\begin{table}%t1
\caption{\label{coreprop}The physical properties of the cores.}
\par
%\centerline
{\small
\begin{tabular}{lrrrrr} 
\hline\hline
Parameter & Core 1 & Core 2 & Core 3 & Core 4 & Core 5 \\ 
\hline 
Galactic longitude (2000) & 123.388 & 123.511 & 
123.559 & 123.687 & 123.690 \\
Galactic latitude (2000) & $+$24.928 & $+$24.915 & 
$+$24.856 & $+$24.894 & $+$24.931\\
Right ascension (2000) & 
01$^{\rm h}$34$^{\rm m}$01.9$^{\rm s}$ & 
01$^{\rm h}$44$^{\rm m}$51.6$^{\rm s}$ & 
01$^{\rm h}$47$^{\rm m}$40.8$^{\rm s}$ & 
01$^{\rm h}$59$^{\rm m}$42.7$^{\rm s}$ & 
02$^{\rm h}$00$^{\rm m}$58.7$^{\rm s}$ \\
Declination (2000) & 
$+$87$^{\circ}$45$^{\prime}$42$^{\prime\prime}$ & 
$+$87$^{\circ}$43$^{\prime}$35$^{\prime\prime}$ & 
$+$87$^{\circ}$39$^{\prime}$33$^{\prime\prime}$ & 
$+$87$^{\circ}$39$^{\prime}$53$^{\prime\prime}$ & 
$+$87$^{\circ}$41$^{\prime}$58$^{\prime\prime}$ \\
Distance (pc) & 150 & 150 & 150 & 150 & 150 \\
Radius (pc) & 0.023 & 0.035 & 0.032 & 0.035 & 0.034 \\
{\it FWHM} (pc) & 0.023 & 0.039 & 0.027 & 0.042 & 0.038 \\
$F^{\rm int}_{\rm 70~\mu m}$  (Jy) & $<$0.18 & $<$0.18 & 
$<$0.18 & $<$0.18 & $<$0.18 \\
$F^{\rm int}_{\rm 160~\mu m}$ (Jy) & 4.26 $\pm$ 0.07 &  10.19 $\pm$ 0.07 &    
7.56 $\pm$ 0.07 & 7.63 $\pm$ 0.07 & 5.44 $\pm$ 0.07 \\
$F^{\rm int}_{\rm 250~\mu m}$ (Jy) & 6.74 $\pm$ 0.04 & 16.77 $\pm$ 0.04 &   
13.10 $\pm$ 0.04 & 15.35 $\pm$ 0.04 & 13.26 $\pm$ 0.04 \\
$F^{\rm int}_{\rm 350~\mu m}$ (Jy) & 3.61 $\pm$ 0.02 &  8.98 $\pm$ 0.02 &    
7.27 $\pm$ 0.02 &  9.05 $\pm$ 0.02 &  8.50 $\pm$ 0.02 \\
$F^{\rm int}_{\rm 500~\mu m}$ (Jy) & 1.72 $\pm$ 0.02 &  4.33 $\pm$ 0.02 &   
3.50 $\pm$ 0.02 &  4.53 $\pm$ 0.02 &  4.40 $\pm$ 0.02 \\
Temperature (K) & 12 $\pm$ 1 & 12 $\pm$ 1 & 12 $\pm$ 1 & 11 $\pm$ 1 &
10 $\pm$ 1 \\
$N$(H$_2$)$_{\rm peak}$ ($\times$10$^{21}$ cm$^{-2}$) & 6 $\pm$ 3 & 7 $\pm$ 3 &
9 $\pm$ 4 & 13 $\pm$ 5 & 13 $\pm$ 5 \\
Mass ($M_\odot$) & 0.1 & 0.3 & 0.3 & 0.4 & 0.5 \\ 
$n$(H$_2$)$_{\rm mean}$ (cm$^{-3}$) & $\sim$5$\times$10$^{4}$ & 
$\sim$$4\times 10^{4}$ &
$\sim$$4\times 10^{4}$ & $\sim$$5\times 10^{4}$ & $\sim$$7\times 10^{4}$\\
$M_{\rm vir}$ ($M_\odot$) & $\sim$0.3--0.5 & $\sim$1.0--1.5 & $\sim$1.0--1.5 & 
$\sim$1.0--1.5 & $\sim$1.0--1.5 \\  \hline
\end{tabular}}
\tablefoot{The Galactic latitude and longitude, as well as right ascension and declination, are listed, along with the assumed distance. The radius
of each core was measured by taking the column density map in Fig.~\ref{5bands} and 
measuring the equivalent radius of the contour that encircled a column 
density of $4 \times 10^{21}$~cm$^{-2}$, and this radius is given in pc. 
The full-width at half maximum ({\it FWHM}) is the geometric mean {\it FWHM} measured
on the peak of each source.
The integrated flux density within this contour at each of the {\it Herschel} 
wavelengths is listed in Jy. The absolute uncertainty in the flux densities 
is $\pm$15\%. As described in the text, a temperature, peak column density 
and mass were derived, and these are also listed. The uncertainty in the 
masses could be as high as a factor of 2. A mean volume density is given, 
assuming each core is spherical, within the given radius. Finally, a virial 
mass for each core is estimated using CO and HCO$+$ linewidths.}\vspace*{-1mm}
\end{table}