Table 7: Bolometric luminosity and distance-normalised flux of Class 0 protostars in our sample.

Source		 $L_{\rm BOL}$ [$L_\odot$] $F_{\rm 1.3}^{\rm 220~pc}$ $L_{\rm BOL}$/ $F_{\rm 1.3}^{\rm 220~pc}$

L 1448 IRS 2		 6.01 0.80 7.5
L 1448 C 8.31 0.53 15.6
L 1455 A1 9.71 0.19 50.2
IRAS 03282 1.22 0.32 3.8
Barnard 1-B 2.8 0.74 3.8
HH 211 3.61 0.61 5.9
L 1527 1.91 0.38 5.0
L 483 13.02 0.70 18.5
SMM 5 3.61 - -
L 723 3.32 0.45 7.4
B 335 3.12 0.45 6.9
L 1157 5.82 0.68 8.6

1 Froebrich (2005); 2 Shirley et al. (2000).

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