Fig. 1.
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Comparison of metallicity distribution for RR Lyrae stars with different calibrations of Li et al. (2023), Clementini et al. (2023), and Varga et al. (in prep.). The distributions of disk stars (circles) and stars with PM anomalies (squares) are categorized by color for RRab and RRc types. The color bars are based on the periods derived from Gaia DR3 (Clementini et al. 2023).
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