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Fig. 2

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Two types of approach in searching for a secondary eclipse by using multiple datasets (already filtered out from all other components – see Sect. 2.1 and Fig. 1). Left: averaging SES statistics of the individual datasets by their SNR. Right: averaging individual LCs by their inverse variance, and then compute SES of the average LC. The sum of the weights are normalized to unity in both cases. See text for more.

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