\begin{table}%ta.13
%%\centering
\par
\caption{\label{disksTable}Compilation of disks masses$^1$.} %\\
\nocite{ack04, pie03, man00, nat97, nat01, hen98b, hen94, dif97, pie06, man97, syl01, fue03, fue06, alo08}
%\centerline
 {\small\begin{tabular}{llllllllll}
\hline\hline 
Name & Spectral & Luminosity & Teff & Distance & Star mass & Age & $\lambda$ & Flux & Disk mass \\ 
 & type & ($L_\odot$) & (K) & (pc) & ($M_\odot$) & (Myr) & (mm) & (mJy) & ($M_\odot$) \\  
\hline 
AB Aur & A0 & 49 & 9500 & 144 & 2.57 & 3.87 & 1.4 & 85 & 0.0278 \\ %  & $>$3 & 2 \\
HD 100546 & B9 & 45 & 10~500 & 103 & 2.53 & 5.59 & 1.3 & 465 & 0.0540 \\ %  & - & 4 \\
HD 142527 & F6 & 69 & 6300 & 200 & 3.54 & 1.11 & 1.3 & 1190 & 1.4860 \\ %  & - & 4 \\
HD 179218 / MWC 614 & B9 & 500 & 10~000 & 240 & 5.02 & 0.473 & 1.3 & 71 & 0.0447 \\ %  & - & 2 \\
HD 100453 & A9 & 8 & 7400 & 114 & 1.66 & 14.1 & 1.2 & 270 & 0.0709 \\ %  & - & 4 \\
CD-36 10010B & F8 & 8 & 6200 & 84 & 1.63 & 9.49 & 1.3 & 142 & 0.0345 \\ %  & - & 4 \\
HD 139614 & A7 & 11 & 7800 & 157 & 1.83 & 10.7 & 1.3 & 242 & 0.1293 \\ %  & - & 4 \\
HD 169142 & B9 & 44 & 10~500 & 145 & 2.5 & 5.69 & 1.3 & 169 & 0.0389 \\ %  & - & 2 \\
HD 142666 & A8 & 8 & 7500 & 116 & 1.65 & 14.9 & 1.2 & 79 & 0.0201 \\ %  & - & 2 \\
HD 144432 & A9 & 32 & 7300 & 200 & 2.26 & 3.87 & 1.3 & 37 & 0.0369 \\ %  & - & 4 \\
HD 150193 / MWC 863 & A1 & 30 & 9500 & 150 & 2.25 & 6.10 & 1.3 & 45 & 0.0143 \\ %  & - & 2 \\
HD 163296 & A1 & 36 & 9500 & 122 & 2.49 & 5.79 & 1.3 & 705 & 0.1485 \\ %  & - & 2 \\
HD 34282 & A0 & 36 & 9500 & 400 & 2.49 & 5.79 & 1.3 & 110 & 0.2259 \\ %  & - & 2 \\
HD 35187 & A2 & 34 & 9100 & 150 & 2.43 & 4.65 & 1.2 & 20 & 0.0055 \\ %  & - & 4 \\
UX Ori & A3 & 42 & 8600 & 430 & 2.43 & 4.22 & 1.2 & 19.8 & 0.0481 \\ %  & 0 & 2 \\
CQ Tau & F2 & 5 & 6800 & 100 & 1.49 & 769 & 1.3 & 143 & 0.0415 \\ %  & - & 2 \\
MWC 758 & A3 & 21 & 8500 & 200 & 2.17 & 6.26 & 1.3 & 72 & 0.0471 \\ %  & $>$2 & 2 \\
LkH$\alpha$259 & A9 & 107 & 7320 & 850 & 3.6 & 1.17 & 2.6 & $<$6 & $<$0.722 \\ %  & - & 3 \\
WW Vul & A3 & 43 & 8600 & 550 & 2.44 & 4.19 & 1.2 & 9.1 & 0.0362 \\ %  & - & 2 \\
BF Ori & A5 & 34 & 8300 & 450 & 2.34 & 4.37 & 1.3 & 6 & 0.0228 \\ %  & 4 & 4 \\
SV Cep & A0 & 14 & 8600 & 715 & 1.91 & 11.7 & 1.3 & 7 & 0.0459 \\ %  & - & 4 \\
V376 Cas & B5 & 190 & 13~800 & 600 & 3.77 & 2.66 & 2.7 & $<$5 & $<$0.089 \\ %  & - & 3 \\
LkH$\alpha$198 & B7 & 210 & 12~000 & 600 & 3.51 & 1.49 & 2.7 & $<$5 & $<$0.1141 \\ %  & 6 & 3 \\
VY Mon & B8 & 1400 & 10~700 & 800 & 6.9 & 0.243 & 1.3 & 120 & 0.6874 \\ %  & 25 & 4 \\
HD 97048 & A0 & 44 & 10~000 & 150 & 2.53 & 4.61 & 1.3 & 452 & 0.1305 \\ %  & - & 4 \\
LkH$\alpha$234 & B5 & 800 & 14~500 & 1250 & 5.01 & 0.524 & 1.3 & $<$20 & $<$0.181 \\ %  & - & 2 \\
T Ori & A3 & 83 & 8500 & 460 & 2.92 & 2.49 & 1.3 & $<$6 & $<$0.021 \\ %  & 5 & 2 \\
V380 Ori & B9 & 100 & 9500 & 460 & 3.05 & 2.00 & 1.3 & $<$24 & $<$0.056 \\ %  & 3 & 4 \\
%HD 52721 & B2 & 67600 & 22400 & 1150 & - & - & 1.3 & 23 & 0.0933 \\ %  & 10 & 4 \\
LkH$\alpha$218 & B9 & 107 & 10~700 & 1150 & 2.97 & 2.77 & 1.3 & $<$27 & $<$0.3906 \\ %  & 8 & 4 \\
Elias 3-1 & A6 & 21 & 8000 & 140 & 2.06 & 6.11 & 2.7 & 45 & 0.1360 \\ %  & $>$2 & 3 \\
BD+404124 & B2 & 5900 & 22~000 & 1000 & -- & -- & 2.7 & $<$5 & $<$0.133 \\ %  & 19 & 3 \\
V1686 Cyg & B5 & 1820 & 15~500 & 1000 & 6.05 & 0.312 & 2.7 & $<$5 & $<$0.246 \\ %  & - & 3 \\
BD+61154 & B8 & 225 & 11~800 & 650 & 3.88 & 1.43 & 2.7 & 11.2 & 0.3509 \\ %  & - & 3 \\
RR Tau & A4 & 150 & 8800 & 800 & 3.57 & 1.34 & 1.3 & $<$20 & $<$0.224 \\ %  & 7 & 4 \\
HD 200775 & B2 & 1900 & 18~500 & 600 & 6.9 & 0.337 & 1.3 & $<$6 & $<$0.007 \\ %  & 8 & 4 \\
MWC 480 & A3 & 25 & 8500 & 130 & 2.19 & 5.98 & 1.4 & 235 & 0.0797 \\ %  & $>$3 & 2 \\
HD 34700 & G0 & 20 & 6000 & 90 & 2.36 & 3.39 & 1.35 & 11.7 & 0.0037 \\ %  & - & 4 \\
MWC 297 & B1.5 & 10~700 & 24~000 & 250 & 9 & 1 & 1.3 & 168.6 & 0.0323 \\ %  & $>$5 & 1 \\
Z CMa & B8 & 9200 & 20~000 & 930 & 12 & 0.05 & 1.4 & 24.1 & 0.2307 \\ %  & $>$1 & 1 \\
R Mon & B0 & 5600 & 25~000 & 800 & 8 & 1 & 1.4 & 8.3 & 0.0093 \\ %  & 1 & 1 \\
MWC 1080 & B0 & 5600 & 25~000 & 1000 & 10 & 1 & 1.4 & 2.1 & 0.0036 \\ %  & $>$9 & 1 \\
MWC 137 & B0 & 15~000 & 26~000 & 1300 & 14 & 1 & 1.4 & 7.1 & $<$0.007 \\ %  & $>$59 & 1 \\
VV Ser & A0 & 50 & 10~000 & 260 & 2.68 & 3.87 & 1.3 & 1.44 & 0.0012 \\ %  & 24 & 1 \\
LkH$\alpha$~215 & B7.5 & 5300 & 22~000 & 800 & 7 & 0.4 & 1.4 & $<$1.5 & $<$0.009 \\ %  & 7 & 1 \\
 \hline
\end{tabular}}
\medskip
$^1$ The flux shown is the excess at 1.3~mm subtracting the free-free contribution in our sources. In MWC~297 we have used the flux of \cite{man07}. References for the mm fluxes are:
  \citet{ack04},  \citet{alo08}, \citet{dif97}, \citet{fue03}, \citet{fue06}, \citet{hen94},  Henning et~al. (1998), Mannings et~al. (1997),
Mannings et~al. (2000), \citet{nat97}, \citet{nat01}, \citet{pie03},
\citet{pie06}, Sylvester et al. (2001).
\end{table}