\begin{table}%t3
\caption{$K_{\rm s}$ band galaxy counts. \label{Kcounts}}
%\centerline
{\begin{tabular}{r r r r r r} \hline \hline
$K_{\rm s}^{\rm lim}$ & $n$ & $N^*$ & 
\multicolumn{1}{r}{$N^*_{\rm Sco}$} & $>$4 & $>$5 \\
(1) & (2) & (3) & (4) & (5) & (6) \\ \hline
18.0 &  19 & $ 2.5\pm0.4$ &	 &  1 &  0 \\
18.5 &  17 & $ 3.8\pm0.6$ &	 &  6 &  1 \\
19.0 &  29 & $ 6.2\pm0.7$ & $ 4.3\pm0.3$ &  9 &  1 \\
19.5 &  34 & $ 8.9\pm0.8$ & $ 6.3\pm0.4$ & 19 &  2 \\
20.0 &  58 & $13.5\pm1.0$ & $ 8.4\pm0.4$ & 26 &  5 \\
20.5 &  69 & $19.0\pm1.2$ & $11.3\pm0.5$ & 37 &  7 \\
21.0 &  59 & $23.8\pm1.4$ & $16.1\pm0.6$ & 47 & 11 \\
21.5 &  84 & $30.5\pm1.6$ &	 & 59 & 16 \\
22.0 &  55 & $34.9\pm1.7$ &	 & 64 & 19 \\
\hline  
\end{tabular}}
\par
\smallskip
\noindent Notes: (1) Limiting $K_{\rm s}$ magnitude; (2)
differential counts between $K_{\rm s}^{\rm lim} - 0.5$ and $K_{\rm s}^{\rm lim}$;
(3) cumulative number arcmin$^{-2}$ of galaxies brighter than limiting
$K_{\rm s}^{\rm lim}$, Poisson error is indicated; (4) same as (3) from blank
field survey by \citet{sco00}; (5) number of objects brighter than
$K_{\rm s}^{\rm lim}$ with $I - K_{\rm s} > 4$; (6) same as (5) for $I - K_{\rm s} > 5$
(see Sect.\ \ref{ero_sec}).
%%\end{center}
\par
\end{table}