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Fig. 18
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G histograms for the stars in the LMC instability strip. The filled polygons are cumulative histograms for the full sample, non-RR Lyr non-Cepheid variables from R23, RR Lyr from R23, and Cepheids from R23. The blue unfilled line is an independent histogram containing all stars with sG > 17 mmag.
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