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2.3 numerical method
we utilize a second-order wisdom–holman symplectic map as our main integration method (wisdom & holman 1991; kinoshita, yoshida & nakai 1991) with a special start-up procedure to reduce the uncation error of angle variables,‘warm start’(saha & tremaine 1992, 1994).
the stepsize for the numerical integrations is 8 d throughout all integrations of the nine planets (n±1,2,3), which is about 1/11 of the orbital perio