\begin{table}%t2
%\centering
\par
\caption{\label{pointing}Equatorial coordinates, $FWHM$ at 100~$\mu$m, 
observed fluxes with 1$\sigma$ statistical errors ($F_{\rm PACS}$), 
and predicted photospheric fluxes ($F_{\star}$). }\vspace*{-2mm}
\begin{tabular}{lccccrrrr}
\hline\hline\noalign{\smallskip}
Star & Optical position & PACS 100~$\mu$m position
& \multicolumn{3}{c}{PACS 100~$\mu$m} & \multicolumn{2}{c}{PACS 160~$\mu$m} \\
        & (J2000)      & (J2000) & $FWHM$ 
& $F_{\rm PACS}$ & $F_{\star}$
& $F_{\rm PACS}$ & $F_{\star}$ \\
\hline
$\delta$ Pav&20:08:43.61 --66:10:55.4 &20:08:43.53 --66:10:58.1&6$\farcs 3 \times 6 \farcs 2$ & $59.6 \pm 1.1$ & 68.7 & $21.0 \pm 1.5$ & 26.9 \\
HR 8501     &22:18:15.62 -53:37:37.5 &22:18:16.14 --53:37:37.1& $6 \farcs 3 \times 6 \farcs 2$& $9.8 \pm 1.2$  & 10.9 &       & 4.3 \\
51 Peg      & 22:57:27.98 +20:46:07.8 &22:57:28.44 +20:46:08.5&5$\farcs 9 \times 6 \farcs 0$ & $11.3 \pm 1.7$ & 10.8 &   & 4.2 \\
\hline
\end{tabular}
\tablefoot{Absolute PACS uncertainties are $\sim$10\% and less than 20\% for 100 and 160~$\mu$m, respectively.  Flux units are mJy.}
\vspace*{-2.5mm}
\end{table}