\begin{table} %t4 %online
%\centering
\par
\caption{Same than Table~\ref{moldisks:results1} but for the Herbig~Ae stars.\label{moldisks:results2}}
\par
\begin{tabular}{lllll}
\hline
\hline
\noalign{\smallskip}
            & \multicolumn{1}{c}{Telescope} & \multicolumn{1}{c}{d$v$} & \multicolumn{1}{c}{$T_{\rm A}^*$} &  \multicolumn{1}{c}{$T_{\rm ther}$}\\
            &             &       \multicolumn{1}{c}{(km s$^{-1}$)} & \multicolumn{1}{c}{(K)} & \multicolumn{1}{c}{(K)}\\
\hline
\noalign{\smallskip}
\multicolumn{5}{c}{\object{HD~163296}}\\
\hline
\noalign{\smallskip}
$^{12}$CO $J\!=\!3\!\rightarrow\!2$               & JCMT &        0.23   &\phantom{$<$}0.920  & 0.130 \\    
$^{13}$CO $J\!=\!3\!\rightarrow\!2$               & JCMT &        0.28   &\phantom{$<$}0.225  & 0.052 \\   
HCO$^+$ $J\!=\!4\!\rightarrow\!3$                 & JCMT &        0.26   &\phantom{$<$}0.128  & 0.030 \\    
CN $J\!=\!3\frac{7}{2}\!\rightarrow\!2\frac{5}{2}$& JCMT &        0.27   &\phantom{$<$}0.115  & 0.018 \\   
HCN $J\!=\!4\!\rightarrow\!3$                     & JCMT &        0.26   &  $<$0.074 (2$\sigma$)  & 0.037 \\  
H$_{\rm 2}$CO $J\!=\!5_{15}\!\rightarrow\!4_{14}$ & JCMT &        0.27   &  $<$0.204 (2$\sigma$)  & 0.102 \\   
H$_{\rm 2}$CO $J\!=\!2_{12}\!\rightarrow\!1_{11}$ & IRAM30 m &     0.17   &  $<$0.018 (2$\sigma$)  & 0.009  \\ 
H$_{\rm 2}$CO $J\!=\!3_{03}\!\rightarrow\!2_{02}$ & IRAM30 m &     0.11   &  $<$0.030 (2$\sigma$)  & 0.015  \\ 
H$_{\rm 2}$CO $J\!=\!3_{12}\!\rightarrow\!2_{11}$ & IRAM30 m &     0.10   &  $<$0.018 (2$\sigma$)  & 0.009 \\  
CH$_{\rm 3}$OH $J\!=\!2_K\!\rightarrow\!1_K$      & IRAM30 m &     0.12   &  $<$0.014 (2$\sigma$)  & 0.007 \\  
\hline
\noalign{\smallskip}
\multicolumn{5}{c}{\object{MWC~480}}\\
\hline
\noalign{\smallskip}
$^{12}$CO $J\!=\!3\!\rightarrow\!2$                   & JCMT &       0.13  & \phantom{$<$}0.498   & 0.073 \\    
$^{13}$CO $J\!=\!3\!\rightarrow\!2$                   & JCMT &       0.28  &\phantom{$<$}0.102   & 0.016 \\    
C$^{18}$O $J\!=\!3\!\rightarrow\!2$                   & JCMT &       0.14  &  $<$0.062 (2$\sigma$)   & 0.031 \\    
HCO$^+$ $J\!=\!4\!\rightarrow\!3$                     & JCMT &       0.26  &\phantom{$<$}0.052   & 0.017 \\    
DCO$^+$ $J\!=\!5\!\rightarrow\!4$                     & JCMT &       0.13  &  $<$0.106 (2$\sigma$)   & 0.053 \\    
CN $J\!=\!3\frac{7}{2}\!\rightarrow\!2\frac{5}{2}$    & JCMT &       0.27  &\phantom{$<$}0.038   & 0.017 \\    
CS $J\!=\!7\!\rightarrow\!6$                          & JCMT &       0.27  &  $<$0.040 (2$\sigma$)   & 0.020 \\    
HCN $J\!=\!4\!\rightarrow\!3$                         & JCMT &       0.53  &  $<$0.024 (2$\sigma$)  & 0.012 \\     
H$_{\rm 2}$CO $J\!=\!3_{12}\!\rightarrow\!2_{11}$     & JCMT &       0.43  &  $<$0.030 (2$\sigma$)  & 0.015 \\     
H$_{\rm 2}$CO $J\!=\!5_{15}\!\rightarrow\!4_{14}$     & JCMT &       0.27  &  $<$0.032 (2$\sigma$)   & 0.016 \\     
H$_{\rm 2}$D$^+$  $J\!=\!1_{10}\!\rightarrow\!1_{11}$ & JCMT &       0.12  &  $<$0.090 (2$\sigma$)   & 0.045 \\    
N$_{\rm 2}$H$^+$  $J\!=\!4\!\rightarrow\!3$           & JCMT &       0.12  &  $<$0.126 (2$\sigma$)   & 0.063 \\    
H$_{\rm 2}$CO $J\!=\!2_{12}\!\rightarrow\!1_{11}$     & IRAM30 m &    0.21  &  $<$0.016 (2$\sigma$)   & 0.008 \\    
H$_{\rm 2}$CO $J\!=\!3_{22}\!\rightarrow\!2_{21}$     & IRAM30 m &    1.37  &  $<$0.006 (2$\sigma$)   & 0.003 \\    
CH$_{\rm 3}$OH $J\!=\!4_{\rm 2}\!\rightarrow\!3_1$ E$^+$  & IRAM30 m    & 1.37  &  $<$0.006 (2$\sigma$)   & 0.003 \\    
\hline
\end{tabular}
\end{table}