Fig. 10
Simulated TTV standard deviation in minutes of Qatar-1b as a function of the outer perturber period, for two values of eccentricity and three values of perturber masses. The gray area on the left correspond to perturber orbits that would make the Qatar-1b orbit unstable. The mean motion resonances 2:1, 3:1, and 5:2 are indicated with vertical dashed lines.
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