\begin{table}%T2
\par
%\centering
\par
\caption{\label{tab:our_model}Numerical values used in this study.~$H$,~$\psi_1$ and~$\omega_1$ are integration constants.}
\begin{tabular}{cl}
\hline
\hline
\noalign{\smallskip}
\multicolumn{2}{c}{Initial values at J2000.0}           \\
\noalign{\smallskip}
\hline
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$H$                             &~$H_{\mbox{\scriptsize MHB}}=3.27379492 \times 10^{-3}$ \\   
\noalign{\smallskip}
$\psi_1$                        &~$5038\farcs481507$/cy                  \\
\noalign{\smallskip}
$\omega_1$                      &~$-0\farcs02575$/cy                     \\
\noalign{\smallskip}
\noalign{\smallskip}
\noalign{\smallskip}
$p_1$                           &~$5028\farcs796195$/cy                  \\
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$\chi_1$                        &~$10\farcs556403$/cy                    \\
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$\epsilon_0$                    &~$84~381\farcs406 = 23^{\circ} 26' 21\farcs406$  \\
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\hline
\noalign{\smallskip}
\multicolumn{2}{c}{}  \\
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\hline
\hline
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\multicolumn{2}{c}{Contributions to the precession rate in longitude (in~$''$/cy)}   \\
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\hline
\noalign{\smallskip}
Lunisolar first order           &~$~~5494.062986 \times \cos \epsilon_0 \simeq 5040.7047$   \\
Planetary first order           &~$~~0.031$                  \\ 
Geodesic precession             &~$-1.919882$              \\
\hline
\end{tabular}
\end{table}