Table 1: Interferometric measurements of dust continuum emission.

Ref.(1)		 $\lambda$ HPBW $F_{{\rm peak}}^{(2)}$ $F_{{\rm int}}^{(3)}$ Size Interf.
  (mm) ( $\hbox{$^{\prime\prime}$ }\times \hbox{$^{\prime\prime}$ }$) (mJy beam-1) (mJy) ( $\hbox{$^{\prime\prime}$ }\times \hbox{$^{\prime\prime}$ }$)  
D01 1.33 2.0 $\times$ 1.7 1200 $\pm$ 16 3100 $\pm$ 470 5.3 $\times$ 4.1 PdBI
D01 2.04 3.2 $\times$ 2.3 450 $\pm$ 14 690 $\pm$ 110 4.4 $\times$ 3.4 NMA
D01 2.19 3.4 $\times$ 2.6 420 $\pm$ 10 580 $\pm$ 90 4.2 $\times$ 3.3 NMA
L00 2.7 5.5 $\times$ 5.0 351 $\pm$ 3 544 $\pm$ 14 25 $\times$ 24 BIMA
    3.0 $\times$ 2.8 280 $\pm$ 2 526 $\pm$ 9 12 $\times$ 18.5 BIMA
    1.2 $\times$ 1.1 172 $\pm$ 2 450 $\pm$ 10 5.4 $\times$ 6.2 BIMA
D01 3.22 2.9 $\times$ 2.6 200 $\pm$ 4.4 320 $\pm$ 49 4.5 $\times$ 3.7 PdBI
D01 6.92 2.1 $\times$ 1.9 16 $\pm$ 0.29 26 $\pm$ 4 3.3 $\times$ 2.8 VLA
D01 13.3 3.8 $\times$ 3.1 3.1 $\pm$ 0.27 4.7 $\pm$ 1.0 6.3 $\times$ 3.6 VLA
(1) References: L00: Looney et al. (2000); D01: Di Francesco et al. (2001). (2) Quoted errors are statistical only and do not include any systematic calibration uncertainties. (3) Flux integrated over a region of size listed in Col. 6.

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