| Issue |
A&A
Volume 671, March 2023
|
|
|---|---|---|
| Article Number | C9 | |
| Number of page(s) | 1 | |
| Section | Planets and planetary systems | |
| DOI | https://doi.org/10.1051/0004-6361/202140989e | |
| Published online | 17 March 2023 | |
Chaotic diffusion of the fundamental frequencies in the Solar System (Corrigendum)
Astronomie et Systèmes Dynamiques, Institut de Mécanique Céleste et de Calcul des Éphémérides CNRS UMR 8028, Observatoire de Paris, Université PSL, Sorbonne Université,
77 Avenue Denfert-Rochereau,
75014
Paris,
France
e-mail: nam.hoang-hoai@obspm.fr
Key words: chaos / diffusion / celestial mechanics / methods: statistical / errata, addenda
There are several misprints in Table 2 of the original publication. The corrected version is given here. This correction does not affect any other elements of the paper.
The authors would like to thank Yujing Wu and Alberto Malinverno for identifying these misprints.
Linear and power-law fits for the time evolution of the parameters (Fig. 10) of the skew Gaussian mixture model (Eq. (19)) for the fundamental frequencies of the Solar System.
© The Authors 2023
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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Linear and power-law fits for the time evolution of the parameters (Fig. 10) of the skew Gaussian mixture model (Eq. (19)) for the fundamental frequencies of the Solar System.
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