\begin{table}%t1
\caption{
Prominent peaks in the power spectrum of Procyon identified
as mode oscillation frequencies (in $\rm\mu Hz$) in terms of $n$ and $l$.}
%\centerline
{
\begin{tabular}{cccc}
\hline\hline
$n^\dagger$&$l=0$&$l=1$&$l=2$\\
\hline
7& &524.5 &\\
9&608.4&&\\
11&&&770.0\\
12&778.7&$(808.6)^\ddagger$&\\
13&834.3&&\\
18&1114.2&1138.8&\\
20&1224.2&1252.0&\\
22&1335.4&&\\
\hline
\end{tabular}}
% %\end{center}
\par
{\tiny {$\dagger$ Deduced from the fit to the asymptotic relationship (\ref{AsymptoticRel}).}\\
{$\ddagger$ Excluded from the fit because of its large deviation from the asymptotic relationship, though the related peak in the power spectrum is a high {\it S/N} one.}}
\label{FI}
\end{table}