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Table 5:

SCUBA observations of the M-dwarfs associated with moving groups in survey I (Lestrade et al. 2006).

Star
Sp. Dist. Integration Flux density a Size b
  type (pc) time 850 $\mu $m        (AU)  
      (h) (mJy)          
GJ82 M4 12.0 2 2.0 $\pm$ 1.4 84
GJ212 M0.5 12.5 2 1.3 $\pm$ 1.4 88
GJ285c M4.5 5.9 1 -0.7 $\pm$ 1.9 41
GJ393c M2 7.2 1 1.9 $\pm$ 1.9 50
GJ507.1 M1.5 17.4 1 -0.4 $\pm$ 2.0 121
GJ696 M0 21.9 2 0.8 $\pm$0.8 150
GJ9809c M0 24.9 1 -5.2 $\pm$ 2.3 174
GJ4247c M4 9.0 1 1.1 $\pm$ 2.1 63
GJ277B M3.5 11.5 1 -2.1 $\pm$ 1.8 80
GJ842.2 M0.5 20.9 4 25.0 $\pm$ 4.6 300
GJ890 M2 21.9 2 -2.6 $\pm$ 1.6 153
GJ875.1 M3 14.2 1 0.52 $\pm$ 2.1 99

a Flux density from wide photometry. b Size is the radius of a debris disk as large as the telescope beam (14''). c Stars also observed by MAMBO-2 in Tables 3 and 4.


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