Table 4: Dust masses of debris disks around A- to K-type main sequence stars. Note that HD 34700 and HD 39944 previously classified as debris disks have been rejected; HD 34700 is a T Tauri (Sterzik et al. 2005) and has gas emission (Dent et al. 2005) and HD 39944 was confused with a background galaxy (Moór et al. 2006).
Star Sp. dist age $ \rm S_{\nu}$ $\lambda$ Disk Dust Dust
  type (pc) (Myr) (mJy) (mm) radius temp mass
            (AU) (K) (moon)
$\tau$ Ceti G8V 3.65 10000 $4.6 \pm 0.6^{a}$ 0.85 55 40 0.04
$\epsilon$ Eri K2V 3.22 730 $40 \pm 1.5^{b}$ 0.85 60 37 0.26
GL 182 M0.5 26.7 20-150 $4.8\pm 1.2^{c}$ 0.85 60 27 3.35
HD 104860 F8 47.9 40 $6.8\pm 1.2^{d}$ 0.85 60 49 7.1
HD 8907 F8 34.2 180 $4.8\pm 1.2^{d}$ 0.85 60 49 2.6
$\beta$ Pic A5V 19.3 12 $104\pm 10^{e}$ 0.85 60 77 11
HD 38393 F7V 8.97 1660 $2.4\pm 1.0^{f}$ 0.85 200 31 0.15
HD 48682 G0V 16.5 3300 $5.5\pm 1.0^{f}$ 0.85 110 38 0.9
HD 74067B A2V 30 63 $7.2\pm 1.5^{h}$ 0.85 60 92 1.4
HD 99803B A3V 100 123 $4.7\pm 1.6^{h}$ 0.85 60 86 11.3
HD 107146 G2V 28.5 80 $20\pm 4^{i}$ 0.85 60 47 7.8
$\eta$ Corvi F2V 18.2 1000 $14.1\pm 1.8^{m}$ 0.85 150 43 2.5
HD 112412 F1 25 28 $3.8\pm 1.1^{h}$ 0.85 60 64 0.8
HD 128167 F2V 15.5 1700 $6.2\pm 1.7^{f}$ 0.85 320 31 1.2
HD 131156 G4V 6.70 200 $6.2\pm 1.9^{j}$ 1.30 60 45 0.4
Vega A0V 7.76 350 $45.7\pm 5.4^{f}$ 0.85 70 97 0.6
AU Mic M1 9.9 12 $14.4\pm 1.8^{c}$ 0.85 40 31 1.2
Fomalhaut A3V 7.69 280 $97\pm 5^{f}$ 0.85 80 61 1.6
HD 218396 A5V 40 n/a $28\pm 11^{k}$ 1.10 60 77 24.6
a Greaves et al. (2004); b Greaves et al. (1998); c Liu et al. (2004); d Najita & Williams (2005); e Zuckerman et al. (1993); f Sheret et al. (2004); h Wyatt et al. (2003); i Williams et al. (2004); j Holmes et al. (2003); k Sylvester et al. (1996); l Wilner et al. (2003); m Wyatt et al. (2005).

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