Table 7: 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. 4.1 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.
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 $L_{\odot}$   $M_{\odot}$  
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              


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