\begin{table}%t6
\caption{\label{tab:bergond}Jeans modelling best fit parameters.}
\small
 %\centering
\par
\begin{tabular}{rlrrllllrrrlr}\hline \hline\noalign{\smallskip}
&&&\multicolumn{7}{|c}{NFW dark halo} & \multicolumn{3}{|c}{Burkert halo}\\
  & & \multicolumn{1}{r|}{$\beta$} & $r_{\rm s}$ & $\varrho_S$ & $\chi^2$ &$\chi^2/\nu$&$M_{\rm{vir}}$&
$R_{\rm{vir}}$&\multicolumn{1}{c|}{$c_{\rm{vir}}$} & $r_{0}$ & $\varrho_0$ & $\chi^2$\\ 
\par
&  &  \multicolumn{1}{r}{} & \multicolumn{1}{|r}{$[\rm{kpc}]$} & $[M_{\odot}~\rm{pc}^{-3}]$ & & &$[10^{12}M_{\odot}]$ &$[\rm{kpc}]$& \multicolumn{1}{c}{}& \multicolumn{1}{|c}{$[\rm{kpc}]$}  & $[M_{\odot}~\rm{pc}^{-3}]$\\
\par
&   \multicolumn{1}{l}{(1)} & \multicolumn{1}{r|}{(2)} & (3) &(4) &(5) &(6) &(7)& (8)&\multicolumn{1}{c|}{(9)} &(10) & (11) & (12)\\
\par
  \hline
\par
  \multicolumn{10}{l}{{{({\it{a}}) NGC~1399 GC data (R\textsc{iii} and B\textsc{iii}):}}}\\ \hline
\par
\it{a1}  &Red (R\textsc{iii})&$-0.5$ & 14 & 0.055 & 0.72 & 0.24 & 4.7& 430 & 31  & 11 & 0.0896 & 0.49\\
\it{a2}  &Red (R\textsc{iii})& 0     & 16 & 0.042 & 0.85 & 0.28 & 5.2& 450 & 28  & 12 & 0.0776 & 0.57\\
\it{a3}  &Red (R\textsc{iii})&$+0.5$ & 24 & 0.019 & 1.02 & 0.34 & 7.9& 490 & 20  & 16 & 0.0447 & 0.72 \rule[-1.5ex]{0ex}{2ex}\\ 
\par
%=================== BLUE
\it{a4}  &Blue (B\textsc{iii})&$-0.5$ & 101      & 0.00271 & 8.5 & 2.1 & 51 & 950   & 9  & 35 & 0.0213 & 6.9\\
\it{a5}  &Blue (B\textsc{iii})&0      & 174      & 0.00099 & 9.5 & 2.4 & 73 & 1075  & 6  & 46 & 0.0119 & 8.0\\
\it{a6}  &Blue (B\textsc{iii})&$+0.5$ &$\geq$$ 200$& 0.00061 & 12  & 3.0 & 58 & 1000  & 5  & 94 & 0.0031 & 9.9\\
\hline
\it{a7}  &\multicolumn{2}{l}{$\rm{Red}_{0.0}$ and $\rm{Blue}_{0.0}$}   & 63 & 0.0038 & 28& 2.8 & 18& 680 & 11 &25 & 0.0237 & 28\\ 
%\hline
\it{a8}  &\multicolumn{2}{l}{$\rm{Red}_{+0.5}$ and $\rm{Blue}_{-0.5}$} & 37 & 0.0110 & 29& 2.9 & 13& 610&  16 & 20 &0.0388 & 27 \\ 
\hline
\it{a9}  &\multicolumn{2}{l}{$\rm{Red}_{0.0}$ and  $\rm{Stars}_{0.0}$}  & 23 & 0.0190 &  8.3& 0.42 &6.1 & 470& 20 & 9 & 0.1343& 14\\ 
\it{a10} &\multicolumn{2}{l}{$\rm{Red}_{0.0}$ and  $\rm{Stars}_{+0.5}$} & 34 & 0.0088 &  7.3& 0.37 &8.0 & 510& 15 & 12 &0.0728& 8.7 \\\hline  
  \multicolumn{10}{l}{{{({\it{b}}) NGC~1399 GCs, extended data set  including  the Bergond et~al.~(\citeyear{bergond07}) GC data (R\textsc{v} and B\textsc{v}):}}}\\ \hline
\it{b1}  &Red (R\textsc{v})&$-0.5$& 12 & 0.093 & 3.8 & 0.63 &5.4& 450& 38 &  9 & 0.166 & 3.4\\ 
\it{b2}  &Red (B\textsc{v})& 0    & 14 & 0.069 & 4.0 & 0.67 &6.1& 470& 34 & 11 & 0.112  & 3.5\\
\it{b3}  &Red (B\textsc{v})&$+0.5$& 19 & 0.038 & 4.5 & 0.75 &7.6& 510& 27 & 14 & 0.071&3.9 \rule[-1.5ex]{0ex}{2ex}\\
  %====================== BLUE GCS ==========================
\it{b4}  &Blue (B\textsc{v})&$-0.5$ & 36 & 0.0140 & 14 & 2.0 & 17 & 660 &18 & 22 & 0.0416 & 11\\
\it{b5}  &Blue (B\textsc{v})&0      & 50 & 0.0071  & 16 & 2.3 & 20 & 690 &14 & 28 & 0.0243 & 13\\
\it{b6}  &Blue (B\textsc{v})&$+0.5$ & 94 & 0.0018  & 19 & 2.7 & 25 & 750 & 8 & 43 & 0.0094 & 16\\
 \hline 
\it{b7}  &\multicolumn{2}{l}{$\rm{Red}_{0.0}$ and  $\rm{Blue}_{0.0}$ }   & 35 & 0.012 &  29&1.8 &13 &600&17 & 20 & 0.03876 & 27 \\ 
\it{b8}  &\multicolumn{2}{l}{$\rm{Red}_{+0.5}$ and  $\rm{Blue}_{-0.5}$ } & 20 & 0.019 &  27& 1.7&13 &590&20 & 18 & 0.05124 & 24\\   
\hline
\it{b9}  &\multicolumn{2}{l}{$\rm{Red}_{0.0}$ and  $\rm{Stars}_{0.0}$ }  & 30 & 0.013 &  13&0.57&8.9&535&18 & 11 &0.1064  & 19 \\ 
\it{b10}
  &\multicolumn{2}{l}{$\rm{Red}_{0.0}$ and  $\rm{Stars}_{+0.5}$} & 38 & 0.0077 &  14& 0.61&9.5 &545&14 &15 & 0.05653 & 14\\ 
  \hline  
   \multicolumn{10}{l}{{{({\it{c}}) Stellar velocity dispersion profile (data from Saglia et~al.~\citeyear{saglia00}):}}}\\ 
\hline
\it{c1} & Stars&0        & 23 & 0.019  & 7.3 & 0.52 &   6.1 & 470 &20  & 5  & 0.2996 & 10\\
\it{c2} & {Stars}&$+0.5$ & 47 & 0.0055 & 5.5 & 0.39&  12  & 590 &13  & 8 & 0.12545 & 7.5 \\  \hline
\label{tab:models}
\end{tabular}\vspace*{-3mm}
\tablefoot{Model identifiers:  
 {\it{(a)}} using our GC
  dataset (i.e.~samples R\textsc{iii} and B\textsc{iii}), {\it{(b)}}
  using the extended data set including the values from
  \cite{bergond07} (R\textsc{v} and B\textsc{v}), and {\it{(c)}} for
  the stellar velocity dispersion profile by \cite{saglia00}.  The
  tracer population is given in the first column, the anisotropy
  parameter $\beta$ in the second. Columns 3 and 4 list the best-fit
  NFW halo parameters. The following columns give the $\chi^2$ and
  $\chi^2/\nu$, where $\nu$ is the number of degrees of freedom
  (i.e. $k-1-p$, where $k$ is the number of data points and $p=2$ the
  number of free parameters). Columns 7--9 give the virial parameters
  of the dark halos, as defined by Bullock et~al.~(2001),
  i.e.~assuming a density contrast of $\Delta=337$. The parameters for
  the \cite{burkert95} halo are shown in Cols.~10--12.}
  \vspace*{-2mm}
\end{table}