\begin{table}%t2
\caption{\label{tab2}The derived properties of the combined galaxies.}
%\scriptsize
\tiny%\centerline
{
\begin{tabular}{llllllr|llllllllll}
\hline \hline
(1)  & (2) & (3) & (4) & (5) & (6) & (7) & (8)  & (9) & (10) & (11) & (12) & (13) & (14) & (15) & (16) & (17)\\
   mass   & s2 ratio  &$n_e$ (cm$^{-3}$)    & o2 ratio  & $T_{\rm e}$([O~{\sc ii}]) (K) &
   $T_{\rm e}$([O~{\sc iii}]) (K) & OH$_{T_{\rm e}}$ & $A_V$ & log$R_{23}$ & log~O$_{32}$ &
   OH$^a_{R_{23}}$ &OH$^b_{R_{23}}$ & $P$ & OH$_{P}$  & $N$2 & OH$_{N2}$ &  log(${\rm N}\over {\rm O}$)    \\ \hline
    8.70    &   1.36   &    58.97    &    44.25   $\pm$   0.95  &   11423    $\pm$   153  &   12034  $\pm$   219  &   8.05  $\pm$  0.03   &   0.18   &  0.77  &    0.08  &   8.48   &   8.63  &  0.54 &  8.39  & --1.08  &    8.28   & --1.29   \\
    8.71    &   1.38   &    39.36    &    51.32   $\pm$   2.76  &   10641    $\pm$   341  &   10916  $\pm$   487  &   8.23  $\pm$  0.07   &   0.42   &  0.82  & --0.05  &   8.34   &   8.58  &  0.47 &  8.29  & --0.94  &    8.36   & --1.31   \\
    8.81    &   1.43   &     3.58    &    47.38   $\pm$   2.39  &   11491    $\pm$   370  &   12130  $\pm$   528  &   8.06  $\pm$  0.07   &   0.38   &  0.78  & --0.11  &   8.47   &   8.63  &  0.44 &  8.31  & --0.94  &    8.36   & --1.24   \\
    8.91    &   1.41   &    14.06    &    63.38   $\pm$   0.29  &   9703     $\pm$    22  &    9576  $\pm$    32  &   8.35  $\pm$  0.01   &   0.35   &  0.75  & --0.21  &   8.56   &   8.67  &  0.38 &  8.32  & --0.88  &    8.40   & --1.31   \\
    9.01    &   1.40   &    24.83    &    62.37   $\pm$   2.23  &   9701     $\pm$   182  &    9572  $\pm$   260  &   8.36  $\pm$  0.05   &   0.39   &  0.75  & --0.22  &   8.54   &   8.66  &  0.38 &  8.31  & --0.86  &    8.41   & --1.29   \\
    9.11    &   1.37   &    50.84    &    64.91   $\pm$   2.75  &   9328     $\pm$   202  &    9039  $\pm$   289  &   8.41  $\pm$  0.06   &   0.36   &  0.72  & --0.24  &   8.62   &   8.70  &  0.36 &  8.34  & --0.80  &    8.44   & --1.25   \\
    9.21    &   1.39   &    33.32    &    69.04   $\pm$   0.80  &   9168     $\pm$    51  &    8812  $\pm$    72  &   8.44  $\pm$  0.02   &   0.41   &  0.71  & --0.28  &   8.64   &   8.71  &  0.34 &  8.34  & --0.77  &    8.46   & --1.23   \\
    9.31    &   1.38   &    40.24    &    69.45   $\pm$   0.39  &   9096     $\pm$    24  &    8709  $\pm$    34  &   8.43  $\pm$  0.01   &   0.40   &  0.68  & --0.31  &   8.70   &   8.75  &  0.33 &  8.36  & --0.74  &    8.48   & --1.19   \\
    9.405   &   1.36   &    57.15    &    63.03   $\pm$   0.50  &   9422     $\pm$    38  &    9174  $\pm$    54  &   8.35  $\pm$  0.01   &   0.47   &  0.66  & --0.36  &   8.73   &   8.77  &  0.30 &  8.37  & --0.72  &    8.49   & --1.14   \\
    9.4505  &   1.39   &    37.63    &    73.34   $\pm$   1.29  &   8883     $\pm$    74  &    8404  $\pm$   105  &   8.48  $\pm$  0.02   &   0.53   &  0.68  & --0.39  &   8.71   &   8.75  &  0.29 &  8.35  & --0.69  &    8.50   & --1.18   \\
    9.505   &   1.42   &    13.25    &    92.13   $\pm$   0.91  &   8169     $\pm$    34  &    7384  $\pm$    49  &   8.67  $\pm$  0.01   &   0.59   &  0.67  & --0.39  &   8.73   &   8.77  &  0.29 &  8.36  & --0.70  &    8.50   & --1.25   \\
    9.5505  &   1.42   &    10.81    &    76.59   $\pm$   2.96  &   8878     $\pm$   164  &    8397  $\pm$   235  &   8.47  $\pm$  0.05   &   0.59   &  0.66  & --0.40  &   8.73   &   8.77  &  0.29 &  8.36  & --0.67  &    8.52   & --1.14   \\
    9.605   &   1.40   &    29.90    &    75.72   $\pm$   0.09  &   8801     $\pm$     5  &    8287  $\pm$     7  &   8.46  $\pm$  0.00   &   0.54   &  0.63  & --0.42  &   8.80   &   8.81  &  0.27 &  8.40  & --0.63  &    8.54   & --1.09   \\
    9.6505  &   1.38   &    41.11    &    79.67   $\pm$   0.77  &   8534     $\pm$    37  &    7906  $\pm$    53  &   8.52  $\pm$  0.01   &   0.67   &  0.62  & --0.46  &   8.81   &   8.82  &  0.26 &  8.40  & --0.63  &    8.54   & --1.11   \\
    9.705   &   1.39   &    32.46    &    83.36   $\pm$   1.99  &   8414     $\pm$    90  &    7735  $\pm$   128  &   8.55  $\pm$  0.03   &   0.66   &  0.62  & --0.45  &   8.81   &   8.82  &  0.26 &  8.40  & --0.62  &    8.55   & --1.11   \\
    9.7505  &   1.38   &    39.36    &    77.80   $\pm$   1.99  &   8636     $\pm$   102  &    8051  $\pm$   146  &   8.47  $\pm$  0.03   &   0.68   &  0.59  & --0.50  &   8.84   &   8.84  &  0.24 &  8.42  & --0.59  &    8.57   & --1.04   \\
    9.805   &   1.38   &    39.36    &    76.95   $\pm$   1.50  &   8679     $\pm$    75  &    8112  $\pm$   108  &   8.42  $\pm$  0.03   &   0.74   &  0.55  & --0.50  &   8.89   &   8.88  &  0.24 &  8.45  & --0.58  &    8.57   & --0.99   \\
    9.8505  &   1.38   &    42.86    &    89.25   $\pm$   1.48  &   8114     $\pm$    58  &    7305  $\pm$    83  &   8.59  $\pm$  0.02   &   0.77   &  0.57  & --0.54  &   8.88   &   8.87  &  0.22 &  8.43  & --0.56  &    8.58   & --1.05   \\
    9.905   &   1.39   &    32.46    &    69.83   $\pm$   2.42  &   9124     $\pm$   156  &    8748  $\pm$   224  &   8.29  $\pm$  0.05   &   0.80   &  0.53  & --0.54  &   8.91   &   8.89  &  0.23 &  8.47  & --0.56  &    8.58   & --0.91   \\
    9.9505  &   1.36   &    64.48    &    66.14   $\pm$   2.55  &   9156     $\pm$   177  &    8794  $\pm$   253  &   8.28  $\pm$  0.05   &   0.83   &  0.53  & --0.55  &   8.92   &   8.90  &  0.22 &  8.47  & --0.53  &    8.60   & --0.88   \\
   10.005   &   1.37   &    54.43    &    88.12   $\pm$   1.56  &   8096     $\pm$    62  &    7281  $\pm$    88  &   8.55  $\pm$  0.02   &   0.81   &  0.52  & --0.56  &   8.92   &   8.91  &  0.21 &  8.48  & --0.52  &    8.60   & --0.97   \\
   10.0505  &   1.38   &    40.24    &    98.15   $\pm$   6.10  &   7813     $\pm$   210  &    6876  $\pm$   299  &   8.63  $\pm$  0.09   &   0.87   &  0.51  & --0.56  &   8.93   &   8.92  &  0.22 &  8.49  & --0.50  &    8.61   & --0.97   \\
   10.11    &   1.34   &    76.67    &    76.26   $\pm$   1.60  &   8563     $\pm$    82  &    7947  $\pm$   118  &   8.39  $\pm$  0.03   &   0.94   &  0.49  & --0.58  &   8.95   &   8.93  &  0.21 &  8.50  & --0.49  &    8.62   & --0.87   \\
   10.21    &   1.34   &    75.72    &   101.92   $\pm$   2.07  &   7531     $\pm$    61  &    6472  $\pm$    88  &   8.70  $\pm$  0.03   &   1.06   &  0.48  & --0.61  &   8.95   &   8.94  &  0.20 &  8.50  & --0.47  &    8.63   & --0.96   \\
   10.31    &   1.32   &    97.12    &    97.23   $\pm$   2.54  &   7579     $\pm$    77  &    6542  $\pm$   110  &   8.66  $\pm$  0.04   &   1.08   &  0.46  & --0.61  &   8.97   &   8.96  &  0.20 &  8.52  & --0.46  &    8.64   & --0.92   \\
   10.41    &   1.33   &    86.29    &    81.74   $\pm$   1.54  &   8197     $\pm$    68  &    7424  $\pm$    97  &   8.45  $\pm$  0.03   &   1.15   &  0.45  & --0.60  &   8.97   &   8.96  &  0.20 &  8.53  & --0.44  &    8.65   & --0.81   \\
   10.51    &   1.36   &    57.15    &   110.86   $\pm$   1.85  &   7368     $\pm$    48  &    6241  $\pm$    69  &   8.76  $\pm$  0.02   &   1.22   &  0.48  & --0.60  &   8.95   &   8.94  &  0.20 &  8.50  & --0.44  &    8.65   & --0.95   \\ \hline
\end{tabular} }  
\smallskip
{\scriptsize Notes: Columns~(1)$-$(17) consequently refer to:
(1) the mass of the center value of the bin;
(2) the ratio of [S~{\sc ii}]$\lambda6717$/[S~{\sc ii}]$\lambda6731$;
(3) the electron density;
(4) the ratio of [O~{\sc ii}]$\lambda\lambda7320,~7330$/[O~{\sc ii}]$\lambda3727$;
(5) the election temperature in low ionization region;
(6) the election temperature in high ionization region;
(7) the oxygen abundances $12+\log($O/H) derived from election temprature;
(8) the dust extinction $A_V$ estimated from H$\alpha$/H$\beta$;
(9) logarithm of the ratio of ([O~{\sc ii}]$\lambda3727+[$O~{\sc
iii}]$\lambda\lambda4959,~5007$)/H$\beta$;
(10) logarithm of the ratio of [O~{\sc iii}]$\lambda\lambda4959,~5007$/[O~{\sc ii}]$\lambda3727$;
(11) the $12+\log($O/H) abundances obtained by using
the $R_{23}$ calibrations derived from DR4 (Eq.~(\ref{eqOHR23}));
(12) the $12+\log($O/H) abundances obtained by using
the $R_{23}$ calibrations derived from DR2 (T04);
(13) the $P$ parameter [O~{\sc iii}]$\lambda\lambda4959,~5007$)/
([O~{\sc ii}]$\lambda3727$+[O~{\sc iii}]$\lambda\lambda4959,~5007$);
(14) the $12+\log($O/H) abundances obtained by using the $P$-method calibration of P01;
(15) the $N2$ index (=log([N~{\sc ii}]$\lambda6583$/H$\alpha$));
(16) the $12+\log($O/H) abundances obtained by using the $N2$ calibration of PP04;
(17) the log(N/O) abundance ratios derived from election temperature method. 
}
\end{table}