\begin{table}%t1
\caption{\label{tab_ct}X-ray spectra of the candidate Compton-thick AGN.}
%\centerline
 {\small \begin{tabular}{lccccccccc}
\hline \hline
\multicolumn{3}{l}{} & \multicolumn{3}{c}{Power-law} & \multicolumn{2}{c}{Reflection} & \multicolumn{2}{c}{}  \\
ID&$\alpha, \delta$ & $z$&$N_{\rm H}$ & $\Gamma$ & $\chi^2$/$\nu$ & $\Gamma$& $\chi^2$/$\nu$& $\log L_{\rm x}$ & Flux \\ 
(1) & (2)& (3) & (4) & (5) & (6 & (7) & (8) & (9) & (10)\\
\hline\noalign{\smallskip}
35 & 12 35 49.44 +62 15 36.9& 2.203 & $<$6.7 & $0.15^{\rm +0.35}_{-0.40}$ & 6.4/8 & $1.75^{\rm +0.44}_{-0.42}$ &  7.8/9 &  42.68 & 1.20 \\
91 & 12 36 11.40 +62 21 49.9 &0.51 (1.78) & $3.0^{\rm +3.2}_{-2.7}$  & $0.30^{\rm +0.62}_{-0.50}$ & 31.2/17 & $1.74^{\rm +0.26}_{-0.54}$ &40.3/19&42.65 & 9.44 \\
92 &12 36 11.80 +62 10 14.5&0.91 & $4.6^{\rm +8}_{-4.6}$ & $-0.14^{\rm +0.94}_{-0.86}$  & 17.2/7 & $1.16^{\rm +0.44}_{-0.66}$ &  23.2/7 &  42.42 & 2.69 \\
107 &   12 36 15.83 +62 15 15.5&0.59 (2.48) & $7.4^{\rm +7.5}_{-6.3}$& $0.66^{\rm +0.37}_{-0.46}$& 11.0/12 & $1.93^{\rm +0.21}_{-0.21}$ &  11.1/13 &43.08  & 1.85 \\
121 &12 36 19.89 +62 19 10.1&  0.520 & $0.3^{\rm +2.1}_{-0.2}$  & $0.49^{\rm +0.37}_{-0.43}$& 4.8/8 & $2.8^{\rm +0.37}_{-0.40}$ & 11.7/9 & 41.93  & 1.90 \\
127 &12 36 21.21 +62 11 08.8&  1.014 & $12.3^{\rm +2.5}_{-9.0} $  & $0.20^{\rm +1.20}_{-0.70}$   & 12.9/12/8 & $1.16^{\rm +0.23}_{-0.31}$ &  13.2/13 &  42.76&  3.98\\
135 &12 36 22.66 +62 16 29.8& 2.466 & $275^{\rm +195}_{-138} $  & 1.8& 5.5/4  &  --  &  -- & 43.61  & 1.14 \\
171 &12 36 32.59 +62 07 59.8& 1.993 & $ 2.2^{\rm +15}_{-2}$  & $-0.02^{\rm +0.75}_{-0.47}$   & 7.2/9 & $1.65^{\rm +0.31}_{-0.36}$ &  6.2/10 &  42.73  & 1.83 \\
190 &     12 36 35.58 +62 14 24.1& 2.005 & $1.5^{\rm +1.0}_{-1.5} $  & $0.28^{\rm +0.51}_{-0.29}$  & 13.2/13 & $1.93^{\rm +0.20}_{-0.20}$ &  11.2/14 &  43.01 & 2.48 \\
191 &    12 36 35.86 +62 07 07.7& 0.28 (0.93) & $<$20  & $-1.4^{\rm +1.40}_{-0.47}$   & 38.1/18 & $0.20^{\rm +0.44}_{-0.78}$ &  27.4/16 &  41.73  & 5.35 \\ 
\hline
\end{tabular}}
\medskip 
The columns are: (1)~Alexander ID number; (2)~X-ray Equatorial Coordinates (J2000); (3)~redshift;  three and two decimal numbers refer to spectroscopic and photometric redshift respectively; in brackets we quote the possible \mbox{X-ray} spectroscopic redshift;  (4)~intrinsic column density in  units  of $10^{22}$~\cunits\  for the power-law model; (5)~photon index in the case of the power-law model; (6)~$\chi^2$ and degrees of freedom for the power-law model; (7)~photon index in the case of  the reflection model; (8)~$\chi^2$ and degrees of freedom for the reflection model; (9)~logarithm of the observed luminosity in the 2--10~keV band in units of \lunits;  (10)~observed flux in the 2--10~keV band in units of $10^{-15}$~\funits. 
\vspace*{7mm}
\end{table}