\begin{table}%ta3
\caption{\label{tab:srcdata2}Fit results with the broken power law model. Columns: (1) source name; (2) absorbing column density  
[$10^{20}$~cm$^{-2}$]; (3) low energy photon index of the power law; (4) high energy photon index; (5) break energy~[keV]; 
(6) normalization of the power law model [$10^{-2}$~ph~cm$^{-2}$~s$^{-1}$~keV$^{-1}$ at $1$~keV]; 
(7) reduced $\chi^2$ and degrees of freedom;
(8) observed flux in the $0.4{-}10$~keV energy band [$10^{-11}$~erg~cm$^{-2}$~s$^{-1}$];
(9) intrinsic luminosity in the $0.4{-}10$ keV energy band rest frame [$10^{45}$~erg~s$^{-1}$];
(10) Ftest probability [\%]; fit with probability below~$90$\% are not reported.
The uncertainties in the parameter estimates are at the~$90\%$ confidence limits for 1 parameter. 
For $N_{{\rm H}}={\rm Gal}$, it means that the absorption column has been fixed to the Galactic value.}
\small%\centerline
{
\begin{tabular}{lccccccccc}
\hline\hline
Name         & $N_{{\rm H}}$   & $\Gamma_1$             & $\Gamma_2$             & $E_{\rm break}$      & $A$                     & $\tilde{\chi}^2$/d.o.f.   & $F$      & $L$      & $Ftest$\\
(1)         & (2)                & (3)                    & (4)                    & (5)                  & (6)                     & (7)              & (8)      & (9)      & (10)\\
\hline
$0219+428$ & Gal.              & $\rm 2.91_{-0.08}^{+0.12}$ & $\rm 2.23_{-0.09}^{+0.10}$ & $1.3\pm 0.2$         & $0.067\pm 0.003$        & $1.05/291$       & $0.24$  & $3.0$     & $>$$99.99$\\
AO~$0235+164$ & Gal.              & $2.33\pm 0.04$         & $2.1\pm 0.1$           & $\rm 3.3_{-0.5}^{+0.7}$  & $0.276\pm 0.006$        & $0.96/616$       & $0.99$  & $69$      & $>$$99.99$\\
PKS~$0521-365$ & Gal.              & $1.95\pm 0.03$         & $1.74\pm 0.03$         & $\rm 1.5_{-0.2}^{+0.3}$  & $0.227\pm 0.003$        & $1.05/1200$      & $1.3$   & $9.4\times 10^{-4}$ & $99.97$\\
S5~$0716+714^{a}$ & Gal.      & $2.70\pm 0.02$         & $\rm 1.98_{-0.09}^{+0.08}$ & $\rm 2.3_{-0.1}^{+0.2}$  & $0.293\pm 0.003$        & $1.06/417$       & $1.1$   & $>$$15.7$    & $>$$99.99$\\
S5~$0836+710$ & Gal.              & $1.25\pm 0.03$         & $1.375\pm 0.007$       & $\rm 1.01_{-0.08}^{+0.15}$& $0.529\pm 0.006$       & $1.07/2271$      & $4.8$   & $860$     & --\\
Mkn~$421^{b}$ & Gal.      & $2.573\pm 0.008$       & $\rm 2.79_{-0.08}^{+0.17}$ & $\rm 4.2_{-0.7}^{+1.0}$  & $6.97\pm 0.02$          & $0.96/1025$      & $26.1$  & $0.578$   & $99.97$\\
{}           & Gal.              & $2.340\pm 0.004$       & $2.73\pm 0.04$         & $4.0\pm 0.2$         & $22.9\pm 0.4$           & $1.06/1490$      & $91.3$  & $2.00$    & $>$$99.99$\\
{}           & Gal.           & $\rm 2.378_{-0.005}^{+0.004}$ & $\rm 2.96_{-0.10}^{+0.08}$ & $\rm 4.7_{-0.3}^{+0.2}$  & $22.6\pm 0.4$           & $1.02/1429$      & $89.1$  & $1.95$    & $>$$99.99$\\
{}           & Gal.              & $2.312\pm 0.007$       & $\rm 2.68_{-0.05}^{+0.07}$ & $4.4\pm 0.3$         & $16.4\pm 0.7$           & $0.99/1446$      & $66.7$  & $1.45$    & $>$$99.99$\\
{}           & Gal.              & $\rm 2.59_{-0.02}^{+0.01}$ & $2.81\pm 0.02$         & $\rm 2.2_{-0.2}^{+0.1}$  & $\rm 11.5_{-0.8}^{+0.7}$    & $1.08/1177$      & $41.8$  & $0.929$   & $>$$99.99$\\
{}           & Gal.              & $2.300\pm 0.007$       & $2.51\pm 0.02$         & $2.2\pm 0.1$         & $14.1\pm 0.4$           & $0.99/1306$      & $56.3$  & $1.23$    & $>$$99.99$\\
PKS~$1127-145^{c}$ & $\rm 12_{-1}^{+2}$ & $\rm 1.40_{-0.05}^{+0.08}$ & $1.22\pm 0.06$    & $\rm 2.7_{-0.8}^{+1.0}$  & $\rm 0.127_{-0.004}^{+0.006}$ & $1.00/888$       & $1.2$   & $61.0$    & $99.58$\\
ON~$231$ & Gal.              & $2.74\pm 0.02$         & $\rm 2.3_{-0.4}^{+0.3}$    & $\rm 4.2_{-1.1}^{+0.9}$  & $0.140\pm 0.002$        & $1.07/652$       & $0.51$  & $0.16$    & $94.50$\\
3C~$273$ & Gal.              & $1.943\pm 0.009$       & $1.697\pm 0.009$       & $1.48\pm 0.06$       & $2.073\pm 0.008$        & $1.13/1596$      & $12.7$  & $8.7$     & $>$$99.99$\\
{}           & Gal.              & $1.97\pm 0.01$         & $1.65\pm 0.01$         & $1.43\pm 0.08$       & $1.97\pm 0.01$          & $1.03/1399$      & $12.5$  & $8.6$     & $>$$99.99$\\
{}           & Gal.              & $1.96\pm 0.01$         & $1.67\pm 0.01$         & $1.35\pm 0.08$       & $1.91\pm 0.01$          & $1.00/1392$      & $12.1$  & $8.3$     & $>$$99.99$\\
{}           & Gal.              & $1.92\pm 0.01$         & $1.654\pm 0.009$       & $1.37\pm 0.05$       & $1.911\pm 0.008$        & $0.97/1645$      & $12.2$  & $8.4$     & $>$$99.99$\\
{}           & Gal.              & $2.121\pm 0.007$       & $1.676\pm 0.008$       & $1.45\pm 0.03$       & $2.604\pm 0.009$        & $1.10/1709$      & $15.7$  & $11.0$     & $>$$99.99$\\
{}           & Gal.              & $2.00\pm 0.02$         & $1.72\pm 0.02$         & $\rm 1.4_{-0.1}^{+0.2}$  & $3.06\pm 0.03$          & $1.00/800$       & $18.4$  & $12.7$     & $>$$99.99$\\
{}           & Gal.              & $1.94\pm 0.03$         & $1.67\pm 0.03$         & $1.5\pm 0.2$         & $2.95\pm 0.03$          & $0.95/804$       & $18.4$  & $12.6$     & $>$$99.99$\\
{}           & Gal.              & $1.97\pm 0.03$         & $\rm 1.79_{-0.04}^{+0.03}$ & $\rm 1.4_{-0.2}^{+0.4}$  & $2.29\pm 0.03$          & $1.01/678$       & $13.1$  & $9.09$     & $>$$99.99$\\
{}           & Gal.              & $2.09\pm 0.02$         & $1.81\pm 0.03$         & $1.6\pm 0.1$         & $3.39\pm 0.03$          & $0.97/788$       & $18.6$  & $13.2$     & $>$$99.99$\\
{}           & Gal.              & $2.16\pm 0.02$         & $\rm 1.83_{-0.03}^{+0.02}$ & $\rm 1.4_{-0.1}^{+0.2}$  & $2.80\pm 0.03$          & $0.99/897$       & $15.1$  & $10.8$     & $>$$99.99$\\
{}           & Gal.              & $2.13\pm 0.02$         & $\rm 1.81_{-0.05}^{+0.04}$ & $\rm 1.7_{-0.2}^{+0.3}$  & $2.88\pm 0.03$          & $0.96/709$       & $15.4$  & $10.9$     & $>$$99.99$\\
{}           & Gal.              & $2.05\pm 0.02$         & $1.76\pm 0.03$         & $1.8\pm 0.2$         & $3.51\pm 0.03$          & $1.02/824$       & $19.5$  & $13.7$     & $>$$99.99$\\
{}           & Gal.              & $2.02\pm 0.02$         & $\rm 1.82_{-0.07}^{+0.03}$ & $\rm 1.9_{-0.3}^{+0.6}$  & $3.05\pm 0.02$          & $1.00/906$       & $16.4$  & $11.6$     & $>$$99.99$\\
{}           & Gal.              & $2.02\pm 0.02$         & $1.70\pm 0.03$         & $\rm 1.7_{-0.1}^{+0.2}$  & $2.26\pm 0.02$          & $1.02/875$       & $13.2$  & $9.20$     & $>$$99.99$\\
{}           & Gal.              & $\rm 2.00_{-0.01}^{+0.02}$ & $1.76\pm 0.02$         & $\rm 1.5_{-0.1}^{+0.2}$  & $1.94\pm 0.01$          & $1.03/1158$      & $11.2$  & $7.8$      & $>$$99.99$\\
Cen~A        & {}                & {}                     & {}                     & {}                   & {}                      & {}               & {}      & {}         & --\\
{}           & {}                & {}                     & {}                     & {}                   & {}                      & {}               & {}      & {}         & --\\
PKS~$1334-127$ & Gal.              & $\rm 1.57_{-0.24}^{+0.08}$ & $1.78\pm 0.03$         & $1.0\pm 0.3$         & $\rm 0.077_{-0.003}^{+0.012}$ & $0.92/608$     & $0.43$  & $4.8$      & $92.31$\\
PKS~$1406-076$ & {}                & {}                     & {}                     & {}                   & {}                      & {}               & {} & {}              & $81.60$\\
{}           & {}                & {}                     & {}                     & {}                   & {}                      & {}               & {} & {}              & $56.30$\\
NGC~$6251$ & $14\pm 1$         & $\rm 2.11_{-0.06}^{+0.08}$ & $1.78\pm 0.07$         & $\rm 2.5_{-0.4}^{+0.3}$  & $0.141\pm 0.004$        & $1.00/810$       & $0.59$  & $0.010$    & $>$$99.99$\\
PKS~$1830-211$ & $\rm 62_{-6}^{+5}$    & $\rm 0.93_{-0.10}^{+0.08}$ & $\rm 1.42_{-0.05}^{+0.10}$ & $\rm 3.6_{-0.5}^{+0.4}$  & $0.11\pm 0.01$          & $0.83/598$       & $1.38$  & $270$      & $>$$99.99$\\
{}           & $62\pm 3$         & $\rm 0.89_{-0.09}^{+0.06}$ & $1.29\pm 0.04$         & $3.1\pm 0.3$         & $\rm 0.103_{-0.08}^{+0.06}$ & $0.97/1660$      & $1.31$  & $243$      & $>$$99.99$\\
{}           & $64\pm 3$         & $1.06\pm 0.04$         & $\rm 1.41_{-0.09}^{+0.12}$ & $\rm 4.7_{-0.4}^{+0.5}$  & $0.108\pm 0.06$         & $1.00/1166$      & $1.20$  & $248$      & $>$$99.99$\\
PKS~$2155-304^{b}$ & Gal.      & $2.588\pm 0.005$       & $\rm 2.73_{-0.08}^{+0.18}$ & $\rm 4.4_{-1.1}^{+1.4}$   & $3.861\pm 0.008$       & $1.01/1265$      & $14.3$  & $5.70$     & $>$$99.99$\\
{}           & Gal.           & $\rm 2.773_{-0.006}^{+0.007}$ & $\rm 2.88_{-0.03}^{+0.06}$ & $\rm 2.8_{-0.4}^{+0.7}$   & $3.246\pm 0.007$       & $0.98/1066$      & $11.6$  & $4.74$     & $>$$99.99$\\
{}           & Gal.              & $2.845\pm 0.006$       & $3.0\pm 0.1$           & $\rm 4.3_{-1.2}^{+0.8}$   & $2.620\pm 0.007$       & $1.02/990$       & $9.31$  & $3.86$     & $99.67$\\
{}           & Gal.              & $2.783\pm 0.006$       & $2.96\pm 0.04$         & $\rm 2.4_{-0.2}^{+0.3}$   & $5.75\pm 0.01$         & $0.97/1130$      & $20.3$  & $8.35$     & $>$$99.99$\\
{}           & Gal.              & $2.75\pm 0.03$         & $\rm 2.70_{-0.02}^{+0.01}$ & $\rm 1.0_{-0.1}^{+0.5}$   & $2.74\pm 0.02$         & $0.99/885$       & $10.0$  & $4.10$     & $96.01$\\
{}           & {}                & {}                     & {}                     & {}                    & {}                     & {}               & {}      & {}         & --\\
{}           & {}                & {}                     & {}                     & {}                    & {}                     & {}               & {}      & {}         & $89.10$\\
{}           & {}                & {}                     & {}                     & {}                    & {}                     & {}               & {}      & {}         & --\\
{}           & {}                & {}                     & {}                     & {}                    & {}                     & {}               & {}      & {}         & $85.00$\\
\hline
\end{tabular}}
\smallskip
$^{a}$ Only MOS1+MOS2, since the PN was set in TIMING. Lower limit of luminosity calculated for $z=0.5$.\\
$^{{b}}$ Fit in the $0.6{-}10$~keV energy range and extrapolation to $0.4$~keV for flux and luminosity calculations.\\
$^{{c}}$ Additional redshifted absorber (\texttt{wa*zwa(bknpo)} model in \texttt{xspec}) along the line of sight.
\end{table}