$\begin{figure} \par\includegraphics[width=8cm,clip]{4068f4.eps} \end{figure}$ Figure 4: Comparisons of models for the precession of the ecliptic (quantity $P_{\rm A}$ ): differences with respect to the solution P03 provided in this paper.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{4068f5.eps} \end{figure}$ Figure 5: Comparisons of models for the precession of the ecliptic (quantity $Q_{\rm A}$ ): differences with respect to the solution P03 provided in this paper.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4068f6.eps} \end{figure}$ Figure 6: Comparisons of models for the precession of the equator (quantity $\psi _{\rm A}$ ): differences with respect to the solution P03 provided in this paper.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4068f7.eps} \end{figure}$ Figure 7: Comparisons of models for the precession of the equator (quantity $\omega _{\rm A}$ ): differences with respect to the solution P03 provided in this paper.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{4068f1.eps} \end{figure}$	Figure 1: Rotation angles $\phi$ and $\epsilon$ to rotate from equatorial to ecliptic frame.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{4068f2.eps} \end{figure}$	Figure 2: Differences P(DE406) - P(VSOP) in $P= \sin\pi\sin\Pi$ .
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{4068f3.eps} \end{figure}$	Figure 3: Differences Q(DE406) - Q(VSOP) in $Q=\sin\pi \cos\Pi$ .
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{4068f4.eps} \end{figure}$	Figure 4: Comparisons of models for the precession of the ecliptic (quantity $P_{\rm A}$ ): differences with respect to the solution P03 provided in this paper.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{4068f5.eps} \end{figure}$	Figure 5: Comparisons of models for the precession of the ecliptic (quantity $Q_{\rm A}$ ): differences with respect to the solution P03 provided in this paper.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4068f6.eps} \end{figure}$	Figure 6: Comparisons of models for the precession of the equator (quantity $\psi _{\rm A}$ ): differences with respect to the solution P03 provided in this paper.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.3cm,clip]{4068f7.eps} \end{figure}$	Figure 7: Comparisons of models for the precession of the equator (quantity $\omega _{\rm A}$ ): differences with respect to the solution P03 provided in this paper.
Open with DEXTER