\begin{table}%t1
\caption{Influence  of  the Cepheid bias on the Hubble constant from long-range distance criteria.\label{Table1}}
%\centerline
{\begin{tabular}{lll}
\hline\hline
Method                              & Uncorrected $H_0$&  Corrected $H_0$ \\
\hline
SNIa           &   $71\pm2$  km~s$^{-1}$~Mpc$^{-1}$   &    $60$  km~s$^{-1}$~Mpc$^{-1}$     \\
TF relation    &   $71\pm3$   &    $58      $   \\
FP method$^\dag$ &   $82\pm6$   &    $60      $   \\
SBF            &   $70\pm5$   &    $61      $  \\
SNII           &   $72\pm9$   &    $65      $  \\
\hline     
Weighted mean  &   $72\pm2.7$ &    $60\pm1.3$  \\
\hline
\end{tabular}}
\par
\smallskip
$^{\dag}$ Based on the distances of Virgo, Fornax and Leo.
\par
\end{table}