Table 8: Comparison with results by David et al.
$M_{\rm B} / M_{\rm A}$ Boundary S/MS Boundary MS/U DQFA
  [AU] [AU] [AU]

0.1		 0.437 $\pm$ 0.001 0.457 $\pm$ 0.001 0.31 $\pm$ 0.04
0.5 0.278 $\pm$ 0.001 0.348 $\pm$ 0.001 0.28 $\pm$ 0.02
Note: Simulations were performed for giant planets with $M_{\rm G}$ = 1  $M_{\rm Jup}$,
whereas David et al. (2003; DQFA) assumed Earth-mass planets.

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Article Contents
1 Introduction
2 Method and code testing
3 Initial conditions and stability criteria
4 Case studies
5 Binary systems with observed giant planets
6 Conclusions
References
List of tables
List of figures