\begin{table}%t1
%\centering
\par
\caption{\label{xrayprop}X-ray properties.}
\begin{tabular}{ccccccccccc}
\hline\hline
\noalign{\smallskip}
Name                    & ObsID & $\rm N_H$              & $\Gamma$               & {\it kT}   & {\it E}  & {\it EW}  & $ \log L_{\rm X}$ & $\log L_{\rm FIR}$ & class. & Ref. \\
 (1)                    & (2)    & (3)                    & (4)                    & (5)      & (6)       & (7)  & (8) & (9) & (10) & (11) \\
\hline
VII Zw031               &   7887     & $<$0.12                & $1.92^{\rm +0.47}_{-0.32}$ & --   & &        &         41.38           & 11.71              &    -- &  x \\
05189--2524          &    2034    & $7.6^{\rm +0.85}_{-0.94}$  & $1.75^{\rm +0.18}_{-0.23}$ & $0.07_{-0.11}^{\rm +0.07}$ & 
 & &   43.30           & 11.83              &   Sy2 &  x, a  \\
Arp55                   &    6857    & $<0.92$                & $2.65_{-0.83}^{\rm +5.3}$  & --  & &    &  40.10           & 11.48              &    -- & x, b  \\ 
09320+6134$\dagger$ &     2033   & $<$0.3                     & $1.17_{-0.21}^{\rm +0.57}$ & -- & $6.76\pm0.04$ & $3500^{\rm +1500}_{-1300}$ &   41.56           & 11.74              &  L&    x, a, b  \\ 
10565+2448          &   3952     & $0.18_{-0.08}^{\rm +0.08}$ & $2.13^{-0.24}_{+0.24}$ & --      & &   &              41.19           & 11.78              &   -- & x, d   \\
12112+0305          &    4934    &  $<$1.2                     & $2.78^{\rm +1.21}_{-0.99}$ & --                & &      & 40.36           & 12.09              &    L & x, d  \\ 
Mrk231$\dagger$         & --     & $273^{\rm +100}_{-68}$   & $2.95^{\rm +0.15}_{-0.16}$ &  & $6.39^{\rm +0.17}_{-0.15}$ &
 $180^{\rm +170}_{-150}$ &    42.41           & 12.15              &     QSO & e, h, a \\
Arp193                  &   7811     & $0.10^{\rm +0.08}_{-0.10}$ & $1.71^{\rm +0.38}_{-0.36}$ & --         & &   &             40.99           & 11.41              &  -- &   x  \\
Mrk273                  &  809      & $46.7_{-5.4}^{\rm +7.0}$   & 2.                     & $0.96^{\rm +0.05}_{-0.07}$ &  $6.59\pm 0.04$ & $220^{\rm +120}_{-100}$  & 42.99           & 11.93              &    Sy2 & x, f, a  \\ 
Arp220$\dagger$         & 869       & $0.43^{\rm +0.54}_{-0.28}$ & $1.11_{-0.28}^{\rm +0.52}$ & $0.92_{-0.05}^{\rm +0.15}$ & & &  40.95           & 11.96              &  L &   x, a, j, k   \\ 
NGC~6240$\dagger$        & --      & $179^{\rm +40}_{-15}$                  & $1.98^{\rm +0.25}_{-0.16}$  &        &    $6.50^{\rm +0.15}_{-0.07}$ & $1880^{\rm +1590}_{-730}$ &  42.01           & 11.57    &  L &        h, g, a \\ 
17208-0014          &    2035    & $0.13_{-0.09}^{\rm +0.10}$ & $1.66_{-0.30}^{\rm +0.26}$ & --            &   &       &  41.28           & 12.17              & HII & x     \\
NGC7469                 & --      &    $<$0.03   &  $2.05^{\rm +0.02}_{-0.03}$ &     &  $6.35^{\rm +0.14}_{-0.07}$ & $84^{\rm +20}_{-19}$    &  43.27       & 11.30 &  Sy1.5 & h    \\
23365+3604          &    4115    & $<$0.4                     & $1.2^{\rm +0.47}_{-0.43}$  & --         &  &       &      41.38           & 11.96              &    L & x, i  \\
 \hline 
\end{tabular}
\par
\tablefoot {
 The columns are:
      (1) Name; A  $\dagger$ denotes candidate Compton-thick sources.
      (2) \chandra Observation ID in the case where we performed our own spectral fits.
      (3) Column density in units of $10^{22}~\rm cm^{-2}$. %~\cunits.
      (4) Power-law photon index. 
      (5) Temperature of the thermal component in keV.
      (6) Energy of the FeK$\alpha$~line in keV. 
      (7) {\it EW} of the FeK$\alpha$~line in eV. 
      (8) Logarithm of the {\it absorbed} hard (2--10~keV) X-ray luminosity (erg s$^{-1}$).
      (9) Logarithm of the far-infrared luminosity (40--100~$\rm \mu m$) in units
          of solar luminosity.
      (10) Optical classification according to \citet*{Veilleux1999} or the NASA Extragalactic Database. 
      (11) X-ray reference: a. \citet{Ptak2003}, b. \citet{Gonzalez-Martin2009},
      c. \citet{Imanishi2003} d. \citet{Iwasawa2009} e. \citet{Braito2004}
      f. \citet{Xia2002} g. \citet{Vignati1999} h. \citet{Dadina2007} i. \citet{Teng2005} j. \citet{Clements2002} k. \citet{Iwasawa2005} 
       x. this work.   
}
\end{table}