Table 1: The correlation coefficients $\rho $ and their significance as derived from Fig. 8 for all the pulsars (right column) and for only pulsars with a  $S/N\geq 100$.
\begin{displaymath}\begin{tabular}{llr@{$\;$}lr@{$\;$}l} \hline \hline Parameter... ...04}$ & $0.22\!$&$^{+0.03}_{-0.02}$\\ [3pt] \hline \end{tabular}\end{displaymath}


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