\begin{table}%t5
\caption{Parameters of the dark matter halos. The first column labels
the models. The mass-to-light ratio ${M/L}_{{R}}$ and
the dark matter fraction are calculated for two~radii
($7.5~{\rm kpc} \simeq R_{{\rm eff}}$ and $30~\rm kpc$
is the radius within which the GCs used in the analysis are found).
From the NFW~parameters of our model halos, we calculate the virial
radius, the virial mass, and the {{concentration parameter}} 
${{(c_{\rm{vir}}= {R}_{{\rm vir}}/r_{{\rm dark}})}}$ using the definitions
of Bullock et~al. (\cite{bullock2001}). Then we give the total mass
within 30~kpc, the mass-to-light ratios ($R$-band), and the dark matter
fraction within 30~kpc and 7.5~kpc (effective radius).
Note that the virial quantities were calculated for the dark halos  without adding the stellar component. Thus, the virial masses presented below are lower limits. } \label{tab:halos}
%\centering
\small
\begin{tabular}{crrlclllcllll}
\hline \hline
% & & & & & & & & & & & & \\[-8pt]
 \# & $\beta$ & $r_{{\rm dark}}$ &
 $\varrho_{{\rm dark},0}$ & rms & ${R}_{{\rm vir}}$ &
 ${M}_{{\rm vir}}$ & $c_{{\rm vir}}$ &
 ${M}_{{\rm < 30~kpc}}$ &
 ${M/L}_{{R}}$ & $\frac{M_{{\rm dark}}}{M_{{\rm total}}}$& ${M/L}_{{R}}$ &
 $\frac{M_{{\rm dark}}}{M_{{\rm total}}}$\\ & & [kpc] & {\small{$[{M}_{\odot}~{\rm pc}^{-3}]$}} & $[\rm km~s^{-1}]$ & [kpc] & [$10^{12}~{M}_{\odot}$] & $\quad$ & $ [10^{11}~{M}_{\odot}]$ & \multicolumn{2}{c}{$(r=30~\rm{kpc})$}& \multicolumn{2}{c}{ $(r=7.5~\rm{kpc})$ } \\ \hline
% & & & & & & & & & & & & \\[-8pt]
&\multicolumn{12}{l}{${M/L}_{{R}}= 6.8$, $\sigma_{{\rm los}}(27~\rm kpc) = 121~\rm{km~s}^{-1}$ (cf.~Fig.~\ref{mod68}, left panels)}  \\ \hline
1& $-2.0$ & 5 & 0.12 & 23 & 207 & $ 0.52 $ & 41.4 & 5.5  & 10.9 & 0.37 & 9.6 & 0.29\\  
2&$-0.5$ & 10 & 0.033 & 20 & 255 & $ 0.96 $ & 25.5 &5.5 & 12.0 & 0.43 & 9.4 & 0.27 \\  
3&$ 0$ & 40 & 0.003 & 21 & 395 & $3.6 $ & 9.9 & 6.6   & 13.1 & 0.48 & 8.4 & 0.19 \\  
4&$0.5$ & 120 & 0.00075 & 26  & 655 & $16.6 $ & 5.5 &7.2  & 14.3 & 0.52 & 8.2 &0.17 \\  
5&$1.0$ & 240 & 0.00050 &  46 & 1100  & 77.9 & 4.57 &9.2  & 18.3 & 0.63 & 8.7 & 0.22 \\ \hline
% & & & & & & & & & & & & \\[-8pt]
&\multicolumn{12}{l}{${M/L}_{{R}}= 4.3$,   ${\sigma_{{\rm los}}(27~\rm kpc) = 121~\rm{km~s}^{-1}}$ (cf.~Fig.~\ref{mod43}, left panels)} \\ \hline
6&$- 2.0$ & 5 & 0.195 & 22 & 248 & $ 0.90 $ & 49.6 &5.5 & 10.9 & 0.61 &8.9& 0.52\\  
7&$- 0.5$ & 5 & 0.230 & 20 & 264 & $ 1.01 $ & 52.8 &6.1 & 12.1&0.64 &9.7&0.56\\  
8&$0$     & 20 & 0.0135 & 20 & 358 & 2.7 & 17.9 &5.3 & 10.6 & 0.59 &5.9& 0.27\\
9&$0.5$     & 120 & 0.00100 & 25 & 743 & 24.1 & 6.2 &7.2 &14.3& 0.70&6.2& 0.30\\
10&$1.0$      & 120 & 0.00145 & 45 & 870 & 39.0 & 7.3 &9.4 &18.7& 0.77&7.0&0.37\\
\hline  
% & & & & & & & & & & & & \\[-8pt]
&\multicolumn{12}{l}{${M/L}_{{R}}= 6.8$,  $\sigma_{{\rm los}}(27~\rm kpc) = 227~\rm{km~s}^{-1}$   (cf.~Fig.~\ref{mod68}, right panels)} \\ \hline
11&$- 2.0$ & 120 & 0.0012 & 18 & 803 & $30.5  $ & 6.7 &9.4 & 18.7&0.64&  9.0& 0.25\\  
12&$- 0.5$ & 80 & 0.0019 & 25 & 650 & $ 16.0 $ & 8.1 &9.0  & 26.7&0.75&   10.5& 0.35 \\  
13&$ 0.0$ & 120 & 0.0011 & 32 & 773 & $ 27.2 $ & 6.4 & 9.0  & 17.7& 0.62& 8.8 & 0.23\\  
14&$ 0.5$ & 120 & 0.0012 & 47  & 803 & $ 30.5 $ & 6.7 &9.5  &18.7& 0.64& 9.0 & 0.25\\  
\hline
 %& & & & & & & & & & & & \\[-8pt]
&\multicolumn{12}{l}{${M/L}_{{R}}= 4.3$,  $\sigma_{{\rm los}}(27~\rm kpc) = 227~\rm{km~s}^{-1}$  (cf.~Fig.~\ref{mod43}, right panels) } \\ \hline
15&$ - 2.0 $ & 80 & 0.0023 & 16 & 703 & $ 20.4 $ & 8.8 &9.0 &18.0&0.76&7.1&0.39\\  
16&$- 0.5$ & 120 & 0.0011 & 24 & 774 & $ 27.3 $ & 6.5 &7.7  &15.2&0.72&6.3& 0.32\\  
17&$ 0.0$ & 120 & 0.00135 & 27 & 845 & $ 35.4 $ & 7.0 &9.0  &17.7&0.76 &6.8&0.37\\  
18&$ 0.5$ & 120 & 0.0014 & 42 & 858 & $ 37.0 $ & 7.15 &9.2  &18.2&0.76&6.9& 0.38\\  
\hline
\end{tabular}
\end{table}