\begin{table}%t2
\caption{\label{tbl:stats}Outflow detection statistics.}
%\centerline
 {\small \begin{tabular}{l c c c c c }
\hline\hline 
Type  & Observed (HARP) & Outflow (YSO?) & Weak outflow (YSO?)
& Confused (YSO?) & No outflow (YSO?)\\
 &(1) &(2)&(3) &(4) &(5)  \\
\hline
\multicolumn{6}{l}{\it SCUBA cores}\\
%\hline
Class 0 & 34 (14) & 21 (2)$^a$ &1 (0)&8 (5) &4 (3)  \\
Class I & 20 (10) &13 (4) &2 (1) &5 (4) &0 \\
Starless& 29 (20) &0  &2 (2)&8 (0)&19 (0) \\      
Total   & 83 (42) &29 (9)&5 (3) &22 (9) &22 (3)\\
\hline
\multicolumn{6}{l}{\it Low-luminosity objects}\\
%\hline
LLOs & 23 (12) &16 (0)$^b$  &2 (0) &2 (0) &3 (2) \\
\hline
\end{tabular}}
\medskip
$^a$~For SCUBA cores, the number in brackets indicate sources where there is disagreement on the protostellar status between  Paper~II, \citet{jorgensen07} and  \citet{gutermuth08}, as given in Table~\ref{tbl:outflows}. $^b$ For LLOs the numbers in brackets indicate sources where there is no SHARC-II detection of a protostar.
\end{table}