\begin{table}%T3
\caption{\label{tab:bepposax}Best fit model parameters for the 15 AGN from the \emph{BeppoSAX} catalogs by Giommi et~al.~(\cite{Giommi2002}) and 
Donato et~al.~(\cite{Donato2005}). The values are the weighted averages obtained from multiple observations (if any) and
from the two catalogs. In the case of 3C~$273$ (3EG~J$1229-0210$) there were 9 observations, 5 best fitted with a broken
power law and 4 with a single power law model: both model averages are reported. For NGC~$6251$ (3EG~J$1621+8203$) the 
average is obtained from Chiaberge et~al. (\cite{Chiaberge2003}) and Guainazzi et~al. (\cite{Guainazzi2003}) from a fit in the energy band $0.1{-}200$~keV. 
Grandi et~al. (\cite{Grandi2003}) is the reference for Cen~A (3EG~J$1324-4314$), from a fit in the energy band $0.4{-}250$~keV excluding
the $5.5{-}7.5$~keV band (iron emission line). The value for PKS~$1830-211$ (3EG~J$1832-2110$) has been obtained by De~Rosa
et~al. (\cite{Rosa2005}) from a fit in the energy band $0.5{-}80$~keV (\emph{Chandra} and \emph{INTEGRAL}).
Columns: (1) name of the source; (2) absorbing column density [$10^{20}$~cm$^{-2}$]; (3)~photon index
$\Gamma$, if the best fit is a simple power law model or soft photon index $\Gamma_1$, if the best fit
model is a broken power law; (4) hard photon index $\Gamma_2$ for the broken power law model; (5) break energy~[keV].}
\small%\centering
\par
\begin{tabular}{lcccc}
\hline\hline
Name          & $N_{\rm H}$     & $\Gamma$/$\Gamma_1$    & $\Gamma_2$             & $E_{\rm break}$ \\
(1)          & (2)             & (3)                    & (4)                    & (5)             \\
\hline
$0219+428$   & Gal.            & $2.22\pm 0.06$         & $-$                    & $-$\\
AO~$0235+164$ & Gal.            & $2.0\pm 0.1$           & $-$                    & $-$\\
PKS~$0521-365$ & Gal.            & $1.74\pm 0.02$         & $-$                    & $-$\\
S5~$0716+714$ & Gal.            & $2.5\pm 0.2$           & $1.8\pm 0.1$           & $3.0\pm 0.4$\\
S5~$0836+710$ & $\rm 78_{-35}^{+55}$& $1.31\pm 0.02$         & $-$                    & $-$\\
Mkn~$421$     & Gal.            & $1.9\pm 0.2$           & $2.3\pm 0.3$           & $1.3\pm 0.8$\\
PKS~$1127-145$ & Gal.            & $1.42\pm 0.05$         & $-$                    & $-$\\
ON~$231$      & Gal.            & $2.58\pm 0.01$         & $1.52\pm 0.06$         & $2.8\pm 0.2$\\
3C~$273$      & Gal.            & $2.0\pm 0.1$           & $1.603\pm 0.006$       & $0.9\pm 0.3$\\
{}            & Gal.            & $1.58\pm 0.03$         & $-$                    & $-$\\
Cen~A         & $\rm 1020_{-40}^{+90}$  & $\rm 1.80_{-0.04}^{+0.03}$ & $-$                    & $-$\\
PKS~$1334-127$ & $-$             & $-$                    & $-$                    & $-$\\
PKS~$1406-076$ & $-$             & $-$                    & $-$                    & $-$ \\
NGC~$6251$     & $9\pm 1$        & $1.79\pm 0.06$         & $-$                    & $-$\\
PKS~$1830-211$ & $\rm 194_{-25}^{+28}$ & $1.09\pm 0.05$       & $-$                    & $-$\\
PKS~$2155-304$ & Gal.            & $2.3\pm 0.1$           & $2.8\pm 0.1$           & $1.7\pm 0.2$ \\
\hline
\end{tabular}
\end{table}