\begin{table}%t2
%\centering
\par
\caption{\label{table:fits}The measured fluxes and parameters of fitted greybody spectra ($T_{\rm dust}$, $\beta$).} %\vspace*{-2mm}
\begin{tabular}{cccccccccc}
\hline\hline\noalign{\smallskip}
Area     &  RA       & Dec     & 
         \multicolumn{5}{c}{Fluxes [Jy]} 
         & $T_{\rm dust}$  & $\beta$    \\
         & (J2000)   & (J2000) &  
         100~$\mu$m & 160~$\mu$m &  250~$\mu$m & 350~$\mu$m & 500~$\mu$m 
         & [K]             &            \\
\hline
PCC288-A   &  22 53 41.0  & +62 31 58   &   
     32.4(3.9) & 49.4(6.4) & 42.8(6.1) & 25.2(3.5) & 11.2(1.6) & 23.0(2.1) & 0.93(0.21)
      \\
PCC288-B   &  22 53 33.5  & +62 32 26   &
      9.5(2.0) & 17.3(3.5) & 13.7(3.2) & 7.7(2.3) & 3.2(1.0) & 20.2(3.3) & 1.36(0.55) 
      \\
PCC288-C    &  22 53 26.9  & +62 32  1 
            & 4.6(1.3) & 8.9(3.7) & 7.2(3.4) & 4.2(2.4) & 1.7(1.0) & 19.6(3.5) &
            1.39(0.82) \\
PCC288-D    &   22 53 38.2 &  +62  28  30 
            & --0.0(0.3) & 1.1(0.6) & 2.4(0.5) & 1.6(0.4) & 0.9(0.2) & 10.4(2.3)
            & 2.49(1.23)\\
PCC288-E    &  22 54 6.2  &   +62 33 37
            & 5.2(1.4) & 4.9(1.4) & 1.6(0.7) & 0.4(0.3) & 0.4(0.2) &
            26.6(1.9)  &  2.0 ~{\rm(fixed)}\\
PCC288-P   &  22 53 31.3  & +62 31 44   &
     25.9(20.9) & 127(41) & 265(104) & 162(48) &  72.8(18.5) 
     & 12.6(2.2) & 1.79(0.63) \\
PCC550-P1  &  12 25 35.6  & --71 42 35   &
   9.2(3.5) & 67.5(14.9) & 180(46) & 110(28) &  49.1(12.1) 
   & 11.3(1.0) & 2.03(0.39)   \\
PCC550-P2  &  12 24 30.0  & --71 50 19   &
   8.9(2.7) & 74.9(17.8) & 196(50) & 118(29) & 51.1(12.7) 
   & 11.3(1.1) & 2.18(0.36) \\
PCC249-P1  &  22 21 26.7  & +63 51 37   &
   1016(184) & 1329(242) & 761(105) & 365(51) & 143(21) 
   & 22.5(1.6) & 1.49(0.16) \\
PCC249-P2  &  22 21 35.0  & +63 37 22   &
   304(53) & 387(91) & 447(130) & 257(70) & 113(30) 
   & 15.9(0.5) & 2.0 ~{\rm(fixed)}   \\
\hline
\end{tabular}\vspace*{-2mm}
\tablefoot{An aperture size of 73$\arcsec$ 
is used for PCC288 sources $A$--$E$. Otherwise, the aperture is 9$\arcmin$ and the fits include {\it Planck} fluxes at 857, 545, and 353~GHz (not listed; see
Fig.~\ref{fig:spectra}).}
%\vspace*{-3mm}
\end{table}