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Fig. A.3


Synthetic CMD for stars around the bump and AGB clump (left panel: SFH for rell < 0.183 deg), compared with observations (right panel). The ridge lines of both observed and synthetic RGB bumps are also marked (solid and dashed lines, respectively). The AGB clump is the feature on the blue side of the RGB, in the range V ~ 19.1–19.4 and (B − V) ~ 0.70−0.75. The dotted line marks the level of the discontinuity of the slope of the RGB+AGB cumulative luminosity function (see text for details).

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