\begin{table}%T1
\caption{Upper limits for $w$ obtained for the assumed values of $\Omega_{{\rm m0}}$ and 
$t_{{\rm GC}}$ at 68\% and 95\% c.l. for globular cluster formation at $z=3$.}
\label{table1}
%\centering
\par
\begin{tabular}{ccccc}
\hline\hline
\noalign{\smallskip}
$t_0$ (Gyr) & $\Omega_{{\rm m0}}$ & $t_{{\rm GC}}$ (Gyr) & $w$ &~$H_0$ (km\ s$^{-1}$\ kpc$^{-1}$) \\
\noalign{\smallskip}
\hline
\noalign{\smallskip}
13.53	& 0.295 & 11.45 & $-$1.21 & 72 \\
11.98	& 0.295 & 10.00 & $-$0.56 & 72 \\
13.66	& 0.260 & 11.45 & $-$1.02 & 72 \\
12.06	& 0.260 & 10.00 & $-$0.52 & 72 \\
13.73	& 0.295 & 11.45 & $-$0.83 & 64 \\
11.88	& 0.295 & 10.00 & $-$0.25 & 64 \\
13.82	& 0.260 & 11.45 & $-$0.57 & 64 \\
11.92	& 0.260 & 10.00 & $-$0.23 & 64 \\
\hline
\end{tabular}
\end{table}