\begin{table}%t3
\caption{Field F02: number of galaxies/stars in the $K$-selected spectroscopic sample.}   
\label{Nspec_maglim}      
\small%\centerline
 {
\begin{tabular}{l c c c c c c c c }         
\hline\hline                  
&&&&&&&& \\[-8pt]
 Flags$^a$  &
 $K^b$ $ \leq$ 19.0 & $K$ $\leq$ 19.5 & $K\leq$ 19.75 & $K\leq$ 19.8 & $K\leq$ 20.0 & $K\leq$ 20.25 & $K\leq$ 20.5 & $K\leq$ 21.5\\
 \hline
any &	893 / 176&
	1303 / 201&
	1566 / 219&
	1613 / 222&
	1810 / 239&
	2113 / 250&
	2426 / 265&
	3489 / 325\\
1, 21 &	 71 / 7&
	 126 / 11&
	 167 / 12&
	 173 / 12&
	199 / 14&
	251 / 14&
	312 / 15&
	534 / 27\\
2, 22 &	 183 / 11&
	 304 / 13 &
	 385 / 14&
	 394 / 15&
	456 / 20&
	551 / 23&
	656 / 27&
	1022 / 52\\
3, 4, 23, 24 &	613 / 158 &
	  834 / 177&
	  968 / 193 &
	  999 / 195&
        1097  / 205&
	1241  / 213&
	1375 / 223&
	1791 / 246\\
9, 29 &	 7 / 0&
	 13 / 0&
	 18 / 0&
	 18 / 0&
	25 / 0&
	36 / 0&
	48 / 0&
	105/ \\
11, 211, 12, 212 & 0 / 0 &
	     0 /0 &
	     0 / 0&
	    0 / 0&
           3 / 0&
	   3 / 0&
	   2  / 0&
	   2 / 0 \\
13, 14, 213, 214 & 16 / 0&
	    21 / 0&
	    22 / 0&
	    22 / 0&
           22 / 0 &
	   23 / 0 &
	   25 / 0 &
	   26 / 0 \\
19, 219 &  3 / 0&
	    5 / 0&
	    6 / 0&
	    7 / 0&
	    7 / 0&
	    8 / 0 &
	    8 / 0 &
	    9 / 0 \\
\hline
\end{tabular}}
\medskip
$^a$ Flags indicate the spectral quality and reliability of redshift measurements
  according to the definitions in \citet{olf05}.  \\ 
$^b$ All $K$ magnitudes are expressed in the Vega system. Magnitudes in the AB~system 
can be obtained by adding +1.84. In this table the star/galaxy separation is based on a purely spectroscopic classification.
\end{table}