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Fig. 11.

image

Comparison between the eccentricity and inclination ephemerides of La2004 and their respective 100-term representations over the time interval from −35 Myr to 5 Myr with origin at J2000. Both representations are in the form of Eq. (31), with the Chebyshev expansions approximating the fundamental frequencies specified in Table A.2, and main frequency index vectors and complex amplitudes of all 100 terms in the full Tables A.3 and A.4 available at the CDS.

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