\begin{table}%t1
\caption{\label{llf-numbers.tab}Number of $0 < z < 0.2$ sources used for the determination of LLFs. }\small%\centering
\par
\begin{tabular}{ccccc}
\hline\hline
\noalign{\smallskip}
Field & 250~$\mu$m & 350~$\mu$m & 500~$\mu$m & Area \\
\hline
LH & 478 (369/109) & 116 (99/17) & 18 (16/2) & 10.7 \\
XFLS & 275 (222/53) & 94 (80/14) & 27 (22/5) & 4.0 \\
Total & 753 (591/162) & 210 (179/31) & 45 (38/7) & 14.7 \\ 
\hline
\end{tabular}\vspace*{-2mm}
\tablefoot{The number of sources with (spectroscopic/photometric) redshifts is indicated after the total number of sources. The 250~$\mu$m sample is also used to determine the IR~bolometric LLF. Field areas are in deg$^2$.}
\end{table}