Fig. 17
Top: histogram with mass distribution for periodic stars. Bottom: r − i vs. r-DM CMD for periodic stars. Mass tracks from Bell et al. (2014) for Pisa models (Tognelli et al. 2012) with semi-empirical corrections are shown as dotted lines. A black arrow shows a reddening vector from Schlegel et al. (1998) for AV = 2m. Black Xs show stars excluded from the mass estimation because they were too far away from the minimum mass track.
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