\begin{table}%t5
\caption{\label{tab:OIlineemission_models}Results for the fine structure emission lines from various disk models and test runs.}
%\centering
 \small 
\begin{tabular}{ll|lll|lll|lll}
\hline\hline\\[-3.5mm] &&&&&&&&&&\\[-2mm]
& & \multicolumn{3}{|c|}{O~{\sc i} 63~$\mu$m} & \multicolumn{3}{|c|}{O~{\sc i} 145~$\mu$m} & \multicolumn{3}{|c}{C~{\sc ii}~157.7~$\mu$m} \\
$M_{\rm disk}$ & Model  & $F_{\rm line}$ & $F_{\rm cont}$ & Peak sep. & $F_{\rm line}$ & $F_{\rm cont}$ & Peak sep. & $F_{\rm line}$ & $F_{\rm cont}$ & Peak sep. \\
  $[M_\odot]$  
& & [$10^{-18}$~W/m$^2$] & [Jy] & [km~s$^{-1}$] &  [$10^{-18}$~W/m$^2$] & [Jy] & [km~s$^{-1}$] & [$10^{-18}$~W/m$^2$] & [Jy] & [km~s$^{-1}$] \\
\hline\\[-6mm] &&&&&&&&&&\\
$2.2 \times 10^{-2}$ & MC & 1.93(3) & 1.44(2) & 1.9 & 2.13(2) & 1.25(2) & 2.6 & 5.39(1) & 1.14(2) & 2.2 \\
$10^{-2}$ & MC & 1.29(3) & 1.03(2) & 2.4 & 1.18(2) & 6.57(1) & 3.0 &     4.69(1) & 5.91(1) & 2.2 \\
$10^{-3}$ & MC & 6.57(2) & 2.58(1) & 2.5 & 3.89(1) & 8.84 & 5.9 &     2.98(1) & 7.69 & 2.2 \\
$10^{-4}$ & MC & 2.65(2) & 4.56 & 5.9 & 8.06 & 9.09(--1) & 6.2 & 1.40(1) & 1.01 & 2.4 \\
$10^{-5}$ & MC & 4.19(1) & 9.89(--1) & 7.7 & 1.11 & 1.72(--1) & 6.0 & 4.53 & 2.71(--1) & 2.3 \\
$10^{-6}$ & MC & 1.99 & 1.50(--1) & 12.2 & 5(--2) & 3(--2) & 10.3 &    2.77 & 1.43(--1) & 2.2 \\ 
\hline \\[-6mm] &&&&&&&&&&\\
$10^{-2}$ & LTE & 2.25(3) & 1.05(2) & 2.2 & 1.30(2) & 6.63(1) & 2.7 &     5.22(1) & 5.96(1) & 2.2 \\
$10^{-2}$ & ES & 1.27(3) & 1.05(2) & 2.3 & 1.23(2) & 6.63(1) & 2.9 &     4.93(1) & 5.96(1) & 2.2 \\
\hline\\[-6mm] &&&&&&&&&&\\
$10^{-2}$ & no O~{\sc i} $>$2000~K & 1.29(3) & 1.03(2) & 2.4 & 1.18(2) & 6.57(1) & 3.0 &     & & \\
$10^{-2}$ & $R_{\rm in,out}=0.5,500$~AU & 1.23(3) & 1.06(2) & 2.6 & 1.14(2) & 6.16(1) & 3.2 &      2.26(1) & 5.41(1) & 2.7 \\
$10^{-2}$ & $R_{\rm in,out}=0.5,300$~AU & 9.40(2) & 1.01(2) & 3.3 & 8.99(1) & 4.98(1) & 4.0 &      7.33 & 4.66(1) & 3.5 \\
$10^{-2}$ & $R_{\rm in,out}=0.5,100$~AU & 5.74(2) & 8.27(1) & 5.6 & 4.18(1) & 3.19(1) & 6.0 &     1.35 & 2.76(1) & 6.3 \\
$10^{-2}$ & $R_{\rm in,out}=0.5,30$~AU & 2.40(2) & 5.03(1) & 11.2 & 1.26(1) & 1.47(1) & 11.4 &     & & \\
$10^{-2}$ & $R_{\rm in,out}=30,100$~AU & 3.70(2) & 3.42(1) & 5.5 & 3.08(1) & 1.75(1) & 6.1 &     & & \\
$10^{-2}$ & $R_{\rm in,out}=30,700$~AU & 1.11(3) & 6.13(1) & 2.5 & 1.08(2) & 5.29(1) & 3.0 &     4.64(1) & 4.82(1) & 2.2 \\
$10^{-2}$ & $R_{\rm in,out}=100,700$~AU &  & &  &  &  &  &     4.59(1) & 3.31(1) & 2.2 \\
\hline\\[-6mm] &&&&&&&&&&\\
$10^{-2}$ & $T_{\rm eff}=9500$~K & 5.53(3) & 1.68(2) & 2.8 & 4.56(2) & 8.60(1) & 2.9 & 1.50(2) & 7.63(1) & 2.3 \\ 
$10^{-2}$ & $T_{\rm eff}=10500$~K & 9.03(3) & 1.78(2) & 3.1 & 6.75(2) & 8.85(1) & 2.8 & 3.17(2) & 7.84(1) & 2.3 \\
\hline\\[-6mm] &&&&&&&&&&\\
$10^{-2}$ & $a_{\rm min,max}=0.01,1~\mu$m & 6.48(2) & 1.42(2) & 2.3 & 3.24(1) & 3.53(1) & 2.5 & 6.30(1) & 2.85(1) & 2.2 \\
$10^{-2}$ & $a_{\rm min,max}=1,200~\mu$m & 3.22(3) & 1.44(2) & 2.7 &  3.17(2) & 7.21(1) & 3.2 & 2.39(1) & 6.42(1) & 2.2 \\
\hline
\end{tabular}
\tablefoot{In the model column, MC, LTE and ES denote the use of level populations from Monte Carlo line radiative transfer, LTE and escape probability, respectively. Line and continuum fluxes are shown for a distance of 131~pc and an inclination of 45~degrees. Numbers in parentheses indicate powers of ten, i.e. $1.93(3)$ denotes $1.93 \times 10^3$. The peak separation is defined as the distance between the two maxima in the double peaked line profile measured in~km~s$^{-1}$.}
%\vspace*{4mm}
\end{table}