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Prospecting for exo-Earths in multiple planet systems with a gas giant

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Figure

Table 2. The constants provided by Kopparapu et al. (2014) which we useto calculate the edges of the HZ for our simulations.
Table 3. The orbital parameters of the TPs and 1 Mparameters, where the parameters are incremented over the given range forulations
Fig. 1, we show those systems that we found to be numerically sta-
Figure 2. The Cartesian plot, and the evolution of the semimajor axes andeccentricities of the four planets in the HD 160691 system
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