\begin{table}%t7
%\centering
\par
\caption{Properties of MAMBO-detected IRAS sources. For every core in
  the c2d MAMBO survey the table lists dust emission peaks and, if
  applicable, the related subcore associated with an IRAS source
  (Sect.~\ref{sec-survey:ass_protostars} discusses the identification of
  associated sources; FSC sources are preceded by an ``F'').   Associated 2MASS sources are
  listed too. The table further lists the spectral index between 12   and $25~\rm \mu m$ wavelength, the bolometric temperature and   luminosity, the submillimetre-to-bolometric luminosity ratio, the   mass within a peak-centered aperture of 4200~AU radius,
  and the infrared SED class.}\label{tab-survey:IRAS_detected}
\small
\begin{tabular}{llllllllll}
\hline \hline
 Core & Asso.  & IRAS source & 2MASS source & $\alpha^{25~\rm \mu m}_{12~\rm \mu m}$ &
 $T_{\rm bol}^{\rm IRAS}$ &  $L_{\rm bol}^{\rm IRAS}$ & $L_{\rm submm}^{\rm IRAS} / L_{\rm bol}^{\rm IRAS}$ & $M^{\rm YSO}_{\rm 4200~\rm AU}$ & Class\\
 & & & & & $K$ & $L_{\odot}$ & & $M_{\odot}$ \\
 \hline
B18-1  & [C2], [P5] & 04292+2422  &  04321540+2428597& $ 0.84 \pm 0.13 $
 & $<$602 & $>$1.09 & $>$0.014 & $>$0.179 &  I \\
 & & \&  F04292+2422  \\
B18--4& C1, P1 &  04325+2402  &  04353539+2408194  & $>$3.76  & $<$83 & $0.42~{\rm to}~0.79  $ & $ 0.053~{\rm to}~0.099 $ & $0.522~{\rm to}~0.589$ &  I \\
 & & \&  F04325+2402  \\
TMC-1C & P3 &  04385+2550  &  04413882+2556267  & $ 0.41 \pm 0.13 $ & $>$596 & $
0.23~{\rm to}~0.47  $ & $0.007~{\rm to}~0.015 $ & $ 0.042~{\rm to}~0.047  $ &  I \\
 & & \&  F04385+2550  \\
TMC-1  & C2, P2 &  04381+2540  &  04411267+2546354  & $ 1.52 \pm 0.14 $ & $ 131 $ & $
0.67 \pm 0.02  $ & $ 0.043 \pm 0.017 $ & $ 0.379 \pm 0.010 $ &  I \\
 & & \&  F04381+2540  \\
IRAS05413
 & C2, P2 &  05412-0105  &  05434630-0104439  & $ >$0.25  & $>$67 & $
0.52~{\rm to}~7.26  $ & $ 0.008~{\rm to}~0.115 $ & $0.308~{\rm to}~0.597  $ &  0 \\
 & & \&  F05411-0106  \\
 & C3, P3 &  05413-0104  &  none  & $ >$--0.70  & $<$55 & $\approx$10.5   & $\approx$0.017 & $\approx$0.95 &  0 \\
CB188
 & C1, P1 &  19179+1129  &  19201494+1135400  & $ >$0.88  & $<$248 & $1.74~{\rm to}~2.14  $ & $ 0.015~{\rm to}~0.018 $ & $0.272~{\rm to}~0.288  $ &  I \\
L1100  & C1, P1 &  20355+6343  &  none  & $ 0.70 \pm 0.18 $ & $<$103 & $
1.22~{\rm to}~2.13  $ & $ 0.023~{\rm to}~0.041 $ & $0.445~{\rm to}~0.515  $ &  I \\
 & & \&  F20355+6343  \\
L1041--2  & C4, P4 &  20361+5733  &  none  & $ >$3.12  & $<$60 & 
$ 3.91~{\rm to}~5.07 $ & $  0.025~{\rm to}~0.033 $ & $ 0.900~{\rm to}~0.966 $ &  0 \\
 & & \&  F20361+5733  \\
L1148  & C1, P1 &  F20404+6712  &  20405664+6723047  & $ >$--0.07 &
$ >$110  & $0.06~{\rm to}~0.40  $ & $ 0.023~{\rm to}~0.165 $ & $0.115~{\rm to}~0.146  $ &  I \\
L1082C
 & C1, P1 &  20503+6006  &  none  & $ >$1.05  & $ >$62  & $ 0.32~{\rm to}~1.73
$ & $  0.026~{\rm to}~0.141 $ & $ 0.402~{\rm to}~0.576 $ &  0\\
 & & \&  F20503+6007  \\
L1082A & C1, P1 &  20520+6003  &  20531346+6014425  & $ 0.39 \pm 0.20 $ & $ <$198  & $
1.00~{\rm to}~2.49  $ & $ 0.018~{\rm to}~0.044 $ & $
0.388~{\rm to}~0.491  $ &  I \\
 & C3, P5 &  20526+5958  &  none  & $  $ & $ <$119  &
$ 0.84~{\rm to}~1.36 $ & $
0.038~{\rm to}~0.061  $ & $ 0.538~{\rm to}~0.602 $ &  I\\
L1228
 & C1, P1 &  20582+7724  &  20571294+7735437  & $ 0.35 \pm 0.11 $ & $ 307 $ & $
2.27 \pm 0.04  $ & $ 0.035 \pm 0.008 $ & $ 0.782 \pm 0.007 $ &  I \\
 & & \&  F20582+7724  \\
Bern48
 & C1, P1 &  21004+7811  &  20591408+7823040  & $ -0.17 \pm 0.10 $ & $ 628 $ & $
11.05 \pm 0.20  $ & $ 0.008 \pm 0.001 $ & $ 0.483 \pm 0.003 $ &  I \\
 & & \&  F21004+7811  \\
L1172A
 & C2, P2 &  21017+6742  &  21022122+6754202  & $ >$--0.13  & $ <$100 & $
0.37~{\rm to}~0.59  $ & $ 0.049~{\rm to}~0.077 $ & $
0.370~{\rm to}~0.403  $ &  I\\
 & & \&  F21017+6742  \\
L1177
 & C1, P2 &  21169+6804  &  21173862+6817340  & $ 1.26 \pm 0.27 $ &
$ < 127 $ & $ 2.50~{\rm to}~3.32  $ & $ 0.038~{\rm to}~0.051 $ & $
1.030~{\rm to}~1.114  $ &  I \\
 & & \&  F21168+6804  \\
L1021
 & P1 &  21197+5046  &  21212751+5059475  & $ -0.82 \pm 0.13 $ & $ >$990 & $
4.09~{\rm to}~6.91  $ & $ 0.001~{\rm to}~0.002 $ & $
0.021~{\rm to}~0.024  $ &  II \\
L1251A
 & C2, P3 &  22290+7458  &  22300004+7513578  & $ >$0.68  & $ > $88  & $
0.12~{\rm to}~0.75  $ & $ 0.033~{\rm to}~0.216 $ & $
0.284~{\rm to}~0.380  $ &  I \\
 & & \&  F22290+7458  \\
\hline
\end{tabular}
\end{table}