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Table 3:

Search for debris disks around nearby M-dwarfs with our new MAMBO-2 data.
Name Spectral D Gal. l. Integration Map rms Mean brightness $\mu / \sigma _{\mu }$ $3\sigma$ flux density
  type (pc) ($^{\circ}$) time (mJy/11'' beam) $\mu \pm \sigma_{\mu}$ (2) upper limit (1.2 mm)
        (h)   (mJy/11'' beam)   (mJy)
          (1) (2)   (3)
GJ699 M4.0 1.82 14 1.5 1.22 -0.03 $\pm$ 0.08 -0.36 <7.9
GJ406 M6.0 2.38 56 2.5 0.99 -0.18 $\pm$ 0.08 -2.29 <4.9
GJ411 M2.0 2.54 65 6.5 0.67 0.06 $\pm$ 0.06 0.97 <3.1
GJ905 M5.5 3.16 -17 0.5 2.30 0.09 $\pm$ 0.24 0.38 <8.6
GJ447 M4.0 3.34 59 1.5 1.19 -0.09 $\pm$ 0.13 -0.69 <4.2
GJ725(*) M3+M3.5 3.57 24 1.0 1.44 0.29 $\pm$ 0.17 1.69 <4.7
GJ1111 M6.5 3.62 32 1.0 1.75 0.09 $\pm$ 0.20 0.44 <5.7
GJ54.1 M4.5 3.72 -79 1.5 1.49 -0.33 $\pm$ 0.18 -1.86 <4.7
GJ273 M3.5 3.79 10 0.5 2.13 0.17 $\pm$ 0.25 0.68 <6.6
GJ234 M4.5+M8 4.12 -6 2.5 1.03 0.30 $\pm$ 0.13 2.23 <2.9
GJ83.1 M4.5 4.44 -46 1.5 1.40 -0.37 $\pm$ 0.18 -2.11 <3.7
GJ687 M3.0 4.53 32 4.0 0.76 0.25 $\pm$ 0.11 2.18 <2.9
LHS292 M6.5 4.54 41 0.5 2.29 -0.35 $\pm$ 1.52 -0.23 <5.9
GJ1002 M5.5 4.69 -69 0.5 2.23 0.14 $\pm$ 0.33 0.43 <5.6
GJ412 M2+M6 4.83 63 0.5 2.26 -0.21 $\pm$ 0.36 -0.58 <5.4
GJ388 M3.0 4.89 54 5.0 0.73 0.20 $\pm$ 0.06 3.25 <1.8
GJ445 M3.5 5.38 38 1.0 1.55 0.05 $\pm$ 0.28 0.18 <3.4
LHS1723 M4.5 5.43 -27 0.5 2.23 0.49 $\pm$ 0.42 1.17 <4.8
GJ526(**) M1.5 5.43 72 16.0 0.58 -0.02 $\pm$ 0.12 -0.16 <1.4
GJ251 M3.0 5.57 15 1.0 1.54 0.14 $\pm$ 0.29 0.48 <1.7
GJ205 M1.5 5.71 -19 1.0 1.86 -1.09 $\pm$ 0.37 -2.93 <2.0
GJ213 M4.0 5.87 -9 0.5 2.19 -0.31 $\pm$ 0.44 -0.70 <2.4
GJ908 M1.0 5.93 -57 0.5 2.01 0.24 $\pm$ 0.39 0.61 <2.2
GJ581 M3 6.27 40 0.5 1.96 -0.75 $\pm$ 0.43 -1.75 <2.1
GJ625 M1.5 6.58 43 5.0 0.69 0.38 $\pm$ 0.15 2.53 <0.7
GJ408 M2.5 6.62 64 2.0 1.13 0.42 $\pm$ 0.14 3.05 <1.2
GJ109 M3.5 7.55 -31 3.0 0.98 0.32 $\pm$ 0.22 1.48 <1.1
GJ102 M4 7.75 -32 0.5 2.20 -0.09 $\pm$ 0.60 -0.15 <2.4
GJ4247 M4 8.96 -21 3.5 0.74 0.63 $\pm$ 0.25 2.56 <0.8
GJ569 (*) M2.5+M8.5 9.81 59 2.0 1.09 -0.46 $\pm$ 0.37 -1.25 <1.2

(1) rms estimated for r < 60'' in the map; (2) mean brightness and uncertainty of mean computed by averaging intensities over an effective disk of radius 60 AU; (3) the $3\sigma$ flux density upper limit is computed also over the same effective area (radius = 60 AU). (*): background sources in map (see Table 2); (**): possibly a large debris disk (see Fig. 1 and Sect. 4.1.3).


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