\begin{table}%t6
\caption{\label{Tempd}Continuum observations and derived properties (dust temperature, C$^{18}$O column density, CO depletion factor) for sources in our survey.} 
\small%\centerline
{
\begin{tabular}{lccccccc}
\hline\hline\noalign{\smallskip}
  Source & IRAS & $F$(60~$\mu$m) & $F$(100~$\mu$m) & Wavelength of additional data  & $T_{\rm Dust}$ & $N$(C$^{18}$O) & $f\rm _D$(CO) \\
  & & [Jy] & [Jy] & [$\mu$m]  & [K] & [cm$^{-2}$] & \\
\hline 
L 1448 IRS 2 & 03222+3034 & 14.3 & $<$169 & 450,~850,~1100$^{1,3}$   & 27           & $6.07\times 10^{15}$ & $2.6\pm 0.6$   \\
L 1448 IRS 3 & 03225+3034 & 25.1 & 169& 1100$^{3}$  & 27                         & $1.08\times 10^{16}$ & $4.4\pm 1.0$ \\ 
L 1448 C &   F03226+3033 & 53.4 & 355 & 450,~850,~1100$^{2,3}$   & 32                 &  $7.18.19\times 10^{15}$ & $2.8\pm 0.6$      \\
L 1455 A1 &  03245+3002 & 47.1 & 93.6 & 1100,~450,~850$^{3,5}$   & 37             &  $3.53\times 10^{15}$ & $1.5\pm 0.4$ \\
L 1455 A2 &  F03247+3001 & 66.4 & 206 & -- &30                              &  $1.83\times 10^{15}$ & -- \\
Per 4 S &   --  & -- & -- & 1100$^{3}$  & --                                         & $3.18\times 10^{15}$ & -- \\
Per 4 N &   03262+3123 & 1.07 & $<$12.4 & 1100$^{3}$ &23                        &  $2.18\times 10^{15}$ & $2.4\pm 0.11$\\
Per 5 &    03267+3128 & 1.88 & $<$10.4 & 1100$^{3}$  & 26                         &  $3.28\times 10^{15}$ & $1.6\pm 0.4$\\
Per 6 &    03271+3013 & 7.53 & 8.19 & -- &45                                 &  $ 4.28\times 10^{15}$ & --\\
IRAS 03282 & 03282+3035 &2.33 & 13.9 & 450,~850,~1100$^{2,3}$  & 23              & $ 3.28\times 10^{15}$ & $3.9\pm 0.9$\\
Barnard 1-B & 03301+3057 & $<$6.18 & 35.5 & 1100,~850$^{3,4}$  & 18             & $1.16\times 10^{16}$ & $2.9\pm 0.7$\\
HH 211 &  03407+3152 & $<$2.06 & $<$30.8 & 1100,~450,~850$^{3,5}$  & $<$21        &   $8.21\times 10^{15}$ & $2.9\pm 0.7$\\
Barnard 5 IRS 1 & 03445+3242 & 15.5 & 15.4 & 1100$^{3}$  & 50                     & $1.23\times 10^{16}$ & $0.3\pm 0.09$\\
L 1527 &  04368+2557 & 17.8 & 73.3 & 450,~850,~1300$^{2}$  & 27                   &  $7.75\times 10^{15}$ & $2.3\pm 0.5$\\
L 483 &  18148-0440  &89.1 & 166 & 450,~850$^{2}$  & 34                           & $ 1.15\times 10^{16}$ & $2.1\pm 0.5$\\
SMM 5 &  --     &--&--    &--& --                                                & $9.70\times 10^{15}$ & -- \\
L 723 &  19156+1906 & 6.93 & 20.7 & 450,~850$^{2}$   & 25                   &  $4.36\times 10^{15}$ & $2.9\pm 0.7$\\
L 673 A & 19180+1114 &2.55 & 10.6 &  --&28                                      & $4.47\times 10^{15}$ & --\\
B 335 & 19345+0727  & 8.3 & 42  & 450,~850,~1300$^{2}$  &27                        &   $4.41\times 10^{15}$ & $3.3\pm 0.8$ \\
L 1157 & 20386+6751  &10.9 & 43.5  & 1300,~450,~850$^{2,5}$  &30                    & $3.19\times 10^{15}$ & $4.2\pm 1.0$\\
\hline
\end{tabular}}
\smallskip
The errors in the dust temperatures are $\sim$$2$~K, and the C$^{18}$O column densities are accurate to 10\%.\\
 References:
$^1$ O'Linger et~al.~(\cite{oli}); $^2$ Shirley et~al.~(\cite{shi}); $^3$ Enoch et~al.~(\cite{eno}); $^4$ Hatchell et~al.~(\cite{hcon}); $^5$~Froebrich et~al.~(\cite{fro2}).
\end{table}