\begin{table}%t1
%\centering
\par
\caption{\label{tab:targets}Target information and {\it Herschel} flux densities.} 
\begin{tabular}{llllllll} 
\hline \hline \noalign{\smallskip}
Name & RA, Dec (J2000) & Type & \multicolumn{5}{c}{$F_\nu$ (mJy)}\\ 
& & & 100~\micron & 160~\micron & 250~\micron & 350~\micron & 500~\micron\\
\hline\noalign{\smallskip}
R71 & 05$^{\rm h}$02$^{\rm m}$07.39$^{\rm s}$, $-$71${\degr}$20${\arcmin}$13.1${\arcsec}$  & LBV & $447\pm8$ & $105\pm10$ & $50\pm6$ & $49\pm13$ & $27\pm9$\\
IRAS05280$-$6910 & 05$^{\rm h}$27$^{\rm m}$40.11$^{\rm s}$, $-$69${\degr}$08${\arcmin}$04.5${\arcsec}$ & RSG, OH/IR &...&...& $205\pm8$ & $46\pm13$ & $<$$11\pm10$ \\
HD~36402 & 05$^{\rm h}$26$^{\rm m}$03.94$^{\rm s}$, $-$67${\degr}$29${\arcmin}$57.9${\arcsec}$ & WC4($+$O?)$+$O8I &...&...&...&...&...\\
HD~36402 IR1/YSO2& 05$^{\rm h}$26$^{\rm m}$02.99$^{\rm s}$, $-$67${\degr}$29${\arcmin}$57.7${\arcsec}$ &YSO?& $531\pm10$ & $872\pm33$ & $677\pm33$ & $<$$431\pm23$ & $<$$132\pm21$\\
\hline
\end{tabular}\vspace*{-2mm}
\tablefoot{Quoted uncertainties are 1$\sigma$. Upper
  limits are either below the 3$\sigma$ detection level or include
  substantial flux from an adjacent unresolved source. IRAS05280--6910
  does not fall within the PACS coverage.  The WR star itself is not
  resolved in {\it Herschel} images; it is severely blended with an IR
  source (IR1/YSO2).  The 350 and 500~\micron{} fluxes of IR1/YSO2
  include a nearby YSO (N51-YSO1), which is unresolved from IR1/YSO2
  at these wavelengths. Aperture corrections for PACS and SPIRE were
estimated using the current point-spread functions, and are roughly~1.4 and~1.2, respectively. None of the sources are heavily affect by
  high and/or variable backgrounds (Fig.~\ref{fig:raw}).}
\vspace*{-2.5mm}\end{table}