Secular spin-axis dynamics of exoplanets (Corrigendum)

Open Access

Erratum

This article is an erratum for:
[https://doi.org/10.1051/0004-6361/201834344]

Table F.4

Quasi-periodic representation of the orbital dynamics of Mars.

z			ζ
	E_j × 10⁸			S_j × 10⁸
17.91550	4902750	335.25	−17.74818	3464962	303.28
17.36469	4004873	303.95	−18.85115	1541097	60.43
4.24882	2030021	30.67	0.00000	1375324	107.59
16.81285	1853846	91.90	−18.30007	745752	89.07
18.46794	1357476	9.91	−17.19656	543058	154.89
17.63081	1139332	201.65	−26.33023	457927	127.29
17.08266	1114353	359.38	−18.01114	262761	62.09
28.22069	706337	128.11	−17.66094	249135	318.93
17.81084	472390	58.56	−17.83857	202620	109.13
18.18553	431698	57.28	−17.54636	180575	66.71
19.01870	399188	39.75	−19.13075	142530	305.90
17.15752	383488	145.02	−17.94404	127098	32.26
17.72293	356895	48.46	−18.59563	116625	278.11
18.01611	303744	44.83	−5.61755	105161	348.70
7.45592	295700	200.24	−19.40256	85957	23.33
16.52731	231195	311.91	−7.07963	77142	93.77
16.26122	210411	58.89	−3.00557	63897	140.33
17.47683	201641	80.26	−0.69189	60870	23.96
18.08627	175373	356.17	−18.97001	59221	73.36
17.55234	162274	17.65	−6.84091	38863	286.50
3.08952	73627	121.36	−7.19493	38505	285.16
52.19257	26717	225.55	−5.50098	37498	342.89
6.93423	25209	170.37	−6.96094	36566	277.95
7.34103	24970	207.85	−18.69743	31116	221.70
7.05595	21406	359.16	−18.77933	30502	222.83
7.57299	17424	11.47	−18.22681	30460	46.30
6.82468	8182	194.53	−19.06544	27285	50.21
29.37998	8059	37.54	−7.33264	22307	16.75
27.06140	8027	38.70	−5.85017	12681	165.47
5.59644	6750	110.35	−5.21610	9492	18.91
7.20563	5106	143.91	−5.37178	9443	35.48
28.86795	4795	212.64	−5.10025	9241	195.38
27.57346	4212	223.74	−6.73842	7310	224.50
7.71663	3182	93.52	−7.40536	6758	53.35
4.36906	3180	40.88	−7.48780	6278	227.95
−19.72306	3055	113.24	−6.56016	5900	123.47
5.40817	2931	120.37	−5.96899	5417	350.64
5.47449	2541	275.01	−8.42342	4915	31.21
53.35188	2250	134.91	−6.15490	3922	89.77
0.66708	2008	73.98	−26.97744	3471	43.07
5.71670	1929	120.52	82.77163	1993	128.95
76.16447	1090	323.03	−1.84625	1457	38.22
5.35823	1037	94.89	18.14984	1419	111.19
51.03334	605	136.30	−4.16482	1278	51.57
4.89647	464	291.74	58.80017	1169	212.90
5.99227	381	113.56	34.82788	924	294.12
5.65485	368	39.22	−2.35835	628	44.46
5.23841	305	272.97	−0.58033	592	17.33
3.60029	250	121.40	−27.48935	592	218.53
1.93168	227	192.09	−25.17116	559	215.94
−56.90922	223	44.11	−50.30212	458	209.84
2.97706	192	306.81	−3.11725	427	326.97
−20.88236	91	203.93	−28.13656	371	314.08
1.82121	65	149.54	0.46547	170	286.88
0.77840	35	65.10	11.50319	136	281.02
−0.49216	10	164.74	−1.19906	96	133.57
			0.57829	59	103.72
			20.96631	53	57.78
			10.34389	52	191.16
			9.18847	33	1.15

Notes. This representation is used in Fig. 3. It has been directly obtained from Laskar (1990), see text.

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