Fig. 4
Left: density distribution of the difference in E(B − V) derived from the Padova and the Yonsei-Yale (YY) isochrones as a function of E(B − V) from the YY isochrones. Right: ratio of distances derived from the Padova isochrones to the YY stellar library as a function of distance. The dashed horizontal lines indicate ± 20% difference.
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