\begin{table}%t2 \caption{Absolute surface brightnesses (in Jy/beam) of \object{Mars}, \object{Uranus}, \object{W3~OH}, \object{K3-50A} and \object{NGC~7027} adopted for the computation of the \mbox{Kelvin-to-Janksy} conversion factors {of the 30~m telescope} at 86~GHz and 229~GHz.\label{primcal}} \par \small %\centerline {\begin{tabular} {lcccccc} \hline\hline\noalign{\smallskip} & \multicolumn{6}{c}{UT days of Nov. 2003}\\ \hline\noalign{\smallskip} Source & 11 & 12 & 13 & 14 & 15 & 16 \\ \hline\noalign{\smallskip} \multicolumn{7}{c}{$86$~GHz}\\ \hline\noalign{\smallskip} \object{Mars}$^{{a}}$ & 149.75 & 146.88 & 144.08 & 141.33 & 138.65 & 136.02 \\ \object{Uranus}$^{{a}}$ & 7.06 & 7.05 & 7.04 & 7.03 & 7.01 & 7.01 \\ \object{W3~OH}$^{{b}}$ & \multicolumn{6}{c}{3.94} \\ \object{K3-50A}$^{{b}}$ & \multicolumn{6}{c}{6.29} \\ \object{NGC~7027}$^{{b}}$ & \multicolumn{6}{c}{4.71} \\ \hline\noalign{\smallskip} \multicolumn{7}{c}{$229$~GHz}\\ \hline\noalign{\smallskip} \object{Mars}$^{{a}}$ & 691.16 & 683.33 & 675.51 & 666.71 & 659.92 & 652.17 \\ \object{Uranus}$^{{a}}$ & 32.88 & 32.83 & 32.77 & 32.72 & 32.67 & 32.61 \\ \object{W3~OH}$^{{b}}$ & \multicolumn{6}{c}{6.48} \\ \object{K3-50A}$^{{b}}$ & \multicolumn{6}{c}{6.98} \\ \object{NGC~7027}$^{{b}}$ & \multicolumn{6}{c}{3.68} \\ \hline \end{tabular}} \par \smallskip $^{{a}}$ Computed from the expressions given in Kramer~(\cite{Kra97}), and references therein, {which take into account the angular size of the planets. The values given for \object{Uranus} were computed from an empirical model which used \object{Mars} as primary calibrator (Griffin \& Orton~\cite{Gri93}).} \par $^{{b}}$ Obtained from averages of measurements performed during several years -- before 1996 -- at the IRAM 30~m telescope. These measurements were themselves calibrated through observations of planets. {The sizes of these calibrators at 1.2~mm are given in Lisenfeld et~al.~(\cite{Lis00}).} \end{table}