\begin{table}%t3
\caption{Best-fit parameters for the X-ray spectral analysis.\label{tab3}}
%\centerline
 {\begin{tabular}{lrrrrrrlrrrr}
\hline
\hline
\multicolumn{1}{l}{Galaxy name} &
\multicolumn{1}{r}{$N_{\rm H_{Gal}}$} &
\multicolumn{1}{r}{$N_{\rm H}$} &
\multicolumn{1}{r}{$\Gamma_{\rm HX}$} &
\multicolumn{1}{r}{$\Gamma_{\rm SX}$} &
\multicolumn{1}{r}{$kT$} &
\multicolumn{1}{r}{{\it EW}(Fe~K)} &
\multicolumn{1}{l}{$\chi^{2}_{\rm red}$/$\nu$} &
\multicolumn{1}{r}{$F_{\rm SX}$} &
\multicolumn{1}{r}{$F_{\rm HX}$} &
\multicolumn{1}{r}{log $L^{\rm int.}_{\rm SX}$} &
\multicolumn{1}{r}{log $L^{\rm int.}_{\rm HX}$} \\
%\multicolumn{1}{l}{} &
%\multicolumn{1}{r}{(10$^{20}$)} &
%\multicolumn{1}{r}{(10$^{22}$)} &
%\multicolumn{1}{r}{} &
%\multicolumn{1}{r}{(keV/cgs/-)} &
%\multicolumn{1}{r}{(eV)} &
%\multicolumn{1}{l}{} &
%\multicolumn{1}{r}{($\times$10$^{-13}$)} &
%\multicolumn{1}{r}{($\times$10$^{-13}$)} &
%\multicolumn{1}{r}{log} &
%\multicolumn{1}{r}{log} \\
\multicolumn{1}{l}{(1)} &
\multicolumn{1}{r}{(2)} &
\multicolumn{1}{r}{(3)} &
\multicolumn{1}{r}{(4)} &
\multicolumn{1}{r}{(5)} &
\multicolumn{1}{r}{(6)} &
\multicolumn{1}{r}{(7)} &
\multicolumn{1}{l}{(8)} &
\multicolumn{1}{r}{(9)} &
\multicolumn{1}{r}{(10)} &
\multicolumn{1}{r}{(11)} &
\multicolumn{1}{r}{(12)} \\
\hline
NGC 676  &4.4 &$\leq$0.1       &1.9~$\pm$~0.3    & -- & --                                &--            &1.2/12   &     0.1 &     0.2 &   38.9 &   39.0 \\ 
NGC 1058$^{\ddagger}$&6.7&$\leq$0.6&1.3~$\pm$~0.9  & -- & --                                &--            &0.2/2    &$<$0.1 &$<$0.4 &$<$38.1 &$<$38.6 \\ 
NGC 1068$^{\dagger*}$&3.5&$\leq$0.1&1.0~$\pm$~0.1&3.5~$\pm$~0.5& 0.7~$\pm$~0.2              &1200~$\pm$~500 &4.3/1399 &   111.3 &    46.2 &   41.4 &   41.1 \\ 
NGC 2685 &4.1 &$\leq$0.3       &0.5~$\pm$~0.2    & -- &--                                 &--            &1.5/8    &     0.2 &     2.7 &   38.8 &   39.9 \\ 
NGC 3031$^{*}$ &4.1 &$\leq$0.1 &1.9~$\pm$~0.1    &--&0.6~$\pm$~0.1                         &40~$\pm$~20    &1.2/1651 &    87.0 &   120.0 &   40.2 &   40.3 \\ 
NGC 3079$^{\dagger}$&0.8&0.05~$\pm$~0.03&1.7~$\pm$~0.1&--&0.7~$\pm$~0.1                       &1480~$\pm$~500 &1.1/264  &$<$2.5 &     3.3 &$<$40.0 &   40.1 \\ 
NGC 3185 &2.1 &$\leq$0.2       &2.1~$\pm$~0.1    &--&--                                   &--            &0.6/5    &     0.2 &     0.2 &   39.0 &   39.0 \\ 
NGC 3227 &2.2 & 6.8~$\pm$~0.3     &1.5~$\pm$~0.1    &$\equiv$$\Gamma_{HX}$&--               &190~$\pm$~40  &1.1/1863  &     4.0 &    81.4 &   41.2 &   41.7 \\ 
NGC 3486 &1.9 &$\leq$0.3       &0.9~$\pm$~0.2    &--& --                                  &--            &1.1/6    &     0.2 &     1.1 &   38.0 &   38.9 \\ 
NGC 3941 &1.9 &$\leq$0.1       &2.1~$\pm$~0.3    &--& --                                  &--            &1.8/8    &     0.4 &     0.4 &   38.8 &   38.9 \\ 
NGC 4051$^{*}$ &1.3 &$\leq$0. 3 &1.2~$\pm$~0.1    &3~$\pm$~0.5&0.2~$\pm$~0.1                 &240~$\pm$~40   &2.2/2006 &    47.3 &    62.7 &   41.2 &   41.3 \\ 
NGC 4138 &1.4 &8.0~$\pm$~1        &1.5~$\pm$~0.1    &$\equiv$$\Gamma_{HX}$&0.3~$\pm$~0.1     &83~$\pm$~30    &1.0/408  &     0.6 &    55.0 &   40.9 &   41.3 \\ 
NGC 4151$^{*}$ &2.0 &7.5~$\pm$~1  &1.6~$\pm$~0.2    &1.8~$\pm$~0.5&--                         &300~$\pm$~30   &1.9/2785 &    29.7 &   451.0 &   42.0 &   42.5 \\ 
NGC 4258$^{\dagger}$&1.2&8.7~$\pm$~0.3&1.7~$\pm$~0.1&1.9~$\pm$~0.1&0.5~$\pm$~0.1               &27~$\pm$~20    & 1.0/899   &$<$3.4 &    83.7 &$<$40.7 &   40.9 \\ 
NGC 4388 &2.6 &27~$\pm$~2         &1.3~$\pm$~0.2    &$\equiv$$\Gamma_{HX}$&0.3~$\pm$~0.1     &450~$\pm$~70   & 1.0/283 &     2.2 &    76.2 &   41.2 &   41.8 \\ 
NGC 4395 &1.3 &5.3~$\pm$~0.3      &1.2~$\pm$~0.1    &$\equiv$$\Gamma_{HX}$&0.2~$\pm$~0.1     &100~$\pm$~25   & 0.97/535&     1.0 &    61.6 &   39.2 &   39.8 \\ 
NGC 4472$^{\ddagger}$&1.7&0.3~$\pm$~0.1&2.7~$\pm$~0.3&--&0.8~$\pm$~0.2                        &--            &1.8/483  &$<$19.8 &$<$3.8 &$<$40.8 &$<$40.1 \\ 
NGC 4477 &2.6 &$\leq$2         &1.9~$\pm$~0.3    &--&0.4~$\pm$~0.1                         &--            &1.0/106  &$<$2.0 &     1.2 &$<$40.0 &   39.6 \\ 
NGC 4501 &2.5 &$\leq$0.2       &1.5$\pm0.3$    &--&0.4~$\pm$~0.1                         &--            &1.1/28   &     0.9 &     1.1 &   39.5 &   39.6 \\ 
NGC 4565 &1.3 &0.12~$\pm$~0.04    &1.8~$\pm$~0.2    &--&--                                   &--            &1.2/70   &     1.1 &     2.4 &   39.2 &   39.4 \\ 
NGC 4579 &2.4 &$\leq$0.02       &1.7~$\pm$~0.1    &--&0.6~$\pm$~0.1                         &170~$\pm$~50   &1.1/1043 &    25.3 &    38.5 &   41.0 &   41.1 \\ 
NGC 4639 &2.4 &$\leq$0.01      &1.8~$\pm$~0.1    &--&--                                   &--            &1.0/176  &     3.0 &     4.9 &   40.0 &   40.2 \\ 
NGC 4698 &1.9 &$\leq$0.4       &2.0~$\pm$~0.2    &--&--                                   &--            &1.2/17   &     0.3 &     0.4 &   39.1 &   39.2 \\ 
NGC 4725 &0.1 &$\leq$5         &1.9~$\pm$~0.5    &--&0.3~$\pm$~0.1                         &--            &0.84/44  &     0.7 &     0.4 &   39.2 &   38.9 \\ 
NGC 5033 &0.1 &$\leq$0.03      &1.7~$\pm$~0.1    &--&--                                   &466~$\pm$~215  &0.97/335 &    15.0 &    28.7 &   40.8 &   41.1 \\ 
NGC 5194 &1.6 &$\leq$0.03      &0.6~$\pm$~0.1    &--&0.5~$\pm$~0.1                         &986~$\pm$~210  &1.65/361 &     7.3 &     4.8 &   39.8 &   39.6 \\	
NGC 5273 &0.1 &0.9~$\pm$~0.1     &1.4~$\pm$~0.1    &$\equiv$$\Gamma_{HX}$&0.2~$\pm$~0.1     &226~$\pm$~75   &1.1/1009 &    13.2 &    67.1 &   41.0 &   41.4 \\ 
% to be inserted: NGC 3982 &-   &-                &-              &-         &-     &-   &   	      & 	  	 &	       &             \\ 
%% excluded for D>30 Mpc:   NGC 4168 &2.6 &$\leq$ 0.03    &2.0$\pm$0.2 &-   &- &1.1/51 & 4.3E-14 &   5.1E-14 &    4.6E-14 &   5.1E-14 & 1.25 & 39.69 & 39.77  \\ 
\hline
\end{tabular}}
\par
\smallskip
Notes: SX = 0.5--2 keV, HX = 2--10 keV.
Galaxies marked with $^{\dagger}$ and $^{\ddagger}$ indicate that the 
nuclear regions are contaminated (by more than 10\%) by off-nuclear 
point-sources and/or diffuse emission in only the soft band (${\dagger}$) or 
in both the soft and hard bands (${\ddagger}$). 
Galaxies marked with "*'' indicate sources with very complex spectra 
for which only a rough parametrization is given here.
See Appendix B for more details on individual sources; 
Col. (1): galaxy name; 
Col. (2): Galactic absorption along the line of sight, in units of 10$^{20}$ cm$^{-2}$; 
Col. (3): measured absorption column density, in units of 10$^{22}$ cm$^{-2}$; 
Col.~(4): power-law photon index; Col. (5): photon index of the soft power-law 
component;
% ($\Gamma_{SX}$),
%ionization parameter of the warm absorber ($\xi$).
%***Massimo: I don't understand the two lines above, which I have
% "commented out,'' because I don't see in this column any values of
% \xi. Please explain.
Col. (6): temperature of the thermal component ($kT$) in units of keV;
Col. (7): equivalent width of the Fe~K line, in units of keV; 
Col. (8): reduced chi-squared and number of degrees of freedom.
Columns (9)--(10): observed fluxes in the soft (0.5--2 keV) and hard (2--10~keV) 
X-ray bands, in units of 10$^{-13}$~erg~cm$^{-2}$~s$^{-1}$;
Cols.~(11)--(12): Log of the absorption-corrected luminosities in the soft 
(0.5--2 keV) and hard (2--10~keV) X-ray bands 
(computed using distances from Table~\ref{tab1}). 
\end{table}