\begin{table}%t1
\caption{The correlation coefficients $\rho$ and their significance as derived from Fig.~\ref{Probability92} for all the pulsars (right column) and for only pulsars with a~$S/N\geq100$.}\label{Probability92Table}
%\centering
$$
\begin{tabular}{llr@{$\;$}lr@{$\;$}l}
\hline
\hline
Parameter & Function & \multicolumn{2}{c}{$\rho$ ($S/N\geq 100$)} & \multicolumn{2}{c}{$\rho$ (all)}\\
\hline
& & & & \\[-8pt]
$a_1=r_{\rm p}/h$ & $5\frac{\displaystyle(\dot P/10^{-15})^{2/7}}{\displaystyle (P/1{\rm s})^{-9/14}}$ & $-0.30\!$&$^{+0.02}_{-0.02}$ & $-0.30\!$&$^{+0.02}_{-0.01}$\\[10pt]
$a_2\propto B_{\rm s}/P^2$ & $\sqrt{\dot PP^{-3}}$                    & $-0.30\!$&$^{+0.02}_{-0.02}$ & $-0.31\!$&$^{+0.02}_{-0.02}$\\[3pt]
$a_3\propto B_{\rm s}$ & $\sqrt{P\dot P}$                             & $-0.2\!$&$^{+0.3}_{-0.2}$    & $0.0\!$&$^{+0.5}_{-0.5}$\\[3pt]
$a_4\propto B_{\rm lc}$ & $\sqrt{\dot P/P^{-5}}$                      & $-0.27\!$&$^{+0.04}_{-0.02}$ & $-0.29\!$&$^{+0.02}_{-0.01}$\\[3pt]
$P$ & $P$                                                                & $0.1\!$& $^{+0.3}_{-0.4}$    & $0.21\!$&$^{+0.01}_{-0.03}$\\[3pt]
$\dot P$ & $\dot P$                                                      & $-0.21\!$&$^{+0.12}_{-0.08}$  & $-0.2\!$&$^{+0.1}_{-0.1}$\\[3pt]
Age & $\frac{1}{2}P/\dot{P}$                                             & $0.26\!$&$^{+0.02}_{-0.04}$  & $0.22\!$&$^{+0.03}_{-0.02}$\\[3pt]
\hline
\end{tabular}
$$
\end{table}