds to MS stars (label = 1) and the blue region corresponds to the beginning of the RC phase (label = 4, 5, and 6). Bottom-right panel: RC and turn-off positions identified from the models, where the colour bar indicates the ages.

Top: examples of the method used to determine the colour and magnitude for RC and turn-off for solar metallicity parsec isochrones of age |$\log [t({\rm yr})]=8.3$| (left), 9.1 (middle), and 9.5 (right). Bottom-left panel: CMD of all isochrones used, where the red region corresponds to MS stars (label = 1) and the blue region corresponds to the beginning of the RC phase (label = 4, 5, and 6). Bottom-right panel: RC and turn-off positions identified from the models, where the colour bar indicates the ages.

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