Fig. 10
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Distribution of the A23 surface gravities before and after the catalogue pipeline (described in Figure 4) is applied on the PDR1 (top) and PGS (bottom) input catalogues. The vertical line at log g=3.5 shows the separation used to validate the selected sample of giants. In all the panels, the overdensity of stars at log g~2.5 from RC stars are clearly visible.
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