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1 Erratum to: Celest Mech Dyn Astr (2011) 111:235–266 DOI 10.1007/s10569-011-9356-0
All time values related to long-term \(N\)-body integration must be multiplied by the factor \(\approx \)0.6119. Hence, the stability tests of Fig. 5 actually correspond to the integration time of 6119 yr, instead of 10000 yr, and those in Sect. 8 to the time \(611.9\) kyr, rather than \(1\) Myr. The secular period of the pericenters revolution, which was mentioned in that section, is actually \(8.8\) yr instead of the stated \(14.3\) yr. This corrected value is in a much better agreement with, e.g., Rivera et al. (2010), who give \(8.7\) yr.
The results of the short-term integrations over the observational time segment (\(\sim \)10 yr) are not affected by this error, because we used a different subroutine for this task. In particular, the \(N\)-body radial velocity fits given in the Tables 1, 2, and 3 are correct.
References
Rivera, E.J., Laughlin, G., Butler, R.P., Vogt, S.S., Haghighipour, N., Meschiari, S.: The Lick-Carnegie exoplanet survey: a Uranus-mass fourth planet for GJ 876 in an extrasolar Laplace configuration. Astrophys. J. 719, 890–899 (2010)
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The online version of the original article can be found under doi:10.1007/s10569-011-9356-0.
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Baluev, R.V. Erratum to: Orbital structure of the GJ876 extrasolar planetary system based on the latest Keck and HARPS radial velocity data. Celest Mech Dyn Astr 117, 215 (2013). https://doi.org/10.1007/s10569-013-9504-9
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DOI: https://doi.org/10.1007/s10569-013-9504-9