\begin{table}%t5
 \caption{Catalog of derived parameters for LCGs.}
  \label{table}
  \small%\centerline
{
  \begin{tabular}{ccccccccllcl}
  \hline
  \hline
& &Stellar mass$^{a}$ & &{\it SFR}($\rho$)& &\multicolumn{2}{c}{Rest frame B}&& && \\
  Our ID & $z$ & ${\rm Log}_{10}(M/M_{\odot})$ & $L_{\rm IR}(10^{10}~L_{\odot})$ &  ($M_{\odot}~{\rm yr}^{-1}$)& {\it HR}$^{b}$  &  $B/T$  & $\chi^{2}_{\rm red}$    &  Type$^{c}$ & $Q^{d}$ &$R_{\rm d}({\rm kpc})^{e}$ & M1/M2$^{f}$  \\
 (1) & (2) & (3) & (4) & (5) & (6) & (7) & (8) & (9) & (10) & (11) & (12)\\
 \hline
904260 & 0.983 & 10.32  &  $<$10.37    & 3.62 $<$ $\rho$ $<$ 17  & &  --     &  --   &  S & 3 & & M2      \\
904604 & 0.990 & 10.94 & $<$10.59     & 0.13 $<$ $\rho$ $<$ 18  & &  0.33 $\pm$ 0.01     &  1.063   &  S & 1 &2.53 $\pm$ 0.04 &    \\
904680 & 0.964 & 10.28  & $<$9.83      & 3.28 $<$ $\rho$ $<$ 16  & &  --     &  --   &   & 4 & & M2   \\
905632 & 0.976 & 10.23  & $<$10.18     & 0.87 $<$ $\rho$ $<$ 17	& &  0.33 $\pm$ 0.03   &  1.093  &  S & 1 &1.16 $\pm$ 0.02 &     \\	
905983 & 0.860 & 10.36  & $<$7.22      & 3.87 $<$ $\rho$ $<$ 12	& &  0.08 $\pm$ 0.02   &  1.129  &  S & 2 &1.85 $\pm$ 0.01	&     \\
~906961$^{g}$ & 0.566 & 10.81  &     70.36     & $<$ 120	 &--0.55 $\pm$ 0.03 & -- &  --   &  E & -- &	&   \\	
907047 & 1.112 & 10.65  & $<$14.49     & 3.32 $<$ $\rho$ $<$ 24	& &  --	   &  --   &   & 4 &  &	M1     \\
907361 & 0.731 & 10.96 & $<$6.69      & 0.18 $<$ $\rho$ $<$ 11	& &  0.80 $\pm$ 0.04   &  1.322  &  E & 2 &	&    \\	
907794 & 1.144 & 10.92 &     20.82     & 35& & 0.67 $\pm$ 0.09   &  1.099  &  S0 & 1 &	&     \\
908243 & 0.726 & 10.23  & $<$6.57      & 2.41 $<$ $\rho$ $<$ 11	& &  0.13 $\pm$ 0.00   &  1.195  &  Tad & 3 &   &  \\	
909015 & 1.039 & 10.25  & $<$12.07     & 0.29 $<$ $\rho$ $<$ 20	& &  --	   &  --   &   & 4 &	   &  \\
909093 & 0.968 & 9.71  & $<$9.97      & 3.37 $<$ $\rho$ $<$ 17	& &  0.65 $\pm$ 0.02   &  1.093  &  Tad & 3 &	&     \\
909429 & 0.737 & 10.32  & $<$6.81      & 4.48 $<$ $\rho$ $<$ 11	& &  --	   &  --   &   & 4 &  &	M2     \\	
910413 & 0.655 & 10.67  &     15.84     & 27& &  --   &  --  &  Tad & 4 &  &	M2     \\
911747 & 0.840 & 10.18  & $<$6.79      & 4.81 $<$ $\rho$ $<$ 11	 & & --	   &  --   &   & 4 &  &	M2     \\	
911780 & 0.664 & 10.38  & $<$5.29      & 3.69 $<$ $\rho$ $<$ 9	 & & 0.26 $\pm$ 0.00   &  1.295  &  S & 2 &2.34 $\pm$ 0.01    &	     \\
911843 & 0.973 & 9.75  & $<$10.09     & 5.50 $<$ $\rho$ $<$ 17	 &  &--	   &  --   &   & 4 &	& M2     \\
912744 & 0.690 & 10.40  & $<$5.81      & 2.31 $<$ $\rho$ $<$ 9	 &  &--   &  --  &  S & 3 &	  &   \\
913482 & 0.664 & 10.71  & 27.17         & $<$ 46 &0.52 $\pm$ 0.06 & 0.48 $\pm$ 0.00	   &  1.221 &  S0 & 3 &	 &   \\	
914038 & 0.667 & 10.50  & 12.00         & 20& & --	   &  --   &   & 4 &	& M2     \\
915400 & 0.764 & 10.42  & $<$7.44      & 1.73 $<$ $\rho$ $<$ 12	 & & 0.08 $\pm$ 0.01 &  1.333  &  S & 2 &2.45 $\pm$ 0.02	&     \\	
916137 & 0.980 & 10.33  & $<$10.29     & 1.40 $<$ $\rho$ $<$ 17	 & & 0.60 $\pm$ 0.02   &  1.094  &  Irr & 3 &   &	     \\
916446 & 0.839 & 10.10  & $<$6.77      & 1.75 $<$ $\rho$ $<$ 11	 & & --	   &  --   &   & 4 &	& M2     \\
916866 & 0.987 & 10.22  & $<$10.48     & 1.68 $<$ $\rho$ $<$ 17	 & & 0.42 $\pm$ 0.03   &  1.137  &  S0 & 2 &	  &   \\
918147 & 1.099 & 10.77  & 39.48         & 67&  &--	   &  --   &   & 4 &	& M1     \\
919573 & 0.665 & 10.61  & 5.89          & $<$ 10&-0.40 $\pm$ 0.03  & 0.61 $\pm$ 0.05	   &  1.172 &  S0 & 3 &	&   \\	
919595 & 0.785 & 10.24  & $<$7.95      & 2.43 $<$ $\rho$ $<$ 13	 &  &0.12 $\pm$ 0.00   &  1.182  &  S & 3 &	   &  \\
920435 & 1.034 & 9.44  & $<$11.91     & 2.66 $<$ $\rho$ $<$ 20	 &  &0.49 $\pm$ 0.01   &  1.116  &  S0 & 2 &    &	     \\	
921406 & 1.095 & 10.37  & $<$13.89     & 5.22 $<$ $\rho$ $<$ 23	 &  &0.31 $\pm$ 0.03   &  1.125  &  S & 1 &2.43 $\pm$ 0.03	  &   \\
922675 & 0.666 & 10.13  & $<$5.32      & 2.79 $<$ $\rho$ $<$ 9	 &  &0.47 $\pm$ 0.01   &  1.142   &  S0 & 1 &	&     \\
922733 & 0.650 & 10.05  & $<$5.01      & 2.24 $<$ $\rho$ $<$ 8	 &  &--	   &  --   &   & 4 &	& M2     \\
922761 & 0.961 & 9.71  & $<$9.77      & 2.56 $<$ $\rho$ $<$ 16	 &  &0.24 $\pm$ 0.01   &  1.095&  Irr & 3 & &      \\	
923085 & 1.122 & 10.68  & 15.74         & 26&  &0.87 $\pm$ 0.01   &  1.212  &  Irr & 3 &    &      \\
923926 & 1.012 & 10.74  & $<$11.23     & 1.17 $<$ $\rho$ $<$ 19	 &0.12 $\pm$ 0.07  &0.64 $\pm$ 0.02   &  1.113   &  S0 & 3 &	&    \\	
924881 & 0.839 & 9.80  & $<$6.77      & 2.95 $<$ $\rho$ $<$ 11	 &  &0.78 $\pm$ 0.01   &  1.277   &  E & 2 &	&     \\
926109 & 0.522 & 10.19  & $<$2.95      & 1.55 $<$ $\rho$ $<$ 5	 &  &--	   &  --   &   & 4 &	& M1     \\	
926217 & 0.767 & 10.27  & $<$7.50      & 1.84 $<$ $\rho$ $<$ 12	 &  &0.50 $\pm$ 0.05   &  1.119   &  S0 & 1 &	&     \\
907305 & 1.185 & 10.11  & $<$17.21     & 3.17 $<$ $\rho$ $<$ 29	 &  &--	   &  --   &   & 4 &	& M1     \\	
914895 & 0.736 & 10.09  & $<$6.78      & 2.36 $<$ $\rho$ $<$ 11	 &  &--	   &  --   &   & 4 &	& M1     \\
  \hline
  \end{tabular}}
\medskip  
$^{a}$ Derived using a diet Salpeter IMF. In order to derive values using a~classic Salpeter~IMF, add 0.15~dex to the values listed here. \\		
$^{b}$ X-ray hardness ratio, defined as $(H-S)/(H+S)$ where $H$ and $S$ are the counts in the hard and soft bands respectively. \\
$^{c}$ Galaxy type -- {E}: 0.8~$<B/T\leq$ 1; {S0}: 0.4~$<B/T\leq$ 0.8; {S}: 0.0~$<B/T\leq$ 0.4; {Irr}: irregular; {Tad}: Tadpole. \\
$^{d}$ $Q$ quality factor -- 1: secure; 2: possibly secure; 3: insecure; 4: fit failed. \\
$^{e}$ Exponential disk scale length(kpc) for disk dominated galaxies. \\
$^{f}$ Merging? -- M1: obvious merging; M2: possible merging. \\
$^{g}$ This object could not be fitted properly due to the presence of a~strong point source at the~center. 
\end{table}