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Table A.1:

Molecular line observations with the 15 m SEST.

Transition
Frequency HPBW $\eta_{\rm mb}$ $T_{\rm sys}$ $T_{\rm rms}$ Backend $\Delta \upsilon_{\rm lsr}$ $\int\!\!T_{\rm
A}^{\star}~\rm d\upsilon$
  (MHz) ( ${}^{\prime \prime}$)   (K) (mK)   ( ${\rm km ~ s^{-1}}$) (K ${\rm km ~ s^{-1}}$)
CO (2-1) 230538.0 23 0.50 500 95/10 HRS/LRS -26.3 to -0.3 $15.6 \pm 0.3$
CO (3-2) 345796.0 15 0.25 1600 470/70 HRS/LRS -16.4 to +0.8 $13.6 \pm 1.4$
SiO (2-1) 86846.9 58 0.75 160 10a HRS    
SiO (3-2) 130268.7 38 0.68 190 15a HRS    
SiO (5-4) 217104.9 23 0.61 750 35/7a HRS/LRS    
Note to the table: a This is the rms of the average spectrum, including all positions.

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