\begin{table}%ta1 \caption{\label{tab:blind_stats_match}PEP fields: total exposure times, noise properties, flux levels for 80\% completeness and 30\% spurious fraction, statistics of \textit{blind} catalogs, and results of maximum-likelihood match to the multi-wavelength ancillary catalogs (labeled ``multi'', GOODS-N only).} %\centering \par \begin{tabular}{l c r c c c c} \hline \hline\noalign{\smallskip} Field & Area & $t_{\exp}$ & rms & $N(PACS)$ & Compl. & Spur.\\ \& band & & $[$h$]$ & $[$mJy$]$ & ${>}3\sigma$ & 80\% & 30\%\\ \hline GOODS-N 100 & $10^\prime\times15^\prime$ & 30 & 1.00 & 291 & 5.5 & 2.5\\ GOODS-N 160 & $10^\prime\times15^\prime$ & 30 & 1.90 & 317 & 11.0 & 7.0\\ 100+160 & -- & -- & -- & 201 & -- & -- \\ 100+multi & -- & -- & -- & 254 & -- & -- \\ 160+multi & -- & -- & -- & 274 & -- & -- \\ 100+160+multi & -- & -- & -- & 187 & -- & -- \\ 100+multi+zspec & -- & -- & -- & 162 & -- & -- \\ 160+multi+zspec & -- & -- & -- & 169 & -- & -- \\ 100+160+multi+zspec & -- & -- & -- & 125 & -- & -- \\ \hline A2218 100 & $4^\prime\times4^\prime$ & 13 & 0.84 & 98 & 5.4 & 3.0 \\ A2218 160 & $4^\prime\times4^\prime$ & 13 & 1.59 & 94 & 11.8 & 7.6 \\ LH\tablefootmark{a} 100 & $24^\prime\times24^\prime$ & 35 & $\sim$1.3 & $\sim$780 & $\sim$7.0 & $\sim$4.0 \\ LH\tablefootmark{a} 160 & $24^\prime\times24^\prime$ & 35 & $\sim$2.7 & $\sim$700 & $\sim$14.5 & $\sim$9.5 \\ COSMOS\tablefootmark{b} 100 & $85^\prime\times85^\prime$ & 182 & $\sim$2.0 & $\sim$5750 & $\sim$9.5 & $\sim$6.3\\ COSMOS\tablefootmark{b} 160 & $85^\prime\times85^\prime$ & 182 & $\sim$4.0 & $\sim$4900 & $\sim$20.5 & $\sim$12.0\\ \hline \end{tabular} \tablefoot{\tablefoottext{a}{The PEP Lockman Hole field is the ROSAT-HRI and XMM field.} \tablefoottext{b}{COSMOS will reach 213~h of integration at full depth.}}\vspace*{2.8mm} \end{table}