\begin{table}%t4
\small
\caption{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. \cite{Sterzik2005}) and has gas emission (Dent et~al. \cite{Dent2005}) and HD~39944 was confused with a background galaxy (Mo\'or et~al. \cite{Mo\'or2006}).}\label{tab4}
%\centerline
{\begin{tabular}[h]{lrccrcccc} 
\hline\hline
Star           & Sp.  & dist   & age    &  $ \rm S_{\nu}$    & $\lambda$ & Disk   & Dust   &  Dust   \\
                      & type &  (pc)  & (Myr)  & (mJy)              &  (mm)     & radius & temp   &  mass  \\
                      &      &        &        &                    &           &   (AU) & (K)    &  (moon)  \\     
\hline 
$\tau$ 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~34700         & G0V  &  89    & n/a    & $40.7\pm 2.4^{d}$  &  0.85     &  60    &  49    & 148     \\
%%    HD~39944         & G1V  &  109   & n/a    & $3.7\pm 0.9^{d}$   &  1.30     &  60    &  48    &  71     \\
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  \\
\hline
\end{tabular}}
\smallskip
  $^a$ Greaves et~al. (\cite{Greaves2004});  $^b$ Greaves et~al. (\cite{Greaves1998}); $^c$ Liu et~al. (\cite{Liue2004}); $^d$ Najita \& Williams (\cite{Najita2005});  $^e$ Zuckerman et~al. (\cite{Zuckerman1993}); $^f$ Sheret  et~al. (\cite{Sheret2004});  $^h$~Wyatt et~al. (\cite{Wyatte2003});  $^i$  Williams et~al. (\cite{Williams2004});   $^j$ Holmes et~al. (\cite{Holmes2003}); $^k$  Sylvester et~al. (\cite{Sylvester1996});  
 $^l$ Wilner et~al. (\cite{Wilner2003}); $^m$  Wyatt et~al.  (\cite{Wyatt2005}).
\end{table}