\begin{table}%t3
\caption{\label{X}Main results obtained from the analysis of the \mbox{X-ray} spectra of the 17~sources of the present sample.}
 
 \begin{tabular}{lcccccccccr}
\hline \hline\noalign{\smallskip}
\multicolumn{1}{c}{Source} & \multicolumn{1}{c}{RA} &\multicolumn{1}{c}{Dec} &$N_{\rm H}$ Gal & $N^{\bullet}_{\rm H}$  &  $\Gamma^{+}$  & $F_{(2-10)~{\rm keV}}$ &$F_{(14-195)~{\rm keV}}$& $L_{\rm X}$&Ref.$^{*}$ \\
& & & $\times 10^{22}$~cm$^{-2}$   &$\times 10^{22}$~cm$^{-2}$  & &$\times 10^{-12}$~erg~s$^{-1}$~cm$^{-2}$&$\times 10^{-11}$~erg~s$^{-1}$~cm$^{-2}$& 10$^{43}$~erg~s$^{-1}$ &\\
\hline\noalign{\smallskip}
Swift J0059.4+3150$^{A}$ &00 59 53.29  & +31 49 36.6 &0.055& --& $\rm 1.67^{+0.03}_{-0.03}$ & 7.3 & 4.2& 0.6 (2--10)&1\\ 
& & & & & & & & 3.1 (14--195)&\\
& & & & & & & & &\\
Swift J0134.1$-$3625$^{A}$ & 01 33 57.71 & $-$36 29 38.4 &0.019& $\rm 75^{+34}_{-21}$ & [1.8]  & 1.9& 5.4& 0.8 (2--10)&1  \\
& & & & & & & &7.2 (14-195) & \\
& & & & & & & & & \\
Swift J0342.0$-$2115$^{A}$  &03 42 03.62 & $-$21 14 39.6 &0.023 & --& $\rm 1.94^{+0.05}_{-0.05}$&23.8&4.6&$\sim$1.3 (2--10)&1 \\
& & & & & & & &1.8 (14--195) &\\
& & & & & & & & &\\
Swift J0350.1$-$5019$^{A}$  &03 50 23.08 &$-$50 18 11.4  &0.012& $\rm 17^{+9}_{-7}$ & [1.8]& 3.1&3.1&1.0 (2--10) &1\\ 
& & & & & & & &9.5 (14--195) &\\
Swift J0505.7$-$2348$^{A}$ &05 05 45.70 &$-$23 51 13.3 & 0.021&$\rm 6^{+0.5}_{-0.5}$& $\rm 1.4^{-0.4}_{+0.3}$& 15.5 &7.2&5.3 (2--10)&1 \\
& & & & & & & &21.6 (14--195) &\\
& & & & & & & & &\\
Swift J0501.9$-$3239$^{A}$&05 19 35.82  &$-$32 39 26.6  & 0.018&--& $\rm 1.45^{+0.05}_{-0.05}$ &13.6&6.2&0.5 (2--10)&1 \\
& & & & & & & &1.2 (14--195) &\\
& & & & & & & & &\\
Swift J0640.1$-$4328$^{A}$&06 40 37.89  & $-$43 21 19.8& 0.025 &$\rm 11.7^{+4.5}_{-3.6}$ &[1.8]& 2.2&2.0&2.3 (2--10)&1\\
& & & & & & & & 28.9 (14--195)&\\
& & & & & & & & &\\
Swift J0727.5$-$2406$^{C}$ & 07 27 21.05& $-$24 06 32.2 &0.650&--& --&0.6&2.2& 2.7 (2--10)&2 \\
& & & & & & & & 93.2 (14--195)&\\
& & & & & & & & &\\
& & & & $\rm 47^{+13}_{-12}, { [0.7]}$ & & & & &\\
Swift J0739.6$-$3144$^{B}$ &07 39 44.61& $-$31 43 01.6& 0.431 &  & { $\rm 1.77^{+0.07}_{-0.09}$} &0.9&2.5&0.2 (2--10)&2\\
& & & & $\rm 14^{+2.3}_{-1.9},{ [0.9]}$ & & & &4.5 (14--195) &\\
& & & & & & & & &\\
& & & & & & & & &\\
Swift J0743.0$-$2543$^{B}$&07 43 14.95 &$-$25 45 44.3  & 0.581& -- & --& 14.7$^{\triangle}$  &2.0& 2.1 (2--10)&2\\
& & & & & & & &2.8 (14--195) &\\
& & & & & & & & &\\
Swift J0811.5+0937$^{C}$&08 11 30.99& +09 33 51.6 &0.024 &--& -- & 0.1&2.6&3.0 (2--10) &2 \\
& & & & & & & &778.1 (14--195) &\\
& & & & & & & & &\\
Swift J0902.0+6007$^{A}$& 09 01 58.81 &+60 09 05.8  & 0.043 & $\rm 8^{+8.6}_{-4.0}$& [1.8]  & 1.1 &3.1&0.04 (2--10)&1\\
& & & & & & & & 1.2 (14--195)&\\
& & & & & & & & &\\
Swift J0904.3+5538$^{A}$& 09 04 36.92  & +55 35 59.7&0.022& --& $\rm 1.44^{+0.07}_{-0.07}$&4.9&  1.9&1.8 (2--10)&1\\
& & & & & & & & 7.2 (14--195)&\\
& & & & & & & & &\\
Swift J0911.2+4533$^{A}$&09 11 29.98  &+45 28 04.1 & 0.012& $\rm 30^{+9.5}_{-7}$&[1.8] &2.0&1.8&0.4 (2--10)&1  \\
& & & & & & & &5.8 (14--195) &\\
& & & & & & & & &\\
Swift J0917.2$-$6221$^{A}$&09 16 09.14&$-$62 19 28.4  &0.158 & $\rm 0.7^{+0.3}_{-0.3}$ & $\rm 1.67^{+0.2}_{-0.2}$  &16.0&3.3&14.8 (2--10)&1  \\
& & & & & & & &28.8 (14--195) &\\
& & & & & & & & &\\
Swift J0923.7+2255$^{A}$&09 23 42.89&+22 54 33.2 & 0.031& -- & $\rm 1.95^{+0.05}_{-0.05}$  &11.8& 4.5&3.7 (2--10)&1 \\
& & & & & & & &12.7 (14--195) &\\
& & & & & & & & &\\
Swift J1049.4+2258$^{A}$ &10 49 30.88& +22 57 52.9 & 0.019 & $\rm 20^{+5}_{-3}$ & [1.8]& 0.7&3.7 &0.2 (2--10)&1 \\
& & & & & & & &10.9 (14--195) &\\
\hline
\end{tabular} 
\medskip
$^+$~The square brackets in the $\Gamma$ column indicate that we used a fixed value; $^*$~this column reports the references for the hard \mbox{X-ray} flux; $^{\triangle}$ source fluxes were calculated from count rates (see \url{http://heasarc.gsfc.nasa.gov/db-perl/W3Browse/w3table.pl}); $^{\bullet}$~the values in the square brackets indicate the covering fraction; $^1$~Tueller et~al. (\cite{Tueller2009}); $^2$ Ajello et~al. (2007); $^{A}$~soft \mbox{X-ray} data from {\it Swift}/XRT; $^{B}$~soft \mbox{X-ray} data from {\it XMM}/EPIC; $^{C}$ soft \mbox{X-ray} data from {\it Chandra}.
\end{table}