Fig. A.1.
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Colour-magnitude diagrams of ω Cen using JWST filters. Panel (a) shows the mF150W2 versus mF150W2 − mF322W2 CMD, while panel (b) displays the mF322W2 versus mF150W2 − mF322W2 CMD, including all stars within the JWST FOV. In both panels, black dots represent stars that pass both the photometric quality and PM selection criteria, while grey dots indicate the remaining stars. The shaded light red and dark red regions highlight areas affected by saturation: the light red region corresponds to saturated photometry, while the dark red region marks severe saturation, where even frame zero is saturated.
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