\begin{table}%t5
\caption{Accretion properties of the $\lambda$ Ori cluster members.}\label{tab:acc_lor} 
%\centerline
 {\small \begin{tabular}{ccccccccc}
\hline \hline\noalign{\smallskip}
ID &   H$\alpha$ pEW  & H$\alpha$ 10\%width & Log~($\dot M_{\rm acc}$) &NII~6583~\AA & HeI~6678~\AA & SII~6716 \AA & SII~6731~\AA &Disk\\
&(\AA)& (km~s$^{-1}$) &($M_{\odot}$/yr) & (\AA)& (\AA)& (\AA) & (\AA)& class$^{~a}$\\
\hline 
L01 &  --$1.13\pm0.15$ &            --  &              --  &      $<$0.04 &      $<$0.04 &      $<$0.04 &      $<$0.04 &  III \\
L02 &  $-0.50\pm0.03$ &    $137\pm15$ &        $<$--11  &      $<$0.03 &      $<$0.03 &      $<$0.03 &      $<$0.03 &    -- \\
L03 &  $-1.58\pm0.13$ &            --  &              --  &      $<$0.03 &      $<$0.03 &      $<$0.03 &      $<$0.03 &  III \\
L04 &  $-1.00\pm0.08$ &    $155\pm13$ &        $<$--11  &      $<$0.03 &      $<$0.03 &      $<$0.03 &      $<$0.03 &    -- \\
L06 &  $-6.96\pm0.69$ &    $219\pm43$ &              --  &      $<$0.03 &         0.12 &      $<$0.03 &      $<$0.03 &  III \\
L07 &  $-2.00\pm0.12$ &    $137\pm20$ &              --  &      $<$0.05 &      $<$0.05 &      $<$0.05 &      $<$0.05 &  III \\
L08 &  $-5.30\pm0.30$ &    $198\pm18$ &              --  &      $<$0.03 &      $<$0.03 &      $<$0.03 &      $<$0.03 &  III \\
L09 &  $-2.44\pm0.23$ &    $155\pm22$ &        $<$--11  &      $<$0.03 &      $<$0.03 &      $<$0.03 &      $<$0.03 &    -- \\
L10 &              --  &            --  &              --  &           --  &           --  &           --  &           --  &  III \\
L11 &  $-8.47\pm0.47$ &    $215\pm25$ & $-10.80\pm0.40$ &      $<$0.06 &      $<$0.06 &      $<$0.06 &      $<$0.06 &   II \\
L12 &  $-3.32\pm0.35$ &    $146\pm34$ &              --  &      $<$0.06 &      $<$0.06 &      $<$0.06 &      $<$0.06 &  III \\
L14 &  $-3.67\pm0.34$ &    $148\pm29$ &              --  &      $<$0.06 &      $<$0.06 &      $<$0.06 &      $<$0.06 &  III \\
L15 &  $-5.15\pm0.62$ &    $141\pm18$ &              --  &      $<$0.08 &      $<$0.08 &      $<$0.08 &      $<$0.08 &  III \\
L16 &  $-7.05\pm0.86$ &    $306\pm52$ &              --  &      $<$0.06 &      $<$0.06 &      $<$0.06 &      $<$0.06 &  III \\
L17 &  $-1.89\pm0.15$ &    $132\pm50$ &        $<$--11  &      $<$0.06 &      $<$0.06 &      $<$0.06 &      $<$0.06 &    -- \\
L18 &  $-3.04\pm0.33$ &    $123\pm27$ &              --  &      $<$0.08 &      $<$0.08 &      $<$0.08 &      $<$0.08 &  III \\
L20 &  $-3.34\pm0.44$ &    $159\pm36$ &        $<$--11  &      $<$0.08 &      $<$0.08 &      $<$0.08 &      $<$0.08 &   EV \\
L22 & $-11.14\pm0.96$ &            --  &              --  &      $<$0.09 &      $<$0.15 &      $<$0.09 &      $<$0.09 &   II \\
L23 &  $-4.98\pm0.49$ &    $100\pm11$ &        $<$ -11  &      $<$0.09 &      $<$0.09 &      $<$0.09 &      $<$0.09 &    -- \\
L24 &  $-2.93\pm0.20$ &    $130\pm22$ &              --  &      $<$0.09 &      $<$0.09 &      $<$0.09 &      $<$0.09 &  III \\
L25 &  $-6.53\pm0.49$ &    $118\pm13$ &              --  &      $<$0.09 &      $<$0.09 &      $<$0.09 &      $<$0.09 &  III \\
L26 &  $-5.57\pm0.81$ &    $130\pm13$ &              --  &      $<$0.10 &         0.15 &      $<$0.10 &      $<$0.10 &  III \\
L27 &  $-5.20\pm0.52$ &    $107\pm11$ &              --  &      $<$0.10 &         0.20 &      $<$0.10 &      $<$0.10 &  III \\
L28 &  $-4.18\pm0.48$ &    $121\pm18$ &              --  &      $<$0.08 &      $<$0.08 &      $<$0.08 &      $<$0.08 &  III \\
L29 & $-13.97\pm1.38$ &    $274\pm15$ & $-10.20\pm0.30$ &      $<$0.10 &         0.18 &      $<$0.10 &      $<$0.10 &   II \\
L30 &  $-4.41\pm0.30$ &    $123\pm22$ &        $<$ -11  &      $<$0.10 &      $<$0.10 &      $<$0.10 &      $<$0.10 &   II \\
L31 &  $-7.90\pm1.26$ &    $116\pm16$ &              --  &      $<$0.10 &      $<$0.15 &      $<$0.10 &      $<$0.10 &  III \\
L32 &  $-7.39\pm1.46$ &            --  &              --  &      $<$0.10 &      $<$0.10 &      $<$0.10 &      $<$0.10 &  III \\
L33 & $-10.71\pm0.98$ &    $326\pm 9$ &              --  &      $<$0.10 &      $<$0.10 &      $<$0.10 &      $<$0.10 &  III \\
L34 & $-19.14\pm2.53$ &    $230\pm 4$ & $-10.70\pm0.30$ &         3.60 &         0.80 &         0.26 &         0.31 &   II \\
L35 &  $-4.92\pm0.60$ &    $121\pm20$ &              --  &      $<$0.10 &      $<$0.10 &      $<$0.10 &      $<$0.10 &  III \\
L36 &  $-5.06\pm0.53$ &    $127\pm25$ &        $<$--11  &      $<$0.10 &      $<$0.20 &      $<$0.10 &      $<$0.10 &   EV \\
L37 & $-14.47\pm1.25$ &    $287\pm41$ & $-10.10\pm0.50$ &         0.10 &      $<$0.10 &      $<$0.10 &      $<$0.10 &   EV \\
L38 &  $-5.32\pm0.68$ &    $134\pm16$ &              --  &      $<$0.10 &         0.10 &      $<$0.10 &      $<$0.10 &  III \\
L39 &  $-5.56\pm0.70$ &    $125\pm18$ &        $<$--11  &      $<$0.10 &      $<$0.20 &      $<$0.10 &      $<$0.10 &   EV \\
L40 &  $-9.44\pm1.12$ &    $107\pm13$ &              --  &      $<$0.10 &         0.17 &      $<$0.10 &      $<$0.10 &  III \\
L41 &  $-2.90\pm0.34$ &    $107\pm29$ &              --  &         0.14 &      $<$0.10 &      $<$0.10 &      $<$0.10 &  III \\
L42 &  $-6.25\pm0.94$ &    $137\pm29$ &              --  &      $<$0.10 &         0.15 &      $<$0.10 &      $<$0.10 &  III \\
L43 & $-15.53\pm2.23$ &    $228\pm18$ &              --  &      $<$0.20 &      $<$0.20 &      $<$0.20 &      $<$0.20 &  III \\
L44 &  $-4.96\pm0.62$ &    $105\pm 9$ &              --  &      $<$0.25 &      $<$0.25 &      $<$0.25 &      $<$0.25 &  III \\
L45 &  $-6.97\pm1.10$ &    $114\pm20$ &        $<$--11  &         0.22 &      $<$0.20 &      $<$0.20 &      $<$0.20 &   II \\
L46 &  $-8.18\pm1.40$ &     $98\pm 6$ &              --  &         0.60 &      $<$0.25 &         0.59 &      $<$0.25 &  III \\
L47 &  $-5.94\pm0.96$ &     $93\pm 4$ &              --  &         0.25 &      $<$0.10 &         0.25 &         0.16 &  III \\
L48 &              --  &            --  &              --  &           --  &           --  &           --  &           --  &  III \\
L49 & $-26.16\pm2.40$ &    $107\pm 4$ &        $<$--11  &         0.70 &         0.40 &         0.40 &         0.30 &   II \\
\hline
\end{tabular}}
\medskip
 $^a$~Disk classification from \cite{Barrado2007ApJ}: -- = Spitzer non-members, III~=~diskless,  
 II~=~thick disk, EV~=~evolved disk.
\end{table}