Table 3: NGC 1068 line parameters.

Transition		 Gaussian V $T_{\rm A}^{*}$ $\Delta V$
  Component [ ${\rm km~s}^{-1}$] [mK] [ ${\rm km~s}^{-1}$]

CO 1-0		 1 $1007 \pm 1$ $225.2 \pm 14.9$ $ 58 \pm 3$
  2 $1100 \pm 3$ $265.1 \pm 3.8 $ $156 \pm 11$
  3 $1234 \pm 2$ $215.3 \pm 10.8$ $ 96 \pm 4$
         
CO 2-1 1 $1007 \pm 2$ $206.8 \pm 32.5$ $ 63 \pm 9 $
  2 $1121 \pm 4$ $529.3 \pm 8.8 $ $179 \pm 16$
  3 $1245 \pm 3$ $222.7 \pm 37.8$ $ 81 \pm 10$
         
CN 1-0 1 $1001 \pm 23$ $12.8 \pm 13.2$ $94\pm42$
  2 $1091 \pm 68$ $19.4 \pm 4.7 $ 154a
  3 $1213 \pm 32$ $15.6\pm9.5$ $136\pm54$
  4 $1946 \pm 26$ 8.3b 154a
         
CN 2-1 1 $1093 \pm 9 $ $10.4\pm 0.9$ $154\pm66$
  2 $1289 \pm 14$ $6.2\pm 0.9$ 154a
         
HCN 3-2 1 $1103\pm7$ $48.7\pm2.4$ $275\pm17$
         
HNC 1-0 1 $1073\pm13$     $9.7\pm1.8$ $114\pm30$
  2 $1268\pm20$ $6.7\pm1.5$ $170\pm62$
         
HNC 3-2 1 $1071\pm 9$ $12.9\pm 1.8$ $134\pm23$
  2 $1250\pm24$ $3.7\pm 2.5$ $70\pm58$
a
The line widths were set to the value found in the main component of the CN 2-1 line.
b
In order to avoid the effect of the artefact in the backend, the intensity was locked to the value expected for this spingroup.

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