\begin{table}%t1
\par
\caption{\label{tbl:disks}FIR and stellar properties of the candidate disks and their associated stars. }\vspace*{-2mm}
\small%\centering
\par
\begin{tabular}{llccccccc}
\hline\hline\noalign{\smallskip}
\mbox{H-ATLAS} ID & SDSS ID &  Sp.~type & Distance (pc) &  $F_{250}$ (mJy) & $F_{350}$ (mJy) & $F_{500}$ (mJy) & $T$ (K) & Dust mass ($M_{\oplus}$)\\
\noalign{\smallskip}\hline
 J090315.8+015758 & J090315.91+015800.9 &  K2 & 90--130 & $51\pm14$ & $53\pm14$ & $19\pm9$ & 65 & 0.06--0.13 \\
 J090240.2$-$014351 & J090240.10-014349.7 & G5 & 190--290 & $86\pm12$ & $48\pm7$ & $17\pm9$ &  60 & 0.5--1.3 \\
 \hline
\end{tabular}\vspace*{-2mm}
\tablefoot{Spectral types are estimated from the $(g - i)$ colour relation of \citet{covey2007} and distances from the photometric parallax from \citet{davenport2006}. Temperatures are estimated by a greybody fit to the 250, 350 and~500~$\mu$m fluxes and the upper limits of 140~mJy at 160~$\mu$m, and 105~mJy at 110~$\mu$m with a fixed $\beta= 0.5$ \citep{wyatt2005}. Masses are calculated using the standard technique with a mass absorption coefficient  $\kappa = 1.7$~cm$^{2}$~g$^{-1}$ at~850~$\mu$m \citep{sheret2004}.}
\vspace*{-3mm}\end{table}