\begin{table}%tA.2
\caption{The local sample: Seyfert 1.8 to 2.0 and narrow line radio galaxies (NLRGs).}
\par
%\centering
\par
\begin{tabular}{lcccrcrcc}
\hline \hline \noalign{\smallskip}
Name& Type& $z$& log~$N_{\rm H}$& $f_{2-10}$& ${\rm Ref}_{\rm X}$& $f_{\rm NeV}$& A& $\rm Ref_{NeV}$\\
(1)& (2)& (3)& (4)& (5)& (6)& (7)& (8)& (9)\\ 
\hline
       NGC~1068&  2.0&  0.0038&   25.00&  --11.34&   1& --11.94&   M&   1\\ 
       NGC~1275&  NLRG& 0.0175&   20.00&  --10.91&   2\tablefootmark{a}& --12.70&   L&   2\\ 
       NGC~1320&  2.0&  0.0089&   24.00&  --12.24&   3& --13.15&   S&   3\\ 
       NGC~1667&  2.0&  0.0152&   24.00&  --13.00&   4& --14.00&   L&   4\\ 
       NGC~2992&  1.9&  0.0077&   21.95&  --10.13&   5& --14.52&   S&  5\\ 
       NGC~3081&  2.0&  0.0079&   23.85&  --11.89&   6& --12.66&   L&   6\\ 
       NGC~3281&  2.0&  0.0106&   24.18&  --11.54&   7& --14.52&   S&   5\\ 
       NGC~3393&  2.0&  0.0125&   25.00&  --12.68&   8& --13.25&   L&   4\\ 
       NGC~4074&  2.0&  0.0224&   23.38&  --11.59&   3& --14.05&   S&  7\\ 
       NGC~4507&  2.0&  0.0118&   23.63&  --10.89&   9& --13.26&   L&   6\\ 
       NGC~5135&  2.0&  0.0136&   24.00&  --12.80&   10& --13.54&   L&   4\\ 
       NGC~5506&  1.9&  0.0062&   22.50&  --10.10&   11& --13.96&   M&  8\\ 
       NGC~5643&  2.0&  0.0040&   23.80&  --12.08&   12& --13.33&   M&  8\\ 
       NGC~5728&  2.0&  0.0093&   24.30&  --11.89&   13& --13.66&   L&   4\\ 
       NGC~7130&  2.0&  0.0161&   24.00&  --12.29&   14& --14.00&   S&  9\\ 
       NGC~7314&  1.9&  0.0048&   22.02&  --10.39&   15& --14.30&   M&  8\\ 
       NGC~7582&  2.0&  0.0052&   24.00&  --11.64&   16& --12.48&   M&  10\\ 
       NGC~7674&  2.0&  0.0289&   25.00&  --12.12&   17& --13.40&   L&  11\\ 
          Mrk~1&  2.0&  0.0159&   24.00&  --12.89&   18& --13.49&   L&   11\\ 
         Mrk~34&  2.0&  0.0505&   24.00&  --12.74&   19& --13.55&   L&   11\\ 
         Mrk~78&  2.0&  0.0371&   23.76&  --12.23&   3& --13.85&   L&   11\\ 
        Mrk~348&  2.0&  0.0150&   23.13&  --10.56&   20& --13.64&   L&   11\\ 
       Mrk~463E&  2.0&  0.0500&   23.85&  --12.39&   21& --13.89&   L&   11\\ 
        Mrk~477&  2.0&  0.0377&   23.38&  --11.92&   22& --13.14&   L&   4\\ 
        Mrk~573&  2.0&  0.0171&   24.00&  --12.92&   23& --13.00&   S&   3\\ 
        Mrk~609&  1.8&  0.0344&   20.00&  --11.83&   24& --14.40&   S&  12\\ 
        Mrk~612&  2.0&  0.0204&   23.81&  --12.44&   18& --13.66&   L&   11\\ 
          3C~33&  NLRG& 0.0597&   23.59&  --11.13&   25& --14.70&   M&  1\\ 
   MCG-5-23-16&  2.0&  0.0085&   22.15&  --10.10&   26& --13.89&   S&   5\\ 
        WAS~49b&  2.0&  0.0630&   22.80&  --12.20&   20& --14.30&   S&  13\\ 
       Cygnus~A&  NLRG& 0.0560&   23.23&  --10.89&   25& --14.40&   M&   14\\ 
        IC~3639&  2.0&  0.0109&   24.00&  --13.10&   18& --13.60&   L&   4\\ 
   Tol~0109-383&  2.0&  0.0117&   24.30&  --11.80&   27& --13.62&   S&   15\\ 
\hline		 	      			\end{tabular}
\tablefoot {Column description: (1) Source name. (2) Spectroscopic classification (1.8, 1.9 and 2.0 refer to Seyfert types). (3) Redshift. (4) Logarithm of the cold X-ray absorbing column density. For those objects in which no cold absorption is measured in excess of the Galactic value, the column has been fixed to log~$N_{\rm H}$~=~20. (5) Observed 2$-$10~keV flux in units of erg~cm$^{-2}$~s$^{-1}$. (6) Reference for the X-ray data. (7) [Ne~V]3426 flux in units of erg~cm$^{-2}$~s$^{-1}$. (8) Aperture used to measure the [Ne~V]~flux, defined following Schmitt (1998): S (small), M (medium) and L (large) correspond to apertures in the ranges 1$-$3$''$, 3$-$7$''$, and $>$7$''$, respectively. (9) Reference for the [Ne~V] data.\\
{\it X-ray references}: (1) \citet{cappi06}; (2) \citet{panessa06}; (3) this work; (4) \citet{bianchi05}; (5) \citet{gilli00}; (6) \citet{bassani99}; (7) \citet{vignali02}; (8) \citet{maio98}; (9) \citet{matt04}; (10) \citet{guainazzi05fabian}; (11) \citet{bianchi03};
(12) \citet{guainazzi04}; (13) \citet{comastri10}; (14) \citet{guido99}; (15) \citet{dg05};
(16) \citet{pico07ngc}; (17) \citet{pino98}; (18) \citet{guainazzi05matt}; (19) \citet{greenhill08}; (20) \citet{awaki00}; (21) \citet{bianchi08}; (22) \citet{levenson01}; (23) \citet{shu07}; (24) \citet{gallo06lehmann}; (25) \citet{evans06}; (26) \citet{balestra04}; (27) \citet{iwa01tol}\\
\tablefoottext{a}{The column density of NGC 1275, which is at the center within the Perseus cluster, is difficult to measure: \citet{evans06} do not find absorption in excess of the Galactic one based on \chandra\ data.} \\
{\it [Ne~V] references}: (1) \citet{koski78}; (2) \citet{anderson70}; (3) \citealt{erkens97}; 
(4) This work (based on the catalog of UV-optical spectra of nearby galaxies by \mbox{Storchi-Bergmann} et~al., see text); (5) \citet{db88}; (6) \citet{db86}; (7) \citet{so81}; (8)~\citet{mw88}; (9) \citet{sf90}; (10) \citet{ward80}; (11) \citet{malkan86}; (12) \citet{o81}; (13) \citet{moran92}; (14) \citet{om75}; (15) \citet{fs83}.}
\vspace*{5.5mm}
\end{table}