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Fig. 6


Left: test for singleness of TTV hot Jupiters. Stars: multiple systems; crosses: single hot Jupiters; large dots: hot Jupiters with significant TTV. The line shows the upper boundary of the region occupied by known coplanar multi systems. Right: test for moons. Large dots: hot Jupiters with single TTV periodicity; stars: systems with multiple frequencies taken from Table 1. The line plots the expected TTV amplitudes assuming 1 MJ planet with a 1 ME moon orbiting at the Hill radius.

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