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Fig. 16


Top: timing of GJ 436 observations with the 3.6 and 4.5 μm IRAC channels. The two vertical lines indicate the datasets having the transit-like features. Bottom: distribution of the possible period range for the putative additive transiting planet. The observational coverage discards all periods below 1.18 days.

This figure is made of several images, please see below:

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