\begin{table}%t2 %\centering \par \caption{\label{t:tabnoi}Quantities for the same GCs, derived by our works.} \begin{tabular}{rccrrrcccccc} \hline\hline\noalign{\smallskip} NGC & $\log T_{\rm eff}^{\rm max}$ & IQR[Na/O] \tablefootmark{1} & $P$ \tablefootmark{2} & $I$ \tablefootmark{2} & $E$ \tablefootmark{2} &$\langle [\alpha/{\rm Fe}] \rangle$ \tablefootmark{3} & [(Mg+Al+Si) &[Mg/Fe]$_{\max}^6$&[Mg/Fe]$_{\min}^6$&[Si/Fe]$_{\rm min}^6$& [Si/Fe]$_{\rm max}^6$\\ & (HB) &&& && & /Fe]$^6$ & & & \\ \hline \noalign{\smallskip} 104 &3.756$^4$ &0.472 & 27 & 69 & 4 &0.42 &0.46 &0.60& +0.47& 0.35& 0.43\\ 288 &4.221$^5$ &0.776 & 33 & 61 & 6 &0.42 &0.41 &0.55& +0.41& 0.30& 0.41\\ 1904 &4.352$^4$ &0.759 & 40 & 50 &10 &0.31 &0.31 &0.40& +0.16& 0.25& 0.34\\ 2808 &4.568$^4$ &0.999 & 50 & 32 &18 &0.33 &0.29 &0.42& $-$0.30& 0.22& 0.38\\ 3201 &4.079$^4$ &0.634 & 35 & 56 & 9 &0.33 &0.32 &0.45& +0.27& 0.25& 0.41\\ 4590 &4.041$^4$ &0.372 & 40 & 60 & 0 &0.35 &0.40 &0.48& +0.28& 0.30& 0.48\\ 5904 &4.176$^4$ &0.741 & 27 & 66 & 7 &0.38 &0.36 &0.55& +0.31& 0.21& 0.39\\ 6121 &3.968$^5$ &0.373 & 30 & 70 & 0 &0.51 &0.54 &0.65& +0.50& 0.45& 0.64\\ 6171 &3.875$^4$ &0.522 & 33 & 60 & 7 &0.49 &0.53 &0.60& +0.46& 0.45& 0.63\\ 6218 &4.217$^4$ &0.863 & 24 & 73 & 3 &0.41 &0.43 &0.60& +0.46& 0.22& 0.43\\ 6254 &4.400$^5$ &0.565 & 38 & 60 & 2 &0.37 &0.37 &0.58& +0.33& 0.18& 0.36\\ 6388 &4.255$^4$ &0.795 & 41 & 41 &19 &0.22 &0.30 &0.40& +0.16& 0.20& 0.46\\ 6397 &3.978$^4$ &0.274 & 25 & 75 & 0 &0.36 & &0.55& +0.40& 0.25& 0.43\\ 6441 &4.230$^4$ &0.660 & 38 & 48 &14 &0.21 &0.34 &0.45& +0.20& 0.15& 0.45\\ 6752 &4.471$^5$ &0.772 & 27 & 71 & 2 &0.43 &0.44 &0.60& +0.36& 0.28& 0.49\\ 6809 &4.153$^5$ &0.725 & 20 & 77 & 2 &0.42 &0.43 &0.60& +0.18& 0.30& 0.51\\ 6838 &3.763$^4$ &0.257 & 28 & 72 & 0 &0.40 &0.44 &0.60& +0.39& 0.30& 0.51\\ 7078 &4.477$^4$ &0.501 & 39 & 61 & 0 &0.40 &0.46 &0.68& $-$0.01& 0.28& 0.60\\ 7099 &4.079$^4$ &0.607 & 41 & 55 & 3 &0.37 &0.44 &0.60& +0.44& 0.20& 0.45\\ \hline \end{tabular} \tablefoot{ \tablefoottext{1}{IQR([Na/O]) comprises stars with GIRAFFE and UVES data;} \tablefoottext{2}{$P,I,E$ are fraction of stars of Primordial, Intermediate, Extreme populations from Paper~VII;} \tablefoottext{3}{[$\alpha$/Fe] is the average of [Mg/Fe]$_{\rm max}$, [Si/Fe]$_{\rm min}$ and [Ca/Fe];} \tablefoottext{4}{$\log T_{\rm eff}^{\rm max}$(HB) taken from Recio-Blanco et~al. (\cite{Recio2006});} \tablefoottext{5}{$\log T_{\rm eff}^{\rm max}$(HB) derived in the present work (see Sect.~5.2);} \tablefoottext{6}{from Paper~VIII.}} \end{table}