\begin{table}%t1
\caption{\label{t:tnew0}Basic parameters for globular clusters considered in this paper ($M_{\rm TO}$ and $M_{\rm RGB}$ are in solar masses).} 
\par
%\centering
\par
\begin{tabular}{lcccccccccccc}
\hline\hline \noalign{\smallskip}
Cluster & Other & [Fe/H] & $(m-M)_V$ & $E(B-V)$ & $M_{\rm V}$ & HBR & Age & $M_{\rm TO}$ & $M_{\rm RGB}$ 
& IQR$_{\rm [Na/O]}$ &  IQR$_{\rm [Al/Mg]}$ & $\log{T_{\rm eff}^{\rm max}}$(HB)\\
         & & dex   &    mag    &   mag   & mag           &     &    &  $M_\odot$   & $M_\odot$ 
& dex                & dex                  & K \\
\hline
NGC~104  &47 Tuc&--0.76 &13.37 & 0.04 &--9.42 & --0.99 & 0.95 & 0.862 & 0.909 &0.472 & 0.091 &3.756 \\
NGC~288  &      &--1.32 &14.83 & 0.03 &--6.74 &  0.98 & 0.90 & 0.827 & 0.869 &0.776 & 0.059 &4.221	\\
NGC~362  &      &--1.30 &14.81 & 0.03 &--8.41 & --0.87 & 0.80 & 0.858 & 0.900 &0.670 &	     &4.079 \\
IC~1257  &      &--1.73 &19.25 & 0.73 &--6.15 & --0.71 &      &       &       &      &	     &	    \\  
NGC~1261 &      &--1.27 &16.10 & 0.01 &--7.81 &  1.00 & 0.79 & 0.847 & 0.887 &      &	     &4.079 \\
\hline
\end{tabular}
\tablefoot{{The complete table is available at the~CDS.}}
\end{table}