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Fig. 11
WASP-43b blending analysis using the MuSCAT2-observed light curves without injected contamination (above), with 10% contamination from a 3600 K star (middle), and with 20% contamination from a 3600 K star (bottom). The dotted lines show the 65, 75, 85, and 95% percentiles for the posterior contamination.
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